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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Research article}?>
  <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-23-8473-2023</article-id><title-group><article-title>Daytime isoprene nitrates under changing NO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula></article-title><alt-title>Daytime Isoprene Nitrates Under Changing NO<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula></alt-title>
      </title-group><?xmltex \runningtitle{Daytime Isoprene Nitrates Under Changing NO${}_{{x}}$ and O${}_{{3}}$}?><?xmltex \runningauthor{A. W. Mayhew et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mayhew</surname><given-names>Alfred W.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5277-1331</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Edwards</surname><given-names>Peter M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1076-6793</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Hamilton</surname><given-names>Jaqueline F.</given-names></name>
          <email>jacqui.hamilton@york.ac.uk</email>
        </contrib>
        <aff id="aff1"><label>1</label><institution>Wolfson Atmospheric Chemistry Laboratories, Department of Chemistry,<?xmltex \hack{\break}?> University of York, Heslington, York, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>National Centre for Atmospheric Science, University of York, York, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jaqueline F. Hamilton (jacqui.hamilton@york.ac.uk)</corresp></author-notes><pub-date><day>31</day><month>July</month><year>2023</year></pub-date>
      
      <volume>23</volume>
      <issue>14</issue>
      <fpage>8473</fpage><lpage>8485</lpage>
      <history>
        <date date-type="received"><day>10</day><month>February</month><year>2023</year></date>
           <date date-type="rev-request"><day>21</day><month>February</month><year>2023</year></date>
           <date date-type="rev-recd"><day>22</day><month>June</month><year>2023</year></date>
           <date date-type="accepted"><day>26</day><month>June</month><year>2023</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2023 </copyright-statement>
        <copyright-year>2023</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="d1e142">Organonitrates are important species in the atmosphere due to their impacts on NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, HO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, and O<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> budgets, and their potential to contribute to secondary organic aerosol (SOA) mass. This work presents a steady-state modelling approach to assess the impacts of changes in NO<inline-formula><mml:math id="M8" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations on the organonitrates produced from
isoprene oxidation. The diverse formation pathways to isoprene organonitrates dictate the responses of different groups of organonitrates
to changes in O<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. For example, organonitrates predominantly formed from the OH-initiated oxidation of isoprene favour
formation under lower-ozone and moderate-NO<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations, whereas
organonitrates formed via daytime NO<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation show the highest
formation under high-O<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations with little dependence on
NO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations. Investigating the response of total organonitrates
reveals complex and nonlinear behaviour with implications that could inform
expectations of changes to organonitrate concentrations as efforts are made
to reduce NO<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations, including a region of
NO<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> space where total organonitrate concentration is relatively insensitive to changes in NO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. These conclusions are further contextualised by estimating the volatility of the isoprene organonitrates revealing the potential for high concentrations of low-volatility species under high-ozone conditions.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Natural Environment Research Council</funding-source>
<award-id>NE/S007458/1</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e309">Organonitrates are important species in the atmosphere due to their impacts on NO<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, HO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, and O<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> budgets through
gas-phase chemistry (Emmerson and Evans, 2009; Bates and Jacob, 2019;
Schwantes et al., 2019, 2020; Vasquez et al., 2020) Their
relatively low volatility also results in the potential to form secondary
organic aerosol (SOA) via condensation onto existing particles, and some
organonitrates can undergo reactive uptake to the particle
phase (Hallquist et al., 2009; Schwantes et al., 2019; Palmer et al.,
2022) Isoprene organonitrates have been widely studied due to the large
emissions of isoprene resulting in the relevance of isoprene chemistry to a
range of environments around the globe (Guenther et al., 2006; Pye et
al., 2015; Reeves et al., 2021; Tsiligiannis et al., 2022).</p>
      <p id="d1e339">Isoprene hydroxynitrate (IHN) is widely studied due to its formation from OH
oxidation in the presence of NO resulting in high concentrations during the
daytime (Fig. 1) (Xiong et al., 2015; Wennberg
et al., 2018) IHN also has formation routes from oxidation with the nitrate
radical (NO<inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Other commonly studied isoprene mononitrates include
isoprene carbonyl nitrate (ICN) and isoprene hydroperoxy nitrate (IPN). IPN
forms through the initial NO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation of isoprene to form an isoprene
nitrooxyperoxy radical (INO<inline-formula><mml:math id="M27" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The reaction of INO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with HO<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> then forms IPN. ICN has a range of formation pathways initiated by OH and
NO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation. Isoprene dinitrate (IDN) can also form from INO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by
its reaction with NO.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e414">Formation routes to form IHN, ICN, IPN, and IDN from the OH- and
NO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-initiated oxidation of isoprene. Additional isomers and reaction
pathways have been omitted for clarity.</p></caption>
        <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f01.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e435">Established formation routes to form IEPOX and INHE via the OH
oxidation of stable hydroperoxide intermediates. Additional isomers and
reaction pathways have been omitted for clarity.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f02.png"/>

      </fig>

      <p id="d1e444">Isoprene epoxides, such as isoprene epoxydiols (IEPOX), have long been of
interest due to their potential to contribute to SOA by reactive uptake to
acidified particles (Paulot et al., 2009; Surratt et al., 2010). Later
