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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-19-14875-2019</article-id><title-group><article-title>OH chemistry of non-methane organic gases (NMOGs) emitted from laboratory and ambient biomass burning smoke: evaluating the influence of furans and oxygenated aromatics on ozone and secondary NMOG formation</article-title><alt-title>OH chemistry of NMOGs emitted by biomass burning</alt-title>
      </title-group><?xmltex \runningtitle{OH chemistry of NMOGs emitted by biomass burning}?><?xmltex \runningauthor{M.~M.~Coggon et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Coggon</surname><given-names>Matthew M.</given-names></name>
          <email>matthew.m.coggon@noaa.gov</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Lim</surname><given-names>Christopher Y.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0030-2191</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff12">
          <name><surname>Koss</surname><given-names>Abigail R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff4">
          <name><surname>Sekimoto</surname><given-names>Kanako</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff13">
          <name><surname>Yuan</surname><given-names>Bin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3041-0329</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Gilman</surname><given-names>Jessica B.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Hagan</surname><given-names>David H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5111-4671</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Selimovic</surname><given-names>Vanessa</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff14">
          <name><surname>Zarzana</surname><given-names>Kyle J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1581-6419</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Brown</surname><given-names>Steven S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7477-9078</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Roberts</surname><given-names>James M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8485-8172</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Müller</surname><given-names>Markus</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-4110-8950</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Yokelson</surname><given-names>Robert</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-8415-6808</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7 aff8">
          <name><surname>Wisthaler</surname><given-names>Armin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5050-3018</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Krechmer</surname><given-names>Jordan E.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3642-0659</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff10">
          <name><surname>Jimenez</surname><given-names>Jose L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6203-1847</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11">
          <name><surname>Cappa</surname><given-names>Christopher</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3528-3368</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kroll</surname><given-names>Jesse H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6275-521X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff10">
          <name><surname>de Gouw</surname><given-names>Joost</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0385-1826</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Warneke</surname><given-names>Carsten</given-names></name>
          <email>carsten.warneke@noaa.gov</email>
        </contrib>
        <aff id="aff1"><label>1</label><institution>Cooperative Institute for Research in Environmental Sciences, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>NOAA Earth Systems Research Laboratory Chemical Sciences Division, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Department of Civil and Environmental Engineering, Massachusetts Institute of Technology, Cambridge, MA, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Graduate School of Nanobioscience, Yokohama City University, Yokohama, Kanagawa, Japan</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Chemistry and Biochemistry, University of Montana, Missoula, MT, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Ionicon Analytik, Innsbruck, Austria</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Institute for Ion Physics and Applied Physics, University of Innsbruck, Innsbruck, Austria</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Department of Chemistry, University of Oslo, Oslo, Norway</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Aerodyne Research, Inc., Billerica, MA, USA</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>Department of Chemistry, University of Colorado, Boulder, CO, USA</institution>
        </aff>
        <aff id="aff11"><label>11</label><institution>Department of Civil and Environmental Engineering, University of California, Davis, CA, USA</institution>
        </aff>
        <aff id="aff12"><label>a</label><institution>now at: Tofwerk A.G., Boulder, CO, USA </institution>
        </aff>
        <aff id="aff13"><label>b</label><institution>now at: Institute for Environment and Climate Research, Jinan University, Guangzhou, China</institution>
        </aff>
        <aff id="aff14"><label>c</label><institution>now at: Department of Chemistry, University of Colorado Boulder, Boulder, CO, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Matthew M. Coggon (matthew.m.coggon@noaa.gov) and Carsten Warneke (carsten.warneke@noaa.gov)</corresp></author-notes><pub-date><day>10</day><month>December</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>23</issue>
      <fpage>14875</fpage><lpage>14899</lpage>
      <history>
        <date date-type="received"><day>30</day><month>May</month><year>2019</year></date>
           <date date-type="rev-request"><day>14</day><month>June</month><year>2019</year></date>
           <date date-type="rev-recd"><day>16</day><month>October</month><year>2019</year></date>
           <date date-type="accepted"><day>18</day><month>October</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e347">Chamber oxidation experiments conducted at the Fire Sciences Laboratory in 2016 are evaluated to identify important chemical processes contributing to the hydroxy radical (OH) chemistry of biomass burning non-methane organic gases (NMOGs).  Based on the decay of primary carbon measured by proton transfer reaction time-of-flight mass spectrometry (PTR-ToF-MS), it is confirmed that furans and oxygenated aromatics are among the NMOGs emitted from western United States fuel types with the highest reactivities towards OH. The oxidation processes and formation of secondary NMOG masses measured by PTR-ToF-MS and iodide-clustering time-of-flight chemical ionization mass spectrometry (I-CIMS) is interpreted using a box model employing a modified version of the Master Chemical Mechanism (v. 3.3.1) that includes the OH oxidation of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol. The model supports the assignment of major PTR-ToF-MS and I-CIMS signals to a series of anhydrides and hydroxy furanones formed primarily through furan chemistry. This mechanism is applied to a Lagrangian box model used previously to model a real biomass burning plume. The customized mechanism reproduces the decay of furans and oxygenated aromatics and the formation of secondary NMOGs, such as maleic anhydride. Based on model simulations conducted with and without furans, it is estimated that furans contributed up to 10 % of ozone and over 90 % of maleic anhydride formed within the first 4 h of oxidation. It is shown that maleic anhydride is present in a<?pagebreak page14876?> biomass burning plume transported over several days, which demonstrates the utility of anhydrides as markers for aged biomass burning plumes.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e359">Biomass burning is a significant source of atmospheric non-methane organic gases (NMOGs). Once emitted, biomass burning NMOGs may undergo photochemical reactions to form ozone and secondary organic aerosol (SOA) <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx80 bib1.bibx3" id="paren.1"/>. Wildfire smoke is believed to significantly contribute to summertime ozone levels in fire-prone regions, such as the western United States <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx40 bib1.bibx41" id="paren.2"/>. An assessment of historical ozone data from 1989 to 2004 has shown that daily mean ozone increases by 2 ppb for every 1 million acres of area burned <xref ref-type="bibr" rid="bib1.bibx38" id="paren.3"/>. A warming, drier climate is likely to increase fire activity, which may lead to increased ozone and PM<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> levels in susceptible regions <xref ref-type="bibr" rid="bib1.bibx75 bib1.bibx39 bib1.bibx16 bib1.bibx27" id="paren.4"/>.</p>
      <p id="d1e383">Despite its importance, the atmospheric chemistry of biomass burning smoke remains poorly understood due to the complexity of smoke processing. Field observations have shown that ozone enhancement ratios (<inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Δ</mml:mi><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi mathvariant="normal">CO</mml:mi></mml:mrow></mml:math></inline-formula>) may increase  <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx54" id="paren.5"><named-content content-type="pre">e.g., 0.7 ppb ppb<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,</named-content></xref>, decrease <xref ref-type="bibr" rid="bib1.bibx4" id="paren.6"><named-content content-type="pre">e.g., <inline-formula><mml:math id="M4" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.07 ppb ppb<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,</named-content></xref>, or remain unchanged downwind of wildfires <xref ref-type="bibr" rid="bib1.bibx39" id="paren.7"/>. The extent of ozone production depends on multiple factors, including <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NMOG</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> ratios, downwind meteorology, and incident solar radiation <xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx41" id="paren.8"/>. Ozone production may also be slowed through peroxyacetyl nitrate formation (PAN), which is affected, in part, by NMOG functionality and total <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and NMOG emissions <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx52 bib1.bibx56 bib1.bibx41" id="paren.9"/>. Biomass burning emissions are produced by distillation and pyrolysis, as well as glowing and flaming combustion <xref ref-type="bibr" rid="bib1.bibx78" id="paren.10"/>. Primary NMOG speciation is largely driven by pyrolysis temperatures and fuel composition <xref ref-type="bibr" rid="bib1.bibx68 bib1.bibx32" id="paren.11"><named-content content-type="pre">e.g.,</named-content></xref>, whereas <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions generally increase with increased flaming combustion and greater fuel nitrogen content <xref ref-type="bibr" rid="bib1.bibx20" id="paren.12"/>.</p>
      <p id="d1e505">Secondary NMOGs may provide insights into the chemical processes that contribute to smoke oxidation. Several studies have identified important secondary NMOGs formed from aging of biomass burning emissions <xref ref-type="bibr" rid="bib1.bibx79 bib1.bibx56 bib1.bibx17 bib1.bibx31" id="paren.13"/>; however, the mechanisms that lead to secondary NMOG formation remain unclear. For example, maleic anhydride has been identified as a significant secondary NMOG formed in smoke within hours of oxidation <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx17 bib1.bibx31" id="paren.14"/>. Maleic anhydride is a known product of aromatic oxidation, but it is also an end product of furan chemistry <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx8 bib1.bibx9" id="paren.15"/>. Understanding the pathways leading to secondary NMOG formation may be useful in constraining smoke properties (e.g., plume age) or identifying significant ozone and SOA precursors.</p>
      <p id="d1e517">Few studies have modeled the detailed chemical mechanisms leading to secondary NMOG formation <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx5 bib1.bibx56 bib1.bibx52" id="paren.16"/>. This work is challenging because a large fraction (22 %–56 %) of the identified reactive carbon is associated with compounds whose OH chemistry is unknown or has not been specified in atmospheric chemistry mechanisms <xref ref-type="bibr" rid="bib1.bibx33" id="paren.17"/>. These species could significantly contribute to ozone or SOA formation. For example, <xref ref-type="bibr" rid="bib1.bibx5" id="text.18"/> modeled the evolution of ozone and SOA formed downwind of a prescribed fire and found that <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production was strongly sensitive to the inclusion of unknown NMOGs that have OH rate constants of <inline-formula><mml:math id="M10" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">molec</mml:mi><mml:msup><mml:mo>.</mml:mo><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. <xref ref-type="bibr" rid="bib1.bibx56" id="text.19"/> explicitly modeled the oxidation of 16 NMOGs emitted from a small understory fire using the Master Chemical Mechanism <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx43 bib1.bibx44 bib1.bibx66" id="paren.20"><named-content content-type="pre">MCM v. 3.3.1,</named-content></xref>. The model captured the loss of important reactive primary NMOGs and reproduced the formation of <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and PAN. The formation of maleic anhydride could not be explained by the model, which reflects the need for additional mechanism development.</p>
      <p id="d1e608">The studies described above demonstrate that highly reactive organic compounds play an important role in the OH oxidation of young biomass burning plumes. Laboratory studies evaluating the reactivity of biomass burning NMOGs have shown that furans, oxygenated aromatics, and aliphatic hydrocarbons (e.g., monoterpenes and cyclopentadiene) are major contributors to calculated or measured OH reactivity <xref ref-type="bibr" rid="bib1.bibx71 bib1.bibx30 bib1.bibx32 bib1.bibx17 bib1.bibx31" id="paren.21"/>. <xref ref-type="bibr" rid="bib1.bibx31" id="text.22"/>, for example, found that furans and phenolic compounds were among the most reactive NMOGs emitted from logwood emissions. The detailed chemical mechanisms of these compounds have been studied in single-component systems <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx6 bib1.bibx8 bib1.bibx9 bib1.bibx85 bib1.bibx77 bib1.bibx48 bib1.bibx26" id="paren.23"/>; however, these mechanisms have not been widely implemented into models of biomass burning smoke. <xref ref-type="bibr" rid="bib1.bibx56" id="text.24"/> included simple mechanisms for furan and furfural; however, other major furan species, such as 2-methylfuran, 2,5-dimethylfuran, and 5-methylfurfural, were omitted.</p>
      <p id="d1e623">A few studies have evaluated biomass burning OH oxidation using proton-transfer-reaction time-of-flight mass spectrometry (PTR-ToF-MS). PTR-ToF-MS is capable of measuring 50 %–80 % of the primary NMOG mass emitted from biomass burning, including oxygenates, aromatics, and heterocyclic compounds <xref ref-type="bibr" rid="bib1.bibx33" id="paren.25"/>. The remaining<?pagebreak page14877?> mass includes compounds that are that are difficult to quantify by proton transfer, such as alkanes and small alkenes. The PTR-ToF-MS  is effective in monitoring the evolution of some secondary NMOGs, such as maleic anhydride <xref ref-type="bibr" rid="bib1.bibx56" id="paren.26"/>. Nonetheless, limitations on isomeric specificity <xref ref-type="bibr" rid="bib1.bibx33" id="paren.27"/>, fragmentation, and sensitivity may hinder the ability of the PTR-ToF-MS to measure other secondary oxygenates or multi-functionalized organics <xref ref-type="bibr" rid="bib1.bibx82" id="paren.28"/>. The iodide-clustering time-of-flight chemical ionization mass spectrometer (I<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>-ToF-CIMS, hereafter referred to as I-CIMS for brevity) is well-suited to measure oxygenated NMOGs. The I-CIMS is sensitive to acids and multifunctional oxygenates <xref ref-type="bibr" rid="bib1.bibx49" id="paren.29"/>, which are likely to form as secondary NMOGs in biomass burning plumes. I-CIMS has been used to evaluate primary NMOG emissions <xref ref-type="bibr" rid="bib1.bibx64 bib1.bibx65 bib1.bibx74" id="paren.30"><named-content content-type="pre">e.g.,</named-content></xref>, biomass burning emissions aged by nocturnal processes <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx65" id="paren.31"/>, and primary particle-phase components <xref ref-type="bibr" rid="bib1.bibx29" id="paren.32"/>. I-CIMS spectra of the NMOGs resulting from the OH oxidation of biomass burning smoke have yet to be reported.</p>
      <p id="d1e662">Presented here are PTR-ToF-MS and I-CIMS measurements from chamber experiments performed during the 2016 laboratory component of the Fire Influence on Regional to Global Environments and Air Quality Experiment (FIREX-AQ) conducted at the Fires Sciences Laboratory in Missoula, MT, US. Based on this data, modifications are made to the MCM (v. 3.3.1) to include the reactions of highly reactive NMOGs, including furan, furfural, 2-methylfuran, 2,5-dimethylfuran, 5-methylfurfural, and guaiacol. This mechanism is applied to a box model to interpret observed increases in secondary NMOGs measured by the PTR-ToF-MS and I-CIMS. The chemical mechanism is also applied to a Lagrangian model previously used to evaluate the OH chemistry of an ambient biomass burning plume <xref ref-type="bibr" rid="bib1.bibx56" id="paren.33"/>. The model output is compared to measured secondary NMOG and <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production to evaluate the influence of furans and oxygenated aromatics on the chemistry of a real biomass burning plume.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Campaign description</title>
      <p id="d1e694">The laboratory component of the FIREX-AQ intensive was conducted at the US Forest Service Fire Sciences Laboratory in Missoula, MT, US, during October–November 2016. The purpose of this study was to simulate the emissions and atmospheric oxidation of biomass burning smoke resulting from the combustion of western US fuels. A full description of the campaign, experimental setup, types of fuels burned, and resulting emissions of key NMOGs is provided elsewhere <xref ref-type="bibr" rid="bib1.bibx69 bib1.bibx46" id="paren.34"/>.</p>
      <p id="d1e700"><?xmltex \hack{\newpage}?>Burn experiments were conducted in a large, indoor combustion room, as described by <xref ref-type="bibr" rid="bib1.bibx69" id="text.35"/>. Inside the room, fuels were assembled on a bed centered below a 20 m (L) <inline-formula><mml:math id="M15" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1.6 m (ID) exhaust stack. The fuels were ignited by a heating plate, and the resulting smoke was vented through the stack at a constant velocity of <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> m s<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Smoke was sampled by instrumentation on a platform located <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">17</mml:mn></mml:mrow></mml:math></inline-formula> m above of the fuel bed or directed to other areas of the laboratory through tubing and ductwork.</p>
      <p id="d1e746">The fuels were chosen to represent ecosystems prone to wildfires in the western US and included components (i.e, leaves, stems, trunks, and duff)  of the following species: ponderosa pine (<italic>Pinus ponderosa</italic>), lodgepole pine (<italic>Pinus contorta</italic>), Engelmann spruce (<italic>Picea engelmanii</italic>), Douglas fir (<italic>Pseudotsuga menziesii</italic>), subalpine fir (<italic>Abies lasiocarpa</italic>), manzanita (<italic>Arctostaphylos</italic>), and chamise (<italic>Adenostoma fasciculatum</italic>). The components of each fuel type were burned individually and in mixtures designed to mimic a real forested ecosystem. A full description of these fuels, including harvesting location, composition, and dry weight are provided elsewhere <xref ref-type="bibr" rid="bib1.bibx69" id="paren.36"/>.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Chamber OH oxidation experiments</title>
      <p id="d1e782">Oxidation experiments were performed using an OH-oxidation chamber. The apparatus, subsequently referred to as the “mini-chamber”, consists of a 150 L Teflon bag centrally located between two ultraviolet-C (UVC) lamps (narrow peak emission 254 nm, Ultra-Violet Products, Inc.). A full description of the instrumentation and operation of the mini-chamber is provided by <xref ref-type="bibr" rid="bib1.bibx50" id="text.37"/>. OH is produced by the photolysis of ozone in the presence of water according to Reactions (<xref ref-type="disp-formula" rid="Ch1.R1"/>)–(<xref ref-type="disp-formula" rid="Ch1.R2"/>).


                <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M19" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R1"><mml:mtd><mml:mtext>R1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">ν</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mi mathvariant="normal">D</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R2"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mi mathvariant="normal">D</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>→</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p id="d1e860">Other sources of OH, such as <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow></mml:math></inline-formula> and aldehydes, were also introduced into the chamber via injection of biomass burning smoke. The relative humidity and ozone mixing ratios in the mini-chamber were adjusted to maintain OH exposures equivalent to 1–5 d of atmospheric oxidation. The UVC lamps initiated photochemistry, and the photon flux at the center of the chamber was measured to be <inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> photons cm<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> using a photodiode sensor (Thorlabs S120VC). Previous studies using oxidation flow reactors have investigated the radical chemistry under 254 nm irradiation to quantify non-OH losses and <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx62 bib1.bibx60" id="paren.38"/>. For most primary NMOGs, losses were dominated by OH oxidation. For some species, photolysis played a significant role. Non-OH loss processes affecting important NMOGs are discussed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS3"/>.</p>
      <p id="d1e929">A suite of particle- and gas-phase instruments sampled from the bag through stainless steel and Teflon tubing,<?pagebreak page14878?> respectively. This study focuses on NMOG measurements (described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS1"/>), but a complete description of aerosol measurements is provided by <xref ref-type="bibr" rid="bib1.bibx50" id="text.39"/>. <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi mathvariant="normal">y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> were not measured from the mini-chamber. Initial <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios are estimated based on the integrated <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">acetonitrile</mml:mi></mml:mrow></mml:math></inline-formula> ratios measured from the stack during mini-chamber filling. HONO, an important source of <inline-formula><mml:math id="M29" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and OH, is estimated similarly.</p>
      <p id="d1e997">The mini-chamber was located in a room <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> m from the top of the stack. To quickly deliver smoke to the chamber, stack air was drawn through a aluminum duct that is 30 m in length and 20 cm in diameter. The residence time within the duct was &lt; 2 s and particle losses were minor <xref ref-type="bibr" rid="bib1.bibx50" id="paren.40"/>. Gas-phase species have a high affinity to metal surfaces and losses to the aluminum ductwork are possible <xref ref-type="bibr" rid="bib1.bibx24" id="paren.41"/>. It is difficult to assess these losses quantitatively; however, the average NMOG <inline-formula><mml:math id="M31" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> acetonitrile ratio measured in the mini-chamber was <inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> %–20 % lower than that measured from the stack (see the Supplement for more details). While these differences likely indicate that NMOGs were lost to ductwork, the relative distribution of NMOGs was not significantly different between the stack and mini-chamber.</p>
      <p id="d1e1034">Mini-chamber experiments were conducted in the following manner. (1) Prior to each burn, the bag was flushed with clean humidified air for <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> min. (2) Immediately following fuel ignition, smoke diluted with clean air was injected into the bag at a <inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> ratio. Injection proceeded until the burn finished or until particle concentrations maximized inside the mini-chamber. For most experiments, the distribution of NMOGs and particles represented an integrated sample of all phases of the burn. (3) 40 ppb of deuterated butanol (butanol-d9, added to monitor OH exposure) was injected into the chamber and the particle and gas mixture was allowed to mix for <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>–10 min. (4) A stream of clean, humidified air (RH <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> %) doped with <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> ppb ozone was continuously added to the mini-chamber to match instrumentation sampling flows (<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> L min<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and maintain a high-OH environment. (5) Once aerosol- and gas-phase concentrations stabilized, the UVC lamps were turned on and photochemistry proceeded for <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula>–45 min. (6) At the end of the experiment, the bag was flushed with clean dilution air in preparation for subsequent experiments.</p>
      <p id="d1e1124">Gas- and particle-phase concentrations were corrected for dilution by monitoring the decay of acetonitrile, which is present at high concentrations in biomass burning smoke, slow to react with OH (lifetime <inline-formula><mml:math id="M41" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">335</mml:mn></mml:mrow></mml:math></inline-formula> d at OH <inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), and not significantly lost to Teflon surfaces <xref ref-type="bibr" rid="bib1.bibx47 bib1.bibx58" id="paren.42"/>. CO was not used as a dilution tracer due to observed CO production following the initiation of photochemistry. The dilution rate estimated by acetonitrile decay agreed well with flow rate calculations <xref ref-type="bibr" rid="bib1.bibx50" id="paren.43"/>. OH exposures in the mini-chamber were estimated based on the dilution-corrected loss of butanol-d9 <xref ref-type="bibr" rid="bib1.bibx11" id="paren.44"><named-content content-type="pre"><inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molec.<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,</named-content></xref>.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Instrumentation</title>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>NMOG measurements</title>
      <p id="d1e1251">NMOG measurements were conducted using a high-resolution proton transfer reaction time-of-flight mass spectrometer <xref ref-type="bibr" rid="bib1.bibx81" id="paren.45"><named-content content-type="pre">PTR-ToF-MS,</named-content></xref> and an iodide-clustering time-of-flight chemical ionization mass spectrometer (I-CIMS, Aerodyne/Tofwerk, AG). The instruments were deployed to measure primary smoke emissions from the stack and room, as well as aged emissions from the mini-chamber. During a burn (and while the mini-chamber was filling with smoke), both instruments sampled from the stack to characterize primary NMOG emissions. At the end of a burn, the sampling lines were switched and the instruments sampled from the mini-chamber through a Teflon inlet that is 10 m in length and has an outer diameter of 3 mm at a total flow rate of <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> L min<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. A full description of the primary NMOG measurements is provided elsewhere, and only a brief description of these measurements is provided here <xref ref-type="bibr" rid="bib1.bibx46" id="paren.46"/>.</p>
      <p id="d1e1284">The PTR-ToF-MS measured at 1 Hz to capture the decay of primary NMOGs and formation of secondary species, respectively. The drift tube was operated with an electric field to number density ratio (<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mi>E</mml:mi><mml:mo>/</mml:mo><mml:mi>N</mml:mi></mml:mrow></mml:math></inline-formula>) of 120 Td, and the high-resolution mass spectrometer (max resolution <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4500</mml:mn></mml:mrow></mml:math></inline-formula>) scanned ions with <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 12–500 Th. The mass spectrometer resolves the molecular formulae of isobaric species but cannot distinguish isomers. This presents challenges in reacting systems as secondary NMOGs formed by OH oxidation could have the same molecular formula as primary NMOGs. <xref ref-type="bibr" rid="bib1.bibx46" id="text.47"/> identified the distribution of primary NMOGs during FIREX-AQ using gas chromatography pre-separation to measure isomer contributions. For most fuel types, over 90 % of the PTR-ToF-MS signal could be assigned. The primary groups detected by PTR-ToF-MS were small oxygenates (<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:mi>v</mml:mi><mml:mo>/</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:math></inline-formula>, dominated by acetic acid, formaldehyde, methanol, and acetaldehyde), aromatics (<inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> %, dominated by catechol, phenol, methoxy phenols, benzene, and toluene), furans (<inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> %, dominated by 5-methylfurfural, 2-furfural, furanone, furan, and methylfurans + dimethylfurans), and a broad range of hydrocarbons (<inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> %, dominated by ethene, propene, butene, and 1,3-butadiene). The same NMOG assignments and sensitivities are applied here to masses observed to be enhanced prior to NMOG oxidation. The temporal profile of some larger primary oxygenates (<inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>) were also influenced by the formation of secondary isomers or unidentified primary species (see Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS2"/>). Calibration factors for primary species are calculated from measured or estimated proton transfer rate constants <xref ref-type="bibr" rid="bib1.bibx67" id="paren.48"><named-content content-type="pre">uncertainty &lt; 50 %,</named-content></xref>.</p>
      <?pagebreak page14879?><p id="d1e1398">Masses detected after the initiation of photochemistry are assigned based on previous literature observations and modeling evidence (see Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS2"/>). A number of laboratory and field studies employing PTR-ToF-MS and open-path Fourier transform infrared spectrometer (OP-FTIR) have observed formation of formic acid (<inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 47), acetic acid (<inline-formula><mml:math id="M61" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 61), maleic anhydride (<inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <italic>m/z</italic> 99), and phthalic anhydride (<inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 149) in aged smoke <xref ref-type="bibr" rid="bib1.bibx79 bib1.bibx80 bib1.bibx2 bib1.bibx56 bib1.bibx17 bib1.bibx31" id="paren.49"/>. Calibration factors for these species are calculated from measured or estimated proton transfer rate constants. In this study, substantial increases in <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 101) and <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 89) are also observed.  <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> could be 5-hydroxy-2(5H)-furanone (or simply hydroxy furanone), its tautomer malealdehydic acid, or succinic anhydride, whereas  <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is likely a C<inline-formula><mml:math id="M72" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> hydroxy carbonyl <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx14 bib1.bibx15 bib1.bibx6 bib1.bibx8 bib1.bibx9 bib1.bibx73 bib1.bibx85" id="paren.50"><named-content content-type="pre">see Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/> and)</named-content></xref>. Due to uncertainties in these assignments, calibration factors for these species are calculated using estimated proton transfer rate constants derived from molecular formula relationships <xref ref-type="bibr" rid="bib1.bibx67" id="paren.51"><named-content content-type="pre">uncertainty to within a factor of 2,</named-content></xref>.</p>
      <p id="d1e1712">The I-CIMS utilizes a “soft” chemical ionization source that forms iodide clusters with polarizable analyte molecules <xref ref-type="bibr" rid="bib1.bibx37 bib1.bibx49" id="paren.52"/>. The instrument used here was operated in a similar configuration to that described in <xref ref-type="bibr" rid="bib1.bibx47" id="text.53"/>. To generate reagent ions, 2 SLPM (standard liter per minute) of clean <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from dewar blow-off was run over a methyl iodide permeation tube and ionized using a Polonium-210 ionizer and into an ion molecule reaction region (IMR). The I-CIMS measured gas-phase signals from the mini-chamber at 1 Hz time resolution. Smoke was diluted with 4 L min<inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> of clean, humidified air at a <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> ratio to minimize reagent ion depletion. A constant flow of isotopically labeled formic acid was delivered to the instrument to measure consistency of response. Reported here are I-CIMS measurements normalized to <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> counts per second of the reagent ion signal at <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 126.905 (normalized counts per second, ncps). Due to unavailability of standards, I-CIMS data are not reported in mixing ratios. Secondary NMOGs measured by I-CIMS are assigned identifications based on modeling results and previous literature.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><?xmltex \opttitle{{$\protect\chem{NO_{\mathit{x}}}$} measurements}?><title><inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> measurements</title>
      <p id="d1e1803"><inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow></mml:math></inline-formula> were measured by an  OP-FTIR, as described by <xref ref-type="bibr" rid="bib1.bibx69" id="text.54"/>. The OP-FTIR  was located on the platform and sampled smoke across the diameter of the stack. The OP-FTIR provides fast measurements and avoids potential sampling artifacts due to sample line losses. OP-FTIR measurements were used for most experiments. <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and HONO were also measured by the NOAA Airborne Cavity Enhanced Spectrometer (ACES), as described by <xref ref-type="bibr" rid="bib1.bibx84" id="text.55"/>. ACES was located on the platform and sampled smoke through a 1 m Teflon inlet. These data were used when OP-FTIR data were unavailable, or when <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions were below OP-FTIR detection limits. Supplementary NO measurements were provided by a custom-built chemiluminescence instrument located in a room on the burn chamber floor. A full description of that instrument is provided by <xref ref-type="bibr" rid="bib1.bibx72" id="text.56"/>.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Box model implementation and evaluation</title>
      <p id="d1e1873">NMOG oxidation processes were simulated using the Framework for 0-D Atmospheric Modeling <xref ref-type="bibr" rid="bib1.bibx76" id="paren.57"><named-content content-type="pre">F0AM v 3.1, <uri>https://sites.google.com/site/wolfegm/models</uri>, last access: 9 January 2018</named-content></xref>. A modified NMOG oxidation mechanism is applied based on the Master Chemical Mechanism <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx43 bib1.bibx44 bib1.bibx66" id="paren.58"><named-content content-type="pre">MCM v. 3.3.1,</named-content></xref>. As described here and in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/>, the box model is used to evaluate NMOG formation in the mini-chamber, as well as for the daytime oxidation of an ambient biomass burning plume <xref ref-type="bibr" rid="bib1.bibx56" id="paren.59"/>. Non-atmospheric photolysis played a role in the evolution of organics in the mini-chamber owing to the use of UVC lamps; consequently, interpretation of the mini-chamber measurements is limited to evaluating the link between OH oxidation of furan and oxygenated aromatics with the formation of several key secondary NMOGs measured by I-CIMS and PTR-ToF-MS. The ambient model is used to quantitatively evaluate the impact of furan and oxygenated aromatic chemistry on secondary NMOGs and ozone formation in real biomass burning plumes.</p>
      <p id="d1e1894">NMOG chemistry and dilution are assumed to follow the first-order differential equation described by Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>).

