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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-23-5815-2023</article-id><title-group><article-title>A new insight into the vertical differences in NO<inline-formula><mml:math id="M1" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous
reaction to produce HONO over<?xmltex \hack{\break}?> inland and marginal seas</article-title><alt-title>NO<inline-formula><mml:math id="M2" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction to produce HONO over inland and marginal seas</alt-title>
      </title-group><?xmltex \runningtitle{NO${}_{{2}}$ heterogeneous reaction to produce HONO over inland and marginal seas}?><?xmltex \runningauthor{C. Xing et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Xing</surname><given-names>Chengzhi</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0265-2358</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Xu</surname><given-names>Shiqi</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Song</surname><given-names>Yuhang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8687-7919</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff2 aff1 aff3 aff4">
          <name><surname>Liu</surname><given-names>Cheng</given-names></name>
          <email>chliu81@ustc.edu.cn</email>
        <ext-link>https://orcid.org/0000-0002-3759-9219</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Liu</surname><given-names>Yuhan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff5">
          <name><surname>Lu</surname><given-names>Keding</given-names></name>
          <email>k.lu@pku.edu.cn</email>
        <ext-link>https://orcid.org/0000-0001-9425-9520</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Tan</surname><given-names>Wei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zhang</surname><given-names>Chengxin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2092-9135</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Hu</surname><given-names>Qihou</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Wang</surname><given-names>Shanshan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Wu</surname><given-names>Hongyu</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8">
          <name><surname>Lin</surname><given-names>Hua</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Lab of Environmental Optics and Technology, Anhui
Institute of Optics and Fine Mechanics,<?xmltex \hack{\break}?> Hefei Institutes of Physical Science, Chinese Academy of Sciences, Hefei 230031, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Precision Machinery and Instrumentation, University of Science and<?xmltex \hack{\break}?> Technology of China, Hefei 230026, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Center for Excellence in Regional Atmospheric Environment, Institute of Urban Environment,<?xmltex \hack{\break}?> Chinese Academy of Sciences, Xiamen 361021, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Key Laboratory of Precision Scientific Instrumentation of Anhui
Higher Education Institutes,<?xmltex \hack{\break}?> University of Science and Technology of China, Hefei 230026, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>State Key Joint Laboratory of Environment Simulation and Pollution
Control, College of Environmental Sciences and Engineering, Peking
University, Beijing 100871, China</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of unclear safety, China Institute of Atomic Energy,
Beijing 102413, China</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>School of Earth and Space Sciences, University of Science and
Technology of China, Hefei 230026, China</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>School of Environmental Science and Optoelectronic Technology, University of Science and<?xmltex \hack{\break}?> Technology of China, Hefei 230026, China</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>Shanghai Key Laboratory of Atmospheric Particle Pollution and
Prevention (LAP³), Department of Environmental Science and Engineering,
Fudan University, Shanghai 200433, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Cheng Liu (chliu81@ustc.edu.cn) and Keding Lu
(k.lu@pku.edu.cn)</corresp></author-notes><pub-date><day>26</day><month>May</month><year>2023</year></pub-date>
      
      <volume>23</volume>
      <issue>10</issue>
      <fpage>5815</fpage><lpage>5834</lpage>
      <history>
        <date date-type="received"><day>9</day><month>September</month><year>2022</year></date>
           <date date-type="rev-request"><day>1</day><month>November</month><year>2022</year></date>
           <date date-type="rev-recd"><day>25</day><month>January</month><year>2023</year></date>
           <date date-type="accepted"><day>3</day><month>May</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>

      <?pagebreak page5816?><p id="d1e270">Ship-based multi-axis differential optical absorption spectroscopy (MAX-DOAS) measurements were conducted along the marginal seas of China from 19 April to 16 May 2018 to measure the vertical profiles of aerosol, nitrogen dioxide (NO<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), and nitrous acid (HONO). Along the cruise route, we found five hot spots with enhanced tropospheric NO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> vertical column densities (VCDs) in the Yangtze River Delta, Taiwan Strait, Guangzhou–Hong Kong–Macau Greater Bay Area, port of Zhanjiang, and port of Qingdao. Enhanced HONO concentrations could
usually be observed under high-level aerosol and NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> conditions,
whereas the reverse was not always the case. To understand the impacts of
relative humidity (RH), temperature, and aerosol on the heterogeneous
reaction of NO<inline-formula><mml:math id="M6" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form HONO in different scenarios, the Chinese Academy
of Meteorological Sciences (CAMS) and Southern University of Science and
Technology (SUST) MAX-DOAS stations were selected as the inland and coastal
cases, respectively. The RH turning points in CAMS and SUST cases were both
<inline-formula><mml:math id="M7" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 65 % (60 %–70 %), whereas two turning peaks
(<inline-formula><mml:math id="M8" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 60 % and <inline-formula><mml:math id="M9" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 85 %) of RH were found in the
sea cases. As temperature increased, the HONO <inline-formula><mml:math id="M10" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio decreased with peak values appearing at <inline-formula><mml:math id="M12" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12.5<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in CAMS, whereas the HONO <inline-formula><mml:math id="M14" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gradually increased and reached peak values at <inline-formula><mml:math id="M16" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 31.5<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in SUST. In the sea cases, when the temperature exceeded 18.0<inline-formula><mml:math id="M18" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, the HONO <inline-formula><mml:math id="M19" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio rose with increasing temperature and
achieved its peak at <inline-formula><mml:math id="M21" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25.0<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. This indicated that
high temperature can contribute to the secondary formation of HONO in the
sea atmosphere. In the inland cases, the correlation analysis between HONO
and aerosol in the near-surface layer showed that the ground surface is more crucial to the formation of HONO via the heterogeneous reaction of NO<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>; however, in the coastal and sea cases, the aerosol surface contributed more. Furthermore, we discovered that the conversion rate of NO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to HONO through heterogeneous reactions in the sea cases is larger than that in the inland cases in higher atmospheric layers (<inline-formula><mml:math id="M25" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 600 m). Three typical events were selected to demonstrate three potential contributing factors of
HONO production under marine conditions (i.e., transport, 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>
heterogeneous reaction, and unknown HONO source). This study elucidates the
sea–land and vertical differences in the forming mechanism of HONO via the
NO<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction and provides deep insights into tropospheric HONO distribution, transforming process, and environmental effects.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>National Natural Science Foundation of China</funding-source>
<award-id>42207113</award-id>
<award-id>41941011</award-id>
<award-id>51778596</award-id>
<award-id>41575021</award-id>
<award-id>41977184</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Natural Science Foundation of Anhui Province</funding-source>
<award-id>2108085QD180</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Hefei Institutes of Physical Science, Chinese Academy of Sciences</funding-source>
<award-id>YZJJ2021QN06</award-id>
</award-group>
<award-group id="gs4">
<funding-source>Chinese Academy of Sciences</funding-source>
<award-id>XDA23020301</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e491">Nitrous acid (HONO) is an important part of the atmospheric nitrogen cycle
and plays a significant role in atmospheric oxidation capacity (Alicke et
al., 2003; Kleffmann et al., 2005). Photolysis of HONO in near-ultraviolet
bands (Reaction R1) is a substantial source of hydroxyl radicals (OH radicals),
which are one of the most important oxidants in the tropospheric atmosphere.
Earlier studies reported that the contribution of HONO photolysis to OH
radicals can reach 40 %–60 %, while exceeding 80 % in the early morning
(Michoud et al., 2012; Ryan et al., 2018; Xue et al., 2020). OH radicals can
oxidize and destroy most atmospheric pollutants, such as CO, NO<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
(NO <inline-formula><mml:math id="M29" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M30" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), SO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and volatile organic compounds (VOCs), thereby
further promoting the formation of secondary pollutants (e.g., ozone
(O<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>), peroxyacetyl nitrate (PAN), and secondary aerosols) and leading
to serious haze pollution events (Huang et al., 2014). Additionally, as a
nitrosating agent, HONO can produce carcinogenic nitrite amines that pose a
threat to human health (Zhang et al., 2015). Therefore, a full understanding
of the source and formation mechanism of HONO is scientifically significant
for the study of tropospheric oxidation and the control of secondary
pollution.</p>
      <p id="d1e537">Currently, the known sources of HONO mainly include direct emissions from
vehicles, ships, biomass burning, and soil; the homogeneous reaction of NO
and OH radicals (Reaction R2); the nighttime and daytime heterogeneous reaction of NO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Reaction R3) on aerosols, vegetation, the ground, and other types of surfaces; and the photolysis of nitrate particles (Reaction R4) (Alicke et al., 2003; Stemmler et al., 2006; Indarto, 2012; Wang et al., 2015; Salgado
and Rossi, 2002; Zhou et al., 2011). Sources of HONO exist that are poorly
understood (Fu et al., 2019). The heterogeneous reaction of NO<inline-formula><mml:math id="M34" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> as a
source of HONO has received continuous attention in recent years. It was
found that the heterogeneous reaction of NO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is one of the most
important sources of HONO in a variety of scenes such as inland, coastal
cities, and offshore seas. Liu et al. (2021) reported the contribution of the
heterogeneous reaction of NO<inline-formula><mml:math id="M36" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the aerosol surface to HONO is 19.2 % in summer, and this contribution on aerosol and ground surfaces to HONO can
reach 54.6 % in winter in Beijing. Yang et al. (2021) and Zha et al. (2014) found that the generation rate of HONO through the heterogeneous
reaction of NO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> under sea-wind conditions could elevate 3–4 times more than
that under land-wind conditions in the northern coastal city of Qingdao and
the southern coastal city of Hong Kong, respectively. Cui et al. (2019)
illustrated that the heterogeneous reaction of NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on aerosol and sea
surfaces is an important source of HONO in the East China Sea in summer. The
process of HONO formed from the heterogeneous reaction of NO<inline-formula><mml:math id="M39" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is
affected by various atmospheric parameters. The relative humidity (RH),
temperature, solar radiation intensity (SRI), and aerosol concentration and
its relative surface area are the particularly important parameters. Earlier
works always used the linear regression relationship between HONO <inline-formula><mml:math id="M40" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and the above parameters to characterize the influence of these parameters
on the formation of HONO through the heterogeneous reaction of NO<inline-formula><mml:math id="M42" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.
Although this kind of simple linear regression method may lead to artificial
correlations and misleading conclusions, considering the vertical evolution
of atmospheric parameters. Wen et al. (2019) found that the increased
temperature could promote the heterogeneous reaction of NO<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form
HONO in sea conditions. The generation rate of HONO could increase rapidly,
when the temperature was greater than 20 <inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. Gil et al. (2019)
found that the HONO formed from the heterogeneous reaction of NO<inline-formula><mml:math id="M45" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> will
increase along with the increase in RH when RH was less than 80 % in a
case of a land park using deep learning forced by measurement results. Fu et
al. (2019) reported that RH and SRI were the main parameters driving the
heterogeneous reaction of NO<inline-formula><mml:math id="M46" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form HONO in the Pearl River Delta, and it
contributes 72 % of the total source of HONO. Cui et al. (2019) found
that the potential of the heterogeneous reaction of NO<inline-formula><mml:math id="M47" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form HONO will
increase with the increase in particle concentration and the specific
surface area of single particles in coastal cities.


