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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ACP</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7324</issn>
<publisher><publisher-name>Copernicus Publications</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-16-9693-2016</article-id><title-group><article-title>On the simultaneous deployment of two single-particle mass spectrometers at
an urban background and a roadside site<?xmltex \hack{\break}?> during SAPUSS</article-title>
      </title-group><?xmltex \runningtitle{On the simultaneous deployment of two single-particle mass spectrometers}?><?xmltex \runningauthor{M. Dall'Osto et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Dall'Osto</surname><given-names>Manuel</given-names></name>
          <email>dallosto@icm.csic.es</email>
        <ext-link>https://orcid.org/0000-0003-4203-894X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Beddows</surname><given-names>David C. S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>McGillicuddy</surname><given-names>Eoin J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff6">
          <name><surname>Esser-Gietl</surname><given-names>Johanna K.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff5">
          <name><surname>Harrison</surname><given-names>Roy M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2684-5226</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Wenger</surname><given-names>John C.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4109-976X</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Institut de Ciències del Mar, Consejo Superior de
Investigaciones Científicas (CSIC), Pg Marítim de la Barceloneta
37–49, 08003 Barcelona, Spain</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Institute of Environmental Assessment and Water Research (IDAEA)
Consejo Superior de Investigaciones Científicas (CSIC) C/Jordi Girona
18–26 08034 Barcelona, Spain</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>National Centre for Atmospheric Science, Division of Environmental
Health and Risk Management, School of Geography, Earth and Environmental
Sciences, University of Birmingham, Edgbaston, Birmingham, B15 2TT, UK</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Department of Chemistry and Environmental Research Institute,
University College Cork, Ireland</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Department of Environmental Sciences/Center of Excellence
in Environmental Studies, King Abdulaziz University,<?xmltex \hack{\newline}?> Jeddah, 21589, Saudi
Arabia</institution>
        </aff>
        <aff id="aff6"><label>a</label><institution>now at: Deutscher Wetterdienst, Meteorological Observatory
Hohenpeißenberg, Hohenpeißenberg, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Manuel Dall'Osto (dallosto@icm.csic.es)</corresp></author-notes><pub-date><day>2</day><month>August</month><year>2016</year></pub-date>
      
      <volume>16</volume>
      <issue>15</issue>
      <fpage>9693</fpage><lpage>9710</lpage>
      <history>
        <date date-type="received"><day>7</day><month>December</month><year>2015</year></date>
           <date date-type="rev-request"><day>5</day><month>February</month><year>2016</year></date>
           <date date-type="rev-recd"><day>17</day><month>May</month><year>2016</year></date>
           <date date-type="accepted"><day>8</day><month>June</month><year>2016</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>The aerosol time-of-flight mass spectrometer (ATOFMS) provides size-resolved
information on the chemical composition of single particles with high time
resolution. Within SAPUSS (Solving Aerosol Problems by Using Synergistic
Strategies), continuous ATOFMS measurements of ambient particles were made
simultaneously at two urban locations: urban background (UB) site and roadside (RS) site in the city of Barcelona (Spain) from 17 September to
18 October 2010. Two different instrumental configurations were used:
ATOFMS (TSI 3800) with a converging nozzle inlet (high efficiency at about
800–2000 nm) at the UB site and ATOFMS (TSI 3800-100) with an aerodynamic
lens inlet (high efficiency at about 300–700 nm) at the RS site. This is the
first time, to our knowledge, that two ATOFMS instruments have been deployed
in the same field study. The different instrument configurations had an
impact on the observed particle types at the two sites. Nevertheless,
10
particle types were detected at both locations, including local and regional
elemental carbon (22.7–58.9 % of total particles), fresh and aged sea salt
(1.0–14.6 %), local and regional nitrate-containing aerosols (3–11.6 %),
local lead-containing metallic particles (0.1–0.2 %), and transported
Fe-nitrate particles (0.8–2.5 %). The ATOFMS at the UB also characterized
four particle types: calcium-containing dust (0.9 %), Saharan dust
(1.3 %), vanadium-containing particles (0.9 %), and vegetative debris
(1.7 %). By contrast, the high statistical counts of fine particles
detected at the RS allowed identification of eight particle types. Four of
these contained organic nitrogen of primary and secondary origin, which
highlights the complex nature of the sources and processes that contribute
to this aerosol chemical component. Aminium salts were found related to
coarse sulfate-rich particle types, suggesting heterogeneous reaction
mechanisms for their formation. The other four particle types mainly
containing organic carbon were found spiking at different types of the day,
also showing a complex single-particle mixing state relationship between
organic carbon and nitrate. This ATOFMS study clearly shows that the
composition of atmospheric fine particles in Barcelona, and likely other
Mediterranean urban areas, is complex, with a wide range of local and
regional sources combining with chemical processing to produce at least
22 different particle types exhibiting different temporal behaviour.