            <disp-formula id="Ch1.E3" content-type="numbered"><label>1</label><mml:math id="M84" display="block"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>m</mml:mi><mml:mi>n</mml:mi></mml:munderover><mml:msub><mml:mi>P</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>r</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mi>m</mml:mi><mml:mi>n</mml:mi></mml:munderover><mml:msub><mml:mi>R</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:msub><mml:mi>r</mml:mi><mml:mi>m</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>k</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the concentration of species <inline-formula><mml:math id="M86" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>P</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the stoichiometric coefficient of reaction <inline-formula><mml:math id="M88" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> leading to the formation of species <inline-formula><mml:math id="M89" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the stoichiometric coefficient of reaction <inline-formula><mml:math id="M91" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> leading to the loss of species <inline-formula><mml:math id="M92" display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M93" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> is the elementary rate of reaction <inline-formula><mml:math id="M94" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a first-order dilution rate constant. A constant dilution term is applied to all species based on the measured loss rate of acetonitrile. Vapor–wall interactions are not considered in this model, and these processes may impact the evolution of intermediate and semi-volatile gases. <xref ref-type="bibr" rid="bib1.bibx50" id="text.60"/> did not observe significant wall losses of primary VOCs during chamber experiments. Vapor–wall interactions have been shown to play a role in the SOA evolution of biomass burning smoke, and partitioning to the gas-phase is greater in diluting systems <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx36" id="paren.61"/>.</p>
      <p id="d1e2076">The MCM treats the photolysis of organic and inorganic species through parameterizations relevant to atmospheric wavelengths. To account for photolysis in the mini-chamber,<?pagebreak page14880?> MCM photolysis frequencies were calculated using literature cross sections and quantum yields of relevant organic and inorganic species <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx19 bib1.bibx45" id="paren.62"/>. Tables S1 and S2 in the Supplement summarize the reactions and databases used to estimate photolysis frequencies in the mini-chamber. For some primary species and <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> reservoirs (e.g., acetone, acetaldehyde, benzaldehyde, PAN), additional reactions were added to account for photolysis pathways at 254 nm (Table S2).</p>
      <p id="d1e2093">Photolysis frequencies are calculated as the product of the absorption cross section, quantum yield, and photon flux at 254 nm. The measured 254 nm photon flux (<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> photons cm<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M99" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) is scaled by a factor of 1.5 in order to reproduce the measured OH-loss of butanol-d9. No other changes are applied to the rate constants or reactions of MCM v. 3.3.1. To account for other reactive NMOGs, literature mechanisms for furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol are included. A full description of these modifications are provided in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/>. Table S3 summarizes the photolysis frequencies and <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> rate constants for the primary NMOG species modeled here.</p>
      <p id="d1e2169">The mini-chamber model is evaluated against two fires – F26 (Engelmann spruce duff) and F38 (ponderosa pine litter). These two fires represent different extreme cases in <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and NMOG composition and were chosen in order to assess the extent to which the variability of primary NMOGs influences secondary NMOG formation. Figure S2 in the Supplement illustrates how F38 and F26 compare to other fires measured in this study. F26 was a unique burn characterized by low-temperature smoldering combustion, which resulted in low <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions (<inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NMOG</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.02</mml:mn></mml:mrow></mml:math></inline-formula> mol mol<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and a NMOG profile with high contributions from oxygenated aromatics such as phenol, cresol, and guaiacol. F38 was representative of many of the burns presented here and was characterized by a mixture of high-temperature flaming combustion and low-temperature smoldering. <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emissions were substantially higher than those of F26 (<inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>/NMOG <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.32</mml:mn></mml:mrow></mml:math></inline-formula>).</p>
      <p id="d1e2264">The mini-chamber model is initialized with the mixing ratio of 47 primary NMOG species measured by PTR-ToF-MS (Table S3). NO, <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and HONO were initialized based on stack measurements, as described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS2"/>. Ozone measurements were conducted using a 2B Technologies ozone monitor (model 202), which exhibited significant interferences upon the addition of smoke or hexafluorobenzene (added as a supplemental dilution tracer). The monitor measures the absorption of <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at wavelengths that are also absorbed by many primary NMOGs. Here, ozone measurements are only used to initialize the model with initial <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios. These initial conditions are based on the signal measured prior to smoke injection and ranged between 5 and 10 ppb.</p>
      <p id="d1e2302">Ozone is continuously added to the chamber over the course of an experiment. This input of ozone is included in the model by applying a constant ozone mixing ratio to the dilution term of Eq. (<xref ref-type="disp-formula" rid="Ch1.E3"/>). It is estimated that the dilution stream contained <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> ppb of ozone based on the expected output from the ozone generator (<inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> ppm) and the measured dilution rate. This input of ozone reproduces the ozone signal measured during dark control experiments to within 20 % (Fig. S1).</p>
      <p id="d1e2327"><inline-formula><mml:math id="M116" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are both emitted from fires. Once injected into the chamber, NO will react with <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> to generate <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. In the atmosphere, <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M121" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> will rapidly cycle owing to <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> photolysis. In the mini-chamber, <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> photolysis is reduced since <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> does not strongly absorb at 254 nm <xref ref-type="bibr" rid="bib1.bibx19" id="paren.63"><named-content content-type="pre">the absorption cross section at 254 nm is a factor of 64 smaller than the peak absorption at 400 nm,</named-content></xref>. Consequently, radical reactions (e.g., <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> + <inline-formula><mml:math id="M126" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> loss processes (e.g., PAN formation) are likely to be sensitive to the initial <inline-formula><mml:math id="M128" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio. The initial <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ratio is estimated assuming that the <inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixture measured from the stack reacts with a constant mixing ratio of ozone (10 ppb) for 10 min (the approximate mixing periods for F26 and F38). This analysis yields a <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> distribution that is <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">95</mml:mn></mml:mrow></mml:math></inline-formula> % <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. This <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> distribution is applied to the mini-chamber model as an initial condition.</p>
      <p id="d1e2544">The ambient Lagrangian box model is the same used by <xref ref-type="bibr" rid="bib1.bibx56" id="text.64"/> to evaluate ozone and NMOG formation from aircraft measurements of a small biomass burning plume during the 2013 DISCOVER-AQ campaign. The mechanism employed by <xref ref-type="bibr" rid="bib1.bibx56" id="text.65"/> was based on MCM v. 3.3.1 and included a simplified scheme to represent furfural and furan chemistry. Only the decay of furfural was modeled, whereas furan oxidation was assumed to form butenedial. The same model used by <xref ref-type="bibr" rid="bib1.bibx56" id="text.66"/> is employed here, except that the mechanism includes the reactions of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol (Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/>). The same initial conditions used by <xref ref-type="bibr" rid="bib1.bibx56" id="text.67"/> are applied here but with the inclusion of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol, phenol, cresol, and catechol. Photolysis in the ambient box model is represented by MCM parameterizations, and dilution rates are calculated based on the observed decay of CO.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Oxidation product measurements</title>
      <p id="d1e2577">Figure S2 summarizes the initial <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and NMOG concentrations, <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NMOG</mml:mi></mml:mrow></mml:math></inline-formula> ratio, and NMOG composition for all the mini-chamber experiments sampled by PTR-ToF-MS and I-CIMS. NMOG composition is reported as the fraction of NMOG signal attributed to high-temperature, low-temperature, and duff pyrolysis, as described by <xref ref-type="bibr" rid="bib1.bibx68" id="text.68"/>. High-temperature pyrolysis results in higher emissions  of non-functionalized hydrocarbons, such as<?pagebreak page14881?> benzene, while low-temperature pyrolysis results in higher emissions of oxygenated species, such as methoxy phenols. Duff pyrolysis generates a NMOG distribution that is similar to the distribution from low-temperature pyrolysis, except that the unique composition of duff results in higher emissions of nitrogen-containing compounds.</p>
      <p id="d1e2609">The initial conditions for mini-chamber experiments varied drastically depending on chamber dilution, fuel type, and burn conditions (Fig. S2). The <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NMOG</mml:mi></mml:mrow></mml:math></inline-formula> ratio varied over several orders of magnitude (0.01–1.2) with NMOG loadings ranging from 90 to 900 ppb. Fires produced varying distributions of NMOGs owing to the extent of high- and low-temperature pyrolysis, while <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> mixing ratios varied depending on fuel nitrogen content <xref ref-type="bibr" rid="bib1.bibx20" id="paren.69"/> and the extent of flaming combustion <xref ref-type="bibr" rid="bib1.bibx68" id="paren.70"/>. For the remaining discussion, only experiments with NMOG loadings &lt; 300 ppb (12 total) are analyzed in order to evaluate biomass burning chemistry at the lowest calculated primary OH reactivities (OHRs), since high OHR values can lead to significant OH suppression <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx62" id="paren.71"/>. The experiments reported here have estimated OHR between 18 and 70 s<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, which are within range of the OHR recommended by <xref ref-type="bibr" rid="bib1.bibx61" id="text.72"/> when using 254 nm lights (50–100 s<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p>
      <p id="d1e2675">Figure <xref ref-type="fig" rid="Ch1.F1"/> shows the temporal evolution of select NMOGs measured by PTR-ToF-MS and I-CIMS during F38 (ponderosa pine). The left column shows the decay of primary NMOGs, while other columns show the temporal profiles of secondary NMOGs exhibiting significant enhancements in PTR-ToF-MS and I-CIMS spectra. Secondary NMOGs are classified based on temporal profile – those exhibiting a relatively fast increase in signal are classified as “fast-forming” products, while those formed more gradually over the course of an experiment are classified as “slow-forming” products. These designations are chosen based on the oxidation timescales that are likely to be observed in ambient biomass burning plumes. Here, OH exposures are estimated by the decay of butanol-d9 and then converted to atmospheric-equivalent timescales assuming an atmospheric OH concentration of <inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M142" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. Fast-forming products generally peaked within 10–20 h of atmospheric-equivalent oxidation, while slow-forming products exhibited no maxima.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e2710">Temporal evolution of select NMOGs from the OH oxidation of smoke resulting from Fire 38 (ponderosa pine). The data have been dilution-corrected based on the decay of acetonitrile. The time basis is calculated based on the decay of deuterated butanol. The first column shows primary NMOGs, the second column illustrates species formed within 20 h of atmospheric-equivalent oxidation (“fast-forming” products), while other columns show species formed over longer timescales (“slow-forming” products). </p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f01.png"/>

        </fig>

      <p id="d1e2719">The loss of reactive primary species occurs quickly (&lt; 20 h of atmospheric-equivalent oxidation). Most species (e.g., dimethylfuran and guaiacol) follow an exponential decay consistent with radical loss pathways; however, some species, such as furfural and 5-methylfurfural, show faster decay immediately following the initiation of lights. The lights employed in these experiments (Ultra-Violet Products, Inc.) emit a narrow band at 254 nm, which is capable of photolyzing furanaldehydes and other absorbing species <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx28" id="paren.73"/>. The furfural photolysis frequency in the mini-chamber is estimated to be 0.13 s<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (Table S2), which is orders of magnitude greater than the photolysis frequency expected under ambient, summertime conditions <xref ref-type="bibr" rid="bib1.bibx22" id="paren.74"><named-content content-type="pre"><inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> s<inline-formula><mml:math id="M145" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>,</named-content></xref>. Furfural photolysis leads to the formation of other highly reactive furans (e.g., furan) at modest yield <xref ref-type="bibr" rid="bib1.bibx28" id="paren.75"><named-content content-type="pre">&lt; 0.3,</named-content></xref>, and these products may contribute to the OH reactivity early on during each experiment.</p>
      <p id="d1e2776">The majority of secondary NMOGs observed by the PTR-ToF-MS are classified as “slow-forming” products. Previous studies employing PTR-ToF-MS have identified acetic acid, formic acid, and maleic anhydride as major products <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx17 bib1.bibx31" id="paren.76"/>. Formic and acetic acid are primary species but also form from OH oxidation of alkene and aromatic species <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx43 bib1.bibx44 bib1.bibx66 bib1.bibx55" id="paren.77"><named-content content-type="pre">e.g.,</named-content></xref>. Maleic anhydride is known to form from the oxidation of aromatics, but it has also been observed to form from the oxidation of furans <xref ref-type="bibr" rid="bib1.bibx15" id="paren.78"/>. The formation of slow-forming products occurs over timescales &gt; 20 h, which is significantly longer than the evolution of fast-forming products (e.g., <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula> h) and losses of the most reactive primary NMOGs (e.g., 2-methylfuran and guaiacol, <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>–10 h). This may be an indication of multigenerational oxidation, or early generation formation via slowly reacting primary species.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e2834">Summary of PTR-ToF-MS measurements during 12 mini-chamber experiments. Shown is the amount of initial NMOG carbon (<inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>NMOG, %) that was consumed (reactant) or formed (product) for a given species after 12 h of atmospheric-equivalent oxidation (OH concentration of <inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). Panel <bold>(a)</bold> shows the average speciated distribution of products (error bars are standard deviations). Panel <bold>(b)</bold> shows <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>C</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>NMOG for reactants and products as lumped categories. A species is classified as a product if the dilution-corrected signal measured by the PTR-ToF-MS increased after 12 h of simulated oxidation, and a reactant if the signal decreased. Categories labeled as “no ID” refer to species for which an assignment could not be confidently prescribed. The numbers in the legend refer to the fire number (composition and initial conditions can be found in Fig. S2). Experiments are ordered according to the fraction of primary carbon transformed to measurable secondary NMOGs (greatest to least).</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f02.png"/>

        </fig>

      <p id="d1e2899">Figure <xref ref-type="fig" rid="Ch1.F2"/> shows the resulting changes in NMOG composition measured by the PTR-ToF-MS after <inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:math></inline-formula> h of atmospheric-equivalent oxidation. Data are shown in terms of primary carbon changes (<inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>NMOG, %), which is the fraction of initial NMOG carbon measured by the PTR-ToF-MS that was consumed (reactant) or formed (product) for a given species or group of species. “Reactant” and “product” classifications were determined based on whether a detected mass exhibited an increase or decrease in dilution-corrected signal after 12 h of atmospheric-equivalent oxidation. The bars in Fig. <xref ref-type="fig" rid="Ch1.F2"/>b represent species-aggregate measurements for each of the 12 fires highlighted in Fig. S2. Figure <xref ref-type="fig" rid="Ch1.F2"/>a shows an average of all secondary NMOGs formed after 12 h of atmospheric-equivalent oxidation. Across most experiments, furans and oxygenated aromatics were the primary NMOGs with the greatest carbon losses. Decreases in oxygenated aromatics were mostly driven by losses of guaiacol, methyl guaiacol, and catechol. Losses of furans were primarily due to decreases in furan, 2-methylfuran, 2,5-dimethylfuran, furfural, and 5-methylfurfural. These observations are consistent with previous PTR-ToF-MS measurements of aged wood burning smoke <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx31" id="paren.79"/>. The contribution from biogenic species in this study was variable, and largely dependent on composition <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx33" id="paren.80"/> and the extent to which monoterpenes were emitted from the distillation phase of combustion <xref ref-type="bibr" rid="bib1.bibx46 bib1.bibx68" id="paren.81"/>. The detected masses associated with the alkene category exhibited both apparent formation and consumption across various experiments. Alkenes are expected to react quickly with OH; thus, observed increases likely point to a species misassignment. It is likely that this increase in signal is the result<?pagebreak page14882?> of PTR-ToF-MS fragmentation of oxygenated NMOGs. For example, some alcohols, acids, and certain aldehydes may fragment in the PTR-ToF-MS to masses that are typically associated with alkenes <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx59" id="paren.82"><named-content content-type="pre">e.g., <inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 69,</named-content></xref>. These species are likely formed from the oxidation of biomass burning precursors and potentially interfere with alkene detection.</p>
      <p id="d1e2958">Across most experiments, small oxygenates and acids (<inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>) were the predominant secondary NMOGs detected by PTR-ToF-MS (Fig. <xref ref-type="fig" rid="Ch1.F2"/>b). As mentioned previously, formic acid, acetic acid, and maleic anhydride are several species with the largest relative increase at longer oxidation timescales (Fig. <xref ref-type="fig" rid="Ch1.F2"/>a); however, formaldehyde, acetaldehyde, acetone, and several <inline-formula><mml:math id="M157" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> species increased significantly. The formation of <inline-formula><mml:math id="M158" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> species follows a similar temporal pattern as maleic anhydride, which may point to similarities in species functionality or formation pathways.</p>
      <p id="d1e3020">In contrast to the PTR-ToF-MS measurements, the I-CIMS measured a mix of fast- and slow-forming products (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). The I-CIMS measured a small fraction of the primary NMOGs, so only secondary NMOGs are discussed here. Fast-forming products included pyruvic acid (<inline-formula><mml:math id="M159" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M160" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>y</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> compounds, and masses likely corresponding to nitroaromatics. Previous studies have reported the formation of nitroaromatics from OH oxidation of catechol and guaiacol in the presence of <inline-formula><mml:math id="M161" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx26" id="paren.83"/>. <inline-formula><mml:math id="M162" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is consistent with the formation of nitroguaiacol, which has been observed in the gas and particle phase from guaiacol <inline-formula><mml:math id="M163" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH (<inline-formula><mml:math id="M164" display="inline"><mml:mo lspace="0mm">+</mml:mo></mml:math></inline-formula><inline-formula><mml:math id="M165" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) chemistry <xref ref-type="bibr" rid="bib1.bibx48" id="paren.84"/>. <xref ref-type="bibr" rid="bib1.bibx26" id="text.85"/> studied the OH oxidation of catechol and observed the formation of nitrocatechol with a molar yield of 0.3. Very little nitrocatechol was observed by the PTR-ToF-MS and I-CIMS, which is likely due to the high aerosol loadings in the chamber (&gt; 50 <inline-formula><mml:math id="M166" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M167" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and high affinity of nitrocatechol to partition to aerosols and surfaces <xref ref-type="bibr" rid="bib1.bibx26" id="paren.86"/>.</p>
      <p id="d1e3157">Figure <xref ref-type="fig" rid="Ch1.F3"/> summarizes the changes in I-CIMS product spectra relative to the total signal measured prior to photochemistry. Shown are the product distributions for short (4 h), medium (12 h), and longer (24 h) atmospheric timescales. Because not all masses could be calibrated, normalized difference spectra (oxidized minus primary) are presented in<?pagebreak page14883?> order to illustrate the ions with the largest relative increases. In general, the secondary NMOGs measured by I-CIMS tend to be multifunctional.  The smallest observed oxygenate is formic acid (<inline-formula><mml:math id="M168" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), while larger molecules tend to be <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M170" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds. After 4 h of oxidation, the largest enhancements are due to fast-forming products such as <inline-formula><mml:math id="M171" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M172" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M173" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The relative importance of these masses decreases at longer timescales, whereas the relative abundance of smaller oxygenates increases (e.g., <inline-formula><mml:math id="M174" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M175" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e3333">Summary of secondary NMOGs measured by I-CIMS during 12 mini-chamber experiments. Shown are ion signals that increased after initiating photochemistry relative to the total integrated signal measured prior to photochemistry. Panels <bold>(a)</bold>–<bold>(c)</bold> show changes in signal after 4, 12, and 24 h of atmospheric-equivalent oxidation, respectively. Error bars represent standard deviations. Note that the masses are presented as I<inline-formula><mml:math id="M176" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> adducts.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f03.png"/>

        </fig>

      <p id="d1e3357">The signal intensity of the fast-forming products (specifically <inline-formula><mml:math id="M177" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M178" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) suggests that these species result from the oxidation of abundant, fast-reacting NMOG precursors with a carbon number of <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>. Modeling results presented in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/> support the assignment of these products as hydroxy furanone (<inline-formula><mml:math id="M180" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and methyl hydroxy furanone (<inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). Based on the loss of primary NMOGs (Fig. <xref ref-type="fig" rid="Ch1.F2"/>), it is likely that these species are formed from the oxidation of furans, oxygenated aromatics, or other fast-reacting NMOGs with <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>. Several studies have investigated the oxidation of furan species and shown that hydroxy furanone <inline-formula><mml:math id="M183" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> tautomer (<inline-formula><mml:math id="M184" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and methyl hydroxy furanone + tautomer (<inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) are major products formed from the oxidation of furfural, furan, 2-methylfuran, and 2,5-dimethylfuran <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx15 bib1.bibx6 bib1.bibx8 bib1.bibx9 bib1.bibx73 bib1.bibx85" id="paren.87"><named-content content-type="pre">e.g.,</named-content></xref>. Secondary NMOGs measured from the OH chemistry of oxygenated aromatic species are largely carbon-retaining (<inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula>), though <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> ring fragments have been measured in low-<inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> catechol oxidation <xref ref-type="bibr" rid="bib1.bibx77" id="paren.88"/>.</p>
      <p id="d1e3576">Notably, inspection of Figs. <xref ref-type="fig" rid="Ch1.F2"/>a and <xref ref-type="fig" rid="Ch1.F3"/> shows that there is little overlap in the species measured by PTR-ToF-MS and I-CIMS. The only masses that exhibit significant enhancements in both spectra are formic acid (<inline-formula><mml:math id="M189" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Moreover, there are significant differences in the temporal evolution of <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. As discussed above, <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measured by I-CIMS most likely corresponds to hydroxy furanone, a fast-forming product (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). In contrast, <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> as<?pagebreak page14884?> measured by the PTR-ToF-MS exhibits a temporal profile resembling that of a slow-forming product. This mass is likely succinic anhydride, which is structurally similar to maleic anhydride and could be formed from multigeneration chemistry.  The differences in these profiles suggests that the there are at least two different <inline-formula><mml:math id="M194" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species present, that PTR-ToF-MS and I-CIMS are sensitive to different biomass burning oxidation products, and that both instruments are needed in order to measure important secondary NMOGs.</p>
      <p id="d1e3707">Previous studies and the mass spectra in Figs. <xref ref-type="fig" rid="Ch1.F2"/> and <xref ref-type="fig" rid="Ch1.F3"/> show that furan chemistry plays a significant role in the OH chemistry of biomass burning plumes <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx31 bib1.bibx30 bib1.bibx32" id="paren.89"/>. In Sect. <xref ref-type="sec" rid="Ch1.S3.SS2"/>, furan chemistry is incorporated into a box model to help interpret the observed small-chamber measurements and previously measured ambient biomass burning plumes.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>NMOG box modeling</title>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Mechanism incorporation</title>
      <p id="d1e3734">The box model described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS4"/> employs NMOG chemistry based on the Master Chemical Mechanism <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx43 bib1.bibx44 bib1.bibx66" id="paren.90"><named-content content-type="pre">MCM v. 3.3.1,</named-content></xref>. The MCM explicitly represents the chemistry of biogenic, alkyl, aromatic, and oxygenated aromatic species. The laboratory measurements described in Sect. 3.1 demonstrate that heterocyclic hydrocarbons, such as the furans, could significantly contribute to secondary NMOG formation. The following discussion motivates and describes mechanism development aimed at expanding the MCM representation of biomass burning OH chemistry.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e3746">Contribution of individual species to the total primary OH reactivity estimated from PTR-ToF-MS measurements following Eq. (<xref ref-type="disp-formula" rid="Ch1.E4"/>). Bar intensity is median for all burns measured by PTR-ToF-MS, whereas circle markers are averages. Error bars indicate 25th and 75th percentiles. Bar colors indicate if a species is included (grey) or not included (red) in the MCM v. 3.3.1. Green bars indicate OH oxidation mechanisms that were added to the MCM (sub-mechanisms for each species can be found in Figs. S4–S9). The concentrations of each species were calculated following the methods described by <xref ref-type="bibr" rid="bib1.bibx46" id="text.91"/>. Only species that were positively identified are included in these calculations. The assumed OH rate constant for each species is given by <xref ref-type="bibr" rid="bib1.bibx46" id="text.92"/>.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f04.png"/>