              <disp-formula specific-use="gather" content-type="numbered reaction"><mml:math id="M48" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R1"><mml:mtd><mml:mtext>R1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi>v</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">400</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R2"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R3"><mml:mtd><mml:mtext>R3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R4"><mml:mtd><mml:mtext>R4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mtable class="split" rowspacing="0.2ex" displaystyle="true" columnalign="right left"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi>v</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow><mml:mo>/</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:mrow></mml:mtd></mml:mtr><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mspace linebreak="nobreak" width="1em"/><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">300</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mtr></mml:mtable></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          However, earlier research generally focused on the near-surface layer of a
single scene, and attention to the influence mechanism of the heterogeneous
reaction of NO<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form HONO in the vertical direction and in different sea
and land scenes is insufficient, which limits the comprehensive<?pagebreak page5817?> assessment
to understand the sea–land differences and impact mechanism of HONO formed
from the heterogeneous reaction of NO<inline-formula><mml:math id="M50" 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="M51" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> could be transported
from inland and coastal cities to offshore seas (Tan et al., 2018). This
part of NO<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can promote the HONO formation through heterogeneous
reactions on the high-level aerosol and sea surfaces in the sea atmosphere
(Zhang et al., 2020). The formed HONO is likely to be carried to land cities
at night by the sea breeze, which will affect the atmospheric oxidation and air
quality and even endanger human health. Additionally, the vertical
distributions and values of atmospheric meteorology and aerosol parameters
are significantly different in land and sea scenes, which provide different
conditions for the heterogeneous reaction of NO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to form HONO in
different height layers. Furthermore, aerosols and NO<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> have complex
evolution and transmission characteristics in the vertical direction. The
vertical upward transport of aerosol and NO<inline-formula><mml:math id="M55" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can promote the HONO
formation through heterogeneous reactions at high altitude, and the vertical
downward transport of HONO will impact the atmospheric environment near the
ground. The vertical observations in land and sea scenes are also helpful to
distinguish the contribution of the heterogeneous reaction of NO<inline-formula><mml:math id="M56" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on
the aerosol, ground, or sea surfaces (Zhang et al., 2020).</p>
      <p id="d1e940">Currently, a variety of HONO measurement techniques have been developed,
which in principle can be roughly divided into wet chemical, spectroscopy,
and mass spectrometry methods (Cheng et al., 2013; Bernard et al., 2016; Gil
et al., 2019; Guo et al., 2020; Jordan and Osthoff, 2020). However, these
technical methods can only measure the HONO information near the surface
layer. Taking tower and aircraft as platforms, these techniques were
performed to measure HONO vertical profiles, and it was found that the peak
values of HONO usually appeared under 200 m in urban and suburban areas
(Kleffmann et al., 2003; Stemmler et al., 2006; Zhang et al., 2009; Wong et
al., 2012; Meng et al., 2020; Zhang et al., 2020). These studies also
revealed that the heterogeneous reaction of NO<inline-formula><mml:math id="M57" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on multiple surfaces
(ground, aerosol, etc.) was an important source of HONO under the planetary
boundary layer (PBL), especially during haze days. Furthermore, they also
reported that the HONO <inline-formula><mml:math id="M58" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M59" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios usually decreased with the increase
in height under 200 m in inland and coastal areas. However, the cost of
the above techniques used to measure HONO vertical profiles was too high, and
the real-time and continuous measurements cannot be realized. Multi-axis
differential optical absorption spectroscopy (MAX-DOAS), as a ground-based
ultra-hyperspectral remote sensing technology, has been widely used for  the vertical
observation of atmospheric pollutants in the past two decades. In the past
5 years, several researchers carried out campaigns based on MAX-DOAS to
measure the vertical profile of HONO in inland and coastal areas, and they
revealed their vertical characteristics, sources, and the contribution to
atmospheric oxidation at different height layers (Garcia-Nieto et al., 2018;
Ryan et al., 2018; Wang et al., 2020; Xing et al., 2021; Xu et al., 2021; He
et al., 2023). Few studies were conducted on the sources of HONO at
different height layers in sea conditions. In this study, MAX-DOAS is used
for the first time to study the spatiotemporal distribution and the sources
of HONO along the Chinese coastline, as well as to learn the differences in the
HONO formed from the heterogeneous reaction of NO<inline-formula><mml:math id="M60" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in different height
layers and land and sea scenes.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods and methodologies</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Measurement cruise</title>
      <p id="d1e992">The ship-based atmospheric observation campaign along the marginal seas of
China was conducted from 19 April to 16 May 2018. The latitude and longitude
ranges of the entire campaign covered 21.12–35.89<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and
110.67–122.16<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E. The detailed voyage records of the observation
ship are shown in Table 1. An integrated and fully automated MAX-DOAS
instrument was installed on board the stern deck of the ship (Fig. S1a in the Supplement). To ensure that the instrument was always kept in a horizontal position, a
photoelectric gyro was used. The angle between the observation and heading
direction of the ship was always maintained at 135<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> during the whole
campaign. The telescope unit of the instrument pointed towards the sea during
cruise no. 3 and no. 6. The telescope unit pointed towards the land during
cruise no. 1, no. 4, and no. 5. During cruise no. 2, the observation telescope
always pointed to Chongming Island. The measurement ship only sailed during
daytime from 19 April to 2 May and continuously sailed during the entire daytime
and nighttime from 3 to 16 May 2018. The ship docked in the port of Daishan on
9–10 May, and no observations were conducted during these 2 d.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e1025">Detailed information of the measurement cruises.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Cruise</oasis:entry>
         <oasis:entry colname="col2">Periods</oasis:entry>
         <oasis:entry colname="col3">Measurement cruise</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">no.</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">No. 1</oasis:entry>
         <oasis:entry colname="col2">08:50 to 21:02 LT 19 April</oasis:entry>
         <oasis:entry colname="col3">Port of Daishan (30.24<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 122.16<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) to Chongming (31.18<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 121.82<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">No. 2</oasis:entry>
         <oasis:entry colname="col2">05:40 to 17:45 LT 20 April</oasis:entry>
         <oasis:entry colname="col3">Sailing around Chongming Island</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">No. 3</oasis:entry>
         <oasis:entry colname="col2">06:03 LT 21 April to 08:07 LT 3 May</oasis:entry>
         <oasis:entry colname="col3">Chongming (31.18<inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 121.82<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) to port of Zhanjiang (21.12<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 110.67<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">No. 4</oasis:entry>
         <oasis:entry colname="col2">08:07 LT 3 May to 06:52 LT 9 May</oasis:entry>
         <oasis:entry colname="col3">Port of Zhanjiang (21.12<inline-formula><mml:math id="M72" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 110.67<inline-formula><mml:math id="M73" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) to port of Daishan (30.24<inline-formula><mml:math id="M74" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 122.16<inline-formula><mml:math id="M75" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">No. 5</oasis:entry>
         <oasis:entry colname="col2">05:40 LT 11 May to 05:55 LT 14 May</oasis:entry>
         <oasis:entry colname="col3">Port of Daishan (30.24<inline-formula><mml:math id="M76" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 122.16<inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) to Qingdao (35.89<inline-formula><mml:math id="M78" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 120.87<inline-formula><mml:math id="M79" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">No. 6</oasis:entry>
         <oasis:entry colname="col2">05:55 LT 14 May to 10:00 LT 16 May</oasis:entry>
         <oasis:entry colname="col3">Qingdao (35.89<inline-formula><mml:math id="M80" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 120.87<inline-formula><mml:math id="M81" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) to port of Daishan (30.24<inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 122.16<inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{1}?></table-wrap>

