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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-20-5425-2020</article-id><title-group><article-title>Origin and transformation of ambient volatile
organic compounds <?xmltex \hack{\break}?>during a dust-to-haze
episode in northwest China</article-title><alt-title>Transformation of VOCs during windblown dust-to-haze pollution episode</alt-title>
      </title-group><?xmltex \runningtitle{Transformation of VOCs during windblown dust-to-haze pollution episode}?><?xmltex \runningauthor{Y.~Xue~et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3 aff4">
          <name><surname>Xue</surname><given-names>Yonggang</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3 aff4">
          <name><surname>Huang</surname><given-names>Yu</given-names></name>
          <email>huangyu@ieecas.cn</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff5">
          <name><surname>Ho</surname><given-names>Steven Sai Hang</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4877-5994</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3 aff4">
          <name><surname>Chen</surname><given-names>Long</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3 aff4">
          <name><surname>Wang</surname><given-names>Liqin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6">
          <name><surname>Lee</surname><given-names>Shuncheng</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2 aff3 aff4">
          <name><surname>Cao</surname><given-names>Junji</given-names></name>
          <email>cao@loess.llqg.ac.cn</email>
        </contrib>
        <aff id="aff1"><label>1</label><institution>Key Lab of Aerosol Chemistry &amp; Physics, Institute of Earth
Environment, Chinese Academy of Sciences,<?xmltex \hack{\break}?> Xi'an 710061, China</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>State Key Lab of Loess and Quaternary Geology (SKLLQG), Institute of Earth Environment, <?xmltex \hack{\break}?>Chinese Academy of Sciences, Xi'an 710061, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Shaanxi Key Laboratory of Atmospheric and Haze-fog Pollution
Prevention, Institute of Earth Environment,<?xmltex \hack{\break}?> Chinese Academy of Sciences,
Xi'an 710061, China</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>CAS Center for Excellence in Quaternary Science and Global Change,
Xi'an 710061, China</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Division of Atmospheric Sciences, Desert Research Institute, Reno,
Nevada, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Department of Civil and Environmental Engineering, The Hong Kong
Polytechnic University,<?xmltex \hack{\break}?> Hung Hom, Hong Kong SAR, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Yu Huang (huangyu@ieecas.cn) and Junji Cao (cao@loess.llqg.ac.cn)</corresp></author-notes><pub-date><day>8</day><month>May</month><year>2020</year></pub-date>
      
      <volume>20</volume>
      <issue>9</issue>
      <fpage>5425</fpage><lpage>5436</lpage>
      <history>
        <date date-type="received"><day>25</day><month>October</month><year>2019</year></date>
           <date date-type="rev-request"><day>10</day><month>December</month><year>2019</year></date>
           <date date-type="rev-recd"><day>26</day><month>March</month><year>2020</year></date>
           <date date-type="accepted"><day>3</day><month>April</month><year>2020</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2020 </copyright-statement>
        <copyright-year>2020</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="d1e181">The high contribution of secondary organic aerosol to the
loading of fine particle pollution in China highlights the roles of volatile
organic compound (VOC) oxidation. In this respect, particulate active metallic
oxides in dust, like <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">TiO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula> ions, were proposed to influence the photochemical reactions of ambient VOCs. A case study was conducted at an urban site in Xi'an, northwest China, to investigate the origin and transformation of VOCs during a windblown dust-to-haze pollution episode, and the assumption that dust would enhance the oxidation of VOCs was
verified. Local vehicle exhaust (25 %) and biomass burning (18 %) were found to be the two largest contributors to ambient VOCs. In the dust
pollution period, a sharp decrease in the loading of VOCs and the aging of their
components were observed. Simultaneously, the secondary oxygenated VOC
fraction (i.e., methylglyoxal) increased. Source strength, physical
dispersion, and regional transport were eliminated as major factors for
the variation of ambient VOCs. In another aspect, about a 2- to 3-fold
increase in the loading of iron (<inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula>) and titanium (<inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula>) was found in the airborne particles, together with a fast decrease in <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios, which demonstrated that dust can accelerate the oxidation of ambient VOCs and the formation of secondary organic aerosol (SOA) precursors.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e235">Secondary aerosols are important components of fine particles in China, which could contribute to about 30 % to 77 % of PM<inline-formula><mml:math id="M5" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> loading; in this respect, secondary organic aerosols (SOAs) take about half of the loading (Huang et al., 2014). Guo et al. (2014) believed that gaseous emissions of volatile organic compounds (VOCs) and nitrogen oxides (<inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) were responsible for the large secondary PM formation. OH-initiated oxidation of <inline-formula><mml:math id="M7" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>-xylene was found to cause the coating thickness of black carbon, which further induced the increase in particle size (1.5 to 10.4 times) and effective density (from 0.43 to 1.45 g cm<inline-formula><mml:math id="M8" 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>) (Guo et al., 2016).</p>
      <p id="d1e277">Solid–gas heterogeneous reactions would cause the transformation of gaseous
pollutants and change the property of particles (Zhang et al., 2000, 2003; He et al., 2014). Recently, the oxidation of organic and inorganic gas on particle surfaces through the transition-metal-catalyzed chain reaction was frequently found to play an important role on the<?pagebreak page5426?> transformation of ambient gas pollutants (Chu et al., 2019). Mineral dust is one of the most important sources of transition metals, like iron (<inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula>) and titanium (<inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula>), in the natural environment (Chen et al., 2012). In addition, mineral dust is one kind of the most abundant components of global airborne PM, and about 1600 to 2000 Tg of mineral dust is transformed into aerosols annually from major deserts (Ginoux et al., 2001). Furthermore, the surface of mineral dust provides plenty of reactive sites for multiple atmospheric trace gas reactions (Cwiertny et al., 2008). As a result, dust
is considered to serve as a catalyst for reactive gases and to modify the
