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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" xml:lang="en" dtd-version="3.0" article-type="research-article"><?xmltex \bartext{Research article}?>
  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-22-11347-2022</article-id><title-group><article-title>The positive effect of formaldehyde on the photocatalytic renoxification of
nitrate on TiO<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> particles</article-title><alt-title>The positive effect of formaldehyde on the renoxification of nitrate</alt-title>
      </title-group><?xmltex \runningtitle{The positive effect of formaldehyde on the renoxification of nitrate}?><?xmltex \runningauthor{Y. Liu et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Liu</surname><given-names>Yuhan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Wang</surname><given-names>Xuejiao</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes">
          <name><surname>Shang</surname><given-names>Jing</given-names></name>
          <email>shangjing@pku.edu.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Xu</surname><given-names>Weiwei</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Sheng</surname><given-names>Mengshuang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no">
          <name><surname>Ye</surname><given-names>Chunxiang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5417-2671</ext-link></contrib>
        <aff id="aff1"><institution>State Key Joint Laboratory of Environmental Simulation and Pollution Control, College of Environmental Sciences and Engineering, Peking University, 5 Yiheyuan Road, Beijing 100871, PR China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Jing Shang (shangjing@pku.edu.cn)</corresp></author-notes><pub-date><day>5</day><month>September</month><year>2022</year></pub-date>
      
      <volume>22</volume>
      <issue>17</issue>
      <fpage>11347</fpage><lpage>11358</lpage>
      <history>
        <date date-type="received"><day>5</day><month>January</month><year>2022</year></date>
           <date date-type="rev-request"><day>27</day><month>January</month><year>2022</year></date>
           <date date-type="rev-recd"><day>4</day><month>August</month><year>2022</year></date>
           <date date-type="accepted"><day>11</day><month>August</month><year>2022</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2022 </copyright-statement>
        <copyright-year>2022</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d1e134">Renoxification is the process of recycling NO<inline-formula><mml:math id="M2" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M3" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> into
NO<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> under illumination and is mostly ascribed to the photolysis of
nitrate. TiO<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>, a typical mineral dust component, is able to play a
photocatalytic role in the renoxification process due to the formation of NO<inline-formula><mml:math id="M7" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> radicals; we define this process as “photocatalytic renoxification”.
Formaldehyde (HCHO), the most abundant carbonyl compound in the atmosphere,
may participate in the renoxification of nitrate-doped TiO<inline-formula><mml:math id="M8" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles.
In this study, we established a 400 L environmental chamber reaction system
capable of controlling 0.8 %–70 % relative humidity at 293 K with the
presence of 1 or 9 ppm HCHO and 4 wt % nitrate-doped TiO<inline-formula><mml:math id="M9" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. The
direct photolyses of both nitrate and NO<inline-formula><mml:math id="M10" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> radicals were excluded by
adjusting the illumination wavelength so as to explore the effect of HCHO
on the “photocatalytic renoxification”. It was found that NO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentrations can reach up to more than 100 ppb for nitrate-doped TiO<inline-formula><mml:math id="M12" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
particles, while almost no NO<inline-formula><mml:math id="M13" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was generated in the absence of HCHO.
Nitrate type, relative humidity and HCHO concentration were found to
influence NO<inline-formula><mml:math id="M14" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> release. It was suggested that substantial amounts of
NO<inline-formula><mml:math id="M15" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> were produced via the NO<inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M18" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M19" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway, where TiO<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> worked for converting
“NO<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>” to “NO<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> ”, that HCHO participated in the
transformation of “NO<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula> ” to “HNO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>” through hydrogen
abstraction, and that “HNO<inline-formula><mml:math id="M25" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>” photolysis answered for mass NOx release. So,
HCHO played a significant role in this “photocatalytic renoxification”
process. These results were found based on simplified mimics for atmospheric
mineral dust under specific experimental conditions, which might deviate
from the real situation but illustrated the potential of HCHO to
influence nitrate renoxification in the atmosphere. Our proposed reaction
mechanism by which HCHO promotes photocatalytic renoxification is helpful
for deeply understanding atmospheric photochemical processes and
nitrogen cycling and could be considered for better fitting atmospheric
model simulations with field observations in some specific scenarios.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e382">The levels of ozone (O<inline-formula><mml:math id="M26" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) and hydroxyl radicals (<inline-formula><mml:math id="M27" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH) in the
troposphere can be promoted by nitrogen oxides (NO<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 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>), such that NO<inline-formula><mml:math id="M31" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> plays an important role in the formation of
secondary aerosols and atmospheric oxidants  (Platt et al., 1980; Stemmler
et al., 2006; Harris et al., 1982; Finlayson-Pitts and Pitts, 1999).
NO<inline-formula><mml:math id="M32" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> can be converted into nitric acid (HNO<inline-formula><mml:math id="M33" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>) and nitrate
(NO<inline-formula><mml:math id="M34" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) through a series of oxidation and hydrolysis reactions and
is eventually removed from the atmosphere through subsequent wet or dry
deposition  (Dentener and Crutzen, 1993; Goodman et al., 2001; Monge et
al., 2010; Bedjanian and El Zein, 2012). However, comparisons of
observations and modeling results for the marine boundary layer, land, and
free troposphere   (Read et al., 2008; Lee et al., 2009; Seltzer et al.,
2015) have shown an underestimation of HNO<inline-formula><mml:math id="M35" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> or NO<inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> content,
NO<inline-formula><mml:math id="M37" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> abundance, and NO<inline-formula><mml:math id="M38" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M39" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M40" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> ratios, indicating the presence
of a new, rapid NO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> circulation pathway  (Ye et al., 2016b; Reed et
al., 2017). Some researchers have suggested that deposited NO<inline-formula><mml:math id="M42" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>
and HNO<inline-formula><mml:math id="M43" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> can be recycled back to gas-phase NO<inline-formula><mml:math id="M44" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> under illumination
via the renoxification process   (Schuttlefield et al., 2008; Romer et al.,
2018; Bao et al., 2020; Shi et al., 2021). Photolytic renoxification occurs
under light with a wavelength of <inline-formula><mml:math id="M45" display="inline"><mml:mi mathvariant="italic">&lt;</mml:mi></mml:math></inline-formula> 350 nm through the photolysis of
NO<inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M47" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M48" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> adsorbed on the solid surface to generate NO<inline-formula><mml:math id="M49" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>.
Notably, the photolysis of NO<inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M51" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> HNO<inline-formula><mml:math id="M52" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is reported to occur at
least 2 orders of magnitude faster on different solid surfaces (natural or
artificial) or on aerosols than in the gas phase (Ye et al., 2016a; Zhou et
al., 2003; Baergen and Donaldson, 2013). Several recent studies have shown
that renoxification has important atmospheric significance  (Deng et al.,
2010; Kasibhatla et al., 2018; Romer et al., 2018; Alexander et al., 2020),
providing the atmosphere with a new source of photochemically reactive
nitrogen species, i.e., HONO or NO<inline-formula><mml:math id="M53" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, resulting in the production of
more photooxidants such as O<inline-formula><mml:math id="M54" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> or <inline-formula><mml:math id="M55" display="inline"><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:math></inline-formula>OH (Ye et al.,
2017), which further oxidize volatile organic compounds (VOCs), leading to
the formation of more chromophores and thereby affecting the photochemical
process (Bao et al., 2020).</p>
      <p id="d1e664">Renoxification processes have recently been observed on different types of
atmospheric particles, such as urban grime and mineral dust  (Ninneman et
al., 2020; Bao et al., 2018; Baergen and Donaldson, 2013; Ndour et al.,
2009). Atmospheric titanium dioxide (TiO<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>) is mainly derived from
windblown mineral dust, with mass mixing ratios ranging from 0.1 % to 10 %
(Chen et al., 2012). TiO<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> is widely used in industrial processes
and building exteriors for its favorable physical and chemical properties.