          </fig>

      <p id="d1e3763">Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the breakdown in OH reactivity of the primary NMOGs measured by PTR-ToF-MS during the Firelab study <xref ref-type="bibr" rid="bib1.bibx46" id="paren.93"/>. Each bar represents a fraction of the total calculated OH reactivity, as represented by Eq. (<xref ref-type="disp-formula" rid="Ch1.E4"/>).
              <disp-formula id="Ch1.E4" content-type="numbered"><label>2</label><mml:math id="M195" display="block"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi mathvariant="normal">OHR</mml:mi><mml:mo>,</mml:mo><mml:mi>i</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msubsup><mml:mo>∑</mml:mo><mml:mi>i</mml:mi><mml:mi>n</mml:mi></mml:msubsup><mml:msub><mml:mi>k</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <italic>i</italic> is the species of interest, <inline-formula><mml:math id="M196" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> is the number of species measured by the PTR-ToF-MS, <inline-formula><mml:math id="M197" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> is the OH rate constant, and <inline-formula><mml:math id="M198" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is the average concentration measured during a burn. Shown are the median, average, 25th, and 75th percentiles for all the burns reported by <xref ref-type="bibr" rid="bib1.bibx46" id="text.94"/>. The color of each bar indicates if a compound is included or missing from the MCM. Species identifications, and the isomer contributions to each detected mass, were determined by <xref ref-type="bibr" rid="bib1.bibx46" id="text.95"/> for four fuel types (Douglas fir, Engelmann spruce duff, subalpine fir, and sage) using gas chromatography pre-separation (GC-PTR-ToF-MS). Additional evidence for species identification was provided by other<?pagebreak page14885?> measurement techniques (e.g., I-CIMS, gas chromatography electron-impact mass spectrometry, and OP-FTIR). On average, the isomer contribution to a given mass measured by PTR-ToF-MS varied by only 11 %. To be consistent with <xref ref-type="bibr" rid="bib1.bibx46" id="text.96"/>, it is assumed that the NMOG contribution to each mass detected by PTR-ToF-MS follows the average distribution measured by GC-PTR-ToF-MS.</p>
      <p id="d1e3863">For most NMOGs measured by PTR-ToF-MS, the contribution to total primary OH reactivity varied by only 25 %. Notably, the contribution from the sum of monoterpenes varied by a factor &gt; 2. Monoterpenes, as well as isoprene and sesquiterpenes, were primarily emitted at the beginning of an experiment, prior to combustion, due to distillation processes associated with fuel heating <xref ref-type="bibr" rid="bib1.bibx68" id="paren.97"/>. This “distillation phase” was most pronounced in fires containing greater amounts of canopy material, or fuel types known to be strong monoterpene emitters (e.g., pines). Other NMOGs were primarily emitted due to pyrolysis processes. For example, <xref ref-type="bibr" rid="bib1.bibx68" id="text.98"/> found that the proportions of NMOGs emitted during low- and high-temperature pyrolysis did not strongly vary by fuel type. In ambient fires, the contribution of monoterpenes to the total OH reactivity will likely differ from the contributions reported here, owing to the different burning process by which monoterpenes and other NMOGs are emitted. In this study, the primary monoterpene isomers measured by GC-PTR-ToF-MS for Engelmann spruce, Douglas fir, and subalpine fir were camphene, <inline-formula><mml:math id="M199" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene, <inline-formula><mml:math id="M200" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene, 3-carene, and limonene, followed by smaller amounts of tricyclene and <inline-formula><mml:math id="M201" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-terpinene (Fig. S3). No other NMOGs detected by the GC-PTR-ToF-MS produced signals at <inline-formula><mml:math id="M202" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 137, which is the primary ion used to quantify monoterpene emissions <xref ref-type="bibr" rid="bib1.bibx46" id="paren.99"><named-content content-type="pre">Fig. S3 and</named-content></xref>.</p>
      <?pagebreak page14886?><p id="d1e3911">The monoterpene distribution for Engelmann spruce (F26) was explicitly measured by GC-PTR-ToF-MS, but this was not the case for ponderosa pine (F38). To account for differences in monoterpene reactivity, the sum of monoterpenes for F26 is speciated using the distribution reported in Fig. S3a. For F38, monoterpenes are speciated using the ponderosa pine distribution reported by <xref ref-type="bibr" rid="bib1.bibx32" id="text.100"/> .  Engelmann spruce smoke measured by GC-PTR-ToF-MS had a monoterpene distribution that was 25 % <inline-formula><mml:math id="M203" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene, 21 % <inline-formula><mml:math id="M204" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene, 25 % 3-carene, 15 % <inline-formula><mml:math id="M205" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-terpinene, and <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % each of limonene and camphene. <xref ref-type="bibr" rid="bib1.bibx32" id="text.101"/> reports that the monoterpenes from ponderosa pine smoke are 10 % <inline-formula><mml:math id="M207" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene and 20 % each for <inline-formula><mml:math id="M208" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene, 3-carene, myrcene, and limonene. The MCM represents the chemistry of <inline-formula><mml:math id="M209" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene, <inline-formula><mml:math id="M210" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene, and limonene but does not explicitly describe other important monoterpenes (e.g., 3-carene or camphene). For the mini-chamber model, the fraction attributed to <inline-formula><mml:math id="M211" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene, <inline-formula><mml:math id="M212" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene, and limonene are explicitly prescribed. The fraction of 3-carene, <inline-formula><mml:math id="M213" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-terpinene, and smaller monoterpenes are lumped to <inline-formula><mml:math id="M214" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene (endocyclic double bond) and the fractions associated with myrcene <inline-formula><mml:math id="M215" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> camphene are lumped to <inline-formula><mml:math id="M216" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-pinene (exocyclic double bond).</p>
      <p id="d1e4023">On average, the MCM v. 3.3.1 captures only <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> % of the primary OH reactivity measured by the PTR-ToF-MS. The MCM generally lacks information about furan species and substituted aromatics, such as guaiacol and methyl guaiacol. Previous work has shown that furans constitute a significant fraction of the total primary OH reactivity <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx32 bib1.bibx33 bib1.bibx46" id="paren.102"><named-content content-type="pre">e.g.,</named-content></xref>; however, no studies have included the known mechanisms of these species when modeling biomass burning smoke chemistry. In this study, 5-methylfurfural and 2,5-dimethylfuran represent the two largest contributors to this “missing reactivity” and account for nearly 10 % of the calculated total reactivity. Up to 75 % of the calculated primary OH reactivity can be accounted for by including the chemistry of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol, along with the known species represented in the MCM. Much of the remaining reactivity is tied into species whose chemistry has not been extensively studied, including less abundant furans and oxygenated aromatics.</p>
      <p id="d1e4041">The mechanisms of select furan and oxygenated species are incorporated to the MCM based on previous work summarized in Figs. S4–S10 <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx6 bib1.bibx8 bib1.bibx9 bib1.bibx73 bib1.bibx85" id="paren.103"/>. In total, 65 reactions are added. The products resulting from the OH oxidation of furan and 2-methylfuran were first investigated by <xref ref-type="bibr" rid="bib1.bibx15" id="text.104"/> and later generalized to 3-methylfuran, 2,3-dimethylfuran, and 2,5-dimethylfuran by <xref ref-type="bibr" rid="bib1.bibx9" id="text.105"/> and <xref ref-type="bibr" rid="bib1.bibx73" id="text.106"/>. Figure <xref ref-type="fig" rid="Ch1.F5"/> shows the generalized furan oxidation scheme. Furan oxidation is initiated by an OH addition to the 2, 5, or 3 position. Addition to the 2 or 5 position is most favorable and results in pathways where substituents are either retained or lost (henceforth referred to as the loss and retention pathways). The retention pathway (path a in Fig. <xref ref-type="fig" rid="Ch1.F5"/>) leads to reactive unsaturated 1,4-dicarbonyls (e.g., 1,4-butenedial from furan oxidation), whereas the loss pathway (paths b1 and b2 in Fig. <xref ref-type="fig" rid="Ch1.F5"/>) results in the formation of hydroxy furanones and unsaturated carbonyl acids <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx73" id="paren.107"/>. The loss pathway becomes more dominant with higher number of substituted methyl groups.This study assumes branching ratios of [0.7 (a), 0.3 (b1)] for furan, [0.31 (a), 0.39 (b1), 0.31 (b2)] for 2-methylfuran, and [0.27 (a), 0.73 (b1)] for 2,5-dimethylfuran <xref ref-type="bibr" rid="bib1.bibx9" id="paren.108"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e4071">Summary of OH oxidation pathways and final products for furan, 2-methylfuran, and 2,5-dimethylfuran, where branch <bold>(a)</bold> is the substituent-retention pathway, and branches <bold>(b1)</bold> and <bold>(b2)</bold> are substituent-loss pathways <xref ref-type="bibr" rid="bib1.bibx9" id="paren.109"><named-content content-type="pre">adapted from</named-content></xref>. In this study, the branching ratios are assumed to be [0.7 <bold>a</bold>, 0.3 <bold>b1</bold>] for furan, [0.31 <bold>a</bold>, 0.39 <bold>b1</bold>, 0.31 <bold>b2</bold>] for 2-methylfuran, and [0.27 <bold>a</bold>, 0.73 <bold>b1</bold>] for 2,5-dimethylfuran. Details of the assumed <inline-formula><mml:math id="M218" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reaction schemes are provided in Figs. S4–S6.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f05.png"/>

          </fig>

      <p id="d1e4129"><inline-formula><mml:math id="M219" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions leading to the formation of carbonyls are implemented based on the mechanisms proposed by <xref ref-type="bibr" rid="bib1.bibx9" id="text.110"/> and
<xref ref-type="bibr" rid="bib1.bibx14" id="text.111"/> (Figs. S4–S6). It is assumed that <inline-formula><mml:math id="M220" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species undergo reactions with <inline-formula><mml:math id="M221" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, and other <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals. Other pathways, such as <inline-formula><mml:math id="M224" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M225" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, are not included; however, these reactions could be important for acyl <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species <xref ref-type="bibr" rid="bib1.bibx57 bib1.bibx62" id="paren.112"/>. For <inline-formula><mml:math id="M227" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> reactions, it is assumed that the alkoxy radical quickly decays (either by thermal degradation or reaction with <inline-formula><mml:math id="M228" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) to form carbonyls. <xref ref-type="bibr" rid="bib1.bibx9" id="text.113"/> did not report species consistent with alkoxy isomerization; thus, these reactions are ignored. Similarly,  <inline-formula><mml:math id="M229" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions are assumed to only form alkoxy radicals, which may subsequently degrade to form carbonyls. Peroxides are assumed to be the only products of <inline-formula><mml:math id="M230" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions. These species are assumed to undergo photolysis to form carbonyls. Peroxides may also react with OH, and the resulting products differ depending on structure. For structures with an alpha hydrogen, it is assumed that OH abstracts at the alpha position, and that the resulting radical quickly decomposes to form a carbonyl <inline-formula><mml:math id="M231" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH (e.g., HYDFURANOOH, Fig. S4). For other structures, it is assumed that the hydrogen of the peroxide group is abstracted to regenerate the <inline-formula><mml:math id="M232" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radical.</p>
      <?pagebreak page14887?><p id="d1e4324">The generic MCM rate constants are applied for <inline-formula><mml:math id="M233" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> reactions (<inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.7</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">360</mml:mn><mml:mo>/</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M236" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molec.<inline-formula><mml:math id="M237" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math id="M239" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2.91</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:msup><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1300</mml:mn><mml:mo>/</mml:mo><mml:mi>T</mml:mi><mml:mo>)</mml:mo><mml:mo>[</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mi>exp⁡</mml:mi><mml:mo>(</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.245</mml:mn><mml:mi>n</mml:mi><mml:mo>)</mml:mo><mml:mo>]</mml:mo></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M240" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molec. <inline-formula><mml:math id="M241" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M242" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). The <inline-formula><mml:math id="M243" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> rate constant is adjusted for the <inline-formula><mml:math id="M244" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> carbon number, <inline-formula><mml:math id="M245" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, as recommended by <xref ref-type="bibr" rid="bib1.bibx66" id="text.114"/>. Photolysis frequencies for peroxides are assumed to be the same as for methyl hydroperoxide (<inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:msub><mml:mi>J</mml:mi><mml:mn mathvariant="normal">41</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the MCM), and peroxide <inline-formula><mml:math id="M247" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH reactions are assumed to have a rate constant of <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M249" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molec.<inline-formula><mml:math id="M250" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M251" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. The assumed rate constants for  <inline-formula><mml:math id="M252" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions are chosen based on those of structurally similar <inline-formula><mml:math id="M253" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals reported in the MCM. <inline-formula><mml:math id="M254" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> H-shift isomerization (autoxidation) is not broadly represented in MCM v. 3.3.1, aside for isoprene oxidation <xref ref-type="bibr" rid="bib1.bibx44" id="paren.115"/>.  <inline-formula><mml:math id="M255" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> isomerization becomes competitive when the bimolecular lifetime of <inline-formula><mml:math id="M256" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is on the order of 10 s <xref ref-type="bibr" rid="bib1.bibx23 bib1.bibx63" id="paren.116"/>. Based on the modeled concentrations of <inline-formula><mml:math id="M257" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M258" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M259" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, the bimolecular lifetime of <inline-formula><mml:math id="M260" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals from furan oxidation is estimated to be <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> s; consequently, <inline-formula><mml:math id="M262" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> isomerization could play a role for certain species.</p>
      <p id="d1e4779">Following <inline-formula><mml:math id="M263" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reaction, it is assumed that the second-generation products continue through the chemistry prescribed by MCM v. 3.3.1. Unsaturated dicarbonyls, such as 1,4-butenedial, and the tautomers of hydroxy furanones are represented in the MCM (Figs. S4–S6). Here, it is assumed that hydroxy furanones undergo the same reactions as the corresponding tautomer, which ultimately leads to anhydride formation. Maleic anhydride is a multigenerational product in the OH oxidation of furan <xref ref-type="bibr" rid="bib1.bibx15" id="paren.117"/> and is considered to be a significant product of hydroxy furanone oxidation <xref ref-type="bibr" rid="bib1.bibx14" id="paren.118"/>.</p>
      <p id="d1e4799">No experimental studies have evaluated the OH oxidation mechanism of furfural or 5-methylfurfural. <xref ref-type="bibr" rid="bib1.bibx85" id="text.119"/> found via theoretical quantum chemistry calculations that OH likely adds to the 2 or 5 position or abstracts a hydrogen from the aldehyde. The resulting reactions follow loss and retention pathways similar to the general mechanism for methyl-substituted furans (Fig. <xref ref-type="fig" rid="Ch1.F6"/>). When OH adds to the 2 position, the ring most likely opens to form an unsaturated tri-carbonyl (retention, path a). When OH adds to the 5 position, the resulting peroxy radical may react with <inline-formula><mml:math id="M264" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M265" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, or other <inline-formula><mml:math id="M266" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species to form a hydroxy furanone <inline-formula><mml:math id="M267" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> carbonyl acid mixture (loss, path b). Hydrogen abstraction from the aldehyde group is believed to ultimately result in the formation of maleic anhydride (loss, path c). <xref ref-type="bibr" rid="bib1.bibx85" id="text.120"/> estimate furfural <inline-formula><mml:math id="M268" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH branching ratios of 0.37 for channel (a), 0.6 for channel (b), and 0.03 for channel (c). The same branching ratios are applied here, but a discussion of secondary NMOG sensitivity to the assumed furfural mechanism is provided in the Supplement. The 5-methylfurfural <inline-formula><mml:math id="M269" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> OH mechanism has not been studied and is assumed to have branching ratios similar to furfural. <inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions are implemented based on the mechanisms proposed by <xref ref-type="bibr" rid="bib1.bibx85" id="text.121"/> (see Figs. S7–S9).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e4878">Summary of OH oxidation pathways and final products for furfural and 5-methylfurfural, where branch <bold>(a)</bold> is the substituent-retention pathway, and branches <bold>(b)</bold> and <bold>(c)</bold> are substituent-loss pathways <xref ref-type="bibr" rid="bib1.bibx85" id="paren.122"><named-content content-type="pre">adapted from</named-content></xref>. The branching ratios estimated by <xref ref-type="bibr" rid="bib1.bibx85" id="text.123"/> are 0.37 for channel <bold>(a)</bold>, 0.6 for channel <bold>(b)</bold>, and 0.03 for channel <bold>(c)</bold>. Details of the assumed RO<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> reaction schemes are provided in Figs. S7–S9.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f06.png"/>

          </fig>

      <p id="d1e4924">Furfural strongly absorbs at 185 and 254 nm <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx34 bib1.bibx25" id="paren.124"/>. Smaller amounts may be lost by photolysis at wavelengths &gt; 300 nm <xref ref-type="bibr" rid="bib1.bibx22" id="paren.125"/>. Approximately 15 % of furfural photolysis leads to the formation of furan and CO, while the remaining percentage results in the formation of propyne, CO, and other <inline-formula><mml:math id="M272" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds <xref ref-type="bibr" rid="bib1.bibx28" id="paren.126"/>. The photolysis frequency is calculated based on the cross sections reported by <xref ref-type="bibr" rid="bib1.bibx25" id="text.127"/> and quantum yield of 0.6 (Vassilis Papadimitriou, personal communication, 2018).</p>
      <p id="d1e4950">Few studies have evaluated the OH oxidation mechanism of guaiacol. <xref ref-type="bibr" rid="bib1.bibx77" id="text.128"/> identified products from low-<inline-formula><mml:math id="M273" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> guaiacol oxidation but did not calculate product yields. <xref ref-type="bibr" rid="bib1.bibx48" id="text.129"/> studied guaiacol oxidation in the presence of <inline-formula><mml:math id="M274" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and observed substantial SOA formation. The only reported gas-phase species were a suite of nitroguaiacols composed primarily of 3- and 6-nitroguaiacol (6 % yield) and 4-nitroguaiacol (10 % yield). The mechanism proposed by <xref ref-type="bibr" rid="bib1.bibx48" id="text.130"/> is applied here assuming a 16 % yield of nitroguaiacol species (Fig. S10).</p>
      <p id="d1e4984">The OH loss of butanol-d9 is also included in the model to validate OH concentrations in the chamber. The OH oxidation of butanol-d9 is assumed to form a single, nonreactive species. The entire mechanism used to model the mini-chamber and ambient biomass burning plume is provided in the Supplement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><label>Figure 7</label><caption><p id="d1e4989">Primary NMOG measurements (blue lines) compared to modeled output (dotted black lines) for Fire 38. The decay of butanol-d9 is shown to demonstrate model performance in reproducing OH exposures, which was achieved by adjusting the measured photon flux by a factor of 1.5. The fuel is ponderosa pine litter, <inline-formula><mml:math id="M275" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>/NMOG <inline-formula><mml:math id="M276" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.3, with a mixture of high- and low-temperature pyrolysis products.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f07.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Model and measurement evaluation</title>
      <p id="d1e5024">Figure <xref ref-type="fig" rid="Ch1.F7"/> shows the model comparison with PTR-ToF-MS measurements of butanol-d9 and select primary NMOGs for F38. Overall, there is good agreement between the measurements and model output for most NMOGs (exceptions include some primary species and small secondary oxygenates, discussed below). The excellent agreement between the measured and modeled loss of butanol-d9 demonstrates that OH concentrations in the chamber are well-represented by the model. Similar agreement is observed for F26, which had an initial <inline-formula><mml:math id="M277" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NMOG</mml:mi></mml:mrow></mml:math></inline-formula> ratio that was an order of magnitude lower than that of F38 (Fig. S11). Figure <xref ref-type="fig" rid="Ch1.F8"/> shows the model output compared to the observed profiles of secondary NMOGs measured during F38. The equivalent for F26 is presented in Fig. S12. Figure <xref ref-type="fig" rid="Ch1.F8"/>a shows measurements of <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (maleic anhydride) as measured by PTR-ToF-MS, whereas Fig. <xref ref-type="fig" rid="Ch1.F8"/>b and c show I-CIMS measurements of <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M280" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, respectively. The measured secondary NMOGs are compared to model outputs of total <inline-formula><mml:math id="M281" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (i.e., the sum of all species with molecular formula <inline-formula><mml:math id="M282" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), total <inline-formula><mml:math id="M283" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, total <inline-formula><mml:math id="M284" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and individual NMOGs. Figure <xref ref-type="fig" rid="Ch1.F8"/> also show model runs with the initial conditions of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and furanone set to zero. The PTR-ToF-MS measurements of <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are reported in units of ppb and can therefore be quantitatively compared to model output.<?pagebreak page14888?> I-CIMS measurements are reported as ncps; consequently, only qualitative comparisons are drawn based on similarities in model and measurement temporal profiles.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><label>Figure 8</label><caption><p id="d1e5224">Secondary NMOG measurements compared to modeled output for Fire 38. Row <bold>(a)</bold> shows PTR-ToF-MS measurements of <inline-formula><mml:math id="M286" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compared to model output of maleic anhydride. Row <bold>(b)</bold> shows I<inline-formula><mml:math id="M287" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>-ToF-CIMS measurements of <inline-formula><mml:math id="M288" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compared to model output of methyl hydroxy furanone and its tautomer: <inline-formula><mml:math id="M289" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-acetylacrylic acid. Row <bold>(c)</bold> shows I<inline-formula><mml:math id="M290" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>-ToF-CIMS measurements of <inline-formula><mml:math id="M291" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compared to model output of hydroxy furanone, its tautomer malealdehydic acid, and 2,3-dioxobutanal. All graphs to the left show full model runs, while graphs to the right show model runs when the initial conditions of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and furanone are set to zero.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f08.png"/>