photochemical processes (Dentener et al., 1996; Dickerson et al., 1997).</p>
      <p id="d1e296">With the controlled experiment of sulfate formation on mineral dust, Zhang
et al. (2019) found that under appropriate humidity and particle acidity,
a surface transition-metal-catalyzed chain reaction together with nitrate
would greatly accelerate the sulfate's formation on the surface of mineral
dust (Zhang et al., 2019). In another aspect, solid–gas heterogeneous
photochemical reactions of organic compounds were also reported on the
illuminated surface of semiconductor metal oxides in the natural
environment, in particular <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">TiO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Chen et al., 2012). Co-existent
heterogeneous photochemical reactions of <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and VOCs on the surface of mineral dust were investigated in recent years. Both synergistic and suppressing effects of VOCs on the formation of sulfate were found, which indicated the competition of reactive oxygen species and active sites between VOCs and inorganic gas pollutants (Chu et al., 2019; Song et al., 2019). In addition, oxidized products, like formate and acetate species,
were observed in the coexistence reaction, which highlights the possibility
of further oxidation of VOCs on the mineral dust (He et al., 2014). In
northwest China, dust from both local sources and long-range transport is
one of the most important components of particulate matter of <inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">2.5</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M15" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> in diameter (PM<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>) (Huang et al., 2014). Xi'an has a population of <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> million (Feng et al., 2016). The sharp
increase in vehicles and other human activities has led to high emissions of
VOCs and <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (Li et al., 2017). Observations showing simultaneous high dust loading and elevated concentrations  of VOCs and <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> suggest possible impacts from heterogeneous reactions on dust particles (Huang et al., 2014; Li et al., 2017). The present study was conducted to investigate the origin and transformation of ambient VOCs during a severe dust-to-haze episode in winter. The transformation and the related chemical processing of
ambient VOCs and the related changes in the composition of PM<inline-formula><mml:math id="M20" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> were
studied within a typical windblown dust-to-haze episode. The potential
pathway of VOC oxidation in the windblown dust-to-haze formation process
was explored.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Materials and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Sampling site</title>
      <p id="d1e418">An observation site (109<inline-formula><mml:math id="M21" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>00<inline-formula><mml:math id="M22" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>7<inline-formula><mml:math id="M23" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> E, 34<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>13<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>22<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N) managed by Xi'an Jiaotong University was used in this study
(Fig. 1). All sampling equipment was deployed on the rooftop of a 15 m
tall academic building. No obvious stationary pollution sources were found
nearby, and the location can be considered as a typical urban location in
Xi'an (Q. Zhang et al., 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e484">Regional and local maps of the study area: <bold>(a)</bold> regional map
showing the location of Xi'an and the surrounding geography; <bold>(b)</bold> local map of Xi'an showing the sampling site (blue dot), main roads (red lines), and secondary roads (blue lines).</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Field sampling</title>
      <p id="d1e507">A severe dust-to-haze episode was observed in Xi'an and the surrounding areas
from 8 to 13 November 2016, and samples were continuously collected during this period to investigate the chemical compositions of both VOCs and fine PM. A total of 57 non-methane VOC species (i.e., <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> saturated and unsaturated aliphatic and aromatic VOCs) were sampled hourly into offline multi-bed adsorbent tubes; the measured 57 VOCs were defined as VOC<inline-formula><mml:math id="M28" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PAMS</mml:mi></mml:msub></mml:math></inline-formula>. The loaded tubes were analyzed using a thermal
desorption and gas chromatography/mass spectrometry (TD-GC/MS) method. In
previous developmental work, humidity and temperature during sampling were
found to significantly impact the analyses; for this study, all sample
collections were made under optimized conditions (Ho et al., 2017, 2018). Sixteen airborne carbonyls (including mono- and dicarbonyls)
were collected over diurnal cycles (i.e., 20:00–08:00 and
08:00–20:00 local time, LT) by 2,4-dinitrophenylhydrazine (DNPH) coated cartridges. Detailed sampling and analytical procedures for VOCs and carbonyls can be found in previous publications (Ho et al., 2017; Dai et al., 2012).</p>
      <p id="d1e537">PM<inline-formula><mml:math id="M29" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> filter samples were sampled with mini-volume samplers (model
MiniVol, Airmetrics Co., Oregon, USA) by an overline flow rate of 5 L min<inline-formula><mml:math id="M30" 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>
(Cao et al., 2005). Fine PM was sampled with 47 mm quartz microfiber filters
(Whatman QM-A, Maidstone, UK), and the filters were pre-heated at
900 <inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C for 3 h before sampling. The loaded filters were transferred
into clean polystyrene petri dishes and stored in a freezer.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Chemical analyses</title>
      <?pagebreak page5427?><p id="d1e578">Analytical procedures for VOC analysis have been described previously (Ho et
al., 2017). In brief, the analytes in the adsorbent tubes were firstly
desorbed in a thermal desorption unit (Series 2 UNITY-xr system with
ULTRA-xr, Markes International Ltd., UK) coupled to a GC/MS (7890A/5977B,
Agilent Technologies, Santa Clara, CA, USA). The loaded tubes were transferred
into the TD unit and blown with ultra-high purity He gas. The targeted VOCs
were desorbed at 330 <inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C within 8 min and then refocused onto a
cryogenic trap (U-T1703P-2S, Markes) at <inline-formula><mml:math id="M33" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">15</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The targeted
VOCs were transferred to a cold GC capillary column head (Rtx<sup>®</sup>-1, <inline-formula><mml:math id="M35" display="inline"><mml:mrow><mml:mn mathvariant="normal">105</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.25</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow><mml:mo>×</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> film thickness, Restek Corporation, USA) at <inline-formula><mml:math id="M36" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">45</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The chromatographic condition can be found in our previous work (Ho et al., 2017).</p>
