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<article xmlns:xlink="http://www.w3.org/1999/xlink" xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:oasis="http://docs.oasis-open.org/ns/oasis-exchange/table" dtd-version="3.0"><?xmltex \makeatother\@nolinetrue\makeatletter?>
  <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 GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-15-11291-2015</article-id><title-group><article-title>Advanced source apportionment of size-resolved trace elements at multiple sites in London during winter</article-title>
      </title-group><?xmltex \runningtitle{Advanced source apportionment of trace elements in London}?><?xmltex \runningauthor{S.~Visser et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Visser</surname><given-names>S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Slowik</surname><given-names>J. G.</given-names></name>
          <email>jay.slowik@psi.ch</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Furger</surname><given-names>M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-2401-6448</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff14">
          <name><surname>Zotter</surname><given-names>P.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bukowiecki</surname><given-names>N.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2925-8553</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Canonaco</surname><given-names>F.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Flechsig</surname><given-names>U.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff15">
          <name><surname>Appel</surname><given-names>K.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2902-2102</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Green</surname><given-names>D. C.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Tremper</surname><given-names>A. H.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff16">
          <name><surname>Young</surname><given-names>D. E.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9177-6485</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Williams</surname><given-names>P. I.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5 aff6">
          <name><surname>Allan</surname><given-names>J. D.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6492-4876</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Coe</surname><given-names>H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3264-1713</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff7">
          <name><surname>Williams</surname><given-names>L. R.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff8 aff17">
          <name><surname>Mohr</surname><given-names>C.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-3291-9295</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9">
          <name><surname>Xu</surname><given-names>L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0021-9876</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff9 aff10">
          <name><surname>Ng</surname><given-names>N. L.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8460-4765</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff11">
          <name><surname>Nemitz</surname><given-names>E.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1765-6298</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff12">
          <name><surname>Barlow</surname><given-names>J. F.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff12">
          <name><surname>Halios</surname><given-names>C. H.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8301-8449</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff13">
          <name><surname>Fleming</surname><given-names>Z. L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Baltensperger</surname><given-names>U.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0079-8713</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Prévôt</surname><given-names>A. S. H.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Laboratory of Atmospheric Chemistry, Paul Scherrer Institute,
Villigen, Switzerland</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Swiss Light Source, Paul Scherrer Institute, Villigen,
Switzerland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>HASYLAB, DESY Photon Science, Hamburg, Germany</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Analytical and Environmental Sciences, King's College London,
London, UK</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>School of Earth, Atmospheric and Environmental Sciences, University
of Manchester, Manchester, UK</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>National Centre for Atmospheric Science, University of Manchester, Manchester, UK</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>Aerodyne Research, Inc., Billerica, MA, USA</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>Department of Atmospheric Sciences, University of Washington,
Seattle, WA, USA</institution>
        </aff>
        <aff id="aff9"><label>9</label><institution>School of Chemical and Biomolecular Engineering, Georgia Institute
of Technology, Atlanta, GA, USA</institution>
        </aff>
        <aff id="aff10"><label>10</label><institution>School of Earth and Atmospheric Sciences, Georgia Institute of
Technology, Atlanta, GA, USA</institution>
        </aff>
        <aff id="aff11"><label>11</label><institution>Centre for Ecology and Hydrology, Penicuik, Midlothian,
Scotland</institution>
        </aff>
        <aff id="aff12"><label>12</label><institution>Department of Meteorology, University of Reading, Reading, UK</institution>
        </aff>
        <aff id="aff13"><label>13</label><institution>National Centre for Atmospheric Science, Department of Chemistry, University of Leicester, Leicester, UK</institution>
        </aff>
        <aff id="aff14"><label>a</label><institution>now at: Lucerne School of Engineering and Architecture, Bioenergy Research, Lucerne University of Applied Sciences and Arts, Horw, Switzerland</institution>
        </aff>
        <aff id="aff15"><label>b</label><institution>now at: European XFEL, Hamburg, Germany</institution>
        </aff>
        <aff id="aff16"><label>c</label><institution>now at: Department of Environmental Toxicology, University of California, Davis, CA, USA</institution>
        </aff>
        <aff id="aff17"><label>d</label><institution>now at: Institute of Meteorology and Climate Research, Karlsruhe Institute of Technology, Karlsruhe, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">J. G. Slowik (jay.slowik@psi.ch)</corresp></author-notes><pub-date><day>12</day><month>October</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>19</issue>
      <fpage>11291</fpage><lpage>11309</lpage>
      <history>
        <date date-type="received"><day>2</day><month>March</month><year>2015</year></date>
           <date date-type="rev-request"><day>26</day><month>May</month><year>2015</year></date>
           <date date-type="rev-recd"><day>30</day><month>August</month><year>2015</year></date>
           <date date-type="accepted"><day>21</day><month>September</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>