The advantage of using two ATOFMS instruments is also demonstrated, with the
nozzle-skimmer configuration enabling detection of coarse dust particles and
the aerodynamic lens configuration allowing better identification of
particles rich in organic carbon and amines. Overall, we find that organic
nitrogen is a considerable fraction of the single particles detected,
especially at the traffic-dominated RS site. Further studies are needed,
especially at high time resolution, to better understand the sources and
properties of particulate organic nitrogen.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>A substantial number of studies have shown a relationship between measures
of particulate air pollution and a variety of adverse health indicators
(WHO, 2004). Formulation of cost-effective air pollution control policies
depends upon a sound knowledge of source contributions to ambient
concentrations. Only with such knowledge can realistic cost-benefit
evaluations be conducted. The major sources of ambient particles in most
urban areas are primary emissions from road traffic and other fuel
combustion, secondary particles arising from condensation or chemical
processing, and resuspension of soils and road dusts (AQEG, 2005; Harrison
et al., 2012). Marine aerosol can also contribute in coastal locations and
the interactions of anthropogenic trace gases with natural aerosol (i.e.
dust, sea salt) can also have significant effects on aerosol composition
(Abbatt et al., 2012).</p>
      <p>Measurement of particle composition by online mass spectrometry has
developed extensively over the last 2 decades and is currently the fastest
growing area of atmospheric aerosol research (Laskin et al., 2012). The
aerosol time-of-flight mass spectrometer (ATOFMS) has been used in many
previous field studies to determine the chemical constituents of atmospheric
aerosols (Pratt and Prather, 2012). It can identify both refractory and
non-refractory species in single particles and can provide size-resolved
information on particle sources and atmospheric processing at high time
resolution (Prather and Pratt, 2012; Laskin et al., 2012). The ATOFMS has
been used in a number of recent field studies in urban areas of Europe
(Dall'Osto and Harrison, 2012; Healy et al., 2013) to
identify and characterize particles from a diverse range of anthropogenic
sources including traffic, solid fuel burning, industry, soil and road dust,
marine aerosol, and secondary aerosol formation processes. However, it is
worthy of mention that ATOFMS source apportionment capabilities are limited
by the difficulties in quantification of its outputs (Reilly et al., 2000;
Schoolcraft et al., 2001). Nevertheless, single-particle analysis is an important
analytical tool that allows us to determine how the myriad chemical
constituents are distributed between individual particles (mixing state;
Pratt and Prather, 2012). The ATOFMS has often reported a number of particle
types, which at times are difficult to associate with a specific aerosol
source (Pastor et al., 2003; Dall'Osto and Harrison, 2006,
2012).</p>
      <p>The objective of the present manuscript is to report a detailed analysis of
the ATOFMS particle types detected during a field measurement campaign
carried out in Barcelona, Spain, as part of the SAPUSS (Solving Aerosol
Problems by Using Synergistic Strategies) project. The ATOFMS cannot provide
quantitative aerosol mass loading concentrations, but its strength relies in
the fact that it can monitor in real-time variations in the single-particle
composition. In other words, small variations in the particle mixing state
results in a single-particle mass spectra. As a result, a number of
atmospheric processes and aerosol sources can be monitored in real time. In
this paper we discuss not only information on the mass spectra but also
diurnal trends persisting over 4 weeks. Further information on the
intensive field campaign can be found in the overview paper by
Dall'Osto et al. (2013a). Two different ATOFMS instruments
were deployed during the 4-week measurement period – one at a roadside
(RS) site and the other at an urban background (UB) site. This is the first
time an ATOFMS has been deployed in Spain and, to the best of our knowledge,
it is also the first time (worldwide) that two ATOFMS instruments have been
deployed simultaneously in the same field campaign. The similarities and
differences in particle types detected at both sites is described in detail