      <p id="d1e660">For carbonyl compounds, the DNPH cartridges were firstly eluted with
acetonitrile (HPLC/GCMS grade, J &amp; K Scientific Ltd., Ontario, Canada)
(Dai et al., 2012). The extracts were analyzed with a typical high-pressure
liquid chromatography (HPLC) system (Series 1200; Agilent Technologies)
equipped with photodiode array detector. The column was matched with a <inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.6</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">250</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mrow class="unit"><mml:mi mathvariant="normal">mm</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> Spheri-5 ODS 5 <inline-formula><mml:math id="M39" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> C-18 reversed-phase column (Perkin-Elmer Corp., Norwalk, CT) (Dai et al., 2012; Ho et al., 2011).</p>
      <p id="d1e689">The particulate organic carbon (OC) and elementary carbon (EC) were analyzed
with a DRI model 2001 carbon analyzer (Atmoslytic, Inc., Calabasas, CA, USA)
(Chow et al., 2007, 1993). Anions (<inline-formula><mml:math id="M40" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M41" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M42" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>) and cations (<inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Na</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NH</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="M45" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M46" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Mg</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Ca</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) in particles were determined in aqueous extracts of the sample filters. Detailed extraction and analytical procedures were presented in a previous publication (Zhang et al., 2011). The abundances of 25 particulate elements (<inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Na</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Mg</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M50" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Al</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Si</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">S</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Cl</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">K</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ca</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sc</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M58" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">V</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Cr</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Mn</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M61" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Co</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ni</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Cu</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">As</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Se</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Br</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Sr</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ba</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Pb</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ga</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Zn</mml:mi></mml:mrow></mml:math></inline-formula>) were measured by energy dispersive X-ray fluorescence (ED-XRF) spectrometry (Epsilon 4 ED-XRF, PANalytical B.V., the Netherlands). The X-ray source was matched with a metal-ceramic X-ray tube with an <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Rh</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ag</mml:mi></mml:mrow></mml:math></inline-formula> anode, and the X-ray source was operated at a maximum current of 3 mA and a maximum accelerating voltage of 50 kV (maximum power 15 W).</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Quality control</title>
      <p id="d1e1024">The minimum detection limits (MDLs) of the VOCs were in the range of
0.003–0.042 ppbv with a 3 L sampling volume (Table S1 in the Supplement). The measurement
precision at 2 ppbv was <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> % (Ho et al., 2017, 2018).
Three field blank samples were collected within each sampling day, and they
were analyzed using the same procedures as those for the ambient air
samples. Most target compounds were not detected in the field blanks, and
propylene, benzene, and toluene were below their MDLs (<inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.23</mml:mn></mml:mrow></mml:math></inline-formula> g per
tube and <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> % of the arithmetic mean of ambient samples). No
breakthrough (<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> %) was observed for VOC<inline-formula><mml:math id="M79" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PAMS</mml:mi></mml:msub></mml:math></inline-formula> except
for <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> hydrocarbons, which were <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> % when the air temperature was <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The MDLs for the carbonyl target compounds were between 0.009 and 0.067 ppbv at a sampling volume of
3.6 m<inline-formula><mml:math id="M84" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>. Negligible breakthrough (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> %) was found under the
sampling conditions and flow rates in the field.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Origins of ambient VOCs during dust and fine particle pollution events</title>
      <?pagebreak page5428?><p id="d1e1159">In the present study, the mixing ratio of the sum of non-methane hydrocarbon was
<inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:mn mathvariant="normal">36.0</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">15.7</mml:mn></mml:mrow></mml:math></inline-formula> ppbv, which was lower compared to those in Beijing and
Guangzhou with values of 51.0 and 47.8 ppbv, respectively (Ho et al., 2004;
Liu et al., 2008b). Similar levels of alkenes were seen in the cities of
Beijing (9.4 ppbv) and Guangzhou (8.2 ppbv) compared to that in the present study (9.2 ppbv, Table S2) (Ho et al., 2004; Liu et al., 2008b).
Unexpectedly, the levels of aromatics were slightly higher in Xi'an (10.3 ppbv) than in Beijing (9.6 ppbv) and 50 % higher than in Guangzhou (6.8 ppbv, Shao et al., 2009; Zou et al., 2015). In this respect,
ethylene, ethane, toluene, isopentane, propane, <inline-formula><mml:math id="M87" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-butane, isobutane,
propylene, <inline-formula><mml:math id="M88" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-pentane, and benzene were the 10 most abundant VOC<inline-formula><mml:math id="M89" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PAMS</mml:mi></mml:msub></mml:math></inline-formula>.