Titanium and nitrate ions have been found to coexist in atmospheric
particulates in different regions worldwide  (Sun et al., 2005; Liu et
al., 2005; Yang et al., 2011; Kim et al., 2012), and the
NO<inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M59" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> (NO<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> TiO<inline-formula><mml:math id="M61" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) mass percentage of total
suspended particulate matter (TSP) during dust storms can be lower than
20 % (Sun et al., 2005). In this case, nitrate-coated
TiO<inline-formula><mml:math id="M62" 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="M63" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M64" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) aerosols containing TiO<inline-formula><mml:math id="M65" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> as the
main body can, to some extent, be used to represent the real situation under
sandstorms. TiO<inline-formula><mml:math id="M66" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is a semiconductor metal oxide that can facilitate the
photolysis of nitrate and the release of NO<inline-formula><mml:math id="M67" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> due to its photocatalytic
activity  (Ndour et al., 2009; Chen et al., 2012; Verbruggen, 2015;
Schwartz-Narbonne et al., 2019). Under UV light, TiO<inline-formula><mml:math id="M68" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
generates electron-hole pairs in the conduction and valence bands,
respectively  (Linsebigler et al., 1995). Nitrate ions adsorbed at
the oxide surface react with the photogenerated holes (h<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>) to form
nitrate radicals (NO<inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>), which are subsequently photolyzed
to NO<inline-formula><mml:math id="M71" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, mainly under visible illumination (Schuttlefield et
al., 2008; George et al., 2015; Schwartz-Narbonne et al., 2019). Thus, the
renoxification of NO<inline-formula><mml:math id="M72" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is faster on TiO<inline-formula><mml:math id="M73" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> than on other oxides
in mineral dust aerosols such as SiO<inline-formula><mml:math id="M74" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or Al<inline-formula><mml:math id="M75" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M76" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>  (Lesko et
al., 2015; Ma et al., 2021). In this study, we refer to renoxification
involving h<inline-formula><mml:math id="M77" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and NO<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> as photocatalytic
renoxification based on the photocatalytic properties of TiO<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>.</p>
      <p id="d1e905">Many previous studies have focused mainly on particulate nitrate–NO<inline-formula><mml:math id="M80" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
photochemical cycling reactions despite the potential impact of other
reactant gases in the atmosphere. Formaldehyde (HCHO), the most abundant
carbonyl compound in the atmosphere, can reach as high as 0.4 ppm in some
specific situations (particularly in some indoor air or in cities with high
traffic density)  (Wilbourn et al.,
1995; Salthammer, 2019). HCHO can react with NO<inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> at night
via hydrogen abstraction reactions to form HNO<inline-formula><mml:math id="M82" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>  (Atkinson, 1991).
Our previous study showed that the degradation rate of HCHO was faster on
NO<inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<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> aerosols than on TiO<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles, perhaps as a
result of HCHO oxidation by NO<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>   (Shang et al.,
2017). To date, no studies have reported the effect of HCHO on
photocatalytic renoxification. Adsorbed HCHO would react with
NO<inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> generated on the NO<inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> aerosol
surface, thus altering the surface nitrogenous species and renoxification
process. The present study is the first to explore the combined effect of
HCHO and photocatalytic TiO<inline-formula><mml:math id="M90" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles on the renoxification of
nitrate. The wavelengths of the light sources were adjusted to exclude
photolytic renoxification while making photocatalytic renoxification
available for better elucidating the reaction mechanism. We investigated the
effects of various influential factors – including nitrate type, nitrate
content, RH, and initial HCHO concentration – to understand the atmospheric
renoxification of nitrate in greater detail.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Environmental chamber setup</title>
      <p id="d1e1038">Details of the experimental apparatus and protocol used in the current study
have been previously described (Shang et al., 2017). Briefly,
the main body of the environmental chamber is a 400 L polyvinyl fluoride
(PVF) bag filled with synthetic air (high purity N<inline-formula><mml:math id="M91" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (99.999 %) mixed
with high purity O<inline-formula><mml:math id="M92" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (99.999 %) with a ratio of 79:21 by volume;
Beijing Huatong Jingke Gas Chemical Co.). The chamber is capable of
temperature (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">293</mml:mn></mml:mrow></mml:math></inline-formula> K) and relative humidity (0.8 %–70 %)
control using a water bubbler and air conditioners, respectively. The
chamber is equipped with two light sources, both with a central wavelength
of 365 nm. One is a set of 36 W tube lamps with a main spectrum of 320–400 nm and a small amount of 480–600 nm visible light (Fig. S1a). The other is
a set of 12 W LED lamps with a narrow main spectrum
of 350–390 nm (Fig. S1b). The light intensities for the tube and LED lamp
at 365 nm were 300 and 200 <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>W cm<inline-formula><mml:math id="M95" 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, as measured in the middle of the chamber. NO<inline-formula><mml:math id="M96" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentrations at the outlet of the chamber were monitored by a
chemiluminescence NO<inline-formula><mml:math id="M97" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> analyzer (ECOTECH, EC9841B). HCHO was generated
by thermolysis of paraformaldehyde at 70 <inline-formula><mml:math id="M98" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>C and detected via an
acetyl acetone spectrophotometric method using a UV–Vis spectrophotometer
(PERSEE, T6) or a fluorescence spectrophotometer (THERMO, Lumina), depending
on different initial HCHO concentrations. The particle size distribution was
measured by a scanning nanoparticle spectrometer (HCT, SNPS-20). Electron
spin resonance (Nuohai Life Science, MiniScope MS 5000) was used to measure
<inline-formula><mml:math id="M99" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH on the surface of the particles. A 5,5-dimethl-1-pyrroline-N-oxide
(DPMO, Enzo) was used as the capture agent. Fifty <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>L particle-containing
suspension mixed with 50 <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>L DMPO (concentration of 200 <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>M) was
loaded in a 1 mm capillary. Four 365 nm LED lamps were placed side by side,
vertically, at a distance of about 1 cm from the capillary, and the
measurement was carried out after 1 min of irradiation. The modulation
frequency was 100 kHz; the modulation amplitude was 0.2 mT; the microwave
power was 10 mW; and the sweep time was 60 s.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><?xmltex \opttitle{Nitrate--TiO${}_{{2}}$ composite samples}?><title>Nitrate–TiO<inline-formula><mml:math id="M103" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> composite samples</title>
      <p id="d1e1168">In our experiments, two nitrate salts – potassium nitrate (AR, Beijing
Chemical Works Co., Ltd) or ammonium nitrate (AR, Beijing Chemical Works
Co., Ltd) – were composited with pure TiO<inline-formula><mml:math id="M104" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (<inline-formula><mml:math id="M105" display="inline"><mml:mo lspace="0mm">≥</mml:mo></mml:math></inline-formula> 99.5 %, Degussa
AG) powder or TiO<inline-formula><mml:math id="M106" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (1 wt %) <inline-formula><mml:math id="M107" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<inline-formula><mml:math id="M108" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> mixed powder to prepare
NO<inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M110" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or NO<inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M112" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (1 wt %) <inline-formula><mml:math id="M113" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<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> samples; 250 mg TiO<inline-formula><mml:math id="M115" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was simply mixed in the nitrate solutions at the
desired mass mixing ratio (with nitrate content of 4 wt %) to obtain a
mash. The mash was dried at 90 <inline-formula><mml:math id="M116" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and then ground carefully for
30 min. A series of samples with different amounts of nitrate were prepared,
and diffuse reflectance Fourier transform infrared spectroscopy (DRIFTS)
measurements were made to test their homogeneity. Figure S2 shows the DRIFTS
spectra of these KNO<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M118" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> composites, of which the 1760 cm<inline-formula><mml:math id="M119" 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>
peak is one of the typical vibrating peaks of nitrate  (Aghazadeh, 2016;
Maeda et al., 2011). The ratio value of the peak area from 1730–1790 cm<inline-formula><mml:math id="M120" 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> for
1 wt %, 4 wt %, 32 wt %, 80 wt % composited samples is <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">4.1</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">29.8</mml:mn><mml:mo>:</mml:mo><mml:mn mathvariant="normal">81.6</mml:mn></mml:mrow></mml:math></inline-formula>, which is very
close to that of theoretical value, proving that the samples were uniformly
mixed. SiO<inline-formula><mml:math id="M122" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (AR, Xilong Scientific Co., Ltd.) with no optical
activity was also chosen for comparison, and samples of KNO<inline-formula><mml:math id="M123" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-SiO<inline-formula><mml:math id="M124" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
and KNO<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M126" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (1 wt %) <inline-formula><mml:math id="M127" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<inline-formula><mml:math id="M128" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples with a potassium
nitrate content of 4 wt % were prepared. The blank 250 mg TiO<inline-formula><mml:math id="M129" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
sample was solved in pure water, using the same procedure as mentioned above.