          </fig>

      <p id="d1e5331"><inline-formula><mml:math id="M292" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M293" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M294" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> were shown in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/> to constitute some of the most abundant photochemical products observed by PTR-ToF-MS and I-CIMS. The model runs in Figs. <xref ref-type="fig" rid="Ch1.F8"/> and  S12 demonstrate that furan chemistry significantly contributes to the modeled formation of these secondary NMOGs. The model also supports the inference that these masses correspond to measurements of maleic anhydride, methyl hydroxy furanone, and hydroxy furanone, respectively. This is most evident by comparing the shape of the temporal profiles between the measurements and modeled output. Maleic anhydride is the only species in the MCM with chemical formula <inline-formula><mml:math id="M295" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and the model generally captures the peak <inline-formula><mml:math id="M296" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> signal after <inline-formula><mml:math id="M297" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> min of oxidation to within the uncertainty of the measurement (<inline-formula><mml:math id="M298" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> %). Several species with chemical formula <inline-formula><mml:math id="M299" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are represented in the MCM. Here, the modeling output is dominated by methyl hydroxy furanone and its tautomer, <inline-formula><mml:math id="M300" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>-acetylacrylic acid. Finally, I-CIMS measurements of <inline-formula><mml:math id="M301" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are best captured by the model output of hydroxy furanone and its tautomer, malealdehydic acid.</p>
      <p id="d1e5513">The temporal profile of <inline-formula><mml:math id="M302" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is also well-described by model output of nitroguaiacol (Fig. S13). Nitroaromatics are formed by the reaction of <inline-formula><mml:math id="M303" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> with the o-semiquinone radical resulting from OH abstraction of the phenolic hydrogen <xref ref-type="bibr" rid="bib1.bibx26" id="paren.131"/>. <inline-formula><mml:math id="M304" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> was abundant at the beginning of mini-chamber experiments initialized with NMOGs resulting from flaming emissions (Fig. S2); thus, nitroaromatics are expected to be present in many burns studied here. Note that only the results from F38 are shown. Very little formation of nitroguaiacol was observed in F26, owing to the relatively low amount of <inline-formula><mml:math id="M305" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> emitted from the smoldering combustion of Engelmann spruce duff.</p>
      <p id="d1e5573">The model provides insights into the formation pathways of important secondary NMOGs, which could be used to place constraints on plume properties. For example, measurements of maleic anhydride, hydroxy furanone, and methyl hydroxy furanone could be used as proxies to estimate plume age since the furanones will likely be enhanced in younger plumes, whereas maleic anhydride will likely be enhanced in aged plumes. In plumes containing high proportions of furans, it could be feasible to evaluate furan chemistry to derive important modeling constraints, such as OH exposures.</p>
      <p id="d1e5576">Despite the success of the model in reproducing a number of observations, several differences exist, as described below. First, the model output exhibits a faster decay of furans than what is observed by PTR-ToF-MS (Fig. <xref ref-type="fig" rid="Ch1.F7"/>). This likely reflects the uncertainty associated with the mass assignment of furan species. Using GC-PTR-ToF-MS, <xref ref-type="bibr" rid="bib1.bibx46" id="text.132"/> showed that nearly 50 % of the primary signal at <inline-formula><mml:math id="M306" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M307" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (mass of 2-methylfuran) and <inline-formula><mml:math id="M308" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M309" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> (mass of 2,5-dimethylfuran) is associated with unidentified oxygenates. These unidentified species likely have different reactivities towards OH which may lead to model and observation<?pagebreak page14889?> disagreement. Likewise, secondary NMOG isomers could also form at these masses, further confounding model predictions of furans.</p>
      <p id="d1e5643">The decay of furfural is distinct from other furans because several processes contribute to temporal profile of <inline-formula><mml:math id="M310" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. Notably, there appears to be a fast decay of <inline-formula><mml:math id="M311" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, followed by a slower decay after 10s of oxidation. The model generally captures the fast decay of <inline-formula><mml:math id="M312" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, which is almost entirely due to photolysis of furfural. This degree of photolysis is different from the real atmosphere and results from furfural's exceptionally large cross section at 254 nm <xref ref-type="bibr" rid="bib1.bibx25" id="paren.133"><named-content content-type="pre">&gt;  <inline-formula><mml:math id="M313" display="inline"><mml:mrow><mml:mn mathvariant="normal">5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">17</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M314" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>,</named-content></xref>. The slower decay appears to result from an interference of another NMOG. This is supported by the I-CIMS, which measured the formation of a mass with formula <inline-formula><mml:math id="M315" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">I</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. The I-CIMS is not sensitive to primary furan species, therefore this species is likely to be a secondary NMOG that is isomeric with furfural. This may explain why PTR-ToF-MS measurements of <inline-formula><mml:math id="M316" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> do not quickly decay to zero, as suggested by the model. It is notable that the formation of this secondary species is significant (<inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> % of the signal of primary furfural), which indicates that this is likely a secondary product formed from an abundant primary NMOG.</p>
      <p id="d1e5829">Despite the complications imposed by furfural photolysis, other furans and oxygenated aromatics do not exhibit strong absorption and are expected to be lost mostly by reaction with OH. Other absorbing species, such as methyl ethyl ketone and benzaldehyde, exhibit modeled photolysis losses on the order of 30 %, which is likely a more typical fraction for other photo-active species. More details comparing the chamber results to chemistry of ambient biomass burning plumes are provided in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS3"/>.</p>
      <?pagebreak page14890?><p id="d1e5834">At the beginning of each experiment, PTR-ToF-MS measurements show a sharp increase in <inline-formula><mml:math id="M318" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that is not readily captured by the model (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). This increase could result from fast formation of maleic anhydride, or is possibly another species with molecular formula <inline-formula><mml:math id="M319" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The model underpredicts maleic anhydride mixing ratios towards the end of the experiment, which likely points to additional sources of maleic anhydride that are not included in the model. The model reproduces peak maleic anhydride mixing ratios in F38 (Fig. <xref ref-type="fig" rid="Ch1.F8"/>a) but overpredicts peak maleic anhydride mixing ratios by a factor of 1.6 in F26 (Fig. S12a).</p>
      <p id="d1e5884">After <inline-formula><mml:math id="M320" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> min of oxidation, the model sum of <inline-formula><mml:math id="M321" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> approaches zero, yet the I-CIMS signal remains elevated (Fig. <xref ref-type="fig" rid="Ch1.F8"/>c). This may indicate that a slow-forming product is detected by I-CIMS, or that the OH rate constant of hydroxy furanone is overestimated. As discussed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS1"/>, the PTR-ToF-MS detects a slow-forming product that likely corresponds to succinic anhydride (Fig. <xref ref-type="fig" rid="Ch1.F1"/>). The I-CIMS is sensitive to anhydrides; thus, it is possible that the elevated signal at longer oxidation timescales corresponds to the measurement of succinic anhydride. Succinic anhydride is not represented in the customized mechanism; consequently, no model output is available for comparison.</p>
      <p id="d1e5924">Figure <xref ref-type="fig" rid="Ch1.F2"/> shows that small oxygenates are also abundant secondary NMOGs (i.e., acetaldehyde and formaldehyde); however, these species are underpredicted by the model by a factor of 10 or more (Fig. S13). This likely reflects additional chemical precursors or chemical pathways that are unaccounted for within the mini-chamber model. Furthermore, heterogeneous reactions, such as those on aerosol particles or Teflon surfaces <xref ref-type="bibr" rid="bib1.bibx83 bib1.bibx21" id="paren.134"><named-content content-type="pre">e.g.,</named-content></xref> or photolysis at 254 nm may contribute to the formation of these small oxygenates.</p>
      <p id="d1e5934">It is noted that without calibrated I-CIMS data it is difficult to assess whether the budget of these secondary NMOGs is fully represented by the model. Although it is expected that furans will be a primary precursor of <inline-formula><mml:math id="M322" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M323" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in real biomass burning plumes, the model indicates that other highly reactive species may also contribute to these masses. In F38, furans account for <inline-formula><mml:math id="M324" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> % of the modeled production of <inline-formula><mml:math id="M325" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M326" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">90</mml:mn></mml:mrow></mml:math></inline-formula> % of the modeled production of <inline-formula><mml:math id="M327" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. In contrast, furans account for <inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> % of the modeled production of <inline-formula><mml:math id="M329" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">85</mml:mn></mml:mrow></mml:math></inline-formula> % of the modeled production of <inline-formula><mml:math id="M331" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during F26. The remaining production in the model is attributed to the OH oxidation of oxygenated aromatics – specifically, phenol and cresol. These oxygenated aromatics are more abundant during F26 due to the higher degree of smoldering combustion. These differences highlight the variability of secondary NMOG production and also imply that there could be remaining precursors of <inline-formula><mml:math id="M332" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M333" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. These precursors would have to be highly reactive molecules with a carbon number of <inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>. There are a number of furans and oxygenated aromatics that could possibly contribute to the formation of these secondary NMOGs (e.g., hydroxymethylfurfural, Fig. <xref ref-type="fig" rid="Ch1.F4"/>) but whose chemical mechanism remains unknown.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Comparison of chamber chemistry to atmospheric conditions</title>
      <p id="d1e6167">The high-OH environment in the mini-chamber is similar to those produced in oxidation flow reactors. <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx62" id="text.135"/> showed that oxidation flow reactors can be operated under conditions that approximate the chemistry of the atmosphere; however, the use of 254 nm light can lead to non-atmospheric reactions. For example, furfural photolysis is unlikely to play a significant role in the chemistry of real smoke, and <inline-formula><mml:math id="M335" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> cycling is faster under ambient photolysis. Furthermore, high-OH environments may lead to <inline-formula><mml:math id="M336" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fates that differ from ambient systems. In the atmosphere, the predominant fate of <inline-formula><mml:math id="M337" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is reaction with NO or <inline-formula><mml:math id="M338" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. In wildfires, <inline-formula><mml:math id="M339" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions with <inline-formula><mml:math id="M340" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> are also important in forming PAN and other peroxy nitrates <xref ref-type="bibr" rid="bib1.bibx4" id="paren.136"/>. In low-<inline-formula><mml:math id="M341" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> environments, <inline-formula><mml:math id="M342" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M343" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> isomerization may also play a role <xref ref-type="bibr" rid="bib1.bibx23 bib1.bibx63" id="paren.137"/>. <inline-formula><mml:math id="M344" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> isomerization was not included in the mechanism described here. The following discussion compares the modeled chemistry in the chamber to that expected for an ambient biomass burning plume.</p>
      <p id="d1e6298">In the atmosphere, primary NMOGs are mostly consumed by reaction with OH or via photolysis during the daytime, and reaction with <inline-formula><mml:math id="M345" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M346" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at night. Table S4 shows the estimated contribution of each process to the primary NMOGs measured during F26 and F38. Also shown are the NMOG losses calculated from simulations of the ambient biomass burning plume described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.138"/>; see Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS4"/> for details of this modeling. For most species, the predominant loss pathway is reaction with OH. Ozonolysis is negligible, except for a small fraction of the monoterpenes (<inline-formula><mml:math id="M347" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> %). On the other hand, significant NMOG losses occur by photolysis, and to a lesser extent, reaction by <inline-formula><mml:math id="M348" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Aside from furfural, loss by photolysis was dominant for acetone and 2,3-butanedione (&gt; 50 %), significant for methyl ethyl ketone and benzaldehyde (<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> %), and moderate for hydroxyacetone, glyoxal, methyl glyoxal, formaldehyde, and acetaldehyde (&lt; 10 %). In general, photolysis losses were dependent on the relative ratio between the OH rate constant and photolysis frequency at 254 nm (Table S3). Photolysis losses were greatest for conjugated aldehydes and species with low OH rate constants and high-absorption cross sections. (e.g., acetone, Table S3). Conjugated aldehydes such as furfural are highly reactive towards OH; consequently, losses due to photolysis are notable since these processes represent unintended sinks of potentially important SOA and ozone precursors. In contrast, photolysis losses of other species, such as acetone, are likely less important since these species are less reactive towards OH. It is noted that other species reported here are likely to photolyze, but their absorption cross sections at 254 nm have not been measured <xref ref-type="bibr" rid="bib1.bibx22" id="paren.139"><named-content content-type="pre">e.g., 5-methylfurfural,</named-content></xref>.</p>
      <?pagebreak page14891?><p id="d1e6365">Because numerous species absorb across a wide wavelength spectrum <xref ref-type="bibr" rid="bib1.bibx19" id="paren.140"><named-content content-type="pre">e.g., acetaldehyde and hydroxyacetone</named-content></xref>, there is some agreement between the photolysis losses estimated in the mini-chamber with those expected under ambient conditions. For hydroxyacetone, 2,3-butanedione, and acetaldehyde, reaction by photolysis was comparable to what was estimated for the ambient biomass burning plume described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.141"/>. In contrast, conjugated aldehydes, such as furfural and benzaldehyde, are characterized with absorption cross sections that favor shorter wavelengths; consequently, photolysis losses in the mini-chamber greatly exceed those expected in ambient plumes. These results highlight the challenges associated with studying multiday oxidation of biomass burning smoke in environmental chambers. Biomass burning emissions contain a myriad of functionalized NMOGs that readily photolyze at wavelengths required to generate high-OH environments. Experimental setups employing UVC lights must weigh the options of operating at high OH exposures (and thus progressing through chemistry quickly) or operating at gradual OH exposures that allow for longer sampling but higher exposures to UVC light. Similar considerations are made for oxidation flow reactors, although nearly all experiments are conducted at high-OH exposures since sampling is conducted at pseudo-steady-state <xref ref-type="bibr" rid="bib1.bibx61" id="paren.142"/>. To avoid high photolysis exposures, future experiments employing 254 nm light may consider operating with higher ozone mixing ratios to increase the losses due to reaction by OH. Alternatively, chamber experiments operated at high relative humidity may employ 185 nm light to generate high-OH environments <xref ref-type="bibr" rid="bib1.bibx61" id="paren.143"/>. In both cases, the chemistry will progress quickly, which may be undesirable for chamber experiments using low time resolution instrumentation. Another approach may be to use UVB or UVA lights and photolyze HONO to generate OH. This approach will reduce photolysis exposures but may only access 1–2 d of atmospheric-equivalent oxidation.</p>
      <p id="d1e6382">Unlike primary emissions that are dependent on the balance between photolysis and oxidant concentrations, the formation of secondary NMOGs largely depends on the fate of the <inline-formula><mml:math id="M350" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radical. Figure <xref ref-type="fig" rid="Ch1.F9"/>a and b show a breakdown of the modeled <inline-formula><mml:math id="M351" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways that contributed to the chemistry of the mini-chamber. The bars show the fraction <inline-formula><mml:math id="M352" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals, separated by carbon number, that reacted through <inline-formula><mml:math id="M353" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M354" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M355" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M356" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways. Figure <xref ref-type="fig" rid="Ch1.F9"/>c shows the breakdown of <inline-formula><mml:math id="M357" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways for simulations of the ambient biomass burning plume.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><label>Figure 9</label><caption><p id="d1e6506">The fate of <inline-formula><mml:math id="M358" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species for <bold>(a)</bold> F26, <bold>(b)</bold> F38, and <bold>(c)</bold> the ambient biomass burning plume described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.144"/>. <inline-formula><mml:math id="M359" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species are grouped by carbon number, and the color of each bar shows the fraction of <inline-formula><mml:math id="M360" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species reacted by <inline-formula><mml:math id="M361" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M362" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M363" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M364" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> pathways. </p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f09.png"/>

          </fig>

      <p id="d1e6629"><inline-formula><mml:math id="M365" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals in F38 largely reacted through two pathways: <inline-formula><mml:math id="M366" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M367" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The <inline-formula><mml:math id="M368" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathway primarily influenced the fate of smaller <inline-formula><mml:math id="M369" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals (C<inline-formula><mml:math id="M370" display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula>3), leading to the formation of peroxy nitrates (specifically, PAN). For larger <inline-formula><mml:math id="M371" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals (<inline-formula><mml:math id="M372" display="inline"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>≥</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>), the dominant pathway was <inline-formula><mml:math id="M373" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. On the other hand, the model suggests that the <inline-formula><mml:math id="M374" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathway played a significant role in the chemistry of F26. This results, in part, from the higher initial NMOG loading for F26 (<inline-formula><mml:math id="M375" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">280</mml:mn></mml:mrow></mml:math></inline-formula> ppb) compared to that of F38 (<inline-formula><mml:math id="M376" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">180</mml:mn></mml:mrow></mml:math></inline-formula> ppb), which enhanced the rate of <inline-formula><mml:math id="M377" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> production. The model suggests that the relative contribution of <inline-formula><mml:math id="M378" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cross-reactions was lower for higher-carbon species; however, it is possible that these reactions produced accretion products unlikely to be found under ambient conditions. As discussed in Sect. <xref ref-type="sec" rid="Ch1.S2.SS3.SSS2"/> and shown in Fig. S2, F26 was not representative of most fires studied here. For the majority of fires presented in Figs. <xref ref-type="fig" rid="Ch1.F2"/> and <xref ref-type="fig" rid="Ch1.F3"/>, the secondary NMOGs were likely formed through the pathways consistent with F38.</p>
      <?pagebreak page14892?><p id="d1e6824">In general, most of the higher-carbon species in F38 followed atmospherically relevant pathways. For some species,  <inline-formula><mml:math id="M379" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> reactions were also observed. While initial NMOG loadings may explain part of the enhanced <inline-formula><mml:math id="M380" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> rate, some fraction may also be attributed to the limited degree of <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> cycling in the mini-chamber. Under ambient conditions, <inline-formula><mml:math id="M382" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is photolyzed to <inline-formula><mml:math id="M383" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula>, which then reacts with <inline-formula><mml:math id="M384" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (and <inline-formula><mml:math id="M385" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) radicals. Consequently, the <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> + <inline-formula><mml:math id="M387" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> pathway may act to lower the fraction of radicals that follow the <inline-formula><mml:math id="M388" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathway. This is evidenced by the biomass burning plume described by  <xref ref-type="bibr" rid="bib1.bibx56" id="text.145"/>, which shows that the <inline-formula><mml:math id="M389" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> pathway is the dominant fate for most <inline-formula><mml:math id="M390" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species under ambient photolysis. In the mini-chamber, <inline-formula><mml:math id="M391" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> does not strongly absorb at 254 nm and is quickly lost to PAN or <inline-formula><mml:math id="M392" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; consequently, <inline-formula><mml:math id="M393" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> does not play a significant role in the chemistry of higher-carbon <inline-formula><mml:math id="M394" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals.</p>
      <p id="d1e7027">The primary focus of this study is to understand the formation of major secondary NMOGs measured by I-CIMS; thus, it is instructive to identify the modeled radical pathways that contribute to these formation rates. Figure S14 shows the pathways for the radicals that lead to the formation of hydroxy furanone and methyl hydroxy furanone. For both experiments, the hydroxy furanone radicals predominantly react through <inline-formula><mml:math id="M395" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways. For F26, <inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> % of the <inline-formula><mml:math id="M397" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals react through the <inline-formula><mml:math id="M398" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathways, whereas <inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> % follow this pathway for F38. These results suggest that the <inline-formula><mml:math id="M400" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathway played some role in both experiments but that the formation of hydroxy furanones in F38 predominantly followed atmospherically relevant pathways. It is noted that, as with other <inline-formula><mml:math id="M401" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals, these species are expected to mostly react with <inline-formula><mml:math id="M402" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> under ambient conditions (Fig. S14). Despite this difference, the <inline-formula><mml:math id="M403" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> pathway and the <inline-formula><mml:math id="M404" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> pathway are both expected to lead to hydroxy furanone formation (Figs. S4 and S5).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <label>3.2.4</label><title>Observations and box modeling of secondary NMOGs in real biomass burning plumes</title>
      <p id="d1e7176">Section <xref ref-type="sec" rid="Ch1.S3.SS2.SSS3"/> shows that the radical pathways in the mini-chamber exhibited similarities, as well as differences, to those expected under atmospheric photolysis. In order to evaluate the impact of furan chemistry under ambient conditions, this work builds upon the model described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.146"/> to evaluate the customized MCM mechanism with measurements from a real biomass burning plume.</p>
      <p id="d1e7184">During the 2013 DISCOVER-AQ aircraft campaign, the NASA P-3B conducted several plume intercepts downwind of a controlled burn conducted in a mixed-forested ecosystem. NMOGs were monitored by a PTR-ToF-MS, meteorological parameters (temperature, pressure, and relative humidity) were monitored by a suite of aircraft instrumentation, and <inline-formula><mml:math id="M405" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M406" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> were monitored by chemiluminescence. <xref ref-type="bibr" rid="bib1.bibx56" id="text.147"/> modeled the chemical evolution of NMOGs using a semi-Lagrangian box model with a modified MCM mechanism that included a basic oxidation scheme for furan and furfural. The authors successfully modeled the loss of primary NMOGs, including furan and furfural, and captured trends in ozone, <inline-formula><mml:math id="M407" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and peroxyacetyl nitrate (PAN). Downwind of the fire, the authors observed the formation of NMOGs, such as maleic anhydride, which could not be explained by the model.</p>
      <p id="d1e7223">The authors initialized the chemistry with measurements of NMOGs, <inline-formula><mml:math id="M408" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M409" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> sampled in close proximity of the fire. Plume dilution was constrained based on the temporal evolution of CO. Background NMOGs, <inline-formula><mml:math id="M410" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M411" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations were prescribed based on aircraft measurements conducted outside of the plume. The plume was simulated for 1 h, and meteorological parameters were constrained based on measurements conducted at each plume crossing. Photolysis was prescribed based on observed <inline-formula><mml:math id="M412" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> photolysis frequencies.</p>
      <p id="d1e7281">The analysis described <xref ref-type="bibr" rid="bib1.bibx56" id="text.148"/> is recreated here but with the full mechanisms of furan, furfural, 2,-methylfuran, 2,5-dimethylfuran, and 5-methylfurfural incorporated into the MCM. Other mechanisms that were not previously analyzed by <xref ref-type="bibr" rid="bib1.bibx56" id="text.149"/> are also considered, including phenol, cresol, and catechol. These species have important contributions to the primary OH reactivity of biomass burning smoke and are explicitly represented in MCM v. 3.3.1 (Fig. <xref ref-type="fig" rid="Ch1.F4"/>). The initial conditions of furan and furfural are prescribed based on the observed mixing ratios reported by <xref ref-type="bibr" rid="bib1.bibx56" id="text.150"/>. The mixing ratios of 2-methylfuran, phenol, and cresol are constrained based on the signals measured at <inline-formula><mml:math id="M413" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 83.05 (<inline-formula><mml:math id="M414" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M415" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M416" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 95.045 (<inline-formula><mml:math id="M417" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M418" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), and <inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 109.066 (<inline-formula><mml:math id="M420" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M421" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), respectively. The signal attributable to 2,5-dimethylfuran is isobaric with furfural and was not fully resolved by PTR-ToF-MS due to the overwhelming signal of furfural (<inline-formula><mml:math id="M422" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> times greater than the signal of other furan species). The mixing ratio of 2,5-dimethylfuran is expected to significantly contribute to total NMOG mixing ratios and OH reactivity (Fig. <xref ref-type="fig" rid="Ch1.F4"/>); therefore, the initial mixing ratio of  2,5-dimethylfuran is constrained based on the dimethylfuran <inline-formula><mml:math id="M423" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> methylfuran ratio reported elsewhere <xref ref-type="bibr" rid="bib1.bibx46" id="paren.151"><named-content content-type="pre"><inline-formula><mml:math id="M424" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>,</named-content></xref>. Finally, methylfurfural and catechol are included based on the signal at <inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 111.049 (<inline-formula><mml:math id="M426" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M427" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), and it is assumed that 50 % of the signal can be attributed to each compound as recommended by <xref ref-type="bibr" rid="bib1.bibx46" id="text.152"/>. The initial mixing ratios of methylfurfural <inline-formula><mml:math id="M428" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> catechol and cresol are adjusted to best match the decay of <inline-formula><mml:math id="M429" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M430" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M431" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula>-<inline-formula><mml:math id="M432" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, respectively.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><label>Figure 10</label><caption><p id="d1e7573">Summary of model results for the understory fire described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.153"/>. Data are presented as mixing ratios corrected for dilution (calculated based on the decay of CO). The initial conditions for methylfurfural <inline-formula><mml:math id="M433" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> catechol and cresol were adjusted to best match the observed decay. Results with furans excluded from the model are shown as dotted lines. Maleic anhydride and ozone are shown to illustrate the impact of furans on secondary product formation.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f10.png"/>

          </fig>

      <p id="d1e7592">Figure <xref ref-type="fig" rid="Ch1.F10"/> compares the model output to the dilution-corrected mixing ratios of furans, oxygenated aromatics, maleic anhydride, and ozone. The model output of hydroxy furanone is also shown but not compared to measurements since an I-CIMS was not onboard the P-3B. Red lines show the model output with furan chemistry included in the model. Dotted blue lines show model output with initial furan mixing ratios set to zero.</p>
      <p id="d1e7597">The model satisfactorily reproduces the temporal profiles of furans, oxygenated aromatic species, maleic anhydride, and ozone. The model also predicts significant formation of hydroxy furanone. Similar to the mini-chamber observations (Fig. <xref ref-type="fig" rid="Ch1.F1"/>), maleic anhydride exhibits a temporal profile that is consistent with a slow-forming product. The model output of hydroxy furanone exhibits a fast-forming temporal profile as expected from the mini-chamber experiments (Fig. <xref ref-type="fig" rid="Ch1.F1"/>).</p>
      <p id="d1e7604">The production of maleic anhydride and hydroxy furanone is negligible when the initial concentrations of furan species are set to zero. For both species, furfural oxidation accounts for more than 50 % of the total production. As discussed in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS1"/>, the furfural mechanism is based on theoretical calculations and the exact branching ratios may differ from those estimated by <xref ref-type="bibr" rid="bib1.bibx85" id="text.154"/>. The assumed branching ratios weakly impact the formation of maleic<?pagebreak page14893?> anhydride, whereas hydroxy furanone is most impacted by the assumed branching ratio of the ring-retaining pathway (channel b, Fig. S16). I-CIMS measurements of hydroxy furanone may provide better constraints on the relative importance of each pathway.</p>
      <p id="d1e7612">Good agreement between ozone measurements and model output was also observed by <xref ref-type="bibr" rid="bib1.bibx56" id="text.155"/>. Most of the ozone production results from reactions involving <inline-formula><mml:math id="M434" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (formed primarily from OH <inline-formula><mml:math id="M435" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> formaldehyde, CO, and furfural reactions), <inline-formula><mml:math id="M436" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals (formed primarily from reactions involving acetaldehyde, 2,3-butanedione, and methylglyoxal), and NO. When furans are removed from the model, predicted ozone mixing ratios decrease by 12 %. It is estimated that <inline-formula><mml:math id="M437" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> ppb of ozone was produced from furan chemistry after 60 min of oxidation. Notably, ozone formation was not sensitive to the assumed furfural branching ratios (Fig. S16). It is noted that the contribution of ozone from furan chemistry will vary depending on <inline-formula><mml:math id="M438" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> conditions and that this estimate is not equivalent to a generalized ozone formation potential.</p>
      <p id="d1e7674">The products of furan chemistry are also reactive (e.g., hydroxy furanone, 1,4-butenedial, methyl hydroxy furanone, Figs. S4–S9), and 1 h of oxidation is too short to capture the total potential ozone produced from the oxidation of furan precursors. Figure <xref ref-type="fig" rid="Ch1.F11"/> extrapolates the model forward to evaluate multigenerational oxidation processes of ozone formation. The model is extrapolated assuming that the dilution rate continues to follow an exponential decay (calculated based on the measured CO loss). The solar zenith angle and <inline-formula><mml:math id="M439" display="inline"><mml:mrow><mml:msub><mml:mi>j</mml:mi><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are calculated based on time of day. Relative humidity, temperature, and pressure are assumed to remain constant following the last measured plume intercept.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><label>Figure 11</label><caption><p id="d1e7697"><bold>(a)</bold> Total ozone, estimated ozone produced by furan chemistry, and fraction of total ozone associated with furan chemistry for the modeled biomass burning plume measured by <xref ref-type="bibr" rid="bib1.bibx56" id="text.156"/>. <bold>(b)</bold> Model predictions of 5-hydroxy-2(5H)-furanone and maleic anhydride production. Shown is an extrapolation of the 1 h model described in Sect. <xref ref-type="sec" rid="Ch1.S3.SS2.SSS4"/>. After 10 min of oxidation, furan chemistry is responsible for &gt; 15 % of total ozone production in the model. The predicted contribution from furan chemistry decreases as furans are consumed and other, slower-reacting primary NMOGs begin to oxidize. Furan chemistry contributes <inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> ppb of ozone after 4.5 h of oxidation.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f11.png"/>