work outlined the similar SOA-forming properties for the nitrated epoxide,
isoprene nitrooxyhydroxy epoxide (INHE), with the first proposed formation
route to INHE involving the OH oxidation of IPN (Fig. 2) (Schwantes et al.,
2015) Recent work aiming to improve the representation of isoprene<?pagebreak page8474?> NO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
chemistry in chemical mechanisms highlighted a previously unrepresented
reaction pathway to forming nitrated epoxides from alkoxy radicals (RO)
(Vereecken et al., 2021; Carlsson et al., 2023). This alkoxy-epoxidation
pathway provides an alternative formation route to INHE that does not rely on
a stable intermediate or the presence of OH (Fig. 3). Additionally, three more nitrated epoxides can result from this pathway: isoprene nitrooxycarbonyl epoxide (INCE), isoprene
nitrooxyhydroperoxy epoxide (INPE), and isoprene dinitrooxy epoxide (IDNE).</p>
      <p id="d1e456">The motivation for the work presented here is based on  findings from the 2017 Atmospheric Pollution and Human Health (APHH) in a Chinese Megacity summer campaign in Beijing, showing the role of NO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> in the formation of
isoprene organonitrates and their successive particle-phase products,
including the afternoon period due to the presence of high-O<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations (Hamilton et al., 2021; Newland et al., 2021). The
presence of high-O<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations increased the conversion of NO to
NO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> which subsequently reduced the loss of NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> to reaction with
NO. Geyer (2003) first highlighted this in 2003, calculating daytime NO<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios of up to 2–5 ppt during the afternoon during a haze period in La Porte, Texas (Geyer, 2003). Since then, daytime NO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> has been highlighted as a potentially important chemical pathway from a range of field campaigns in various cities around the world (Brown et al., 2005; Osthoff et al., 2006; Khan et al., 2015; Xue et al., 2016; Wang et al., 2020; Foulds et al., 2021). Daytime NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> chemistry has also been shown to be potentially significant under forest canopies, where photolytic processes are diminished (Forkel et al., 2006; Hu et al., 2013; Mermet et al., 2021).</p>
      <p id="d1e532">The co-occurrence of organonitrate formation from OH and NO<inline-formula><mml:math id="M42" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> chemistry,
along with the multistage chemistry often required for their formation,
results in the potential for complex dependencies on NO<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M44" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations. However, these NO<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> dependencies have not
previously been investigated. This work describes efforts to investigate the
sensitivity of daytime isoprene organonitrate chemistry to changes in
NO<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations through a series of steady-state models.
This work also aims to identify the role of O<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations in
daytime NO<inline-formula><mml:math id="M50" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> chemistry and determine the NO<inline-formula><mml:math id="M51" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations that facilitate this understudied reaction pathway. While the
data presented here solely focus on nitrated species resulting from isoprene, similar variations in organonitrate speciation under different NO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> regimes are likely to hold for any volatile organic compound (VOC) which can undergo oxidation by both OH and NO<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> radicals.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Experimental</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Model description</title>
      <p id="d1e678">The goal of this work is to investigate changes in NO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> on
the chemistry of isoprene nitrates in the afternoon period in Beijing. To do
this, the models should demonstrate the favoured reaction pathways under
different oxidant concentrations in the absence of other variables. This
means that physical and photolytic processes should be held constant, i.e.
the models will describe the chemistry occurring at a representative point
in the day. Species must also be allowed to reach their steady-state
concentrations in order to eliminate the role of the model spin-up period on
resultant species concentrations. Comparison of the concentrations of
species in these so-called steady-state models then allows for conclusions
to be drawn as to the preferred oxidation products under various conditions.</p>
      <p id="d1e699">All models described in this work were run using AtChem2, an open-source
zero-dimensional box model (Sommariva et al., 2020). All models
also made use of the isoprene mechanism published by Vereecken et al. (2021)
(henceforth the FZJ mechanism) which aimed to improve the representation of
NO<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> chemistry of isoprene by building on chemistry from the Master
Chemical Mechanism (MCM) and the review of isoprene chemistry published by
Wennberg  et al. (2018) (Jenkin et al., 2015; Wennberg et al., 2018; Vereecken et al., 2021; Carlsson et al., 2023). In order to make the species naming consistent between the MCM portion and the added chemistry of the FZJ mechanism, ISOPCNO3 was renamed to EISOP1N4OH as both identical species are present in the original FZJ mechanism.</p>
      <p id="d1e711">The steady-state models are sets of models run at a range of fixed NO<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
and O<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Models were run for NOx mixing ratios up to 45 ppb and O<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios of 140 ppb, corresponding to the upper limit of measurements made in the Beijing 2017 campaign (Shi et al., 2019). In order to provide additional OH reactivity, a constant concentration of
methane was added to all of the models to ensure that the modelled OH
reactivity matched measured values under Beijing-like conditions; this is
discussed further in the “Model Validation” section. The required mixing ratio corresponded to 82 ppm of methane in all of the models. The modelled
concentration of species is taken as the final<?pagebreak page8475?> concentration after 5 model
days, after all species had been allowed to reach steady-state concentrations. Each model was run at photolysis conditions corresponding to
those calculated by AtChem2 for 16:00 LT in Beijing, China. This was
around the time of peak daytime NO<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations in Beijing, before
concentrations rapidly increased during sunset. To ensure steady-state was
reached in a reasonable time, and to provide loss routes for species without
losses, species were removed from the model at a dilution rate of
