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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-23-3083-2023</article-id><title-group><article-title>Impacts of estimated plume rise on PM<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance prediction during extreme wildfire events: a comparison of three schemes (Briggs, Freitas, and Sofiev)</article-title><alt-title>Impacts of estimated plume rise on PM<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance prediction during extreme wildfire events</alt-title>
      </title-group><?xmltex \runningtitle{Impacts of estimated plume rise on PM${}_{{2.5}}$ exceedance prediction during extreme wildfire events}?><?xmltex \runningauthor{Y.~Li et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Li</surname><given-names>Yunyao</given-names></name>
          <email>yli74@gmu.edu</email>
        <ext-link>https://orcid.org/0000-0002-3073-3227</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3">
          <name><surname>Tong</surname><given-names>Daniel</given-names></name>
          <email>qtong@gmu.edu</email>
        <ext-link>https://orcid.org/0000-0002-4255-4568</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Ma</surname><given-names>Siqi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Freitas</surname><given-names>Saulo R.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9879-646X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Ahmadov</surname><given-names>Ravan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Sofiev</surname><given-names>Mikhail</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9542-5746</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Zhang</surname><given-names>Xiaoyang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Kondragunta</surname><given-names>Shobha</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff10">
          <name><surname>Kahn</surname><given-names>Ralph</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5234-6359</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2 aff3">
          <name><surname>Tang</surname><given-names>Youhua</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7089-7915</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Baker</surname><given-names>Barry</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6431-2391</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Campbell</surname><given-names>Patrick</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0987-8402</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Saylor</surname><given-names>Rick</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Grell</surname><given-names>Georg</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Li</surname><given-names>Fangjun</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Atmospheric, Oceanic and Earth Sciences, George Mason University, Fairfax, VA 22030, USA</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Center for Spatial Information Science and Systems, George Mason
University, Fairfax, VA 22030, USA</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Air Resources Laboratory, National Oceanic and Atmospheric
Administration, College Park, MD 20740, USA</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Center for Weather Forecasting and Climate Studies, National Institute for Space Research, <?xmltex \hack{\break}?>São José dos Campos 12227, Brazil</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Cooperative Institute for Research in Environmental Sciences,
<?xmltex \hack{\break}?>University of Colorado at Boulder, Boulder, CO 80305, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Global Systems Laboratory, National Oceanic and Atmospheric
Administration, Boulder, CO 80305, USA</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Atmospheric Composition Research, Finnish Meteorological Institute,
Helsinki 00101, Finland</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Geospatial Sciences Center of Excellence, Department of Geography and Geospatial Sciences, <?xmltex \hack{\break}?>South Dakota State University, Brookings, SD 57007, USA</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Satellite Meteorology and Climatology Division, National Oceanic and Atmospheric Administration, <?xmltex \hack{\break}?>College Park, MD 20740, USA</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>Earth Sciences Division, National Aeronautics and Space Administration Goddard Space Flight Center, Greenbelt, MD 20771, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yunyao Li (yli74@gmu.edu) and Daniel Tong (qtong@gmu.edu)</corresp></author-notes><pub-date><day>9</day><month>March</month><year>2023</year></pub-date>
      