      <p id="d1e1320">The aim of this campaign was to learn the vertical differences in the NO<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
heterogeneous reaction to produce HONO in marginal seas of China and compare
the influence mechanism of that in inland cities. To fully understand the
differences of the impacts of RH, temperature, and aerosol on the HONO
secondary formation in land and sea conditions, the Chinese Academy of
Meteorological Sciences (CAMS) and Southern University of Science and
Technology (SUST) MAX-DOAS stations were selected as inland and coastal
areas for analysis, respectively. CAMS is located in the urban area of Beijing
(39.94<inline-formula><mml:math id="M85" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 116.32<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), and SUST is located in Shenzhen
(22.60<inline-formula><mml:math id="M87" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 114.00<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) (Fig. S2). This study will provide
scientific guidance for understanding regional oxidation capacity and
controlling the secondary air pollution.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>MAX-DOAS measurements</title>
<sec id="Ch1.S2.SS2.SSS1">
  <label>2.2.1</label><title>Instrument setup</title>
      <?pagebreak page5818?><p id="d1e1383">The compact instrument consists of an ultraviolet spectrometer
(AvaSpec-ULS2048L-USB2, 300–460 nm spectral range, 0.6 nm spectral
resolution) at a 20<inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C fixed temperature with a deviation of
<inline-formula><mml:math id="M90" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.01<inline-formula><mml:math id="M91" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, a one-dimensional charge-coupled device (CCD) detector (Sony ILX511, 2048 individual pixels), and a telescope unit driven by a stepper motor to collect scattered sunlight from different elevation angles. The accuracy of
elevation angle is <inline-formula><mml:math id="M92" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.1<inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, and the telescope field of view (open
angle) is <inline-formula><mml:math id="M94" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3<inline-formula><mml:math id="M95" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. A full scanning sequence consists of 11
elevation angles (1, 2, 3, 4, 5, 6, 8, 10, 15, 30, and 90<inline-formula><mml:math id="M96" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>). The integration time
of one individual spectrum was set to 30 s, and each scanning sequence took
about 5.5 min. Besides, the controlling electronic devices and connecting
fiber are mounted inside. The instrument is equipped with a high-precision
global position system (GPS) to record the real-time coordinated positions
of the cruise ship. The detailed description of the setup of MAX-DOAS in
CAMS and SUST can be found in Liu et al. (2021).</p>
</sec>
<sec id="Ch1.S2.SS2.SSS2">
  <label>2.2.2</label><title>Data processing and filtering</title>
      <p id="d1e1461">The MAX-DOAS measurements could be influenced by the exhaust from the
measurement ship. Therefore, the data contaminated by the exhaust were
filtered out. As shown in Fig. S1b, the direction and speed of the plume
exhausted from the ship depend on the ship and the true wind
speeds and directions. Individual measurements taken under unfavorable plume
directions (plume directions between 45 and 135<inline-formula><mml:math id="M97" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> with respect to the heading
of the ship) were discarded. To avoid the strong influence of the
stratospheric absorption, the spectra measured with solar zenith angle (SZA)
larger than 75<inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> were filtered out. Under these two filtering
criteria, 4.9 % and 8.3 % of all data were rejected before DOAS analysis (Xing et al., 2017, 2019, 2020).</p>
</sec>
<sec id="Ch1.S2.SS2.SSS3">
  <label>2.2.3</label><title>DOAS analysis</title>
      <p id="d1e1490">The MAX-DOAS measured spectra were analyzed using the software QDOAS which
is developed by BIRA-IASB (<uri>http://uv-vis.aeronomie.be/software/QDOAS/</uri>, last access: 24 May 2023). The
DOAS fit results are the differential slant column densities (DSCDs), i.e., the difference of the slant column density (SCD) between the off-zenith and
the corresponding zenith reference spectra. Details of the DOAS fit settings
are listed in Table 2. A typical DOAS retrieval example for the oxygen dimer
(O<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>), nitrogen dioxide (NO<inline-formula><mml:math id="M100" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>), and nitrous acid (HONO) is shown in
Fig. 1. The stratospheric contribution was approximately eliminated by
taking the zenith spectra of each scan as a reference in the DOAS analysis.
Before profile retrieval, DOAS fit results of O<inline-formula><mml:math id="M101" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M102" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HONO
with root mean square (RMS) of residuals larger than 3 <inline-formula><mml:math id="M103" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M104" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
were filtered. Furthermore, the SCD data under the color index (CI) being
<inline-formula><mml:math id="M105" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 10 % of the thresholds obtained through fitting a fifth-order
polynomial to CI data, which is a function of time, were filtered out to ensure
a high signal-to-noise ratio (SNR) of the spectra. This filtering criteria
remove 2.1 %, 3.9 %, and 5.3 % for O<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, 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>, and HONO, respectively.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e1580">Detailed retrieval settings of O<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math id="M109" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HONO.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Parameter</oasis:entry>
         <oasis:entry colname="col2">Data source</oasis:entry>
         <oasis:entry rowsep="1" namest="col3" nameend="col5" align="center">Fitting internals (nm) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">O<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">NO<inline-formula><mml:math id="M113" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5">HONO</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Wavelength range</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">338–370</oasis:entry>
         <oasis:entry colname="col4">338–370</oasis:entry>
         <oasis:entry colname="col5">335–373</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<inline-formula><mml:math id="M114" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">298 K, <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">0</mml:mn><mml:mo>∗</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>-corrected, Vandaele et al. (1998)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M116" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M117" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M118" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">NO<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">220 K, <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">0</mml:mn><mml:mo>∗</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>-corrected, Vandaele et al. (1998)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M121" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M122" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M123" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">O<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">223 K, <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">0</mml:mn><mml:mo>∗</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>-corrected, Serdyuchenko et al. (2014)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M126" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M127" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M128" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">O<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">243 K, <inline-formula><mml:math id="M130" display="inline"><mml:mrow><mml:msubsup><mml:mi>I</mml:mi><mml:mn mathvariant="normal">0</mml:mn><mml:mo>∗</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>-corrected, Serdyuchenko et al. (2014)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M131" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M132" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M133" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">O<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">293 K, Thalman and Volkamer (2013)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M135" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M136" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M137" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HCHO</oasis:entry>
         <oasis:entry colname="col2">298 K, Meller and Moortgat (2000)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M138" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M139" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M140" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">H<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O</oasis:entry>
         <oasis:entry colname="col2">HITEMP, Rothman et al. (2010)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M142" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M143" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M144" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BrO</oasis:entry>
         <oasis:entry colname="col2">223 K, Fleischmann et al. (2004)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M145" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M146" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M147" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">HONO</oasis:entry>
         <oasis:entry colname="col2">296 K, Stutz et al. (2000)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M148" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M149" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M150" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ring</oasis:entry>
         <oasis:entry colname="col2">Calculated with QDOAS</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M151" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M152" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M153" display="inline"><mml:mo>✓</mml:mo></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Polynomial degree</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">Order 5</oasis:entry>
         <oasis:entry colname="col4">Order 5</oasis:entry>
         <oasis:entry colname="col5">Order 5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Intensity offset</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">Constant</oasis:entry>
         <oasis:entry colname="col4">Constant</oasis:entry>
         <oasis:entry colname="col5">Constant</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p id="d1e1601"><inline-formula><mml:math id="M110" display="inline"><mml:msup><mml:mi/><mml:mo>∗</mml:mo></mml:msup></mml:math></inline-formula> Solar <inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msub><mml:mi>I</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> correction; Aliwell et al. (2002).​​​​​​​</p></table-wrap-foot><?xmltex \gdef\@currentlabel{2}?></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e2175">Plots depicting typical DOAS spectral fittings for <bold>(a)</bold> O<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>, <bold>(b)</bold> NO<inline-formula><mml:math id="M155" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and <bold>(c)</bold> HONO.</p></caption>
            <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f01.png"/>