The high fractions of these markers reflect strong emissions from traffic
and coal combustion or from biomass burning (Liu et al., 2008a; Ho et al., 2009; Huang et al., 2015; Fan et al., 2014; Z. Zhang et al., 2015). Previous
studies found higher contributions of non-fossil sources to carbonaceous
aerosols in Xi'an than in Beijing (Ni et al., 2018). Generally,
non-fossil emissions mainly originate from biomass burning (Ni et al., 2018), and the higher contribution of non-fossil sources to carbonaceous aerosols in
Xi'an would indicate that remarkable biomass burning activities exist in Xi'an
and the surrounding areas (Huang et al., 2014; Xu et al., 2016).</p>
      <p id="d1e1197">Receptor models and correlations between individual VOCs have been used for
source assessments. In this study, a significant correlation (<inline-formula><mml:math id="M90" 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:mn mathvariant="normal">0.62</mml:mn></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>, slope of 1.59) was found for a least squares regression
between toluene and benzene (Fig. S1 in the Supplement). The ratio of toluene to benzene
(<inline-formula><mml:math id="M92" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula>) has been shown to be different among combustion sources; for
example, Liu et al. (2006) reported <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> ratios of 1.5–2.0 in
gasoline-related emissions collected in a tunnel. In contrast, <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> ratios ranged from 0.23–0.68 and 0.13–0.71 for biomass burning and coal combustion, respectively (Z. Zhang et al., 2015). The <inline-formula><mml:math id="M95" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> ratios in our samples (<inline-formula><mml:math id="M96" 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:mn mathvariant="normal">0.62</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>, slope of 1.59) implied a strong impact
from traffic on the ambient VOCs in Xi'an. Significant correlations
(<inline-formula><mml:math id="M98" display="inline"><mml:mrow><mml:mi>p</mml:mi><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>) were observed among <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> alkanes: between propane and <inline-formula><mml:math id="M100" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-butane (<inline-formula><mml:math id="M101" 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:mn mathvariant="normal">0.75</mml:mn></mml:mrow></mml:math></inline-formula>, slope <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.91</mml:mn></mml:mrow></mml:math></inline-formula>), <inline-formula><mml:math id="M103" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-pentane and isopentane
(<inline-formula><mml:math id="M104" 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:mn mathvariant="normal">0.85</mml:mn></mml:mrow></mml:math></inline-formula>, slope <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.35</mml:mn></mml:mrow></mml:math></inline-formula>), and <italic>trans</italic>-2-butene and <italic>cis</italic>-2-butene
(<inline-formula><mml:math id="M106" 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:mn mathvariant="normal">0.99</mml:mn></mml:mrow></mml:math></inline-formula>, slope <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.84</mml:mn></mml:mrow></mml:math></inline-formula>) (Fig. S1). The observed ratio of propane to
<inline-formula><mml:math id="M108" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-butane in Xi'an was 1<inline-formula><mml:math id="M109" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>1, which is close to that (1.36) observed in the
tunnel study cited above (Liu et al., 2008a). High loadings of <inline-formula><mml:math id="M110" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-pentane and
isopentane are indicative of unburned vehicular emissions, and Liu et al. (2008b) reported a ratio of isopentane / <inline-formula><mml:math id="M111" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-pentane of 3 in tunnel air, which is consistent with the slope of 2.85 found in the present study. The ratios of <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula>, <italic>trans</italic>-<inline-formula><mml:math id="M113" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula><italic>cis</italic>-2-butene, propane / <inline-formula><mml:math id="M114" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-butane, and <inline-formula><mml:math id="M115" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>-pentane<inline-formula><mml:math id="M116" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula>isopentane
indicated that gasoline emissions were a dominant source of ambient VOCs. The source apportionment by PMF (positive matrix factorization) model and the detailed description of
source apportionment will be carried out in the following section.</p>
      <p id="d1e1505">A PMF model was used to identify the major pollution sources; the data input
to the model was the mixing ratios and uncertainties in the mixing
ratios of the VOCs for all valid samples collected during the study. Five sources were
identified (Fig. S2), and the detailed process of source apportionment is
given in the supplement. Biomass burning and gasoline exhaust
were the two most significant pollution sources, contributing 25 % and
18 %, respectively. The combustion of LPG and CNG (25 %), diesel exhaust (15 %), and coal combustion (17 %) were also found to be important sources of ambient VOCs (Fig. S2). Biomass is commonly used for heating and cooking in rural areas of the basin in winter due to its low cost compared to natural gas and electricity. Consistent with our results, previous studies have found a high contribution of biomass burning and gasoline exhaust to the organic aerosol in the Guanzhong basin (Cao et al., 2005).</p>
      <p id="d1e1508">Clear air conditions occurred at the beginning of the sampling period, but
severe dust and fine particle pollution events were observed afterward. The
high dust event was defined by the loading of particulate matter <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> with an aerodynamic diameter (PM<inline-formula><mml:math id="M119" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:math></inline-formula>) between 300 and 500 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, and these conditions occurred from 12:00 LT on 9 November to 13:00 LT on 10 November. The abatement of dust before the fine particle pollution event is referred to as the transition period (i.e., PM<inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">300</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and PM<inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>). The loading of PM<inline-formula><mml:math id="M125" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> subsequently increased, and heavy fine particle pollution
(PM<inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>) occurred after 18:00 LT on 11 November.</p>
      <p id="d1e1669">Ratios of individual VOCs can be used to identify the origins of the
compounds and to study atmospheric aging processes due to the special
composition of VOCs in a typical source and the different lifetimes of VOCs
species (Xue et al., 2017; Z. Zhang et al., 2015). In addition, influences
from meteorological variation and atmospheric transport also need to be
considered when the potential sources of the compounds in ambient air are
characterized. To investigate the impacts of air mass transport on VOC
concentrations, we calculated air mass back trajectories using the NOAA
HYSPLIT model for the dust event (Fig. S4a) and for the fine particle
pollution episode (Fig. S4b) (Stein et al., 2015; Rolph et al., 2017). The
trajectories were calculated at an arrival height of 500 m above ground level at
the observation site. In view of the short atmospheric lifetimes of VOCs
(for example, isoprene <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.4</mml:mn></mml:mrow></mml:math></inline-formula> h; propylene <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5.3</mml:mn></mml:mrow></mml:math></inline-formula> h; toluene 2.1 d) (Atkinson and Arey, 2003), 24 h back trajectories were used for this assessment.</p>
      <p id="d1e1692">Clear different air mass back trajectories and VOC ratios were observed
between dust pollution and haze pollution periods. From 9 to 10 November (in the dust pollution period), the air mass reaching Xi'an passed over
areas to the west of the city (i.e., Gansu province and the Ningxia Hui Autonomous
Region) through long-range transport; after 11 November (formation of haze),
the transport of air mass was mainly limited to areas around southern Xi'an.