Four wt % HNO<inline-formula><mml:math id="M130" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M131" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> composite particles were prepared for
comparison. Concentrated nitric acid (AR, Beijing Chemical Works Co., Ltd)
was diluted to 1 M, and 250 mg TiO<inline-formula><mml:math id="M132" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was added to the nitric acid
solution and stirred evenly. A layer of aluminum foil was used to cover the
surface of the HNO<inline-formula><mml:math id="M133" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M134" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> homogenate, which was then dried naturally in the
room and then ground for use.  We also selected Arizona Test Dust (ATD,
Powder Technology Inc.), whose chemical composition and weight percentage
were shown in Table S1, as a substitute of NO<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M136" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> TiO<inline-formula><mml:math id="M137" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to
investigate the “photocatalytic renoxification” process of nitrate and the
positive effect of HCHO.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Environmental chamber experiments</title>
      <p id="d1e1506">For the chamber operation, we completely evacuated the chamber after every
experiment; we then cleaned the chamber walls with deionized water and dried them by flushing the chamber with ultra-zero air to remove any particles or
gases that had collected on the chamber walls. The experiments carried out in the
environmental chamber can be divided into two categories according to
whether HCHO was involved or not. (1) No HCHO involvement in the reaction.
The PVF bag was inflated by 260 L synthetic air, and then 75 mg particles
were instantly sprayed into the chamber by a transient high-pressure
airflow. As shown in Fig. S3, the particle number concentration of the
KNO<inline-formula><mml:math id="M138" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M139" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or TiO<inline-formula><mml:math id="M140" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples decreased rapidly owing to the wall
effect, including the possible electrostatic adsorption of the particles by
the environmental chamber. The size distributions of the KNO<inline-formula><mml:math id="M141" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M142" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
TiO<inline-formula><mml:math id="M143" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples were similar, with both becoming stable after about 60 min.
The peak number concentration was averaged between 3991 and 3886 particle cm<inline-formula><mml:math id="M144" 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> during the illumination period for the KNO<inline-formula><mml:math id="M145" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M146" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
TiO<inline-formula><mml:math id="M147" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples, respectively, indicating that the repeatability of the
introduction of particles into the chamber is good. This can be attributed
to the strict cleaning of the chamber and the same operation of each batch
experiment. (2) With the participation of HCHO. The PVF bag was inflated by
125 L synthetic air followed by the introduction of HCHO, and then the
chamber was filled up with zero air to about 250 L. In order to know the
HCHO adsorption before and after the particles' introduction, we conducted a
conditional experiment in the dark. It can be seen from Fig. S4 that it
took about 90 min for the concentration of HCHO to reach stability and be
sustained. Then, 75 mg TiO<inline-formula><mml:math id="M148" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> or NO<inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M150" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> TiO<inline-formula><mml:math id="M151" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> powders were
introduced instantly, and the concentration of HCHO decreased upon the
introduction. It took about 60 min for HCHO to reach its second adsorption
equilibrium and for the concentration of HCHO to remain stable for several hours
in the dark. Therefore, for the irradiation experiments, the particles were
injected at 90 min after HCHO's introduction, and the lamps were turned on
at 60 min after the particle's introduction.</p>
      <p id="d1e1641">To determine the background value of NO<inline-formula><mml:math id="M152" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the reaction system, four
blank experiments were carried out under illumination without nitrate:
“synthetic air”, “synthetic air <inline-formula><mml:math id="M153" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TiO<inline-formula><mml:math id="M154" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>”, “synthetic air <inline-formula><mml:math id="M155" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HCHO”, and “synthetic air <inline-formula><mml:math id="M156" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> HCHO <inline-formula><mml:math id="M157" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TiO<inline-formula><mml:math id="M158" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>”. In the blank
experiments of “synthetic air” and “synthetic air <inline-formula><mml:math id="M159" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> TiO<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>”, the
NO<inline-formula><mml:math id="M161" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration remained stable during 180 min illumination, and the
concentration change was no more than 0.5 ppb (Fig. S5a). Therefore, the
environmental chamber, the synthetic air, and the surface of TiO<inline-formula><mml:math id="M162" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles
were thought to be relatively clean, and there was no generation and
accumulation of NO<inline-formula><mml:math id="M163" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> under illumination. When HCHO was introduced into
the environmental chamber, NO<inline-formula><mml:math id="M164" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> accumulated <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> ppb in 120
min with or without TiO<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> particles (Fig. S5b). Compared with the
blank experiment results when there was no HCHO, NO<inline-formula><mml:math id="M167" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> might come from
the generation process of HCHO (impurities in paraformaldehyde). However,
considering the high concentration level of NO<inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> produced in the
NO<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<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> system containing HCHO under the same conditions in
this study (see later in Fig. 2), the NO<inline-formula><mml:math id="M171" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> generated in this blank
experiment can be negligible.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><?xmltex \opttitle{The positive effect of TiO${}_{{2}}$ on the renoxification process}?><title>The positive effect of TiO<inline-formula><mml:math id="M172" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the renoxification process</title>
      <p id="d1e1847">We investigated the photocatalytic role of TiO<inline-formula><mml:math id="M173" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on renoxification. The
light source was two 365 nm tube lamps containing small amounts of 400–600 nm visible light; this setup was suitable for exciting TiO<inline-formula><mml:math id="M174" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and the
photolysis of available nitrate radicals. Raw NO<inline-formula><mml:math id="M175" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> data measured in the
chamber under dark and illuminated conditions for 4 wt %
KNO<inline-formula><mml:math id="M176" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-SiO<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 4 wt % KNO<inline-formula><mml:math id="M178" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (1 wt %) <inline-formula><mml:math id="M180" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<inline-formula><mml:math id="M181" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
are shown in Fig. 1. The ratio of 1 wt % TiO<inline-formula><mml:math id="M182" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to SiO<inline-formula><mml:math id="M183" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
corresponds to their ratio in sand and dust particles. We observed no
NO<inline-formula><mml:math id="M184" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the KNO<inline-formula><mml:math id="M185" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-SiO<inline-formula><mml:math id="M186" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sample under darkness or illumination,
indicating very weak direct photolysis of nitrate under our 365 nm tube-lamp
illumination conditions. However, when the sample containing
TiO<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> <inline-formula><mml:math id="M188" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was illuminated, NO<inline-formula><mml:math id="M190" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> continually accumulated in the
chamber. This finding confirms that NO<inline-formula><mml:math id="M191" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production arising from
photodissociation of NO<inline-formula><mml:math id="M192" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on TiO<inline-formula><mml:math id="M193" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> <inline-formula><mml:math id="M194" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>,SiO<inline-formula><mml:math id="M195" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was caused by the
photocatalytic property of TiO<inline-formula><mml:math id="M196" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (i.e., photocatalytic renoxification)
and was not due to the direct photolysis of NO<inline-formula><mml:math id="M197" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (photolytic
renoxification).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e2081">Effect of illumination on the release of NO<inline-formula><mml:math id="M198" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> from 4 wt %
