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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-19-14933-2019</article-id><title-group><article-title>Observations of highly oxidized molecules and particle nucleation<?xmltex \hack{\break}?> in the atmosphere of Beijing</article-title><alt-title>Observations of highly oxidized molecules and particle nucleation</alt-title>
      </title-group><?xmltex \runningtitle{Observations of highly oxidized molecules and particle nucleation}?><?xmltex \runningauthor{J. Brean et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Brean</surname><given-names>James</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff4">
          <name><surname>Harrison</surname><given-names>Roy M.</given-names></name>
          <email>r.m.harrison@bham.ac.uk</email>
        <ext-link>https://orcid.org/0000-0002-2684-5226</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Shi</surname><given-names>Zongbo</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7157-543X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Beddows</surname><given-names>David C. S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Acton</surname><given-names>W. Joe F.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Hewitt</surname><given-names>C. Nicholas</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7973-2666</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Squires</surname><given-names>Freya A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3364-4617</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Lee</surname><given-names>James</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-5397-2872</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Division of Environmental Health and Risk Management, School of Geography, Earth and Environmental Sciences, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Lancaster Environment Centre, Lancaster University, Lancaster LA1 4YQ, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>National Centre for Atmospheric Science, Wolfson Atmospheric Chemistry Laboratories,<?xmltex \hack{\break}?> University of York, York YO10 5DD, UK</institution>
        </aff>
        <aff id="aff4"><label>a</label><institution>also at: Department of Environmental Sciences/Center of Excellence in Environmental Studies,<?xmltex \hack{\break}?> King Abdulaziz University, P.O. Box 80203, Jeddah,
21589, Saudi Arabia</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Roy M. Harrison (r.m.harrison@bham.ac.uk)</corresp></author-notes><pub-date><day>10</day><month>December</month><year>2019</year></pub-date>
      