          </fig>

      <p id="d1e7726">Figure <xref ref-type="fig" rid="Ch1.F11"/> shows the extrapolated modeling results of ozone, hydroxy furanone, and maleic anhydride until 17:30 local time when the solar zenith angle approaches 70<inline-formula><mml:math id="M441" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math id="M442" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> h before sunset). Hydroxy furanone production maximizes after 1 h of oxidation, and subsequently decays due to OH oxidation. In contrast, maleic anhydride continues to increase. Figure <xref ref-type="fig" rid="Ch1.F11"/>a shows the estimated ozone produced from furan chemistry (calculated as the difference between model<?pagebreak page14894?> runs initialized with and without furan species). Ozone production from furan oxidation continues to rise after 1 h of aging, in part because of the oxidation of reactive secondary NMOGs such as hydroxy furanone. After 4.5 h of oxidation, the total ozone produced from furan chemistry is <inline-formula><mml:math id="M443" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> ppb.</p>
      <p id="d1e7762">Figure <xref ref-type="fig" rid="Ch1.F11"/> demonstrates that furan chemistry contributed to the evolution of ozone within 4 h of emission. After 2 h of aging, most furans have reacted (&lt; 20 % remain), and their contribution to ozone production via reactions of secondary NMOGs diminishes. It is important to note that ozone production will vary depending on <inline-formula><mml:math id="M444" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> availability, <inline-formula><mml:math id="M445" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:mi mathvariant="normal">NMOG</mml:mi></mml:mrow></mml:math></inline-formula> ratios, the chemical composition of the NMOG mixture, and meteorological conditions. Despite these factors, furan chemistry will likely play a role in ozone production for many biomass burning plumes due to the ubiquitous presence of furans in smoke <xref ref-type="bibr" rid="bib1.bibx70 bib1.bibx71 bib1.bibx30 bib1.bibx32 bib1.bibx17 bib1.bibx31 bib1.bibx46 bib1.bibx68" id="paren.157"/>.</p>
      <p id="d1e7796">The plume described above is relatively young; however, observations from the mini-chamber (Fig. <xref ref-type="fig" rid="Ch1.F1"/>) and the continued formation of maleic anhydride in the extrapolated model suggests that this compound could be present in highly aged plumes. During the NOAA Shale Oil and Natural Gas Nexus (SONGNEX <uri>https://www.esrl.noaa.gov/csd/projects/songnex/</uri>, last access: 4 January 2018) field campaign, the NOAA WP-3D aircraft intercepted a large biomass burning plume in the free troposphere above MT, US, on 21 April 2015 <xref ref-type="bibr" rid="bib1.bibx12" id="paren.158"/>. The plume had been transported at least 4 d from wildfires in Siberia and affected large portions of the western US. The PTR-ToF-MS described in this study was also deployed on the WP-3B and the resulting measurements are presented in Fig. <xref ref-type="fig" rid="Ch1.F12"/>. The aged plume (indicated by elevated mixing ratios of acetonitrile and acetic acid) exhibited clear enhancements in maleic anhydride and <inline-formula><mml:math id="M446" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which is attributed to succinic anhydride. In contrast, furan mixing ratios did not increase above background levels, indicating that these species completely reacted before sampling by the P-3.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><label>Figure 12</label><caption><p id="d1e7832">PTR-ToF-MS measurements of a wild fire plume transported to the US from southern Siberia. The plume was intercepted 21 April 2015 during the SONGNEX field campaign and is described in detail by <xref ref-type="bibr" rid="bib1.bibx12" id="text.159"/>.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14875/2019/acp-19-14875-2019-f12.png"/>

          </fig>

      <p id="d1e7845">The lifetimes of maleic and succinic anhydride are long (&gt; 5 d at OH concentrations of <inline-formula><mml:math id="M447" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M448" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>); consequently, these species may have formed from the OH oxidation of furans and oxygenated aromatics shortly downwind of the fire and survived transport to the western US. These species may have also formed during transit from the oxidation of slow-reacting aromatics, such as benzene. The detection of anhydrides in highly aged plumes is consistent with the behavior of the mini-chamber (Fig. <xref ref-type="fig" rid="Ch1.F1"/>) and demonstrates the relevance of furans and aromatic oxidation on plume chemistry far downwind of fire sources.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e7887">This study evaluates the influence of understudied NMOG chemistry on the chemical evolution of laboratory and<?pagebreak page14895?> ambient biomass burning smoke. Smoke reacted with OH radicals exhibits fast decay of highly reactive organic species, such as furans and oxygenated aromatics, and significant formation of <inline-formula><mml:math id="M449" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M450" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> oxygenates. A model incorporating furan chemistry into the MCM (v. 3.3.1) indicates that furan and oxygenated aromatic species are significant precursors of the secondary NMOGs measured by PTR-ToF-MS and I-CIMS. Similar results are observed from modeling of a small understory fire <xref ref-type="bibr" rid="bib1.bibx56" id="paren.160"/>, which demonstrates the importance of furan chemistry in real biomass burning plumes.</p>
      <p id="d1e7915">Maleic anhydride (<inline-formula><mml:math id="M451" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and succinic anhydride (<inline-formula><mml:math id="M452" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) are identified as important secondary NMOGs measured by PTR-ToF-MS. Those measured by I-CIMS are identified as methyl hydroxy furanone (<inline-formula><mml:math id="M453" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and a mixture of hydroxy furanone and succinic anhydride (<inline-formula><mml:math id="M454" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). The link between these species and furan precursors may be useful in constraining OH exposures for biomass burning plumes measured in the ambient.</p>
      <p id="d1e8002">Previous studies have suggested that furan chemistry could play a significant role in ozone or SOA formation <xref ref-type="bibr" rid="bib1.bibx17 bib1.bibx31 bib1.bibx30 bib1.bibx32" id="paren.161"/>. For the biomass burning plume described by <xref ref-type="bibr" rid="bib1.bibx56" id="text.162"/>, furan species likely contributed up to <inline-formula><mml:math id="M455" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> % of total ozone production. The extent to which furans contribute to ozone formation will vary depending on burn conditions, and models should include these species in order to improve ozone predictions, especially for young biomass burning plumes.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e8026">The mechanism used to model the mini-chamber and ambient biomass burning plume is provided in the Supplement. Data from mini-chamber experiments and the SONGNEX flight from 21 April 2015 are available online (SONGNEX: <uri>https://www.esrl.noaa.gov/csd/projects/songnex/</uri> and Fire Lab: <uri>https://www.esrl.noaa.gov/csd/projects/firex/firelab/</uri>.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e8035">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-19-14875-2019-supplement" xlink:title="zip">https://doi.org/10.5194/acp-19-14875-2019-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e8044">Firelab data were measured and processed by the following people: PTR-ToF-MS (MMC, ARK, KS, JdG, and CW); ACES (KJZ, SSB); I-CIMS (BY, JEK, and JLJ); OP-FTIR (VS, RY); GC/PTR-ToF-MS (ARK, JBG); NO (JMR). JHK and CC designed the mini-chamber experiments. CYL and DHH operated the mini-chamber. Ambient VOC measurements from the 2013 DISCOVER-AQ campaign were provided by MM and AW. MMC customized the MCM and conducted the model runs. MMC prepared the manuscript with contributions from all co-authors.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e8050">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e8056">The authors thank all those who helped organize and participated in the 2016 Fire Lab experiments, particularly Edward O'Donnell and Maegan Dills for lighting the fires; Ted Christian, Roger Ottmar, David Weise, Mark Cochrane, Kevin Ryan, and Robert Keane for assistance with the fuels; and Shawn Urbanski and Thomas Dzomba for logistical support. The authors also thank Denise D. Montzka, David J. Knapp, and Andrew J. Weinheimer for giving us permission to use <inline-formula><mml:math id="M456" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M457" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements from the WP-3D, and John D. Barrick for giving us permission to use <inline-formula><mml:math id="M458" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">j</mml:mi><mml:mrow><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> measurements.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e8097">This research has been was supported by the National Oceanic and Atmospheric Administration Atmospheric Chemistry, Carbon Cycle and Climate Program (award nos. NA16OAR4310111 and NA16OAR4310112). Christopher Y. Lim and Abigail R. Koss were additionally supported by the National Science Foundation Graduate Research Fellowship Program.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e8103">This paper was edited by Andreas Hofzumahaus and reviewed by William Stockwell and two anonymous referees.</p>
  </notes><ref-list>
    <title>References</title>