KNO<inline-formula><mml:math id="M199" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-SiO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 4 wt % KNO<inline-formula><mml:math id="M201" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M202" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>(1 wt %) <inline-formula><mml:math id="M203" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> SiO<inline-formula><mml:math id="M204" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
at 293 K and 0.8 % of relative humidity. 365 nm tube lamps were used
during the illumination experiments.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/11347/2022/acp-22-11347-2022-f01.png"/>

        </fig>

      <p id="d1e2152">TiO<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can be excited by UV illumination to generate electron-hole pairs,
and the h<inline-formula><mml:math id="M206" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> can react with adsorbed NO<inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to produce
NO<inline-formula><mml:math id="M208" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula> (Ndour et al., 2009). Thus, in the
present study, NO<inline-formula><mml:math id="M209" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> mainly absorbed visible light emitted
from the tube lamps, which was subsequently photolyzed to NO<inline-formula><mml:math id="M210" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>through
Eqs. (3) and (4) (Wayne et al., 1991), which explains
why NO<inline-formula><mml:math id="M211" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was observed in this study. Thus, we demonstrated that
TiO<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> can be excited at illumination wavelengths of <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">365</mml:mn></mml:mrow></mml:math></inline-formula> nm, even when then content was very low, and that NO<inline-formula><mml:math id="M214" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> accumulated due
to the production and further photolysis of NO<inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>. However,
the production rate of NO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was very slow, reaching only 1.3 ppb during
90 min of illumination. This result may have been caused by the blocking
effect of K<inline-formula><mml:math id="M217" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> on NO<inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. K<inline-formula><mml:math id="M219" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> forms ion pairs with
NO<inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, and electrostatic repulsion between K<inline-formula><mml:math id="M221" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and h<inline-formula><mml:math id="M222" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>
prevents NO<inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> from combining with h<inline-formula><mml:math id="M224" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> to generate
NO<inline-formula><mml:math id="M225" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula> to a certain extent, thereby weakening the positive
effect of TiO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> on the renoxification of KNO<inline-formula><mml:math id="M227" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>  (Rosseler et
al., 2013).

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M228" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E1"><mml:mtd><mml:mtext>1</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">TiO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">390</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:msup><mml:mi mathvariant="normal">e</mml:mi><mml:mo>-</mml:mo></mml:msup><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mo>+</mml:mo></mml:msup><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">640</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>(</mml:mo><mml:mn mathvariant="normal">585</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>&lt;</mml:mo><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">640</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">nm</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><?xmltex \opttitle{The synergistic positive effect of TiO${}_{{2}}$ and HCHO on the
renoxification process}?><title>The synergistic positive effect of TiO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HCHO on the
renoxification process</title>
      <p id="d1e2597">LED lamps with a wavelength range of 350–390 nm and no visible light were
used to irradiate 4 wt % KNO<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M231" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> without generating NO<inline-formula><mml:math id="M232" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
(NO<inline-formula><mml:math id="M233" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO concentrations fluctuate within the error range of the
instrument) (Fig. S5). TiO<inline-formula><mml:math id="M234" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can be excited under this range of
irradiation, producing NO<inline-formula><mml:math id="M235" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> radicals as discussed above. The lack of
NO<inline-formula><mml:math id="M236" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> generation indicates that neither nitrate photolysis nor
NO<inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> photolysis occurred under 365 nm LED lamp illumination
conditions. In addition, it has been shown that NO<inline-formula><mml:math id="M238" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>
photolysis only occurs in visible light  (Aldener et al.,
2006). Therefore, the LED lamp setup was used in subsequent experiments to
exclude the direct photolysis of both KNO<inline-formula><mml:math id="M239" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>
but to allow the excitation of TiO<inline-formula><mml:math id="M241" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. This approach allowed us to
investigate the process of photocatalytic renoxification caused by HCHO in
the presence of photogenerated NO<inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e2731">Atmospheric trace gases can undergo photocatalytic reactions on the surface
of TiO<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>  (Chen et al., 2012). As the illumination time increased,
the concentration of HCHO showed a linear downward trend, which was found to
fit zero-order reaction kinetics (Fig. S7). The zero-order reaction rate
constants of HCHO on TiO<inline-formula><mml:math id="M244" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 4 wt % KNO<inline-formula><mml:math id="M245" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M246" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles
were <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> ppm min<inline-formula><mml:math id="M249" 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>,
respectively, which were much higher than that for gaseous HCHO photolysis
(Shang et al., 2017). We suggested that the produced
NO<inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> contributed to the enhanced uptake of HCHO. In the
following study, the effect of HCHO on the photocatalytic renoxification of
NO<inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M252" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was explored.</p>
      <p id="d1e2852">The variation in NO<inline-formula><mml:math id="M253" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations within the chamber containing
nitrate–TiO<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> particles with or without HCHO is shown in Fig. 2. For 4 wt % KNO<inline-formula><mml:math id="M255" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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> particles, the NO<inline-formula><mml:math id="M257" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration began to
increase upon irradiation in the presence of HCHO, reaching <inline-formula><mml:math id="M258" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 3861 mmol normalized ppb (equivalent to 110 ppb) within 120 min. This result
indicates that HCHO greatly promoted photocatalytic renoxification of
KNO<inline-formula><mml:math id="M259" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> on the surfaces of TiO<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> particles. This reaction process can
be divided into two stages: a rapid increase within the first 60 min and a
slower increase within the following 60 min, each consistent with zero-orde
reaction kinetics. The slow stage is due to the photodegradation of HCHO on
KNO<inline-formula><mml:math id="M261" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M262" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> aerosols, which led to a decrease in its concentration,
gradually weakening the positive effect. NO<inline-formula><mml:math id="M263" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is the sum of 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> and
NO, both of which showed a two-stage concentration increase (Fig. S8). The
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> generation rate was nearly 6 times that of NO as compared to using
the zero-order rate constant within 60 min (1.18 ppb min<inline-formula><mml:math id="M266" 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="M267" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
<inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.96; 0.19 ppb min<inline-formula><mml:math id="M269" 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="M270" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 0.91). This burst-like
generation of NO<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> can be ascribed to the reaction between generated
NO<inline-formula><mml:math id="M272" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> and HCHO via hydrogen abstraction to form adsorbed
nitric acid (HNO<inline-formula><mml:math id="M273" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads)) on TiO<inline-formula><mml:math id="M274" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles. We measured the pH of
water extracts in NO<inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M276" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> systems with and without HCHO. It