and attributed to a range of local and regional sources as well as to
different chemical and physical processes.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <title>Location</title>
      <p>The SAPUSS field measurement campaign involved a large variety of
instrumentation deployed simultaneously at a number of monitoring sites in
Barcelona (Spain), between 17 September and 18 October 2010
(local time, UTC <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula> 2) (Dall'Osto et al., 2013a). ATOFMS
measurements were made at the two main SAPUSS supersites.</p>
      <p>RS site was situated in a car park next to a major road (Carrer
Urgell). The road, which crosses the city from south-east to north-west, is
a street canyon composed of a two-way cycling path and a one-way four lane
vehicle road. Vehicle intensity for the month of measurements was about
17 000 vehicles per day.</p>
      <p>UB site was situated in a small park at the north-western
periphery of the city centre. A main road (Avenida Diagonal, 127 000 vehicles day<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) is located about 500 m away from the site.</p>
      <p>The two sites were about 2 km from each other (Dall'Osto et al., 2013a).
While the UB site was open to wind from all directions, the wind flow and
turbulence at the RS site were partially affected by the nearby street
canyons and vehicular traffic. Previous reports from the SAPUSS campaign,
based on measurements of organic and elemental components of the aerosol,
indicate that the particle composition and thus sources are similar at both
sites (Dall'Osto et al., 2013b; Alier et al., 2013).
Specifically, six organic aerosol (OA) components were identified at both
sites: two of primary anthropogenic origin, three of secondary origin, and
one whose source was not clearly defined (Alier et al., 2013). Elemental
analysis provided by particle-induced X-ray emission (PIXE) enabled
identification of nine different aerosol sources at both sites: three of
regional origin, three types of dust aerosols, and three types of industrial
aerosols (Dall'Osto et al., 2013b).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Instrumentation</title>
      <p>The mass spectrometers were housed in air-conditioned trailers at both
sites. Sampling was performed ca. 4 m above ground using a quarter-inch
internal diameter stainless steel tube fitted with a PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula> cyclone. The
sample air was dried (through a Nafion dryer, Perma-Pure, length 100 cm,
relative humidity <inline-formula><mml:math display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 40 %) before arriving at the instruments. The two ATOFMS
instruments used in this study had different configurations. The instrument
deployed at the RS site was an ATOFMS TSI model 3800-100, in which particles
are sampled through an orifice and accelerated through an aerodynamic lens
to the sizing region of the instrument (Su et al., 2004). By contrast, the
instrument at the UB site was an ATOFMS TSI model 3800 that utilized a
converging nozzle inlet (Gard et al., 1997). Both instruments provide the
aerodynamic diameter of particles sizes between about 100 nm and 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m
by calculating their time of flight between two orthogonally positioned
continuous wave lasers (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn>532</mml:mn></mml:mrow></mml:math></inline-formula> nm). However, the transmission
efficiencies of the two instruments are quite different. While the
aerodynamic lens affords a much higher transmission efficiency for particles
with diameters less than about 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, its performance for larger
particles is not as good as the converging nozzle inlet. Following the
sampling and sizing, particles are transferred to the mass spectrometry
region where a pulsed laser (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">λ</mml:mi><mml:mo>=</mml:mo><mml:mn>266</mml:mn></mml:mrow></mml:math></inline-formula> nm, about 1 mJ pulse<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
desorbs and ionizes material within the particle in the centre of the ion
source of a bipolar reflectron time-of-flight mass spectrometry. Thus, positive and negative ion mass
spectra of a single particle are obtained. Overall, during the SAPUSS field