      <abstract>
    <p>Trace element measurements in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>
and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> aerosol were performed with 2 h time resolution
at kerbside, urban background and rural sites during the ClearfLo winter 2012
campaign in London. The environment-dependent variability of emissions was
characterized using the Multilinear Engine implementation of the positive
matrix factorization model, conducted on data sets comprising all three sites
but segregated by size. Combining the sites enabled separation of sources
with high temporal covariance but significant spatial variability. Separation
of sizes improved source resolution by preventing sources occurring in only a
single size fraction from having too small a contribution for the model to
resolve. Anchor profiles were retrieved internally by analysing data subsets,
and these profiles were used in the analyses of the complete data sets of all
sites for enhanced source apportionment.</p>
    <p>A total of nine different factors were resolved (notable elements in
brackets): in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, brake wear (Cu, Zr, Sb, Ba), other
traffic-related (Fe), resuspended dust (Si, Ca), sea/road salt (Cl), aged sea
salt (Na, Mg) and industrial (Cr, Ni); in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, brake wear,
other traffic-related, resuspended dust, sea/road salt, aged sea salt and
S-rich (S); and in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, traffic-related (Fe, Cu, Zr, Sb,
Ba), resuspended dust, sea/road salt, aged sea salt, reacted Cl (Cl), S-rich
and solid fuel (K, Pb). Human activities enhance the kerb-to-rural
concentration gradients of coarse aged sea salt, <?xmltex \hack{\mbox\bgroup}?>typically considered<?xmltex \hack{\egroup}?> to have
a natural source, by 1.7–2.2. These site-dependent concentration differences
reflect the effect of local resuspension processes in London. The
anthropogenically influenced factors traffic (brake wear and other
traffic-related processes), dust and sea/road salt provide further
kerb-to-rural concentration enhancements by direct source emissions by a
factor of 3.5–12.7. The traffic and dust factors are mainly emitted in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and show strong diurnal variations with concentrations
up to 4 times higher during rush hour than during night-time.
Regionally influenced S-rich and solid fuel factors, occurring primarily in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, have negligible resuspension influences, and
concentrations are similar throughout the day and across the regions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Acute and chronic exposure to trace elements in ambient aerosols induces
adverse respiratory and cardiovascular health effects <xref ref-type="bibr" rid="bib1.bibx60" id="paren.1"/>.
<xref ref-type="bibr" rid="bib1.bibx6" id="text.2"/> and <xref ref-type="bibr" rid="bib1.bibx38" id="text.3"/> reveal different mortality
and morbidity effects for exposure to individual particle size fractions such
as PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>1.0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>
(particulate matter with an aerodynamic diameter, <inline-formula><mml:math display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula>, of 10 to 2.5, 2.5 to 1.0
and smaller than 1.0 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>, respectively). These particles are
emitted into the atmosphere by different sources.</p>
      <p>The major source of PM in most urban areas is road traffic, comprising
exhaust and non-exhaust (abrasion and resuspension) contributions
<xref ref-type="bibr" rid="bib1.bibx16 bib1.bibx44" id="paren.4"/>. Other sources include industrial
activities, fossil fuel use and biomass burning for heating and energy
production, crustal material, sea salt, and cooking, as well as contributions
of secondary inorganic and organic aerosols
<xref ref-type="bibr" rid="bib1.bibx20 bib1.bibx55 bib1.bibx68" id="paren.5"/>. Source apportionment by positive matrix
factorization (PMF; <xref ref-type="bibr" rid="bib1.bibx42" id="altparen.6"/>) is a powerful tool to quantify
sources based on trace element measurements. Many studies have applied PMF on
either elements alone or in combination with other species, such as carbon
species and inorganic ions
<xref ref-type="bibr" rid="bib1.bibx3 bib1.bibx22 bib1.bibx23 bib1.bibx53 bib1.bibx64 bib1.bibx69" id="paren.7"/>. However,
such measurements are typically performed only for a single size fraction and
with 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> time resolution, preventing the study of diurnal behaviours
of emission sources and short-term changes in air pollution exposure levels.
Anthropogenic sources such as traffic (Fe, Cu, Zn, Ba), resuspension (Al, Si,
Ca) and biomass burning for home heating (S, K) typically show distinct
diurnal variations, while regional and natural sources such as secondary
sulfate (S) and sea salt (Na, Mg, Cl) usually exhibit small diurnal
variability <xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx14 bib1.bibx56" id="paren.8"/>. Elements in
different size fractions typically serve as markers for different sources. S
from secondary sulfate for example is mainly found in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>1.0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>,
whereas PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> S can indicate sea salt and/or mineral sulfate
<xref ref-type="bibr" rid="bib1.bibx33" id="paren.9"/>. <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>1.0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> K mostly originates from wood burning,
but is attributed to dust in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx55" id="paren.10"/>. It is
vital to understand the extent to which emission sources affect air quality,
especially in urban areas, where the global population has increased from
34 % (in 1960) to 56 % (in 2014) and is expected to grow further
<xref ref-type="bibr" rid="bib1.bibx61" id="paren.11"/>.</p>
      <p>Only a limited number of studies have applied PMF to explore trace element
emission sources across multiple sites or size fractions, or with high time
resolution
<xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx11 bib1.bibx14 bib1.bibx34 bib1.bibx51" id="paren.12"/>.
<xref ref-type="bibr" rid="bib1.bibx32" id="text.13"/> showed a higher degree of source separation by
applying PMF on combined <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data than on
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> data alone, due to a lack of variability in the sum of
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations of certain key tracers. The
Multilinear Engine solver (ME-2; <xref ref-type="bibr" rid="bib1.bibx39" id="altparen.14"/>) improves on
conventional PMF analyses by allowing complete and efficient exploration of
the solution space, facilitating source separation. <xref ref-type="bibr" rid="bib1.bibx1" id="text.15"/> and
<xref ref-type="bibr" rid="bib1.bibx50" id="text.16"/> used ME-2 to achieve improved source separation by
requiring the solution to be consistent with local emission profiles and
providing environmentally reasonable element ratios within factor profiles.
Some caution is needed when combining sites in PMF, because one needs to assume
that the chemical profiles of the resolved sources do not vary significantly
between the sites. This prerequisite is usually valid if the sites are only
a few kilometres apart <xref ref-type="bibr" rid="bib1.bibx14" id="paren.17"/>.</p>
      <p><inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations in London frequently exceed the legal daily
limit of 50 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (permitted exceedances per year of 35).
These exceedances are caused by local and regional emission sources in
combination with meteorological factors
<xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx25 bib1.bibx26 bib1.bibx30" id="paren.18"/>. A better
understanding of the temporal behaviour of emission sources throughout the
city is needed. The objective of this study is to characterize the
environment-dependent variability of emissions by source apportionment of
size-resolved trace elements measured simultaneously at three sites. We apply
the ME-2 implementation of the PMF model to 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> element
concentrations measured at two urban sites in London (Marylebone Road and North
Kensington) and one rural site southeast of London (Detling), United Kingdom
(UK), during the ClearfLo (Clean Air for London) field campaign
<xref ref-type="bibr" rid="bib1.bibx5" id="paren.19"/>. PMF analysis is conducted on data sets comprising
all three sites but analysed separately for each size (PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>). We demonstrate that
rotational control of the solutions using anchor profiles in ME-2 is
essential for a successful source apportionment. This approach results in
enhanced source separation compared to using unconstrained PMF. We
investigate the size dependence of sources such as traffic, resuspended dust,
and sea salt and also identify sources unique to particular size fractions.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <title>Measurement sites and instrumentation</title>
      <p>Measurements were conducted as part of the ClearfLo project
(<uri>http://www.clearflo.ac.uk/</uri>), a multinational collaboration to
investigate the processes driving air quality in and around London
<xref ref-type="bibr" rid="bib1.bibx5" id="paren.20"/>. This study focuses on the winter intensive
observation period (IOP), which took place from 6 January to
11 February 2012. Trace element measurements were conducted at kerbside,
urban background and rural sites, at or near permanent air quality
measurement stations of the Automatic Urban and Rural Network (AURN) or Kent
and Medway Air Quality Monitoring Network (see Fig. <xref ref-type="fig" rid="Ch1.F1"/>). The
kerbside site was located at Marylebone Road (MR; lat
51<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>31<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>21<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N, long
0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>09<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>17<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> W) at the southern side of
a street canyon <xref ref-type="bibr" rid="bib1.bibx10" id="paren.21"/>. Measurements were performed at
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from a six-lane road with a traffic flow of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn>73</mml:mn></mml:mrow></mml:math></inline-formula> 000 vehicles per day (15 % heavy duty vehicles; traffic counts by
vehicle group from road sensors (number of vehicles per 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>)).
A signal-controlled junction at 200 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and a heavily used pedestrian
light-controlled crossing at 65 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> from the site resulted in frequent
braking and stationary vehicle queues in front of the site. The urban
background site, the main sampling site during ClearfLo, was located at the
grounds of the Sion Manning Secondary School in North Kensington (NK; lat
51<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>31<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>21<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N, long
0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>12<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>49<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> W). Although the site is in a suburban area about 4.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> west of MR that experiences heavy traffic, measurements took
place away from main roads, and this site is representative of the urban
background air quality in London <xref ref-type="bibr" rid="bib1.bibx4" id="paren.22"/>. The rural site was
situated at approximately 45 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> to the southeast of downtown London
at the Kent Showgrounds at Detling (DE; lat
51<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>18<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>07<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N, long
0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>22<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> E) on a plateau at
200 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> surrounded by fields and villages <xref ref-type="bibr" rid="bib1.bibx36" id="paren.23"/>.
A busy road with a traffic flow of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn>42</mml:mn></mml:mrow></mml:math></inline-formula> 000 vehicles per day
<xref ref-type="bibr" rid="bib1.bibx17" id="paren.24"/> is located approximately 150 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> south
of the site.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Map of southeastern UK. Indicated are the sampling sites MR
(kerbside site Marylebone Road), NK (urban background site North Kensington),
DE (rural site Detling), and the elevated BT Tower site for meteorological
measurements (adapted from Google Maps).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f01.pdf"/>

        </fig>

      <p>Aerosols were sampled by rotating drum impactors (RDIs) with 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> time
resolution and a flow rate of 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">h</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, and were segregated by
size into PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (coarse), PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>
(intermediate) and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (fine) fractions. Trace element
composition of the RDI samples was determined by synchrotron
radiation-induced X-ray fluorescence spectrometry (SR-XRF) at the X05DA
beamline <xref ref-type="bibr" rid="bib1.bibx21" id="paren.25"/> at the Swiss Light Source (SLS), Paul
Scherrer Institute (PSI), Villigen PSI, Switzerland, and at Beamline L at the
Hamburger Synchrotronstrahlungslabor (HASYLAB), Deutsches
Elektronen-Synchrotron (DESY), Hamburg, Germany (beamline dismantled
November 2012). In total 25 elements were quantified (Na, Mg, Al, Si, P, S,
Cl, K, Ca, Ti, V, Cr, Mn, Fe, Ni, Cu, Zn, Br, Sr, Zr, Mo, Sn, Sb, Ba, Pb).
Details of the RDI-SR-XRF analysis are described in <xref ref-type="bibr" rid="bib1.bibx57" id="text.26"/> and in
previous application examples in <xref ref-type="bibr" rid="bib1.bibx8" id="text.27"/> and
<xref ref-type="bibr" rid="bib1.bibx46" id="text.28"/>.</p>
      <p>Additional measurements discussed in this paper are briefly described here.
Aerosol mass spectrometers (Aerodyne Research, Inc., Billerica, MA, USA) were
deployed at MR (5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution), NK (5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> sampling
interval every 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>) and DE (2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution) to
characterize the non-refractory submicron aerosol components (organic matter,
sulfate, nitrate, ammonium, chloride; <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx29" id="altparen.29"/>);
a quadrupole AMS was deployed at MR; and a high-resolution time-of-flight AMS was deployed at NK and DE.
Particle light absorption was derived with seven-wavelength Aethalometers
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn>370</mml:mn></mml:mrow></mml:math></inline-formula>–950 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>, model AE 31, Magee Scientific;
5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution) at NK (3.5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> cyclone) and DE
(2.5 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> cyclone). The measured absorption was apportioned to
traffic and wood burning based on the absorption coefficients at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn>470</mml:mn></mml:mrow></mml:math></inline-formula> and 950 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>, assuming absorption exponents of 1 and 2 for traffic
and wood burning emissions, respectively
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx36 bib1.bibx48" id="paren.30"/>. At MR and NK, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
measurements were performed with NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> chemiluminescent analysers (API,
A Series, model M200A; 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution). At DE, NO (Thermo
Scientific 42i analyser) and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (Aerodyne CAPS-<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and
QCL-76-D) data were collected and summed to obtain total NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
concentrations (1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution). Wind direction and wind speed data
for the two city sites were taken from the nearby BT Tower, where sonic
anemometers (20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula>) were placed at the top of an open lattice
scaffolding tower of 18 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> height on top of the main structure
(190.8 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>; lat 51<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>31<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>17<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> N,
long 0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>08<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>′</mml:mo></mml:msup></mml:math></inline-formula>19<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>′</mml:mo><mml:mo>′</mml:mo></mml:mrow></mml:msup></mml:math></inline-formula> W; 30 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution;
<xref ref-type="bibr" rid="bib1.bibx63" id="altparen.31"/>), while local data were used at DE. Relative humidity (RH)
data at NK were derived with a Vaisala WXT sensor (5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> resolution).
Finally, the UK Met Office's Numerical Atmospheric Modelling Environment
(NAME) dispersion model <xref ref-type="bibr" rid="bib1.bibx31" id="paren.32"/> <?xmltex \hack{\mbox\bgroup}?>provided<?xmltex \hack{\egroup}?> back trajectory
simulations for analysis of air mass origins <xref ref-type="bibr" rid="bib1.bibx5" id="paren.33"/>.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Positive matrix factorization</title>
      <p>PMF is a powerful source apportionment method to describe measurements, using
the bilinear factor model <xref ref-type="bibr" rid="bib1.bibx42" id="paren.34"/>