      <volume>23</volume>
      <issue>5</issue>
      <fpage>3083</fpage><lpage>3101</lpage>
      <history>
        <date date-type="received"><day>29</day><month>July</month><year>2022</year></date>
           <date date-type="rev-request"><day>16</day><month>August</month><year>2022</year></date>
           <date date-type="rev-recd"><day>14</day><month>February</month><year>2023</year></date>
           <date date-type="accepted"><day>14</day><month>February</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="d1e301">Plume height plays a vital role in wildfire smoke dispersion and the subsequent effects on air quality and human health. In this study, we assess the impact of different plume rise schemes on predicting the dispersion of wildfire air pollution and the exceedances of the National Ambient Air Quality Standards (NAAQS) for fine particulate matter (PM<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>) during the 2020 western United States wildfire season. Three widely used plume rise schemes (Briggs, 1969; Freitas et al., 2007; Sofiev et al., 2012) are compared within the Community Multiscale Air Quality (CMAQ) modeling framework. The plume heights simulated by these schemes are comparable to the aerosol height observed by the Multi-angle Imaging SpectroRadiometer (MISR) and Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO). The performance of the simulations with these schemes varies by fire case and weather conditions. On average, simulations with higher plume injection heights predict lower aerosol optical depth (AOD) and surface PM<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations near the source region but higher AOD and PM<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> in downwind regions due to the faster spread of the smoke plume once ejected. The 2-month mean AOD difference caused by different plume rise schemes is approximately 20 %–30 % near the source regions and 5 %–10 % in the downwind regions. Thick smoke blocks sunlight and suppresses photochemical reactions in areas with high AOD. The surface PM<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference reaches 70 % on the West Coast of the USA, and the difference is lower than 15 % in the downwind regions. Moreover, the plume injection height affects pollution exceedance (<inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) predictions. Higher plume heights generally produce larger downwind PM<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance areas. The PM<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance areas predicted by the three schemes largely overlap, suggesting that all schemes perform similarly during large wildfire events when the predicted concentrations are well above the exceedance threshold. At the edges of the smoke plumes, however, there are noticeable differences in the PM<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration and predicted PM<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance region. For the whole period of study, the difference in the total number of exceedance<?pagebreak page3084?> days could be as large as 20 d in northern California and 4 d in the downwind regions. This disagreement among the PM<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance forecasts may affect key decision-making regarding early warning of extreme air pollution episodes at local levels during large wildfire events.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e424">Wildfires release large amounts of aerosol and trace gases into the
atmosphere, which degrades the air quality and adversely affects human
health (Koning et al., 1985). Previous studies (Reid et al., 2016; Cascio,
2018) have demonstrated that a strong association exists between exposure to
wildfire smoke and all-cause mortality and respiratory morbidity. The global
average mortality attributable to landscape fire smoke exposure was
estimated at 339 000 deaths annually (Johnston et al., 2012). O'Neill et al. (2021) discuss the regional health impacts of the 2017 northern California wildfires and estimated 83 excess deaths from exposure to PM<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> (i.e., particles having aerodynamic diameter of less than 2.5 <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>), of which
47 % were attributable to wildfire smoke during the smoke episode. Liu et
al. (2021) assessed the health impact of the 2020 Washington State wildfire
smoke episode, which caused 38.4 more all-cause mortality cases and 15.1
more respiratory mortality cases. Aerosols emitted from wildfires also
affect the photolysis rates and photochemistry (Tang et al., 2003) and
ozone photochemical production (Val Martin et al., 2006; Akagi et al.,
2013). Wilmot et al. (2022) produced a decadal-scale wildfire plume rise
climatology for the USA West Coast and Canada and found trends toward enhanced plume heights and surface smoke injection to the free troposphere, which suggest a growing impact of wildfires on air quality and regional climate.</p>
      <p id="d1e446">Previous studies have found that the smoke injection height plays a vital
role in smoke dispersion, as wind speed and direction generally vary with
altitude (e.g., Mallia et al., 2018; Vernon et al., 2018). In addition, a
higher injection height will reduce near-source concentration, increase
downwind concentrations (Li et al., 2020), and can influence the removal
processes and atmospheric lifetime of emitted particles and trace gases. Briggs (1969) introduced a set of semi-empirical formulas to estimate plume
injection height for stack emissions from stationary power plant point
sources in different atmospheric stability states using buoyancy flux,
horizontal wind speed, static stability, and atmospheric turbulence
conditions. This scheme is widely used in dispersion models such as the
National Oceanic and Atmospheric Administration (NOAA) Hybrid
Single-Particle Lagrangian Integrated Trajectory model (HYSPLIT; Draxler and
Hess, 1998) and Community Multiscale Air Quality Modeling System (CMAQ; Byun
and Schere, 2006). However, the Briggs scheme was not designed for irregular-occurrence, large point source emissions, such as forest fires. Also, some of the input parameters, such as heat flux, are difficult to obtain. Freitas et al. (2007) developed a 1-D plume rise and transport parameterization for low-resolution atmospheric chemistry models, which was built upon governing equations, for the first law of thermodynamics, vertical motion, and continuity for the water phases. Sofiev et al. (2012) developed a new plume rise scheme, which utilizes the fire radiative power (FRP), planetary boundary layer (PBL) height, and the Brunt–Vaisala frequency in the free troposphere to estimate the plume injection height from wildfires. The parameters of the new scheme were determined using the plume height observations collected by the Multi-angle Imaging SpectroRadiometer (MISR) Plume Height Project (Kahn et al., 2008; Mazzoni et al., 2007) in North America (Val Martin et al., 2010) and Siberia. The plume height estimation in models is of great uncertainty. Sessions et al. (2011) tested the Freitas et al. (2007) plume rise scheme with Weather Research and Forecasting model coupled with Chemistry (WRF-Chem) and found that differences in injection heights produce different transport pathways. Roy et al. (2017) compared the simulated plume heights from two different approaches, namely Western Regional Air Partnership's (WRAP) plume model and the Freitas et al. (2007) plume model. Results show that the Freitas et al. (2007) plume model had a
better diurnal variation in the plume rise height. Mallia et al. (2018)
tested different ways to distribute the fire emissions vertically for
prescribed fires. Results indicated that plume height plays a critical role
in determining how smoke distributes downwind of the fire. Ye et al. (2021)
compared the calculated plume heights from 12 state-of-the-art air quality
forecasting systems during the Williams Flats fire in Washington State, USA,
in August 2019, during the Fire Influence on Regional to Global Environments
and Air Quality (FIREX-AQ) field campaign. They found that there was a large
spread of the modeled plume heights.</p>
      <p id="d1e449">In the summer and early autumn of 2020, the western United States (USA)
experienced a record-breaking wildfire season. A series of large wildfires
fueled by accumulated biomass, heat waves, and dry winds burned more than
<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:mn mathvariant="normal">10</mml:mn><mml:mspace width="0.25em" linebreak="nobreak"/><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> acres (National Interagency Fire Center, 2020). From late August to early October 2020, the West Coast wildfires contributed 23 % of surface PM<inline-formula><mml:math id="M17" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> pollution nationwide and caused 3720 observed PM<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedances (daily PM<inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, based on
National Ambient Air Quality Standards – NAAQS; Li et al., 2021). The thick fire smoke<?pagebreak page3085?> that originated in California, Oregon, and Washington was injected
into the free troposphere and transported across the country by the prevailing wind, which caused hazy days (indicated by the  high-aerosol-optical-depth (AOD) region) in 19 states (Fig. 1).</p>
      <p id="d1e519">This study aims to evaluate the impact of different plume rise schemes on
aerosol distribution and photochemistry during the 2020 record-breaking
wildfire season. We use the George Mason University (GMU) wildfire forecast
system (Li et al., 2021) that relies on satellite estimates of biomass
burning emissions and CMAQ to simulate the emission, transport, and
transformation of smoke during the 2020 summer wildfire season. Three plume
rise schemes are used, namely Briggs (1969), Freitas et al. (2007), and Sofiev et al. (2012). The Briggs (1969) scheme was implemented in the standard release of the CMAQ version. Li et al. (2021) implemented the Sofiev et al. (2012) scheme into CMAQ, and in this work, the Freitas et al. (2007) scheme is also implemented. The plume injection height's impact on PM<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> vertical distribution is evaluated in Sect. 3.2. Its impact on AOD and photochemistry is discussed in Sect. 3.3. Finally, we discussed plume rise impact on surface pollution level and PM<inline-formula><mml:math id="M22" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance in Sect. 3.4.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e543">Observations of wildfire smoke on 15 September 2020, over
the continental United States by the Visible Infrared Imaging Radiometer
Suite (VIIRS) aboard the Suomi National Polar-orbiting Partnership (Suomi NPP) satellite. <bold>(a)</bold> True-color image and <bold>(b)</bold> 550 nm aerosol optical depth (AOD).</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f01.jpg"/>

      </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Experiment design</title>
      <p id="d1e575">Biomass burning is an important source of global aerosols that has a great
impact on air quality. Figure 2 shows how wildfire smoke affects local and
downwind air quality (Koppmann et al., 2005; Seinfeld and Pandis, 2016;
Schlosser et al., 2017). Wildfire emissions include primary aerosols (direct
emission) and large amounts of gases that can be oxidized to form secondary
aerosols (generated after emission). In the biomass burning input of our
model, the major components of the primary aerosols are organic carbon,
non-carbon organic matter, elemental carbon, chloride, and potassium. The
other wildfire emissions like SO<inline-formula><mml:math id="M23" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (NO <inline-formula><mml:math id="M25" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), NH<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and volatile organic compounds (VOCs) may form secondary aerosols such as sulfate, nitrate, ammonium, and secondary organic aerosols (SOAs) after being emitted. The temporal and spatial impacts of plume rise on different primary or secondary aerosol species may be different, as the generation of the secondary aerosols usually takes time. The difference in the dispersion of primary and secondary aerosols will contribute to further differences in photochemistry and health impacts. Therefore, it is important to discuss the impact of plume rise on each primary and secondary aerosol species.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e623">Wildfire primary emissions and downwind evolution. Note that the percentage for primary aerosols is from the CMAQ biomass burning input file. The percentage for the secondary aerosols is not real; it is just for illustration purposes. Moreover, the CMAQ model separates organic carbon (OC) and non-carbon elements (O, H, etc.) in organic matter (OM).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f02.png"/>

