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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-18-17437-2018</article-id><title-group><article-title>Vertical characterization of highly oxygenated molecules (HOMs) below and
above a boreal forest canopy</article-title><alt-title>Vertical characterization of HOMs below and above a boreal forest canopy</alt-title>
      </title-group><?xmltex \runningtitle{Vertical characterization of HOMs below and above a boreal forest canopy}?><?xmltex \runningauthor{Q. Zha et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Zha</surname><given-names>Qiaozhi</given-names></name>
          <email>qiaozhi.zha@helsinki.fi</email>
        <ext-link>https://orcid.org/0000-0001-6301-7086</ext-link></contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Yan</surname><given-names>Chao</given-names></name>
          <email>chao.yan@helsinki.fi</email>
        <ext-link>https://orcid.org/0000-0002-5735-9597</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Junninen</surname><given-names>Heikki</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Riva</surname><given-names>Matthieu</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0054-4131</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sarnela</surname><given-names>Nina</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Aalto</surname><given-names>Juho</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Quéléver</surname><given-names>Lauriane</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Schallhart</surname><given-names>Simon</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dada</surname><given-names>Lubna</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1105-9043</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Heikkinen</surname><given-names>Liine</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7837-967X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Peräkylä</surname><given-names>Otso</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2089-0106</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Zou</surname><given-names>Jun</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Rose</surname><given-names>Clémence</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wang</surname><given-names>Yonghong</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2498-9143</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Mammarella</surname><given-names>Ivan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4 aff5">
          <name><surname>Katul</surname><given-names>Gabriel</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9768-3693</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Vesala</surname><given-names>Timo</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff6">
          <name><surname>Worsnop</surname><given-names>Douglas R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Kulmala</surname><given-names>Markku</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3464-7825</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Petäjä</surname><given-names>Tuukka</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1881-9044</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bianchi</surname><given-names>Federico</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2996-3604</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ehn</surname><given-names>Mikael</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0215-4893</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institute for Atmospheric and Earth System Research/Physics, Faculty of Science, University of Helsinki,<?xmltex \hack{\break}?> P.O. Box 64, 00014 Helsinki, Finland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>CMA-NJU Joint Laboratory for Climate Prediction Studies, Institute for Climate and Global Change Research,<?xmltex \hack{\break}?> School of Atmospheric Sciences, Nanjing University, Nanjing, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute for Atmospheric and Earth System Research/Physics, Faculty of Science, University of Helsinki,<?xmltex \hack{\break}?> P.O. Box 68, 00014 Helsinki, Finland</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Nicholas School of the Environment, Duke University, Durham, North Carolina, USA</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Civil and Environmental Engineering, Duke University, Durham, North Carolina, USA</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>Aerodyne Research, Inc., Billerica, MA 01821, USA</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Qiaozhi Zha (qiaozhi.zha@helsinki.fi) and Chao Yan (chao.yan@helsinki.fi)</corresp></author-notes><pub-date><day>10</day><month>December</month><year>2018</year></pub-date>
      
      <volume>18</volume>
      <issue>23</issue>
      <fpage>17437</fpage><lpage>17450</lpage>
      <history>
        <date date-type="received"><day>24</day><month>November</month><year>2017</year></date>
           <date date-type="rev-request"><day>8</day><month>December</month><year>2017</year></date>
           <date date-type="rev-recd"><day>28</day><month>August</month><year>2018</year></date>
           <date date-type="accepted"><day>30</day><month>October</month><year>2018</year></date>
      </history>
      <permissions>
        