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>p</mml:mi></mml:munderover><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>k</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>+</mml:mo><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the <inline-formula><mml:math display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>th species concentration measured in the <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th
sample, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the contribution of the <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>th source to the <inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>th
sample (factor time series) and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>k</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the concentration of the <inline-formula><mml:math display="inline"><mml:mi>j</mml:mi></mml:math></inline-formula>th
species in the <inline-formula><mml:math display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>th source (factor profiles). The part of the data
remaining unexplained by the model is represented by the residual matrix
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. The entries of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>g</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>k</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>k</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (required to be non-negative)
are fit using a least-squares algorithm that iteratively minimizes the
objective function <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula>:

                <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>i</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>n</mml:mi></mml:munderover><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>j</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>m</mml:mi></mml:munderover><mml:msup><mml:mfenced close=")" open="("><mml:mfrac><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mfrac></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are the measurement uncertainties.</p>
      <p>The PMF model solution is subject to rotational ambiguity; that is, different
solutions may be found having similar values of <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx43" id="paren.35"/>. This
ambiguity can be reduced within the ME-2 algorithm by adding a priori
information into the PMF model (e.g. source profiles) to reduce the available
rotational space and direct the solution towards a unique, optimized and
environmentally meaningful solution.</p>
      <p>In this study, trace element source apportionment is performed using the ME-2
implementation of PMF <xref ref-type="bibr" rid="bib1.bibx39" id="paren.36"/>, with configuration and analysis in
the SoFi (Source Finder) toolkit <xref ref-type="bibr" rid="bib1.bibx9" id="paren.37"/> for the IGOR Pro
software environment (WaveMetrics, Inc., Portland, OR, USA). The ME-2 solver
executes the PMF algorithm in a similar way to the PMF solver <xref ref-type="bibr" rid="bib1.bibx42" id="paren.38"/> but
has the advantage that the full rotational space is accessible. One way to
efficiently explore this space is with the <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>-value approach. Here one or
more factor profiles are constrained by the scalar <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>, which defines how
much the resolved factors are allowed to deviate from the input “anchor”
profiles, according to

                <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>j</mml:mi><mml:mo>,</mml:mo><mml:mtext>solution</mml:mtext></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>±</mml:mo><mml:mi>a</mml:mi><mml:mo>×</mml:mo><mml:msub><mml:mi>f</mml:mi><mml:mi>j</mml:mi></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> can be set between 0 and 1. If, for example, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn>0.1</mml:mn></mml:mrow></mml:math></inline-formula>, all elements
in the profile are allowed to vary within <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>10 % of the input factor
profile. For clarity, we here use the term “ME-2” to refer to solving the
PMF model with the ME-2 solver using the <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>-value approach, whereas the term
“unconstrained ME-2” refers to solving the PMF model using the ME-2 solver
but without a priori constraints on the solution.</p>
      <p>These algorithms require both a data matrix (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, 25 elements measured
with 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> time resolution) and a corresponding uncertainty matrix
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>). Uncertainties that uniformly affect an entire row or column
of the data matrix (e.g. RDI flow rate, absolute or relative calibration) do
not alter the PMF solution and are thus not considered in constructing the
uncertainty matrix. Uncertainties are calculated according to
Eq. (<xref ref-type="disp-formula" rid="Ch1.E4"/>) and account for the detector counting efficiency
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>Det</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) and the energy calibration of an X-ray line as
function of detector channel (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>EC</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>):

                <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:msup><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>Det</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>+</mml:mo><mml:msup><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>EC</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:msqrt><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          The <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>Det</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> depend on the efficiency with which one
photon is counted by the detector and is defined as the square root of the
signal. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>EC</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> were estimated at 0.01 keV for SLS
spectra (representing <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> channels) and 0.02 keV for HASYLAB spectra
(representing <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> channel). Gaussian probability distributions
representing energy calibration biases (i.e. keV or energy offsets) are
constructed using the above values as the standard deviation (SD). From these
distributions, several offsets are selected, such that the perturbations are
uniformly sampled according to probability, and the XRF spectra are refitted
(here 20 offsets). The <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mtext>EC</mml:mtext><mml:mo>,</mml:mo><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> are defined as the SD of
the refitted spectra across these 20 iterations. Entries in <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with
a signal-to-noise ratio (SNR) below 2 are downweighted by replacing the
corresponding <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>/</mml:mo><mml:msub><mml:mtext>SNR</mml:mtext><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. This approach, as
opposed to downweighting an entire variable (i.e. increasing the uncertainty
associated with an entire column rather than a single point;
<xref ref-type="bibr" rid="bib1.bibx40" id="altparen.39"/>), allows variables with low average SNR but high SNR
periods to remain in the data matrix, as these peaks might contain valuable
information regarding sources (e.g. sources systematically sampled from
particular wind vectors).</p>
      <p>Missing values in one or several entries in <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>x</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (e.g. a line fit failure
of one or more elements) are set to zero and the corresponding error is set
to <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>10</mml:mn><mml:mn mathvariant="normal">9</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>. Missing data points in time (e.g. a power failure during sampling)
are removed from the data and error matrices.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Selection of ME-2 solutions</title>
      <p>The multi-size, multi-site nature of this data set allowed for several methods
of constructing the input data set for ME-2 (i.e. single
size <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> single site; single size <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> multiple sites; multiple
sizes <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> single site; multiple sizes <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> multiple sites).
Although all combinations were investigated, the analysis herein focuses
primarily on the single size <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> multiple sites option. That is, we
investigated three data sets, with each containing a single size
(PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> or PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>
fraction) and data from all three measurement sites (MR, NK and DE).
Combining the sites enabled separation of sources with high temporal
covariance but significant spatial variability. Separation of sizes improved
source resolution by preventing sources occurring in only a single size
fraction from having too small a contribution to <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> for the model to
resolve. Sources occurring only at one site were resolved, as discussed
below.</p>
      <p>ME-2 solutions were evaluated using a number of mathematical and physical
criteria. The two major aspects of the analysis are (1) selection of the
optimum number of factors and (2) evaluation of whether this solution is
acceptable as a final solution or requires additional/modified rotational
control. The primary criteria used for this evaluation are as follows:<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?><?xmltex \hack{\noindent}?>Mathematical
<list list-type="bullet"><list-item><p>Investigation of the decrease in <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mtext>expected</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula>
or the number of remaining degrees of freedom of the system) with increasing
<inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> (number of factors) due to the increased degrees of freedom in the model
<xref ref-type="bibr" rid="bib1.bibx41" id="paren.40"/>. A large decrease indicates significantly increased
explanation of the data, while a small decrease suggests that additional
factors are not providing new information and a smaller <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> is sufficient.</p></list-item><list-item><p>The element <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> (scaled residuals) are approximately
normally distributed between approximately <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx40" id="paren.41"/> and
show comparable frequency distributions across sites.</p></list-item></list></p>
      <p><?xmltex \hack{\noindent}?>Physical
<list list-type="bullet"><list-item><p>Attribution of elements to sources and element-to-element ratios within
a source are consistent with existing measurements (e.g. published source
profiles and source-based element-to-element ratios).</p></list-item><list-item><p>Sources retrieved in several size fractions show reasonable consistent
attribution of elements with co-varying time series.</p></list-item><list-item><p>Sources show meaningful diurnal variations and concentration gradients
from kerbside to urban background to rural sites (local: strong variations
and large gradients; regional: flat diurnal patterns and minimal gradients).</p></list-item><list-item><p>Correlations of factor time series with external tracers (e.g. traffic
with NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>) are logical.</p></list-item></list></p>
      <p>The goal of the present analysis is to conduct ME-2 analyses (unconstrained
or constrained) that meet the criteria outlined above for each of the three
size fractions on the combined data from all three sites. However, for all
size fractions, unconstrained ME-2 (i.e. uncontrolled rotations or
conventional PMF) yielded factors containing signatures of multiple emission
sources (e.g. mixed brake wear and other traffic-related processes, or mixed
S-rich and solid fuel) and were therefore considered non-optimal solutions
(Supplement Figs. S1–S4). Therefore, we applied rotational controls, using
the <inline-formula><mml:math display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> value approach (Eq. <xref ref-type="disp-formula" rid="Ch1.E3"/>). A central challenge of
this approach is the construction of appropriate anchor profiles, which
cannot be drawn directly from the literature, because the attribution of
elements to sources and the element-to-element ratios within a source are not
consistent across different studies (e.g. <xref ref-type="bibr" rid="bib1.bibx55" id="altparen.42"/>). Therefore, to
find clean model rotations, anchor profiles were determined within the ME-2
analysis as described below.</p>
      <p>In brief, this analysis strategy (outlined in Fig. <xref ref-type="fig" rid="Ch1.F2"/>,
and illustrated for the current study in Supplement Fig. S5) involves the
construction of a basis set of source profiles by iterating between
(1) analysis of a subset of data in which one or more factors can be clearly
resolved and their profiles added to the basis set and (2) analysis of the
full data set using the existing basis set as anchors to determine whether the
existing basis set is sufficient or additional anchor profiles are needed.
Finally, sensitivity tests are used to assess the uncertainties associated
with the final solution. Implementation of this analysis strategy requires
four types of ME-2 analyses, denoted ME2_all, ME2_subset,
Profile_unresolved, and Sensitivity_test, which are discussed in detail
below.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Schematic representation of the ME-2 analysis strategy. Four types
of ME-2 analyses are represented: (1) ME-2 on entire data set (ME2_all),
(2) ME-2 on a subset of data (ME2_subset, e.g. by high and low SNR),
(3) profile determination or estimation of factors unresolvable by ME2_all
or ME2_subset (PROF_unresolved), and (4) sensitivity tests to quantify
rotational model uncertainties (Sensitivity_test). For simplicity, we show
a case where analysis of two subsets of the data set is sufficient to
construct the source profile basis set but where in theory <inline-formula><mml:math display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula> segments can be
used. See Supplement Fig. S5 for application to data sets used in this study.</p></caption>
          <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f02.pdf"/>