Differences in the chemical compositions of ambient VOCs in the dusty versus
in the hazy events can clearly be seen (Fig. 2) in the ratios of toluene to
benzene (<inline-formula><mml:math id="M130" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula>) (toluene: <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">K</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M132" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.96</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M133" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M134" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M135" 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>; benzene: <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">K</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.22</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M138" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M140" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and <inline-formula><mml:math id="M141" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M142" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-xylene to ethylbenzene (<inline-formula><mml:math id="M143" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula>) (<inline-formula><mml:math id="M144" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>-xylene: <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">K</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.30</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M147" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M148" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>; <inline-formula><mml:math id="M150" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-xylene: <inline-formula><mml:math id="M151" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">K</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.43</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M155" 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>; ethylbenzene: <inline-formula><mml:math id="M156" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">K</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.00</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">12</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M160" 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>). During the clear and dust periods, the <inline-formula><mml:math id="M161" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M162" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> ratios varied significantly with time of day; that is, the highest values for <inline-formula><mml:math id="M163" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> (4.5–9.0) and <inline-formula><mml:math id="M164" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> (0.98–1.05) were
seen during rush hour (07:00–09:00 and 17:00–19:00 LT), while the
lowest values (0.50–1.95 for <inline-formula><mml:math id="M165" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and 0.89–0.96 for <inline-formula><mml:math id="M166" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula>) occurred in the early afternoon (i.e., 14:00–15:00 LT). The timings of the high <inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M168" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E<?pagebreak page5429?></mml:mi></mml:mrow></mml:math></inline-formula> ratios suggest that fresh emissions from local traffic were the major source of the ambient VOCs, and this implies that long-range transport did not have a strong impact on the ambient VOCs during the clear or dust parts of the study (Ho et al., 2004; Liu et al., 2008a). During the transitional and fine PM pollution periods, both <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M170" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> varied but at relatively lower values compared to the earlier parts of the study (<inline-formula><mml:math id="M171" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula>: <inline-formula><mml:math id="M172" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.33</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.97</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.21</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.86</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.91</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.74</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.01</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.56</mml:mn></mml:mrow></mml:math></inline-formula> in clear, dust, transitional, and fine particle pollution periods, respectively; <inline-formula><mml:math id="M176" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula>: <inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.00</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.05</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.05</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.12</mml:mn></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.93</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.17</mml:mn></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.95</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.13</mml:mn></mml:mrow></mml:math></inline-formula> in clear, dust, transitional, and fine particle pollution periods, respectively). These synchronous lower values of <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> in transitional and fine particle pollution periods were indicative of aged air masses (Z. Zhang et al., 2015; Xue et al., 2017; Warneke et al., 2013).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e2331">Variations in the ratios of indicator volatile organic compound
low loading (VOC) species (toluene/benzene (<inline-formula><mml:math id="M183" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula>) and <inline-formula><mml:math id="M184" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula>-,<inline-formula><mml:math id="M185" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>-xylene/ethylbenzene (<inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula>)) and fine particle loadings during the study period.</p></caption>
          <?xmltex \igopts{width=412.564961pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f02.png"/>

        </fig>

      <p id="d1e2378">Variations in the air mass transport pathway and <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> ratios during
different sampling periods (clear, dust, transitional, fine particle
pollution) confirmed that ambient VOCs were fresh in the clear and dust
periods but relatively aged during the transitional and fine particle