        
      <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/18/17437/2018/acp-18-17437-2018.html">This article is available from https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018.pdf</self-uri>
      <abstract>
    <p id="d1e315">While the role of highly oxygenated molecules (HOMs) in new particle
formation (NPF) and secondary organic aerosol (SOA) formation is not in
dispute, the interplay between HOM chemistry and atmospheric conditions
continues to draw significant research attention. During the Influence of
Biosphere-Atmosphere Interactions on the Reactive Nitrogen budget (IBAIRN)
campaign in September 2016, profile measurements of neutral HOMs below and
above the forest canopy were performed for the first time at the boreal
forest SMEAR II station. The HOM concentrations and composition distributions
below and above the canopy were similar during daytime, supporting a
well-mixed boundary layer approximation. However, much lower nighttime HOM
concentrations were frequently observed at ground level, which was likely due
to the formation of a shallow decoupled layer below the canopy. Near the
ground HOMs were influenced by the changes in the precursors and oxidants and
enhancement of the loss on surfaces in this layer, while the HOMs above the
canopy top were not significantly affected. Our findings clearly illustrate
that near-ground HOM measurements conducted under stably stratified
conditions at this site might only be representative of a small fraction of
the entire nocturnal boundary layer. This could, in turn, influence the
growth of newly formed particles and SOA formation below the canopy where the
large majority of measurements are typically conducted.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p id="d1e325">Highly oxygenated molecules (HOMs), a subgroup of the oxidation products of
volatile organic compounds (VOCs) identified by their high oxidation states,
have been recognized as important precursors for organic aerosol in the
atmosphere (Ehn et al., 2014). They have also been found
to enhance new particle formation (NPF) and growth (Kulmala
et al., 2013; Zhao et al., 2013; Ehn et al., 2014; Bianchi et al., 2016;
Kirkby et al., 2016; Tröstl et al., 2016). The importance of HOMs has
been confirmed in ambient environments, especially in monoterpene-dominated
regions such as the boreal forest (Kulmala et al., 2013; Ehn et al.,
2014), but also in high-altitude mountain regions (Bianchi et
al., 2016) and in rural areas (Jokinen et al., 2014;
Kürten et al., 2016). In laboratory studies, HOM formation has been
observed from<?pagebreak page17438?> various precursor molecules (Ehn
et al., 2017), including both biogenic and anthropogenic emissions (Molteni et al., 2018).</p>
      <p id="d1e328">The direct observation of HOMs has only recently become possible, following
the developments of the atmospheric-pressure-interface time-of-flight
(APi-TOF, measures the naturally charged HOMs) (Junninen et al., 2010) and chemical-ionization
atmospheric-pressure-interface time-of-flight (CI-APi-TOF, measures the
neutral HOMs) (Jokinen et al., 2012) mass
spectrometers. Ehn et al. (2010) and Bianchi et al. (2017)
found that the naturally charged HOM clusters could be observed every night
in the boreal forest during spring. Out of the observed ambient mass
spectra, a significant part could be reproduced in a chamber by introducing
the monoterpene <inline-formula><mml:math id="M1" display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>-pinene (<inline-formula><mml:math id="M2" 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:mrow></mml:math></inline-formula>, the major biogenic VOC
in the boreal forest) and ozone (<inline-formula><mml:math id="M3" 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>) (Ehn
et al., 2012).</p>
      <p id="d1e365">Further investigations of HOM formation chemistry have been carried out in
both laboratory and field studies. Based on current understanding from
laboratory experiments, the formation of HOMs involves three main steps:
(1) initial formation of peroxy radicals (<inline-formula><mml:math id="M4" 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>) from VOC oxidation;
(2) <inline-formula><mml:math id="M5" 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> autoxidation, that is, the isomerization of the
<inline-formula><mml:math id="M6" 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> via intramolecular H shifts and subsequent oxygen
(<inline-formula><mml:math id="M7" 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 (3) radical termination, forming closed-shell
molecules (Crounse et al., 2013; Ehn et al., 2014; Jokinen et al., 2014,
2016; Rissanen et al., 2014; Mentel et al., 2015). In the atmosphere, HOM
formation studies are complicated by the plethora of different compounds and
processes taking place. However, recent ambient measurements together with
factor analysis were able to shed light on the HOM formation pathways in the
boreal forest (Yan et al., 2016). They showed that the majority of the
daytime production of HOMs was from reactions initiated by the oxidation of
monoterpenes (MTs) with hydroxyl radicals (OH) or <inline-formula><mml:math id="M8" 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>. The
<inline-formula><mml:math id="M9" 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> after autoxidation were often terminated by hydroperoxyl
radicals (<inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) or self-termination (Orlando and Tyndall, 2012) to
form a non-nitrate HOM monomer (CHO<inline-formula><mml:math id="M11" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula>, mainly <inline-formula><mml:math id="M12" 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>
and <inline-formula><mml:math id="M13" 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, with masses between 290 and
450 Th after clustering with the charging
ion (<inline-formula><mml:math id="M14" 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>) of the instrument), or reacting with nitrogen oxides
(<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow><mml:mo>=</mml:mo><mml:mrow class="chem"><mml:mi mathvariant="normal">NO</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:mrow></mml:math></inline-formula>) to form organonitrate HOM monomers
(CHON<inline-formula><mml:math id="M16" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula>). During nighttime, MTs were mainly oxidized by <inline-formula><mml:math id="M17" 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="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> radicals. Furthermore, due to the lower nocturnal <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M20" 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 addition to the production of CHON<inline-formula><mml:math id="M21" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula>, the
<inline-formula><mml:math id="M22" 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> products readily reacted with other <inline-formula><mml:math id="M23" 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> to form either
non-nitrate HOM dimers (CHO<inline-formula><mml:math id="M24" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula>, mainly <inline-formula><mml:math id="M25" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mrow><mml:mn mathvariant="normal">16</mml:mn><mml:mtext>–</mml:mtext><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> compounds with
masses between 450 and 600 Th after clustering with <inline-formula><mml:math id="M26" 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>) or
organonitrate HOM dimers (CHON<inline-formula><mml:math id="M27" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula>), depending on the oxidants forming
the <inline-formula><mml:math id="M28" 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> (Ehn
et al., 2014; Jokinen et al., 2014; Yan et al., 2016; Berndt et al., 2018).</p>
      <p id="d1e660">Beyond those chemical pathways, varied meteorological conditions are also
factors influencing the MT and oxidants at different heights above the
forest floor. Unsurprisingly, the oxidants producing HOMs (e.g., <inline-formula><mml:math id="M29" 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>)
have been found almost uniformly distributed within the well-mixed daytime
boundary layer (Chen et al., 2018). In contrast,
the nocturnal boundary layer was shallow with stability regimes that
depended on radiative cooling within the canopy and turbulent shear stresses
at the canopy top. In Hyytiälä, the depletion of <inline-formula><mml:math id="M30" 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> below the
canopy has been frequently observed during nighttime, while the <inline-formula><mml:math id="M31" 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>
above the canopy was less affected (Chen et al.,
2018). The MT concentration at ground level increased when <inline-formula><mml:math id="M32" 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> was
depleted (Eerdekens et al., 2009). The
inhomogeneous distribution of the precursors and oxidants below and above
the canopy might further impact nocturnal HOM distributions, which frames
the scope of this study. Until now, all CI-APi-TOF deployments have been at
ground level, and the main subject of inquiry here is the vertical
information on HOMs and the role of meteorological condition in shaping
them. A characterization of the HOMs at different heights provides a
decisive advantage in disentangling the role of nonuniform mixing within
the atmospheric layers impacted by strong thermal stratification, especially
inside the canopy volume.</p>
      <p id="d1e708">The first measurements of the HOM concentrations at two different heights
(36 m and 1.5 m a.g.l.) are presented and discussed. The influence of
boundary layer dynamics on the HOMs at these different heights at SMEAR II
station is analyzed and characterized in conjunction with auxiliary
turbulence and micrometeorological measurements.</p>
</sec>
<sec id="Ch1.S2">
  <title>Experimental</title>
<sec id="Ch1.S2.SS1">
  <title>Measurement site description</title>
      <p id="d1e722">The measurements were performed at the SMEAR II station (Station for
Measuring Ecosystem–Atmosphere Relations) in the boreal forest in
Hyytiälä, southern Finland (61<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>51<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> N, 24<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>17<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula> E,
181 m a.s.l.; Hari and Kulmala, 2005; Hari et al., 2013) during September
2016. There is no large anthropogenic emission source at or near the site.
The closest sources are the two sawmills <inline-formula><mml:math id="M37" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">5</mml:mn></mml:mrow></mml:math></inline-formula> km southeast of the site
and the city area of Tampere (<inline-formula><mml:math id="M38" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> km away). The forest surrounding the
station is primarily Scots pine with a mean canopy height of <inline-formula><mml:math id="M39" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">17.5</mml:mn></mml:mrow></mml:math></inline-formula> m,
a total leaf area index (LAI) of <inline-formula><mml:math id="M40" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">6.5</mml:mn></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>m<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, a stand density
of <inline-formula><mml:math id="M43" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1400</mml:mn></mml:mrow></mml:math></inline-formula> trees ha<inline-formula><mml:math id="M44" 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 an average diameter at breast height
(DBH) of <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.16</mml:mn></mml:mrow></mml:math></inline-formula> m (Bäck et al., 2012; Launiainen et al., 2013). The
forest floor is majorly covered with a shallow dwarf shrub (a LAI of <inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>m<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and moss layer (a LAI of <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula>m<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)
(Kulmala et al., 2008; Launiainen et al., 2013). The planetary boundary layer
height at the SMEAR II station has been determined from previous studies
using radiosondes (Lauros et al., 2007; Ouwersloot et al., 2012) and balloon
soundings (Eerdekens et al., 2009). Roughly, these heights span some 400 m
(March) to 1700 m (August) at noontime and 100 m (March) to <inline-formula><mml:math id="M52" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">160</mml:mn></mml:mrow></mml:math></inline-formula> m
(April) at midnight.</p><?xmltex \hack{\newpage}?>
</sec>
<?pagebreak page17439?><sec id="Ch1.S2.SS2">
  <title>Instrumentation</title>
      <p id="d1e936">Concentration of HOMs was measured with two nitrate-ion-based CI-APi-TOF mass
spectrometers. The CI-APi-TOF measuring at higher altitude was deployed at
the top of a 35 m tower located <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> m horizontally from the ground
measurement location. Both instruments were working in rooms with
air-conditioning and room temperatures controlled at 25 <inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C. The
inlets of the two instruments were pointed to the southeast direction and
fixed at <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">36</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.5</mml:mn></mml:mrow></mml:math></inline-formula> m above ground. The tower measurement is
at about twice the canopy height, which is still within the roughness
sublayer of the forest (Raupach and Thom, 1981). The instrument setup of the
two CI-APi-TOF mass spectrometers was similar. In brief, the CI-APi-TOF was
the combination of a chemical ionization (CI) inlet and an APi-TOF mass
spectrometer (Aerodyne Research Inc., USA, and Tofwerk AG, Switzerland). The
ambient air was first drawn into the inlet with a sample flow of
7 L min<inline-formula><mml:math id="M57" 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> (liter per minute) and then centered to an ion reaction tube
surrounded by sheath flow (filtered air, 35 L min<inline-formula><mml:math id="M58" 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>). Meanwhile, the
nitrate ions carried by the sheath gas, which were generated by exposing the
nitric acid (<inline-formula><mml:math id="M59" 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>) to soft X-ray radiation, were guided into the
sample gas by an electrical field at ambient pressure (<inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> ms
reaction time). Neutral molecules (<inline-formula><mml:math id="M61" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>) in the sample air were ionized by
either clustering with charged nitrate <inline-formula><mml:math id="M62" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> nitric acid
(<inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mo>(</mml:mo><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:msub><mml:mo>)</mml:mo><mml:mrow><mml:mi>n</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msub><mml:mo>⋅</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:mrow></mml:math></inline-formula>) to form <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi>M</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:mrow></mml:math></inline-formula> cluster ions or losing a proton to the charging ions to
form deprotonated ions (e.g., <inline-formula><mml:math id="M65" display="inline"><mml:mrow><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:mo>+</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><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:mo>+</mml:mo><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:mrow></mml:math></inline-formula>). The ions then entered the APi part,
which was a three-stage vacuum chamber, through a pinhole. In the APi, two
quadrupoles and a stack of ion lenses guided the ions into the TOF mass
analyzer, in which ions were separated based on their mass-to-charge (<inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula>)
ratios. A more detailed description of this instrument has been given by
Junninen et al. (2010) and Jokinen et al. (2012), and discussion on
selectivity of this nitrate ion charging was provided by Hyttinen et
al. (2015). Mass spectra obtained from the instrument were analyzed using the
“tofTools” program described in Junninen et al. (2010). Determination of
the concentration of a measured molecule <inline-formula><mml:math id="M67" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula> was based on the following
equation:
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M68" display="block"><mml:mrow><mml:mfenced close="]" open="["><mml:mi>M</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∑</mml:mo><mml:mi>M</mml:mi></mml:mrow><mml:mrow><mml:mo>∑</mml:mo><mml:mi mathvariant="normal">reagent</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">ion</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">count</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">rates</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>×</mml:mo><mml:mi>C</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where the sum of ion count rates (<inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>∑</mml:mo><mml:mi>M</mml:mi></mml:mrow></mml:math></inline-formula>) in the numerator includes all
detected ions relating to compound <inline-formula><mml:math id="M70" display="inline"><mml:mi>M</mml:mi></mml:math></inline-formula>, whether deprotonated or in clusters
with reagent ions, and the sum of reagent ion count rates in the denominator
is the total signal of the nitrate ions. <inline-formula><mml:math id="M71" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is the calibration coefficient,
which was assigned the same value for all detected compounds. This
assignment is only valid for compounds that cluster with the reagent ions at
the collision limit, such as <inline-formula><mml:math id="M72" 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> (Viggiano et al., 1997), and have equal
collision rates. The collision rates of nitrate ions with <inline-formula><mml:math id="M73" 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>
and with HOMs are expected to be very close (Ehn et al., 2014). Here, a
calibration coefficient of <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">10</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec cm<inline-formula><mml:math id="M75" 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>, estimated
from previous calibrations with similar settings using sulfuric acid and
theoretical constraints (Ehn et al., 2014), with an
uncertainty of at least <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">50</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi><mml:mo>/</mml:mo><mml:mo>+</mml:mo><mml:mn mathvariant="normal">100</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula>, was used in calculating the HOM
concentrations for both instruments. Ultimately, the absolute HOM
concentrations in this work are of secondary importance, as we focus on the
relative comparison of HOM concentrations measured at different heights.
However, the comparability of the two CI-APi-TOF instruments is of great
importance, and results cannot be allowed to vary as a result of
inevitable differences in the mass-dependent transmission efficiency (TE), for example.
For a detailed discussion on factors affecting the TE of a CI-APi-TOF, we
refer to Heinritzi et al. (2016). To
this end, instead of directly evaluating the TE of each instrument, a
“relative” TE of the two CI-APi-TOFs was used for data correction: we
selected a time period at noontime on 9 September with a well-mixed
boundary layer, identified by the clear and sunny weather and homogeneous
vertical distribution of monoterpene and other trace gases, and we assumed the
HOM concentrations at the two heights to be the same. Thus, the relative TE
was obtained from the concentration ratio between the two CI-APi-TOFs at
each <inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> (Fig. 1). A fitted relative TE curve (<inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.97</mml:mn></mml:mrow></mml:math></inline-formula>), which
represents how the TE of the tower CI-APi-TOF was changed at each <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> over
the TE of the ground one, was obtained using power-law regression. Weaker
correlation was obtained in the 200–250 and 500–600 Th mass ranges, but in
the mass range in which most of the HOMs were located (290–500 Th) there is
very little scatter around the fitted curve, clearly suggesting that
observed differences in the two instruments' responses were mainly due to
differences in TE. To test our assumption of negligible vertical gradients
of HOMs during daytime, we analyzed the behavior of sulfuric acid. We found
that the uncertainty related to this assumption corresponds to a value of
26 % (see Fig. S1 in the Supplement). An upper limit of uncertainty relating to our TE
correction (Fig. 1) was also estimated, yielding a value of 10 %, giving
a total uncertainty from these two sources of 28 %. This value is much
smaller than the observed deviation of HOM concentrations during inversion
nights, as will be discussed later. Additionally, an intercomparison
between the two instruments with a permeation tube containing
trinitrotriazinane (<inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">C</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">6</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>) was conducted in the field
right after the campaign. The results showed good agreement with the
relative TE, lending confidence to the method used here. Finally, it should
be noted that the difference in TE between the two instruments was larger
than one would normally expect since the tower CI-APi-TOF had been tuned
for higher sensitivity at the largest masses (at the expense of transmission
at the lower masses).</p>
      <p id="d1e1373">In comparison to the direct determination of TE (Heinritzi et al., 2016), this method
increases the uncertainty in the quantification of HOM concentrations.
However, as mentioned, a more accurate knowledge of the exact<?pagebreak page17440?> HOM
concentrations would not influence the main findings of this study.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p id="d1e1378">The relative transmission curve between the two CI-APi-TOF mass
spectrometers, determined during a period of strong turbulent mixing.
Intercomparison results using a permeation tube containing
trinitrotriazinane (<inline-formula><mml:math id="M81" 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">6</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">6</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>) are shown in red circles.
The fitted green line was used to scale the measured signals between the two
instruments to match, in order to compare relative changes during times of
limited vertical mixing.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f01.png"/>