      <volume>19</volume>
      <issue>23</issue>
      <fpage>14933</fpage><lpage>14947</lpage>
      <history>
        <date date-type="received"><day>14</day><month>February</month><year>2019</year></date>
           <date date-type="rev-request"><day>27</day><month>March</month><year>2019</year></date>
           <date date-type="rev-recd"><day>15</day><month>October</month><year>2019</year></date>
           <date date-type="accepted"><day>29</day><month>October</month><year>2019</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2019 </copyright-statement>
        <copyright-year>2019</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="d1e170">Particle nucleation is one of the main sources of atmospheric particulate
matter by number, with new particles having great relevance for human health
and climate. Highly oxidized multifunctional organic molecules (HOMs) have
been recently identified as key constituents in the growth and, sometimes,
in initial formation of new particles. While there have been many studies of
HOMs in atmospheric chambers, flow tubes, and clean environments, analyses of
data from polluted environments are scarce. Here, measurements of HOMs and
particle size distributions down to small molecular clusters are presented
alongside volatile organic compounds (VOCs) and trace-gas data from a
campaign in June 2017, in Beijing. Many gas-phase HOMs have been
characterized and their temporal trends and behaviours analysed in the
context of new particle formation. The HOMs identified have a
degree of oxidation comparable to that seen in other, cleaner, environments, likely
due to an interplay between the higher temperatures facilitating rapid
hydrogen abstractions and the higher concentrations of <inline-formula><mml:math id="M1" 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> and other
<inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> terminators ending the autoxidation sequence more rapidly.
Our data indicate that alkylbenzenes, monoterpenes, and isoprene are
important precursor VOCs for HOMs in Beijing. Many of the <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M4" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds derived from isoprene and monoterpenes have a slightly
greater degree of average oxidation state of carbon compared to those from
other precursors. Most HOMs except for large dimers have daytime peak
concentrations, indicating the importance of <inline-formula><mml:math id="M5" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> chemistry in the
formation of HOMs, as <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> tends to be lower on days with higher HOM
concentrations; similarly, VOC concentrations are lower on the days with
higher HOM concentrations. The daytime peaks of HOMs coincide with the
growth of freshly formed new particles, and their initial formation
coincides with the peak in sulfuric acid vapours, suggesting that the
nucleation process is sulfuric-acid-dependent, with HOMs contributing to
subsequent particle growth.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e251">Atmospheric particle nucleation, or the formation of solid or liquid
particles from vapour-phase precursors, is one of the dominant sources of
global aerosol by number, with primary emissions typically dominating the
mass loadings (Tomasi et al., 2017). New particle formation (NPF) or the
secondary formation of fresh particles is a two-step process comprising
initial homogeneous nucleation of thermodynamically stable clusters and
their subsequent growth. The rate of growth needs be fast enough to
outcompete the loss of these particles by coagulation and condensation
processes in order for the new particles to grow, and hence NPF is a
function of the competition between source and sink (Gong et al., 2010). New
particle formation has been shown to occur across a<?pagebreak page14934?> wide range of
environments (Kulmala et al., 2005). The high particle load in urban
environments was thought to suppress new particle formation until
measurements in the early 2000s (McMurry et al., 2000; Shi et al., 2001;
Alam et al., 2003), with frequent occurrences observed even in the most
polluted urban centres. NPF events in Beijing occur on about 40 % of days
annually, with the highest rates in the spring (Wu et al., 2007, 2008; Wang
et al., 2016). Chu et al. (2019) review many studies of NPF which have taken
place in China and highlight the need for long-term observations and
mechanistic studies.</p>
      <p id="d1e254">NPF can lead to the production of cloud condensation nuclei (CCN)
(Wiedensohler et al., 2009; Yu and Luo, 2009; Yue et al., 2011; Kerminen et
al., 2012), which influences the radiative atmospheric forcing (Penner et
al., 2011). A high particle count, such as that caused by nucleation events,
has been shown to precede haze events in environments such as Beijing (Guo
et al., 2014). These events are detrimental to health and quality of life.
The sub-100 nm fraction of particles to which new particle formation
contributes is often referred to as the ultrafine fraction. Ultrafine
particles (UFPs) pose risks to human health due to their high number
concentration. UFPs exhibit gas-like behaviour and enter all parts of the
lung before penetrating the bloodstream (Miller et al., 2017). They can
initiate inflammation via oxidative stress responses, progressing conditions
such as atherosclerosis and initiating cardiovascular responses such as
hypertension and myocardial infarction (Delfino et al., 2005; Brook
et al., 2010).</p>
      <p id="d1e257">Highly oxidized multifunctional molecules (HOMs), organic molecules with O : C
ratios <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula>, are the result of atmospheric autoxidation and have
recently been subject to much investigation, in part because the extremely
low volatilities arising from their high O : C ratios favour their
condensation into the particulate phase. HOMs are most well characterized as
the product of oxidation of the biogenic monoterpenoid compound <inline-formula><mml:math id="M8" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene (Riccobono et al., 2014; Tröstl et al., 2016; Bianchi et al.,
2017). Although globally biogenic volatile organic compound (BVOC)
concentrations far exceed anthropogenic volatile organic compound (AVOC)
concentrations, in the urban environment the anthropogenic fraction is far
more significant. Formation of HOMs from aromatic compounds has been
demonstrated in laboratory studies and these have been hypothesized to be
large drivers of NPF in urban environments (Wang et al., 2017; Molteni et
al., 2018; Qi et al., 2018). The formation of HOMs through autoxidation
processes begins with the reaction of VOCs with <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, or
<inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>; formation of a peroxy radical (<inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>) is followed
by rapid <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> additions and intra-molecular hydrogen abstractions
(Jokinen et al., 2014; Rissanen et al., 2014; Kurtén et al., 2015).
Furthermore, generation of oligomers from stabilized Criegee intermediates
arising from short-chain alkenes has been hypothesized as a contributor of
extremely low-volatility organic compounds (ELVOCs) and low-volatility
organic compounds (LVOCs) (Zhao et al., 2015). The low volatilities of these
molecules arise from their numerous oxygen-containing functionalities, and
this allows them to make a significant contribution to early stage particle
growth where other species cannot due to the Kelvin effect (Tröstl et
al., 2016), although the contribution of HOMs to the initial molecular
clusters is still debated (Kurtén et al., 2016; Elm et al., 2017; Myllys
et al., 2017).</p>
      <p id="d1e337">Recent technological advances have facilitated insights into the very first
steps of nucleation, which were previously unseen, with mass spectrometric
techniques such as the atmospheric-pressure-interface time-of-flight mass
spectrometer (APi-ToF-MS) and its chemical ionization counterpart (CI-APi-ToF-MS)
allowing for high-mass and high-time-resolution measurements of low-volatility
compounds and molecular clusters. Diethylene glycol-based particle counters,
such as the particle size magnifier (PSM), allow for measurements of particle
size distributions down to the smallest molecular clusters nearing 1 nm.
Recent chamber studies have elucidated the contribution of individual
species to particle nucleation, ammonia, and amines, greatly enhancing the
rate of sulfuric acid nucleation (Kirkby et al., 2011; Almeida et al.,
2013). In these studies, HOMs have been identified, formed through
autoxidation mechanisms (Schobesberger et al., 2013; Riccobono et al., 2014;
Ehn et al., 2014). These are key to early particle growth (Tröstl et
al., 2016) and can nucleate even in the absence of sulfuric acid in chambers
(Kirkby et al., 2016) and in the free troposphere (Rose et al., 2018). In
this paper, we report the results of HOM and particle size measurements
during a summer campaign in Beijing, China.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Sampling site</title>
      <p id="d1e355">Sampling was performed as part of the Air Pollution and Human Health in a
Developing Megacity (APHH-Beijing) campaign, a large international
collaborative project examining emissions, processes, and health effects of
air pollution. For a comprehensive overview of the programme, see Shi et al. (2019). All sampling was conducted across a 1-month period at the
Institute for Atmospheric Physics (IAP), Chinese Academy of Sciences,
Beijing (39<inline-formula><mml:math id="M14" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>58.53<inline-formula><mml:math id="M15" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N, 116<inline-formula><mml:math id="M16" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>22.69<inline-formula><mml:math id="M17" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> E). The sampling was conducted from
a shipping container, with sampling inlets 1–2 m above ground level,
the nearest road being 30 m away. Meteorological parameters (wind
speed, wind direction, relative humidity (RH), and temperature) were measured
at the IAP meteorological tower, 20 m away from the sampling site, 30 m from the nearest road at a height of 120 m. Data were
continuously taken from the CI-APi-ToF-MS during a 2-week period, but due to
data losses only 5 d of data are presented here. Particle size
distribution measurements were taken during a 33 d period from 24 May to 26 June 2017.</p><?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page14935?><sec id="Ch1.S2.SS2">
  <label>2.2</label><title>Chemical ionization atmospheric-pressure-interface time-of-flight mass spectrometry</title>
      <p id="d1e403">The Aerodyne nitrate chemical ionization atmospheric-pressure-interface time-of-flight mass spectrometer (CI-APi-ToF-MS) was used to make measurements of
neutral oxidized organic compounds, sulfuric acid, and their molecular
clusters at high time resolution with high resolving power. The ionization
system charges molecules by adduct formation, such as in the case of organic
compounds with two or more hydrogen bond donor groups (Hyttinen et al.,
2015), or proton transfer in the case of strong acids like sulfuric acid.
Hydroxyl or hydroperoxyl functionalities are both common hydrogen-bond-donating groups, with hydroperoxyl being the more efficient hydrogen bond
donor (Møller et al., 2017). This instrument has been explained in great
detail elsewhere (Junninen et al., 2010; Jokinen et al., 2012), but briefly
the front end consists of a chemical ionization system where a 10 L min<inline-formula><mml:math id="M18" 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> sample
flow is drawn in through the 1 m long 1 in. OD stainless-steel tubing
opening. A secondary flow was run parallel and concentric to this sample
flow, rendering the reaction chamber effectively wall-less. A 3 cm<inline-formula><mml:math id="M19" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> min<inline-formula><mml:math id="M20" 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> flow of
a carrier gas (<inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) is passed over a reservoir of liquid <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
entraining vapour, which is subsequently ionized to <inline-formula><mml:math id="M23" 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> via an
X-ray source. This flow is then guided into the sample flow. The nitrate
ions will then charge molecules by either clustering or proton transfer. The
mixed flows travelling at 10 L min<inline-formula><mml:math id="M24" 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> enter the critical orifice at the front end
of the instrument at 0.8 L min<inline-formula><mml:math id="M25" 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 are guided through a series of
differentially pumped chambers before reaching the ToF analyser. Two of
these chambers contain quadrupoles, which can be used to select greater
sensitivity for certain mass ranges, and the voltages across each individual
chamber can be tuned to maximize sensitivity and resolution for ions of
interest. Mass spectra are taken at a frequency of 20 kHz but are recorded
at a rate of 1 Hz. All data analysis was carried out in the Tofware package in Igor Pro 6 (Tofwerk
AG, Switzerland). A seven-point mass calibration was performed for every
minute of data, and all data were normalized to signal at 62, 80, and 125 <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> to
account for fluctuations in ion signal, these masses representing
<inline-formula><mml:math id="M27" 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>, <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msubsup><mml:mi mathvariant="normal">ONO</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="M29" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><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>
respectively. Typical values for calibration coefficients range from
10<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:math></inline-formula> to 10<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M32" 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> from these normalized data
(Kürten et al., 2012), producing peak sulfuric acid concentrations in
the range of 10<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M34" 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>. From the very limited periods