          </fig>

<?xmltex \hack{\newpage}?>
</sec>
</sec>
<?pagebreak page5819?><sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Vertical profile retrieval</title>
      <p id="d1e2222">Aerosol and trace gas (i.e., NO<inline-formula><mml:math id="M156" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO) vertical profiles are
retrieved from MAX-DOAS measurements using the algorithm reported by Liu et
al. (2021). The inversion algorithm is developed based on the optical
estimation method (OEM) (Rodgers, 2000), which employs the radiative
transfer model VLIDORT as the forward model. The detailed retrieval
procedure is displayed in Sect. S1 and Fig. S3.</p>
      <p id="d1e2234">In this study, an exponentially decreasing a priori profile with a scale height of 1.0 km was used as the initial profile for both the aerosol and trace gas
retrievals (Fig. S4). The surface concentrations of aerosol, NO<inline-formula><mml:math id="M157" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and
HONO were set to 0.2 km<inline-formula><mml:math id="M158" 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>, 3.0 ppb, and 1.0 ppb, respectively. We
assume a fixed set of aerosol optical properties with an asymmetry parameter of
0.69, a single scattering albedo of 0.90, and ground albedo of 0.05.
Furthermore, the uncertainty of the aerosol and trace gas a priori profile
was set to 100 %, and the correlation length was set to 0.5 km. The
averaging kernels indicated that the sensitivity of the profile retrieval
tended to decrease with increasing altitude and the retrieval especially sensitive to
the layers within 0–1.5 km (Fig. S5). The sum of the diagonal elements in
the averaging kernel matrix is the degree of freedom (DOF), which denotes
the number of independent pieces of information contained in the
measurements.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Error analysis</title>
      <p id="d1e2266">For profile retrieval, the error sources can be divided into four different
types: smoothing error, measurement noise error, forward model error, and
model parameter error (Frieß et al., 2006). However, in terms of this
classification, some errors are difficult to calculate or estimate. For
example, forward model error, which is caused by an imperfect representation
of the physics of the system, is hard to quantify due to the difficulty
of acquiring an improved forward model. Given calculation convenience and
contributing ratios of different errors in total error budget, we mainly
took into account error sources based on the following classification, which
were smoothing and noise errors, algorithm error, cross-section error, and
uncertainty related to the aerosol retrieval (only for trace gas). Here, we
estimated the contribution of different error sources to the trace gas
vertical column densities (VCDs) and aerosol optical depth (AOD), as well as near-surface (0–200 m) trace
gas concentrations and aerosol extinction coefficients (AECs).
The detailed demonstrations and estimation methods are displayed below, and
the final results are summarized in Table 3.
<list list-type="custom"><list-item><label>a.</label>
      <p id="d1e2271">Smoothing errors arise from the limited vertical resolution of profile
retrieval. Measurement noise errors denote the noise in the spectra (i.e.,
the fitting error of DOAS fits). They can be quantified by averaging the
error of retrieved profiles, as the error of the retrieved state vector
equals the sum of these two independent errors. We calculated the sum of
smoothing and noise errors on near-surface concentrations and column
densities, which were 14 % and 5 % for aerosols, 16 % and 17 % for NO<inline-formula><mml:math id="M159" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and 20 % and 22 % for HONO, respectively in the sea scene. The corresponding values were 13 % and 5 % for aerosols, 14 % and 16 % for NO<inline-formula><mml:math id="M160" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and 18 % and 20 % for HONO, respectively, at SUST and 13 % and 5 % for aerosols, 15 % and 17 % for NO<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and 19 % and 21 % for HONO
at CAMS.</p></list-item><list-item><label>b.</label>
      <p id="d1e2302">Algorithm error is the discrepancy between the measured and modeled DSCDs.
This error contains the forward model error from an imperfect approximation of
forward function (e.g., spatial inhomogeneities of<?pagebreak page5820?> absorbers and aerosols),
forward model parameter error from the selection of parameters, and error not
related to the forward function parameters, such as detector noise (Frieß et al., 2006). Algorithm error is a function of the viewing angle, and it is
difficult to assign this error to each altitude of profile. Usually, the
algorithm errors of the near-surface values and column densities are
estimated by calculating the average relative differences between the
measured and modeled DSCDs at the minimum and maximum elevation angles
(except 90<inline-formula><mml:math id="M162" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) (Wagner et al., 2004). Considering its
trivial role in the total error budget, we estimated these errors of the
near-surface values and the column densities at 4 and 8 % for aerosols, 3 % and 11 % for NO<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and 20 % and 20 % for HONO, according to Wang et al. (2017, 2020).</p></list-item><list-item><label>c.</label>
      <p id="d1e2324">Cross-section error is the error arising from an uncertainty in the cross section. According to Thalman and Volkamer (2013), Vandaele et al. (1998), and Stutz et al. (2000), we adopted 4 %, 3 %, and 5 % for O<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> (aerosols), NO<inline-formula><mml:math id="M165" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HONO, respectively.</p></list-item><list-item><label>d.</label>
      <p id="d1e2346">The trace gas profile retrieval error represents the one which is sourced
from aerosol extinction profile retrieval and propagated to retrieved trace
gas profile. This error could be roughly estimated based on a linear
propagation of the total error budgets of the aerosol retrievals. The errors
of trace gases were roughly estimated at 15 % for VCDs and 10 % for
near-surface concentrations for the two trace gases in the sea scene. The
corresponding values were 14 % and 10 % for near-surface concentrations and VCDs, respectively, at SUST, and 14 % and 10 % at CAMS.</p></list-item></list>
The total uncertainty was calculated by adding all the error terms in the
Gaussian error propagation, and the final results were listed in the bottom
row of Table 3. We found that the sum of smoothing and noise errors played a
dominant role in the total uncertainty.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><?xmltex \currentcnt{3}?><label>Table 3</label><caption><p id="d1e2353">Error budget estimation (in %) of the retrieved
near-surface (0–200 m) trace gas concentrations and AECs, as well as trace gas
VCDs and AOD.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry rowsep="1" namest="col4" nameend="col7" align="center">Error source </oasis:entry>
         <oasis:entry colname="col8">Total</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">Smoothing</oasis:entry>
         <oasis:entry colname="col5">Algorithm</oasis:entry>
         <oasis:entry colname="col6">Cross-</oasis:entry>
         <oasis:entry colname="col7">Related to the</oasis:entry>
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">and noise</oasis:entry>
         <oasis:entry colname="col5">error</oasis:entry>
         <oasis:entry colname="col6">section</oasis:entry>
         <oasis:entry colname="col7">aerosol retrieval</oasis:entry>
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4">errors</oasis:entry>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6">error</oasis:entry>
         <oasis:entry colname="col7">(only for trace</oasis:entry>
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">gases)</oasis:entry>
         <oasis:entry colname="col8"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">Cruise</oasis:entry>
         <oasis:entry colname="col2">Near-surface</oasis:entry>
         <oasis:entry colname="col3">Aerosol</oasis:entry>
         <oasis:entry colname="col4">14</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">15</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">route</oasis:entry>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M166" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">16</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">15</oasis:entry>
         <oasis:entry colname="col8">22</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2"/>
         <oasis:entry rowsep="1" colname="col3">HONO</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">20</oasis:entry>
         <oasis:entry rowsep="1" colname="col5">20</oasis:entry>
         <oasis:entry rowsep="1" colname="col6">5</oasis:entry>
         <oasis:entry rowsep="1" colname="col7">15</oasis:entry>
         <oasis:entry rowsep="1" colname="col8">32</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">VCD or AOD</oasis:entry>
         <oasis:entry colname="col3">AOD</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">8</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">17</oasis:entry>
         <oasis:entry colname="col5">11</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">23</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">HONO</oasis:entry>
         <oasis:entry colname="col4">22</oasis:entry>
         <oasis:entry colname="col5">20</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">32</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">SUST</oasis:entry>
         <oasis:entry colname="col2">Near-surface</oasis:entry>
         <oasis:entry colname="col3">Aerosol</oasis:entry>
         <oasis:entry colname="col4">13</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">14</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">14</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">14</oasis:entry>
         <oasis:entry colname="col8">20</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2"/>
         <oasis:entry rowsep="1" colname="col3">HONO</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">18</oasis:entry>
         <oasis:entry rowsep="1" colname="col5">20</oasis:entry>
         <oasis:entry rowsep="1" colname="col6">5</oasis:entry>
         <oasis:entry rowsep="1" colname="col7">14</oasis:entry>
         <oasis:entry rowsep="1" colname="col8">31</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">VCD or AOD</oasis:entry>
         <oasis:entry colname="col3">AOD</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">8</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M169" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">16</oasis:entry>
         <oasis:entry colname="col5">11</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">22</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">HONO</oasis:entry>
         <oasis:entry colname="col4">20</oasis:entry>
         <oasis:entry colname="col5">20</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">30</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CAMS</oasis:entry>
         <oasis:entry colname="col2">Near-surface</oasis:entry>
         <oasis:entry colname="col3">Aerosol</oasis:entry>
         <oasis:entry colname="col4">13</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">14</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M170" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">15</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">14</oasis:entry>
         <oasis:entry colname="col8">21</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry rowsep="1" colname="col2"/>
         <oasis:entry rowsep="1" colname="col3">HONO</oasis:entry>
         <oasis:entry rowsep="1" colname="col4">19</oasis:entry>
         <oasis:entry rowsep="1" colname="col5">20</oasis:entry>
         <oasis:entry rowsep="1" colname="col6">5</oasis:entry>
         <oasis:entry rowsep="1" colname="col7">14</oasis:entry>
         <oasis:entry rowsep="1" colname="col8">31</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">VCD or AOD</oasis:entry>
         <oasis:entry colname="col3">AOD</oasis:entry>
         <oasis:entry colname="col4">5</oasis:entry>
         <oasis:entry colname="col5">8</oasis:entry>
         <oasis:entry colname="col6">4</oasis:entry>
         <oasis:entry colname="col7">–</oasis:entry>
         <oasis:entry colname="col8">10</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">NO<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">17</oasis:entry>
         <oasis:entry colname="col5">11</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">23</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">HONO</oasis:entry>
         <oasis:entry colname="col4">21</oasis:entry>
         <oasis:entry colname="col5">20</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">10</oasis:entry>
         <oasis:entry colname="col8">31</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><?xmltex \gdef\@currentlabel{3}?></table-wrap>

</sec>
<sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Ancillary data</title>
      <p id="d1e3029">Meteorological data (including temperature, pressure, relative humidity,
visibility, solar radiation intensity, wind speed, and wind direction) with
a temporal resolution of 1 min were measured by the weather station installed
on the ship. NO was measured using an NO analyzer (Thermo Scientific model 42i)
with a 1 min resolution. The speed of the ship was calculated referring to
the GPS data.</p>
      <p id="d1e3032">The temperature and relative humidity of two ground-based stations (i.e.,
CAMS and SUST) were collected from the Weather Underground website, the temporal
resolution of which is around 3 h.</p>
      <p id="d1e3035">The backward trajectory was calculated using HYSPLIT (Hybrid Single-Particle
Lagrangian Integrated Trajectory) developed by the National Oceanic and
Atmospheric Administration Air Resource Laboratory (NOAA-ARL). The
meteorological data with a 1<inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M173" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M174" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> spatial resolution and
24 layers were collected from the Global Data Assimilation System (GDAS).</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Overview of the MAX-DOAS observations over marginal seas of
China</title>
      <p id="d1e3079">The radiative transfer model SCIATRAN was used to convert SCDs of NO<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
HONO to their tropospheric VCDs. The vertical profiles of aerosol, NO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
and HONO retrieved from MAX-DOAS; the temperature and pressure vertical
profiles simulated using a dynamical chemical model (WRF-Chem); and the
geo-position data collected by GPS were introduced as inputs in SCIATRAN for
the NO<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO air mass factor (AMF) calculation. Missing data are
due to power and instrument system failure, interference of ship plume,
unfavorable weather conditions (i.e., heavy rain), and night sailing. During
the cruise of Chongming to Zhanjiang, NO<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCDs varied from
1.05 <inline-formula><mml:math id="M179" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M180" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> to 4.02 <inline-formula><mml:math id="M181" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M182" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M183" 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> with an averaged value of 3.90 <inline-formula><mml:math id="M184" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M186" 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>. From Zhanjiang to Qingdao, NO<inline-formula><mml:math id="M187" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCDs varied from 1.08 <inline-formula><mml:math id="M188" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M189" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> to
2.60 <inline-formula><mml:math id="M190" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M191" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M192" 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> with an averaged value of
4.27 <inline-formula><mml:math id="M193" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M195" 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>. From Chongming to Zhanjiang, HONO VCDs varied from 1.00 <inline-formula><mml:math id="M196" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M197" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> to 2.58 <inline-formula><mml:math id="M198" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M200" 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> with a mean value of 2.39 <inline-formula><mml:math id="M201" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M202" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M203" 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>.
From Zhanjiang to Qingdao, HONO VCDs varied from 1.01 <inline-formula><mml:math id="M204" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> to
2.61 <inline-formula><mml:math id="M206" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M207" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M208" 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> with a mean value of 2.74 <inline-formula><mml:math id="M209" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M210" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M211" 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>.</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="d1e3423">Maps showing the spatial distributions of NO<inline-formula><mml:math id="M212" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO VCDs.
Panels <bold>(a)</bold> and <bold>(b)</bold> show the NO<inline-formula><mml:math id="M213" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO VCDs along the cruise route from Chongming to Zhanjiang. Panels <bold>(c)</bold> and <bold>(d)</bold> depict the NO<inline-formula><mml:math id="M214" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO VCDs along
the cruise route from Zhanjiang to Qingdao.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f02.png"/>