        </fig>

      <p id="d1e1413">The MT, trace gases, and meteorological parameters were continuously
monitored at the different heights (4.2, 8.4, 16.8, 33.6, 50.4,
67.2, 101, and 125 m) on a 126 m mast <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> m away from the
location of the CI-APi-TOFs. The data at 4.2 and 33.6 m were used in this
study to represent the concentrations at near ground and tower levels,
respectively. MT concentrations were measured every third hour using a
proton transfer reaction mass spectrometer with a lower detection limit of 1 pptv (PTR-MS, Ionicon
Analytik GmbH; Taipale et al., 2008). The <inline-formula><mml:math id="M83" 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> concentration was measured
with a UV light absorption analyzer that had a lower detection limit of 1 ppbv (TEI model 49C, Thermo Fisher Scientific, USA). The <inline-formula><mml:math id="M84" 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>
measurement was conducted using a chemiluminescence analyzer (TEI model 42C
TL, Thermo Fisher Scientific, USA). The lower detection limit of the
<inline-formula><mml:math id="M85" 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> analyzer is 100 pptv. The <inline-formula><mml:math id="M86" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurement was performed using
an infrared detection system (LI-840, LI-COR Biosciences, Lincoln, NE, USA).
The aerosol number concentration size distributions were obtained with a
twin differential mobility particle sizer (twin DMPS) for the size range
from 3 to 1000 nm (Aalto et al., 2001) at 8 m in
height above ground, and was used to calculate condensation sink (CS) based
on the method from Kulmala et
al. (2001). Air temperature was measured with PT-100 resistance
thermometers. Air relative humidity (RH) was measured with RH sensors
(Rotronic HygroMet model MP102H with HygroClip HC2S3, Rotronic AG,
Switzerland). Global radiation (solar radiation in the wavelength range of
0.3–4.8 <inline-formula><mml:math id="M87" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m) was obtained with a Pyranometer (Reemann TP3, Astrodata,
Estonia) above the canopy top at 18 m. All the data presented are at 10 min
averaging intervals, except for the MT (at a 1 h averaging interval). A
schematic figure showing sampling locations of all the measured parameters
is provided in Fig. S2.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <title>Data overview</title>
      <p id="d1e1490">The Influence of Biosphere-Atmosphere Interactions on the Reactive Nitrogen
budget (IBAIRN) campaign was conducted from 1 to 25 September 2016. After
data quality checks, only the measurements collected after 5 September were
used. Figure 2 shows the overall time series of the meteorological parameters
measured at ground and tower levels, including the temperature, RH, global
radiation, concentrations of trace gases, MT, and total HOMs (Zha, 2018). The
weather was generally sunny and clear during the campaign except for a few
cloudy (10, 15, and 22–23 September) and drizzling (24 and 25 September)
days. The mean air temperature and RH observed at ground level were <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.8</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3.3</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M89" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and <inline-formula><mml:math id="M90" display="inline"><mml:mrow><mml:mn mathvariant="normal">87</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">13</mml:mn></mml:mrow></mml:math></inline-formula> % (1<inline-formula><mml:math id="M91" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> standard deviation) and at
the tower level were <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3.0</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M93" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C and <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mn mathvariant="normal">88</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula> %,
respectively. The <inline-formula><mml:math id="M95" 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> concentrations measured at ground and tower
levels were <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:mn mathvariant="normal">21</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:mn mathvariant="normal">25</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> ppbv, respectively. The air
temperature, RH, and <inline-formula><mml:math id="M98" 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> measured at the two heights were close to
each other during daytime. The <inline-formula><mml:math id="M99" 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 were quite
low throughout the campaign; the mean <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
were mostly around the reported detection limit at <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula> ppbv
(ground) and <inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> ppbv (tower), yet showed an overall good
agreement between the measurements at the different heights. The MT
concentrations at ground level (<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.38</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.34</mml:mn></mml:mrow></mml:math></inline-formula> ppbv on average) were
generally higher than those above the canopy level (<inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.20</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.16</mml:mn></mml:mrow></mml:math></inline-formula> ppbv).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p id="d1e1686">The overall time series of the measured trace gases, meteorological
parameters, and estimated total HOM concentrations at the ground (blue) and
tower (red) levels.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f02.pdf"/>