with simultaneous data for <inline-formula><mml:math id="M35" 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>, OH radical, and condensation sink, it
was possible to calculate <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations of 10<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula> to
10<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> molec. cm<inline-formula><mml:math id="M39" 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>, in which range the calibration constant was <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mn mathvariant="normal">7.0</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M41" 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>, which fits well with that expected for this
concentration range (Kürten et al., 2012). The nitrate–water cluster is
included as the presence of many nitrate–water clusters of the general
formula <inline-formula><mml:math id="M42" display="inline"><mml:mrow class="chem"><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:msub><mml:mo>)</mml:mo><mml:mi>x</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">HNO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mi mathvariant="normal">y</mml:mi></mml:msub><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 found, where <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">3</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">…</mml:mi><mml:mn mathvariant="normal">20</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>,</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. No sensitivity calibration was performed for
these measurements, and so all values are reported in normalized signal
intensity. Due to the high resolving power of the CI-APi-ToF-MS system (mass resolving power of 3500 <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula> and mass accuracy of 20 ppm at 288 <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>; resolving power is measured as the mass/charge, termed <inline-formula><mml:math id="M47" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> divided by the peak width at its half maximum, dubbed <inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>m</mml:mi></mml:mrow></mml:math></inline-formula>), multiple
peaks can be fit at the same unit mass and their molecular formulae
assigned. These peaks follow the general formula
<inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>y</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi>z</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>–20, <inline-formula><mml:math id="M51" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>–32, <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn></mml:mrow></mml:math></inline-formula>–16, and
<inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–2, spanning from small organic acids like oxalic and malonic acid
through to large dimers of oxidized monoterpene <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> radicals such as <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">31</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>. Beyond 500 <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>, peak fitting and
assignment of compositions becomes problematic as signal decreases, mass
accuracy decreases, and the total number of chemical compositions increases,
so peaks above the <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> region have not been assigned, and a number of
peaks have been unassigned due to this uncertainty (Cubison and Jimenez,
2015). As proton transfer mostly happens with acids, and nearly all HOM
molecules will be charged by adduct formation, it is possible to infer the
uncharged formula; therefore all HOMs from here onwards will be listed as
their uncharged form.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Size distribution measurements</title>
      <p id="d1e978">Two scanning mobility particle sizer (SMPS) instruments measured particle
size distributions at 15 min time resolution, with one long SMPS (TSI 3080 EC,
3082 long DMA, 3775 CPC, TSI, USA) and one nano SMPS (3082 EC, 3082 nano DMA,
3776 CPC, TSI, USA) measuring the ranges 14–615 and 4–65 nm respectively.
A particle size magnifier (A10, Airmodus, FN) linked to a CPC (3775, TSI,
USA) measured the sub-3 nm size fraction. The PSM was run in stepping mode,
operating at four different saturator flows to vary the lowest size cut-off
of particles that it will grow (this cut-off is technically a point of
50 % detection efficiency) of <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1.30</mml:mn></mml:mrow></mml:math></inline-formula>, 1.36, 1.67, and 2.01 nm. The
instrument switched between saturator flows per 2.5 min, giving a
sub-2.01 nm size distribution every 10 min. The data were treated with a
moving-average filter to account for jumps in total particle count, and due
to the similar behaviour of the two upper and two lower size cuts, these
have been averaged to two size cuts at 1.30 and 1.84 nm.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Calculations</title>
      <p id="d1e999">The condensation sink (CS) was calculated from the size distribution data as
follows:
            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M59" display="block"><mml:mrow><mml:mi mathvariant="normal">CS</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4</mml:mn><mml:mi mathvariant="italic">π</mml:mi><mml:mi>D</mml:mi><mml:munder><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:msub><mml:msup><mml:mi>d</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:munder><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mrow><mml:mi>m</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:msup><mml:mi>d</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:msub><mml:msub><mml:msup><mml:mi>d</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi mathvariant="normal">p</mml:mi></mml:msub><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:msub><mml:msup><mml:mi>d</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M60" display="inline"><mml:mi>D</mml:mi></mml:math></inline-formula> is the diffusion coefficient of the diffusing vapour (assumed
sulfuric acid), <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi>m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a transition regime correction (Kulmala et
al., 2012), <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msubsup><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> is particle diameter, and <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mrow><mml:msubsup><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the
number of particles at diameter <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:msubsup><mml:mi>d</mml:mi><mml:mi mathvariant="normal">p</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p><?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page14936?><sec id="Ch1.S2.SS5">
  <label>2.5</label><title>Other measurements</title>
      <p id="d1e1140">Measurements of the classical air pollutants were measured at the same site
and have been reported in the campaign overview paper (Shi et al., 2019).
<inline-formula><mml:math id="M65" 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> was measured using a 43i <inline-formula><mml:math id="M66" 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> analyser (Thermo Fisher
Scientific, USA), <inline-formula><mml:math id="M67" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> with a 49i <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> analyser (Thermo Fisher
Scientific, USA), and <inline-formula><mml:math id="M69" 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> with a 42i-TL trace <inline-formula><mml:math id="M70" 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> analyser
(Thermo Fisher Scientific, USA) and a T500U CAPS <inline-formula><mml:math id="M71" 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> analyser
(Teledyne API, USA). VOC mixing ratios were measured using a proton-transfer-reaction time-of-flight mass spectrometer (PTR-ToF-MS 2000, Ionicon, Austria).</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>Characteristics of sampling period</title>
      <p id="d1e1237">A total of 5 d of CI-API-ToF-MS data were collected successfully, from
21 June 2017 midday through 26 June 2017 midday. New particle formation events
were observed on 24 June in the late afternoon and 25 June at
midday. Some nighttime formation of molecular clusters was seen earlier in
the campaign, as were several peaks in the 1.5–100 nm size range, likely
from pollutant plumes containing freshly nucleating condensable materials.
The trace gases, <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M73" 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>, NO, and <inline-formula><mml:math id="M74" 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>, are plotted in
Fig. S1 in the Supplement. <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> shows mid-afternoon peaks, around <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">120</mml:mn></mml:mrow></mml:math></inline-formula> ppb on the first 2 d of the campaign and 50–70 ppb for the later
days. <inline-formula><mml:math id="M77" 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> shows a large peak, reaching 4 ppb on 22 June but <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> ppb for the rest of campaign. NO shows strong mid-morning rush-hour-related
peaks, declining towards midday due to being rapidly consumed by <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.
<inline-formula><mml:math id="M80" 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> shows large traffic-related peaks. The sulfuric acid signal
across this period as measured by <inline-formula><mml:math id="M81" 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> CI-APi-ToF-MS showed
strong midday peaks, with the highest signal on 24 and 25 June 2017. The
meteorological data are shown in Fig. S2 alongside condensation sink (CS).
The conditions were generally warm and humid, with temperature reaching its
maximum on 25 June 2017, with a peak hourly temperature of 31 <inline-formula><mml:math id="M82" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. High
temperatures were also seen on 21 and 24 June, 30 and 26 <inline-formula><mml:math id="M83" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C
respectively.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Gas-phase HOM chemistry</title>
<sec id="Ch1.S3.SS2.SSS1">
  <label>3.2.1</label><title>Bulk chemical properties</title>
      <p id="d1e1385">For the peaks that have had chemical formulae assigned, oxidation state of
carbon, or OS<inline-formula><mml:math id="M84" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:math></inline-formula>, can be used to describe their bulk oxidation chemistry.
OS<inline-formula><mml:math id="M85" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:math></inline-formula> is defined as (Kroll et al., 2011)
              <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M86" display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">OS</mml:mi><mml:mi mathvariant="normal">c</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mo>(</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mo>×</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">O</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">H</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mo>:</mml:mo><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">C</mml:mi></mml:mrow><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
            This does not account for the presence of nitrate ester groups, which has
been accounted for previously by subtracting 5 times the N : C ratio
(Massoli et al., 2018), under the assumption that all nitrogen-containing
functionality is in the form of nitrate ester (<inline-formula><mml:math id="M87" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RONO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) groups. In
Beijing, multiple sources of nitrate-containing organic compounds are seen,
in the forms of amines, nitriles, and heterocycles. The variation in
oxidation state with carbon number (<inline-formula><mml:math id="M88" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) without correction for nitrate
esters is plotted in Fig. 1. The average oxidation state of carbon in this
dataset tends to decrease with an increase in <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, highest where
<inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>, attributable to both high O : C and peak area, for the peak
assigned to <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> 288. <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> also
shows the greatest distribution of oxidation states, likely due to the high
ambient concentration of isoprene and therefore its many oxidation products
being of high enough signal for many well-resolved peaks to be seen in this
dataset. It is worth noting that some of the ions plotted here may not form
through peroxy radical autoxidation, such as <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
which may be a second-generation oxidation product of isoprene under high
<inline-formula><mml:math id="M95" 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> (Lee et al., 2016). <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> and 15 also see a small increase
in average oxidation number compared to their neighbours. The lower
oxidation state of the larger products is likely a function of two things.
First and foremost, any autoxidation mechanism must undergo more steps in
order for a larger molecule to reach an O : C ratio equivalent to that of a smaller
one, and the equivalent O : C ratio is ultimately less likely to be reached
before the radical is terminated (Massoli et al., 2018). Secondly, the lower
vapour pressures of these larger products will lead to their partitioning
into the condensed phase more readily than the smaller; thus they are more
rapidly lost (Mutzel et al., 2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><label>Figure 1</label><caption><p id="d1e1609">Oxidation state of carbon calculated as 2 times the
oxygen-to-carbon ratio minus the hydrogen-to-carbon ratio against carbon
number for (coloured) individual ions and (blue circles) signal-weighted
average for each carbon number. Area and colour are both proportional to the
peak area for each ion.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f01.png"/>