pollution periods (Z. Zhang et al., 2015; Xue et al., 2017; Warneke et al., 2013). This indicates that the long-range transport of air mass had a
relatively weak influence on the ambient VOCs even during the high dust
period. Otherwise, the composition of ambient VOCs should be relatively aged due
to the long exposure time with dust transport. Indeed, emissions from local
vehicular exhausts and biomass burning in Xi'an and the surrounding areas
were the main contributors to ambient VOCs throughout our study.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Transformation of VOCs between dust and fine particle events</title>
      <p id="d1e2413">With the shading of dust, levels of ambient VOCs decreased with time, and
the low concentrations (8.3–33.9 ppbv) were observed from 13:00 LT on 10 November to 01:00 LT on 11 November (Fig. 3). During the fine particle
pollution period (12–13 November), the <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mo>∑</mml:mo><mml:msub><mml:mtext>VOC</mml:mtext><mml:mi mathvariant="normal">PAMS</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> increased, reaching an average of 38.0 ppbv in the last 24 h, compared to 19.0 ppbv in the transitional period and 21.5 ppbv in the first 12 h of the fine particle pollution episode (Fig. 3). This buildup of VOCs can be explained by weak dispersion and relatively shallow boundary layers (400–1000 m) during the event (Fig. 3). In addition, during this transition period, much lower ratios of <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> were observed in comparison with those in other periods (as mentioned in Sect. 3.1.2). We propose the possibility that windblown dust, which includes sustainable <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">TiO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, can influence the atmospheric photochemistry of VOCs, which would accelerate the oxidation of ambient VOCs (Chu et al., 2019; Nie et al., 2014).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2466">Temporal variations in volatile organic compound (VOC) concentrations and particle levels during the sampling period (9–13 November 2016).</p></caption>
          <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f03.png"/>

        </fig>

      <p id="d1e2475">Changes in the emission sources and their strengths, physical dispersion, regional transport, and the aging of air masses could all affect VOC
levels and composition (Xue et al., 2013, 2017). As a result, to evaluate the aging of ambient VOCs in different periods, the impact of dust on the transformation of ambient VOCs, and the relative processes, the mentioned
factors should be fully considered.</p>
      <p id="d1e2479">To evaluate the impact of source types on the variation of VOCs in the
dust-to-haze episode, the diurnal variation of VOCs was depicted. During the
clear and dust periods – and similar to the trends in <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M194" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> ratios – peaks in <inline-formula><mml:math id="M195" display="inline"><mml:mrow><mml:mo>∑</mml:mo><mml:msub><mml:mtext>VOC</mml:mtext><mml:mi mathvariant="normal">PAMS</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> were seen from 17:00 to 20:00 and 09:00 to 12:00 LT (Fig. 3), which highlighted the impacts of local traffic emissions (Liu et al., 2008a; Huang et al., 2015). 1,3-Butadiene is often used as a marker of gasoline-powered motor vehicles (Huang et al., 2015), while ethane is a key chemical marker for biomass and coal combustion (Liu et al., 2008a). Time series plots of 1,3-butadiene and ethane (Fig. S5) show that peaks in 1,3-butadiene mostly occurred during rush hour,
while higher concentrations of ethane were seen during the night. These
results support the conclusion that there were strong impacts from
gasoline-powered motor vehicles in the daytime and from biomass burning or
coal combustion for heating at night. In addition, winter heating activities
was relatively active because of low temperatures during the transitional
period, and this limited the possibility of reduced emission amounts. Hence,
the variations of source strength were eliminated as being a major factor which
caused the extremely low concentration and relative aged composition of
ambient VOCs.</p>
      <p id="d1e2519">The variation of physical dispersion was also eliminated. With the shading of
dust transport, shallow boundary layers were observed in the transitional
period. For the clear and dust transport period, the boundary layer between
08:00 to 14:00 LT was relatively high (1150–1500 m). In contrast, the boundary layer height decreased sharply to <inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">800</mml:mn></mml:mrow></mml:math></inline-formula> m on 11 November in the
transitional period. This limited the possibility that diffusion caused the
sharp decrease in ambient VOCs in the transitional period.</p>
      <p id="d1e2532">The significant impact of air mass input was eliminated. Input of air mass would
certainly cause the variations in the composition and loading of VOCs (Xue et al., 2014). In the present study, the long-range transport of air masses had limited
impacts on the characteristic of ambient VOCs during the sampling period. In
another aspect, relatively active VOCs would be firstly degraded; hence, the
composition of ambient VOCs would be aged with long-range transport (Ho et
al., 2009; Xue et al., 2017). In the present study, as mentioned
above, the composition of ambient VOCs was relatively fresh under the long-range
transport of air masses (during dust transport). In contrast, the composition of ambient VOC was relatively aged in the transitional period, and the air mass in this period was limited within Xi'an and the surrounding area. This phenomenon indicated that
regional transport cannot be a major factor inducing the relatively aged
composition and excess low loading of the ambient VOCs in the transitional
period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2537">Temporal variations in <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios in the
dust, transitional, and fine particle pollution periods.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f04.png"/>

        </fig>

      <p id="d1e2552">Synchronous changes in the VOC isomerides were found in the windblown
dust-to-haze episode, which supplied the evidence of the accelerated
photochemistry reactions. In the present study, we found a fast decrease in
<italic>trans</italic>-/<italic>cis</italic>-2-butene ratios during dust transporting, which confirmed the
accelerated photochemical reactions of ambient VOCs (Fig. 4).