        </fig>

      <p id="d1e1695">The estimated total HOM concentration is representative for the overall
concentration level of HOMs and is here defined as the sum of the detected
signals among ions from <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 200 to 600 after removing identified background
peaks. The gaps in the estimated total HOM at ground level were due to
automatic zero checks. During the campaign, a significant difference was
found in the estimated total HOM concentrations below and above the canopy
(mean and median concentrations of <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.7</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> and <inline-formula><mml:math id="M107" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.8</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="M108" 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> at ground level and <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.7</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.3</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> and <inline-formula><mml:math id="M110" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.3</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="M111" 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> at
tower level). The causes of these differences (<inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">55</mml:mn></mml:mrow></mml:math></inline-formula> % in
mean and <inline-formula><mml:math id="M113" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">71</mml:mn></mml:mrow></mml:math></inline-formula> % in median) frame the upcoming discussion.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Intercomparison of estimated total HOM concentrations</title>
      <p id="d1e1829">The estimated total HOM concentrations at the two heights were not different
during the day (mean <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> standard deviation and median
concentrations of <inline-formula><mml:math id="M115" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.1</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.3</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> and <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mn mathvariant="normal">3.6</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="M117" 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> at ground level, <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.6</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> and <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mn mathvariant="normal">4.0</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="M120" 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> at tower level),
which validates the use of only 1 day of data for scaling the TE of the
ground CI-APi-TOF to<?pagebreak page17441?> match the HOM signals of the two instruments. The good
daytime agreement throughout the campaign period also verifies that the
response of each instrument stayed stable. Contrary to the daytime results,
the estimated total HOM concentration at ground level usually diverged from
the tower measurement in the nocturnal boundary layer. The concentration
below the canopy became even lower when temperature inversions were
observed, accompanied by a decreasing ground-level <inline-formula><mml:math id="M121" 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 increasing MT
concentrations. Figure 3 shows a comparison between the estimated total HOM
concentrations observed at two heights. Herein, good agreement could be
found for the group of points representing the concentrations around
noontime (<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.89</mml:mn></mml:mrow></mml:math></inline-formula>). The points indicating the nighttime estimated
total HOM concentrations were scattered (<inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.28</mml:mn></mml:mrow></mml:math></inline-formula>), and the ground
concentrations were found to be much lower than the tower ones.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p id="d1e1980">Comparison between ground (<inline-formula><mml:math id="M124" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis) and tower (<inline-formula><mml:math id="M125" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis)
measurements of the estimated total HOM concentrations. The black line
denotes the 1 : 1 ratio. Color code indicates the sampling time of HOMs.</p></caption>
          <?xmltex \igopts{width=184.942913pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f03.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p id="d1e2005">Mean mass spectra with the averaging periods of daytime
(09:00–15:00) and nighttime (21:00–03:00) at the ground and tower levels.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f04.pdf"/>

        </fig>

      <p id="d1e2015">Figure 4 shows the mean mass spectra (in unit mass resolution, UMR, for
<inline-formula><mml:math id="M126" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 200–600) obtained from the ground and tower. It is worth mentioning
that there might be some signals not attributable to HOMs in the plotted
spectra, but only as a small proportion. Only selected periods
(09:00–15:00 for daytime and
21:00–03:00 for nighttime; all the times are given in Finnish winter time, UTC <inline-formula><mml:math id="M127" display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 2) are included in
the averaging period to eliminate the effect of sunrise and sunset periods.
During daytime, a good agreement (<inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.87</mml:mn></mml:mrow></mml:math></inline-formula>) was obtained from the
mass-by-mass comparison using the UMR concentrations extracted from daytime
mean spectra, suggesting a uniform composition distribution in the daytime
boundary layer condition. During nighttime, the mean concentrations of all
HOMs in the ground mean spectra were much lower than the tower spectra. The
HOM concentrations shown in the ground and tower mean spectra were also less
correlated. Therefore, a logical outcome is that the conditions below and
above the canopy experience different<?pagebreak page17442?> turbulent mixing strength and/or
source–sink regimes during the night.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p id="d1e2055">Summary of the “Non-inversion night” and “Inversion night”
types.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.82}[.82]?><oasis:tgroup cols="12">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right" colsep="1"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:colspec colnum="10" colname="col10" align="right"/>
     <oasis:colspec colnum="11" colname="col11" align="right"/>
     <oasis:colspec colnum="12" colname="col12" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">Type </oasis:entry>
         <oasis:entry namest="col3" nameend="col7" align="center" colsep="1">Non-inversion night </oasis:entry>
         <oasis:entry namest="col8" nameend="col12" align="center">Inversion night </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col2">Date </oasis:entry>
         <oasis:entry namest="col3" nameend="col7" align="center" colsep="1">6, 7, 9, 11, 15, 16, 21 September<inline-formula><mml:math id="M131" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
         <oasis:entry namest="col8" nameend="col12" align="center">5, 8, 10, 12, 13, 14, 19 September<inline-formula><mml:math id="M132" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col2">Parameters </oasis:entry>
         <oasis:entry colname="col3">Temperature</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M133" 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></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M134" 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></oasis:entry>
         <oasis:entry colname="col6">MT</oasis:entry>
         <oasis:entry colname="col7">Estimated</oasis:entry>
         <oasis:entry colname="col8">Temperature</oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M135" 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></oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M136" 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></oasis:entry>
         <oasis:entry colname="col11">MT</oasis:entry>
         <oasis:entry colname="col12">Estimated</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">(<inline-formula><mml:math id="M137" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C)</oasis:entry>
         <oasis:entry colname="col4">(ppbv)</oasis:entry>
         <oasis:entry colname="col5">(ppbv)</oasis:entry>
         <oasis:entry colname="col6">(ppbv)</oasis:entry>
         <oasis:entry colname="col7">total HOM</oasis:entry>
         <oasis:entry colname="col8">(<inline-formula><mml:math id="M138" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C)</oasis:entry>
         <oasis:entry colname="col9">(ppbv)</oasis:entry>
         <oasis:entry colname="col10">(ppbv)</oasis:entry>
         <oasis:entry colname="col11">(ppbv)</oasis:entry>
         <oasis:entry colname="col12">total HOM</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7">(10<inline-formula><mml:math id="M139" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula> cm<inline-formula><mml:math id="M140" 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>)</oasis:entry>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
         <oasis:entry colname="col10"/>
         <oasis:entry colname="col11"/>
         <oasis:entry colname="col12">(10<inline-formula><mml:math id="M141" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">8</mml:mn></mml:msup></mml:math></inline-formula> cm<inline-formula><mml:math id="M142" 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>)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Tower</oasis:entry>
         <oasis:entry colname="col2">Mean <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> standard</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:mn mathvariant="normal">25</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.31</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.31</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.9</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.9</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M149" display="inline"><mml:mrow><mml:mn mathvariant="normal">9.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1.7</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M150" display="inline"><mml:mrow><mml:mn mathvariant="normal">24</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M151" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.3</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M152" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.24</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.04</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.8</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">deviation</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
         <oasis:entry colname="col10"/>
         <oasis:entry colname="col11"/>
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Median</oasis:entry>
         <oasis:entry colname="col3">10.9</oasis:entry>
         <oasis:entry colname="col4">24</oasis:entry>
         <oasis:entry colname="col5">0.4</oasis:entry>
         <oasis:entry colname="col6">0.17</oasis:entry>
         <oasis:entry colname="col7">2.8</oasis:entry>
         <oasis:entry colname="col8">9.2</oasis:entry>
         <oasis:entry colname="col9">23</oasis:entry>
         <oasis:entry colname="col10">0.3</oasis:entry>
         <oasis:entry colname="col11">0.23</oasis:entry>
         <oasis:entry colname="col12">2.3</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">Ground</oasis:entry>
         <oasis:entry colname="col2">Mean <inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> standard</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M155" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.7</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:mn mathvariant="normal">21</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.4</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M158" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.52</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.74</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7"><inline-formula><mml:math id="M159" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.6</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col8"><inline-formula><mml:math id="M160" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col9"><inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mn mathvariant="normal">16</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col10"><inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.3</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col11"><inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.70</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.28</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col12"><inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.8</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">deviation</oasis:entry>
         <oasis:entry colname="col3"/>
         <oasis:entry colname="col4"/>
         <oasis:entry colname="col5"/>
         <oasis:entry colname="col6"/>
         <oasis:entry colname="col7"/>
         <oasis:entry colname="col8"/>
         <oasis:entry colname="col9"/>
         <oasis:entry colname="col10"/>
         <oasis:entry colname="col11"/>
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Median</oasis:entry>
         <oasis:entry colname="col3">11.5</oasis:entry>
         <oasis:entry colname="col4">22</oasis:entry>
         <oasis:entry colname="col5">0.3</oasis:entry>
         <oasis:entry colname="col6">0.22</oasis:entry>
         <oasis:entry colname="col7">1.7</oasis:entry>
         <oasis:entry colname="col8">8.5</oasis:entry>
         <oasis:entry colname="col9">17</oasis:entry>
         <oasis:entry colname="col10">0.3</oasis:entry>
         <oasis:entry colname="col11">0.70</oasis:entry>
         <oasis:entry colname="col12">0.7</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><table-wrap-foot><p id="d1e2058"><inline-formula><mml:math id="M129" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> MT data not available on 5 and 19 September.
<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> MT data not available on 15 and 16 September.</p></table-wrap-foot></table-wrap>