          </fig>

      <p id="d1e1618">The degrees of OSc observed here are similar to those seen in other
environments such as during the SOAS campaign in 2013 in the southern United
States, characterized by low <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi><mml:mo>/</mml:mo><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 high temperatures, where
campaign averages of 0.3 ppb, 0.4–0.5 ppb, and 25 <inline-formula><mml:math id="M98" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C respectively were
measured, although an additional parameter to account for nitrogen-containing VOCs is included in the calculation (Massoli et al., 2018). The
OS<inline-formula><mml:math id="M99" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:math></inline-formula> observed in Beijing is also higher than that seen in the boreal
forest environment of Hyytiälä, despite extremely low <inline-formula><mml:math id="M100" 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>
concentrations, likely due to low temperature conditions dominating in those
conditions (Schobesberger et al., 2013). These degrees of
oxidation relatively similar to those seen in other, cleaner environments are likely due to an
interplay between the higher temperatures facilitating rapid hydrogen
abstractions (Crounse et al., 2013; Quéléver et al., 2019) and the
higher concentrations of <inline-formula><mml:math id="M101" 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>, <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>, and other
<inline-formula><mml:math id="M103" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> molecules terminating the autoxidation sequence more
efficiently (Praske et al., 2018; Rissanen, 2018; Garmash et al., 2019).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><label>Figure 2</label><caption><p id="d1e1706">Mass defect plot of fitted mass spectral peaks between
100 and 600 mass units at <bold>(a)</bold> 10:30–12:00 CST on 23 June 2017, a non-nucleation day,
and <bold>(b)</bold> at 10:30–12:00 CST on 25 June 2017, a nucleation day. Mass defect can be
defined as the mass – integer mass. The size of point is proportional to the
signal intensity. As <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mi mathvariant="normal">H</mml:mi></mml:mrow></mml:math></inline-formula> has a positive mass defect (1.007276 Da), the
upward trend along the horizontal indicates increasing carbon chain length,
and differences at similar masses are due to increasing oxygen
functionality and clustering with species such as sulfuric acid (negative mass
defect) and ammonia (positive mass defect), as <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">32</mml:mn></mml:msup><mml:mi mathvariant="normal">S</mml:mi></mml:mrow></mml:math></inline-formula> have
negative mass defects (15.9949 and 31.9721 Da respectively), while <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>
has a positive mass defect at 14.0031 Da. The two large peaks seen at 201
and 288 <inline-formula><mml:math id="M108" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> are the nitrophenol–nitrate cluster and a <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–nitrate
cluster respectively.</p></caption>
            <?xmltex \igopts{width=426.791339pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f02.png"/>

          </fig>

      <p id="d1e1808">A mass defect plot is shown in Fig. 2, which shows nominal mass plotted
against mass defect for all peaks in this dataset. Mass defect is defined as
the ion mass minus integer mass. This is shown for two separate daytime
periods, one where nucleation was not occurring and HOM concentrations are
lower (10:30–12:00 CST 23 June 2017) and one where nucleation was occurring
under high HOM concentrations (10:30–12:00 CST 25 June 2017). The band of<?pagebreak page14937?> lower
mass defect is characterized by a number of large peaks with high signal,
for example, at <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> 436 the ion
<inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">SO</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:msubsup><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>. The upper
component of the mass defect is dominated by organic compounds, and the upper
end of the more positive mass defect is occupied by molecules with more <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mi mathvariant="normal">H</mml:mi></mml:mrow></mml:math></inline-formula>
(mass defect 7.825 mDa) and <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">14</mml:mn></mml:msup><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula> (mass defect 3.074 mDa). The end of the
less positive mass defect has lower <inline-formula><mml:math id="M114" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">1</mml:mn></mml:msup><mml:mi mathvariant="normal">H</mml:mi></mml:mrow></mml:math></inline-formula> and more <inline-formula><mml:math id="M115" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi/><mml:mn mathvariant="normal">16</mml:mn></mml:msup><mml:mi mathvariant="normal">O</mml:mi></mml:mrow></mml:math></inline-formula> (mass defect
<inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5.085</mml:mn></mml:mrow></mml:math></inline-formula> mDa); alternatively put, the mass defect reflects the variation in
OS<inline-formula><mml:math id="M117" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:math></inline-formula>. The organic components with more positive mass defects will be more
volatile than their lower mass defect counterparts as they will contain
fewer oxygen functionalities (Tröstl et al., 2016; Stolzenburg et al.,
2018). These higher-volatility products may still contribute to larger size
particle growth. The more negative mass defect components will be those of
greater O : C and therefore lower volatility, LVOCs, and the yet larger and
more oxidized components, ELVOCs (Tröstl et al., 2016). During the
nucleation period, the signal intensity for the species in the upper band of
more negative mass defect have the most marked increase in concentration,
with significantly less difference <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>. This region 200–400 <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> will contain most of the <inline-formula><mml:math id="M121" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> monomer HOMs seen in this
dataset.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <label>3.2.2</label><title>Diurnal trends of HOMs</title>
      <p id="d1e2002">Temporal trends of HOMs in the urban atmosphere can reveal their sources and
behaviour in the atmosphere. Most of the HOM species peak in the daytime.
These species all follow a similar diurnal trend, as shown in Fig. 3.
The concentrations of both <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> are high during the summer
period in Beijing (although the nitrate chemical ionization technique is not
sensitive to all <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> oxidation products; Berndt et al., 2015).
Figure S1 shows the time series of concentrations of NO, which is
considered a dominant peroxy radical terminator of particular importance in
the polluted urban environment (Khan et al., 2015). Radicals such as
<inline-formula><mml:math id="M126" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> also typically peak during daytime. The
HOM components peaking in the daytime are presumed to be the oxidation
products of a mixture of anthropogenic and biogenic components, such as
alkylbenzenes, monoterpenes, and isoprene. The oxidation of monoterpenes,
specifically the monoterpene <inline-formula><mml:math id="M128" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene, has been the subject of
extensive study recently, with the <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-initiated autoxidation sequence
being the best characterized (Ehn et al., 2014; Jokinen et al., 2014;
Kurtén et al., 2015; Kirkby et al., 2016); ozonolysis of <inline-formula><mml:math id="M130" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene opens the ring structure and produces a <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> radical (Kirkby et al., 2016). In the case of aromatics, <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> addition to the ring and the subsequently formed bicyclic peroxy radical
are the basis for the autoxidation of compounds such as xylenes and
trimethylbenzenes (Molteni et al., 2018; Wu et al., 2017).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><label>Figure 3</label><caption><p id="d1e2116">Summed time series of the normalized signals of <bold>(a)</bold> all
non-nitrogen-containing HOMs and all organonitrates identified; <bold>(b)</bold> <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M134" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
and <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> components, assumed to be dominated by isoprene, monoterpene monomer,
and monoterpene dimers, and signal for <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> multiplied 50 times to fit scale; and
<bold>(c)</bold> summed <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M138" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> components and summed <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M140" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> components, assumed to
be dominated by alkylbenzenes and other larger components respectively.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f03.png"/>