        </fig>

      <p id="d1e3472">Figure 2 shows the spatial distribution of NO<inline-formula><mml:math id="M215" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO VCDs over the
marginal seas of China. Five enhanced tropospheric NO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCD hot spots
were observed during the whole campaign, i.e., the coastal areas of the Yangtze
River Delta, Taiwan Strait, Guangzhou–Hong Kong–Macau Greater Bay Area,
port of Zhanjiang, and port of Qingdao. In the coastal areas of Yangtze River
Delta, the hot spots were mainly distributed in the Yangtze River estuary,
Hangzhou Bay, port of Ningbo, port of Taizhou, and port of Wenzhou. These areas are
mostly important shipping channels or shipping ports and are great NO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
emission sources. The averaged NO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCDs in the above five areas reached
1.07 <inline-formula><mml:math id="M219" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M220" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula>, 1.30 <inline-formula><mml:math id="M221" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M222" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula>, 7.27 <inline-formula><mml:math id="M223" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M224" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula>, 5.34 <inline-formula><mml:math id="M225" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M226" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula>, and 3.12 <inline-formula><mml:math id="M227" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M228" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M229" 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>, respectively (Fig. S6a). HONO exhibited similar spatial
distribution characteristics as NO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and the averaged HONO VCDs in the
above five hot-spot areas reached 1.01 <inline-formula><mml:math id="M231" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">15</mml:mn></mml:msup></mml:math></inline-formula>, 7.91 <inline-formula><mml:math id="M233" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M234" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>, 6.02 <inline-formula><mml:math id="M235" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M236" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>, 5.36 <inline-formula><mml:math id="M237" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M238" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula>, and
5.17 <inline-formula><mml:math id="M239" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M240" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M241" 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>, respectively (Fig. S6b). It
indicates that NO<inline-formula><mml:math id="M242" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is an important precursor of HONO. Earlier studies
reported that HONO can be generated from NO<inline-formula><mml:math id="M243" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> through heterogeneous
reactions on the surface of aerosol and the sea (Yang et al., 2021). However,
there are obvious differences in the concentration distribution of HONO and
NO<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2<?pagebreak page5821?></mml:mn></mml:msub></mml:math></inline-formula> in the southeast coastal area of Jiangsu (from Qidong to Dongtai).
In this area, NO<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> showed a higher concentration (1.66 <inline-formula><mml:math id="M246" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M247" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M248" 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>, which is 4 times higher than the mean NO<inline-formula><mml:math id="M249" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCD), while HONO showed a lower concentration (2.06 <inline-formula><mml:math id="M250" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M251" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M252" 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>, which is <inline-formula><mml:math id="M253" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 80 % of the mean HONO VCD). It
may be the fresh ship emission plume on the route enhancing the NO<inline-formula><mml:math id="M254" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration and HONO had not been fully formed from the NO<inline-formula><mml:math id="M255" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous
reaction in time, since the observations from the ship-based MAX-DOAS are
instantaneous.</p>
      <p id="d1e3837">The surface concentrations of NO<inline-formula><mml:math id="M256" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO were extracted from their
corresponding vertical profiles. As shown in Fig. 3, the total averaged
near-surface NO<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations under sea-oriented and land-oriented
measurements were 8.46 and 11.31 ppb, respectively. The total averaged
near-surface HONO concentrations were 0.23 and 0.27 ppb under sea-oriented
and land-oriented measurements. The total averaged near-surface
HONO <inline-formula><mml:math id="M258" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M259" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios in sea-oriented and land-oriented measurements were 0.027 and 0.024, respectively. Earlier studies reported that vehicle and
ship emissions were the main primary HONO sources on land and sea,
respectively, and NO<inline-formula><mml:math id="M260" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reactions on the surfaces of the ground,
sea, vegetation, and aerosol were the important secondary HONO sources (Liu
et al., 2021). Additionally, Yang et al. (2021) found that the surface HONO concentrations
in the sea cases were lower than that those in the land cases, especially in
the morning and evening. Figure 4 shows the time series
of AOD, the surface concentrations of NO<inline-formula><mml:math id="M261" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO, and the surface
HONO <inline-formula><mml:math id="M262" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M263" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during the whole campaign. We found that the time series of AOD and NO<inline-formula><mml:math id="M264" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were similar. The high AOD and NO<inline-formula><mml:math id="M265" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> usually appeared in busy shipping channels and ports, and the obvious high-value areas were the coast of the Yangtze River Delta, the Taiwan Strait, port of Xiamen, port of Zhanjiang, and port of Qingdao (with mean AOD and NO<inline-formula><mml:math id="M266" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> of 1.28 and 18.90 ppb,
respectively). HONO always appeared under high AOD and NO<inline-formula><mml:math id="M267" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> conditions;
however, high AOD and NO<inline-formula><mml:math id="M268" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were not necessarily accompanied by a high
HONO concentration. This was because the heterogeneous formation of HONO
requires suitable meteorological conditions (i.e., RH and temperature) in
addition to its precursor (NO<inline-formula><mml:math id="M269" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) and the reaction surface (aerosol) (Liu
et al., 2019). The high HONO <inline-formula><mml:math id="M270" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values were found on 2, 13, and 14 May with an average value of 0.45. Furthermore, we found the high values of HONO <inline-formula><mml:math id="M272" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M273" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> always appeared from 11:00 to 14:00 LT (UTC<inline-formula><mml:math id="M274" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>8)​​​​​​​ during the whole campaign.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e4006">Bar plots of the averaged aerosol extinction, NO<inline-formula><mml:math id="M275" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration, HONO concentration, and HONO <inline-formula><mml:math id="M276" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio during the
campaign. The red and blue boxes denote sea-oriented and land-oriented
measurements, respectively.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e4042">Histograms of the time series of <bold>(a)</bold> AOD, <bold>(b)</bold> surface NO<inline-formula><mml:math id="M278" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, <bold>(c)</bold> surface HONO concentration, and <bold>(d)</bold> surface HONO <inline-formula><mml:math id="M279" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M280" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f04.png"/>

        </fig>

</sec>
<?pagebreak page5822?><sec id="Ch1.S3.SS2">
  <label>3.2</label><?xmltex \opttitle{Relationship between HONO\,$/$\,NO${}_{{2}}$ with RH,
temperature, and aerosol for land and sea}?><title>Relationship between HONO <inline-formula><mml:math id="M281" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M282" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with RH,
temperature, and aerosol for land and sea</title>
      <p id="d1e4114">Sun et al. (2020) reported that HONO concentrations could increase by up to
40 %–100 % over the shipping routes and international ports, and Huang et al. (2017) reported vehicle exhaust could contribute to <inline-formula><mml:math id="M283" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12 %–49 % of the atmospheric HONO budget. Since the direct emissions of the
measurement ship were removed before data analysis, the primary source of
HONO during the whole campaign was mainly from the direct emissions of cargo
ships. By subtracting the average marine background of NO<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and HONO
from the ship plume emission values, the impact of background values is
reduced and the emission ratio of <inline-formula><mml:math id="M285" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>HONO <inline-formula><mml:math id="M286" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M287" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<inline-formula><mml:math id="M288" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> can be obtained, and this emission ratio can be used for quantifying the primary
HONO (Sun et al., 2020; Xu et al., 2015). In this study, we used an averaged
0.46 <inline-formula><mml:math id="M289" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.31 % emission ratio of <inline-formula><mml:math id="M290" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>HONO <inline-formula><mml:math id="M291" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M292" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<inline-formula><mml:math id="M293" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> referring
to Sun et al. (2020) to understand the primary source of HONO on the sea
surface during the campaign. The NO was measured using an in situ instrument,
and sea surface NO<inline-formula><mml:math id="M294" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was extracted from the retrieved NO<inline-formula><mml:math id="M295" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> vertical
profiles (NO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M297" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> NO <inline-formula><mml:math id="M298" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>). Additionally, the calculation
method of emission ratios of <inline-formula><mml:math id="M300" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>HONO <inline-formula><mml:math id="M301" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M302" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in CAMS and SUST was
taken from Xu et al. (2015), Liu et al. (2019), and Xing et al. (2021)
(Sect. S2). The averaged emission ratios in CAMS and SUST were
0.82 <inline-formula><mml:math id="M304" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.34 % and 0.79 <inline-formula><mml:math id="M305" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.31 %, respectively. The direct
emissions were deduced in the following study of the secondary formation of
HONO. The ratios of HONO <inline-formula><mml:math id="M306" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M307" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in CAMS, SUST, and the ship-based campaign
can be found in Fig. S7. Furthermore, the main secondary formation
pathway of HONO is considered the heterogeneous reaction of NO<inline-formula><mml:math id="M308" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on
the surface. The linear regression between HONO and NO<inline-formula><mml:math id="M309" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the land<?pagebreak page5823?> and
static sea scenarios is shown in Fig. 5. We found the fitting slopes in
static sea scenes were <inline-formula><mml:math id="M310" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 8–10 times larger than those in land
scenes, especially for sea-oriented measurements under static weather
conditions (slope <inline-formula><mml:math id="M311" display="inline"><mml:mo>≈</mml:mo></mml:math></inline-formula> 0.06). The correlation coefficients (<inline-formula><mml:math id="M312" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) in
inland and static sea scenarios were all <inline-formula><mml:math id="M313" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.62, except in SUST
(<inline-formula><mml:math id="M314" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M315" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.58), which indicates the formation rate of secondary HONO from
NO<inline-formula><mml:math id="M316" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction in static sea scenarios may be faster than
that in land scenarios. The corresponding temperature and RH conditions of
each spot are displayed in Fig. S8, which roughly reveals the impact of RH
and temperature on the process of NO<inline-formula><mml:math id="M317" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> forming HONO through
heterogeneous reactions.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e4395">Linear regression plots between surface NO<inline-formula><mml:math id="M318" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO
concentrations in <bold>(a)</bold> CAMS, <bold>(b)</bold> SUST, and ship-based measurements of <bold>(c)</bold> sea-oriented and <bold>(d)</bold> land-oriented observations under static weather conditions.</p></caption>
          <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f05.png"/>