<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.31</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">5</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> s<inline-formula><mml:math id="M64" 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>, corresponding to a dilution lifetime of
12 h. This value was selected based on a combination of the physical
loss processes included in previous modelling work, and the impact of this
decision is assessed in Sect. 3.1 (Mayhew et al., 2022; Edwards et al., 2014, 2013).</p>
      <p id="d1e781">All models were run at a temperature of 298.15 K, a pressure of 1013 mbar,
and a relative humidity of 50 %. The latitude, longitude, and date used
for photolysis calculations were 39.909<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, 116.398<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>,
and 1 June 2022. NO<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was constrained by adjusting the NO and NO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentrations at the beginning of each time step such that the total
NO<inline-formula><mml:math id="M69" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> matched the desired concentration, but the ratio of NO and NO<inline-formula><mml:math id="M70" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
remained constant.</p>
      <p id="d1e840">Models were also run to simulate conditions in the Amazon region, with VOC
concentrations adjusted to match observations of isoprene concentrations and
OH reactivity in this region. These models were run at a higher-isoprene
concentration of 5 ppb and methane concentrations of 100 ppm (Williams
et al., 2016; Pfannerstill et al., 2021; Langford et al., 2022). The latitude
and longitude values used corresponded to the city of Manaus and were
<inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3.132</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">60.01</mml:mn></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, respectively. The time of day was
kept at 16:00 LT.</p>
      <p id="d1e871">These models are designed for comparison between one another to gain insight
into the impact of changes in NO<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> on organonitrate
concentration. The models show the concentrations at steady state for the
provided photolysis conditions, chemistry, and dilution rate, which is in
contrast to the constantly changing photolysis and dilution encountered
under ambient conditions. This means that chemistry that would occur at
other times (e.g. nighttime chemistry) does not contribute to the results
of these models. Previous work has demonstrated not only the importance of nighttime chemistry for understanding organonitrates but also that many of the organonitrates produced overnight will decrease in concentrations over the early-morning period to reach low concentrations in the afternoon (Kenagy et al., 2020; Mayhew et al., 2022). The downstream chemistry of these nighttime organonitrates, and other nighttime species, will have some impacts on daytime chemistry that are not captured by the models presented here. However, Sect. 3.1 illustrates that the conclusions made in this paper are applicable to the Beijing afternoon conditions being investigated and that the conclusions are robust to changes in the modelling approach.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e894">The alkoxy-epoxidation pathway to form a range of nitrated
epoxides, as proposed by Vereecken et al. (2021). Additional isomers and
reaction pathways have been omitted for clarity.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f03.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Model isopleths</title>
      <p id="d1e911">Throughout this paper, the model results are investigated through the use of
isopleth plots. These plots consist of the steady-state concentration of a
species (or another model output such as OH reactivity) in each of the
models plotted as a coloured circle at the corresponding position on a set
of NO<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M77" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> axes. The colour scale is indicated by a colour bar
placed alongside each set of axes and will be a different scale for each
plot. A continuous colour gradient is then overlaid on the axes by
interpolation over a triangular grid of the model points. Ten contour lines
are also drawn over the top<?pagebreak page8476?> of each plot to highlight the contour shape.
These lines are equally spaced in the coloured dimension (e.g. species
concentration), meaning close vertical lines would correspond to a strong
sensitivity to changes in O<inline-formula><mml:math id="M78" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and close horizontal lines would
correspond to a strong sensitivity to changes in NO<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>.</p>
      <p id="d1e950">Under real-world conditions, the O<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations will be determined
by the nonlinear interactions of NO<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and VOCs, which is in contrast to
the models where NO<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, O<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and VOCs are all constrained. This means
that some sections of the model isopleths will be inaccessible. For example,
some amount of O<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> will form in the presence of NO<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and VOCs, so
occupying the upper-left corner of the isopleths may not be possible outside
of the constrained model scenario. Similarly, it may not be possible to map
real-world changes to one dimension (such as a decrease in NO<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> onto
the isopleth plots without accounting for a change in the other dimension
(such as a change in O<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>).</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Volatility calculations</title>
      <p id="d1e1037">Section 3.6 makes use of the vapour pressure (often expressed as a log value to the base of 10) to investigate the potential contributions to SOA. The UManSysProp facility was used to do this (Topping et al., 2016); UManSysProp can estimate the vapour pressure of compounds represented as SMILES strings via a range of different group contribution methods (Barley and Mcfiggans, 2010; O'Meara et al., 2014). This work used predictions at 298 K throughout and used the “evaporation” technique, though sensitivity to all of the available prediction methods is described in Sect. 3.6.</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>Model validation</title>
      <p id="d1e1056">As a test of the ability of the steady-state models to represent conditions
present under ambient scenarios, the model results were compared to
measurements collected in the summer of 2017 in Beijing (Shi et al.,
2019; Hamilton et al., 2021; Whalley et al., 2021; Reeves et al., 2021;
Newland et al., 2021; Mayhew et al., 2022). The NO<inline-formula><mml:math id="M88" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios
measured in the afternoon periods in Beijing ranged between 5 and 20 ppb, and O<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios ranged from around 60 to 140 ppb.