      <ref id="bib1.bibx1"><label>Ahern et al.(2018)</label><?label Ahern:2018?><mixed-citation>Ahern, A. T., Goldberger, L., Jahl, L., Thornton, J., and Sullivan, R. C.:
Production of <inline-formula><mml:math id="M459" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M460" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">ClNO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through Nocturnal Processing of Biomass-Burning
Aerosol, Environ. Sci. Technol., 52, 550–559,
<ext-link xlink:href="https://doi.org/10.1021/acs.est.7b04386" ext-link-type="DOI">10.1021/acs.est.7b04386</ext-link>, 2018.</mixed-citation></ref>
      <?pagebreak page14896?><ref id="bib1.bibx2"><label>Akagi et al.(2012)</label><?label Akagi:2012?><mixed-citation>Akagi, S. K., Craven, J. S., Taylor, J. W., McMeeking, G. R., Yokelson, R. J.,
Burling, I. R., Urbanski, S. P., Wold, C. E., Seinfeld, J. H., Coe, H.,
Alvarado, M. J., and Weise, D. R.: Evolution of trace gases and particles
emitted by a chaparral fire in California, Atmos. Chem. Phys.,
12, 1397–1421, <ext-link xlink:href="https://doi.org/10.5194/acp-12-1397-2012" ext-link-type="DOI">10.5194/acp-12-1397-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx3"><label>Akagi et al.(2013)</label><?label Akagi:2013?><mixed-citation>Akagi, S. K., Yokelson, R. J., Burling, I. R., Meinardi, S., Simpson, I.,
Blake, D. R., McMeeking, G. R., Sullivan, A., Lee, T., Kreidenweis, S.,
Urbanski, S., Reardon, J., Griffith, D. W. T., Johnson, T. J., and Weise,
D. R.: Measurements of reactive trace gases and variable <inline-formula><mml:math id="M461" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> formation
rates in some South Carolina biomass burning plumes, Atmos. Chem.
Phys., 13, 1141–1165, <ext-link xlink:href="https://doi.org/10.5194/acp-13-1141-2013" ext-link-type="DOI">10.5194/acp-13-1141-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bibx4"><label>Alvarado et al.(2010)</label><?label Alvarado:2010?><mixed-citation>Alvarado, M. J., Logan, J. A., Mao, J., Apel, E., Riemer, D., Blake, D., Cohen, R. C., Min, K.-E., Perring, A. E., Browne, E. C., Wooldridge, P. J., Diskin, G. S., Sachse, G. W., Fuelberg, H., Sessions, W. R., Harrigan, D. L., Huey, G., Liao, J., Case-Hanks, A., Jimenez, J. L., Cubison, M. J., Vay, S. A., Weinheimer, A. J., Knapp, D. J., Montzka, D. D., Flocke, F. M., Pollack, I. B., Wennberg, P. O., Kurten, A., Crounse, J., Clair, J. M. St., Wisthaler, A., Mikoviny, T., Yantosca, R. M., Carouge, C. C., and Le Sager, P.: Nitrogen oxides and PAN in plumes from boreal fires during ARCTAS-B and their impact on ozone: an integrated analysis of aircraft and satellite observations, Atmos. Chem. Phys., 10, 9739–9760, <ext-link xlink:href="https://doi.org/10.5194/acp-10-9739-2010" ext-link-type="DOI">10.5194/acp-10-9739-2010</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bibx5"><label>Alvarado et al.(2015)</label><?label Alvarado:2015?><mixed-citation>Alvarado, M. J., Lonsdale, C. R., Yokelson, R. J., Akagi, S. K., Coe, H., Craven, J. S., Fischer, E. V., McMeeking, G. R., Seinfeld, J. H., Soni, T., Taylor, J. W., Weise, D. R., and Wold, C. E.: Investigating the links between ozone and organic aerosol chemistry in a biomass burning plume from a prescribed fire in California chaparral, Atmos. Chem. Phys., 15, 6667–6688, <ext-link xlink:href="https://doi.org/10.5194/acp-15-6667-2015" ext-link-type="DOI">10.5194/acp-15-6667-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx6"><label>Alvarez et al.(2009)</label><?label Alvarez:2009?><mixed-citation>
Alvarez, E. G., BorrAs, E., Viidanoja, J., and Hjorth, J.: Unsaturated
dicarbonyl products from the OH-initiated photo-oxidation of furan,
2-methylfuran and 3-methylfuran, Atmos. Environ., 43, 1603–1612,
2009.</mixed-citation></ref>
      <ref id="bib1.bibx7"><label>Andreae et al.(1988)</label><?label Andraea:1988?><mixed-citation>Andreae, M. O., Browell, E. V., Garstang, M., Gregory, G. L., Harriss, R. C.,
Hill, G. F., Jacob, D. J., Pereira, M. C., Sachse, G. W., Setzer, A. W.,
Dias, P. L. S., Talbot, R. W., Torres, A. L., and Wofsy, S. C.:
Biomass-burning emissions and associated haze layers over Amazonia, J. Geophys. Res.-Atmos., 93, 1509–1527,
<ext-link xlink:href="https://doi.org/10.1029/JD093iD02p01509" ext-link-type="DOI">10.1029/JD093iD02p01509</ext-link>, 1988.</mixed-citation></ref>
      <ref id="bib1.bibx8"><label>Aschmann et al.(2011)</label><?label Aschmann:2011?><mixed-citation>
Aschmann, S. M., Nishino, N., Arey, J., and Atkinson, R.: Kinetics of the
Reactions of OH Radicals with 2- and 3-Methylfuran, 2,3- and
2,5-Dimethylfuran, and E- and Z-3-Hexene-2,5-dione, and Products of OH +
2,5-Dimethylfuran, Environ. Sci. Technol., 45, 1859–1865,
2011.</mixed-citation></ref>
      <ref id="bib1.bibx9"><label>Aschmann et al.(2014)</label><?label Aschmann:2014?><mixed-citation>
Aschmann, S. M., Nishino, N., Arey, J., and Atkinson, R.: Products of the OH
Radical-Initiated Reactions of Furan, 2- and 3-Methylfuran, and 2,3- and
2,5-Dimethylfuran in the Presence of NO, J. Phys. Chem. A., 118, 457–466,
2014.</mixed-citation></ref>
      <ref id="bib1.bibx10"><label>Atkinson et al.(2006)</label><?label Atkinson:2006?><mixed-citation>Atkinson, R., Baulch, D. L., Cox, R. A., Crowley, J. N., Hampson, R. F., Hynes,
R. G., Jenkin, M. E., Rossi, M. J., Troe, J., and Subcommittee, I.: Evaluated
kinetic and photochemical data for atmospheric chemistry: Volume II – gas
phase reactions of organic species, Atmos. Chem. and Phys., 6,
3625–4055, <ext-link xlink:href="https://doi.org/10.5194/acp-6-3625-2006" ext-link-type="DOI">10.5194/acp-6-3625-2006</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx11"><label>Barmet et al.(2012)</label><?label Barmet:2012?><mixed-citation>Barmet, P., Dommen, J., DeCarlo, P. F., Tritscher, T., Praplan, A. P., Platt, S. M., Prévôt, A. S. H., Donahue, N. M., and Baltensperger, U.: OH clock determination by proton transfer reaction mass spectrometry at an environmental chamber, Atmos. Meas. Tech., 5, 647–656, <ext-link xlink:href="https://doi.org/10.5194/amt-5-647-2012" ext-link-type="DOI">10.5194/amt-5-647-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx12"><label>Baylon et al.(2017)</label><?label Baylon:2017?><mixed-citation>
Baylon, P., Jaffe, D. A., de Gouw, J., and Warneke, C.: Influence of
Long-Range Transport of Siberian Biomass Burning at the Mt. Bachelor
Observatory during the Spring of 2015, Aerosol  Air Qual. Res., 17,
2751–2761, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx13"><label>Bian et al.(2015)</label><?label Bian:2015?><mixed-citation>Bian, Q., May, A. A., Kreidenweis, S. M., and Pierce, J. R.: Investigation of
particle and vapor wall-loss effects on controlled wood-smoke smog-chamber
experiments, Atmos. Chem. Phys., 15, 11027–11045,
<ext-link xlink:href="https://doi.org/10.5194/acp-15-11027-2015" ext-link-type="DOI">10.5194/acp-15-11027-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx14"><label>Bierbach et al.(1994)</label><?label Bierbach:1994?><mixed-citation>
Bierbach, A., Barnes, I., and Becker, K. H.: Atmospheric chemistry of
unsaturated carbonyls: Butenedial, 4-oxo-2-pentenal, 3-hexene-2, 5-dione,
maleic anhydride, 3H-furan-2-one, and 5-methyl-3H-furan-2-one, Environ.
Sci. Technol., 28, 715–729, 1994.</mixed-citation></ref>
      <ref id="bib1.bibx15"><label>Bierbach et al.(1995)</label><?label Bierbach:1995?><mixed-citation>Bierbach, A., Barnes, I., and Becker, K. H.: Product and kinetic study of the
OH-initiated gas-phase oxidation of furan, 2-methylfuran and furanaldehydes
at <inline-formula><mml:math id="M462" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> K, Atmos. Environ., 29, 2651–2660, 1995.</mixed-citation></ref>
      <ref id="bib1.bibx16"><label>Brey and Fischer(2016)</label><?label Brey:2016?><mixed-citation>
Brey, S. J. and Fischer, E. V.: Smoke in the City: How Often and Where Does
Smoke Impact Summertime Ozone in the United States?, Environ. Sci.
Technol., 50, 1288–1294, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx17"><label>Bruns et al.(2017)</label><?label Bruns:2017?><mixed-citation>Bruns, E. A., Slowik, J. G., El Haddad, I., Kilic, D., Klein, F., Dommen, J., Temime-Roussel, B., Marchand, N., Baltensperger, U., and Prévôt, A. S. H.: Characterization of gas-phase organics using proton transfer reaction time-of-flight mass spectrometry: fresh and aged residential wood combustion emissions, Atmos. Chem. Phys., 17, 705–720, <ext-link xlink:href="https://doi.org/10.5194/acp-17-705-2017" ext-link-type="DOI">10.5194/acp-17-705-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx18"><label>Buhr et al.(2002)</label><?label Buhr:2002?><mixed-citation>
Buhr, K., van Ruth, S., and Delahunty, C.: Analysis of volatile flavour
compounds by Proton Transfer Reaction-Mass Spectrometry: fragmentation
patterns and discrimination between isobaric and isomeric compounds,
Int. J. Mass Spectrom., 221, 1–7, 2002.</mixed-citation></ref>
      <ref id="bib1.bibx19"><label>Burkholder et al.(2015)</label><?label Burkholder:2015?><mixed-citation>Burkholder, J., Sander, S., Abbatt, J., Barker, J., Huie, R., Kolb, C., Kurylo,
M., Orkin, V., Wilmouth, D., and Wine, P.: Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies, Evaluation No. 18, JPL Publication 15-10, Jet Propulsion Laboratory, Pasadena,  <uri>http://jpldataeval.jpl.nasa.gov</uri> (last access: 4 December 2019), 2015.</mixed-citation></ref>
      <ref id="bib1.bibx20"><label>Burling et al.(2010)</label><?label Burling:2010?><mixed-citation>Burling, I. R., Yokelson, R. J., Griffith, D. W. T., Johnson, T. J., Veres, P., Roberts, J. M., Warneke, C., Urbanski, S. P., Reardon, J., Weise, D. R., Hao, W. M., and de Gouw, J.: Laboratory measurements of trace gas emissions from biomass burning of fuel types from the southeastern and southwestern United States, Atmos. Chem. Phys., 10, 11115–11130, <ext-link xlink:href="https://doi.org/10.5194/acp-10-11115-2010" ext-link-type="DOI">10.5194/acp-10-11115-2010</ext-link>, 2010.</mixed-citation></ref>
      <ref id="bib1.bibx21"><label>Chapleski et al.(2016)</label><?label Chapleski:2016?><mixed-citation>Chapleski, R. C., Zhang, Y., Troya, D., and Morris, J. R.: Heterogeneous
chemistry and reaction dynamics of the atmospheric oxidants, O3, NO3,
and OH, on organic surfaces, Chem. Soc. Rev., 45, 3731–3746,
<ext-link xlink:href="https://doi.org/10.1039/C5CS00375J" ext-link-type="DOI">10.1039/C5CS00375J</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx22"><label>Colmenar et al.(2015)</label><?label Colmenar:2015?><mixed-citation>
Colmenar, I., González, S., Jiménez, E., Martín, P., Salgado, S.,
Cabañas, B., and Albaladejo, J.: UV absorption cross sections between
290 and 380 nm of a series of furanaldehydes: Estimation of their photolysis
lifetimes, Atmos. Environ., 103, 1–6, 2015.</mixed-citation></ref>
      <?pagebreak page14897?><ref id="bib1.bibx23"><label>Crounse et al.(2013)</label><?label Crounse:2013?><mixed-citation>Crounse, J. D., Nielsen, L. B., Jørgensen, S., Kjaergaard, H. G., and
Wennberg, P. O.: Autoxidation of Organic Compounds in the Atmosphere,
J. Phys. Chem. Lett., 4, 3513–3520,
<ext-link xlink:href="https://doi.org/10.1021/jz4019207" ext-link-type="DOI">10.1021/jz4019207</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bibx24"><label>Deming et al.(2019)</label><?label Deming:2019?><mixed-citation>Deming, B. L., Pagonis, D., Liu, X., Day, D. A., Talukdar, R., Krechmer, J. E., de Gouw, J. A., Jimenez, J. L., and Ziemann, P. J.: Measurements of delays of gas-phase compounds in a wide variety of tubing materials due to gas-wall interactions, Atmos. Meas. Tech., 12, 3453–3461, <ext-link xlink:href="https://doi.org/10.5194/amt-12-3453-2019" ext-link-type="DOI">10.5194/amt-12-3453-2019</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx25"><label>Ferreira da Silva et al.(2015)</label><?label FerreiradaSilva:2015?><mixed-citation>
Ferreira da Silva, F., Lange, E., Limão-Vieira, P., Jones, N. C., Hoffmann,
S. V., Hubin-Franskin, M. J., Delwiche, J., Brunger, M. J., Neves, R. F. C.,
Lopes, M. C. A., de Oliveira, E. M., da Costa, R. F., Varella, M. T. d. N.,
Bettega, M. H. F., Blanco, F., García, G., Lima, M. A. P., and Jones,
D. B.: Electronic excitation of furfural as probed by high-resolution vacuum
ultraviolet spectroscopy, electron energy loss spectroscopy, and ab
initiocalculations,  J. Chem. Phys., 143, 144308–144314,
2015.</mixed-citation></ref>
      <ref id="bib1.bibx26"><label>Finewax et al.(2018)</label><?label Finewax:2018?><mixed-citation>Finewax, Z., de Gouw, J. A., and Ziemann, P. J.: Identification and
Quantification of 4-Nitrocatechol Formed from OH and <inline-formula><mml:math id="M463" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> Radical-Initiated
Reactions of Catechol in Air in the Presence of <inline-formula><mml:math id="M464" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>: Implications for
Secondary Organic Aerosol Formation from Biomass Burning, Environ.
Sci. Technol., 52, 1981–1989, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx27"><label>Ford et al.(2018)</label><?label Ford:2018?><mixed-citation>
Ford, B., Val Martin, M., Zelasky, S. E., Fischer, E. V., Anenberg, S. C.,
Heald, C. L., and Pierce, J. R.: Future Fire Impacts on Smoke
Concentrations, Visibility, and Health in the Contiguous United States,
GeoHealth, 2, 229–247, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx28"><label>Gandini et al.(1976)</label><?label Gandini:1976?><mixed-citation>
Gandini, A., Parsons, J. M., and Back, R. A.: The photochemistry of
2-furaldehyde vapour. II. Photodecomposition: direct photolysis at 253.7 and
313 nm and Hg(3P1)-sensitized decomposition, Can. J. Chem.,
54, 3095–3101, 1976.</mixed-citation></ref>
      <ref id="bib1.bibx29"><label>Gaston et al.(2016)</label><?label Gaston:2016?><mixed-citation>Gaston, C. J., Lopez-Hilfiker, F. D., Whybrew, L. E., Hadley, O., McNair, F.,
Gao, H., Jaffe, D. A., and Thornton, J. A.: Online molecular characterization
of fine particulate matter in Port Angeles, WA: Evidence for a major impact
from residential wood smoke, Atmos. Envrion., 138, 99–107,
<ext-link xlink:href="https://doi.org/10.1016/j.atmosenv.2016.05.013" ext-link-type="DOI">10.1016/j.atmosenv.2016.05.013</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx30"><label>Gilman et al.(2015)</label><?label Gilman:2015?><mixed-citation>Gilman, J. B., Lerner, B. M., Kuster, W. C., Goldan, P. D., Warneke, C., Veres, P. R., Roberts, J. M., de Gouw, J. A., Burling, I. R., and Yokelson, R. J.: Biomass burning emissions and potential air quality impacts of volatile organic compounds and other trace gases from fuels common in the US, Atmos. Chem. Phys., 15, 13915–13938, <ext-link xlink:href="https://doi.org/10.5194/acp-15-13915-2015" ext-link-type="DOI">10.5194/acp-15-13915-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx31"><label>Hartikainen et al.(2018)</label><?label Hartikainen:2018?><mixed-citation>
Hartikainen, A., Yli-Pirilä, P., Tiitta, P., Leskinen, A., Kortelainen, M.,
Orasche, J., Schnelle-Kreis, J., Lehtinen, K. E. J., Zimmermann, R.,
Jokiniemi, J., and Sippula, O.: Volatile Organic Compounds from Logwood
Combustion: Emissions and Transformation under Dark and Photochemical Aging
Conditions in a Smog Chamber, Environ. Sci. Technol., 52,
4979–4988, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx32"><label>Hatch et al.(2015)</label><?label Hatch:2015?><mixed-citation>Hatch, L. E., Luo, W., Pankow, J. F., Yokelson, R. J., Stockwell, C. E., and Barsanti, K. C.: Identification and quantification of gaseous organic compounds emitted from biomass burning using two-dimensional gas chromatography–time-of-flight mass spectrometry, Atmos. Chem. Phys., 15, 1865–1899, <ext-link xlink:href="https://doi.org/10.5194/acp-15-1865-2015" ext-link-type="DOI">10.5194/acp-15-1865-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx33"><label>Hatch et al.(2017)</label><?label Hatch:2017?><mixed-citation>Hatch, L. E., Yokelson, R. J., Stockwell, C. E., Veres, P. R., Simpson, I. J., Blake, D. R., Orlando, J. J., and Barsanti, K. C.: Multi-instrument comparison and compilation of non-methane organic gas emissions from biomass burning and implications for smoke-derived secondary organic aerosol precursors, Atmos. Chem. Phys., 17, 1471–1489, <ext-link xlink:href="https://doi.org/10.5194/acp-17-1471-2017" ext-link-type="DOI">10.5194/acp-17-1471-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx34"><label>Hiraoka and Srinivasan(1968)</label><?label Hiraoka:1968?><mixed-citation>
Hiraoka, H. and Srinivasan, R.: Vapor-Phase Photochemistry of Furfural, The
J. Chem. Phys., 48, 2185–2189, 1968.</mixed-citation></ref>
      <ref id="bib1.bibx35"><label>Hobbs et al.(2003)</label><?label Hobbs:2003?><mixed-citation>Hobbs, P. V., Sinha, P., Yokelson, R. J., Christian, T. J., Blake, D. R., Gao,
S., Kirchstetter, T. W., Novakov, T., and Pilewskie, P.: Evolution of gases
and particles from a savanna fire in South Africa, J. Geophys.
Res., 108, 8485, <ext-link xlink:href="https://doi.org/10.1029/2002JD002352" ext-link-type="DOI">10.1029/2002JD002352</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx36"><label>Hodshire et al.(2019)</label><?label Hodshire:2019?><mixed-citation>Hodshire, A. L., Bian, Q., Ramnarine, E., Lonsdale, C. R., Alvarado, M. J.,
Kreidenweis, S. M., Jathar, S. H., and Pierce, J. R.: More Than Emissions and
Chemistry: Fire Size, Dilution, and Background Aerosol Also Greatly Influence
Near-Field Biomass Burning Aerosol Aging, J. Geophys. Res.-Atmos., 124, 5589–5611, <ext-link xlink:href="https://doi.org/10.1029/2018JD029674" ext-link-type="DOI">10.1029/2018JD029674</ext-link>,
2019.</mixed-citation></ref>
      <ref id="bib1.bibx37"><label>Huey et al.(1995)</label><?label Huey:1995?><mixed-citation>Huey, L. G., Hanson, D. R., and Howard, C. J.: Reactions of SF6- and I- with
Atmospheric Trace Gases,   J. Phys. Chem., 99, 5001–5008,
<ext-link xlink:href="https://doi.org/10.1021/j100014a021" ext-link-type="DOI">10.1021/j100014a021</ext-link>, 1995.</mixed-citation></ref>
      <ref id="bib1.bibx38"><label>Jaffe et al.(2008)</label><?label Jaffe:2008?><mixed-citation>Jaffe, D., Chand, D., Hafner, W., Westerling, A., and Spracklen, D.: Influence
of Fires on <inline-formula><mml:math id="M465" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> Concentrations in the Western US, Environ. Sci.
Technol., 42, 5885–5891, 2008.</mixed-citation></ref>
      <ref id="bib1.bibx39"><label>Jaffe and Wigder(2012)</label><?label Jaffe:2012?><mixed-citation>
Jaffe, D. A. and Wigder, N. L.: Ozone production from wildfires: A critical
review, Atmos. Environ., 51, 1–10, 2012.</mixed-citation></ref>
      <ref id="bib1.bibx40"><label>Jaffe et al.(2013)</label><?label Jaffe:2013?><mixed-citation>
Jaffe, D. A., Wigder, N., Downey, N., Pfister, G., Boynard, A., and Reid,
S. B.: Impact of Wildfires on Ozone Exceptional Events in the Western US,
Environ. Sci. Technol., 47, 11065–11072, 2013.</mixed-citation></ref>
      <ref id="bib1.bibx41"><label>Jaffe et al.(2018)</label><?label Jaffe:2018?><mixed-citation>
Jaffe, D. A., Cooper, O. R., Fiore, A. M., Henderson, B. H., Tonneson, G. S.,
Russell, A. G., Henze, D. K., Langford, A. O., Lin, M., and Moore, T.:
Scientific assessment of background ozone over the US: Implications for
air quality management, Elem. Sci. Anth., 6, 30 pp., 2018.</mixed-citation></ref>
      <ref id="bib1.bibx42"><label>Jenkin et al.(1997)</label><?label Jenkin:1997?><mixed-citation>
Jenkin, M. E., Saunders, S. M., and Pilling, M. J.: The tropospheric
degradation of volatile organic compounds: a protocol for mechanism
development, Atmos. Environ., 31, 81–104, 1997.</mixed-citation></ref>
      <ref id="bib1.bibx43"><label>Jenkin et al.(2003)</label><?label Jenkin:2003?><mixed-citation>Jenkin, M. E., Saunders, S. M., Wagner, V., and Pilling, M. J.: Protocol for the development of the Master Chemical Mechanism, MCM v3 (Part B): tropospheric degradation of aromatic volatile organic compounds, Atmos. Chem. Phys., 3, 181–193, <ext-link xlink:href="https://doi.org/10.5194/acp-3-181-2003" ext-link-type="DOI">10.5194/acp-3-181-2003</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx44"><label>Jenkin et al.(2015)</label><?label Jenkin:2015?><mixed-citation>Jenkin, M. E., Young, J. C., and Rickard, A. R.: The MCM v3.3.1 degradation scheme for isoprene, Atmos. Chem. Phys., 15, 11433–11459, <ext-link xlink:href="https://doi.org/10.5194/acp-15-11433-2015" ext-link-type="DOI">10.5194/acp-15-11433-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx45"><label>Keller-Rudek et al.(2013)</label><?label Keller-Rudek:2013?><mixed-citation>Keller-Rudek, H., Moortgat, G. K., Sander, R., and Sörensen, R.: The
MPI-Mainz UV/VIS Spectral Atlas of Gaseous Molecules of Atmospheric Interest,
Earth Syst. Sci. Data, 5, 365–373, <ext-link xlink:href="https://doi.org/10.5194/essd-5-365-2013" ext-link-type="DOI">10.5194/essd-5-365-2013</ext-link>,
2013.</mixed-citation></ref>
      <ref id="bib1.bibx46"><label>Koss et al.(2018)</label><?label Koss:2018?><mixed-citation>Koss, A. R., Sekimoto, K., Gilman, J. B., Selimovic, V., Coggon, M. M.,
Zarzana, K. J., Yuan, B., Lerner, B. M., Brown, S. S., Jimenez, J. L.,
Krechmer, J., Roberts, J. M., Warneke, C., Yokelson, R. J., and de Gouw, J.:
Non-methane organic gas emissions from biomass burning: identification,
quantification, and emission factors from PTR-ToF during the FIREX 2016
laboratory experiment, Atmos. Chem. Phys., 18, 3299–3319,
<ext-link xlink:href="https://doi.org/10.5194/acp-18-3299-2018" ext-link-type="DOI">10.5194/acp-18-3299-2018</ext-link>, 2018.</mixed-citation></ref>
      <?pagebreak page14898?><ref id="bib1.bibx47"><label>Krechmer et al.(2016)</label><?label Krechmer:2016?><mixed-citation>Krechmer, J. E., Pagonis, D., Ziemann, P. J., and Jimenez, J. L.:
Quantification of Gas-Wall Partitioning in Teflon Environmental Chambers
Using Rapid Bursts of Low-Volatility Oxidized Species Generated in Situ,
Environ. Sci. Technol., 50, 5757–5765,
<ext-link xlink:href="https://doi.org/10.1021/acs.est.6b00606" ext-link-type="DOI">10.1021/acs.est.6b00606</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx48"><label>Lauraguais et al.(2014)</label><?label Lauraguais:2014?><mixed-citation>
Lauraguais, A., Coeur-Tourneur, C., Cassez, A., Deboudt, K., Fourmentin, M.,
and Choël, M.: Atmospheric reactivity of hydroxyl radicals with guaiacol
(2-methoxyphenol), a biomass burning emitted compound: Secondary organic
aerosol formation and gas-phase oxidation products, Atmos. Environ.,
86, 155–163, 2014.</mixed-citation></ref>
      <ref id="bib1.bibx49"><label>Lee et al.(2014)</label><?label Lee:2014?><mixed-citation>
Lee, B. H., Lopez-Hilfiker, F. D., Mohr, C., Kurtén, T., Worsnop, D. R.,
and Thornton, J. A.: An Iodide-Adduct High-Resolution Time-of-Flight
Chemical-Ionization Mass Spectrometer: Application to Atmospheric Inorganic
and Organic Compounds, Enviro. Sci. Technol., 48,
6309–6317, 2014.</mixed-citation></ref>
      <ref id="bib1.bibx50"><label>Lim et al.(2019)</label><?label Lim:2019?><mixed-citation>Lim, C. Y., Hagan, D. H., Coggon, M. M., Koss, A. R., Sekimoto, K., de Gouw,
J., Warneke, C., Cappa, C. D., and Kroll, J. H.: Secondary organic aerosol
formation from the laboratory oxidation of biomass burning emissions,
Atmos. Chem. Phys., 19, 12797–12809,
<ext-link xlink:href="https://doi.org/10.5194/acp-19-12797-2019" ext-link-type="DOI">10.5194/acp-19-12797-2019</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx51"><label>Liu et al.(1999)</label><?label Liu:1999?><mixed-citation>
Liu, X., Jeffries, H. E., and Sexton, K. G.: Atmospheric Photochemical
Degradation of 1,4-Unsaturated Dicarbonyls, Environ. Sci.
Technol., 33, 4212–4220, 1999.</mixed-citation></ref>
      <ref id="bib1.bibx52"><label>Liu et al.(2016)</label><?label Liu:2016?><mixed-citation>Liu, X., Zhang, Y., Huey, L. G., Yokelson, R. J., Wang, Y., Jimenez, J. L.,
Campuzano-Jost, P., Beyersdorf, A. J., Blake, D. R., Choi, Y., St. Clair,
J. M., Crounse, J. D., Day, D. A., Diskin, G. S., Fried, A., Hall, S. R.,
Hanisco, T. F., King, L. E., Meinardi, S., Mikoviny, T., Palm, B. B.,
Peischl, J., Perring, A. E., Pollack, I. B., Ryerson, T. B., Sachse, G.,
Schwarz, J. P., Simpson, I. J., Tanner, D. J., Thornhill, K. L., Ullmann, K.,
Weber, R. J., Wennberg, P. O., Wisthaler, A., Wolfe, G. M., and Ziemba,
L. D.: Agricultural fires in the southeastern US during SEAC4RS: Emissions
of trace gases and particles and evolution of ozone, reactive nitrogen, and
organic aerosol, J. Geophys. Res.-Atmos., 121,
7383–7414, <ext-link xlink:href="https://doi.org/10.1002/2016JD025040" ext-link-type="DOI">10.1002/2016JD025040</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx53"><label>Mason et al.(2001)</label><?label Mason:2001?><mixed-citation>Mason, S. A., Field, R. J., Yokelson, R. J., Kochivar, M. A., Tinsley, M. R.,
Ward, D. E., and Hao, W. M.: Complex effects arising in smoke plume
simulations due to inclusion of direct emissions of oxygenated organic
species from biomass combustion, J. Geophys. Res.-Atmos., 106, 12527–12539, <ext-link xlink:href="https://doi.org/10.1029/2001JD900003" ext-link-type="DOI">10.1029/2001JD900003</ext-link>, 2001.</mixed-citation></ref>
      <ref id="bib1.bibx54"><label>Mauzerall et al.(1998)</label><?label Mauzerall:1998?><mixed-citation>
Mauzerall, D. L., Logan, J. A., Jacob, D. J., Anderson, B. E., Blake, D. R.,
Bradshaw, J. D., Heikes, B., Sachse, G. W., Singh, H., and Talbot, B.:
Photochemistry in biomass burning plumes and implications for tropospheric
ozone over the tropical South Atlantic, Geophys. Res., 103, 8401–8423, 1998.</mixed-citation></ref>
      <ref id="bib1.bibx55"><label>Millet et al.(2015)</label><?label Millet:2015?><mixed-citation>
Millet, D. B., Baasandorj, M., Farmer, D. K., Thornton, J. A., Baumann, K., Brophy, P., Chaliyakunnel, S., de Gouw, J. A., Graus, M., Hu, L., Koss, A., Lee, B. H., Lopez-Hilfiker, F. D., Neuman, J. A., Paulot, F., Peischl, J., Pollack, I. B., Ryerson, T. B., Warneke, C., Williams, B. J., and Xu, J.: A large and ubiquitous source of atmospheric formic acid, Atmos. Chem. Phys., 15, 6283–6304, https://doi.org/10.5194/acp-15-6283-2015, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx56"><?xmltex \def\ref@label{{M{\"{u}}ller et~al.(2016)}}?><label>Müller et al.(2016)</label><?label Muller:2016?><mixed-citation>Müller, M., Anderson, B. E., Beyersdorf, A. J., Crawford, J. H., Diskin, G. S., Eichler, P., Fried, A., Keutsch, F. N., Mikoviny, T., Thornhill, K. L., Walega, J. G., Weinheimer, A. J., Yang, M., Yokelson, R. J., and Wisthaler, A.: In situ measurements and modeling of reactive trace gases in a small biomass burning plume, Atmos. Chem. Phys., 16, 3813–3824, <ext-link xlink:href="https://doi.org/10.5194/acp-16-3813-2016" ext-link-type="DOI">10.5194/acp-16-3813-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx57"><label>Orlando and Tyndall(2012)</label><?label Orlando:2012?><mixed-citation>Orlando, J. J. and Tyndall, G. S.: Laboratory studies of organic peroxy radical
chemistry: an overview with emphasis on recent issues of atmospheric
significance, Chem. Soc. Rev., 41, 6294–6317, <ext-link xlink:href="https://doi.org/10.1039/c2cs35166h" ext-link-type="DOI">10.1039/c2cs35166h</ext-link>,
2012.</mixed-citation></ref>
      <ref id="bib1.bibx58"><label>Pagonis et al.(2017)</label><?label Pagonis:2017?><mixed-citation>Pagonis, D., Krechmer, J. E., de Gouw, J., Jimenez, J. L., and Ziemann, P. J.: Effects of gas-wall partitioning in Teflon tubing and instrumentation on time-resolved measurements of gas-phase organic compounds, Atmos. Meas. Tech., 10, 4687–4696, <ext-link xlink:href="https://doi.org/10.5194/amt-10-4687-2017" ext-link-type="DOI">10.5194/amt-10-4687-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx59"><label>Pagonis et al.(2019)</label><?label Pagonis:2019?><mixed-citation>Pagonis, D., Sekimoto, K., and de Gouw, J.: A library of proton-transfer
reactions of <inline-formula><mml:math id="M466" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mo>+</mml:mo></mml:msub></mml:mrow></mml:math></inline-formula> ions used for trace gas detection, J. Am. Soc. Mass
Spectrom.,   30, 1330–1335, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx60"><label>Peng and Jimenez(2017)</label><?label Peng:2017?><mixed-citation>Peng, Z. and Jimenez, J. L.: Modeling of the chemistry in oxidation flow reactors with high initial NO, Atmos. Chem. Phys., 17, 11991–12010, <ext-link xlink:href="https://doi.org/10.5194/acp-17-11991-2017" ext-link-type="DOI">10.5194/acp-17-11991-2017</ext-link>, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx61"><label>Peng et al.(2016)</label><?label Peng:2016?><mixed-citation>Peng, Z., Day, D. A., Ortega, A. M., Palm, B. B., Hu, W., Stark, H., Li, R., Tsigaridis, K., Brune, W. H., and Jimenez, J. L.: Non-OH chemistry in oxidation flow reactors for the study of atmospheric chemistry systematically examined by modeling, Atmos. Chem. Phys., 16, 4283–4305, <ext-link xlink:href="https://doi.org/10.5194/acp-16-4283-2016" ext-link-type="DOI">10.5194/acp-16-4283-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx62"><label>Peng et al.(2019)</label><?label Peng:2019?><mixed-citation>Peng, Z., Lee-Taylor, J., Orlando, J. J., Tyndall, G. S., and Jimenez, J. L.:
Organic peroxy radical chemistry in oxidation flow reactors and environmental
chambers and their atmospheric relevance, Atmos. Chem. Phys.,
19, 813–834, <ext-link xlink:href="https://doi.org/10.5194/acp-19-813-2019" ext-link-type="DOI">10.5194/acp-19-813-2019</ext-link>, 2019.</mixed-citation></ref>
      <ref id="bib1.bibx63"><label>Praske et al.(2018)</label><?label Praske:2018?><mixed-citation>Praske, E., Otkjær, R. V., Crounse, J. D., Hethcox, J. C., Stoltz, B. M.,
Kjaergaard, H. G., and Wennberg, P. O.: Atmospheric autoxidation is
increasingly important in urban and suburban North America, P. Natl. Acad. Sci. USA, 115, 64–69, <ext-link xlink:href="https://doi.org/10.1073/pnas.1715540115" ext-link-type="DOI">10.1073/pnas.1715540115</ext-link>,
2018.</mixed-citation></ref>
      <ref id="bib1.bibx64"><label>Priestley et al.(2018)</label><?label Priestly:2018?><mixed-citation>Priestley, M., Le Breton, M., Bannan, T. J., Leather, K. E., Bacak, A.,
Reyes-Villegas, E., De Vocht, F., Shallcross, B. M. A., Brazier, T.,
Anwar Khan, M., Allan, J., Shallcross, D. E., Coe, H., and Percival, C. J.:
Observations of Isocyanate, Amide, Nitrate, and Nitro Compounds From an
Anthropogenic Biomass Burning Event Using a ToF-CIMS, J. Geophys.
Res.-Atmos., 123, 7687–7704, <ext-link xlink:href="https://doi.org/10.1002/2017JD027316" ext-link-type="DOI">10.1002/2017JD027316</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx65"><label>Reyes-Villegas et al.(2018)</label><?label ReyesVillegas:2018?><mixed-citation>Reyes-Villegas, E., Priestley, M., Ting, Y.-C., Haslett, S., Bannan, T.,
Le Breton, M., Williams, P. I., Bacak, A., Flynn, M. J., Coe, H., Percival,
C., and Allan, J. D.: Simultaneous aerosol mass spectrometry and chemical
ionisation mass spectrometry measurements during a biomass burning event in
the UK: insights into nitrate chemistry, Atmos. Chem. Phys.,
18, 4093–4111, <ext-link xlink:href="https://doi.org/10.5194/acp-18-4093-2018" ext-link-type="DOI">10.5194/acp-18-4093-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx66"><label>Saunders et al.(2003)</label><?label Saunders:2003?><mixed-citation>Saunders, S. M., Jenkin, M. E., Derwent, R. G., and Pilling, M. J.: Protocol for the development of the Master Chemical Mechanism, MCM v3 (Part A): tropospheric degradation of non-aromatic volatile organic compounds, Atmos. Chem. Phys., 3, 161–180, <ext-link xlink:href="https://doi.org/10.5194/acp-3-161-2003" ext-link-type="DOI">10.5194/acp-3-161-2003</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx67"><label>Sekimoto et al.(2017)</label><?label Sekimoto:2017?><mixed-citation>
Sekimoto, K., Li, S.-M., Yuan, B., Koss, A., Coggon, M., Warneke, C., and
de Gouw, J.: Calculation of the sensitivity of proton-transfer-reaction mass
spectrometry (PTR-MS) for organic trace gases using molecular properties,
Int. J. Mass Spectrom., 421, 71–94, 2017.</mixed-citation></ref>
      <?pagebreak page14899?><ref id="bib1.bibx68"><label>Sekimoto et al.(2018)</label><?label Sekimoto:2018?><mixed-citation>Sekimoto, K., Koss, A. R., Gilman, J. B., Selimovic, V., Coggon, M. M., Zarzana, K. J., Yuan, B., Lerner, B. M., Brown, S. S., Warneke, C., Yokelson, R. J., Roberts, J. M., and de Gouw, J.: High- and low-temperature pyrolysis profiles describe volatile organic compound emissions from western US wildfire fuels, Atmos. Chem. Phys., 18, 9263–9281, <ext-link xlink:href="https://doi.org/10.5194/acp-18-9263-2018" ext-link-type="DOI">10.5194/acp-18-9263-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx69"><label>Selimovic et al.(2018)</label><?label Selimovic:2018?><mixed-citation>Selimovic, V., Yokelson, R. J., Warneke, C., Roberts, J. M., de Gouw, J.,
Reardon, J., and Griffith, D. W. T.: Aerosol optical properties and trace gas
emissions by PAX and OP-FTIR for laboratory-simulated western US wildfires
during FIREX, Atmos. Chem. Phys., 18, 2929–2948,
<ext-link xlink:href="https://doi.org/10.5194/acp-18-2929-2018" ext-link-type="DOI">10.5194/acp-18-2929-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx70"><label>Stockwell et al.(2014)</label><?label Stockwell:2014?><mixed-citation>Stockwell, C. E., Yokelson, R. J., Kreidenweis, S. M., Robinson, A. L., DeMott,
P. J., Sullivan, R. C., Reardon, J., Ryan, K. C., Griffith, D. W. T., and
Stevens, L.: Trace gas emissions from combustion of peat, crop residue,
domestic biofuels, grasses, and other fuels: configuration and Fourier
transform infrared (FTIR) component of the fourth Fire Lab at Missoula
Experiment (FLAME-4), Atmos. Chem. Phys., 14, 9727–9754,
<ext-link xlink:href="https://doi.org/10.5194/acp-14-9727-2014" ext-link-type="DOI">10.5194/acp-14-9727-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bibx71"><label>Stockwell et al.(2015)</label><?label Stockwell:2015?><mixed-citation>Stockwell, C. E., Veres, P. R., Williams, J., and Yokelson, R. J.:
Characterization of biomass burning emissions from cooking fires, peat, crop
residue, and other fuels with high-resolution proton-transfer-reaction
time-of-flight mass spectrometry, Atmos. Chem. Phys., 15,
845–865, <ext-link xlink:href="https://doi.org/10.5194/acp-15-845-2015" ext-link-type="DOI">10.5194/acp-15-845-2015</ext-link>, 2015.</mixed-citation></ref>
      <ref id="bib1.bibx72"><label>Stockwell et al.(2018)</label><?label Stockwell:2018?><mixed-citation>Stockwell, C. E., Kupc, A., Witkowski, B., Talukdar, R. K., Liu, Y., Selimovic, V., Zarzana, K. J., Sekimoto, K., Warneke, C., Washenfelder, R. A., Yokelson, R. J., Middlebrook, A. M., and Roberts, J. M.: Characterization of a catalyst-based conversion technique to measure total particulate nitrogen and organic carbon and comparison to a particle mass measurement instrument, Atmos. Meas. Tech., 11, 2749–2768, <ext-link xlink:href="https://doi.org/10.5194/amt-11-2749-2018" ext-link-type="DOI">10.5194/amt-11-2749-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx73"><label>Strollo and Ziemann(2013)</label><?label Strollo:2013?><mixed-citation>Strollo, C. M. and Ziemann, P. J.: Products and mechanism of secondary organic
aerosol formation from the reaction of 3-methylfuran with OH radicals in the
presence of <inline-formula><mml:math id="M467" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi mathvariant="normal">x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, Atmos. Environ., 77, 534–543, 2013.</mixed-citation></ref>
      <ref id="bib1.bibx74"><label>Tomaz et al.(2018)</label><?label Tomaz:2018?><mixed-citation>Tomaz, S., Cui, T., Chen, Y., Sexton, K. G., Roberts, J. M., Warneke, C.,
Yokelson, R. J., Surratt, J. D., and Turpin, B. J.: Photochemical Cloud
Processing of Primary Wildfire Emissions as a Potential Source of Secondary
Organic Aerosol, Environ. Sci. Technol., 52, 11027–11037,
<ext-link xlink:href="https://doi.org/10.1021/acs.est.8b03293" ext-link-type="DOI">10.1021/acs.est.8b03293</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx75"><label>Westerling(2006)</label><?label Westerling:2006?><mixed-citation>
Westerling, A. L.: Warming and Earlier Spring Increase Western US Forest
Wildfire Activity, Science, 313, 940–943, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx76"><label>Wolfe et al.(2016)</label><?label Wolfe:2016?><mixed-citation>Wolfe, G. M., Marvin, M. R., Roberts, S. J., Travis, K. R., and Liao, J.: The Framework for 0-D Atmospheric Modeling (F0AM) v3.1, Geosci. Model Dev., 9, 3309–3319, <ext-link xlink:href="https://doi.org/10.5194/gmd-9-3309-2016" ext-link-type="DOI">10.5194/gmd-9-3309-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx77"><label>Yee et al.(2013)</label><?label Yee:2013?><mixed-citation>Yee, L. D., Kautzman, K. E., Loza, C. L., Schilling, K. A., Coggon, M. M., Chhabra, P. S., Chan, M. N., Chan, A. W. H., Hersey, S. P., Crounse, J. D., Wennberg, P. O., Flagan, R. C., and Seinfeld, J. H.: Secondary organic aerosol formation from biomass burning intermediates: phenol and methoxyphenols, Atmos. Chem. Phys., 13, 8019–8043, <ext-link xlink:href="https://doi.org/10.5194/acp-13-8019-2013" ext-link-type="DOI">10.5194/acp-13-8019-2013</ext-link>, 2013.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bibx78"><label>Yokelson et al.(1996)</label><?label Yokelson:1996?><mixed-citation>Yokelson, R. J., Griffith, D. W. T., and Ward, D. E.: Open-path Fourier
transform infrared studies of large-scale laboratory biomass fires, J. Geophys. Res.-Atmos., 101, 21067–21080,
<ext-link xlink:href="https://doi.org/10.1029/96JD01800" ext-link-type="DOI">10.1029/96JD01800</ext-link>, 1996.</mixed-citation></ref>
      <ref id="bib1.bibx79"><label>Yokelson et al.(2003)</label><?label Yokelson:2003?><mixed-citation>Yokelson, R. J., Bertschi, I. T., Christian, T. J., Hobbs, P. V., Ward, D. E.,
and Hao, W. M.: Trace gas measurements in nascent, aged, and cloud-processed
smoke from African savanna fires by airborne Fourier transform infrared
spectroscopy (AFTIR), J. Geophys. Res., 108,  8478,
<ext-link xlink:href="https://doi.org/10.1029/2002JD002322" ext-link-type="DOI">10.1029/2002JD002322</ext-link>, 2003.</mixed-citation></ref>
      <ref id="bib1.bibx80"><label>Yokelson et al.(2009)</label><?label Yokelson:2009?><mixed-citation>Yokelson, R. J., Crounse, J. D., DeCarlo, P. F., Karl, T., Urbanski, S., Atlas,
E., Campos, T., Shinozuka, Y., Kapustin, V., Clarke, A. D., Weinheimer, A.,
Knapp, D. J., Montzka, D. D., Holloway, J., Weibring, P., Flocke, F., Zheng,
W., Toohey, D., Wennberg, P. O., Wiedinmyer, C., Mauldin, L., Fried, A.,
Richter, D., Walega, J., Jimenez, J. L., Adachi, K., Buseck, P. R., Hall,
S. R., and Shetter, R.: Emissions from biomass burning in the Yucatan,
Atmos. Chem. Phys., 9, 5785–5812,
<ext-link xlink:href="https://doi.org/10.5194/acp-9-5785-2009" ext-link-type="DOI">10.5194/acp-9-5785-2009</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bibx81"><label>Yuan et al.(2016)</label><?label Yuan:2016?><mixed-citation>Yuan, B., Koss, A., Warneke, C., Gilman, J. B., Lerner, B. M., Stark, H., and
de Gouw, J. A.: A high-resolution time-of-flight chemical ionization mass
spectrometer utilizing hydronium ions (<inline-formula><mml:math id="M468" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msup><mml:mi mathvariant="normal">O</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> ToF-CIMS) for
measurements of volatile organic compounds in the atmosphere, Atmos.
Meas. Tech., 9, 2735–2752, <ext-link xlink:href="https://doi.org/10.5194/amt-9-2735-2016" ext-link-type="DOI">10.5194/amt-9-2735-2016</ext-link>, 2016.</mixed-citation></ref>
      <ref id="bib1.bibx82"><label>Yuan et al.(2017)</label><?label Yuan:2017?><mixed-citation>
Yuan, B., Koss, A. R., Warneke, C., Coggon, M., Sekimoto, K., and de Gouw,
J. A.: Proton-Transfer-Reaction Mass Spectrometry: Applications in
Atmospheric Sciences, Chem. Rev., 117, 13187–13229, 2017.</mixed-citation></ref>
      <ref id="bib1.bibx83"><?xmltex \def\ref@label{{Z{\'{a}}dor et~al.(2006)}}?><label>Zádor et al.(2006)</label><?label Zador:2006?><mixed-citation>Zádor, J., Turányi, T., Wirtz, K., and Pilling, M. J.: Measurement and
investigation of chamber radical sources in the European Photoreactor
(EUPHORE), J. Atmos. Chem., 55, 147–166,
<ext-link xlink:href="https://doi.org/10.1007/s10874-006-9033-y" ext-link-type="DOI">10.1007/s10874-006-9033-y</ext-link>, 2006.</mixed-citation></ref>
      <ref id="bib1.bibx84"><label>Zarzana et al.(2018)</label><?label Zarzana:2018?><mixed-citation>Zarzana, K. J., Selimovic, V., Koss, A. R., Sekimoto, K., Coggon, M. M., Yuan, B., Dubé, W. P., Yokelson, R. J., Warneke, C., de Gouw, J. A., Roberts, J. M., and Brown, S. S.: Primary emissions of glyoxal and methylglyoxal from laboratory measurements of open biomass burning, Atmos. Chem. Phys., 18, 15451–15470, <ext-link xlink:href="https://doi.org/10.5194/acp-18-15451-2018" ext-link-type="DOI">10.5194/acp-18-15451-2018</ext-link>, 2018.</mixed-citation></ref>
      <ref id="bib1.bibx85"><label>Zhao and Wang(2017)</label><?label Zhao:2017?><mixed-citation>
Zhao, X. and Wang, L.: Atmospheric Oxidation Mechanism of Furfural Initiated
by Hydroxyl Radicals, J. Phys. Chem. A., 121, 3247–3253, 2017.</mixed-citation></ref>