was found that the pH decreased by 1.7 % for KNO<inline-formula><mml:math id="M277" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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>,
suggesting the formation of acidic species such as HNO<inline-formula><mml:math id="M279" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) in this
study. Based on the analysis of the absorption cross section of HNO<inline-formula><mml:math id="M280" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
adsorbed on the fused silica surface, the HNO<inline-formula><mml:math id="M281" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) absorption spectrum has
been reported to be red-shifted compared to HNO<inline-formula><mml:math id="M282" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(g), extending from 350
to 365 nm, with a simultaneous cross-sectional increase  (Du and Zhu,
2011). Therefore, HNO<inline-formula><mml:math id="M283" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) was subjected to photolysis to produce
NO<inline-formula><mml:math id="M284" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and HONO (Eqs. 6–8) under the LED lamp used in this study. A
previous study of HNO<inline-formula><mml:math id="M285" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> photolysis on the surface of Pyrex glass showed
that the ratio of the formation rates of photolysis products
<inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mi>J</mml:mi><mml:mrow><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>J</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:msub><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mi>x</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HONO</mml:mi></mml:mrow><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was <inline-formula><mml:math id="M287" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 97 % at RH <inline-formula><mml:math id="M288" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0 %
(Zhou et al., 2003), suggesting that NO<inline-formula><mml:math id="M289" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is the main
gaseous product under dry conditions. Thus, the effect of HONO on product
distribution and NO<inline-formula><mml:math id="M290" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration was negligible in this study.
Together, these results suggest that NO<inline-formula><mml:math id="M291" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>  and HCHO
generate HNO<inline-formula><mml:math id="M292" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) on particle surfaces through hydrogen abstraction,
which contributes to the substantial release of NO<inline-formula><mml:math id="M293" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> via photolysis.
This photocatalytic renoxification via the
NO<inline-formula><mml:math id="M294" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M295" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M296" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M297" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway is important
considering the high abundance of hydrogen donor organics in the atmosphere.

                <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M298" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E5"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HCHO</mml:mi></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">CHO</mml:mi></mml:mrow><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">HN</mml:mi></mml:mrow><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd><mml:mtext>6</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi>h</mml:mi><mml:mi mathvariant="italic">υ</mml:mi><mml:mo>→</mml:mo><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msup><mml:mo>]</mml:mo><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msup><mml:mo>]</mml:mo><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi mathvariant="normal">O</mml:mi><mml:msup><mml:mo>(</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mi mathvariant="normal">P</mml:mi><mml:mo>)</mml:mo><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E8"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>[</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msup><mml:mo>]</mml:mo><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo><mml:mo>→</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">ads</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e3527">Effect of formaldehyde on the renoxification processes of
different nitrate-doped particles at 293 K and 0.8 % of relative
humidity; 365 nm LED lamps were used during the illumination experiment. The
initial concentration of HCHO was about 9 ppm.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/11347/2022/acp-22-11347-2022-f02.png"/>

        </fig>

      <p id="d1e3536">To demonstrate the proposed HCHO mechanism and the photolysis contribution
of HNO<inline-formula><mml:math id="M299" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> to NO<inline-formula><mml:math id="M300" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, we prepared an HNO<inline-formula><mml:math id="M301" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M302" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> sample by
directly dissolving TiO<inline-formula><mml:math id="M303" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> into dilute nitric acid. The formation of
NO<inline-formula><mml:math id="M304" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> on HNO<inline-formula><mml:math id="M305" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M306" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> without HCHO under illumination was obvious
and at a rate comparable with that on KNO<inline-formula><mml:math id="M307" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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> with HCHO (Fig. 2). The renoxification of HNO<inline-formula><mml:math id="M309" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M310" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles was further enhanced
following the introduction of HCHO. This is because HNO<inline-formula><mml:math id="M311" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
dissociates on particle surfaces to generate NO<inline-formula><mml:math id="M312" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, such that
HNO<inline-formula><mml:math id="M313" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> exists on TiO<inline-formula><mml:math id="M314" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> as both HNO<inline-formula><mml:math id="M315" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) and
NO<inline-formula><mml:math id="M316" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>(ads). Similarly, NO<inline-formula><mml:math id="M317" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>(ads) completed the
NO<inline-formula><mml:math id="M318" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M319" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M320" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M321" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway, as described
above, through the reaction process shown in Eqs. (2) to (8). The rates of
NO<inline-formula><mml:math id="M322" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production from HNO<inline-formula><mml:math id="M323" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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> particles with and without HCHO
were similar for the first 60 min (Fig. 2), mainly due to the direct
photolysis of partial HNO<inline-formula><mml:math id="M325" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads). However, after 60 min, NO<inline-formula><mml:math id="M326" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was
generated rapidly in the presence of HCHO, perhaps due to the dominant
photocatalytic renoxification of NO<inline-formula><mml:math id="M327" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>(ads). These findings
indicate that HCHO converts NO<inline-formula><mml:math id="M328" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on particle surfaces into
HNO<inline-formula><mml:math id="M329" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) by reacting with NO<inline-formula><mml:math id="M330" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>, and then
HNO<inline-formula><mml:math id="M331" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) photolyzes at a faster rate to generate NO<inline-formula><mml:math id="M332" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, allowing
HCHO to enhance the formation of NO<inline-formula><mml:math id="M333" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Overall, the photocatalytic
renoxification of NO<inline-formula><mml:math id="M334" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<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> particles affects atmospheric
oxidation and the nitrogen cycle, and the presence of HCHO further enhances
this impact.</p>
      <p id="d1e3905">Photocatalytic renoxification reactions occur on the surfaces of mineral
dust due to the presence of semiconductor oxides with photocatalytic
activity such as TiO<inline-formula><mml:math id="M336" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>  (Ndour et al., 2009). In
order to confirm this, we synthesized nitrate with inert SiO<inline-formula><mml:math id="M337" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> as a
comparison. It can be seen from Fig. S9 that no NO<inline-formula><mml:math id="M338" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> formation was
observed regardless of whether or not HCHO was present, indicating that photocatalytically
active particle TiO<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> is critical to the photocatalytic renoxification
process. Furthermore, a kind of commercial mineral dust ATD was selected to
study the effects of HCHO on this process. We detected <inline-formula><mml:math id="M340" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH in
irradiated pure TiO<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> and ATD samples using the electron spin resonance
(ESR) technique and found that, for ATD samples, the peak intensity of
<inline-formula><mml:math id="M342" display="inline"><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:math></inline-formula>OH generation was 40 % that of TiO<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> samples (Fig. S10).