        </fig>

      <p id="d1e632">To evaluate the impact of different plume rise schemes on aerosol dispersion
and photochemistry modeling during the 2020 record-breaking wildfire season, four CMAQ simulations were conducted. In the first run (B69), we used the CMAQ default plume rise scheme based on Briggs (1969). In the second run (F07), we implemented the Freitas et al. (2007) scheme into the CMAQ model and used it to calculate the plume injection height. In the third run (S12), we used the Sofiev et al. (2012) plume rise scheme, as implemented in Li et al. (2021). In the fourth run (NoFire), we turned off all types of biomass burning emissions. The wildfire impact is represented by the difference between the simulation with fire and the NoFire run. More information on the
three plume rise schemes is provided in Sect. 2.3. Besides the difference
in the plume rise scheme, the setups for these three runs are the same. More
details about the CMAQ setup are given in Sect. 2.2. Comparing results from these three simulations elucidates the impacts of plume injection height predictions on the distribution of each aerosol species (Sect. 3.2), AOD, and photochemistry (Sect. 3.3), as well as surface air quality and PM<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedances (Sect. 3.4).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Description of the model system</title>
      <p id="d1e652">The George Mason University (GMU) air quality modeling system was employed
to simulate the 2020 summer wildfire season from 1 August to 30 September 2020 over the contiguous United States (CONUS) domain. This system uses CMAQ version 5.3.1 (United States Environmental<?pagebreak page3086?> Protection Agency, 2020a) as the chemical transport model and the Weather Research and Forecasting (WRF; Skamarock et al., 2019) model (Version 4.2 output) as the meteorology inputs for the CMAQ model. The model domain is configured with 12 km by 12 km horizontal resolution and 35 vertical layers (the same horizontal and vertical resolution as NOAA's operational National Air Quality Forecasting Capability). The initial and boundary conditions for WRF are from the Global Data Assimilation System
(GDAS) 0.25<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> analysis and forecast. The main physics choices were the
Grell–Freitas scheme (Grell and Freitas, 2014) for parameterized cumulus
processes, the Mellor–Yamada–Janjic scheme (Janjic, 1994) for planetary
boundary layer (PBL) processes, the two-moment Morrison microphysics
(Morrison et al., 2009) for cloud physics processes, the rapid radiative transfer model for general circulation models (RRTMG) scheme (Iacono et al., 2008) for longwave and shortwave radiation, and the Noah scheme (Koren et al., 1999) for land surface processes. The biomass burning emissions product used in this study is the 0.1<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> daily blended Global Biomass Burning Emissions Product (GBBEPx) from the Moderate Resolution Imaging Spectroradiometer (MODIS) and Visible Infrared Imaging Radiometer Suite (VIIRS; GBBEPx V3; Zhang et al., 2012, 2019). The GBBEPx fire radiative power (FRP) in the GBBEPx is averaged from observations from MODIS on Terra and Aqua MODIS and VIIRS M band on the Suomi National Polar-orbiting Partnership (SNPP) and the Joint Polar Satellite System-1 (JPSS) VIIRS. A climatological diurnal cycle from the Western Regional Air Partnership (WRAP) work was applied to the daily GBBEPx emission to derive hourly model-ready emission input. Anthropogenic emissions were prepared with the 2016v1 emissions modeling platform, using the baseline emissions taken from the National Emissions Inventory (NEI) 2016 collaboration (Eyth et al., 2021). We then shifted the base year emission to the prediction year 2020 using representative days of each month. The model-ready emission files are processed and generated by the Sparse Matrix Operator Kernel Emissions (SMOKE) model (Baek and Seppanen, 2019) V4.7. The carbon bond 6 (CB6) gas-phase chemical mechanism (Luecken et al., 2019), CMAQ aerosol module 7 (AE07) aerosol scheme (Pye et al., 2015; Xu et al., 2018), and aqueous chemistry (Fahey et al., 2017) are used in the CMAQ system. Details about the system setup are shown in Table S1 of Li et al. (2021).</p>
      <p id="d1e673">The evaluation of the model performance with the Sofiev et al. (2012) plume rise scheme has been discussed by Li et al. (2021). The average correlation
between observed (from AirNow) and simulated daily PM<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations
is 0.55. The averaged normalized mean error in the simulated surface
PM<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> is 3.9 % for the year 2020. The average area hit ratio for
exceedances is 0.68 (Fig. 2a in Li et al., 2021). A high area hit ratio
represents a good capture of the region impacted by smoke. During the peak
pollution days (from 12 to 16 September), the area hit ratios were higher than 0.96, with a maximum of 1.0 on 13 September 2020. This suggests that the model could predict more than 96 % of the observed exceedances when the smoke pollution was at its peak. Also, the simulated PM<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> vertical profiles along the West Coast and in central USA matched the vertical profiles of backscatter from Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations (CALIPSO) near the wildfire source region<?pagebreak page3087?> and downwind area (Fig. S2 in Li et al., 2021). Overall, the model can reproduce wildfire smoke dispersion, especially when the smoke is thick.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Description of the plume rise schemes</title>
      <p id="d1e711">Three plume rise schemes are used in this study, namely Briggs (1969), Freitas et al. (2007), and Sofiev et al. (2012).</p>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Briggs scheme (B69)</title>
      <p id="d1e721">The default plume rise scheme in CMAQ is based on Briggs (1969) and has been
modified by revisions in Briggs (1971, 1972, 1984). It uses a set of semi-empirical formulas to estimate plume injection height (<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) in different atmospheric stability states (i.e., neutral, stable, and
unstable). Heat flux (<inline-formula><mml:math id="M35" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula>), horizontal wind speed (<inline-formula><mml:math id="M36" display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula>), static stability (<inline-formula><mml:math id="M37" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>), and friction velocity (<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:msup><mml:mi>x</mml:mi><mml:mo>∗</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) are used to estimate the plume injection height as follows:
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M39" display="block"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced close="" open="["><mml:mtable class="array" columnalign="left"><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">1.33</mml:mn><mml:mo>×</mml:mo><mml:mi>B</mml:mi><mml:msup><mml:mi>U</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mi>x</mml:mi><mml:mrow><mml:mo>∗</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo><mml:mtext> neutral</mml:mtext></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">2.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi>B</mml:mi><mml:msup><mml:mi>U</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mi>S</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mfenced><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>,</mml:mo><mml:mtext> stable</mml:mtext></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd><mml:mrow><mml:mn mathvariant="normal">30</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mfenced close=")" open="("><mml:mrow><mml:mi>B</mml:mi><mml:msup><mml:mi>U</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mfenced><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">3</mml:mn><mml:mn mathvariant="normal">5</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>,</mml:mo><mml:mtext> unstable</mml:mtext></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mfenced><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            Previous studies found that FRP is about 10 %–20 % of the total fire heat (Wooster et al., 2005; Freeborn et al., 2008). In this study, we derive the heat flux from FRP provided by the GBBEPx dataset multiplied by a factor of 10, following Val Martin et al. (2012). The Briggs (1969) scheme is widely used in chemical transport models; however, it was not designed for forest fires.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><title>Freitas et al. (2007) scheme (F06)</title>
      <p id="d1e893">Freitas et al. (2007) developed a 1-D plume rise and transport parameterization for low-resolution atmospheric chemistry models, which was
built upon governing equations for the first law of thermodynamics, vertical
motion, and continuity for the water phases (Eqs. 1–5 in Freitas et al., 2007). It takes in fire information, including fire area and heat flux, in addition to atmospheric profile information, including temperature, moisture,
density, and wind velocity. The plume-top height is defined as the altitude
at which the plume is neutrally buoyant and is approximated as a vertical
velocity <inline-formula><mml:math id="M40" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 1 m s<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. The Freitas et al. (2007) scheme is the default plume rise scheme in WRF-Chem and has been widely used in many studies (e.g., Sessions et al., 2011; Val Martin et al., 2012; Roy et al., 2017; Mallia et al., 2018). However, the Freitas et al. (2007) scheme has never before been used with CMAQ. In this work, the FRP-based Freitas et al. (2007) scheme from High-Resolution Rapid Refresh coupled with Smoke (HRRR–Smoke; Ahmadov et al., 2017) model has been implemented into CMAQ. Wind, temperature, pressure, and humidity from WRFV4.2 meteorology inputs, as well as FRP and fire burning area, are used to calculate the plume injection height in the model. The FRP from GBBEPx and fire size from RAP–Chem (Rapid Refresh with Chemistry; Archer-Nicholls et al., 2015) are used to calculate fire buoyancy in the model.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>Sofiev et al. (2012) scheme (S12)</title>
      <p id="d1e923">Sofiev et al. (2012) developed a new plume rise scheme that considers
wildfire plumes in a way similar to convective available potential energy