Isoprene mixing ratios ranged up to around 2 ppb in the afternoon period,
hence a typical value of 1 ppb was chosen for the steady-state models. The
concentration isopleths for inorganic species that were zoomed in to this
representative range of O<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios are provided in
the Supplement (Sect. S1).</p>
      <p id="d1e1095">Measurements of OH reactivity (<inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> during the afternoon period were between around 10 and 30 s<inline-formula><mml:math id="M93" 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> (Whalley et al., 2021),
which the models reproduced at the appropriate NO<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing
ratios by design due to the additional methane included in the model run for
this purpose (Fig. 4a). The modelled NO<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> reactivity (<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><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:msub></mml:mrow></mml:math></inline-formula>) is around 0.4–1.9 s<inline-formula><mml:math id="M98" 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> compared to the estimated value of around 0.5 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> presented in Hamilton et al. (2021) (Fig. 4b) (Hamilton et al., 2021). Values of <inline-formula><mml:math id="M100" 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:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><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:msub></mml:mrow></mml:math></inline-formula> at a
wider range of NO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios are provided in Fig. S1.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1238">Modelled steady-state <inline-formula><mml:math id="M104" 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:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:msub><mml:mi>k</mml:mi><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:msub></mml:mrow></mml:math></inline-formula> values at different NO<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further details on interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f04.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1295">Modelled steady-state mixing ratios of NO and NO<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at
different NO<inline-formula><mml:math id="M109" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further details on
interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f05.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1333">Modelled steady-state concentrations of NO<inline-formula><mml:math id="M111" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, OH, and HO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
at different NO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further details on
interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f06.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1380">Modelled steady-state concentrations of isoprene hydroxynitrate
(IHN)
, isoprene carbonylnitrate (ICN), and isoprene hydroperoxynitrate (IPN)
at different NO<inline-formula><mml:math id="M115" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M116" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further details on
interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f07.png"/>

        </fig>

      <?pagebreak page8477?><p id="d1e1407">In the NO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> space corresponding to typical Beijing afternoon
conditions, the models show NO mixing ratios of around 0.3–2.8 ppb
(Figs. 5a, S2a), consistent with the low-NO observations in the afternoon period in Beijing with observed mixing ratios of around 0.25 and 3 ppb (Newland et al., 2021). The models show NO<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios of 0.4 to 2 ppt (Figs. 6a, S3a), which are slightly below the measured NO<inline-formula><mml:math id="M120" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio in the afternoon of around 2 ppt (Hamilton et al., 2021). The modelled OH concentrations are between <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</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> and <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.5</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> molecules cm<inline-formula><mml:math id="M123" 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> (Figs. 6b, S3b), which are slightly below
the measured concentrations of around <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.5</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> molecules cm<inline-formula><mml:math id="M125" 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>. HO<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is generally overpredicted with a range between <inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.2</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M129" 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>, compared to measurements of around <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules cm<inline-formula><mml:math id="M131" 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> (Figs. 6c, S3c) (Whalley et
al., 2021). This is consistent with previous modelling studies that indicate
an overprediction of HO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by models, particularly under the low-NO
afternoon conditions being investigated here (Mayhew et al., 2022;
Whalley et al., 2021). Furthermore, models that included an additional sink
of HO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to bring it in line with measurements resulted in an
underprediction of OH due to the HO<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> removed from the system.</p>
      <p id="d1e1623">A series of sensitivity tests were carried out in order to assess the
sensitivity of our conclusions to changes in model parameters. Four
different parameters were adjusted: the concentration of isoprene, the
concentration of methane, the dilution rate, and the time of day. These
sensitivity tests were found to have little impact on the conclusions drawn
in this work, and any potential impacts are discussed where required.
Further details on tests are provided in the Supplement (Sect. S2).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1629">Modelled steady-state concentrations of isoprene
hydroxynitrooxyepoxide (INHE), isoprene carbonylnitrooxyepoxide (INCE), and
isoprene hydroperoxynitrooxyepoxide (INPE) at different NO<inline-formula><mml:math id="M135" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M136" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios. Further details on interpreting these plots are given in
Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f08.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Mononitrates</title>
      <p id="d1e1664">The IHN concentration isopleth (Fig. 7a) shows a strong similarity to the OH isopleth (Fig. 6b), highlighting its rapid formation from the OH oxidation of isoprene and subsequent RO<inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO reaction to form the nitrate group
(Fig. 1). This means that at high-O<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios, IHN shows a strong dependence on NO<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, and the dependence on O<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> becomes more significant at lower-O<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios.</p>
      <p id="d1e1715">IPN shows increasing concentrations with increasing O<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and decreasing
NO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (Fig. 7b). This reflects the requirement for low-NO concentrations to be present for two reasons. Firstly, high-NO<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations are required to form the INO<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> radical by the reaction of isoprene with NO<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. Secondly, the RO<inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> HO<inline-formula><mml:math id="M148" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> reaction is required to form the hydroperoxide group of IPN, and so lower-NO concentrations will reduce competition with the rapid RO<inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO reaction. Additionally, HO<inline-formula><mml:math id="M150" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations are highest under low-NO<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions (Fig. 6c), further favouring the RO<inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> HO<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> reaction.</p>
      <p id="d1e1837">In contrast to the other nitrated species investigated here, ICN shows two
peaks in concentration, one at very low O<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and the other at very high
O<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (Fig. 7c). This is because ICN can be formed from many different routes. These routes include the abstraction of an H atom from IHN which provides a formation route under lower-O<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions, when OH and IHN are both high in concentration. Alternatively, under higher-O<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions, ICN can form from the reaction of OH and IPN or the decomposition of nitrated alkoxy radicals (INO). The result of these multiple peaks is that under moderate NO<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions, the concentration of ICN is relatively insensitive to changes in both NO<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. It is also important to note that the absolute concentrations of ICN predicted to form in these models are very low (the peaks in concentration corresponding to mixing ratios of just over 1 ppt) due to low production rates, which is consistent with low daytime ICN mixing ratios previously identified in Beijing (Reeves et al., 2021; Mayhew et al., 2022).</p>