</sec>
<sec id="Ch1.S3.SS3">
  <title>Influence of nocturnal boundary layer dynamics and micrometeorological
processes</title>
      <p id="d1e2811">The nighttime HOMs at ground level are likely influenced by transport
processes below the canopy since the estimated total HOM concentrations were
found much lower on the nights when temperature inversions were observed. To
further investigate the potential impact of such micrometeorological
phenomena on ground-level HOMs, the nights during the campaign without
precipitation or instrument failure were selected (14 nights in total) and
categorized into two types based on the occurrence of temperature inversions:
(1) the “non-inversion night” type included seven nights when no
temperature inversion was recorded; (2) the “inversion night” type category
consisted of seven nights that had encountered temperature inversions, and
the ground temperatures were generally <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M166" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C lower than tower
temperatures during these nights.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p id="d1e2835"><bold>(a)</bold> Time series of ground and tower concentrations of
<inline-formula><mml:math id="M167" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M168" 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="M169" 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>, MT, and selected HOM
groups in the selected non-inversion night (11 September) and
<bold>(b)</bold> inversion night (8 September) types. <italic>Ri</italic> is calculated
with the meteorology data of the ground and tower levels. CS is determined
based on the aerosol data measured at 8 m above ground level.</p></caption>
          <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f05.png"/>