        </fig>

      <p>ME2_all refers to the analysis of the entire data set (i.e. all time
points). The initial ME2_all analysis in Fig. <xref ref-type="fig" rid="Ch1.F2"/> is an
unconstrained analysis and is primarily used to identify time segments that
may be useful for resolving anchor profiles of specific factors. All
subsequent ME2_all analyses utilize the profile basis set built up in
previous steps by constraining successfully retrieved profiles during these
steps. An ME2_all analysis is defined as successful only when the entire
data set is well explained according to the criteria given above.</p>
      <p>ME2_subset denotes analysis of a subset of the full data set in the rows
(<inline-formula><mml:math display="inline"><mml:mi>i</mml:mi></mml:math></inline-formula>) dimension. This subset need not be a single continuous block and can be
constructed, for example, from separate periods in which a particular source is
evident. ME2_subset analyses utilize the basis set built up in previous
steps and are considered successful (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>) if the
entire subset is well explained according to the above criteria. To maximize
adaptation of the basis set to the entire data set (rather than remaining
fixed to a previously analysed and quasi-arbitrary subset), the basis set is
allowed to evolve after each successful ME2_subset (or ME2_all)
analysis – i.e. the ME2_subset output profiles become the new basis set.
Strategies used for selecting subsets may vary with the data set; however, it
is critical that the entire data set be well investigated, by ensuring that
the entire data set is contained in subsets and/or careful inspection of
ME2_all residuals. As an example, in the present analysis high
signal-to-noise data at MR and NK were analysed separately (subset 1)
from low signal-to-noise data at DE (subset 2). The need for a separate
DE analysis was indicated by strong residuals in the ME2_all analysis
using the basis set derived from subset 1. This indicated that an
additional source (industrial) was needed to fully describe the data set.
Other subset selection strategies could include, for example, size fraction, air mass
origin, wind direction, or suspected source influence.</p>
      <p>Profile_unresolved is used to generate an appropriate anchor profile for a
factor whose presence is indicated in the solution but cannot be cleanly
resolved by ME2_subset. Thus while Profile_unresolved and ME2_subset
may employ similar analytical strategies (e.g. analysis of a data subset),
Profile_unresolved is distinguished in that (1) success/failure criteria
are applied only with respect to a specific factor and that (2) only the profile
of this specific factor is added to the basis set for future analyses. As an
example, in the present study, a profile for the PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> brake
wear factor was resolved by analysing NK data using an excessive number of
factors. Although non-brake wear factors exhibited non-interpretable
mixing/splitting, the brake wear factor was judged clean based on element
ratios consistent with literature, a strong temporal correlation with
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, and low overall unexplained variation in the solution. Other
Profile_unresolved methods could include, for example, (1) an average profile over
periods where the source of interest dominates the total signal or (2) use or
estimation of a profile from the literature.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Source profile constraints.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Criteria</oasis:entry>  
         <oasis:entry colname="col3">Constraints</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Relative intensity in brake wear factor of</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Cu <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Zn <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Zr <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Mo <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Sn <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Sb <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ba</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>75</mml:mn></mml:mrow></mml:math></inline-formula> %</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Al <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Si in resuspended dust factor</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>40 % of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>0.3</mml:mn><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Mg <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na in aged sea salt factor</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>40</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula> of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>0.12</mml:mn><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Relative intensity in brake wear factor of</oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Cu <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Zn <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Zr <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Mo <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Sn <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Sb <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> Ba</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>70</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="italic">%</mml:mi></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Al <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Si in resuspended dust factor</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>40 % of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>0.3</mml:mn><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Mg <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na in aged sea salt factor</oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>40 % of <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn>0.12</mml:mn><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col2">Avg. Cl <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na in mean good solutions of PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> in sea/road salt factor</oasis:entry>  
         <oasis:entry colname="col3">Cl <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 20 % of avg.</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">All</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>  
         <oasis:entry colname="col3"><inline-formula><mml:math display="inline"><mml:mo>≤</mml:mo></mml:math></inline-formula> 10 % of min. <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>/</mml:mo><mml:msubsup><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext><mml:mi mathvariant="normal">c</mml:mi></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table><table-wrap-foot><p> <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx47" id="text.43"/>, also used, for example, by
<xref ref-type="bibr" rid="bib1.bibx13" id="text.44"/>. <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> Average sea water composition
<xref ref-type="bibr" rid="bib1.bibx49" id="paren.45"/>. <inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> Minimum <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> of good
solutions, after physical criteria are met.</p></table-wrap-foot></table-wrap>