  </ref-list></back>
    <!--<article-title-html>OH chemistry of non-methane organic gases (NMOGs) emitted from laboratory and ambient biomass burning smoke: evaluating the influence of furans and oxygenated aromatics on ozone and secondary NMOG formation</article-title-html>
<abstract-html><p>Chamber oxidation experiments conducted at the Fire Sciences Laboratory in 2016 are evaluated to identify important chemical processes contributing to the hydroxy radical (OH) chemistry of biomass burning non-methane organic gases (NMOGs).  Based on the decay of primary carbon measured by proton transfer reaction time-of-flight mass spectrometry (PTR-ToF-MS), it is confirmed that furans and oxygenated aromatics are among the NMOGs emitted from western United States fuel types with the highest reactivities towards OH. The oxidation processes and formation of secondary NMOG masses measured by PTR-ToF-MS and iodide-clustering time-of-flight chemical ionization mass spectrometry (I-CIMS) is interpreted using a box model employing a modified version of the Master Chemical Mechanism (v. 3.3.1) that includes the OH oxidation of furan, 2-methylfuran, 2,5-dimethylfuran, furfural, 5-methylfurfural, and guaiacol. The model supports the assignment of major PTR-ToF-MS and I-CIMS signals to a series of anhydrides and hydroxy furanones formed primarily through furan chemistry. This mechanism is applied to a Lagrangian box model used previously to model a real biomass burning plume. The customized mechanism reproduces the decay of furans and oxygenated aromatics and the formation of secondary NMOGs, such as maleic anhydride. Based on model simulations conducted with and without furans, it is estimated that furans contributed up to 10&thinsp;% of ozone and over 90&thinsp;% of maleic anhydride formed within the first 4&thinsp;h of oxidation. It is shown that maleic anhydride is present in a biomass burning plume transported over several days, which demonstrates the utility of anhydrides as markers for aged biomass burning plumes.</p></abstract-html>
<ref-html id="bib1.bib1"><label>Ahern et al.(2018)</label><mixed-citation>
Ahern, A. T., Goldberger, L., Jahl, L., Thornton, J., and Sullivan, R. C.:
Production of N<sub>2</sub>O<sub>5</sub> and ClNO<sub>2</sub> through Nocturnal Processing of Biomass-Burning
Aerosol, Environ. Sci. Technol., 52, 550–559,
<a href="https://doi.org/10.1021/acs.est.7b04386" target="_blank">https://doi.org/10.1021/acs.est.7b04386</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib2"><label>Akagi et al.(2012)</label><mixed-citation>
Akagi, S. K., Craven, J. S., Taylor, J. W., McMeeking, G. R., Yokelson, R. J.,
Burling, I. R., Urbanski, S. P., Wold, C. E., Seinfeld, J. H., Coe, H.,
Alvarado, M. J., and Weise, D. R.: Evolution of trace gases and particles
emitted by a chaparral fire in California, Atmos. Chem. Phys.,
12, 1397–1421, <a href="https://doi.org/10.5194/acp-12-1397-2012" target="_blank">https://doi.org/10.5194/acp-12-1397-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib3"><label>Akagi et al.(2013)</label><mixed-citation>
Akagi, S. K., Yokelson, R. J., Burling, I. R., Meinardi, S., Simpson, I.,
Blake, D. R., McMeeking, G. R., Sullivan, A., Lee, T., Kreidenweis, S.,
Urbanski, S., Reardon, J., Griffith, D. W. T., Johnson, T. J., and Weise,
D. R.: Measurements of reactive trace gases and variable O<sub>3</sub> formation
rates in some South Carolina biomass burning plumes, Atmos. Chem.
Phys., 13, 1141–1165, <a href="https://doi.org/10.5194/acp-13-1141-2013" target="_blank">https://doi.org/10.5194/acp-13-1141-2013</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib4"><label>Alvarado et al.(2010)</label><mixed-citation>
Alvarado, M. J., Logan, J. A., Mao, J., Apel, E., Riemer, D., Blake, D., Cohen, R. C., Min, K.-E., Perring, A. E., Browne, E. C., Wooldridge, P. J., Diskin, G. S., Sachse, G. W., Fuelberg, H., Sessions, W. R., Harrigan, D. L., Huey, G., Liao, J., Case-Hanks, A., Jimenez, J. L., Cubison, M. J., Vay, S. A., Weinheimer, A. J., Knapp, D. J., Montzka, D. D., Flocke, F. M., Pollack, I. B., Wennberg, P. O., Kurten, A., Crounse, J., Clair, J. M. St., Wisthaler, A., Mikoviny, T., Yantosca, R. M., Carouge, C. C., and Le Sager, P.: Nitrogen oxides and PAN in plumes from boreal fires during ARCTAS-B and their impact on ozone: an integrated analysis of aircraft and satellite observations, Atmos. Chem. Phys., 10, 9739–9760, <a href="https://doi.org/10.5194/acp-10-9739-2010" target="_blank">https://doi.org/10.5194/acp-10-9739-2010</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib5"><label>Alvarado et al.(2015)</label><mixed-citation>
Alvarado, M. J., Lonsdale, C. R., Yokelson, R. J., Akagi, S. K., Coe, H., Craven, J. S., Fischer, E. V., McMeeking, G. R., Seinfeld, J. H., Soni, T., Taylor, J. W., Weise, D. R., and Wold, C. E.: Investigating the links between ozone and organic aerosol chemistry in a biomass burning plume from a prescribed fire in California chaparral, Atmos. Chem. Phys., 15, 6667–6688, <a href="https://doi.org/10.5194/acp-15-6667-2015" target="_blank">https://doi.org/10.5194/acp-15-6667-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib6"><label>Alvarez et al.(2009)</label><mixed-citation>
Alvarez, E. G., BorrAs, E., Viidanoja, J., and Hjorth, J.: Unsaturated
dicarbonyl products from the OH-initiated photo-oxidation of furan,
2-methylfuran and 3-methylfuran, Atmos. Environ., 43, 1603–1612,
2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib7"><label>Andreae et al.(1988)</label><mixed-citation>
Andreae, M. O., Browell, E. V., Garstang, M., Gregory, G. L., Harriss, R. C.,
Hill, G. F., Jacob, D. J., Pereira, M. C., Sachse, G. W., Setzer, A. W.,
Dias, P. L. S., Talbot, R. W., Torres, A. L., and Wofsy, S. C.:
Biomass-burning emissions and associated haze layers over Amazonia, J. Geophys. Res.-Atmos., 93, 1509–1527,
<a href="https://doi.org/10.1029/JD093iD02p01509" target="_blank">https://doi.org/10.1029/JD093iD02p01509</a>, 1988.
</mixed-citation></ref-html>
<ref-html id="bib1.bib8"><label>Aschmann et al.(2011)</label><mixed-citation>
Aschmann, S. M., Nishino, N., Arey, J., and Atkinson, R.: Kinetics of the
Reactions of OH Radicals with 2- and 3-Methylfuran, 2,3- and
2,5-Dimethylfuran, and E- and Z-3-Hexene-2,5-dione, and Products of OH +
2,5-Dimethylfuran, Environ. Sci. Technol., 45, 1859–1865,
2011.
</mixed-citation></ref-html>
<ref-html id="bib1.bib9"><label>Aschmann et al.(2014)</label><mixed-citation>
Aschmann, S. M., Nishino, N., Arey, J., and Atkinson, R.: Products of the OH
Radical-Initiated Reactions of Furan, 2- and 3-Methylfuran, and 2,3- and
2,5-Dimethylfuran in the Presence of NO, J. Phys. Chem. A., 118, 457–466,
2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib10"><label>Atkinson et al.(2006)</label><mixed-citation>
Atkinson, R., Baulch, D. L., Cox, R. A., Crowley, J. N., Hampson, R. F., Hynes,
R. G., Jenkin, M. E., Rossi, M. J., Troe, J., and Subcommittee, I.: Evaluated
kinetic and photochemical data for atmospheric chemistry: Volume II – gas
phase reactions of organic species, Atmos. Chem. and Phys., 6,
3625–4055, <a href="https://doi.org/10.5194/acp-6-3625-2006" target="_blank">https://doi.org/10.5194/acp-6-3625-2006</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib11"><label>Barmet et al.(2012)</label><mixed-citation>
Barmet, P., Dommen, J., DeCarlo, P. F., Tritscher, T., Praplan, A. P., Platt, S. M., Prévôt, A. S. H., Donahue, N. M., and Baltensperger, U.: OH clock determination by proton transfer reaction mass spectrometry at an environmental chamber, Atmos. Meas. Tech., 5, 647–656, <a href="https://doi.org/10.5194/amt-5-647-2012" target="_blank">https://doi.org/10.5194/amt-5-647-2012</a>, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib12"><label>Baylon et al.(2017)</label><mixed-citation>
Baylon, P., Jaffe, D. A., de Gouw, J., and Warneke, C.: Influence of
Long-Range Transport of Siberian Biomass Burning at the Mt. Bachelor
Observatory during the Spring of 2015, Aerosol  Air Qual. Res., 17,
2751–2761, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib13"><label>Bian et al.(2015)</label><mixed-citation>
Bian, Q., May, A. A., Kreidenweis, S. M., and Pierce, J. R.: Investigation of
particle and vapor wall-loss effects on controlled wood-smoke smog-chamber
experiments, Atmos. Chem. Phys., 15, 11027–11045,
<a href="https://doi.org/10.5194/acp-15-11027-2015" target="_blank">https://doi.org/10.5194/acp-15-11027-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib14"><label>Bierbach et al.(1994)</label><mixed-citation>
Bierbach, A., Barnes, I., and Becker, K. H.: Atmospheric chemistry of
unsaturated carbonyls: Butenedial, 4-oxo-2-pentenal, 3-hexene-2, 5-dione,
maleic anhydride, 3H-furan-2-one, and 5-methyl-3H-furan-2-one, Environ.
Sci. Technol., 28, 715–729, 1994.
</mixed-citation></ref-html>
<ref-html id="bib1.bib15"><label>Bierbach et al.(1995)</label><mixed-citation>
Bierbach, A., Barnes, I., and Becker, K. H.: Product and kinetic study of the
OH-initiated gas-phase oxidation of furan, 2-methylfuran and furanaldehydes
at  ≈ 300&thinsp;K, Atmos. Environ., 29, 2651–2660, 1995.
</mixed-citation></ref-html>
<ref-html id="bib1.bib16"><label>Brey and Fischer(2016)</label><mixed-citation>
Brey, S. J. and Fischer, E. V.: Smoke in the City: How Often and Where Does
Smoke Impact Summertime Ozone in the United States?, Environ. Sci.
Technol., 50, 1288–1294, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib17"><label>Bruns et al.(2017)</label><mixed-citation>
Bruns, E. A., Slowik, J. G., El Haddad, I., Kilic, D., Klein, F., Dommen, J., Temime-Roussel, B., Marchand, N., Baltensperger, U., and Prévôt, A. S. H.: Characterization of gas-phase organics using proton transfer reaction time-of-flight mass spectrometry: fresh and aged residential wood combustion emissions, Atmos. Chem. Phys., 17, 705–720, <a href="https://doi.org/10.5194/acp-17-705-2017" target="_blank">https://doi.org/10.5194/acp-17-705-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib18"><label>Buhr et al.(2002)</label><mixed-citation>
Buhr, K., van Ruth, S., and Delahunty, C.: Analysis of volatile flavour
compounds by Proton Transfer Reaction-Mass Spectrometry: fragmentation
patterns and discrimination between isobaric and isomeric compounds,
Int. J. Mass Spectrom., 221, 1–7, 2002.
</mixed-citation></ref-html>
<ref-html id="bib1.bib19"><label>Burkholder et al.(2015)</label><mixed-citation>
Burkholder, J., Sander, S., Abbatt, J., Barker, J., Huie, R., Kolb, C., Kurylo,
M., Orkin, V., Wilmouth, D., and Wine, P.: Chemical Kinetics and Photochemical Data for Use in Atmospheric Studies, Evaluation No. 18, JPL Publication 15-10, Jet Propulsion Laboratory, Pasadena,  <a href="http://jpldataeval.jpl.nasa.gov" target="_blank"/> (last access: 4 December 2019), 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib20"><label>Burling et al.(2010)</label><mixed-citation>
Burling, I. R., Yokelson, R. J., Griffith, D. W. T., Johnson, T. J., Veres, P., Roberts, J. M., Warneke, C., Urbanski, S. P., Reardon, J., Weise, D. R., Hao, W. M., and de Gouw, J.: Laboratory measurements of trace gas emissions from biomass burning of fuel types from the southeastern and southwestern United States, Atmos. Chem. Phys., 10, 11115–11130, <a href="https://doi.org/10.5194/acp-10-11115-2010" target="_blank">https://doi.org/10.5194/acp-10-11115-2010</a>, 2010.
</mixed-citation></ref-html>
<ref-html id="bib1.bib21"><label>Chapleski et al.(2016)</label><mixed-citation>
Chapleski, R. C., Zhang, Y., Troya, D., and Morris, J. R.: Heterogeneous
chemistry and reaction dynamics of the atmospheric oxidants, O3, NO3,
and OH, on organic surfaces, Chem. Soc. Rev., 45, 3731–3746,
<a href="https://doi.org/10.1039/C5CS00375J" target="_blank">https://doi.org/10.1039/C5CS00375J</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib22"><label>Colmenar et al.(2015)</label><mixed-citation>
Colmenar, I., González, S., Jiménez, E., Martín, P., Salgado, S.,
Cabañas, B., and Albaladejo, J.: UV absorption cross sections between
290 and 380&thinsp;nm of a series of furanaldehydes: Estimation of their photolysis
lifetimes, Atmos. Environ., 103, 1–6, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib23"><label>Crounse et al.(2013)</label><mixed-citation>
Crounse, J. D., Nielsen, L. B., Jørgensen, S., Kjaergaard, H. G., and
Wennberg, P. O.: Autoxidation of Organic Compounds in the Atmosphere,
J. Phys. Chem. Lett., 4, 3513–3520,
<a href="https://doi.org/10.1021/jz4019207" target="_blank">https://doi.org/10.1021/jz4019207</a>, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib24"><label>Deming et al.(2019)</label><mixed-citation>
Deming, B. L., Pagonis, D., Liu, X., Day, D. A., Talukdar, R., Krechmer, J. E., de Gouw, J. A., Jimenez, J. L., and Ziemann, P. J.: Measurements of delays of gas-phase compounds in a wide variety of tubing materials due to gas-wall interactions, Atmos. Meas. Tech., 12, 3453–3461, <a href="https://doi.org/10.5194/amt-12-3453-2019" target="_blank">https://doi.org/10.5194/amt-12-3453-2019</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib25"><label>Ferreira da Silva et al.(2015)</label><mixed-citation>
Ferreira da Silva, F., Lange, E., Limão-Vieira, P., Jones, N. C., Hoffmann,
S. V., Hubin-Franskin, M. J., Delwiche, J., Brunger, M. J., Neves, R. F. C.,
Lopes, M. C. A., de Oliveira, E. M., da Costa, R. F., Varella, M. T. d. N.,
Bettega, M. H. F., Blanco, F., García, G., Lima, M. A. P., and Jones,
D. B.: Electronic excitation of furfural as probed by high-resolution vacuum
ultraviolet spectroscopy, electron energy loss spectroscopy, and ab
initiocalculations,  J. Chem. Phys., 143, 144308–144314,
2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib26"><label>Finewax et al.(2018)</label><mixed-citation>
Finewax, Z., de Gouw, J. A., and Ziemann, P. J.: Identification and
Quantification of 4-Nitrocatechol Formed from OH and NO<sub>3</sub> Radical-Initiated
Reactions of Catechol in Air in the Presence of NO<sub><i>x</i></sub>: Implications for
Secondary Organic Aerosol Formation from Biomass Burning, Environ.
Sci. Technol., 52, 1981–1989, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib27"><label>Ford et al.(2018)</label><mixed-citation>
Ford, B., Val Martin, M., Zelasky, S. E., Fischer, E. V., Anenberg, S. C.,
Heald, C. L., and Pierce, J. R.: Future Fire Impacts on Smoke
Concentrations, Visibility, and Health in the Contiguous United States,
GeoHealth, 2, 229–247, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib28"><label>Gandini et al.(1976)</label><mixed-citation>
Gandini, A., Parsons, J. M., and Back, R. A.: The photochemistry of
2-furaldehyde vapour. II. Photodecomposition: direct photolysis at 253.7 and
313&thinsp;nm and Hg(3P1)-sensitized decomposition, Can. J. Chem.,
54, 3095–3101, 1976.
</mixed-citation></ref-html>
<ref-html id="bib1.bib29"><label>Gaston et al.(2016)</label><mixed-citation>
Gaston, C. J., Lopez-Hilfiker, F. D., Whybrew, L. E., Hadley, O., McNair, F.,
Gao, H., Jaffe, D. A., and Thornton, J. A.: Online molecular characterization
of fine particulate matter in Port Angeles, WA: Evidence for a major impact
from residential wood smoke, Atmos. Envrion., 138, 99–107,
<a href="https://doi.org/10.1016/j.atmosenv.2016.05.013" target="_blank">https://doi.org/10.1016/j.atmosenv.2016.05.013</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib30"><label>Gilman et al.(2015)</label><mixed-citation>
Gilman, J. B., Lerner, B. M., Kuster, W. C., Goldan, P. D., Warneke, C., Veres, P. R., Roberts, J. M., de Gouw, J. A., Burling, I. R., and Yokelson, R. J.: Biomass burning emissions and potential air quality impacts of volatile organic compounds and other trace gases from fuels common in the US, Atmos. Chem. Phys., 15, 13915–13938, <a href="https://doi.org/10.5194/acp-15-13915-2015" target="_blank">https://doi.org/10.5194/acp-15-13915-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib31"><label>Hartikainen et al.(2018)</label><mixed-citation>
Hartikainen, A., Yli-Pirilä, P., Tiitta, P., Leskinen, A., Kortelainen, M.,
Orasche, J., Schnelle-Kreis, J., Lehtinen, K. E. J., Zimmermann, R.,
Jokiniemi, J., and Sippula, O.: Volatile Organic Compounds from Logwood
Combustion: Emissions and Transformation under Dark and Photochemical Aging
Conditions in a Smog Chamber, Environ. Sci. Technol., 52,
4979–4988, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib32"><label>Hatch et al.(2015)</label><mixed-citation>
Hatch, L. E., Luo, W., Pankow, J. F., Yokelson, R. J., Stockwell, C. E., and Barsanti, K. C.: Identification and quantification of gaseous organic compounds emitted from biomass burning using two-dimensional gas chromatography–time-of-flight mass spectrometry, Atmos. Chem. Phys., 15, 1865–1899, <a href="https://doi.org/10.5194/acp-15-1865-2015" target="_blank">https://doi.org/10.5194/acp-15-1865-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib33"><label>Hatch et al.(2017)</label><mixed-citation>
Hatch, L. E., Yokelson, R. J., Stockwell, C. E., Veres, P. R., Simpson, I. J., Blake, D. R., Orlando, J. J., and Barsanti, K. C.: Multi-instrument comparison and compilation of non-methane organic gas emissions from biomass burning and implications for smoke-derived secondary organic aerosol precursors, Atmos. Chem. Phys., 17, 1471–1489, <a href="https://doi.org/10.5194/acp-17-1471-2017" target="_blank">https://doi.org/10.5194/acp-17-1471-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib34"><label>Hiraoka and Srinivasan(1968)</label><mixed-citation>
Hiraoka, H. and Srinivasan, R.: Vapor-Phase Photochemistry of Furfural, The
J. Chem. Phys., 48, 2185–2189, 1968.
</mixed-citation></ref-html>
<ref-html id="bib1.bib35"><label>Hobbs et al.(2003)</label><mixed-citation>
Hobbs, P. V., Sinha, P., Yokelson, R. J., Christian, T. J., Blake, D. R., Gao,
S., Kirchstetter, T. W., Novakov, T., and Pilewskie, P.: Evolution of gases
and particles from a savanna fire in South Africa, J. Geophys.
Res., 108, 8485, <a href="https://doi.org/10.1029/2002JD002352" target="_blank">https://doi.org/10.1029/2002JD002352</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib36"><label>Hodshire et al.(2019)</label><mixed-citation>
Hodshire, A. L., Bian, Q., Ramnarine, E., Lonsdale, C. R., Alvarado, M. J.,
Kreidenweis, S. M., Jathar, S. H., and Pierce, J. R.: More Than Emissions and
Chemistry: Fire Size, Dilution, and Background Aerosol Also Greatly Influence
Near-Field Biomass Burning Aerosol Aging, J. Geophys. Res.-Atmos., 124, 5589–5611, <a href="https://doi.org/10.1029/2018JD029674" target="_blank">https://doi.org/10.1029/2018JD029674</a>,
2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib37"><label>Huey et al.(1995)</label><mixed-citation>
Huey, L. G., Hanson, D. R., and Howard, C. J.: Reactions of SF6- and I- with
Atmospheric Trace Gases,   J. Phys. Chem., 99, 5001–5008,
<a href="https://doi.org/10.1021/j100014a021" target="_blank">https://doi.org/10.1021/j100014a021</a>, 1995.
</mixed-citation></ref-html>
<ref-html id="bib1.bib38"><label>Jaffe et al.(2008)</label><mixed-citation>
Jaffe, D., Chand, D., Hafner, W., Westerling, A., and Spracklen, D.: Influence
of Fires on O<sub>3</sub> Concentrations in the Western US, Environ. Sci.
Technol., 42, 5885–5891, 2008.
</mixed-citation></ref-html>
<ref-html id="bib1.bib39"><label>Jaffe and Wigder(2012)</label><mixed-citation>
Jaffe, D. A. and Wigder, N. L.: Ozone production from wildfires: A critical
review, Atmos. Environ., 51, 1–10, 2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib40"><label>Jaffe et al.(2013)</label><mixed-citation>
Jaffe, D. A., Wigder, N., Downey, N., Pfister, G., Boynard, A., and Reid,
S. B.: Impact of Wildfires on Ozone Exceptional Events in the Western US,
Environ. Sci. Technol., 47, 11065–11072, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib41"><label>Jaffe et al.(2018)</label><mixed-citation>
Jaffe, D. A., Cooper, O. R., Fiore, A. M., Henderson, B. H., Tonneson, G. S.,
Russell, A. G., Henze, D. K., Langford, A. O., Lin, M., and Moore, T.:
Scientific assessment of background ozone over the US: Implications for
air quality management, Elem. Sci. Anth., 6, 30 pp., 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib42"><label>Jenkin et al.(1997)</label><mixed-citation>
Jenkin, M. E., Saunders, S. M., and Pilling, M. J.: The tropospheric
degradation of volatile organic compounds: a protocol for mechanism
development, Atmos. Environ., 31, 81–104, 1997.
</mixed-citation></ref-html>
<ref-html id="bib1.bib43"><label>Jenkin et al.(2003)</label><mixed-citation>
Jenkin, M. E., Saunders, S. M., Wagner, V., and Pilling, M. J.: Protocol for the development of the Master Chemical Mechanism, MCM v3 (Part B): tropospheric degradation of aromatic volatile organic compounds, Atmos. Chem. Phys., 3, 181–193, <a href="https://doi.org/10.5194/acp-3-181-2003" target="_blank">https://doi.org/10.5194/acp-3-181-2003</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib44"><label>Jenkin et al.(2015)</label><mixed-citation>
Jenkin, M. E., Young, J. C., and Rickard, A. R.: The MCM v3.3.1 degradation scheme for isoprene, Atmos. Chem. Phys., 15, 11433–11459, <a href="https://doi.org/10.5194/acp-15-11433-2015" target="_blank">https://doi.org/10.5194/acp-15-11433-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib45"><label>Keller-Rudek et al.(2013)</label><mixed-citation>
Keller-Rudek, H., Moortgat, G. K., Sander, R., and Sörensen, R.: The
MPI-Mainz UV/VIS Spectral Atlas of Gaseous Molecules of Atmospheric Interest,
Earth Syst. Sci. Data, 5, 365–373, <a href="https://doi.org/10.5194/essd-5-365-2013" target="_blank">https://doi.org/10.5194/essd-5-365-2013</a>,
2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib46"><label>Koss et al.(2018)</label><mixed-citation>
Koss, A. R., Sekimoto, K., Gilman, J. B., Selimovic, V., Coggon, M. M.,
Zarzana, K. J., Yuan, B., Lerner, B. M., Brown, S. S., Jimenez, J. L.,
Krechmer, J., Roberts, J. M., Warneke, C., Yokelson, R. J., and de Gouw, J.:
Non-methane organic gas emissions from biomass burning: identification,
quantification, and emission factors from PTR-ToF during the FIREX 2016
laboratory experiment, Atmos. Chem. Phys., 18, 3299–3319,
<a href="https://doi.org/10.5194/acp-18-3299-2018" target="_blank">https://doi.org/10.5194/acp-18-3299-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib47"><label>Krechmer et al.(2016)</label><mixed-citation>
Krechmer, J. E., Pagonis, D., Ziemann, P. J., and Jimenez, J. L.:
Quantification of Gas-Wall Partitioning in Teflon Environmental Chambers
Using Rapid Bursts of Low-Volatility Oxidized Species Generated in Situ,
Environ. Sci. Technol., 50, 5757–5765,
<a href="https://doi.org/10.1021/acs.est.6b00606" target="_blank">https://doi.org/10.1021/acs.est.6b00606</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib48"><label>Lauraguais et al.(2014)</label><mixed-citation>
Lauraguais, A., Coeur-Tourneur, C., Cassez, A., Deboudt, K., Fourmentin, M.,
and Choël, M.: Atmospheric reactivity of hydroxyl radicals with guaiacol
(2-methoxyphenol), a biomass burning emitted compound: Secondary organic
aerosol formation and gas-phase oxidation products, Atmos. Environ.,
86, 155–163, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib49"><label>Lee et al.(2014)</label><mixed-citation>
Lee, B. H., Lopez-Hilfiker, F. D., Mohr, C., Kurtén, T., Worsnop, D. R.,
and Thornton, J. A.: An Iodide-Adduct High-Resolution Time-of-Flight
Chemical-Ionization Mass Spectrometer: Application to Atmospheric Inorganic
and Organic Compounds, Enviro. Sci. Technol., 48,
6309–6317, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib50"><label>Lim et al.(2019)</label><mixed-citation>
Lim, C. Y., Hagan, D. H., Coggon, M. M., Koss, A. R., Sekimoto, K., de Gouw,
J., Warneke, C., Cappa, C. D., and Kroll, J. H.: Secondary organic aerosol
formation from the laboratory oxidation of biomass burning emissions,
Atmos. Chem. Phys., 19, 12797–12809,
<a href="https://doi.org/10.5194/acp-19-12797-2019" target="_blank">https://doi.org/10.5194/acp-19-12797-2019</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib51"><label>Liu et al.(1999)</label><mixed-citation>
Liu, X., Jeffries, H. E., and Sexton, K. G.: Atmospheric Photochemical
Degradation of 1,4-Unsaturated Dicarbonyls, Environ. Sci.
Technol., 33, 4212–4220, 1999.
</mixed-citation></ref-html>
<ref-html id="bib1.bib52"><label>Liu et al.(2016)</label><mixed-citation>
Liu, X., Zhang, Y., Huey, L. G., Yokelson, R. J., Wang, Y., Jimenez, J. L.,
Campuzano-Jost, P., Beyersdorf, A. J., Blake, D. R., Choi, Y., St. Clair,
J. M., Crounse, J. D., Day, D. A., Diskin, G. S., Fried, A., Hall, S. R.,
Hanisco, T. F., King, L. E., Meinardi, S., Mikoviny, T., Palm, B. B.,
Peischl, J., Perring, A. E., Pollack, I. B., Ryerson, T. B., Sachse, G.,
Schwarz, J. P., Simpson, I. J., Tanner, D. J., Thornhill, K. L., Ullmann, K.,
Weber, R. J., Wennberg, P. O., Wisthaler, A., Wolfe, G. M., and Ziemba,
L. D.: Agricultural fires in the southeastern US during SEAC4RS: Emissions
of trace gases and particles and evolution of ozone, reactive nitrogen, and
organic aerosol, J. Geophys. Res.-Atmos., 121,
7383–7414, <a href="https://doi.org/10.1002/2016JD025040" target="_blank">https://doi.org/10.1002/2016JD025040</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib53"><label>Mason et al.(2001)</label><mixed-citation>
Mason, S. A., Field, R. J., Yokelson, R. J., Kochivar, M. A., Tinsley, M. R.,
Ward, D. E., and Hao, W. M.: Complex effects arising in smoke plume
simulations due to inclusion of direct emissions of oxygenated organic
species from biomass combustion, J. Geophys. Res.-Atmos., 106, 12527–12539, <a href="https://doi.org/10.1029/2001JD900003" target="_blank">https://doi.org/10.1029/2001JD900003</a>, 2001.
</mixed-citation></ref-html>
<ref-html id="bib1.bib54"><label>Mauzerall et al.(1998)</label><mixed-citation>
Mauzerall, D. L., Logan, J. A., Jacob, D. J., Anderson, B. E., Blake, D. R.,
Bradshaw, J. D., Heikes, B., Sachse, G. W., Singh, H., and Talbot, B.:
Photochemistry in biomass burning plumes and implications for tropospheric
ozone over the tropical South Atlantic, Geophys. Res., 103, 8401–8423, 1998.
</mixed-citation></ref-html>
<ref-html id="bib1.bib55"><label>Millet et al.(2015)</label><mixed-citation>
Millet, D. B., Baasandorj, M., Farmer, D. K., Thornton, J. A., Baumann, K., Brophy, P., Chaliyakunnel, S., de Gouw, J. A., Graus, M., Hu, L., Koss, A., Lee, B. H., Lopez-Hilfiker, F. D., Neuman, J. A., Paulot, F., Peischl, J., Pollack, I. B., Ryerson, T. B., Warneke, C., Williams, B. J., and Xu, J.: A large and ubiquitous source of atmospheric formic acid, Atmos. Chem. Phys., 15, 6283–6304, https://doi.org/10.5194/acp-15-6283-2015, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib56"><label>Müller et al.(2016)</label><mixed-citation>
Müller, M., Anderson, B. E., Beyersdorf, A. J., Crawford, J. H., Diskin, G. S., Eichler, P., Fried, A., Keutsch, F. N., Mikoviny, T., Thornhill, K. L., Walega, J. G., Weinheimer, A. J., Yang, M., Yokelson, R. J., and Wisthaler, A.: In situ measurements and modeling of reactive trace gases in a small biomass burning plume, Atmos. Chem. Phys., 16, 3813–3824, <a href="https://doi.org/10.5194/acp-16-3813-2016" target="_blank">https://doi.org/10.5194/acp-16-3813-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib57"><label>Orlando and Tyndall(2012)</label><mixed-citation>
Orlando, J. J. and Tyndall, G. S.: Laboratory studies of organic peroxy radical
chemistry: an overview with emphasis on recent issues of atmospheric
significance, Chem. Soc. Rev., 41, 6294–6317, <a href="https://doi.org/10.1039/c2cs35166h" target="_blank">https://doi.org/10.1039/c2cs35166h</a>,
2012.
</mixed-citation></ref-html>
<ref-html id="bib1.bib58"><label>Pagonis et al.(2017)</label><mixed-citation>
Pagonis, D., Krechmer, J. E., de Gouw, J., Jimenez, J. L., and Ziemann, P. J.: Effects of gas-wall partitioning in Teflon tubing and instrumentation on time-resolved measurements of gas-phase organic compounds, Atmos. Meas. Tech., 10, 4687–4696, <a href="https://doi.org/10.5194/amt-10-4687-2017" target="_blank">https://doi.org/10.5194/amt-10-4687-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib59"><label>Pagonis et al.(2019)</label><mixed-citation>
Pagonis, D., Sekimoto, K., and de Gouw, J.: A library of proton-transfer
reactions of H<sub>3</sub>O<sub>+</sub> ions used for trace gas detection, J. Am. Soc. Mass
Spectrom.,   30, 1330–1335, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib60"><label>Peng and Jimenez(2017)</label><mixed-citation>
Peng, Z. and Jimenez, J. L.: Modeling of the chemistry in oxidation flow reactors with high initial NO, Atmos. Chem. Phys., 17, 11991–12010, <a href="https://doi.org/10.5194/acp-17-11991-2017" target="_blank">https://doi.org/10.5194/acp-17-11991-2017</a>, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib61"><label>Peng et al.(2016)</label><mixed-citation>
Peng, Z., Day, D. A., Ortega, A. M., Palm, B. B., Hu, W., Stark, H., Li, R., Tsigaridis, K., Brune, W. H., and Jimenez, J. L.: Non-OH chemistry in oxidation flow reactors for the study of atmospheric chemistry systematically examined by modeling, Atmos. Chem. Phys., 16, 4283–4305, <a href="https://doi.org/10.5194/acp-16-4283-2016" target="_blank">https://doi.org/10.5194/acp-16-4283-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib62"><label>Peng et al.(2019)</label><mixed-citation>
Peng, Z., Lee-Taylor, J., Orlando, J. J., Tyndall, G. S., and Jimenez, J. L.:
Organic peroxy radical chemistry in oxidation flow reactors and environmental
chambers and their atmospheric relevance, Atmos. Chem. Phys.,
19, 813–834, <a href="https://doi.org/10.5194/acp-19-813-2019" target="_blank">https://doi.org/10.5194/acp-19-813-2019</a>, 2019.
</mixed-citation></ref-html>
<ref-html id="bib1.bib63"><label>Praske et al.(2018)</label><mixed-citation>
Praske, E., Otkjær, R. V., Crounse, J. D., Hethcox, J. C., Stoltz, B. M.,
Kjaergaard, H. G., and Wennberg, P. O.: Atmospheric autoxidation is
increasingly important in urban and suburban North America, P. Natl. Acad. Sci. USA, 115, 64–69, <a href="https://doi.org/10.1073/pnas.1715540115" target="_blank">https://doi.org/10.1073/pnas.1715540115</a>,
2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib64"><label>Priestley et al.(2018)</label><mixed-citation>
Priestley, M., Le Breton, M., Bannan, T. J., Leather, K. E., Bacak, A.,
Reyes-Villegas, E., De Vocht, F., Shallcross, B. M. A., Brazier, T.,
Anwar Khan, M., Allan, J., Shallcross, D. E., Coe, H., and Percival, C. J.:
Observations of Isocyanate, Amide, Nitrate, and Nitro Compounds From an
Anthropogenic Biomass Burning Event Using a ToF-CIMS, J. Geophys.
Res.-Atmos., 123, 7687–7704, <a href="https://doi.org/10.1002/2017JD027316" target="_blank">https://doi.org/10.1002/2017JD027316</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib65"><label>Reyes-Villegas et al.(2018)</label><mixed-citation>
Reyes-Villegas, E., Priestley, M., Ting, Y.-C., Haslett, S., Bannan, T.,
Le Breton, M., Williams, P. I., Bacak, A., Flynn, M. J., Coe, H., Percival,
C., and Allan, J. D.: Simultaneous aerosol mass spectrometry and chemical
ionisation mass spectrometry measurements during a biomass burning event in
the UK: insights into nitrate chemistry, Atmos. Chem. Phys.,
18, 4093–4111, <a href="https://doi.org/10.5194/acp-18-4093-2018" target="_blank">https://doi.org/10.5194/acp-18-4093-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib66"><label>Saunders et al.(2003)</label><mixed-citation>
Saunders, S. M., Jenkin, M. E., Derwent, R. G., and Pilling, M. J.: Protocol for the development of the Master Chemical Mechanism, MCM v3 (Part A): tropospheric degradation of non-aromatic volatile organic compounds, Atmos. Chem. Phys., 3, 161–180, <a href="https://doi.org/10.5194/acp-3-161-2003" target="_blank">https://doi.org/10.5194/acp-3-161-2003</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib67"><label>Sekimoto et al.(2017)</label><mixed-citation>
Sekimoto, K., Li, S.-M., Yuan, B., Koss, A., Coggon, M., Warneke, C., and
de Gouw, J.: Calculation of the sensitivity of proton-transfer-reaction mass
spectrometry (PTR-MS) for organic trace gases using molecular properties,
Int. J. Mass Spectrom., 421, 71–94, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib68"><label>Sekimoto et al.(2018)</label><mixed-citation>
Sekimoto, K., Koss, A. R., Gilman, J. B., Selimovic, V., Coggon, M. M., Zarzana, K. J., Yuan, B., Lerner, B. M., Brown, S. S., Warneke, C., Yokelson, R. J., Roberts, J. M., and de Gouw, J.: High- and low-temperature pyrolysis profiles describe volatile organic compound emissions from western US wildfire fuels, Atmos. Chem. Phys., 18, 9263–9281, <a href="https://doi.org/10.5194/acp-18-9263-2018" target="_blank">https://doi.org/10.5194/acp-18-9263-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib69"><label>Selimovic et al.(2018)</label><mixed-citation>
Selimovic, V., Yokelson, R. J., Warneke, C., Roberts, J. M., de Gouw, J.,
Reardon, J., and Griffith, D. W. T.: Aerosol optical properties and trace gas
emissions by PAX and OP-FTIR for laboratory-simulated western US wildfires
during FIREX, Atmos. Chem. Phys., 18, 2929–2948,
<a href="https://doi.org/10.5194/acp-18-2929-2018" target="_blank">https://doi.org/10.5194/acp-18-2929-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib70"><label>Stockwell et al.(2014)</label><mixed-citation>
Stockwell, C. E., Yokelson, R. J., Kreidenweis, S. M., Robinson, A. L., DeMott,
P. J., Sullivan, R. C., Reardon, J., Ryan, K. C., Griffith, D. W. T., and
Stevens, L.: Trace gas emissions from combustion of peat, crop residue,
domestic biofuels, grasses, and other fuels: configuration and Fourier
transform infrared (FTIR) component of the fourth Fire Lab at Missoula
Experiment (FLAME-4), Atmos. Chem. Phys., 14, 9727–9754,
<a href="https://doi.org/10.5194/acp-14-9727-2014" target="_blank">https://doi.org/10.5194/acp-14-9727-2014</a>, 2014.
</mixed-citation></ref-html>
<ref-html id="bib1.bib71"><label>Stockwell et al.(2015)</label><mixed-citation>
Stockwell, C. E., Veres, P. R., Williams, J., and Yokelson, R. J.:
Characterization of biomass burning emissions from cooking fires, peat, crop
residue, and other fuels with high-resolution proton-transfer-reaction
time-of-flight mass spectrometry, Atmos. Chem. Phys., 15,
845–865, <a href="https://doi.org/10.5194/acp-15-845-2015" target="_blank">https://doi.org/10.5194/acp-15-845-2015</a>, 2015.
</mixed-citation></ref-html>
<ref-html id="bib1.bib72"><label>Stockwell et al.(2018)</label><mixed-citation>
Stockwell, C. E., Kupc, A., Witkowski, B., Talukdar, R. K., Liu, Y., Selimovic, V., Zarzana, K. J., Sekimoto, K., Warneke, C., Washenfelder, R. A., Yokelson, R. J., Middlebrook, A. M., and Roberts, J. M.: Characterization of a catalyst-based conversion technique to measure total particulate nitrogen and organic carbon and comparison to a particle mass measurement instrument, Atmos. Meas. Tech., 11, 2749–2768, <a href="https://doi.org/10.5194/amt-11-2749-2018" target="_blank">https://doi.org/10.5194/amt-11-2749-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib73"><label>Strollo and Ziemann(2013)</label><mixed-citation>
Strollo, C. M. and Ziemann, P. J.: Products and mechanism of secondary organic
aerosol formation from the reaction of 3-methylfuran with OH radicals in the
presence of NO<sub>x</sub>, Atmos. Environ., 77, 534–543, 2013.
</mixed-citation></ref-html>
<ref-html id="bib1.bib74"><label>Tomaz et al.(2018)</label><mixed-citation>
Tomaz, S., Cui, T., Chen, Y., Sexton, K. G., Roberts, J. M., Warneke, C.,
Yokelson, R. J., Surratt, J. D., and Turpin, B. J.: Photochemical Cloud
Processing of Primary Wildfire Emissions as a Potential Source of Secondary
Organic Aerosol, Environ. Sci. Technol., 52, 11027–11037,
<a href="https://doi.org/10.1021/acs.est.8b03293" target="_blank">https://doi.org/10.1021/acs.est.8b03293</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib75"><label>Westerling(2006)</label><mixed-citation>
Westerling, A. L.: Warming and Earlier Spring Increase Western US Forest
Wildfire Activity, Science, 313, 940–943, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib76"><label>Wolfe et al.(2016)</label><mixed-citation>
Wolfe, G. M., Marvin, M. R., Roberts, S. J., Travis, K. R., and Liao, J.: The Framework for 0-D Atmospheric Modeling (F0AM) v3.1, Geosci. Model Dev., 9, 3309–3319, <a href="https://doi.org/10.5194/gmd-9-3309-2016" target="_blank">https://doi.org/10.5194/gmd-9-3309-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib77"><label>Yee et al.(2013)</label><mixed-citation>
Yee, L. D., Kautzman, K. E., Loza, C. L., Schilling, K. A., Coggon, M. M., Chhabra, P. S., Chan, M. N., Chan, A. W. H., Hersey, S. P., Crounse, J. D., Wennberg, P. O., Flagan, R. C., and Seinfeld, J. H.: Secondary organic aerosol formation from biomass burning intermediates: phenol and methoxyphenols, Atmos. Chem. Phys., 13, 8019–8043, <a href="https://doi.org/10.5194/acp-13-8019-2013" target="_blank">https://doi.org/10.5194/acp-13-8019-2013</a>, 2013.