          </fig>

      <p id="d1e2223">The identified compounds have been roughly separated into several
categories, each of these plotted in Fig. 3. Figure 3a shows the separation
of components into non-nitrogen-containing HOMs and nitrogen-containing
HOMs, or organonitrates (ONs). The ON signal is much higher than that of the
HOM, attributable in part to a few ions of high signal, such as the isoprene
organonitrate <inline-formula><mml:math id="M141" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. A few similar structural
formulae are seen (<inline-formula><mml:math id="M142" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M144" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, etc.), some of which have been identified as
important gas-phase oxidation products of isoprene under high-<inline-formula><mml:math id="M145" 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> conditions (Xiong et al., 2015), and their contribution to secondary organic aerosol (SOA) has been
explored previously (Lee et al., 2016). A high nitrophenol signal is also
seen, <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The signal for HOM compounds is less dominated
by a few large ions. The prevalence of ON compounds points towards the
important role of <inline-formula><mml:math id="M147" 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> as a peroxy radical terminator, with the
probability of the <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> reaction producing nitrate ester compounds increasing with the size of the <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> molecule (Atkinson et al., 1982). The <inline-formula><mml:math id="M150" 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> concentrations in urban
Beijing are approximately a factor of 10 higher than seen at the
Hyytiälä station in Finland as reported by Yan et al. (2016), and
hence it is expected to be a more significant peroxy radical terminator.</p>
      <p id="d1e2409">Despite the very large fluxes of anthropogenic organic pollutants in
Beijing, biogenic emissions are still an important source of reactive VOCs
in the city, with abundant isoprene oxidation products observed (see above),
as well as monoterpene monomers (<inline-formula><mml:math id="M151" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">16</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M152" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>) and some dimer products (<inline-formula><mml:math id="M153" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">30</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M154" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">31</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>). The time series of the signals of all <inline-formula><mml:math id="M155" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
<inline-formula><mml:math id="M156" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and <inline-formula><mml:math id="M157" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> molecules is plotted in Fig. 3b, with <inline-formula><mml:math id="M158" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species assumed to be isoprene-dominated and <inline-formula><mml:math id="M159" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M160" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> assumed to be monoterpene-dominated. Signals for<?pagebreak page14938?> isoprene oxidation
products are higher, with abundant isoprene nitrate and dinitrate products.
<inline-formula><mml:math id="M161" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products show similar behaviour, with, for example, several
<inline-formula><mml:math id="M162" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula>–9 compounds seen. The <inline-formula><mml:math id="M164" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> signal
intensities are low and follow the general formula
<inline-formula><mml:math id="M165" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi mathvariant="normal">y</mml:mi></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mi mathvariant="normal">z</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:mi>x</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">26</mml:mn></mml:mrow></mml:math></inline-formula>–32, <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:mi>y</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">7</mml:mn></mml:mrow></mml:math></inline-formula>–11, and <inline-formula><mml:math id="M168" display="inline"><mml:mrow><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>–2;
in Fig. 3 the signal for <inline-formula><mml:math id="M169" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds has been multiplied by a
factor of 50 for visibility. The low signals reflect the lack of
<inline-formula><mml:math id="M170" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> cross reactions necessary for the production of these
accretion products.</p>
      <p id="d1e2712">Other identified peaks are plotted in Fig. 3c. The <inline-formula><mml:math id="M171" 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:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M172" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> components are summed together, these being small organic acids such as
malonic acid and oxalic acid, as well as products such as
<inline-formula><mml:math id="M173" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula>. Malonic acid is the most prominent here, seen as both an <inline-formula><mml:math id="M174" 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> adduct (<inline-formula><mml:math id="M175" 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:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><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
a proton transfer product (<inline-formula><mml:math id="M176" 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:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msubsup><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) at a ratio of around
2 : 3. Measurements of particle-phase dicarboxylic acids in cities typically
show greater concentrations of oxalic acid than malonic acid (Ho et al.,
2010), and these acids are primarily produced in the aqueous phase (Bikkina
et al., 2014). Primary sources of dicarboxylic acid include fossil fuel
combustion (Kawamura and Kaplan, 1987) and biomass burning (Narukawa et al.,
1999), which are both plentiful in urban Beijing. The <inline-formula><mml:math id="M177" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M178" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> components are assumed to be dominated by oxidation products of
alkylbenzenes such as <inline-formula><mml:math id="M179" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, although fragments of other
compounds, i.e. monoterpenes, can also occupy this region
(Isaacman-Vanwertz et al., 2018). It is assumed the majority of the signal
for these peaks come from alkylbenzenes. This assumption is supported by the
relative signal intensity ratios of the oxygen numbers of monomer
<inline-formula><mml:math id="M180" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mi>n</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> compounds being similar to those seen for xylene
oxidation products in previous work (Molteni et al., 2018). The largest
fraction, <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">18</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, includes the larger compounds,
oxidation products of larger aromatics, or products of the cross reaction of
smaller <inline-formula><mml:math id="M183" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> radicals. Here they are grouped without more
sophisticated disaggregation as they all follow much the same time series, with
species such as <inline-formula><mml:math id="M184" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">11</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula> following the same temporal trends
as <inline-formula><mml:math id="M185" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">15</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">16</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M186" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">16</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">24</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><label>Figure 4</label><caption><p id="d1e2992">Time series for the whole sampling campaign for the
concentrations of (left axis) VOCs as measured by PTR-ToF-MS and (right axis) a
selected HOM product associated with that precursor.</p></caption>
            <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f04.png"/>