      <?pagebreak page8478?><p id="d1e1913">Recent work has highlighted species with the formula C<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>
as potentially major oxidation products of isoprene (Tsiligiannis et
al., 2022). Consistent with previous modelling studies (Mayhew et al., 2022), these models largely form C<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula> from OH-initiated oxidation, meaning the concentration isopleth is similar to that of OH and IHN.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Nitrated epoxides</title>
      <p id="d1e1979">Both INHE and INPE show a similar pattern as IPN in the NO<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
isopleths (Fig. 8a, b), with the highest concentrations occurring at low NO<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and very high O<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. INPE is reliant on high NO<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and HO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in a similar manner to IPN as the RO<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> HO<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> step is still required to form INPE. While HO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is not required to form INHE via the alkoxy-epoxidation pathway, the formation of INHE from IPN is the major formation route under lower-NO<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions. Additionally, the alkoxy-epoxidation pathway to the formation of INHE relies
on an RO<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>–RO<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> cross reaction. This cross reaction will be favoured
under low-NO<inline-formula><mml:math id="M180" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–high-O<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions, where NO concentrations will be
the lowest, meaning that the competition with the rapid RO<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>–NO reaction
is minimal. This requirement for very high O<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and low NO<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> means
that we should expect very low concentrations of daytime INHE and INPE under
typical urban conditions. This is consistent with modelling of Beijing which
showed that while INHE may comprise a large fraction of nighttime
C<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula> compounds, the daytime contribution is very small
(Mayhew et al., 2022).</p>
      <p id="d1e2168">In contrast, INCE shows reasonably high concentrations under high-O<inline-formula><mml:math id="M188" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios at a range of NO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios. The profile of these
concentrations is very similar to the NO<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> isopleth
(Fig. 6a) and stems from the main formation route to INCE requiring the NO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation of isoprene followed by an RO<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO reaction step. This formation route shares similarities with the dinitrates discussed in Sect. 3.4.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Dinitrates</title>
      <p id="d1e2227">As previously noted for INCE, Fig. 9 shows that
the steady-state concentrations of isoprene dinitrate (IDN) and isoprene
dinitrooxyepoxide (IDNE) are very similar to the NO<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentration
isopleth (Fig. 6a). This is indicative of the
formation route of IDN and IDNE, where an initial NO<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation is
followed by the reaction of the resulting RO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with NO to form the
second nitrate group (Figs. 1 and 3). At any daytime concentration of NO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> where sufficient NO<inline-formula><mml:math id="M197" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is present to perform the initial oxidation step, there will also be sufficient NO present to rapidly react with the resulting RO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Although the high-O<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios observed in Beijing result in low-NO concentrations compared to typical daytime concentrations in a polluted megacity, there is still ample NO present to react with peroxy radicals produced by the initial NO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation.
Figure 9 shows that at each O<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, there is a critical NO<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration above which the concentration of IDN, IDNE,
and INCE is almost exclusively controlled by O<inline-formula><mml:math id="M203" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations. This
critical NO<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratio is reasonably low compared to typical urban
NO<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> mixing ratios, indicating that the concentration of dinitrates in
urban environments may be largely controlled by the O<inline-formula><mml:math id="M206" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios
present.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e2360">Modelled steady-state concentrations of isoprene dinitrate (IDN)
and isoprene dinitrooxyepoxide (IDNE) at different NO<inline-formula><mml:math id="M207" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M208" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
mixing ratios. Further details on interpreting these plots are given in
Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f09.png"/>

        </fig>

      <p id="d1e2387">As discussed in Sect. S2, increasing the total VOC in the model leads to
a broadening in the NO<inline-formula><mml:math id="M209" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> axis of the transition between sensitive regimes of NO<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M211" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> for NO<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>; the same also applies to IDN,
IDNE, and INCE. For a fixed ozone concentration, increasing the NO<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
from 0 will increase IDN, IDNE, or INCE concentrations due to the increased
NO<inline-formula><mml:math id="M214" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> resulting from the increased availability of NO<inline-formula><mml:math id="M215" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
(Fig. 10). Then, once the threshold NO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration is reached and NO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations are not limited by the availability of NO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, the concentration becomes controlled by O<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and HO<inline-formula><mml:math id="M220" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2<?pagebreak page8479?></mml:mn></mml:msub></mml:math></inline-formula> (Sect. S2), creating the “hump” in concentration which then stabilises as HO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations begin to decrease at high NO<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
the <inline-formula><mml:math id="M223" 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:mo>/</mml:mo><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow></mml:math></inline-formula> ratio becomes increasingly controlled by the fixed O<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentration. This means that with high-VOC concentrations, at a given O<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentration, reductions in NO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> will result in increased IDN, IDNE, or ICNE concentrations sooner than under lower-VOC conditions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e2564">Modelled steady-state concentrations of IDN with changing
NO<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in models runs with 50 ppb of O<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and different mixing ratios
of NO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and additional methane.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f10.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS5">
  <label>3.5</label><title>Total organonitrates</title>
      <p id="d1e2609">By summing the model concentrations for all organonitrates present in the
mechanism, an isopleth of total organonitrates was obtained
(Fig. 11). This shows a band of high-organonitrate concentrations at moderate NO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. At high O<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, further
changes to O<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> have little effect on the total organonitrate
concentration. Total organonitrates also become less sensitive to changes in
NO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in this high-O<inline-formula><mml:math id="M234" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> region. This band is the result of
organonitrates produced by OH and NO<inline-formula><mml:math id="M235" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation of isoprene. At low-O<inline-formula><mml:math id="M236" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios, the total organonitrates are dominated by
OH-initiated species such as IHN (Fig. 7a).