(CAPE) computations. It utilizes FRP, PBL height (<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">PBL</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and the Brunt–Vaisala frequency in the free troposphere (BV<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">FT</mml:mi></mml:msub></mml:math></inline-formula>) to estimate the plume injection height from wildfires as follows:
              <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M44" display="block"><mml:mrow><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:msub><mml:mi>H</mml:mi><mml:mi mathvariant="normal">PBL</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="italic">β</mml:mi><mml:msup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mtext>FRP</mml:mtext><mml:mrow><mml:msub><mml:mtext>FRP</mml:mtext><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mi mathvariant="italic">γ</mml:mi></mml:msup><mml:mi mathvariant="normal">exp</mml:mi><mml:mfenced close=")" open="("><mml:mrow><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msubsup><mml:mtext>BV</mml:mtext><mml:mi mathvariant="normal">FT</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow><mml:mrow><mml:msubsup><mml:mtext>BV</mml:mtext><mml:mn mathvariant="normal">0</mml:mn><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where FRP<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:math></inline-formula> is the reference fire radiative power, which equals 10<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> W, BV<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:math></inline-formula> is the reference Brunt–Vaisala frequency, which equals
<inline-formula><mml:math id="M48" 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:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> s<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and <inline-formula><mml:math id="M50" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M51" display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M52" display="inline"><mml:mi mathvariant="italic">γ</mml:mi></mml:math></inline-formula>,
<inline-formula><mml:math id="M53" display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula> are constants. In our previous study, we added the Sofiev et al. (2012) scheme to CMAQ (Li et al., 2021) and applied it to predict air quality during the 2020 wildfire season with the same constants found in Sofiev et al. (2012).</p>
      <p id="d1e1099">After obtaining the estimated plume injection height from the three schemes,
the fire emissions were distributed between 0.5–1.5 times the plume injection height (default setting in CMAQ). The three schemes used in the current experiment are very different in their nature and underlying assumptions, but they all were developed with an individual fire as a model source of buoyancy and smoke. In this experiment, and in many other applications of these schemes, the input fire information is gridded with a
grid cell size of several kilometers or larger. Strictly speaking, such a setup goes beyond the area of applicability of these schemes. However, with a growing number of gridded fire emission products and their applications for
atmospheric composition and air quality tasks, it is important to evaluate
this very setup – and to compare the robustness of these models to the violation of their underlying assumptions. In this study, we use the default
coefficient settings in each scheme. We did not tune the coefficient of any
scheme to obtain the best simulation for any major fire case. The main focus of this study is to evaluate the impact of different plume injection heights on the near-source and downwind air quality, and the 2-month average state is
more important to our results and future health studies.</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Observation data</title>
<sec id="Ch1.S2.SS4.SSS1">
  <label>2.4.1</label><title>MISR and CALIPSO plume height observation</title>
      <p id="d1e1118">The predicted plume height is evaluated using observations from Multi-angle
Imaging SpectroRadiometer (MISR) and Cloud-Aerosol Lidar and Infrared
Pathfinder Satellite Observations (CALIPSO). The MISR instrument obtains
imagery<?pagebreak page3088?> of each location within its 380 km wide swath at nine viewing angles, ranging from 70<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> forward, through the nadir, to 70<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> aft, along the orbit track, in each of four spectral bands centered at 446
(blue), 558 (green), 672 (red), and 866 nm (near-infrared) wavelengths
(Diner et al., 1998). MISR is in a sun-synchronous orbit, crossing the
Equator at approximately 10:30 local time (LT), so observations in the study
region occurred in the mid-to-late morning, The MISR INteractive eXplorer
(MINX) software is used in this study to derive plume heights from MISR
imagery (Nelson et al., 2013; Val Martin et al., 2018). The MINX
wind-corrected plume height information is then used to evaluate the
simulated plume height in this paper.</p>
      <p id="d1e1139">CALIPSO is an Earth science observation mission that was launched on 28 April 2006 and flies in a nominal orbital altitude of 705 km and an
inclination of 98<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, as part of a constellation of Earth-observing
satellites. CALIPSO's lidar instrument, the Cloud-Aerosol Lidar with
Orthogonal Polarization (CALIOP), provides high-resolution vertical profiles
of aerosol and cloud-attenuated-backscatter signals at 532 and 1064 nm
(Winker et al., 2007). The footprint of the lidar beam has a 100 m
cross section, with an overpass around 13:30 LT. The CALIPSO smoke injection heights are directly calculated from level 1 attenuated-backscatter profiles at 532 nm, following Amiridis et al. (2010). There are several steps involved in this process. First, GBBEPx FRP data were used to locate the fire location along the CALIPSO swath. Then, a slope method (Pal et al., 1992) is applied to each profile to smooth out the original level 1 532 nm attenuated-backscatter-coefficient profiles at each fire point. Next, we calculate the steep gradient in the attenuated-backscatter profiles. The
height of the minimum gradient value is selected as the smoke injection
height.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <label>2.4.2</label><?xmltex \opttitle{AirNow surface PM${}_{{2.5}}$ data}?><title>AirNow surface PM<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> data</title>
      <p id="d1e1169">The hourly ground PM<inline-formula><mml:math id="M58" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> observations from the U.S. EPA AirNow network
are used to evaluate the surface air pollution predictions in this study. The real-time AirNow measurements are collected by the state, local, or tribal environmental agencies either using federal references or equivalent monitoring methods approved by EPA. The measurements contain air quality data for more than 500 cities across the USA, Canada, and Mexico.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS3">
  <label>2.4.3</label><title>VIIRS AOD data</title>
      <p id="d1e1189">The simulated AOD results are compared to the VIIRS Enterprise AOD from
SNPP (Zhang et al., 2016; Laszlo and Liu, 2022). The VIIRS
Enterprise Aerosol Algorithm retrieves AOD at the 750 m pixel level for the
nominal wavelength of 550 nm, using radiances from 11 VIIRS channels (412,
445, 488, 555, 672, 746, 865, 1240, 1378, 1610, and 2250 nm). The AOD is
calculated separately for land and ocean, using a lookup table of precomputed values for several atmospheric parameters to simplify radiative transfer calculations.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Comparing simulated plume heights against MISR and CALIPSO
observations</title>
      <p id="d1e1209">The simulated plume heights from three simulations, i.e., B69, F07, and S12, are compared with MISR observations for the Milepost 21 fire on 15 August 2020 and the August Complex fire on 31 August 2020 (Fig. 3) at the MISR local overpass time of around 19:00 UTC. The smoke heights from the model 3-D fields were interpolated to the MISR observation pixels using the nearest-neighbor approach. The performance of different schemes varies by fire cases and weather conditions. For the Milepost 21 fire, the plume heights simulated by B69 and S12 are similar but 25 % and 3 % lower than that by F07 for the easterly and westerly plume. In the case of the August Complex fire northerly plume, the plume heights simulated by S12 are 4 % and 8 % higher than that by B69 and F07, respectively. For the southerly plume, the plume heights simulated by B69 are 16 % and 5 % higher than that by F07 and S12. The simulated PBL heights are displayed in Fig. 3 as a reference. When the fire injection height is lower than the PBL height, then the pollution could become confined to the PBL (Sofiev et al., 2012; Thapa et al., 2022). However, when the plume height is higher than PBL, then the fire smoke can be dispersed into the free troposphere where wind speeds are stronger, leading to a wider range of pollution dispersion. In all four cases analyzed in Fig. 3, the simulated plume heights from the three schemes surpassed the model PBL. Previous studies found that, for large fires that are injected above the PBL, the plume height calculated by S12 is less sensitive to FRP than that calculated by B69 (Li et al., 2020). Some of the fire points during the August Complex fire had higher FRP than that during the Milepost 21 fire, so the estimated plume height by B69 is higher than that by S12. For the F07 scheme, the plume injection height is higher when it is wetter (Freitas et al., 2007). The water vapor mixing ratio on 15 August is higher than on
31 August, which contributes to the higher plume height during the Milepost
21 fire than during the August Complex fire. According to the box-and-whisker chart shown in the right panel of Fig. 3, the simulated plume heights are all within the range of MISR observation. Overall, the simulated plume heights with all three schemes are reasonably comparable to the MISR observations.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e1214">MISR plume heights superposed on the MODIS Terra visible images <bold>(a–d)</bold> and the comparisons of the observed plume height with the simulated plume heights <bold>(e–h)</bold> for the 15 August Milepost 21 fire easterly plume <bold>(a, e)</bold> and westerly plume <bold>(b, f)</bold> and the 31 August Complex fire northerly plume <bold>(c, g)</bold> and southerly plume <bold>(d, h)</bold>. Source: MISR Active Aerosol Plume-Height (AAP) Project, with Ralph A. Kahn, Katherine J. Noyes, James Limbacher (NASA Goddard Space Flight Center), Abigail Nastan (JPL-Caltech), Jason Tackett, and Jean-Paul Vernier (NASA Langley Research Center).</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f03.jpg"/>