          </fig>

      <p id="d1e3001">Nearly all ions with the exception of the larger compounds attributed to the
cross reaction of <inline-formula><mml:math id="M187" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> monomers follow similar temporal patterns, with
the majority of peaks occurring in the daytime. This reflects the importance
of the concentration of atmospheric oxidants. Some selected oxidation
products are plotted against their precursor VOCs in Fig. 4. The
concentration of isoprene is plotted against the signal of a nitrate HOM
product, <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Xiong et al., 2015; Lee et al., 2016),
while monoterpenes are plotted against <inline-formula><mml:math id="M189" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">16</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Ehn et al.,
2014; Berndt et al., 2016; Yan et al., 2016; Kirkby et al., 2016; Massoli et
al., 2018) and <inline-formula><mml:math id="M190" 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:mrow></mml:math></inline-formula> benzenes against <inline-formula><mml:math id="M191" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Molteni et
al., 2018; Wang et al., 2017). The first half of the time series shows
little correlation between the VOC species and the resultant oxidation
products, while isoprene, monoterpenes, and <inline-formula><mml:math id="M192" 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:mrow></mml:math></inline-formula> benzenes follow their
usual diurnal cycles, with isoprene having the most distinct cycle with a strong midday
peak. The last 2 d, however, show<?pagebreak page14939?> similar and coinciding peaks in
both the VOCs and HOMs – HOMs show afternoon peaks on both days and an
initial shelf on the final half day. The <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> peak
follows some of the peaks of the isoprene, but not all (e.g. morning shelf
of isoprene on 24 June). Concentrations of isoprene do not seem to determine
directly the signal of HOM, as the day with the lowest isoprene of all is
the day with the highest <inline-formula><mml:math id="M194" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The <inline-formula><mml:math id="M195" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">16</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> trace also has coincidental peaks with the monoterpene trace, including
two 4 h separated simultaneous peaks on 25 June. The peaks in the
concentrations of <inline-formula><mml:math id="M196" 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:mrow></mml:math></inline-formula> benzenes are nearly synchronous with the peaks in
<inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">8</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, for which the data exhibit a strong mid-afternoon
peak likely due to the lack of an efficient ozonolysis reaction pathway; the
main oxidant of <inline-formula><mml:math id="M198" 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:mrow></mml:math></inline-formula> benzenes is the <inline-formula><mml:math id="M199" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> radical. Trends of both
<inline-formula><mml:math id="M200" 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:mrow></mml:math></inline-formula> benzenes and their HOMs are much the same as <inline-formula><mml:math id="M201" 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:mrow></mml:math></inline-formula> benzenes as
discussed above, pointing to similar sources and oxidation chemistries.
The concentration of precursor VOC is likely a driving force in the identity
and quantity of various HOM products, but not the sole determinant, as while
there are simultaneous peaks of VOCs and HOMs, both the condensation sink
and oxidant concentrations also influence HOM product signals.</p>
      <p id="d1e3241">The first half of campaign measurements are marked by an episode of low HOM
signals. A diurnal cycle still exists but it is weak. The radiation
intensity was significantly lower on these prior days than it was on
24 June. No data are available for the final period of measurement. Ozone is
higher on the prior measurement days with lower HOM signals (see Fig. S1).
Little agreement is seen between VOC concentration and HOM signals on these
days. The condensational sinks are roughly similar to those on days of
higher HOM concentrations, but temperature and solar<?pagebreak page14940?> radiation are much
lower. HOM formation is largely dependent upon VOC concentration, oxidant
concentration (which will be lower if solar radiation is lower, especially
in the case of <inline-formula><mml:math id="M202" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>, the main oxidant of aromatic species especially),
and temperature (as H shifts are highly temperature-dependent)
(Quéléver et al., 2019), as well as losses by <inline-formula><mml:math id="M203" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>
termination before a molecule can become HOM and losses to condensational
sink. The low HOM concentration is likely due to these lower temperatures
and weaker solar radiation not facilitating HOM formation.</p>
      <p id="d1e3269">The <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds plotted in Fig. 3b show no strong diurnal
sequence, contrasting with other HOMs. We can presume that all <inline-formula><mml:math id="M205" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> compounds identified are the result of the reaction of two monoterpenoid
<inline-formula><mml:math id="M206" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M207" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> radicals, a reasonable assumption as all
identified <inline-formula><mml:math id="M208" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> species follow the general formula outlined for these
reactions (<inline-formula><mml:math id="M209" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mrow><mml:mn mathvariant="normal">28</mml:mn><mml:mtext>–</mml:mtext><mml:mn mathvariant="normal">32</mml:mn></mml:mrow></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mtext>–</mml:mtext><mml:mn mathvariant="normal">16</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>). The formation of <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">20</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> dimers is dependent upon two processes, initial oxidation of monoterpenes
and <inline-formula><mml:math id="M211" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M212" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> termination. Initial oxidation is contingent upon
oxidant concentration, which is highest in the daytime, and
<inline-formula><mml:math id="M213" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M214" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> termination is contingent upon the probability
of the molecular collision between the <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> molecules
occurring before other radical termination (i.e.
<inline-formula><mml:math id="M216" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M217" 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> or <inline-formula><mml:math id="M218" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>–<inline-formula><mml:math id="M219" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula>). There is likely
a strong diurnal sequence in the dominant <inline-formula><mml:math id="M220" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> termination
mechanisms across the daytime period, and the combination of the two factors
discussed above results in there being no strong diurnal trend in these
molecules. A lower oxidant concentration at night results in fewer
<inline-formula><mml:math id="M221" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> molecules, but less NO and <inline-formula><mml:math id="M222" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> results in a greater chance for those <inline-formula><mml:math id="M223" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> molecules to
dimerise (Rissanen, 2018; Garmash et al., 2019). As the levels of <inline-formula><mml:math id="M224" 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> in Beijing fall, the peroxy radical termination reactions will be less
probable<?pagebreak page14941?> compared to continued autoxidation (Praske et al., 2018), and it is
expected that more oxidized HOM products will be seen with lower
volatilities and therefore a greater potential contribution to earlier stage
particle formation and growth.</p>
</sec>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>New particle formation</title>
      <p id="d1e3557">Nearly all the signal intensity in the CI-APi-ToF-MS instrument arises from
molecules charged by <inline-formula><mml:math id="M225" 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>; therefore plotting the unit mass
resolution data (the data gained by integrating over the entire area at each
<inline-formula><mml:math id="M226" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> integer) against time simply describes the evolution of oxidized organic
molecules, acids, and their molecular clusters with both each other and
stabilizing amine species. This is done in Fig. 5. As the signal intensity
varies by factors of 10 from mass to mass, each value has been normalized so
they have maxima at 1. This has been done separately for 2 d for
clarity, as the signal intensity also varies from day to day. PSM data for
these 2 d is also plotted in Fig. 5, with both total particle count
<inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.30</mml:mn></mml:mrow></mml:math></inline-formula> nm in black and the number difference between the lower
and upper size cuts (1.30 and 1.84 nm) in blue, which shows the number of
particles between these sizes. The relationship between mass and electrical
mobility diameter can be defined thus (Tammet, 1995)
            <disp-formula id="Ch1.E3" content-type="numbered"><label>3</label><mml:math id="M228" display="block"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mn mathvariant="normal">6</mml:mn><mml:mi>m</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="italic">π</mml:mi><mml:mi mathvariant="italic">ρ</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mn mathvariant="normal">1</mml:mn><mml:mn mathvariant="normal">3</mml:mn></mml:mfrac></mml:mstyle></mml:msup><mml:mo>+</mml:mo><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M229" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the electrical mobility diameter of the cluster or
particle, <inline-formula><mml:math id="M230" display="inline"><mml:mi>m</mml:mi></mml:math></inline-formula> is the mass of the cluster or particle expressed in kilogrammes, <inline-formula><mml:math id="M231" display="inline"><mml:mi mathvariant="italic">ρ</mml:mi></mml:math></inline-formula> is
the density, and <inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi>d</mml:mi><mml:mi mathvariant="normal">g</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the effective gas diameter, determined to be 0.3 nm for smaller particles (Larriba et al., 2011). We can use this to draw a
comparison between the PSM and CI-APi-ToF-MS measurements. If a density of 1.2 g cm<inline-formula><mml:math id="M233" 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> is assumed, then once molecular clusters reach the
<inline-formula><mml:math id="M234" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M235" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> range, they will be seen in the lowest size cut of the PSM,
or <inline-formula><mml:math id="M236" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">700</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M237" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> if a density of 2.0 g cm<inline-formula><mml:math id="M238" 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> is assumed. A full
table of densities is provided in the Supplement.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><?xmltex \currentcnt{5}?><label>Figure 5</label><caption><p id="d1e3745">Normalized unit mass <inline-formula><mml:math id="M239" 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> CI-APi-ToF-MS signal intensity on
24 June 2017 <bold>(a)</bold> and 25 June 2017 <bold>(b)</bold>. Each individual unit mass was normalized
to a maximum of 1. Each period is normalized separately so the individual
signal maxima on each day are visible. The graph is plotted between 200 and 600
mass units, with every 10 mass units averaged for simplicity. On the
secondary axis PSM data are plotted, both total particle count <inline-formula><mml:math id="M240" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.30</mml:mn></mml:mrow></mml:math></inline-formula> nm (black trace) and total clusters between 1.30 and 1.84 nm (blue
trace). Data are plotted at 1 h time resolution.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f05.png"/>