Conversely, at high-O<inline-formula><mml:math id="M237" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios, NO<inline-formula><mml:math id="M238" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-initiated species such
as IDN comprise a larger fraction of total organonitrates
(Fig. 9a). This is illustrated in the pie charts
in Fig. 11 which show the organonitrate
composition under different NO<inline-formula><mml:math id="M239" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M240" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> regimes.</p>
      <p id="d1e2712"><?xmltex \hack{\newpage}?>The composition breakdown also reveals that total isoprene organonitrates
are dominated by IHN under most conditions, but this fraction decreases as
ozone mixing ratios increase. At higher O<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, a large fraction of the
composition comes from IDN, IDNE, and INCE due to their higher
concentrations under high-O<inline-formula><mml:math id="M242" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions (Sect. 3.3 and 3.4).
CH<inline-formula><mml:math id="M243" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M244" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula> comprises a substantial fraction of total organonitrates in these
models. CH<inline-formula><mml:math id="M245" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M246" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula> can be formed by the OH oxidation of methane via the
methylperoxy radical, and so its concentrations in these models are
exaggerated due to the large amounts of methane added to the model.
Formation from the OH oxidation of methane comprises the majority of all of
the methylperoxy formation in all of the models, excluding formation from
the reversible decomposition of methane peroxynitrate (CH<inline-formula><mml:math id="M247" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula>O<inline-formula><mml:math id="M248" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M249" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>) which is
balanced by the opposing formation reaction. CH<inline-formula><mml:math id="M250" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M251" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>OOH is also listed in
Fig. 11. CH<inline-formula><mml:math id="M252" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M253" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>OOH is formed from the products of
isoprene ozonolysis, explaining the higher concentrations under high-O<inline-formula><mml:math id="M254" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
conditions. There are no chemical losses in the mechanism for CH<inline-formula><mml:math id="M255" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>NO<inline-formula><mml:math id="M256" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula>OOH,
which likely explains the high contribution to total organonitrates. The
remaining portion of “other” organonitrates corresponds to a wide range of
species, none of which contribute more than 6 % to the total organonitrate
sum in any models.</p>
      <p id="d1e2836">As noted in Sect. S2, changing the VOC concentration affects the position
in NO<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M258" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> space where the maximum organonitrate concentrations are
observed. In the case of total organonitrates, decreasing the total VOC
concentration results in the band of high concentrations moving to lower
NO<inline-formula><mml:math id="M259" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Figures S7 and S8 show that with lower-methane
concentrations in the model, the peak organonitrate concentrations occur at
around 12 ppb of NO<inline-formula><mml:math id="M260" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> whereas this increases to around 25 ppb of
NO<inline-formula><mml:math id="M261" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the high-methane case. The peak organonitrate concentrations at
each of these NO<inline-formula><mml:math id="M262" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations are similar in each of these sets of
model runs.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e2897">Modelled steady-state concentrations of the total organonitrates
at different NO<inline-formula><mml:math id="M263" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M264" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios along with the composition
of the total organonitrates at selected NO<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M266" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios.
Further details on interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f11.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page8480?><sec id="Ch1.S3.SS6">
  <label>3.6</label><title>Volatility assessment</title>
      <p id="d1e2952">One of the major motivations for studying isoprene nitrates is their
potential to contribute to secondary organic aerosol (SOA) by condensation
or reactive uptake to existing particles. While the highest concentration
species such as IHN and IDN may be most significant when considering the
role of isoprene nitrates as NO<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> reservoirs, low-concentration species
can be much more important for SOA formation if they are of a sufficiently
low volatility. As an estimation of the impact of changing NO<inline-formula><mml:math id="M268" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
O<inline-formula><mml:math id="M269" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> on particle-phase processes, the log of the vapour pressure was
estimated for each organonitrate in the mechanism based on the species'
structure using UManSysProp (Topping et al., 2016). As a measure of a
compound's volatility, a lower vapour pressure value corresponds to a less
volatile compound which will more readily partition into existing particles.