        </fig>

<sec id="Ch1.S3.SS3.SSS1">
  <title>Statistics of the non-inversion night and inversion night
types</title>
      <p id="d1e2890">Table 1 shows the overall statistics including the mean and median values of
the temperatures, <inline-formula><mml:math id="M170" 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="M171" 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>, MT, and estimated total HOM
concentrations for the non-inversion night and inversion night
types. On the non-inversion nights, the air below and above the canopy was
relatively well mixed. The mean and median concentrations of the ground
<inline-formula><mml:math id="M172" 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="M173" display="inline"><mml:mrow><mml:mn mathvariant="normal">21</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">8</mml:mn></mml:mrow></mml:math></inline-formula> and 22 ppbv) were close to the tower values (<inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:mn mathvariant="normal">25</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:math></inline-formula> and 24 ppbv). The slight difference might be attributed to
the higher VOC emissions (Rantala et al.,
2014) and larger sink near ground level. In contrast, during the inversion
nights, the mean estimated total HOM concentration and <inline-formula><mml:math id="M175" 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> at ground
level were generally much lower, only <inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">33</mml:mn></mml:mrow></mml:math></inline-formula> % and
<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">69</mml:mn></mml:mrow></mml:math></inline-formula> % of the tower concentrations, respectively. Instead,
the mean and median ground MT concentration (<inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.70</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.28</mml:mn></mml:mrow></mml:math></inline-formula> and 0.70 ppbv) were <inline-formula><mml:math id="M179" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> times higher than the tower ones (<inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.24</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.04</mml:mn></mml:mrow></mml:math></inline-formula> and 0.23 ppbv). The measured <inline-formula><mml:math id="M181" 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 were
similar in both categories and at both heights, though the ambient concentrations
were close to the detection limit and therefore small differences might not
be observable.</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <title>Case study</title>
      <p id="d1e3034">Two individual nights representing the non-inversion night and inversion
night types were selected and further compared. Figure 5a shows the time
series of the meteorological parameters, trace gases, and HOMs measured at
ground and tower levels of one selected night for the non-inversion night
type (11–12 September, from 21:00 to 03:00). A
number of measures can be used to assess the local atmospheric stability
conditions at a given layer. These measures are commonly based on either the
Obukhov length and its associated atmospheric stability parameter or a
Richardson number (flux based, gradient based, or bulk). Because of its
simplicity and the availability of high-resolution mean air temperature
profiles, the bulk Richardson number (<italic>Ri</italic>) was used here (Mahrt et
al., 2001; Mammarella et al., 2007; Vickers et al., 2012; Alekseychik et al.,
2013). It is calculated using
              <disp-formula id="Ch1.E2" content-type="numbered"><mml:math id="M182" display="block"><mml:mrow><mml:mtext mathvariant="italic">Ri</mml:mtext><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>g</mml:mi><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi></mml:mrow><mml:mrow><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>(</mml:mo><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M183" display="inline"><mml:mi>g</mml:mi></mml:math></inline-formula> is the gravitational acceleration, <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> are the mean potential temperature (10 min averaging interval,
same as measurement data) and height difference between the ground and tower
levels, respectively, and <inline-formula><mml:math id="M186" display="inline"><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and <inline-formula><mml:math id="M187" display="inline"><mml:mover accent="true"><mml:mi>u</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> are the mean
potential temperature and mean wind velocity at tower level, respectively.
During the selected non-inversion night, <italic>Ri</italic> was generally positive but
close to 0 (shown in Fig. 5a), indicating a weakly stable and relatively
well-mixed (i.e., <inline-formula><mml:math id="M188" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mover accent="true"><mml:mi mathvariant="italic">θ</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mo>→</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> condition (Mahrt, 1998; Mammarella et al., 2007). This was
also confirmed using the well-correlated ground and tower MT and trace gas
concentrations.</p>
      <p id="d1e3159">Selected HOMs representing the major HOM types (and formation
pathways) were summed up and categorized into four groups, as shown in Table 2.
Each pathway might be influenced differently by boundary layer dynamics and
micrometeorological processes. In this study, OH-initiated HOMs were assumed
negligible due to the very low OH level in the nocturnal boundary layer.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p id="d1e3165">Compositions of selected HOMs and their main oxidants (Yan
et al., 2016).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Molecule compositions</oasis:entry>
         <oasis:entry colname="col3">Main oxidants</oasis:entry>
         <oasis:entry colname="col4">Main terminators</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">CHO<inline-formula><mml:math id="M189" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><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">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">14</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <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">10</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">14</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></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M192" 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></oasis:entry>
         <oasis:entry colname="col4">Self-termination or <inline-formula><mml:math id="M193" 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></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CHON<inline-formula><mml:math id="M194" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><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">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>, <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">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">11</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M197" 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="M198" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4">NO or self-termination–<inline-formula><mml:math id="M199" 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></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CHO<inline-formula><mml:math id="M200" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><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">19</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">28</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="M202" 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">14</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M203" 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></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M204" 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></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">CHON<inline-formula><mml:math id="M205" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><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">20</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">32</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">12</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M207" 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">13</mml:mn></mml:msub><mml:mi mathvariant="normal">N</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M208" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M209" 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></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d1e3550">All the HOM groups in Fig. 5a show stable patterns, and good agreement is
observed between the ground and tower measurements in the first half of the
night. Variations were observed when air mass change occurred at around
01:00, as indicated by the drop of <inline-formula><mml:math id="M210" 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> concentration and horizontal
wind shift (not shown here). A rapid decrease was found in CS, which
represents the rate of condensation of low-volatility vapors onto the existing
aerosol particles (Dada et al.,
2017), implying that the aerosol population also changed. However, the HOM
groups were still well correlated with each other, suggesting well-mixed
conditions in the non-inversion night.</p>
      <p id="d1e3565">Figure 5b shows the time series of the trace gases, MT, and HOM groups of
both ground and tower measurements during an inversion night case
(8–9 September, from 21:00 to 03:00). <italic>Ri</italic> was generally higher
during this night, and increased from <inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">0.03</mml:mn></mml:mrow></mml:math></inline-formula> (indicating a weakly stable
condition; Mammarella et al., 2007), at around midnight, to a maximum of
<inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1.13</mml:mn></mml:mrow></mml:math></inline-formula> (indicating a very stable condition) for the rest of the night.
Roughly, <italic>Ri</italic> values in excess of unity indicate that stably
stratified conditions appreciably diminish the inverse turbulent Prandtl
number (<italic>Pr</italic>) and the efficiency of turbulence to mix heat when
compared to momentum (Katul et al., 2014). The parameters measured at tower
level were not significantly affected by strong <italic>Ri</italic> fluctuations
throughout the night; in contrast, significant variations were observed at
ground level.</p>
      <?pagebreak page17443?><p id="d1e3601"><?xmltex \hack{\newpage}?>The ground <inline-formula><mml:math id="M213" 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> concentration experienced a rapid decrease at
midnight. In about an hour (from 23:30 to 00:30), ground <inline-formula><mml:math id="M214" 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>
concentration dropped by more than half (from 20 to 9 ppbv), and
<inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration increased as well (from 404 to 423 ppbv). Conversely, the MT concentration at ground level almost doubled (from 0.49
to 0.80 ppbv) during the same period. Theoretically, the enhancement of HOM
precursor VOC and the decrease in oxidant would compensate for each other if the
sink remained the same, and the ground HOM concentrations should also remain
constant. However, all the HOM groups showed a significant decrease after
midnight, despite the CS (generally the main sink for HOM in the atmosphere)
staying practically constant. In particular, the concentration of the
CHO<inline-formula><mml:math id="M216" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula> group dropped <inline-formula><mml:math id="M217" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">80</mml:mn></mml:mrow></mml:math></inline-formula> %, from <inline-formula><mml:math id="M218" display="inline"><mml:mrow><mml:mn mathvariant="normal">8.6</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M219" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.7</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M220" 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>, and the concentration of the
CHO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula> group decreased from <inline-formula><mml:math id="M222" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> to <inline-formula><mml:math id="M223" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">0.1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">6</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M224" 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>. The concentrations of the CHON<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">monomer</mml:mi></mml:msub></mml:math></inline-formula>
and CHON<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula> groups also experienced large declines (<inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">34</mml:mn></mml:mrow></mml:math></inline-formula> % and <inline-formula><mml:math id="M228" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> %, respectively) in the latter half of the
night. At 03:00, the CHON<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">dimer</mml:mi></mml:msub></mml:math></inline-formula> concentration was already below
the detection limit (<inline-formula><mml:math id="M230" display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">4</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> cm<inline-formula><mml:math id="M231" 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>). Therefore, the much lower
ground HOM concentrations might not be totally explained by the change of HOM
production but rather due to some other processes such as additional losses.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p id="d1e3832">Schematic figure showing how vertical mixing, vertical advection,
and horizontal advection influence ground-level <inline-formula><mml:math id="M232" 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> concentrations
differently on non-inversion nights and inversion nights at the SMEAR II
station.</p></caption>
            <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f06.png"/>

          </fig>

      <p id="d1e3852">A previous study by Alekseychik
et al. (2013) at the SMEAR II station showed that nocturnal decoupled air layers
were frequently (with a fraction of 18.6 % based on a long-term dataset)
observed under high-<italic>Ri</italic> conditions in the boreal forest. The decoupled layer
could strongly influence the ground <inline-formula><mml:math id="M233" 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>, MT, and <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations (Rannik
et al., 2009, 2012; Alekseychik et al., 2013; Chen et al., 2018) and could
also explain the occurrence of the strong temperature inversion during the
inversion nights. To explore the possible mechanism resulting in
significantly different <inline-formula><mml:math id="M235" 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>, MT, and HOM concentrations below the canopy,
the mean continuity equation for high-Reynolds-number flows within the
canopy is formulated as (e.g., Katul et al., 2006)