        </fig>

      <p id="d1e3783">A burst in the signal seen by the CI-APi-ToF-MS occurs first in the late
morning in Fig. 5a, and this is at the same time as peaks
begin to rise in the identified HOMs (see Fig. 3). Here, the PSM is not
available due to an instrumental fault until 16:00 CST; however, at that point,
an elevation to particle count and a large elevation to cluster count can be
seen. Moving into the evening period, the mass contour shows peaks in larger
masses <inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M242" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>. These are likely dimerized compounds and products of
<inline-formula><mml:math id="M243" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula> chemistry with little contribution to newly forming
particles but still sensitive to chemical ionization by <inline-formula><mml:math id="M244" 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>.
Many of these peaks cannot be assigned due to uncertainties in the
structural formula assignment for higher mass peaks, as the number of
possible dimerized compounds is many, being the combination of most possible
<inline-formula><mml:math id="M245" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">RO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals. Graphically, these are over-represented in Fig. 5 due
to the normalization, and their signals (especially <inline-formula><mml:math id="M246" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">500</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>) are much
lower than the signals <inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">400</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><label>Figure 6</label><caption><p id="d1e3893">SMPS <inline-formula><mml:math id="M250" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> PSM contour plot for two nucleation days on
24 and 25 June 2017. Data in the bottom panel are from the PSM instrument, and the
top panel from the nano SMPS; units in the colour bar are <inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi>log⁡</mml:mi><mml:mn mathvariant="normal">10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>N</mml:mi><mml:mo>/</mml:mo><mml:mi>log⁡</mml:mi><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>)
for <inline-formula><mml:math id="M253" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> in reciprocal cubic centimetres. Points signify normalized sulfuric acid concentration
(right axis) as measured by CI-APi-ToF-MS.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/19/14933/2019/acp-19-14933-2019-f06.png"/>