This volatility-based approach does not account for potential reactive
uptake, which is likely to be important for the epoxide species previously
discussed. Furthermore, the hydrolysis of organonitrates, particularly
tertiary nitrates, may reduce particle-phase concentrations (Vasquez et
al., 2020). This particle-phase hydrolysis may then have knock-on effects for
the gas-phase organonitrates, particularly where the tertiary nitrate isomer
comprises a large fraction of the composition, such as for IHN.</p>
      <p id="d1e2982">Figure 12 shows the total organonitrate plot
normalised to the vapour pressure value for each compound, which gives an
estimation of the contribution of organonitrate uptake to SOA at each
NO<inline-formula><mml:math id="M270" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratio. Since the predicted vapour pressures
range over 10 orders of magnitude, lower-volatility species can have a large
effect on SOA formation despite their much lower concentration. The lowest
vapour pressures predicted here are for the two MCM species NC524NO<inline-formula><mml:math id="M272" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula> and
NC524OOH. These two compounds comprise almost 100 % of the normalised
concentration in Fig. 12 under all NO<inline-formula><mml:math id="M273" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
O<inline-formula><mml:math id="M274" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> conditions, and their individual concentration profiles can be seen
in Fig. 13. The concentration isopleths for the
15 lowest volatility compounds are shown in Fig. S17. Many of these
species show profiles similar to that of NC524OOH, with the highest
concentrations occurring at low urban NO<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e3040">Modelled steady-state concentrations of the total organonitrates
normalised to each compound's estimated vapour pressure at different
NO<inline-formula><mml:math id="M276" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further details on interpreting these
plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f12.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e3070">Modelled steady-state concentrations of the MCM species NC524NO3
and NC524OOH at different NO<inline-formula><mml:math id="M278" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M279" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios. Further
details on interpreting these plots are given in Sect. 2.2.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f13.png"/>

        </fig>

      <p id="d1e3097">According to Fig. 12, reductions in NO<inline-formula><mml:math id="M280" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> from
typical urban conditions would result in higher normalised concentrations of
organonitrates, meaning the contribution of isoprene nitrates to SOA may
increase with decreasing NO<inline-formula><mml:math id="M281" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> until very low urban NO<inline-formula><mml:math id="M282" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions
are met. However, it is important to note the difficulty in representing the
lowest-volatility species in the isoprene oxidation mechanism. Many of these
species are the product of multiple oxidation steps with large uncertainties
surrounding their rates of formation. Additionally, many of the lowest-volatility species do not contain any chemical losses in the mechanism due to a lack of information on their reactions.</p>
      <?pagebreak page8481?><p id="d1e3127"><?xmltex \hack{\newpage}?>The low predicted volatilities of NC524NO3 and NC524OOH are the result of
the many functional groups present in the molecules. Similarly, oxidised
species could be described as highly oxidised molecules (HOMs) (Bianchi et al., 2019). The chemistry of HOMs is not currently well represented in many mechanisms due to their varied autoxidation formation pathways. For example, the profile of NC524OOH concentrations in Fig. 13b results from the
requirement of HO<inline-formula><mml:math id="M283" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form the hydroperoxide group, hence the profile
is similar to that of HO<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. If an RO<inline-formula><mml:math id="M285" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> H-shift formation pathway to
NC524OOH, or similar HOMs, were included in the mechanism, then this might
alter the profile in Fig. 12 (Vereecken
and Nozière, 2020). It should be expected that the formation of HOMs
would be sensitive to changes in ozone as the lower-NO concentrations at
higher ozone will reduce the competition of the RO<inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO pathway with
the RO<inline-formula><mml:math id="M287" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> autoxidation reactions that form HOMs. Inclusion of improved
autoxidation chemistry in the mechanisms would also increase the number of
low-volatility compounds produced from the oxidation of isoprene. There is
also the potential for the oxidation products of nighttime species to be
low-volatility compounds that would contribute to SOA but would not be
captured by these models which represent the steady-state concentration of
organonitrates at 16:00 LT, without the contribution of chemistry occurring at other times of the day.</p>
      <p id="d1e3179">Figure S16 shows that the results presented here are reasonably insensitive
to the choice of vapour pressure and boiling point prediction methods
selected within UManSysProp. Section S3 also outlines the results using an
alternative volatility estimation method, making use of only the molecular
formula of each compound.</p>
</sec>
<sec id="Ch1.S3.SS7">
  <label>3.7</label><title>Application to less polluted environments</title>
      <p id="d1e3190">In order to test the investigation of less polluted environments, a series
of models were run at a range of lower-NO<inline-formula><mml:math id="M288" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and lower-O<inline-formula><mml:math id="M289" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios.
Measurements collected in the Amazon rainforest were taken as an example of
an unpolluted environment, and the model was adjusted to match typical
isoprene mixing ratios and OH reactivity observed in this environment. The
results from these models are presented in the supplementary information
(Sect. S5).</p>
      <p id="d1e3211">The reduced NO<inline-formula><mml:math id="M290" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M291" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> mixing ratios used in these models mean
that, despite the changes to isoprene and methane concentrations, they
correspond well to higher-resolution models of the low-NO<inline-formula><mml:math id="M292" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and low-O<inline-formula><mml:math id="M293" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> portions of the Beijing models. Figure S19 shows that the total
organonitrates in the Amazon models are sensitive to changes in NO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>,
with increasing ozone slightly reducing total organonitrates.</p>
      <p id="d1e3259">As discussed in the introduction, IEPOX is one of the major precursors of
isoprene SOA, particularly under low-NO<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions where the IEPOX
precursor, ISOPOOH, can form from oxidation by OH and further reaction with
HO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. This dependence on HO<inline-formula><mml:math id="M297" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> means that the Amazon models predict
increasing concentrations of IEPOX as NO<inline-formula><mml:math id="M298" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is increased from close to 0,
regardless of the O<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentration (Fig. 14b). This is in agreement with findings from Shrivastava et al. who found
increases in isoprene SOA resulting from increases in NO<inline-formula><mml:math id="M300" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
from an urban plume (Shrivastava et al., 2019). The increased SOA could be
further explained by the increases in nitrated epoxides and dinitrated
species predicted on increasing both NO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (Fig. S19).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e3347">Modelled steady-state IEPOX and MVK <inline-formula><mml:math id="M304" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> MACR concentrations for
the Beijing <bold>(a, c)</bold> and Amazon <bold>(b, d)</bold> models.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/8473/2023/acp-23-8473-2023-f14.png"/>

        </fig>