</mixed-citation></ref-html>
<ref-html id="bib1.bib78"><label>Yokelson et al.(1996)</label><mixed-citation>
Yokelson, R. J., Griffith, D. W. T., and Ward, D. E.: Open-path Fourier
transform infrared studies of large-scale laboratory biomass fires, J. Geophys. Res.-Atmos., 101, 21067–21080,
<a href="https://doi.org/10.1029/96JD01800" target="_blank">https://doi.org/10.1029/96JD01800</a>, 1996.
</mixed-citation></ref-html>
<ref-html id="bib1.bib79"><label>Yokelson et al.(2003)</label><mixed-citation>
Yokelson, R. J., Bertschi, I. T., Christian, T. J., Hobbs, P. V., Ward, D. E.,
and Hao, W. M.: Trace gas measurements in nascent, aged, and cloud-processed
smoke from African savanna fires by airborne Fourier transform infrared
spectroscopy (AFTIR), J. Geophys. Res., 108,  8478,
<a href="https://doi.org/10.1029/2002JD002322" target="_blank">https://doi.org/10.1029/2002JD002322</a>, 2003.
</mixed-citation></ref-html>
<ref-html id="bib1.bib80"><label>Yokelson et al.(2009)</label><mixed-citation>
Yokelson, R. J., Crounse, J. D., DeCarlo, P. F., Karl, T., Urbanski, S., Atlas,
E., Campos, T., Shinozuka, Y., Kapustin, V., Clarke, A. D., Weinheimer, A.,
Knapp, D. J., Montzka, D. D., Holloway, J., Weibring, P., Flocke, F., Zheng,
W., Toohey, D., Wennberg, P. O., Wiedinmyer, C., Mauldin, L., Fried, A.,
Richter, D., Walega, J., Jimenez, J. L., Adachi, K., Buseck, P. R., Hall,
S. R., and Shetter, R.: Emissions from biomass burning in the Yucatan,
Atmos. Chem. Phys., 9, 5785–5812,
<a href="https://doi.org/10.5194/acp-9-5785-2009" target="_blank">https://doi.org/10.5194/acp-9-5785-2009</a>, 2009.
</mixed-citation></ref-html>
<ref-html id="bib1.bib81"><label>Yuan et al.(2016)</label><mixed-citation>
Yuan, B., Koss, A., Warneke, C., Gilman, J. B., Lerner, B. M., Stark, H., and
de Gouw, J. A.: A high-resolution time-of-flight chemical ionization mass
spectrometer utilizing hydronium ions (H<sub>3</sub>O<sup>+</sup> ToF-CIMS) for
measurements of volatile organic compounds in the atmosphere, Atmos.
Meas. Tech., 9, 2735–2752, <a href="https://doi.org/10.5194/amt-9-2735-2016" target="_blank">https://doi.org/10.5194/amt-9-2735-2016</a>, 2016.
</mixed-citation></ref-html>
<ref-html id="bib1.bib82"><label>Yuan et al.(2017)</label><mixed-citation>
Yuan, B., Koss, A. R., Warneke, C., Coggon, M., Sekimoto, K., and de Gouw,
J. A.: Proton-Transfer-Reaction Mass Spectrometry: Applications in
Atmospheric Sciences, Chem. Rev., 117, 13187–13229, 2017.
</mixed-citation></ref-html>
<ref-html id="bib1.bib83"><label>Zádor et al.(2006)</label><mixed-citation>
Zádor, J., Turányi, T., Wirtz, K., and Pilling, M. J.: Measurement and
investigation of chamber radical sources in the European Photoreactor
(EUPHORE), J. Atmos. Chem., 55, 147–166,
<a href="https://doi.org/10.1007/s10874-006-9033-y" target="_blank">https://doi.org/10.1007/s10874-006-9033-y</a>, 2006.
</mixed-citation></ref-html>
<ref-html id="bib1.bib84"><label>Zarzana et al.(2018)</label><mixed-citation>
Zarzana, K. J., Selimovic, V., Koss, A. R., Sekimoto, K., Coggon, M. M., Yuan, B., Dubé, W. P., Yokelson, R. J., Warneke, C., de Gouw, J. A., Roberts, J. M., and Brown, S. S.: Primary emissions of glyoxal and methylglyoxal from laboratory measurements of open biomass burning, Atmos. Chem. Phys., 18, 15451–15470, <a href="https://doi.org/10.5194/acp-18-15451-2018" target="_blank">https://doi.org/10.5194/acp-18-15451-2018</a>, 2018.
</mixed-citation></ref-html>
<ref-html id="bib1.bib85"><label>Zhao and Wang(2017)</label><mixed-citation>
Zhao, X. and Wang, L.: Atmospheric Oxidation Mechanism of Furfural Initiated
by Hydroxyl Radicals, J. Phys. Chem. A., 121, 3247–3253, 2017.
</mixed-citation></ref-html>--></article>