        </fig>

      <p id="d1e3946">The second day plotted in Fig. 5b (25 June 2017) shows a
strong afternoon peak to the HOMs (for most HOMs, stronger than that on the
day prior). Particle formation is shown in the PSM data. A strong midday
peak to particle number is seen with two distinct peaks in cluster count.
These two peaks are not coincidental with the two peaks in HOM signal (i.e.
nitrogen-containing HOMs in Fig. 3a peaking at 11:00 and 16:00 CST). Sulfuric
acid, however, does peak synchronously with the particle number count.
Sulfuric acid is plotted across the contour plot in Fig. 6, where PSM data
are also shown in the bottom panel. The peak in CI-APi-ToF-MS mass signal,
visible in Fig. 5, occurs at around 12:00–13:00 CST; peaks in the PSM cluster
count occur at 10:00 and 13:00 CST. Peaks in mass up to 550 <inline-formula><mml:math id="M254" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>Q</mml:mi></mml:mrow></mml:math></inline-formula> are seen in the
CI-APi-ToF-MS at 13:00 CST. Assuming the density of these species is <inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:mo>≤</mml:mo><mml:mn mathvariant="normal">1.6</mml:mn></mml:mrow></mml:math></inline-formula> g cm<inline-formula><mml:math id="M256" 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>, then these will be suitably sized to be grown in the PSM
saturator. These newly formed<?pagebreak page14942?> particles then go on to grow and contribute
significantly to the larger particle count (Fig. S3). As initial particle
formation coincides with sulfuric acid signal peaks and before HOM signals
peak, it can be assumed on these days that the HOM contribution to the initial
particle formation is modest.</p>
      <p id="d1e3983">There is recent strong evidence to suggest that the driving force of the
earliest stages of particle formation in urban Shanghai is sulfuric
acid and <inline-formula><mml:math id="M257" 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:mrow></mml:math></inline-formula> amines (Yao et al., 2018), and the coincidental peaks of
sulfuric acid with new particles as seen in Fig. 6 suggest a similar
behaviour. Dimethylamine (DMA) can efficiently stabilize the sulfuric acid
clusters (Almeida et al., 2013). Here, few larger sulfuric acid–DMA clusters
were visible in the dataset, as seen in the work by Yao et al. (2018).
Although five sulfuric acid–dimethylamine (SA–DMA) ions were observed, the
others were likely too low in signal to be confidently resolved from their
neighbouring peaks; however, clusters of up to four sulfuric acid molecules and
three dimethylamine molecules were seen, with similar diurnal trends in sulfuric
acid. The scarcity of SA–DMA clusters is likely due to instrumental
conditions, rather than their absence in the atmosphere. The nitrate
chemical ionization system tends to evaporate amine compounds upon charging,
and as specific voltage-tuning setups can lend themselves towards
preservation or breakage of molecular clusters, the signal for larger
sulfuric acid clusters was also very weak. The formation of HOM–sulfuric
acid clusters is unlikely under atmospheric conditions (Elm et al., 2017)
and few of these were observed. Signals of HOMs seem to coincide with later
particle growth; it can be expected that HOM molecules make a more
significant contribution to particle growth than to early particle
formation, with the largest and most oxidized being involved in early
growth and the smaller and less oxidized contributing to later growth as
the necessary vapour pressure properties become less demanding.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <label>4</label><title>Conclusions</title>
      <p id="d1e4006">The average degree of HOM oxidation in Beijing is comparable with that seen
in other environments. Rapid intramolecular hydrogen shifts during
autoxidation due to the higher temperatures are probably offset by the
frequent termination reactions due to high <inline-formula><mml:math id="M258" 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> concentrations.
OS<inline-formula><mml:math id="M259" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msub></mml:math></inline-formula> values seem to be marginally higher for biogenic species.</p>
      <p id="d1e4029">The temporal trend of nearly every HOM shows afternoon or evening maxima.
Both <inline-formula><mml:math id="M260" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M261" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi mathvariant="normal" class="Radical">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> have high daytime concentrations, and these
likely drive the initial oxidation steps. The species arising from
alkylbenzene precursors show sharper afternoon peaks, probably since their
oxidation is <inline-formula><mml:math id="M262" display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">OH</mml:mi><mml:mi class="Radical" mathvariant="normal">⚫</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula>-dominated. Many of the rest of the peaks,<?pagebreak page14943?> coming
from largely BVOC precursors, show broader daytime peaks, being influenced by
<inline-formula><mml:math id="M263" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> also. There seems to be no direct link between VOC concentrations
and HOM signals, with days of lower precursor VOC sometimes having higher
HOM signals and vice versa.</p>
      <p id="d1e4076">Initial particle formation coincides with peak sulfuric acid signals, while
the growth of the particles correlates more closely with the signals of
HOMs. This is very similar to behaviour observed in a study of NPF in
Shanghai which was attributed to sulfuric acid–dimethylamine–water
nucleation with condensing organic species contributing to particle growth
(Yao et al., 2018), and this is further backed up by numerous SA–DMA
clusters present in this dataset. The freshly formed particles grow and
contribute significantly to total particle loading. This is visible when the
unit mass CI-APi-ToF-MS data are plotted as a contour plot, and further this
is visible in the PSM data, with bursts in both total number count
<inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1.30</mml:mn></mml:mrow></mml:math></inline-formula> nm and the number of molecular clusters between 1.30 and
1.84 nm. As <inline-formula><mml:math id="M265" 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> levels fall in Beijing due to traffic emission
control measures being enforced, it is likely that autoxidation will become
increasingly significant in the new particle formation processes. The number
of molecules detected by the <inline-formula><mml:math id="M266" 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> CI-APi-ToF-MS is undoubtedly many more
than have had formulae assigned here, but to identify more requires a more
sophisticated data deconvolution.</p>
</sec>

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

      <p id="d1e4118">Data supporting this publication are openly available from the UBIRA eData
repository at <ext-link xlink:href="https://doi.org/10.25500/edata.bham.00000304" ext-link-type="DOI">10.25500/edata.bham.00000304</ext-link> (Brean and Harrison, 2019).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e4124">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-19-14933-2019-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-19-14933-2019-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e4133">The study was conceived and planned by RMH and ZS. DCSB and JB set up and
operated the main instrumental measurements, and JB prepared the first draft
of the paper and responded to comments from RMH and ZS. CNH and WJFA
contributed the hydrocarbon data and provided comments on the draft
paper, and FAS and JL contributed the gas-phase pollutant data.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e4139">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e4145">This article is part of the special issue “In-depth study of air pollution sources and processes within Beijing and its surrounding region (APHH-Beijing) (ACP/AMT inter-journal SI)”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4151">This was part of the APHH-Beijing programme funded by the UK Natural
Environmental Research Council, the National Centre for Atmospheric Science, and the Natural Sciences
Funding Council of China. We thank Xinming Wang from the Guangzhou Institute of Geochemistry, Chinese Academy of
Sciences; Brian Davison from Lancaster University; and Ben Langford, Eiko Nemitz, Neil Mullinger, and other staff from the Centre for Ecology and
Hydrology, Edinburgh for assistance with the VOC measurements and associated
infrastructure.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e4156">This research has been supported by the Natural Environmental Research Council (grant no. NE/N007190/1) and the Natural Sciences Funding Council of China. It was additionally facilitated by the National Centre for Atmospheric Science ODA national capability programme ACREW (NE/R000034/1), which is supported by NERC and the GCRF.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e4162">This paper was edited by Kimitaka Kawamura and reviewed by three anonymous referees.</p>
  </notes><ref-list>
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<abstract-html><p>Particle nucleation is one of the main sources of atmospheric particulate
matter by number, with new particles having great relevance for human health
and climate. Highly oxidized multifunctional organic molecules (HOMs) have
been recently identified as key constituents in the growth and, sometimes,
in initial formation of new particles. While there have been many studies of
HOMs in atmospheric chambers, flow tubes, and clean environments, analyses of
data from polluted environments are scarce. Here, measurements of HOMs and
particle size distributions down to small molecular clusters are presented
alongside volatile organic compounds (VOCs) and trace-gas data from a
campaign in June 2017, in Beijing. Many gas-phase HOMs have been
characterized and their temporal trends and behaviours analysed in the
context of new particle formation. The HOMs identified have a
degree of oxidation comparable to that seen in other, cleaner, environments, likely
due to an interplay between the higher temperatures facilitating rapid
hydrogen abstractions and the higher concentrations of NO<sub><i>x</i></sub> and other
RO<sub>2</sub><sup>⚫</sup> terminators ending the autoxidation sequence more rapidly.
Our data indicate that alkylbenzenes, monoterpenes, and isoprene are
important precursor VOCs for HOMs in Beijing. Many of the C<sub>5</sub> and
C<sub>10</sub> compounds derived from isoprene and monoterpenes have a slightly
greater degree of average oxidation state of carbon compared to those from
other precursors. Most HOMs except for large dimers have daytime peak
concentrations, indicating the importance of OH<sup>⚫</sup> chemistry in the
formation of HOMs, as O<sub>3</sub> tends to be lower on days with higher HOM
concentrations; similarly, VOC concentrations are lower on the days with
higher HOM concentrations. The daytime peaks of HOMs coincide with the
growth of freshly formed new particles, and their initial formation
coincides with the peak in sulfuric acid vapours, suggesting that the
nucleation process is sulfuric-acid-dependent, with HOMs contributing to
subsequent particle growth.</p></abstract-html>
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