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M236" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>C</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>U</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>C</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>+</mml:mo><mml:mover accent="true"><mml:mi>W</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mi>C</mml:mi><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mi>S</mml:mi><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>c</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∂</mml:mo><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>c</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:mrow><mml:mrow><mml:mo>∂</mml:mo><mml:mi>x</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              where <inline-formula><mml:math id="M237" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> is time, <inline-formula><mml:math id="M238" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M239" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> are the longitudinal and vertical directions,
respectively, <inline-formula><mml:math id="M240" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> is the scalar concentration, <inline-formula><mml:math id="M241" display="inline"><mml:mi>U</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M242" display="inline"><mml:mi>W</mml:mi></mml:math></inline-formula> are the
longitudinal and vertical velocity components, <inline-formula><mml:math id="M243" display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>w</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>c</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> and
<inline-formula><mml:math id="M244" display="inline"><mml:mover accent="true"><mml:mrow><mml:msup><mml:mi>u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:msup><mml:mi>c</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow><mml:mo mathvariant="normal">‾</mml:mo></mml:mover></mml:math></inline-formula> are the turbulent scalar fluxes in the vertical and
horizontal, respectively, <inline-formula><mml:math id="M245" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> represents the net sources or sinks
(physical, chemical, and biological) of <inline-formula><mml:math id="M246" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula>, and the overline represents time
averaging over turbulent scales. The six terms in this equation represent the
following (left to right): local rate of change (<inline-formula><mml:math id="M247" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), horizontal
advection by the mean velocity (<inline-formula><mml:math id="M248" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), vertical advection by the mean
velocity (<inline-formula><mml:math id="M249" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), net sources or sinks (<inline-formula><mml:math id="M250" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), net vertical
transport by the vertical turbulent flux gradient (<inline-formula><mml:math id="M251" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), and net
horizontal transport by the horizontal turbulent flux gradient (<inline-formula><mml:math id="M252" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>).
Generally, <inline-formula><mml:math id="M253" display="inline"><mml:mrow><mml:mfenced close="|" open="|"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:mrow></mml:mfenced><mml:mo>≪</mml:mo><mml:mfenced open="|" close="|"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:mfenced></mml:mrow></mml:math></inline-formula> and is hereafter
ignored in the discussion.</p>
      <?pagebreak page17445?><p id="d1e4258">During the non-inversion night, the ground <inline-formula><mml:math id="M254" 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> could be replenished by vertical turbulent transport (<inline-formula><mml:math id="M255" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), mean vertical advection
from the upper boundary layer (<inline-formula><mml:math id="M256" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>), or horizontal advection below the
canopy (<inline-formula><mml:math id="M257" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) (as shown in Fig. 6). However, for highly stratified
flows, <inline-formula><mml:math id="M258" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> becomes small, as the efficiency of turbulence to transport
<inline-formula><mml:math id="M259" 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> to layers near the ground becomes weak (Katul et
al., 2014). Vertical and horizontal advection were also small within such a
stable layer, and the reduced mean velocity would result in smaller
contributions from <inline-formula><mml:math id="M260" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M261" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Note that these advective terms tend
to be opposite in sign by the virtue of the mean fluid continuity equation
(Katul et al., 2006). Instead, the sink of <inline-formula><mml:math id="M262" 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="M263" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) was stronger because of the increasing loss due to a higher
surface area-to-volume density (<inline-formula><mml:math id="M264" display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>/</mml:mo><mml:mi>V</mml:mi></mml:mrow></mml:math></inline-formula>) in this shallow decoupled layer. Under
this circumstance, the ground <inline-formula><mml:math id="M265" 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> concentration dramatically decreased
when the air layer was forming and eventually reached a much lower
concentration. The decoupled layer also affected MT and <inline-formula><mml:math id="M266" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> below the
canopy in the inversion night but resulted in concentration increases as
opposed to <inline-formula><mml:math id="M267" 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>. The weakened vertical turbulence (<inline-formula><mml:math id="M268" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) tended to
retain the emissions from ground and understory vegetation within the layer,
though <inline-formula><mml:math id="M269" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> also increased. In general, the increased <inline-formula><mml:math id="M270" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (primary
source from the ground) and MT (primary source from the canopy) at ground
level are good indicators for the extent of the mixing in the shallow
decoupled layer. At the same time, the strong decrease in <inline-formula><mml:math id="M271" 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 how
the sinks in this layer are no longer balanced by a large flux of <inline-formula><mml:math id="M272" 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>
from upper layers. However, the stabilization of ground-level <inline-formula><mml:math id="M273" 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>
concentrations at nonzero values after the initial fast decrease suggests
that a small amount of inflow, either via <inline-formula><mml:math id="M274" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> or <inline-formula><mml:math id="M275" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, is still
taking place.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p id="d1e4510">Mass defect (MD) plots of the selected <bold>(a)</bold> non-inversion
night case (11 September) and <bold>(b)</bold> inversion night case
(8 September). Color code indicates the ratios between tower and ground HOM
concentrations. The grey shaded area denotes the dimer range
(<inline-formula><mml:math id="M276" display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 450–600 Th).</p></caption>
            <?xmltex \igopts{width=327.206693pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f07.pdf"/>

          </fig>

      <p id="d1e4537">Therefore, the differences between the ground and tower measurements were
due to the joint effects of (i) decoupling between the stably stratified
near-ground layer and the canopy top and the consequent formation of a
shallow layer, (ii) weakening of advective and turbulent flux transport
terms thereby inhibiting mass exchange between the ground decoupled layer
and the remaining nocturnal boundary layer, and (iii) an increased surface area-to-volume ratio within the decoupled layer thereby enhancing <inline-formula><mml:math id="M277" display="inline"><mml:mrow><mml:msub><mml:mi>N</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p id="d1e4553">Hourly changes of
the ratios between estimated tower and ground HOM concentrations from 12:00
on 11 September to 11:00 on 12 September (non-inversion night). Markers are
sized by ground HOM concentrations and colored by the <inline-formula><mml:math id="M278" 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> difference
between the tower and ground <inline-formula><mml:math id="M279" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:msub><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">tower</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mo>-</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:msub><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">ground</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Hourly ambient temperatures at ground (Tg)
and tower (Tt) levels and RH at ground (RHg) and tower (RHt) levels are shown
in each subplot.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f08.pdf"/>