      <p>Sensitivity_test investigates the uncertainties in the ME-2 solution
associated with the final basis set (fully constrained ME2_all). The
robustness or uncertainty is investigated with anchor sensitivity analyses
for each size fraction separately (three sites combined per size). Random
profiles of all source profiles in ME2_all are generated over 10 000 runs
by varying the relative intensity of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>f</mml:mi><mml:mrow><mml:mi>k</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with an anchor of <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>20 %
of the final model solutions. This allowed a systematic exploration of
a large area of the solution space around the final solutions. Physically and
mathematically meaningful solutions were selected according to the source
profile constraints given in Table <xref ref-type="table" rid="Ch1.T1"/>. By obeying these
constraints in this study, one assures that the other source profiles are
meaningful solutions as well. In the coarse fraction, 26 % of the runs
were classified as good solutions, while 40 and 64 % are good in
intermediate and fine fractions. Factor profile and time series uncertainties
are defined as 1 SD of the good solutions (note that these uncertainties
are rather small (see, for example, small shaded areas in time series in
Figs. <xref ref-type="fig" rid="Ch1.F4"/>, <xref ref-type="fig" rid="Ch1.F5"/>,
<xref ref-type="fig" rid="Ch1.F7"/>–<xref ref-type="fig" rid="Ch1.F12"/>,
<xref ref-type="fig" rid="Ch1.F14"/>) and an implication of the criteria in
Table <xref ref-type="table" rid="Ch1.T1"/>, even though these criteria are not strongly
restrictive). An anchor of <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>50 % led to a higher percentage of
meaningless solutions, while the uncertainties were comparable to the
<inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>20 % anchor runs. This indicates that the rotational model
uncertainties are rather driven by the criteria in
Table <xref ref-type="table" rid="Ch1.T1"/> than by how much the profiles are allowed to
vary. In other words, the percentage of accepted solutions reflects
computational efficiency rather than the robustness of the base solution. The
brake wear profile constraint ensures a clean factor without mixing of
elements related to other traffic processes or resuspended dust that occurs
due to the dominant contribution of MR to <inline-formula><mml:math display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> with its high temporal
covariance of most elements. The constraints based on literature values
guarantee solutions that have environmentally meaningful attributions of
elements to sources and element-to-element ratios within a source. Note that
the errors reported for this analysis deal explicitly with model errors and
do not account for systematic errors in the RDI-SR-XRF system that do not
affect the PMF model operation (e.g. flow rate, element calibrations). For a
detailed discussion of these sources of uncertainty, see <xref ref-type="bibr" rid="bib1.bibx57" id="text.46"/>.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results and discussion</title>
<sec id="Ch1.S3.SS1">
  <title>ME-2 source apportionment</title>
      <p>The ME-2 analysis on the three data sets resulted in a total of nine source
profiles as shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/> (values in Supplement
Tables S1–S3), with the factor time series for each site in Supplement
Figs. S6–S8 (PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, respectively). The coarse fraction yielded the source
factors (notable elements in brackets) brake wear (Cu, Zr, Sb, Ba), other
traffic-related (Fe), resuspended dust (Si, Ca), sea/road salt (Cl), aged sea
salt (Na, Mg) and industrial (Cr, Ni). The intermediate fraction yielded the
same factors except for the industrial, instead yielding an S-rich (S) factor. In the
fine fraction a traffic-related (Fe, Cu, Zr, Sb, Ba) factor was found as well
as resuspended dust, sea/road salt, aged sea salt, reacted Cl (Cl), S-rich
and solid fuel (K, Pb). The other elements (Al, P, Ti, V, Mn, Zn, Br, Sr, Mo,
Sn) are not uniquely emitted by a particular emission source and are
attributed to several factors. It should be noted that the concentrations for
the factor time series reported below reflect only the elements measured by
SR-XRF analysis and not the other constituents associated with the various
source types. In particular the lighter elements (H, C, N, O) are not
included and may in some cases dominate the total mass associated with
a source. The relative contribution to the factors discussed herein are also
relative to the measured elemental mass resolved. Although the analysis below
includes only trace elements, which constitute a minor fraction of the total
mass, the results are important for determining source temporal
characteristics and interpreting trends in bulk particle properties such as
total PM mass.</p><?xmltex \hack{\newpage}?>
<sec id="Ch1.S3.SS1.SSS1">
  <title>Brake wear and other traffic-related</title>
      <p>Factors related to brake wear were resolved in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> size fractions; the profiles are shown in
Fig. <xref ref-type="fig" rid="Ch1.F3"/>, with time series and diurnal variations in
Fig. <xref ref-type="fig" rid="Ch1.F4"/>. The relative contribution to this factor
is more than 70 % for V, Cu, Zn, Zr, Sn, Sb and Ba in both size
fractions, and more than 70 % for Cr, Ni, Sr and Mo in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Zn can be emitted both from brake and tyre wear,
indicating that these factors might be a mixture of various wearing processes
<xref ref-type="bibr" rid="bib1.bibx44" id="paren.47"/>. Factors for other traffic-related emissions in these two
size fractions (Figs. <xref ref-type="fig" rid="Ch1.F3"/> and <xref ref-type="fig" rid="Ch1.F5"/>)
are dominated by Fe, with around 86 % of the mass explained by this
element. The fine-fraction analysis retrieved one traffic factor with
a mixture of brake wear and other traffic-related emissions with 84 % of
the mass explained by Fe (relative contributions more than 70 % for Fe,
Cu, Zr, Sb and Ba). This mixed factor is similar to that reported by
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx3" id="text.48"/> and <xref ref-type="bibr" rid="bib1.bibx8" id="text.49"/> although the ratio of
Fe to other elements is variable between studies. V and Sr are typically not
attributed to traffic factors but rather to industrial or oil combustion
emissions (V) and dust resuspension (Sr) <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx37" id="paren.50"/>.
However, both elements are found in trace amounts in fuel additives and brake
lining, and <xref ref-type="bibr" rid="bib1.bibx24" id="text.51"/> showed enhanced Sr and V concentrations
inside a tunnel compared with ambient concentrations outside. In the absence
of other sources, the relative contribution of these elements might dominate
these traffic factors.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Source profiles of ME-2 results on combined data of the MR-NK-DE
sites. The bars (left <inline-formula><mml:math display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) represent the average element intensity to
each factor in ng <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">ng</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; circles (right <inline-formula><mml:math display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis) represent the
fraction of the total predicted concentration for a given element. Data are
given as mean of good solutions <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>1 SD from the anchor sensitivity
analysis. Note that not all factors are retrieved in all size fractions. See
Supplement Tables S1–S3 for the values.</p></caption>
            <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f03.pdf"/>

          </fig>

      <p>For the brake wear and the PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> traffic factors, the
Cu <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Sb ratios of 6.3–7.1 fall within the range of 5.7–8.2 for previous
measurements at MR and NK by <xref ref-type="bibr" rid="bib1.bibx28" id="text.52"/> and depend on brake pad
compositions and contributions of metals from other sources <xref ref-type="bibr" rid="bib1.bibx44" id="paren.53"/>.
The Cu <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Ba ratios of 1.1–1.4 are in good agreement with the median
ratio of 1.2 obtained by <xref ref-type="bibr" rid="bib1.bibx50" id="text.54"/>.</p>
      <p><?xmltex \hack{\newpage}?>All the traffic-related factors are strongly influenced by local traffic
emissions with steep MR to NK to DE concentration gradients
(Figs. <xref ref-type="fig" rid="Ch1.F4"/>–<xref ref-type="fig" rid="Ch1.F5"/>).
Concentrations at MR are 3.6–6.8 and 9.9–28 times higher than at NK and DE,
respectively. The diurnal variations show a double maximum during the day
corresponding to rush hours. Most of the mass is emitted in the coarse
fraction, with concentrations at MR being 2.6–3.6 and 7.5 times higher than
in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, respectively. The time
series correlate well across sizes (Pearson's <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> 0.67–0.81), indicating
similar emission processes. Both traffic sources are well correlated with
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> across sites and sizes (Pearson's <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> 0.53–0.72) as shown in
Fig. <xref ref-type="fig" rid="Ch1.F6"/> for MR (NK and DE in Supplement Fig. S9).
Figure <xref ref-type="fig" rid="Ch1.F6"/> also shows traffic flows at MR of light-
(LDV) and heavy-duty vehicles (HDV) (vehicles <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn>5.2</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> long, LDV;
vehicles <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>5.2</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> long, HDV). The diurnal variations are much stronger for
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and HDV than for the traffic factors and LDV. The ratios between
values at 08:00 and 02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> are about 4.1 for the former and 2.0
for the latter, probably caused by more strongly enhanced emissions between
HDV and LDV for NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (factor of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn>37</mml:mn></mml:mrow></mml:math></inline-formula>) relative to brake wear (factor
of <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>∼</mml:mo><mml:mn>10</mml:mn></mml:mrow></mml:math></inline-formula>), as identified by <xref ref-type="bibr" rid="bib1.bibx8" id="text.55"/>. NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> seems
therefore more directly related to HDV numbers, while the traffic factors are
more influenced by total vehicle number.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the brake wear
factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>.
Time series show the mean of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas.
Diurnals show the mean of the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the
hour being the start of a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>
means sampling from 00:00 to 02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f04.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the other
traffic-related factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f05.pdf"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS2">
  <title>Resuspended dust</title>
      <p>Resuspended dust factors were resolved in all size fractions; the profiles
are shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>, with time series and diurnal
variations in Fig. <xref ref-type="fig" rid="Ch1.F7"/>. The source profiles are very
similar across sizes and the mass is dominated by Si, Ca and Fe, consistent
with the upper continental crust composition <xref ref-type="bibr" rid="bib1.bibx47" id="paren.56"/> and previous
source apportionment studies <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx14 bib1.bibx46" id="paren.57"/>.</p>
      <p>The scaled residuals (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>) ratios exceed <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>3 for Na, Si
and Ca (coarse); Na, Al, Si and Ca (intermediate); and Al and Si (fine) and/or
are skewed at the sites relative to each other. This spread in the scaled
residuals for these dust-related elements may indicate different dust
profiles across sites, especially at DE relative to the city sites. This is
potentially caused by varying dust compositions or emission processes.
Resuspension in the city is dominated by road dust influenced by
anthropogenic activities and by other dust-generating activities, such as
construction works, in contrast to influences from natural soils at DE. This
is in line with <xref ref-type="bibr" rid="bib1.bibx50" id="text.58"/>, where city-specific soil profiles are
constrained in the ME-2 analysis on data of combined cities, and with
<xref ref-type="bibr" rid="bib1.bibx1" id="text.59"/>, where ME-2 yielded a road dust resuspension distinct from
a mineral dust factor. In the current study, increasing <inline-formula><mml:math display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula> yielded factors
with high relative intensities of Ca and of Al and Si. However,
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>Q</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mtext>exp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and structures in <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>e</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>i</mml:mi><mml:mi>j</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> remain unaffected,
indicating that temporal co-variance and emission source strengths of these
elements are too similar across sites for the model to retrieve more than one
dust factor.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Diurnal variations in the brake wear (PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> –
coarse, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> – intermediate) and other traffic-related (coarse,
intermediate, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> – fine) factors at MR compared to diurnal
variations of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> (left) and traffic flow (right). Hour of day is start
of a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00
to 02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>). Note the scaling applied to several tracers.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f06.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the resuspended
dust factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f07.pdf"/>