        </fig>

<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>RH dependence on HONO formation</title>
      <p id="d1e4432">The scatter plots of HONO <inline-formula><mml:math id="M319" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> against RH in different land and sea
conditions are illustrated in Fig. 6. The highest values can represent
varying ranges of data in each interval and reveal concentration levels of
data distribution. To eliminate the influence of other factors, the average
of the six highest HONO <inline-formula><mml:math id="M321" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in each 10 % RH interval is calculated to
reflect the distribution range of data in each interval (Liu et al., 2019).
The dependence of the averaged top-six HONO <inline-formula><mml:math id="M323" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M324" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values on RH reveals an overall variation tendency of HONO <inline-formula><mml:math id="M325" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> against RH. In the inland (CAMS) and coastal (SUST) cases, the RH turning points are both <inline-formula><mml:math id="M327" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 65 % (60 %–70 %), where increasing trend switches to decreasing tendency. The HONO <inline-formula><mml:math id="M328" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> increases along with RH when RH is less than 65 %, and the HONO <inline-formula><mml:math id="M330" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> will decrease when RH is larger than 65 %, which implies
that it contributes to the HONO formation from the heterogeneous reaction of
NO<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on wet surfaces with the gradual increase in RH until 65 %. The
decrease in HONO <inline-formula><mml:math id="M333" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M334" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with RH larger than 65 % is presumably due to the efficient uptake of HONO on wet surfaces and the wet surfaces being less accessible or less reactive to NO<inline-formula><mml:math id="M335" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> when RH is larger than
65 % (Liu et al., 2019). However, two turning peaks of RH were found in
the sea cases. The first RH turning peak occurred in <inline-formula><mml:math id="M336" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 60 %,
which is similar to that in the inland and coastal cases, and another
RH turning peak appeared in <inline-formula><mml:math id="M337" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 85 % (80 %–90 %). This
implies that high RH also could increase the HONO formation in sea cases.
Additionally, the HONO <inline-formula><mml:math id="M338" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M339" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> decreased sharply when RH was larger than 95 % because the reaction surface will asymptotically approach a water droplet state to limit the formation of HONO with RH larger than 95 %.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e4607">Scatter plots between RH and HONO <inline-formula><mml:math id="M340" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M341" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios for <bold>(a)</bold> CAMS, <bold>(b)</bold> SUST, and <bold>(c)</bold> the ship-based campaigns.</p></caption>
            <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f06.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Temperature dependence on HONO formation</title>
      <?pagebreak page5825?><p id="d1e4650">The scatter plots of HONO <inline-formula><mml:math id="M342" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M343" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> against temperature in different land and sea conditions are shown in Fig. 7. Similar to the scatter plots of
HONO <inline-formula><mml:math id="M344" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M345" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> against RH, we also adopted the averaged top-six  HONO <inline-formula><mml:math id="M346" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M347" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values in each 5<inline-formula><mml:math id="M348" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C interval to represent a general variation tendency of HONO <inline-formula><mml:math id="M349" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M350" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> against temperature. In the inland condition (CAMS), the HONO <inline-formula><mml:math id="M351" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M352" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> decreased along with the increase in temperature, and the highest values of HONO <inline-formula><mml:math id="M353" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M354" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> appeared at <inline-formula><mml:math id="M355" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12.5<inline-formula><mml:math id="M356" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. However, we found that HONO <inline-formula><mml:math id="M357" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M358" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> increased along with
the increase in temperature, and the highest values of HONO <inline-formula><mml:math id="M359" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M360" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
appeared at <inline-formula><mml:math id="M361" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 31.5<inline-formula><mml:math id="M362" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in coastal conditions (SUST),
which indicates that the HONO formation from NO<inline-formula><mml:math id="M363" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction
will be accelerated under lower and higher temperature in the inland and
coastal conditions, respectively. In the sea condition, the HONO <inline-formula><mml:math id="M364" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M365" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> increased along with the increase in temperature with a high value under <inline-formula><mml:math id="M366" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25.0<inline-formula><mml:math id="M367" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C when the atmospheric temperature was higher than 18.0<inline-formula><mml:math id="M368" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, and simultaneously, a <inline-formula><mml:math id="M369" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.9 averaged
HONO <inline-formula><mml:math id="M370" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M371" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> high value was found under <inline-formula><mml:math id="M372" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 15.0<inline-formula><mml:math id="M373" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
(14.0–17.0<inline-formula><mml:math id="M374" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C). Furthermore, we found that the appearance of
HONO <inline-formula><mml:math id="M375" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M376" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> high values under lower temperature (14.0–17.0<inline-formula><mml:math id="M377" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) was usually accompanied by land breezes. Wen et al. (2019) also reported that
relatively high temperature could contribute to the formation of HONO in the
sea condition.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e4953">Scatter plots between temperature and HONO <inline-formula><mml:math id="M378" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M379" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios for <bold>(a)</bold> CAMS, <bold>(b)</bold> SUST, and <bold>(c)</bold> the ship-based campaigns.</p></caption>
            <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f07.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <label>3.2.3</label><title>Impact of aerosol on HONO formation</title>
      <p id="d1e4995">To further understand the HONO formation from the NO<inline-formula><mml:math id="M380" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous
reaction on the aerosol surface, several correlation analyses were conducted. As
shown in Fig. 8, the linear regression plot between HONO and aerosol in
land and sea conditions was performed. It was found that the correlation
coefficient (<inline-formula><mml:math id="M381" display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula>) between HONO and aerosol varied in the order of coastal
(0.55) <inline-formula><mml:math id="M382" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> sea (0.51) <inline-formula><mml:math id="M383" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> inland (0.14). Additionally, the
fitting slopes under coastal and sea conditions (0.07) are about 2.3 times
larger than those under inland conditions (0.03), which implies that the
ground surface may be more important than the aerosol surface during the process
of HONO formed from NO<inline-formula><mml:math id="M384" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reactions in the ground surface
layer inland. In the coastal and sea conditions, the aerosol and sea
are both important in providing a heterogeneous reaction surface for NO<inline-formula><mml:math id="M385" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
to form HONO (Cui et al., 2019; Wen et al., 2019; Yang et al., 2021).
Additionally, we found the averaged values of HONO <inline-formula><mml:math id="M386" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M387" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were
0.011 <inline-formula><mml:math id="M388" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.004, 0.014 <inline-formula><mml:math id="M389" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.006, 0.008 <inline-formula><mml:math id="M390" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.003, and 0.007 <inline-formula><mml:math id="M391" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.003 when aerosol extinctions are 0–0.3, 0.3–0.6, 0.6–0.9, and <inline-formula><mml:math id="M392" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.9 km<inline-formula><mml:math id="M393" 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> in the inland cases, respectively (Fig. 8b).
As shown in Fig. 8, the high values of HONO <inline-formula><mml:math id="M394" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M395" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> were mainly with
aerosol extinction being less than 1.0 km<inline-formula><mml:math id="M396" 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> with averaged values of
0.012 <inline-formula><mml:math id="M397" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.006 and 0.090 <inline-formula><mml:math id="M398" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.004 in the coastal and sea cases,
respectively. It indicates that the aerosol surface plays a more important role
in forming HONO through NO<inline-formula><mml:math id="M399" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reactions in the sea condition
than that in the land condition.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e5165">Panels <bold>(a)</bold>, <bold>(c)</bold>, and <bold>(e)</bold> show the linear regression plots between surface aerosol extinction and HONO concentrations for CAMS, SUST, and the ship-based campaigns, respectively. Panels <bold>(b)</bold>, <bold>(d)</bold>, and <bold>(f)</bold> depict the HONO <inline-formula><mml:math id="M400" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M401" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
ratio distribution under different aerosol extinction coefficient conditions
for CAMS, SUST, and the ship-based campaigns.</p></caption>
            <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f08.png"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><?xmltex \opttitle{Vertical distributions of HONO\,$/$\,NO${}_{{2}}$ under
different aerosol conditions for land and sea}?><title>Vertical distributions of HONO <inline-formula><mml:math id="M402" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M403" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> under
different aerosol conditions for land and sea</title>
      <p id="d1e5235">To further investigate the height dependence of HONO <inline-formula><mml:math id="M404" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M405" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> under land and sea conditions, two cases in the Pearl River Delta (PRD) were selected from the whole campaign. As shown in Fig. 9, “A” and “B” had a similar aerosol level (the extinction coefficients in the surface layer being 0.45–0.60 km<inline-formula><mml:math id="M406" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and vertical distribution structure and were all observed from 10:00 to 11:00 LT. The instrument viewing the sea accompanied with sea wind in “A” is named the sea scene, and the instrument viewing the land accompanied with land wind in “B” is named the land scene. The NO<inline-formula><mml:math id="M407" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in the sea and land scenes have
a similar vertical structure, and the NO<inline-formula><mml:math id="M408" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations in the land scene
are larger than those in the sea scene except on the surface layer. The HONO have
the same vertical distribution structure in the above two scenes, and the
HONO concentration in the land scene is always larger than that in the sea
scene. In Fig. 9e, we found that HONO <inline-formula><mml:math id="M409" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M410" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> under 0–400 m in the
land scene is higher than that in the sea scene; however, the HONO <inline-formula><mml:math id="M411" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M412" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values are obviously lower in the land scene than those in the sea scene above 400 m. Furthermore, the growth rate of HONO <inline-formula><mml:math id="M413" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M414" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> with the increase
in height in the sea scene is significantly faster than that in the land
scene above 400 m. This indicates the generation rates of HONO sourced from
NO<inline-formula><mml:math id="M415" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction on the aerosol surface in the sea scene are
larger than those in the land scene above 400 m. Under 400 m, the HONO
generation rates in the land scene are larger than those in the sea scene.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e5345">Panel <bold>(a)</bold> shows the two measurement points (A: black, sea-oriented with sea wind; B: red, land-oriented with land wind) during the campaign. Panels <bold>(b)</bold>–<bold>(e)</bold> show the vertical profiles of aerosol, NO<inline-formula><mml:math id="M416" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, HONO, and HONO <inline-formula><mml:math id="M417" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M418" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratios in the above two measurement points, respectively.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f09.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e5392">Plots showing the vertical distributions of <bold>(a)</bold> aerosol
extinction, <bold>(b)</bold> NO<inline-formula><mml:math id="M419" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, <bold>(c)</bold> HONO concentration, and <bold>(d)</bold> HONO <inline-formula><mml:math id="M420" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M421" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio. The blue and red lines represent a ship-based campaign case and a CAMS case, respectively.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f10.png"/>