        </fig>

      <p id="d1e1242">The vertical profiles of CMAQ-simulated PM<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> are also compared to the
CALIPSO daytime aerosol vertical profile. The daytime CALIPSO overpass
occurs around 13:30 LT, closer to the peak fire behavior in the afternoon than the MISR observations. Figure 4 shows the comparison between the CALIPSO plume height results and the estimated plume heights from the three plume rise schemes for West Coast fires. The mean bias for the three schemes is <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.60</mml:mn></mml:mrow></mml:math></inline-formula> for B69, <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">0.67</mml:mn></mml:mrow></mml:math></inline-formula> for F07, and 0.13 for S12. In most cases, the plume<?pagebreak page3089?> heights from the three schemes are close to each other, especially for the cases with plume tops under 4 km. For strong fires with plume tops higher than 4 km, S12 seems to be more skillful than B69 and F07. It successfully simulates the high plume top observed by CALIPSO, whereas B69 and F07 tend to underestimate the plume heights.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e1277">Comparisons of plume-top heights from three simulations, namely B69 (blue rectangle), F07 (orange dot), and S12 (red triangle), against
aerosol height observations from the CALIPSO for West Coast fires.</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f04.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><?xmltex \opttitle{Impact of estimated plume rise on PM${}_{{2.5}}$ vertical distribution}?><title>Impact of estimated plume rise on PM<inline-formula><mml:math id="M62" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> vertical distribution</title>
      <?pagebreak page3090?><p id="d1e1304">In this section, we investigate the impact of plume injection height on
different PM<inline-formula><mml:math id="M63" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> chemical components. Figure 5 shows the vertical
profile of the 2-month average PM<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration for the three
experiments. Over 2 months, B69 simulated a higher average plume height and injected more PM<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> in the free troposphere than F07 and S12. Meanwhile, F07 simulated a lower average plume height and therefore kept more PM<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> in the boundary layer than B69 and S12.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1345">Vertical profile of 2-month average PM<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration
for B69, F07, and S12 in the CONUS domain.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f05.png"/>