          </fig>

      <p>Similar to the factor termed “traffic-related”, dust is mainly emitted in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> with up to 13.6 times higher concentrations than in the
smaller fractions. The factor time series (Fig. <xref ref-type="fig" rid="Ch1.F7"/>)
indicate enrichment at MR relative to NK and DE, especially for the coarse
fraction (MR <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> NK ratio of 3.4 and MR <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> DE of 7.8) and are well
correlated among all sizes (Pearson's <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> 0.62–0.78). The diurnal variations
show strong daytime maxima, most likely from anthropogenic <?xmltex \hack{\mbox\bgroup}?>activities<?xmltex \hack{\egroup}?> (mainly
traffic) throughout the day. The increase at 08:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> (sampling
08:00–10:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>) occurs 2 h after increasing traffic numbers,
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and traffic-related source emissions
(Fig. <xref ref-type="fig" rid="Ch1.F6"/>). The delay is probably caused by
a combination of two effects. On the one hand, the RH still increases during
morning hours, resulting in wetter road surfaces than later in the day
(Supplement Fig. S10). On the other hand, increasing traffic flows induce
increased wind movements in the street canyon, resulting in enhanced particle
resuspension <xref ref-type="bibr" rid="bib1.bibx7" id="paren.60"/>.</p>
</sec>
<sec id="Ch1.S3.SS1.SSS3">
  <title>Sea/road salt, aged sea salt and reacted Cl</title>
      <p>Sea/road salt and aged sea salt were resolved in all sizes;
Fig. <xref ref-type="fig" rid="Ch1.F3"/> shows the profiles, with time series and diurnal
variations in
Figs. <xref ref-type="fig" rid="Ch1.F8"/>–<xref ref-type="fig" rid="Ch1.F9"/>. The mass
of sea/road salt comes almost exclusively from Na and Cl, whereas aged sea
salt is largely driven by Na. The crustal component of Na is less than
1 % in this study, based on the Na <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Si ratio found in the upper
continental crust <xref ref-type="bibr" rid="bib1.bibx59" id="paren.61"/>. Therefore, the combination of Na with
relative contributions of more than 50 % for coarse Mg, S and K, but
depleted Cl supports aged particles with a sea salt origin, in which the Na
is neutralized by compounds not resolved by our analysis (e.g. nitrate). The
Mg <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> Na mass ratio of the sea/road salt factor is only 0.054 in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (theoretical sea salt ratio is 0.12;
<xref ref-type="bibr" rid="bib1.bibx49" id="altparen.62"/>). De-icing salt was applied on the roads in London
during the measurement campaign, and this salt is typically composed of
coarse NaCl, resulting in enriched coarse Na relative to Mg concentrations
after the particles are resuspended in the air. The low concentrations of
fine sea salt are in line with <xref ref-type="bibr" rid="bib1.bibx33" id="text.63"/>, since sea salt is mainly
emitted as particles with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>&gt;</mml:mo><mml:mn>1.0</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the sea/road
salt factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f08.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the aged sea
salt factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f09.pdf"/>

          </fig>

      <p>The data suggest that a fraction of the aged sea salt is directly
transported from the sea, while part comes from resuspended sea salt
particles after deposition on roads. Direct transport is indicated by the
diurnal variations
(Figs. <xref ref-type="fig" rid="Ch1.F8"/>–<xref ref-type="fig" rid="Ch1.F9"/>), which
have no obvious pattern – peaks occur at different hours of the day
throughout the entire time series, whereas resuspension would likely peak
during the day with vehicle use. Additional support is provided by NAME
dispersion modelling and wind direction analyses, which indicate that high
concentration episodes in the aged sea salt factor coincide with air masses
from the sea. The sea salt concentrations also increase with increasing wind
speed, consistent with other Na observations in the UK (Supplement Fig. S11;
<xref ref-type="bibr" rid="bib1.bibx52" id="altparen.64"/>). However, the PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> concentrations of
the aged sea salt factor are enhanced by a factor of 1.3 and 2.2 at the
kerbside (MR) site relative to the urban background (NK) and rural (DE)
sites, respectively. This suggests that aged sea salt concentrations are also
significantly modulated by human activity in the form of resuspension.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the reacted Cl
factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f10.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the S-rich
factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD
as whiskers, with the hour being the start of a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period
(00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to 02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f11.pdf"/>