      <p id="d1e3369">Methyl vinyl ketone (MVK) and methacrolein (MACR) are also often of interest
in isoprene oxidation, particularly in pristine environments such as the
Amazon where the production of MVK and MACR relies on the presence of
NO (Langford et al., 2022). This is illustrated
in Fig. 14d, whereas
Fig. 14c illustrates that the abundance of NO
under typical urban conditions means that the MVK <inline-formula><mml:math id="M305" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> MACR concentrations in
the Beijing models are dependent on OH concentrations.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e3388">The work presented here illustrates that each isoprene nitrate species will
have a different NO<inline-formula><mml:math id="M306" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–O<inline-formula><mml:math id="M307" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> regime in which maximum concentrations
will be produced during the afternoon period. For example, the facile
formation of IHN from OH oxidation means that daytime concentrations are
largely dictated by the concentration of OH. Alternatively, the
concentrations of species such as IDN, IDNE, and ICN are largely dictated by
the available daytime NO<inline-formula><mml:math id="M308" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> as the reaction of RO<inline-formula><mml:math id="M309" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with NO is very
rapid, even under low urban NO<inline-formula><mml:math id="M310" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions. Finally, IPN, INHE, and
INPE only show the highest concentrations under low-NO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>–high-O<inline-formula><mml:math id="M312" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
conditions due to their increased formation under high-NO<inline-formula><mml:math id="M313" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
concentrations and their requirement for low NO<inline-formula><mml:math id="M314" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> to avoid competition
with the RO<inline-formula><mml:math id="M315" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> NO reaction pathway.</p>
      <p id="d1e3485">The fact that the concentrations of different organonitrates will respond
differently to changes in NO<inline-formula><mml:math id="M316" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and O<inline-formula><mml:math id="M317" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> will have implications for
those considering pathways to reducing the concentrations of organonitrates
in the atmosphere. The work presented here indicates that reductions in
NO<inline-formula><mml:math id="M318" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> may not reduce total organonitrate concentrations until low urban
NO<inline-formula><mml:math id="M319" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> conditions are met and that, for many of the species resulting from
the daytime NO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> oxidation of isoprene, organonitrate concentrations may
be much more sensitive to changes in O<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> than in NO<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Additionally,
accounting for the volatility of the organonitrates can have very large
impacts, and the models presented here are dominated by a small<?pagebreak page8482?> number of
low-volatility compounds. An improved representation of late-stage oxidation
and autoxidation is likely to improve the ability to predict the effect of
changing O<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M324" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> on SOA formation. It is important to note that
the simplified models presented here represent the formation of daytime
isoprene organonitrates at 16:00 LT and will not capture the effect of
organonitrates produced during the nighttime or those produced from the
oxidation of nighttime products or other VOCs.</p>
      <p id="d1e3570">As efforts are made to reduce NO<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, VOC, and O<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> concentrations
around the world, care should be taken to ensure that the nonlinearity of
responses to changes does not result in unintended increases in important
SOA precursors. For example, previous work has indicated that Beijing
occupies a VOC-limited regime with respect to O<inline-formula><mml:math id="M327" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> formation and that
decreasing NO<inline-formula><mml:math id="M328" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations without a concurrent decrease in VOC
concentrations would result in increased O<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> (Wei et al.,
2019; Ren et al., 2021). Figure 12 suggests that
many of the lowest-volatility daytime isoprene organonitrates may form in
higher concentrations under higher O<inline-formula><mml:math id="M330" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and lower NO<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Furthermore,
INHE, IDNE, INPE, and INCE all favour formation under high-O<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
conditions and may be subject to reactive uptake to the particle phase. This
may be further compounded or mitigated with changing VOC concentrations due
to the impact on the organonitrate isopleths as well as the nonlinear
behaviour of O<inline-formula><mml:math id="M333" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> with changing NO<inline-formula><mml:math id="M334" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and VOC.</p>
      <p id="d1e3664">Future chamber and field studies could validate the findings from this work
by making more comprehensive observations of total and speciated
organonitrates under different NO<inline-formula><mml:math id="M335" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, O<inline-formula><mml:math id="M336" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and VOC concentrations.
The comparative nature of these isopleth plots mean that the organonitrate
measurement would not necessarily need to be calibrated, provided that the
instrument response to specific organonitrates can be assumed to be
constant. This makes long-term measurements made with chemical ionisation
mass spectrometry (CIMS) a promising dataset as various CIMS techniques
using a range of reagent ions (including I<inline-formula><mml:math id="M337" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, Br<inline-formula><mml:math id="M338" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, and
CF<inline-formula><mml:math id="M339" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M340" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> have been shown to be very sensitive to these
multifunctional compounds, but calibration is often difficult (Mayhew et
al., 2022; Lee et al., 2014; Schwantes et al., 2019; Carlsson et al., 2023).</p>
</sec>

      
      </body>
    <back><notes notes-type="codeavailability"><title>Code availability</title>

      <p id="d1e3730">The AtChem2 software used for modeling is open source and freely available via <uri>https://github.com/AtChem</uri> (AtChem, 2023; <ext-link xlink:href="https://doi.org/10.5194/gmd-13-169-2020" ext-link-type="DOI">10.5194/gmd-13-169-2020</ext-link>, Sommariva et al., 2020).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e3742">No data sets were used in this article.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3745">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-23-8473-2023-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-23-8473-2023-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3754">AWM performed the model simulations and prepared the paper. PME and JFH provided supervision and advice throughout the project.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3760">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d1e3766">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3772">This project was undertaken on the Viking Cluster, which is a  high-performance compute facility provided by the University of York. We are
grateful for computational support from the University of York High Performance Computing service, Viking and the Research Computing team.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3777">This work has been supported by the Leeds–York–Hull Natural Environment Research Council (NERC) Doctoral Training Partnership (DTP) Panorama (grant no. NE/S007458/1).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3783">This paper was edited by Steven Brown and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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