        </fig>

      <p id="d1e1363">Figure 6 shows the distribution of simulated PM<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> components from both
direct emissions and secondary formation (the impact of other PM<inline-formula><mml:math id="M69" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
sources was removed by subtracting the results of NoFire run) from B69, F07,
and S12 in three different regions, namely western USA (west of  120<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), central USA (between 120 and 100<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W), and eastern USA (between 100 and 80<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W). For all three schemes, organic matter (OM) dominates the chemical composition of PM<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>, with 63 %–64 % near the source region in western USA, and remains dominant in the downwind regions at <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">61</mml:mn></mml:mrow></mml:math></inline-formula> %, between 120 and 100<inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W, and 57 %, between 100 and 80<inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W. A high-OM portion highlights the predominant effect of wildfire emissions on air quality during the gigafire period (Li et al., 2021). The second most abundant component is nitrate (NO<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>), with 11 %–12 % near the source region and 13 %–16 % in the downwind region. A higher portion of NO<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> in the downwind region than in the source region reflects the decreased contribution of primary aerosols and increases in secondary aerosols. The other component with a similar spatial gradient is ammonium (NH<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>), which contributes 3 % to PM<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> near the source region and 5 %–6 % in the downwind region. Elemental carbon contributes 10 % to PM<inline-formula><mml:math id="M81" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration near the source region and 8 %–9 % in the downwind region. Potassium (K), a fingerprint element
to indicate fire contribution, accounts for 3 % of PM<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> near the
source region and 2 %–3 % in the downwind region. Sulfate (SO<inline-formula><mml:math id="M83" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>) contributed 3 % near the source region and 6 %–8 % in the downwind region. In summary, PM<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species that are not significantly affected by secondary aerosol formation, such as elemental carbon and potassium, see a decrease in their contributions when transported downwind. For the PM<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species that are affected by secondary aerosol formation (e.g., nitrate, sulfate, and ammonium), the contribution increases when transported downwind. These results show that the PM<inline-formula><mml:math id="M86" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> composition, integrated over all vertical layers, is not sensitive to the choice of plume rise scheme.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1544">The simulated PM<inline-formula><mml:math id="M87" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> chemical components (%) with the B69, F07, and S12 plume rise schemes in three different regions, i.e., to the west of 120<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W <bold>(a, d, g)</bold>, between 120 and  100<inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W <bold>(b, e, h)</bold>, and between 100 and  80<inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W <bold>(c, f, i)</bold>. The data are integrated over all vertical layers and averaged during the analysis period. The top six components are labeled in each plot.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f06.png"/>

        </fig>

      <p id="d1e1599">Figure 7 shows the difference in the zonal mean (average for each latitude)
concentrations of six major PM<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species (i.e., organic matter,
nitrate, elemental carbon, ammonium, potassium, and sulfate) and total
PM<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> when using different plume rise schemes over the whole domain.
Overall, most of the differences are found over the West Coast region (to
the west of 115<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W). The simulation with B69 produces a higher plume height on average, resulting in greater transport of smoke aloft, and hence higher downwind PM<inline-formula><mml:math id="M94" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> than that with the F07 or S12 schemes. The B69 plume rise scheme has a higher downwind impact and slightly lower near-source impact for PM<inline-formula><mml:math id="M95" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species that contain secondary aerosols (e.g., organic matter, nitrate, ammonium, and sulfate) than primary aerosols (e.g., elemental carbon and potassium), due to the time required to form secondary aerosols.</p>
      <?pagebreak page3091?><p id="d1e1647">Among the three simulations, the largest differences in PM<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> are found from the surface to 8 km over the source region. Over the downwind region, the bulk of PM<inline-formula><mml:math id="M97" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> differences is found in the middle and upper troposphere. In addition, we noticed that the simulations with F07 and S12 produce more PM<inline-formula><mml:math id="M98" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> than that with B69 between 6–8 km during the analysis period. This is because, in the cases of a strong fire, the plume injection height simulated by F07 or S12 could be higher than B69 (e.g., Fig. 3e). However, the difference in PM<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> above 6 km is very small compared to those particles below 6 km. The total PM<inline-formula><mml:math id="M100" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference caused by different plume rise schemes is about 30 % near the source and 5 % in the downwind region. The difference in surface PM<inline-formula><mml:math id="M101" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> has a large impact on surface pollution levels and human health. More discussion on the impact of plume height on surface air quality is presented in Sect. 3.4. Although the upper-level PM<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference is expected to have a smaller impact on human health, it may affect cloud formation, photochemical reactions, and the radiative budget in the Earth system.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1716"><bold>(a–n)</bold> Zonal mean difference in predicted concentrations of
six major PM<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species among the simulations using the B69, F07, and S12 schemes from 1 August to 30 September 2020 for organic matter <bold>(a, b)</bold>, nitrate <bold>(c, d)</bold>, elemental carbon <bold>(e, f)</bold>, ammonium <bold>(g, h)</bold>, potassium <bold>(i, j)</bold>, and sulfate <bold>(k, l)</bold>. The difference in total PM<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> is displayed by both the absolute values <bold>(m, n)</bold> and percentage <bold>(o, p)</bold>.</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f07.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Impact of estimated plume rise on aerosol optical depth and
photochemistry</title>
      <?pagebreak page3093?><p id="d1e1778">Wildfire smoke increases the aerosol loading in the atmosphere and consequently the AOD over both the source region and downwind regions. According to our previous study (Li et al., 2021), from 14–17 September 2020 smoke from the West Coast was transported to the northeastern part of the USA. The downwind transport of wildfire smoke is highly dependent on plume rise estimation. Figure 8a shows the 2-month-averaged AOD from VIIRS compared with model simulations (Fig. 7b–d). The CMAQ-predicted AOD was interpolated to the VIIRS pixels that passed quality control using the nearest-neighbor approach. When comparing the CMAQ AOD to VIIRS AOD (Fig. 7b–d), we applied VIIRS AOD saturation level (AOD <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>) to CMAQ AOD results (any CMAQ AOD values higher than 5 were changed to 5). In the West Coast high-peak region, all three runs capture the observed AOD high peak near the San Francisco region, but the simulated AOD peak is lower than VIIRS observed. The average AOD from VIIRS observation is higher than 2. However, among the three CMAQ runs, only F07 simulated an average AOD higher than 2. In the downwind region, all three CMAQ runs reproduce the general downwind transport pattern, but the simulated smoke-affected region (AOD <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula>) is smaller than the observations.</p>
      <p id="d1e1801">Figure 7e–h show the AOD differences and the difference ratio (percentage
of the difference relative to B69) between the different plume rise scheme
simulations. When comparing different model simulations, the AOD saturation
level is removed. Near the source region, F07 and S12 simulate more AOD than
B69, a pattern that is the opposite of that for plume rise estimation (lower
plume height than that with B69). In the downwind region, B69 simulates more
AOD than F07 and S12. The difference is approximately 20 %–30 % over the source region and 5 %–10 % over the downwind region. One possible reason that B69 predicts lower AOD near the source region and higher AOD in the downwind region compared to F07 and S12 is that a higher plume height will inject more aerosol into the free troposphere where the wind speed is stronger, accelerating the dispersion of the fire pollution. Therefore, the higher plume height will lead to lower AOD near the source region but higher AOD in the downwind region. The result is consistent with previous studies (Mallia et al., 2018; Vernon et al., 2018; Li et al., 2020).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1806">The 2-month average AOD from VIIRS <bold>(a)</bold>, B69 run <bold>(b)</bold>, F07 run <bold>(c)</bold>, and S12 run <bold>(d)</bold> from 1 August to 30 September 2020. The average AOD differences between F07 and B69 <bold>(e)</bold> and between S12 and B69 <bold>(f)</bold> during the same period as in panel <bold>(a)</bold>. The average AOD difference ratio between F07 and B69 <bold>(g)</bold> and between S12 and B69 <bold>(h)</bold> during the same
period as in panel <bold>(a)</bold>.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f08.jpg"/>