          </fig>

      <p>Reacted Cl is unique to PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (profile in
Fig. <xref ref-type="fig" rid="Ch1.F3"/>) and is mainly driven by an event at MR and NK
lasting from 16:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> on 5 February to 04:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> on 7 February 2012 (time
series and diurnal variations in Fig. <xref ref-type="fig" rid="Ch1.F10"/>; around
12 February concentrations at MR are high as well, but SR-XRF data at NK and
meteorological data at BT Tower are absent during this period, making it
impossible to study this episode in detail). Stagnant conditions prevailed in
the city with low average wind speed of 2.1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> at about
190 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">g</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> (data from BT Tower). The NAME 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> backwards
footprints show that the air sampled at MR and NK was dominated by local
London air. In contrast, during this episode the air mass at DE is dominated
by a mixture of London air and air from the southern UK. Although fine Cl can be
emitted by combustion sources such as waste incineration <xref ref-type="bibr" rid="bib1.bibx35" id="paren.65"/>
and coal combustion <xref ref-type="bibr" rid="bib1.bibx65" id="paren.66"/>, this factor does not correlate with
combustion-related species such as K, Zn, Pb and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The event
discussed above does correlate with a strong peak in coarse-mode aged sea
salt (Figs. <xref ref-type="fig" rid="Ch1.F9"/>–<xref ref-type="fig" rid="Ch1.F10"/>). Sea
salt particles in all size fractions have likely reacted with nitric acid
(<inline-formula><mml:math 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>), forming hydrochloric acid (HCl). Due to stagnant conditions,
follow-up reactions between HCl and ammonia (<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) could have taken
place, forming ammonium chloride (<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mi mathvariant="normal">Cl</mml:mi></mml:mrow></mml:math></inline-formula>). These particles occur
mainly in the fine mode due to the highest surface-to-volume ratios.
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations were high during this
event, favouring such reactions. AMS measurements also show this unique
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> episode at MR and NK (<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is negligible during the
rest of the IOP and at DE). For this specific period the AMS aerosol charge
balance in the city holds when <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">Cl</mml:mi><mml:mo>-</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> is included, while this ion is
not needed at DE or during the rest of the time to balance <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mo>+</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>
within the uncertainties of the measurements, indicating the presence of fine
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mi mathvariant="normal">Cl</mml:mi></mml:mrow></mml:math></inline-formula> particles.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the solid fuel
factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f12.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><caption><p>Time series of the solid fuel factor at NK and DE compared to the
Aethalometer wood burning absorption coefficient at wavelength 470 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mtext>abs</mml:mtext><mml:mo>,</mml:mo><mml:mtext>wb</mml:mtext></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> at 470 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>) and to the solid fuel organic
aerosol (SFOA) factors resolved with AMS-PMF.</p></caption>
            <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f13.pdf"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS1.SSS4">
  <title>S-rich and solid fuel</title>
      <p>The S-rich factor, mainly composed of S, was resolved in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>; the profile is shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>,
with time series and diurnal variations in Fig. <xref ref-type="fig" rid="Ch1.F11"/>.
This factor likely corresponds to secondary sulfates, consistent with the
results of many previous source apportionment studies
<xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx46 bib1.bibx54" id="paren.67"/>. All sites show similar
concentrations without any patterns visible in the diurnal variations,
consistent with regional sources. This factor correlates well with AMS
<inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> measurements (Pearson's <inline-formula><mml:math display="inline"><mml:mi>R</mml:mi></mml:math></inline-formula> 0.61–0.86) and is elevated
with air masses from the European mainland, mainly occurring during the
second half of the campaign (Supplement Fig. S12).</p>
      <p>The solid fuel factor was also resolved in the fine fraction (profile in
Fig. <xref ref-type="fig" rid="Ch1.F3"/>, time series and diurnal variations in
Fig. <xref ref-type="fig" rid="Ch1.F12"/>). The mass of this factor is dominated by S
and K, while the relative contributions to this factor are more than 60 %
for K, Zn and Pb. Surprisingly, the time series are very similar at all sites
and are likely influenced by relatively fresh emissions from many point
sources surrounding the measurement stations, including wood, coal and peat
emissions in varying contributions <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx67" id="paren.68"/>. The
S <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> K ratio of 1.5 is well within the observed range of 0.5–8 for fresh
to transported and aged emissions
<xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx46 bib1.bibx56" id="paren.69"/>. The solid fuel source is
compared to particle light absorption data by Aethalometer measurements
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>b</mml:mi><mml:mrow><mml:mtext>abs</mml:mtext><mml:mo>,</mml:mo><mml:mtext>wb</mml:mtext></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> in <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>; not available at MR) and solid fuel factors resolved by AMS-PMF on organic aerosol data
<xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx66 bib1.bibx67" id="paren.70"/>. The time series of the various
solid fuel tracers are very similar, especially for the light-absorbing
particles and organic aerosol as shown for NK and DE in
Fig. <xref ref-type="fig" rid="Ch1.F13"/> (tracers at MR are similar to NK). The
different correlations seen in this figure are caused by the sampling of air
containing various burning stages of solid fuel burning, emitting K and other
species in different ratios.</p>
      <p>In the intermediate fraction S contributes around 58 % to the mass of the
S-rich factor (profile in Fig. <xref ref-type="fig" rid="Ch1.F3"/>, time series and diurnal
variations in Fig. <xref ref-type="fig" rid="Ch1.F11"/>) and the relative contributions
of S, Br and Pb are <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>50</mml:mn></mml:mrow></mml:math></inline-formula> % in this factor. <xref ref-type="bibr" rid="bib1.bibx33" id="text.71"/> showed
that S is predominantly found in <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, but particles of up to
several micron were identified to contain S as well. The intermediate
S-rich factor contains signatures of both fine-fraction S-rich and solid fuel
with similar concentrations at all sites and no obvious diurnal patterns.</p>
</sec>
<sec id="Ch1.S3.SS1.SSS5">
  <title>Industrial</title>
      <p>Constrained ME-2 analysis in the PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> fraction on data
across sites revealed large residuals with clear structures at DE for Cr, Ni
and Mo, indicating that the data at the rural site were not fully explained.
The “ME2_seg_low_SNR” analysis on DE PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (see
Fig. <xref ref-type="fig" rid="Ch1.F2"/> and Supplement Fig. S5) <?xmltex \hack{\mbox\bgroup}?>successfully<?xmltex \hack{\egroup}?> yielded
a factor, potentially industrial, containing mainly these three elements
without significant residuals.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F3"/> shows the source profile and
Fig. <xref ref-type="fig" rid="Ch1.F14"/> the time series and diurnal variations.
This source is mainly found at DE and consists of 70 % of Cr and Ni. The
time series at MR and NK show only a few single peaks and can therefore not
be attributed to this particular source. The spiky time series at DE are
typical indications for influences of one or several point sources close to
this rural site. These sources are possibly found in the southwest as concentrations
were elevated under these conditions (Supplement Fig. S13). The towns of
Detling and Maidstone are located towards the southwest of the Kent Showgrounds.
<xref ref-type="bibr" rid="bib1.bibx58" id="text.72"/> studied Cr, Ni and Mo in Sweden and found that road
traffic including road wear is the largest emitter of these elements,
followed by industries, incineration, agriculture and waste water treatment.
<xref ref-type="bibr" rid="bib1.bibx19" id="text.73"/> identified Pb, Ni and Cr in emissions from municipal
wastewater sludge incinerators. Except for agricultural fields, none of those
activities likely contribute to the emission source at DE. Probably some
local activities at the Kent Showgrounds or small-scale industry in Maidstone
like stainless steel production <xref ref-type="bibr" rid="bib1.bibx45 bib1.bibx62" id="paren.74"/> contributes to
this factor.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><caption><p>Time series (left) and diurnal variations (right) of the industrial
factor at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Time series show the mean
of all good solutions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as shaded areas. Diurnals show the mean of
the time series <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> SD as whiskers, with the hour being the start of
a 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> sampling period (00:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula> means sampling from 00:00 to
02:00 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">UTC</mml:mi></mml:math></inline-formula>).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f14.pdf"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Synthesis</title>
      <p>The trace element source apportionment results indicate the ability to
characterize the environment-dependent variability of emissions in and around
London. The analyses of data from the combined sites retrieve a single source
profile representative of all three sites, thus allowing a direct comparison
of the source strengths across sites. Source strengths strongly differ
between sites and sizes, as seen in Fig. <xref ref-type="fig" rid="Ch1.F15"/>. Most of
the analysed element mass is emitted in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> with 78 %
at MR, 73 % at NK and 65 % at DE, while only 17–22 % and
6–13 % is emitted in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
respectively.</p>
      <p>The separate analyses on the three size fractions provide insights into the
emissions of sources to specific size fractions
(Fig. <xref ref-type="fig" rid="Ch1.F15"/>). The regionally influenced S-rich and solid fuel factors are restricted to the smaller size fractions with concentration
ratios of 1.0–1.8 between sites roughly 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> apart. These factors,
especially solid fuel, are affected by many anthropogenic point sources and
are influenced by emissions not only in and around London but also from
elsewhere in the UK and northern Europe. In contrast to other sources, solid
fuel is expected to be more prevalent in more rural parts of the UK than in
the smoke-controlled inner city areas. The industrial factor is restricted to
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and affects the air quality under specific
meteorological conditions around the rural site, which is generally a region
characterized by much lower pollution.</p>
      <p>The other sources, except reacted Cl, emit elements in all three size
fractions. London's city centre is a hotspot of anthropogenic activities,
resulting in high pollution levels of locally influenced sources directly
related to population density. Brake wear, other traffic-related and
resuspended dust factor concentrations are drastically different within
different micro-environments and size fractions, indicating major
heterogeneity in human exposure patterns. Concentrations at the kerbside are
up to 7 and 28 times higher than at NK and DE, respectively, and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> concentrations are up to 4 and 14 times higher than
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, respectively. During this
winter period the sea salt sources, although from natural origin and strongly
meteorologically driven, are enriched in the city in the form of sea salt
resuspension from the roads.</p>
      <p>Both direct emissions and resuspension have been identified above as
important sources of trace elements. The trend in coarse aged sea salt across
the three sites provides insight into the relative importance of these
processes. We assume that all aged sea salt originates from a regional,
site-independent source, and that the concentration gradient in this factor
between sites thus reflects the effect of local resuspension processes of
naturally deposited aged sea salt. Although sea salt emissions are typically
considered a natural process, human activities (vehicle-induced resuspension)
enhance the concentrations of the coarse aged sea salt by 1.7–2.2 in the
city relative to the rural site (Fig. <xref ref-type="fig" rid="Ch1.F15"/>). These
ratios provide an upper limit for the resuspension enhancement (and thus
a lower limit for the enhancement due to direct emissions) for the
anthropogenically influenced factors, whose concentrations at DE may already
be increased by local emissions. The lower limits for direct emission
enhancement ratios in the coarse fraction at MR relative to DE are 3.5 to
12.7 for brake wear, other traffic-related, dust and sea/road salt factors
(1.4–5.5 for NK <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> DE). Direct emissions for the traffic-related factor
show similar enhancement in all size fractions, whereas enhancement of the
other anthropogenically influenced factors are a factor of 1.5–3.0 lower in
the smaller size fractions. These results indicate that direct source
emission processes occur mainly for coarse particles and are dependent on the
micro-environment. The S-rich and solid fuel factors have negligible
resuspension influences (similar concentrations across sites). Air quality in
London can be improved by the development of policies aiming to reduce
resuspension processes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><caption><p>Mean, median and 25–75th percentile concentrations of the nine
different ME-2 factor time series at MR, NK and DE for PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. Note that not all factors
are retrieved in all size fractions.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/15/11291/2015/acp-15-11291-2015-f15.pdf"/>