          </fig>

      <p id="d1e4605">Examination of the selected HOMs was useful and efficient to assess
the changes in HOMs; however, such an analysis might only indicate the major
formation pathways. Hence, it was also worthwhile to have a holistic view of
the entire mass spectra and all the detected HOMs. The mass defect (MD) plot
(Fig. 7) separates all identified compounds according to their exact masses
on the <inline-formula><mml:math id="M280" display="inline"><mml:mi>x</mml:mi></mml:math></inline-formula> axis and the deviation from the integer mass on the <inline-formula><mml:math id="M281" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis. Each
circle represents a compound, with the areas scaled by concentrations and
colored by the ratios between tower and ground concentrations. Figure 7a and
b are MD plots showing the mean spectra of the selected non-inversion night
(11 September) and inversion night (8 September), respectively. Without the
formation of a decoupled layer, nearly the same concentration distributions
of HOMs were observed. In contrast, during the inversion night (8 September,
Fig. 7b), large differences could be found between the two measurement
heights. Moreover, a significant fraction of the ground HOMs disappeared on
the inversion night, and the concentrations of the remaining HOMs were also
lower, confirming the aforementioned results obtained with the selected HOM
groups.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p id="d1e4624">Hourly changes of the ratios between estimated tower and ground HOM
concentrations from 12:00 on 8 September to 11:00 on 9 September (inversion
night). Markers are sized by ground HOM concentrations and colored by the O3
difference between tower and ground <inline-formula><mml:math id="M282" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:msub><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">tower</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mo>-</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mrow><mml:msub><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="normal">ground</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Hourly ambient temperatures at ground (Tg)
and tower (Tt) levels and RH at ground (RHg) and tower (RHt) levels are
shown in each subplot.</p></caption>
            <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/18/17437/2018/acp-18-17437-2018-f09.pdf"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Study limitations</title>
      <p id="d1e4672">Several limitations still exist in this study. From the measurement side, one
major concern was the comparability between our two CI-APi-TOF mass
spectrometers. In the worst case, our conclusion might be biased if
instrument responses changed due to some parameter that correlated with the
observed inversions. The main parameters in this case would be ambient
temperature and RH. As both instruments were located in
temperature-controlled containers and the sample flow was mixed 1 : 2 with
dry sheath air in the CI-APi-TOF drift tube, neither of these were expected
to yield such large changes. However, for confirmation, we compared the
detailed spectral evolution during days and nights of the study. Figure 8
shows an example of hourly changes of the ratios between tower and ground
HOMs, over a 24 h period without nighttime temperature inversion
(11 September). During this period, ambient temperatures changed from
19.1 <inline-formula><mml:math id="M283" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (12:00) to 8.8 <inline-formula><mml:math id="M284" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C (07:00) at ground level, and from
17.9 to 8.1 <inline-formula><mml:math id="M285" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C at tower level. Ambient RHs also increased from
72 % to 96 % at ground level, and from 74 % to 98 % at tower
level. While some scatter is visible in the 200–300 Th range during some
parts of the night, good agreement was observed between the<?pagebreak page17446?> two instruments
throughout the night, despite large variability in temperatures and RHs.</p>
      <p id="d1e4702">In contrast, during a 24h period with nighttime temperature inversion
(8 September, shown in Fig. 9), the ratios agreed well only during daytime
(from 12:00 to 17:00, and 09:00 to 11:00 on the next day). Between these two
periods, temperature and RH were most of the time in the same range as on
11 September  (when no strong deviations were observed), but now the HOM
behavior changed dramatically between the two heights. The ratios increased
from <inline-formula><mml:math id="M286" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> (during daytime) up to <inline-formula><mml:math id="M287" display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> at 07:00
for some of the measured molecules.</p>
      <p id="d1e4725">Figures 8 and 9 clearly imply that the large differences between ground and
tower HOM concentrations were driven by temperature inversions and consequent
changes in the composition of the air in the two detached layers. Large
changes in HOMs were observed only when the ground temperature was lower than
the tower temperature and when the ozone concentration at ground level was
several parts per billion lower than at the tower (shown as a color scale in
Figs. 8 and 9). Absolute temperatures or RHs at the two heights were not able
to explain the changes. As a concrete example, good agreement was observed at
07:00 on 12 September, while ambient temperatures were low (ground and tower
temperatures were 9.3 and 8.6 <inline-formula><mml:math id="M288" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, respectively) and RHs were high
(ground and tower RHs were 92 % and 96 %, respectively), but large
deviations were found at 20:00, 8 September, when higher temperatures (ground
and tower temperatures were 10.2 and 12.1 <inline-formula><mml:math id="M289" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>C, respectively) and
lower RHs (ground and tower RHs were 88 % and 76 %, respectively)
were observed. In other words, neither low temperatures nor high RHs caused
large changes to our instruments. Instead,<?pagebreak page17447?> the large discrepancies between
the two CI-APi-TOFs were only observed when other key parameters (like ozone)
were found to deviate considerably between the two heights.</p>
      <p id="d1e4746">From the micrometeorology side, the contribution from the potential
micrometeorological processes in the layer between 1.5 and 4.2 m (between
the sampling heights of the ground HOMs and other parameters) could not be
estimated with the current experiment design (i.e., only two measurement
heights). Similarly, the influence from horizontal advection could not be
entirely ruled out as a reason for the reduced ground-level HOM
concentrations (and other significantly changed species) because of the
possible horizontal inhomogeneity of HOM precursors and oxidants below the
canopy. However, our conclusion was confirmed by the incompatibility between
the increasing ground-level MT and <inline-formula><mml:math id="M290" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations and the advection
hypothesis (i.e., all species would show similar tendencies if advection
played a major role), indicating the influence of horizontal and vertical
advection is probably minor when compared to the increasing sink. However,
conclusive evidence is still needed, which highlights the need for joint
vertical–planar HOM studies, measuring both vertical and horizontal
distribution of HOM concentrations.</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusion</title>
      <p id="d1e4767">Highly oxygenated molecules (HOMs) were measured above the canopy and at
ground level (below the canopy) in a boreal forest environment during the
IBAIRN campaign that took place in September 2016. Boundary layer dynamics
and micrometeorology were found to be important factors that influence the
abundance of and trends in HOMs at ground level, by perturbing both their
sources and sinks. In the well-mixed boundary layer (e.g., during daytime or
nights without strong inversion), HOM concentrations and other measured
species were overall similar between the ground and tower measurements. In
contrast, much lower ground-level HOM concentrations were observed when
nighttime temperature inversion and formation of a decoupled layer occurred
below the canopy. On the one hand, the production of the ground-level HOMs could
be affected by the decreasing <inline-formula><mml:math id="M291" 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> concentrations and the increasing MT
concentration in the shallow layer. On the other hand, the surface area-to-volume ratio dramatically increased in the shallow layer compared to the
nocturnal boundary layer. The possibility of losses on surfaces for
ground-level HOMs became much larger than usual during inversion nights. The
enhanced interaction of air in the decoupled layer with the forest floor was
supported by increased concentrations of <inline-formula><mml:math id="M292" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, emitted mainly from the
ground, in this layer.</p>
      <p id="d1e4792">We have presented the first detailed measurements of HOMs below and above
the canopy across a wide range of atmospheric stability conditions. The
results highlight the significance of near-ground boundary layer dynamics
and micrometeorological processes on the ambient HOMs, showing that
ground-based HOM measurement at this site might not be representative for
the entire nocturnal boundary layer. Conventionally, field measurements of
HOMs and other parameters are mostly performed close to the ground, and the
possible effect of boundary layer dynamics and micrometeorological processes
to the HOM concentrations has rarely been considered. Aerosol particle
growth and SOA formation rates at ground level are likely to be influenced
by the reduced HOM concentrations on the inversion nights. However, there
are still limitations due to current experiment design, such as horizontal
separation in instrument setup, or the uncertainties from using point
measurements at two heights to infer larger-scale exchange. Clearly, more
vertical and planar measurements of HOMs are needed to confirm the<?pagebreak page17448?> emerging
picture presented here. Influence of boundary layer dynamics should be
better characterized and evaluated in future field campaigns.</p>
</sec>

      
      </body>
    <back><notes notes-type="dataavailability">

      <p id="d1e4800">The time series of the measured trace gases, meteorological
parameters, and estimated total HOM concentrations at the ground and tower
levels will be available at the end of December 2018
(<ext-link xlink:href="https://doi.org/10.5281/zenodo.1489079" ext-link-type="DOI">10.5281/zenodo.1489079</ext-link>, Zha, 2018). For other data please contact the
first author via email (qiaozhi.zha@helsinki.fi).</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e4806">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-18-17437-2018-supplement" xlink:title="pdf">https://doi.org/10.5194/acp-18-17437-2018-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution">

      <p id="d1e4815">QZ, MR, and ME designed the study. QZ, CY, HJ, MR, NS, JA, and SS
collected the data. QZ and CY analyzed the data. QZ wrote the paper. All
coauthors contributed to data interpretation and commented on the paper.</p>
  </notes><notes notes-type="competinginterests">

      <p id="d1e4821">The authors declare that they have no conflict of
interest. Douglas R. Worsnop is affiliated with Aerodyne Research, who
produce the CI-APi-TOF instruments used in this study.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e4827">This work was supported by the IBAIRN project, the Academy of Finland Center
of Excellence in Atmospheric Science, European commission Actris2 and Actris
PPP, the European Research Council (grant 638703-COALA), transnational access
from ENVRI plus, and the SMEAR II technical team. Qiaozhi Zha thanks ATM-DP
(Doctoral Program in Atmospheric Sciences) graduate programs, John Crowley
and the Max Plank Institute in association with the IBAIRN proposal, and the
tofTools team for providing tools for mass spectrometry analysis.
Gabriel Katul acknowledges the support from the US National Science
Foundation (NSF-EAR-1344703, NSF-AGS-1644382), the U.S. Department of Energy
(DE-SC0011461), and the University of Helsinki for supporting a 3-month
sabbatical leave at the Division of Atmospheric Sciences.
Otso Peräkylä thanks the Vilho,  Yrjö and
Kalle Väisälä Foundation.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Kyung-Eun
Min<?xmltex \hack{\newline}?> Reviewed by: two anonymous referees</p></ack><ref-list>
    <title>References</title>

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<abstract-html><p>While the role of highly oxygenated molecules (HOMs) in new particle
formation (NPF) and secondary organic aerosol (SOA) formation is not in
dispute, the interplay between HOM chemistry and atmospheric conditions
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Biosphere-Atmosphere Interactions on the Reactive Nitrogen budget (IBAIRN)
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above the forest canopy were performed for the first time at the boreal
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below and above the canopy were similar during daytime, supporting a
well-mixed boundary layer approximation. However, much lower nighttime HOM
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ground HOMs were influenced by the changes in the precursors and oxidants and
enhancement of the loss on surfaces in this layer, while the HOMs above the
canopy top were not significantly affected. Our findings clearly illustrate
that near-ground HOM measurements conducted under stably stratified
conditions at this site might only be representative of a small fraction of
the entire nocturnal boundary layer. This could, in turn, influence the
growth of newly formed particles and SOA formation below the canopy where the
large majority of measurements are typically conducted.</p></abstract-html>
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