<inline-formula><mml:math id="M344" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH originates in the reaction of h<inline-formula><mml:math id="M345" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> with surface-adsorbed
water (Ahmed et al., 2014). ATD contains semiconductor oxides
such as TiO<inline-formula><mml:math id="M346" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and Fe<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>O<inline-formula><mml:math id="M348" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and is thought to exhibit
photocatalytic properties affecting the renoxification of nitrate. The
NO<inline-formula><mml:math id="M349" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> content of ATD is <inline-formula><mml:math id="M350" display="inline"><mml:mrow><mml:mn mathvariant="normal">4</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">17</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molecules m<inline-formula><mml:math id="M351" 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="M352" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.25 wt % of the total mass
(Huang et al., 2015; Park et al., 2017). The NO<inline-formula><mml:math id="M353" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentration changes observed in the environmental chamber demonstrated
that HCHO promoted the renoxification of ATD particles (Fig. S11). This
result suggests that mineral dust containing photocatalytic semiconductor
oxides such as TiO<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>, Fe<inline-formula><mml:math id="M355" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M356" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and ZnO can greatly promote the
conversion of granular nitrate to NO<inline-formula><mml:math id="M357" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the presence of HCHO.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Influential factors on the photocatalytic renoxification process</title>
<sec id="Ch1.S3.SS3.SSS1">
  <label>3.3.1</label><title>The influence of nitrate type</title>
      <p id="d1e4128">As discussed above, HNO<inline-formula><mml:math id="M358" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> and KNO<inline-formula><mml:math id="M359" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> undergo different renoxification
processes on the surface of TiO<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> under the same illumination
conditions, suggesting that cations bound to NO<inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> significantly
affect NO<inline-formula><mml:math id="M362" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production. Different types of cations coexist with nitrate
ions in atmospheric particulate matter, among which ammonium ions
(NH<inline-formula><mml:math id="M363" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) are important water-soluble ions that can be higher in
content than K<inline-formula><mml:math id="M364" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> in urban fine particulate matter  (Zhou et al., 2016;
Tang et al., 2021; Wang et al., 2021), especially in heavily polluted
cities (Tian et al., 2020). Equal amounts of 4 wt %
NH<inline-formula><mml:math id="M365" 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="M366" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M367" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles were introduced into the chamber and
illuminated under the same conditions. Similar to Fig. 2, millimole
normalized ppb was used in order to compare the amount of NO<inline-formula><mml:math id="M368" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> released
for different kinds of nitrate with the same percentage weight. It can be seen
that HCHO had a much stronger positive effect on the release of NO<inline-formula><mml:math id="M369" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
over NH<inline-formula><mml:math id="M370" 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="M371" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M372" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles (Fig. 3), which may be
ascribed to NH<inline-formula><mml:math id="M373" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. Combined with the results of
NH<inline-formula><mml:math id="M374" 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="M375" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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> and KNO<inline-formula><mml:math id="M377" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M378" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles, it seems
that the affinity rather than electrostatic repulsion should be the primary
effect of cations on the production of NO<inline-formula><mml:math id="M379" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. On substrates without
photocatalytic activity, such as SiO<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> and Al<inline-formula><mml:math id="M381" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M382" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>,
NH<inline-formula><mml:math id="M383" 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="M384" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> cannot generate NO<inline-formula><mml:math id="M385" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, such that NO<inline-formula><mml:math id="M386" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production
depends on the effect of TiO<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> (Ma et al., 2021). The h<inline-formula><mml:math id="M388" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>
generated by TiO<inline-formula><mml:math id="M389" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> excitation reacts with adsorbed H<inline-formula><mml:math id="M390" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O to produce
<inline-formula><mml:math id="M391" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH (Eq. 9), which gradually oxidizes NH<inline-formula><mml:math id="M392" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> to
NO<inline-formula><mml:math id="M393" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> (Eq. 10). In our previous study, we demonstrated that
irradiated (NH<inline-formula><mml:math id="M394" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>SO<inline-formula><mml:math id="M395" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M396" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> samples had lower
NH<inline-formula><mml:math id="M397" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and NO<inline-formula><mml:math id="M398" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> peaks  (Shang et al., 2017).
Therefore, more NO<inline-formula><mml:math id="M399" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> participated in the photocatalytic
renoxification process via the NO<inline-formula><mml:math id="M400" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M401" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M402" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M403" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway to generate NO<inline-formula><mml:math id="M404" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Moreover, the results
without HCHO are shown in Fig. S12. Both NH<inline-formula><mml:math id="M405" 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="M406" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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>
particles and KNO<inline-formula><mml:math id="M408" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M409" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles produced almost no
NO<inline-formula><mml:math id="M410" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, indicating the importance of HCHO for renoxification to occur. Due
to the high content of NH<inline-formula><mml:math id="M411" 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="M412" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> in atmospheric particulate matter,
the positive effect of HCHO on the photocatalytic renoxification process may
have some impact on the concentrations of NO<inline-formula><mml:math id="M413" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and other atmospheric
oxidants.

                  <disp-formula specific-use="gather" content-type="numbered"><mml:math id="M414" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E9"><mml:mtd><mml:mtext>9</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mo>+</mml:mo></mml:msup><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:mo>→</mml:mo><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E10"><mml:mtd><mml:mtext>10</mml:mtext></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi><mml:mi mathvariant="normal">OH</mml:mi><mml:mo>+</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>→</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>→</mml:mo><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e4762">Effect of formaldehyde on the renoxification processes of 4 wt % NH<inline-formula><mml:math id="M415" 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="M416" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M417" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 4 wt % KNO<inline-formula><mml:math id="M418" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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>
particles at 293 K and 0.8 % of relative humidity; 365 nm LED lamps were
used during the irradiation experiment. The initial concentration of HCHO
was about 9 ppm.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/11347/2022/acp-22-11347-2022-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="d1e4818">Effect of relative humidity on the release of NO<inline-formula><mml:math id="M420" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> <bold>(a)</bold>,
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> <bold>(b)</bold>, NO <bold>(c)</bold> over 4 wt % NH<inline-formula><mml:math id="M422" 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="M423" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M424" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 4 wt % KNO<inline-formula><mml:math id="M425" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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> particles at 293 K; 365 nm LED lamps were used
during the illumination experiment. The initial concentration of HCHO was
about 9 ppm.</p></caption>
            <?xmltex \igopts{width=483.69685pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/11347/2022/acp-22-11347-2022-f04.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <label>3.3.2</label><title>The influence of relative humidity</title>
      <p id="d1e4908">Water on particle surfaces can participate directly in the heterogeneous
reaction process. As shown in Eq. (9), H<inline-formula><mml:math id="M427" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O can be captured by h<inline-formula><mml:math id="M428" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>
to generate <inline-formula><mml:math id="M429" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH with strong oxidizability in photocatalytic
reactions. The first-order photolysis rate constant of NO<inline-formula><mml:math id="M430" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> on
TiO<inline-formula><mml:math id="M431" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles decreases by an order of magnitude from (<inline-formula><mml:math id="M432" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula>) <inline-formula><mml:math id="M433" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M434" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M435" 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> on dry surfaces to (<inline-formula><mml:math id="M436" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn></mml:mrow></mml:math></inline-formula>)
<inline-formula><mml:math id="M437" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M438" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M439" 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> when nitrate is coadsorbed with water above
monolayer coverage (Ostaszewski et al.,
2018). We explored the positive effect of HCHO on the
NO<inline-formula><mml:math id="M440" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M441" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particle photocatalytic renoxification at different
RH levels; the results are shown in Fig. 4a. For KNO<inline-formula><mml:math id="M442" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<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>
particles, the rate of NO<inline-formula><mml:math id="M444" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> production decreased as the RH of the
environmental chamber increased, indicating that increased water content in
the gas phase hindered photocatalytic renoxification for two reasons:
H<inline-formula><mml:math id="M445" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O competes with NO<inline-formula><mml:math id="M446" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> for h<inline-formula><mml:math id="M447" display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> on the surface of
TiO<inline-formula><mml:math id="M448" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to generate <inline-formula><mml:math id="M449" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH, reducing the generation of
NO<inline-formula><mml:math id="M450" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>, and competitive adsorption between H<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>O and HCHO
causes the generated <inline-formula><mml:math id="M452" display="inline"><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:math></inline-formula>OH to compete with NO<inline-formula><mml:math id="M453" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> for
HCHO, hindering the formation of HNO<inline-formula><mml:math id="M454" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) on particle surfaces.