        </fig>

      <p id="d1e5439">Additionally, we selected inland cases (CAMS) to learn the difference in
height dependence of HONO <inline-formula><mml:math id="M422" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M423" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> compared with sea scenes with  different
aerosol loads. As shown in Fig. 10, the sea and inland scenes had similar
aerosol levels (low aerosol level: <inline-formula><mml:math id="M424" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.2 km<inline-formula><mml:math id="M425" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and vertical
structure. Furthermore, the NO<inline-formula><mml:math id="M426" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO in the sea and inland scenes
have a similar vertical structure, although their concentrations in the sea
scene are all larger than those in the inland scene. In Fig. 10d, we
found that the HONO <inline-formula><mml:math id="M427" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M428" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sea scene was obviously larger than that in the inland scene above 400 m. The HONO <inline-formula><mml:math id="M429" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M430" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sea scene was about 4.5 times larger than that in the inland scene especially above 600 m. As shown in Fig. 11, the aerosols in the sea and inland scenes exhibited similar extinction levels (relatively high level: <inline-formula><mml:math id="M431" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.8 km<inline-formula><mml:math id="M432" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and vertical structure. The NO<inline-formula><mml:math id="M433" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration in the sea scene was higher than that in the inland scene but with a similar vertical structure. The HONO concentration in the sea scene was lower than that in the inland scene under 400 m, while the concentration in the sea scene was larger than that in the inland scene above 400 m. In Fig. 11d, we found the HONO <inline-formula><mml:math id="M434" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M435" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the inland scene was larger than that in the sea scene under 600 m, while the HONO <inline-formula><mml:math id="M436" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M437" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sea scene was about 2 times
larger than that in the inland scene above 600 m. All the above cases
indicated that the HONO generation rate from NO<inline-formula><mml:math id="M438" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction
in the sea scene was larger than that in the inland scene in higher
atmospheric layers above 400–600 m. The high-altitude (<inline-formula><mml:math id="M439" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 400–600 m) atmospheric parameters in the sea scene were more conductive to
promote the HONO formation through the heterogeneous reaction of NO<inline-formula><mml:math id="M440" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.
As shown in Fig. S9, the ratio of HONO <inline-formula><mml:math id="M441" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M442" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> also generally increased
with the increase in height above 0.2 km during the whole ship-based
campaign. The greatest sensitivity under 1.5 km and the high DOF for aerosol, NO<inline-formula><mml:math id="M443" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HONO gave confidence in the
retrieval results (Fig. S10).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e5633">Plots showing the vertical distributions of <bold>(a)</bold> aerosol
extinction, <bold>(b)</bold> NO<inline-formula><mml:math id="M444" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration, <bold>(c)</bold> HONO concentration, and <bold>(d)</bold> HONO <inline-formula><mml:math id="M445" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M446" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio. The blue and red lines represent a ship-based campaign case and a CAMS case, respectively.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f11.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Case study</title>
      <p id="d1e5688">The important factors and precursors to drive the formation of HONO through
heterogeneous reactions had complex evolution and transport characteristics.
To further clarify the role of these parameters in the heterogeneous process
of NO<inline-formula><mml:math id="M447" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2<?pagebreak page5826?></mml:mn></mml:msub></mml:math></inline-formula> to form HONO, three typical processes were selected to reveal
the favorable conditions for HONO formation in the sea scene.</p>
<sec id="Ch1.S3.SS4.SSS1">
  <label>3.4.1</label><title>20 April: a typical transport event</title>
      <p id="d1e5707">As shown in Fig. 12, the aerosol mainly distributed in 0–200 m with a
mean extinction coefficient larger than 0.74 km<inline-formula><mml:math id="M448" 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>. NO<inline-formula><mml:math id="M449" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was mainly
distributed near the ground surface with a mean concentration of 28.54 ppb
before 13:20 LT. The NO<inline-formula><mml:math id="M450" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> during this period may come from local ship
emissions, as this area is a main shipping channel. From 14:25 to 17:10 LT, a
high-concentration NO<inline-formula><mml:math id="M451" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> air mass (average 13.29 ppb) was found at
<inline-formula><mml:math id="M452" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 2.0 km. To understand the source of this high-altitude
NO<inline-formula><mml:math id="M453" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> air mass, we further investigated the possible influence of
transport by using the backward trajectories. We calculated 24 h backward
trajectories of air masses at 500, 1000, and 2000 m using HYSPLIT (Fig. S11). In Fig. S11, we found that the dominant wind direction during this period was southeast at all heights, i.e., 500, 1000, and 2000 m. The
transport of air masses carried NO<inline-formula><mml:math id="M454" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emitted by ships in the ports of Ningbo and
Zhoushan to the main cargo ports of China and Shanghai. Furthermore, the
concentration of NO<inline-formula><mml:math id="M455" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was low (averaged 2.32 ppb) near the ground
surface from 14:25 to 17:10 LT. As shown in Fig. 12e and g, a low-pressure (<inline-formula><mml:math id="M456" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 1020 hPa), north-dominant wind direction with a wind
speed <inline-formula><mml:math id="M457" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 12 m s<inline-formula><mml:math id="M458" 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> appeared at the ground surface during this period,
which implies that the clean air from the north reduced the local surface
NO<inline-formula><mml:math id="M459" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The HONO was mainly distributed near the surface with a mean
concentration of 0.07 ppb, and the two peaks were found in the early morning
(averaged 0.15 ppb) and at 12:15 LT (averaged 0.11 ppb), respectively (Fig. S12). The relatively high concentration of HONO appearing in the early
morning was possibly attributed to the accumulation with the stabilization
of the boundary layer and attenuation of solar radiation after sunset the day
before (Xing et al., 2021). The HONO peak appearing at 12:15 LT may be sourced
from the heterogeneous reaction of NO<inline-formula><mml:math id="M460" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the aerosol surface under a
<inline-formula><mml:math id="M461" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 80 % RH, 18.5<inline-formula><mml:math id="M462" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C temperature, and 1 <inline-formula><mml:math id="M463" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M464" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> W m<inline-formula><mml:math id="M465" 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> SRI conditions.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e5876">Case of 20 April 2018. Gradient images showing the time series of
<bold>(a)</bold> aerosol extinction, <bold>(b)</bold> NO<inline-formula><mml:math id="M466" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and <bold>(c)</bold> HONO vertical profiles. Panel <bold>(d)</bold> shows the time series of surface RH. Panel <bold>(e)</bold> depicts the time series of surface temperature and pressure. Panel <bold>(f)</bold> shows the time series of surface
SRI. Panel <bold>(g)</bold> depicts the time series of surface wind speed and wind direction.</p></caption>
            <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f12.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <label>3.4.2</label><?xmltex \opttitle{28 April: a typical event of HONO produced from
NO${}_{{2}}$ heterogeneous reaction}?><title>28 April: a typical event of HONO produced from
NO<inline-formula><mml:math id="M467" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction</title>
      <p id="d1e5934">From a typical port observation case, the measurement ship was moored at the port of  Xiamen
on 28 April. As shown in Fig. 13, we found two peaks for aerosol and
NO<inline-formula><mml:math id="M468" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from 09:00–11:00 and 14:00–16:00 LT, respectively (averaged aerosol
extinction coefficient <inline-formula><mml:math id="M469" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.8 km<inline-formula><mml:math id="M470" 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>, averaged NO<inline-formula><mml:math id="M471" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
concentration <inline-formula><mml:math id="M472" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 12.0 ppb). NO<inline-formula><mml:math id="M473" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was mainly distributed near
the sea surface layer at 0–200 m, and a high-concentration NO<inline-formula><mml:math id="M474" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> air mass
was found from 1.0–2.0 km from 13:00–14:00 LT due to the short-distance
transport of NO<inline-formula><mml:math id="M475" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emitted from ships in the port of Xiamen (Fig. S13).
However, aerosol appeared in the range of 0.0–2.0 km from 09:00–11:00
and 14:00–16:00 LT. In Fig. 13g, we found that the<?pagebreak page5827?> wind speeds in the
above two peak periods were obviously higher than those in other periods.
From 09:00–11:00 LT, the wind speed was <inline-formula><mml:math id="M476" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 5.0 m s<inline-formula><mml:math id="M477" 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> with a
northwest-dominant direction (urban), and the wind speed was <inline-formula><mml:math id="M478" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 6.0 m s<inline-formula><mml:math id="M479" 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> with a southeast-dominant direction (port gateway)  from 14:00–16:00 LT, which indicates that the short-distance high-altitude
transport caused the appearance of high-extinction aerosol mass during the
above two periods.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e6050">Case of 28 April 2018. Gradient images showing the time series of
<bold>(a)</bold> aerosol extinction, <bold>(b)</bold> NO<inline-formula><mml:math id="M480" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and <bold>(c)</bold> HONO vertical profiles. Panel <bold>(d)</bold> shows the time series of surface RH. Panel <bold>(e)</bold> depicts the time series of surface temperature and pressure. Panel <bold>(f)</bold> shows the time series of surface SRI. Panel <bold>(g)</bold> depicts the time series of surface wind
speed and wind direction.</p></caption>
            <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f13.png"/>