<italic>Trans</italic>-2-butene and <italic>cis</italic>-2-butene are two isomerides that are mostly emitted from the
same sources (Fang et al., 2017; Y. Zhang et al., 2015). <italic>Trans</italic>-2-butene
has a higher photochemical reaction rate with OH radicals in the atmosphere
(<inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">k</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:mn mathvariant="normal">6.40</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M200" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M201" 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>) than <italic>cis</italic>-2-butene (<inline-formula><mml:math id="M202" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">k</mml:mi><mml:mi mathvariant="normal">OH</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M203" display="inline"><mml:mrow><mml:mn mathvariant="normal">5.64</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">11</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> molecule<inline-formula><mml:math id="M205" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M206" 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>) (Perring et al., 2013); hence, <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios would
decrease with the photochemical reactions (Y. Zhang et al., 2015). Firstly, relatively higher <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios were observed during rush hour
(evening rush hour 17:00–20:00 LT;<?pagebreak page5431?> morning rush hour 07:00–10:00 LT) (Fig. 4), which indicated fresh emissions from local traffic activities (Y. Zhang et al., 2015). In addition, a sharp decrease in <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios was observed from the later half of the windblown dust period to the end of the transitional
period (Fig. 4). The quick shrinking of <italic>trans</italic>-2-butene compared to
<italic>cis</italic>-2-butene in the dust pollution period indicated that the oxidation of
ambient VOCs was accelerated in the period with high loading of the
suspended dust particles (Y. Zhang et al., 2015).</p>
      <p id="d1e2726">A significant increase in particulate active metals was found in the dust
pollution period, which further verified the promotion of dust on the
heterogeneous reactions. Previous studies found that mineral dust can affect
the chemistry of the atmosphere by scavenging gaseous compounds (Zhang et
al., 2000; Chen et al., 2012); it can also promote heterogeneous reactions
of atmospheric substances, including VOCs, because the particle surfaces can
provide sites for photo-catalytic reactions (Cwiertny et al., 2008; Ndour et
al., 2009). In the present study, iron (<inline-formula><mml:math id="M207" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula>) and titanium (<inline-formula><mml:math id="M208" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula>) contents of the particulate increased significantly during the period with dust transport (Fig. 5). In detail, the content of <inline-formula><mml:math id="M209" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula> increased from 19.3 <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> on clear days to 40.8 <inline-formula><mml:math id="M211" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> on dust pollution days, and the content of <inline-formula><mml:math id="M212" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula> increased from 0.92 to 2.98 <inline-formula><mml:math id="M213" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Hence, the huge increase in <inline-formula><mml:math id="M214" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula> concentrations in the particulate phase during the period of dust pollution could possibly promote the solid–gas photochemical reaction of the ambient VOCs, which would reasonably explain the relative low level and aged composition of ambient VOCs in this period (Chu et al., 2019; He et al., 2014; Song et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e2837">Composition of selected metallic elements in the PM<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> samples.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f05.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e2857">Variations in <bold>(a)</bold> the mixing ratios of 17 carbonyl compounds and acetone to methylglyoxal (<inline-formula><mml:math id="M217" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow></mml:math></inline-formula>) ratios in the gas phase, <bold>(b)</bold> particulate carbon fractions, and <bold>(c)</bold> particulate water-soluble ions during the study period.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/20/5425/2020/acp-20-5425-2020-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Variation of carbonyl compounds between dust and fine particle pollution periods: further formation of oxygenated VOCs with aging of primary VOCs</title>
      <p id="d1e2895">The aging of primary VOCs and the formation of carbonyl compounds were observed synchronously as the fine particle pollution event developed (Figs. 3, 6a). As discussed above, relatively low <inline-formula><mml:math id="M218" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">T</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">B</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M219" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">X</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">E</mml:mi></mml:mrow></mml:math></inline-formula> ratios were
observed during the transitional and fine PM periods after the dust event
(Sect. 3.2). In our study, the carbonyl levels increased after the clear and dust periods, and the highest levels were seen during the fine particle pollution event (Fig. 6a). Carbonyl compounds are produced from the primary sources and form through secondary processes (Dai et al., 2012; Duan et<?pagebreak page5432?> al., 2012). We found higher carbonyl concentrations during daytime than at night (Fig. 6a). This is consistent with previous studies in Xi'an
(Dai et al., 2012), which confirmed the secondary formation of carbonyl
compounds under sunlight illumination.</p>
      <p id="d1e2922">Methylglyoxal is generally considered to be a secondary species, while
acetone is mainly from primary emissions; the ratio of acetone to
methylglyoxal (<inline-formula><mml:math id="M220" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow></mml:math></inline-formula>) has been used as an indicator of air mass aging (Dai et al., 2012; Liu et al., 2006). In the present study, <inline-formula><mml:math id="M221" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow></mml:math></inline-formula> ranged from 12 to 14
during the clear period and the first half of the dust period but then dropped sharply
and stayed between 6 and 9 during the later parts of the dust pollution period, the transitional period, and the high PM event (Fig. 6a). Increases in the abundance
of carbonyl compounds and lower <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">A</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">M</mml:mi></mml:mrow></mml:math></inline-formula> ratios suggested relatively stronger aging of the air masses, which is further evidence of the fast degradation of VOCs in the late half of the windblown dust event, and the primary VOCs were oxidized and served as precursors of SOA. In consequence, composition of particles changed with the oxidation of ambient VOCs across the sampling periods.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><?xmltex \opttitle{Variations of PM${}_{{2.5}}$ chemical composition during dust and
fine PM pollution periods}?><title>Variations of PM<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula> chemical composition during dust and
fine PM pollution periods</title>
      <p id="d1e2979">Significant variations of water-soluble inorganic ions, OC, and EC were
observed diurnally and between dust and fine particle pollution events
(Fig. 6b, c). For instance, the concentrations of <inline-formula><mml:math id="M224" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> were
relatively high in the daytime, while <inline-formula><mml:math id="M225" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> were more
abundant at night. The diurnal cycles can be explained by the formation of
secondary particles through photochemical processes during the daytime and
by the impacts from biomass and coal burning for heating at night (Dai et
al., 2012; Zhang et al., 2018; Cong et al., 2015). The concentrations of