Moreover, it is also possible that the loss of NO<inline-formula><mml:math id="M455" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> on the wall
increases under high humidity conditions, resulting in a decrease in its
concentration. This competitive process also occurs on the surface of
NH<inline-formula><mml:math id="M456" 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="M457" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M458" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles, but at RH <inline-formula><mml:math id="M459" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 70 %, the NO<inline-formula><mml:math id="M460" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
generation rate constant is slightly higher. The deliquescent humidity of
NH<inline-formula><mml:math id="M461" 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="M462" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> at 298 K is <inline-formula><mml:math id="M463" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 62 %, such that
NH<inline-formula><mml:math id="M464" 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="M465" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> had already deliquesced at RH <inline-formula><mml:math id="M466" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 70 %, forming an
NH<inline-formula><mml:math id="M467" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M468" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NH<inline-formula><mml:math id="M469" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>-NO<inline-formula><mml:math id="M470" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> liquid system on the particle
surfaces. This quasi-liquid phase improved the dispersion of TiO<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> in
NH<inline-formula><mml:math id="M472" 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="M473" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, resulting in greater NO<inline-formula><mml:math id="M474" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> release. The deliquescent
humidity of KNO<inline-formula><mml:math id="M475" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M476" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was <inline-formula><mml:math id="M477" display="inline"><mml:mi mathvariant="italic">&gt;</mml:mi></mml:math></inline-formula> 90 % (2009), such that
no phase change occurred at RH <inline-formula><mml:math id="M478" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 70 %, and the renoxification reaction
rate retained a downward trend. In the presence of H<inline-formula><mml:math id="M479" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O, in addition to
the NO<inline-formula><mml:math id="M480" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>-NO<inline-formula><mml:math id="M481" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>-HNO<inline-formula><mml:math id="M482" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> pathway observed in this
study, there are a variety of HNO<inline-formula><mml:math id="M483" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> generation paths, such as the
hydrolysis of N<inline-formula><mml:math id="M484" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M485" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula> via the NO<inline-formula><mml:math id="M486" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>-N<inline-formula><mml:math id="M487" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M488" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>-HNO<inline-formula><mml:math id="M489" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
pathway (Brown et al., 2005), the oxidation of
NO<inline-formula><mml:math id="M490" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> by <inline-formula><mml:math id="M491" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH  (Burkholder et al., 1993), and the
reaction of NO<inline-formula><mml:math id="M492" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula> with H<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>O  (Schutze and Herrmann,
2005), all of which require further consideration and study.</p>

      <?xmltex \floatpos{h!}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e5551">Positive role of HCHO on the photocatalytic renoxification of
nitrate–TiO<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> composite particles via the
NO<inline-formula><mml:math id="M495" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M496" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M497" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M498" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/22/11347/2022/acp-22-11347-2022-f05.png"/>

          </fig>

      <p id="d1e5611">The formation rates of NO 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> are shown in Fig. 4b and c,
respectively. 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> was the main product of surface HNO<inline-formula><mml:math id="M501" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> photolysis.
Under humid conditions, generated 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>(ads) continued to react with
H<inline-formula><mml:math id="M503" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O adsorbed on the surface to form HONO(ads). HONO was desorbed from
the surface and released into the gas phase  (Zhou et al., 2003; Bao et
al., 2018; Pandit et al., 2021), providing gaseous HONO to the reaction
system. Because the NO<inline-formula><mml:math id="M504" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration remained high, the effect of HONO
on NO<inline-formula><mml:math id="M505" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> analyzer results was negligible (Shi et al., 2021).
As NO<inline-formula><mml:math id="M506" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> can form NO<inline-formula><mml:math id="M507" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> with e<inline-formula><mml:math id="M508" display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, a reverse reaction also
occurred between NO<inline-formula><mml:math id="M509" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and HONO in the presence of H<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>O  (Ma
et al., 2021; Garcia et al., 2021). Therefore, the increase in H<inline-formula><mml:math id="M511" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O
increased the proportion of HONO in the nitrogen-containing products, such
that the NO<inline-formula><mml:math id="M512" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> generation rate decreased as RH increased. Comparing
Fig. 4b and c shows that, as RH increased, the NO production rate constant
decreased more than that 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>. HONO and 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> generated by the
photolysis of HNO<inline-formula><mml:math id="M515" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>(ads) decreased accordingly, i.e., the NO source
decreased. However, generated 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 NO underwent photocatalytic
oxidation on the surface of TiO<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>, and NO photodegradation was more
significant under the same conditions  (Hot et al., 2017).
Generally, a certain amount of HONO will be generated during the reaction
between HCHO and NO<inline-formula><mml:math id="M518" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<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> particles when RH is high, which
affects the concentrations of atmospheric <inline-formula><mml:math id="M520" display="inline"><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:math></inline-formula>OH, NO<inline-formula><mml:math id="M521" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, and
O<inline-formula><mml:math id="M522" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. This process is more likely to occur in summer due to high RH and
light intensity affecting atmospheric oxidation. In drier winters or dusty
weather, when TiO<inline-formula><mml:math id="M523" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> content is high, HCHO greatly promotes the
photocatalytic renoxification of NO<inline-formula><mml:math id="M524" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M525" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles, thereby
releasing more NO<inline-formula><mml:math id="M526" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> into the atmosphere, affecting the global
atmospheric nitrogen budget. Thus, regardless of the seasonal and regional
changes, renoxification has significant practical importance.</p>
</sec>
<sec id="Ch1.S3.SS3.SSS3">
  <label>3.3.3</label><title>The influence of initial HCHO concentrations</title>
      <p id="d1e5888">To explore whether HCHO promotes nitrate renoxification at natural
concentration levels, we reduced the initial concentration of HCHO in the
environmental chamber by a factor of 10 to <inline-formula><mml:math id="M527" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 1.0 ppm. The
positive effect of HCHO on the photocatalytic renoxification of
KNO<inline-formula><mml:math id="M528" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M529" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles was clearly weakened, with the 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>
concentration first increasing and then decreasing, and the NO concentration
remaining stable (Fig. S13). The HCHO concentration decreased due to its
consumption during the reaction, making its positive effect decline quickly.