          </fig>

      <p id="d1e6090">Furthermore, we found the high-concentration HONO only appeared at
14:00–16:00 LT with a 0.57 ppb averaged concentration under 0.9 km, while it was only about 0.14 ppb during the 09:00–11:00 LT period. The slight increase in
RH and temperature (Tem) at 14:00–16:00 LT (RH: <inline-formula><mml:math id="M481" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 75.0 %; Tem:
23.7<inline-formula><mml:math id="M482" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C) may contribute more to HONO formation through heterogeneous
reactions of NO<inline-formula><mml:math id="M483" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the aerosol surface than that at 09:00–11:00 LT
(Fig. 13d–e, Sect. 3.2). Contrarily, the SRI (<inline-formula><mml:math id="M484" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 600 W m<inline-formula><mml:math id="M485" 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>) at 09:00–11:00 LT was obviously larger
than that (<inline-formula><mml:math id="M486" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 250 W m<inline-formula><mml:math id="M487" 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>) at 14:00–16:00 LT (Fig. 13f).
The higher SRI accelerated the photolysis of HONO during the 09:00–11:00 LT period
(Kraus and Hofzumahaus, 1998). Therefore, the lower formation rate and higher
photolysis rate lead to a significantly lower HONO concentration at
09:00–11:00 LT than that at 14:00–16:00 LT.</p>
</sec>
<?pagebreak page5828?><sec id="Ch1.S3.SS4.SSS3">
  <label>3.4.3</label><title>3 May: a typical event with unknown HONO source</title>
      <p id="d1e6165">The measurement ship conducted observations in the sea area near Zhanjiang on
3 May, 2018. As shown in Fig. 14, we found that there was an obvious
sinking process for aerosol from <inline-formula><mml:math id="M488" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.0 km from 09:00–16:00 LT that eventually accumulated near the sea surface with a high extinction
coefficient <inline-formula><mml:math id="M489" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.92 km<inline-formula><mml:math id="M490" 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 NO<inline-formula><mml:math id="M491" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was mainly
concentrated near the sea surface layer (0–400 m) with an averaged
concentration of 8.93 ppb from 08:00 to 09:00 LT. Thereafter, with the rise in the
PBL height after sunrise, NO<inline-formula><mml:math id="M492" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was gradually
mixed and spread throughout the PBL from 09:00–13:00 LT. During this period,
it was accompanied by the increase in the NO<inline-formula><mml:math id="M493" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (averaged
11.2 ppb) under the PBL (Fig. S14). It is due to the contribution of ship
emissions near the sea surface. Contrarily, the regional transport of
NO<inline-formula><mml:math id="M494" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> from land also increased the NO<inline-formula><mml:math id="M495" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration in this area of
the sea, with wind speed increasing from 2.5 to 7.8 m s<inline-formula><mml:math id="M496" 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> with a north wind direction from 10:00 to 16:00 LT (Fig. 14g).</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e6254">Case of 3 May 2018. Gradient images showing the time series of
<bold>(a)</bold> aerosol extinction, <bold>(b)</bold> NO<inline-formula><mml:math id="M497" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and <bold>(c)</bold> HONO vertical profiles. Panel <bold>(d)</bold> shows the time series of surface RH. Panel <bold>(e)</bold> depicts the time series of surface temperature and pressure. Panel <bold>(f)</bold> shows the time series of surface SRI. Panel <bold>(g)</bold> depicts the time series of surface wind
speed and wind direction.</p></caption>
            <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://acp.copernicus.org/articles/23/5815/2023/acp-23-5815-2023-f14.png"/>

          </fig>

      <p id="d1e6294">Several HONO peaks (<inline-formula><mml:math id="M498" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 0.2 ppb) at 0.5–1.0 km were found from
09:45 to 13:00 LT, and the aerosol and NO<inline-formula><mml:math id="M499" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> high values were also observed
at this height layer, simultaneously, which implies that the heterogeneous
reaction of NO<inline-formula><mml:math id="M500" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the aerosol surface is more important than that on the
sea surface for HONO source under sea atmosphere. Additionally, HONO
concentration obviously elevated after 14:00 LT, especially from 14:00–16:00 LT
(<inline-formula><mml:math id="M501" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 0.4 ppb). It may be sourced from the heterogeneous reaction of
NO<inline-formula><mml:math id="M502" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the aerosol surface, with RH being <inline-formula><mml:math id="M503" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 92.5 %
(Fig. 14d). The photolysis of HONO also decreased with SRI <inline-formula><mml:math id="M504" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 150 W m<inline-formula><mml:math id="M505" 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> (Fig. 14f) during this period. Furthermore, a HONO peak
(<inline-formula><mml:math id="M506" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 0.32 ppb) was observed from 16:40–17:10 LT. However, the
NO<inline-formula><mml:math id="M507" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration always remained low (<inline-formula><mml:math id="M508" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 1.5 ppb) after 16:00 LT, and the temperature was lower than 17<inline-formula><mml:math id="M509" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (Fig. 14e), which
indicates the heterogeneous reaction of NO<inline-formula><mml:math id="M510" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> not being the source of the
observed HONO peak. The wind was north-dominant with an average speed at 7.8 m s<inline-formula><mml:math id="M511" 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> after 15:00 LT, which implies that the regional transport may not be the
source of the observed high-concentration of HONO. Furthermore, the SRI was
lower than 87.5 W m<inline-formula><mml:math id="M512" 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 it shows the photolysis of nitrate aerosol
also not being the source of the elevated HONO. The unknown HONO sources in
this area of the sea need to be further explored.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary and conclusions</title>
      <?pagebreak page5829?><p id="d1e6441">Currently, many uncertainties in the study of the HONO forming mechanism
through the heterogeneous reaction of NO<inline-formula><mml:math id="M513" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> exist. Earlier studies
mostly focused on the near-surface layer, and the assessment of the
contribution of the NO<inline-formula><mml:math id="M514" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction to HONO formation in the
vertical direction of the boundary layer is insufficient. Therefore, we aim
to learn the sea–land and vertical differences of the HONO forming mechanism
from the NO<inline-formula><mml:math id="M515" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction and provide deep insights into the
distribution characteristics, transforming process, and environmental
effects of tropospheric HONO. Ship-based MAX-DOAS observations along the
marginal seas of China were performed from 19 April to 16 May 2018.
Simultaneously, two ground-based MAX-DOAS observations were conducted in the
inland station CAMS and the coastal station SUST to measure the aerosol,
NO<inline-formula><mml:math id="M516" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, and HONO vertical profiles.</p>
      <p id="d1e6480">Along the cruise route, we found five hot spots with enhanced tropospheric
NO<inline-formula><mml:math id="M517" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VCDs in the Yangtze River Delta, Taiwan Strait, Guangzhou–Hong
Kong–Macau Greater Bay Area, port of Zhanjiang, and port of Qingdao. Under
high-level NO<inline-formula><mml:math id="M518" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> conditions in the above five hot spots, we also observed
enhanced HONO levels. Contrastingly, the low-concentration HONO accompanied
high-level NO<inline-formula><mml:math id="M519" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the southeast coastline of Jiangsu province. When
peak AOD and NO<inline-formula><mml:math id="M520" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> conditions were observed, enhanced HONO was observed,
although the reverse was not always the case.</p>
      <p id="d1e6519">To understand the impacts of RH, temperature, and aerosol on the
heterogeneous reaction of NO<inline-formula><mml:math id="M521" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to produce HONO, the emission ratios of
<inline-formula><mml:math id="M522" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>HONO <inline-formula><mml:math id="M523" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M524" display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>NO<inline-formula><mml:math id="M525" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> were calculated to quantify the contribution of the primary HONO source to the total production of HONO. We found that the RH turning points in CAMS and SUST cases were both <inline-formula><mml:math id="M526" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 65 %
(60 %–70 %), whereas two turning peaks (<inline-formula><mml:math id="M527" display="inline"><mml:mo lspace="0mm">∼</mml:mo></mml:math></inline-formula> 60 % and
<inline-formula><mml:math id="M528" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 85 %) of RH were found in the sea cases. This implied that
high RH could contribute to the secondary formation of HONO in the sea
atmosphere. With an increase in temperature, the HONO <inline-formula><mml:math id="M529" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M530" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> decreased with peak values appearing at <inline-formula><mml:math id="M531" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 12.5<inline-formula><mml:math id="M532" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in CAMS, whereas the
HONO <inline-formula><mml:math id="M533" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M534" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> gradually increased and reached peak values at <inline-formula><mml:math id="M535" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 31.5<inline-formula><mml:math id="M536" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C in SUST. In the sea cases, when the temperature exceeded
18.0<inline-formula><mml:math id="M537" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, the HONO <inline-formula><mml:math id="M538" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M539" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> increased with the increasing temperature and achieved a peak at <inline-formula><mml:math id="M540" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25.0<inline-formula><mml:math id="M541" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. This indicated that
high temperature could promote the secondary formation of HONO in the sea
and coastal atmosphere. Additionally, the correlation analysis under
different sea–land conditions indicated that the ground surface is more
crucial to the formation of HONO from the NO<inline-formula><mml:math id="M542" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction in the
inland cases, whereas the aerosol surface contributed more in the coastal and
sea cases.</p>
      <?pagebreak page5832?><p id="d1e6699">Furthermore, we found that the HONO <inline-formula><mml:math id="M543" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M544" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> in the sea cases was about 4.5 times larger than that in the inland cases above 600 m when the AEC was
<inline-formula><mml:math id="M545" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.2 km<inline-formula><mml:math id="M546" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, and the HONO <inline-formula><mml:math id="M547" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NO<inline-formula><mml:math id="M548" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> ratio in the sea cases
was about 2 times larger than that in the inland cases above 600 m when the AEC
was <inline-formula><mml:math id="M549" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.8 km<inline-formula><mml:math id="M550" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, which implied that the generation rate of
HONO from NO<inline-formula><mml:math id="M551" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction in the sea cases is larger than
that in the inland cases in higher atmospheric layers (<inline-formula><mml:math id="M552" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 600 m).
To have a deep understanding of three potential contributing factors of HONO
production under marine conditions, we selected three typical events, which
represented the impacts of transport, NO<inline-formula><mml:math id="M553" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> heterogeneous reaction, and
unknown HONO source.</p>
</sec>

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

      <p id="d1e6803">All measurement data used in this study can be made available for scientific purpose upon request to the corresponding author (Cheng Liu, chliu81@ustc.edu.cn).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e6806">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-23-5815-2023-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-23-5815-2023-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e6815">CX, CL, and KL designed the research and organized this paper. CX wrote this paper, and CL and KL edited it. CX, SX, and YS contributed to the retrieval of MAX-DOAS vertical profile data. CX, YL, CZ, QH, and SW contributed to data analysis. CX, WT, HW, and HL contributed to the MAX-DOAS instrument setup and observations. All the above authors contributed to the revision of the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e6821">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="d1e6827">Publisher’s note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e6833">We would like to also thank Fudan University (Jianmin Chen's group) for organizing the ship-based campaign and providing meteorological data.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e6838">This research has been supported by the National Natural Science Foundation of China (grant nos. 42207113, 41941011, 51778596, 41575021, and 41977184); the Anhui Provincial Natural Science Foundation (grant no. 2108085QD180); the Presidential Foundation of the Hefei Institutes of Physical Science, Chinese Academy Sciences (grant no. YZJJ2021QN06); the Strategic Priority Research Program of the Chinese Academy of Sciences (grant no. XDA23020301); and the National High-Resolution Earth Observation Project of China (grant no. 05-Y30B01-9001-19/20-3).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e6844">This paper was edited by John Liggio and reviewed by two anonymous referees.</p>
  </notes><ref-list>
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