        </fig>

      <p>Trace elements are often used as chemically conserved source markers. Here we
assess the ability of elements measured herein to serve as unique tracers for
specific sources. For a tracer to be considered good, we require that a given
source has a high relative contribution (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>70</mml:mn></mml:mrow></mml:math></inline-formula> %) to a specific element,
i.e. that the element is mainly attributed to a single source
(Fig. <xref ref-type="fig" rid="Ch1.F3"/>). We suggest Cu, Zr, Sb or Ba as markers for
brake wear in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>. The relative
contributions are <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>93</mml:mn></mml:mrow></mml:math></inline-formula>, 83, 93 and 96 % for Cu, Zr, Sb and Ba,
respectively. The attribution of these elements to the traffic factor in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> with relative contributions between 69 and 84 %
also suggests brake wear emissions in this size fraction. Fe is typically
also attributed to brake wear emissions
<xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx8 bib1.bibx28" id="paren.75"/>. However, we observed no Fe
in the brake wear factors; instead 86 and 65 % of Fe were attributed to
other traffic-related processes in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (74 % of Fe to the traffic-related factor in
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>). Furthermore, around 19 % of Fe contributed to
the resuspended dust factors in all three size fractions. We therefore
recommend attributing Fe only to a specific source in combination with other
markers. Si and Ca in all size fractions can be used as a surrogate for
resuspended dust with relative contributions between 72 and 75 % for Si
and between 80 and 85 % for Ca. Coarse and intermediate
fraction Cl (relative contributions <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn>87</mml:mn></mml:mrow></mml:math></inline-formula> %) are markers for fresh sea
salt (preferably combined with Na and Mg), while fine-fraction Cl is not
a unique source indicator. Depending on the data set it can indicate waste
incineration <xref ref-type="bibr" rid="bib1.bibx35" id="paren.76"/>, coal combustion <xref ref-type="bibr" rid="bib1.bibx65" id="paren.77"/> or reacted
Cl as <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">NH</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:mi mathvariant="normal">Cl</mml:mi></mml:mrow></mml:math></inline-formula> particles (current study, relative contribution
59 %). A combination of fine-fraction K and Pb with relative
contributions of around 80 % indicates solid fuel in this study, but can
also be attributed to wood, coal or peat burning separately. Fine-fraction S
can typically be attributed to regionally transported secondary sulfate
(here only a 65 % relative contribution). Other elements can also be used
as source markers, but rather as a combination of elements than individually,
and preferably combined with measurements of other species.</p>
      <p>The analysis herein clearly shows the advantages of rotationally controlled
analyses relative to an unconstrained PMF solution. Supplement Figs. S1–S4
show the best solutions retrieved from unconstrained analyses for the
separate size fractions (four-, four-, and five-factor solutions for
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>,
respectively). The unconstrained PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> solution (Supplement
Figs. S1 and S4) yields high residuals of Ni, Cr, and Mo and does not resolve
a brake wear factor. The unconstrained PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> solution
(Supplement Figs. S2 and S4) likewise does not yield brake wear and
additionally fails to resolve aged (reacted) sea salt from regionally
transported sulfate and solid fuel, despite strong evidence for this
processing in the raw time series. Finally, the unconstrained
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> solution (Supplement Figs. S3 and S4) mixes secondary
sulfur and solid fuel sources. It also fails to explain major events
contained in the Cl-rich factor, apportioning significant Na to these events,
leading to high Na residuals. Higher-order solutions do not resolve these
problems, instead leading to uninterpretable splitting of the dust factor,
factors consisting only of single elements, and unstable solutions that are
highly dependent on algorithm initialization (seed).</p>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Trace element measurements were performed at kerbside, urban background and
rural sites to characterize the environment-dependent variability of
emissions in the European megacity of London during winter 2012. Sampling
with rotating drum impactors and subsequent synchrotron radiation-induced
X-ray fluorescence spectrometry yielded 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> element mass
concentrations in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> aerosol. Source apportionment using the ME-2 algorithm
in the PMF model was conducted on data sets comprising all three sites but
analysed separately for each size. Combining the sites enabled separation of
sources with high temporal covariance but significant spatial variability.
Separation of sizes improved source resolution by preventing sources
occurring in only a single size fraction from having too small a contribution
for the model to resolve. Anchor profiles for several factors were retrieved
by analysing specific data subsets and these profiles were successfully used
in the analyses of the complete data sets to retrieve clean factor profiles
and time series at all sites.</p>
      <p>The coarse fraction yielded (elements with highest relative contributions in
brackets) brake wear (Cu, Zr, Sb, Ba), other traffic-related (Fe),
resuspended dust (Si, Ca), sea/road salt (Cl), aged sea salt (Na, Mg) and
industrial (Cr, Ni) factors. The intermediate fraction yielded the same
factors except for the industrial, instead yielding an S-rich (S) factor. In
the fine fraction a traffic-related factor (Fe, Cu, Zr, Sb, Ba) was found as
well as resuspended dust, sea/road salt, aged sea salt, reacted Cl (Cl),
S-rich and solid fuel (K, Pb). The other analysed elements (Al, P, Ti, V, Mn,
Zn, Br, Sr, Mo, Sn) could not be attributed to a single factor. The brake
wear, industrial, reacted Cl and solid fuel factors could only be resolved
with the help of anchor profiles retrieved internally in the data sets.
Unconstrained ME-2 only led to mixed traffic-related/brake wear, resuspended
dust, sea/road salt and aged sea salt factors in the coarse fraction; to
mixed traffic-related/brake wear, resuspended dust, sea/road salt and mixed
aged sea salt/regional transport factors in the intermediate fraction; and to
traffic-related, resuspended dust, aged sea salt, mixed S-rich/solid fuel and
mixed sea/road salt/Cl-rich factors in the fine fraction.</p>
      <p>The regionally influenced S-rich and solid fuel factors are restricted to the
smaller size fractions, and have similar concentrations throughout the day
and across larger regions. The locally influenced sources show major
heterogeneity in human exposure patterns within different micro-environments.
The brake wear, other traffic-related and resuspended dust sources show steep
concentration gradients from kerbside to urban background to rural sites and
from PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> to PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> to
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> (ratios up to 28 and 14 for kerb-to-rural and
PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>-to-PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, respectively) and are
directly related to anthropogenic activities (mainly traffic flows) with
concentrations up to a factor of 4 higher during daytime relative to
night-time. The relative mass contributions are dominated by the sea salt
factors in PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>10</mml:mn><mml:mtext>–</mml:mtext><mml:mn>2.5</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula> and PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>2.5</mml:mn><mml:mtext>–</mml:mtext><mml:mn>1.0</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>, while the
regionally influenced factors dominate PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:mn>1.0</mml:mn><mml:mtext>–</mml:mtext><mml:mn>0.3</mml:mn></mml:mrow></mml:msub></mml:math></inline-formula>.</p>
      <p>The site-dependent concentration gradients in aged sea salt reflect the
effect of local resuspension processes. Human activities enhance the kerbside
concentrations of the coarse aged sea salt by a factor of 1.7–2.2 compared
with the rural site. For anthropogenically influenced factors, direct source
emissions provide a further kerb-to-rural enhancement of concentrations by
a factor of 3.5–12.7, and these direct emissions occur mainly for coarse
particles.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/acp-15-11291-2015-supplement" xlink:title="pdf">doi:10.5194/acp-15-11291-2015-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>We thank the Swiss National Science Foundation (SNSF grant 200021_132467/1),
the UK Natural Environment Research Council (NERC) ClearfLo consortium (NERC
grant NE/H00324X/1, NE/H0081368/1), and the European Community's Seventh
Framework Programme (FP/2007-2013, grant number 312284). J. G. Slowik was
supported by the SNSF Ambizione programme (grant PX00P2_31673), and
D. E. Young by a NERC PhD studentship (grant NE/I528142/1). The Detling site
was supported by the US Department of Energy Atmospheric Systems Research
Program (DOE award no. DE-SC0006002). We thank Empa for the RDI they loaned
us during the ClearfLo project. Parts of the work were carried out at the
Swiss Light Source, Paul Scherrer Institute, Villigen, Switzerland. We thank
Andreas Jaggi and Christophe Frieh for technical support at the beamline
X05DA. Parts of the study were also performed at the light source facility DORIS III at
HASYLAB/DESY. DESY is a member of the Helmholtz Association
(HGF).<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: X. Querol</p></ack><ref-list>
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