<inline-formula><mml:math id="M227" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Ca</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M228" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Mg</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M229" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Na</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, which are typically associated with dust in inland areas (Wu et al., 2011), increased sharply during the dust period and then declined rapidly afterwards.</p>
      <?pagebreak page5433?><p id="d1e3057">As discussed, the apparent contribution of VOCs to the formation of SOAs
increased when the dusty conditions transitioned into a fine particle
pollution event. Temporal changes in the chemical composition of PM<inline-formula><mml:math id="M230" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>
are consistent with this suggestion. During the fine particle pollution
period, the concentrations of secondary ions, particularly
<inline-formula><mml:math id="M231" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>, increased as the haze event developed. A similar trend was
seen for OC (Fig. 6b), and the content of particulate OC increased from 11.1 <inline-formula><mml:math id="M232" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the dust event period to 47.1 <inline-formula><mml:math id="M233" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the haze period. In another aspect, the ratio of <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OC</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> increased from 1.3 to 4.9 in the dust-to-haze episode. The previous studies on the characterization of particles from traffic emissions reported <inline-formula><mml:math id="M235" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OC</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> ratios in the range of 0.28 to 0.92 in diesel vehicles, and the <inline-formula><mml:math id="M236" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OC</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> ratios were reported as <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> in gasoline vehicles (Cadle et al., 1999; Huang et al., 2006). In addition, the <inline-formula><mml:math id="M238" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OC</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> ratios were reported in the range of 0.9 to 1.6 in the urban region of the city of Guangzhou (Tao et al., 2019). In the present study, the consistent increase in <inline-formula><mml:math id="M239" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OC</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">EC</mml:mi></mml:mrow></mml:math></inline-formula> would prove the formation of
SOAs in the dust-to-haze episode. Combined with the findings regarding the
composition of VOCs and PM<inline-formula><mml:math id="M240" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2.5</mml:mn></mml:msub></mml:math></inline-formula>, these results indicate that the
reactions of VOCs led to the formation of SOAs, and in so doing they contributed
to the fine particle pollution.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Summary and conclusion</title>
      <p id="d1e3209">Comprehensive field work was carried out to investigate the origin and
transformation of VOCs within the dust and fine particle pollution periods in winter
in the city of Xi'an. The assumption of the promotion of dust on the
heterogeneous reactions of VOCs was further verified. Local vehicle exhaust
and heating activities were found to be the most important sources of
ambient VOCs in Xi'an during winter, while long-range transport air masses have
limited impacts. Within the period of dust transport, loading of ambient
VOCs decreased sharply from the latter half of the period, and the lowest
concentration was observed in the transitional period, in accordance with
the aging of primary VOCs. In addition, the loading and proportion of secondary VOCs
in the gaseous phase and the secondary ions and organic carbon in the particulate phase
increased with the aging of primary VOCs. Source strength, physical
dispersion, and regional transport were eliminated as major factors for
the variation of the ambient VOCs. Another aspect is the sharp increase in
active metal concentrations (<inline-formula><mml:math id="M241" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Ti</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M242" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">Fe</mml:mi></mml:mrow></mml:math></inline-formula>) and the fast decrease in <italic>trans</italic>-/<italic>cis</italic>-2-butene ratios which were observed from the latter half of the dust transport
period. In consequence, we conclude that windblown dust might accelerate the
solid–gas heterogeneous reactions of atmospheric VOCs and further induce
the formation of SOA precursors.</p><?xmltex \hack{\newpage}?>
</sec>

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

      <p id="d1e3240">All of the research data have been included in the Supplement.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e3243">The following information is provided in the Supplement: sampling procedures, chemical analysis, source characterization, Figs. S1–S5, and Tables S1–S2. The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-20-5425-2020-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-20-5425-2020-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e3252">YX designed the study. YX and YH wrote the paper. SSHH, JC, and SL revised the paper. LC and LW analyzed the data. All authors reviewed and commented on the paper.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e3258">The authors declare that they have no conflict of interest.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e3264">Yu Huang was also supported by the “Hundred Talent Program” of the Chinese
Academy of Sciences. The authors gratefully acknowledge the NOAA Air
Resources Laboratory (ARL) for the provision of the HYSPLIT transport and
dispersion model and the READY website (<uri>https://www.ready.noaa.gov</uri>, last access: 30 April 2020) used in
this publication. The data used are listed in the Supplement.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e3272">This research has been supported by the National Key Research and Development Program of China (grant nos. 2017YFC0212200 and 2016YFA0203000), the National Natural Science Foundation of China (grant nos. 41701565, 21661132005, and 41573138), and the Strategic Priority Research Program of the Chinese Academy of Sciences, China (grant no. XDA23010).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e3278">This paper was edited by Kimitaka Kawamura and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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    <!--<article-title-html>Origin and transformation of ambient volatile organic compounds during a dust-to-haze episode in northwest China</article-title-html>
<abstract-html><p>The high contribution of secondary organic aerosol to the
loading of fine particle pollution in China highlights the roles of volatile
organic compound (VOC) oxidation. In this respect, particulate active metallic
oxides in dust, like TiO<sub>2</sub> and Fe ions, were proposed to influence the photochemical reactions of ambient VOCs. A case study was conducted at an urban site in Xi'an, northwest China, to investigate the origin and transformation of VOCs during a windblown dust-to-haze pollution episode, and the assumption that dust would enhance the oxidation of VOCs was
verified. Local vehicle exhaust (25&thinsp;%) and biomass burning (18&thinsp;%) were found to be the two largest contributors to ambient VOCs. In the dust
pollution period, a sharp decrease in the loading of VOCs and the aging of their
components were observed. Simultaneously, the secondary oxygenated VOC
fraction (i.e., methylglyoxal) increased. Source strength, physical
dispersion, and regional transport were eliminated as major factors for
the variation of ambient VOCs. In another aspect, about a 2- to 3-fold
increase in the loading of iron (Fe) and titanium (Ti) was found in the airborne particles, together with a fast decrease in <i>trans</i>-/<i>cis</i>-2-butene ratios, which demonstrated that dust can accelerate the oxidation of ambient VOCs and the formation of secondary organic aerosol (SOA) precursors.</p></abstract-html>
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