        </fig>

      <p id="d1e1847">The difference in the dispersion of fire pollution caused by the various
estimated plume injection heights leads to further differences in the
chemistry and photolysis reactions. Previous studies found that the thicker
smoke, indicated by higher AOD, may absorb and/or scatter a larger fraction
of sunlight, hence affecting photolysis reactions (Dickerson et al., 1997;
Castro et al., 2001; Kumar et al., 2014; Baylon et al., 2018). Here, we
simply examine how the plume rise differences affects photochemistry by
comparing the photolysis rate of NO<inline-formula><mml:math id="M107" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (NO<inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi>v</mml:mi><mml:mo>→</mml:mo></mml:mrow></mml:math></inline-formula> NO <inline-formula><mml:math id="M109" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> O)
from the three runs, which is a key reaction that leads to the formation of
tropospheric ozone. The differences in the NO<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> photolysis rate
(NO2_IUPAC10; in min<inline-formula><mml:math id="M111" 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>) are shown in Fig. 9. Figure 9a and d show the photolysis rate difference and difference ratio between B69 and the NoFire experiments. The photolysis rate results in B69 were lower than the NoFire simulation, which proves that fire smoke led to the reduction in the photolysis rate, consistent with the findings of previous studies. The photolysis rate reduction caused by the fire smoke was found in the whole domain, both in the near-source region and the downwind region. Near the fire source, the photolysis rate reduction was more than 50 %. Figure 9b, c, e, and f show the photolysis rate difference and difference ratio between the three experiments with different plume rise schemes. Near the source region, where F07 and S12 simulate a higher AOD than B69 (Fig. 8), the NO2_IUPAC10 is reduced. Meanwhile, in the downwind region, where F07 and S12 simulate a lower AOD, the photolysis rate is higher than B69. Therefore, the difference in the plume injection height would affect the fire-induced photolysis rate reduction.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e1907">The average photolysis rate NO2_IUPAC10 differences between B69 and NoFire <bold>(a)</bold>, between F07 and B69 <bold>(b)</bold>, and
between S12 and B69 <bold>(c)</bold> from 1 August to 30 September 2020. The average photolysis rate NO2_IUPAC10 difference ratio between B69 and NoFire <bold>(d)</bold>, between F07 and B69 <bold>(e)</bold>, and between S12 and B69 <bold>(f)</bold> during the same period.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f09.jpg"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><?xmltex \opttitle{Impact of estimated plume rise on surface PM${}_{{2.5}}$ and exceedance of NAAQS}?><title>Impact of estimated plume rise on surface PM<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> and exceedance of NAAQS</title>
      <p id="d1e1953">Surface or ambient PM<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> is the common measure used to link exposure to
wildfire smoke to health endpoints such as asthma and chronic obstructive
pulmonary disease (Reid et al., 2016). To protect human health and the
environment, the National Ambient Air Quality Standards (NAAQS) have been
established for PM<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> and other criteria air pollutants (NO<inline-formula><mml:math id="M115" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, 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>, SO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, PM<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>, and lead). The daily PM<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> NAAQS level is 35 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> for the 24 h mean PM<inline-formula><mml:math id="M121" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentration (United States Environmental Protection Agency, 2020b). The simulated surface PM<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> differences caused by different plume rise schemes are shown in Fig. 10. The F07 and S12 simulations, which have averaged lower initial plume heights, yield higher surface PM<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations than the B69 simulation over the West Coast, whereas the opposite patterns are found in the central and the eastern USA. The surface PM<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference caused by different plume rise schemes reaches 70 % over the West Coast, which is much higher than the AOD differences. In the downwind regions, the surface PM<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference caused by different plume rise schemes is less than 15 %, meaning that the effects of the plume rise estimation on surface PM<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> occur mainly near the source region.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e2096">Simulated and observed surface PM<inline-formula><mml:math id="M127" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> from 1 August to 30 September 2020. <bold>(a)</bold> Average surface PM<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> simulated with B69 overlaid by AirNow observations. <bold>(b)</bold> Difference in averaged surface PM<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> between F07 and B69. <bold>(c)</bold> Difference between S12 and B69. Panels <bold>(d)</bold> and <bold>(e)</bold> are the same as panels <bold>(b)</bold> and <bold>(c)</bold> but for the differences in percentage (%) between F07 and B69 and between S12 and B69, respectively.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f10.jpg"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e2157">Predicted surface PM<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations above unhealthy levels by the S12, F07, and B69 runs for 20 August 2020. <bold>(a)</bold> The daily mean surface PM<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference between F07 and B69 runs. <bold>(b)</bold> Simulated PM<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance regions by B69, F07, and S12  overlaid by AirNow observed exceedance (PM<inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). Panel <bold>(c)</bold> is the same as panel <bold>(b)</bold> but for U.S. EPA-defined unhealthy regions (PM<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). Panel <bold>(d)</bold> is the same as panel <bold>(b)</bold> but for U.S. EPA-defined very unhealthy regions (PM<inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">150</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M138" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). The brown color represents the region where the runs with all three schemes simulate PM<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedances. The blue (red/yellow) color represents the region where only B69 (S12 or F07) simulates the PM<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance. The green color represents the region where both the B69 and F07 simulate the PM<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance. The magenta color represents the region where both the B69 and S12 simulate the PM<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance. The orange color represents the region where both F07 and S12 simulate the PM<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance.</p></caption>
          <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f11.jpg"/>