The photocatalytic oxidation reaction between NO<inline-formula><mml:math id="M531" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and photogenerated
reactive oxygen species (ROS) on the TiO<inline-formula><mml:math id="M532" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> surface further decreased the
NO<inline-formula><mml:math id="M533" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentration. Photocatalytic oxidation of NO<inline-formula><mml:math id="M534" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> by ROS on
TiO<inline-formula><mml:math id="M535" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles occurred at an HCHO concentration of 9 ppm, but the
positive effect of HCHO remained dominant. Thus, no decrease in NO<inline-formula><mml:math id="M536" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentration was observed within 120 min in our experiments.</p>
      <p id="d1e5980">The concentration of HCHO in the atmosphere is relatively low, with a
balance between the photocatalytic oxidation decay of NO<inline-formula><mml:math id="M537" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and the
release of NO<inline-formula><mml:math id="M538" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> via photocatalytic renoxification. The mutual
transformation between particulate NO<inline-formula><mml:math id="M539" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and gaseous NO<inline-formula><mml:math id="M540" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> is
more complex. The effect of low-concentration HCHO on the renoxification of
NO<inline-formula><mml:math id="M541" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–TiO<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> particles requires further investigation. However,
many types of organics provide hydrogen atoms in the atmosphere, including
alkanes (e.g., methane and n-hexane), aldehydes (e.g., acetaldehyde),
alcohols (e.g., methanol and ethanol), and aromatic compounds (e.g., phenol)
that react with NO<inline-formula><mml:math id="M543" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula> to produce nitric acid   (Atkinson,
1991). These organics, together with HCHO, play similar positive roles in
photocatalytic renoxification and, therefore, influence NO<inline-formula><mml:math id="M544" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentrations.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Atmospheric implications</title>
      <p id="d1e6075">Nitric acid and nitrate are not only the final sink of NO<inline-formula><mml:math id="M545" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> in the
atmosphere but are also among its important sources. NO<inline-formula><mml:math id="M546" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> generated from nitrate through renoxification is easily overlooked. The renoxification of nitrate
on the surface of TiO<inline-formula><mml:math id="M547" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles can be divided into photolytic
renoxification and photocatalytic renoxification. The photocatalytic
performance of TiO<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> promotes the renoxification process, which explains
the influence of semiconducting metal oxide components on atmospheric
mineral particles during the renoxification of nitrate. Although most
previous studies have focused on solid-phase nitrate renoxification, our
exploration of the roles of HCHO in this study will allow us to examine
complex real-world pollution scenarios, in which multiple atmospheric
pollutants coexist, as well as the effects of organic pollutants on the
renoxification process. Atmospheric HCHO is taken up at the surface of
particulate matter, accounting for up to <inline-formula><mml:math id="M549" display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50 % of its
absorption (Li et al., 2014), such that the heterogeneous participation
of HCHO during renoxification is important. This study is the first to
report that HCHO has a positive effect on the photocatalytic renoxification
of nitrate on TiO<inline-formula><mml:math id="M550" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles via the
NO<inline-formula><mml:math id="M551" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M552" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M553" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M554" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway (Fig. 5),
further increasing the release of NO<inline-formula><mml:math id="M555" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and other nitrogen-containing
active species, which in turn affects the photochemical cycle of HO<inline-formula><mml:math id="M556" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
radicals in the atmosphere and the formation of important atmospheric
oxidants such as O<inline-formula><mml:math id="M557" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>. Although the response to the real situation will be biased in the case of high concentrations of
HCHO, as in our experiment,
the results of this study illustrate a possible way in which HCHO influences
nitrate renoxification in the atmosphere. Factors such as particulate matter
composition, RH, and initial HCHO concentration all influence the positive
effect of HCHO; notably, H<inline-formula><mml:math id="M558" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O competes with NO<inline-formula><mml:math id="M559" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> for
photogenerated holes. Based on these findings, two balance systems should be
explored in depth: the influence of RH on the generation rates of HONO and
NO<inline-formula><mml:math id="M560" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, as water increases the proportion of HONO in nitrogen-containing
products; and the balance between the photocatalytic degradation of
generated NO<inline-formula><mml:math id="M561" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> on TiO<inline-formula><mml:math id="M562" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> particles and the positive effect of HCHO on
NO<inline-formula><mml:math id="M563" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> generation at low HCHO concentrations.</p>
      <p id="d1e6259">Based on our results, we conclude that, in photochemical processes on the
surfaces of particles containing semiconductor oxides, with the
participation of hydrogen donor organics, a significant synergistic
photocatalytic renoxification enhancement effect could alter the composition
of surface nitrogenous species via the NO<inline-formula><mml:math id="M564" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>–NO<inline-formula><mml:math id="M565" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:mrow></mml:math></inline-formula>–HNO<inline-formula><mml:math id="M566" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–NO<inline-formula><mml:math id="M567" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> pathway, thereby affecting atmospheric oxidation and
nitrogen cycling. The positive effect of HCHO can be extended from TiO<inline-formula><mml:math id="M568" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
in this study to other components of mineral dust, such as Fe<inline-formula><mml:math id="M569" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M570" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
and ZnO with photocatalytic activity, which may have practical applications.
Our proposed reaction mechanism by which HCHO promotes photocatalytic
renoxification could improve existing atmospheric chemistry models and
reduce discrepancies between model simulations and field observations.</p>
</sec>

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

      <p id="d1e6337">All data are available upon request from the corresponding authors:
shangjing@pku.edu.cn.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e6340">Detailed information of Figs. S1–S13 (which include the spectra of the
lamps, size distribution of 4 wt % KNO<inline-formula><mml:math id="M571" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>–TiO<inline-formula><mml:math id="M572" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and TiO<inline-formula><mml:math id="M573" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
particles, changes in HCHO concentrations in the environmental chamber,
changes in NO<inline-formula><mml:math id="M574" display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> concentrations under different reaction conditions,
photodegradation curve of HCHO, and ESR spectra of TiO<inline-formula><mml:math id="M575" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and ATD particles)
and Table S1 (which demonstrates ATD chemical composition). The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-22-11347-2022-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-22-11347-2022-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e6394">YL and JS prepared the paper with contributions from other co-authors. JS
and XW designed the experiments and carried them out. YL, XW and WX prepared the supplement. YL, JS, MS and CY discussed the results. JS
and YL revised the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e6400">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="d1e6406">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="d1e6412">The authors are grateful for the financial support provided by National
Natural Science Foundation of China (nos. 21876003, 41961134034 and
21277004), the Second Tibetan Plateau Scientific Expedition and Research
(no. 2019QZKK0607).</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e6417">This research has been supported by the National Natural Science Foundation of China (grant nos. 21876003, 41961134034, and 21277004) and the Second Tibetan Plateau Scientific Expedition and Research (grant no. 2019QZKK0607).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e6423">This paper was edited by Ryan Sullivan and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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