        </fig>

      <?pagebreak page3096?><p id="d1e2358">Next, we examine how the plume rise estimation affects the prediction of
PM<inline-formula><mml:math id="M144" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedances. Figure 11a shows the daily mean surface PM<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
difference between the F07 and B69 runs for 20 August 2020 (the first
fire peak during the study period). The simulated PM<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance
regions (PM<inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">35</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, as defined by NAAQS, and at same level as U.S. EPA-defined unhealthy regions for sensitive groups), unhealthy regions (PM<inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, as defined by U.S. EPA), and very unhealthy regions (PM<inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">150</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M152" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, as defined by U.S. EPA) as seen by different plume rise schemes overlaid by the AirNow-observed exceedance for the same day are shown in Fig. 10b, c, and d. According to Fig. 11b and c, on 20 August 2020, B69 and S12 simulated more PM<inline-formula><mml:math id="M153" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance and a larger unhealthy region in the downwind regions (Wyoming (WY) and Idaho (ID); magenta and blue region), whereas F07 and S12 simulated more exceedance and a larger unhealthy region in the southeastern USA (yellow and orange region), where prescribed fires were the major biomass burning sources. In WY and ID, where F07 did not simulate the PM<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance, whereas B69 and S12 did, the difference between F07 and B69 reached 15 <inline-formula><mml:math id="M155" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (Fig. 11a). Furthermore, B69 and S12 simulate some very unhealthy regions in Nevada, whereas F07 simulates more very unhealthy regions in central and southern California. Although these schemes agree on the PM<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance forecast in the majority of the region, the disagreements in the downwind areas (i.e., ID and WY for this case) may affect key decision-making on early warnings of extreme air pollution episodes at local levels during large wildfire events.</p>
      <p id="d1e2535">The total number of predicted exceedance days from the B69 simulation and
the differences between B69, F07, and S12 are shown in Fig. 12. All the
states on the West Coast and in the mountain region experienced at least 1 d
of PM<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance (Fig. 12a). Most of the region in northern California experienced more than 20 exceedance days, with a maximum of more
than 35 d. F07 and S12 simulate more exceedance days on the West Coast
near the source region and in the southeast. The difference in the exceedance days could be as large as 20 d in northern California. B69 simulates more exceedance days in downwind regions such as Nevada, Idaho, Montana, and Wyoming. The difference could reach 4 d in the downwind regions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e2549">The CMAQ B69-predicted total number of PM<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance days during August–September 2020 <bold>(a)</bold>. The difference in the number of predicted exceedance days between B69 and F07 <bold>(b)</bold> and between B69 and S12 <bold>(c)</bold>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/3083/2023/acp-23-3083-2023-f12.jpg"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusion</title>
      <p id="d1e2585">In this study, we use CMAQ with three different plume rise schemes, namely
Briggs (1969; B69), Freitas et al. (2007; F07), and Sofiev et al. (2012; S12), to understand the impact of plume rise calculation on aerosol and photochemistry during the 2020 western USA wildfire season. The plume heights simulated by all three schemes are comparable to MISR and CALIPSO observations of aerosol height. The<?pagebreak page3097?> performance of the simulations with different schemes varies for different fire cases and weather conditions (i.e., humidity). On average, the B69 predicts higher injection heights than F07 and S12, leading to higher downwind PM<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations due to the stronger transport at the higher altitude. The largest PM<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> differences are found from the surface to 8 km over the source region. Over the downwind region, the bulk of the PM<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> differences is found in the middle and upper troposphere. The total PM<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference is approximately 30 % near the source and 5 % in the downwind region. Furthermore, we found that the plume rise scheme has a higher downwind impact and slightly lower near-source impact for PM<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> species that contain more secondary aerosols than primary aerosols.</p>
      <p id="d1e2633">Thick fire smoke also increases AOD in the source and the downwind regions. On average, F07 and S12, which estimate lower plume height, simulate greater smoke AOD near the fire source region than B69. In the downwind region, B69 simulates higher AOD than F07 and S12. The difference is approximately 20 %–30 % near the source region and 5 %–10 % in the downwind region. When AOD is higher, the thicker smoke may block more sunlight and affect the photolysis reaction rates. Near the source region, where F07 and S12 simulate a higher AOD, the photolysis reaction rate decreases.</p>
      <p id="d1e2636">Finally, we analyzed the effect of plume rise estimation on the prediction of PM<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedances. The F07 and S12 simulations, which have lower averaged plume heights, predict higher surface PM<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> concentrations than B69 over the West Coast, whereas the opposite patterns are found in the central and the eastern USA. The effects of the plume rise estimation on surface PM<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> occur mainly near the source region. The surface PM<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> difference caused by different plume rise schemes reaches 70 %
over the West Coast and is less than 15 % in the downwind regions. These
results suggest that the effects of plume rise estimation on surface
PM<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> occur mainly near the source region, whereas in the downwind
region, the majority of effects are in the free troposphere. For the PM<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance prediction, higher plume height produces a larger PM<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance area in the downwind region. In most affected areas, the predicted PM<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance regions from the three schemes overlapped. In non-overlapping regions, the simulated differences in PM<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> could reach 15 <inline-formula><mml:math id="M173" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. For the whole period of study, the difference in the total number of exceedance days could be as large as 20 d in northern California and 4 d in the downwind regions. F07 and S12 simulated more exceedance days near the fire source region, while B69 simulates more exceedance days in downwind regions such as Nevada, Idaho, Montana, and Wyoming. Such PM<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> exceedance forecast differences may affect key decision-making on early warnings of extreme air pollution episodes at local levels during large wildfire events.</p>
      <p id="d1e2749">The WRF-CMAQ system used in this study is an offline model. The heat emitted
by the fire calculated in the CMAQ does not influence the meteorology model
(WRF), such as the PBL height, temperature, and wind field. In the future,
online models will be utilized to further study the plume rise estimation
impacts on air quality.</p>
</sec>

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

      <p id="d1e2757">CMAQ documentation and released versions of the source code are available on the U.S. EPA modeling site <ext-link xlink:href="https://doi.org/10.5281/zenodo.3585898" ext-link-type="DOI">10.5281/zenodo.3585898</ext-link> (United States Environmental Protection Agency, 2020a). The WRF V4.2 model code is distributed by National Center for Atmospheric Research: <uri>https://github.com/wrf-model/WRF</uri> (National Center for Atmospheric Research, 2020).</p>
  </notes><notes notes-type="dataavailability"><title>Data availability</title>

      <p id="d1e2769">The MISR, GBBEPx, VIIRS, and AirNow data used in this paper can be found at <ext-link xlink:href="https://doi.org/10.5281/zenodo.7702951" ext-link-type="DOI">10.5281/zenodo.7702951</ext-link> (Li et al., 2023).</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2778">YL and DT designed the study and performed the research, with contributions from all co-authors. SRF, RA, MS, and GG prepared the plume rise code. SM, XZ, SK, and FL prepared fire emission data. RK prepared the MISR data and guided the evaluation of plume height estimation. YL and DT wrote and revised the paper, with input from YT, BB, and PC. All authors commented on drafts of the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2784">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="d1e2790">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e2796">This article is part of the special issue “The role of fire in the Earth system: understanding interactions with the land, atmosphere, and society (ESD/ACP/BG/GMD/NHESS inter-journal SI)”. It is a result of the EGU General Assembly 2020, 4–8 May 2020.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2802">This work has been financially supported by the NASA Health and Air Quality
Program, NOAA Weather Program Office, and George Mason University College of
Science. The observation data from NASA, NOAA, and U.S. EPA are gratefully
acknowledged.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2807">This research has been supported by the Earth Sciences Division (NASA Health and Air Quality Program) and the NOAA Research, NOAA Weather Program Office (NOAA Weather Program Office).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2813">This paper was edited by Yuan Wang and reviewed by three anonymous referees.</p>
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