study the ATOFMS was operating for 68 and 97 % of the time at the UB
and at the RS site, respectively. It is also worth noting that an intercomparison of the two instruments was attempted at the same site, but this
could not be completed due to complex logistical and technical factors.</p>
      <p>The two different inlet configurations (aerodynamic lens and nozzle skimmer)
strongly affect the size distributions of the detected particles and the
overall aerosol population (Gard et al., 1997; Su et al., 2004). Hence, only
a qualitative description of the detected particles is presented in this
study. Furthermore, the ATOFMS mass spectrum is qualitative in that the
intensities of the mass spectral peaks are not directly proportional to the
component mass but are dependent on the particle matrix, the coupling
between the laser and the particle, as well as the shot-to-shot variability
of the laser (Dall'Osto and Harrison, 2012). Recent studies
(Jeong et al., 2011) report excellent correlations for inorganic species
(sulfate, nitrate, and ammonium) but weaker ones between total organic and
elemental carbon (EC) detected with ATOFMS and other instruments (Jeong et al.,
2011). However, the ATOFMS can provide quantitative information on particle
number as a function of composition, providing a measure of all particle
components, and can be used to assess mixing state.</p>
      <p>The ATOFMS datasets were imported individually into YAADA (Yet Another
ATOFMS Data Analyzer) and single-particle mass spectra were grouped with
adaptive resonance theory neural network, ART-2a (Song et al., 1999). The
parameters used for ART-2a in this study were learning rate 0.05, vigilance
factor 0.85, and 20 iterations. Further details of the parameters can be
found elsewhere (Dall'Osto and Harrison 2006; Rebotier and Prather 2007).
An ART-2a area matrix (AM) of a particle cluster represents the average
intensity for each <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> for all particles within a group. An ART-2a AM
therefore reflects the typical mass spectra of the particles within a group.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Meteorological parameters and air mass back-trajectory analysis</title>
      <p>The study area is affected by a convergence of air masses with different
characteristics: the cold air coming down from medium and high latitudes
and the warm air coming up from tropical and subtropical latitudes
(Dall'Osto et al., 2013a). Five air mass meteorological
regimes were classified during the SAPUSS field study, following the
procedure described in Dall'Osto et al. (2013b): Atlantic (ATL),
European-Mediterranean (EUR), North African east (NAF_E),
North African west (NAF_W), and Regional (REG). Furthermore,
meteorological variables (atmospheric pressure, wind speed, wind
direction, solar radiation, temperature, and relative humidity)
were also recorded at UB and RS SAPUSS monitoring sites during the whole
field study. For further details, the reader is referred to the SAPUSS
overview paper (Dall'Osto et al., 2013a).</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>ATOFMS particle clusters identified from the SAPUSS campaign.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.97}[.97]?><oasis:tgroup cols="8">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1">Monitoring</oasis:entry>  
         <oasis:entry colname="col2">Particle</oasis:entry>  
         <oasis:entry colname="col3">Particle</oasis:entry>  
         <oasis:entry colname="col4">%</oasis:entry>  
         <oasis:entry colname="col5">Monitoring</oasis:entry>  
         <oasis:entry colname="col6">Particle</oasis:entry>  
         <oasis:entry colname="col7">Particle</oasis:entry>  
         <oasis:entry colname="col8">%</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">RS site</oasis:entry>  
         <oasis:entry colname="col2">type</oasis:entry>  
         <oasis:entry colname="col3">number</oasis:entry>  
         <oasis:entry colname="col4"/>  
         <oasis:entry colname="col5">UB site</oasis:entry>  
         <oasis:entry colname="col6">type</oasis:entry>  
         <oasis:entry colname="col7">number</oasis:entry>  
         <oasis:entry colname="col8"/>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Local and regional EC</oasis:entry>  
         <oasis:entry colname="col2">EC_Aged_L</oasis:entry>  
         <oasis:entry colname="col3">277 151</oasis:entry>  
         <oasis:entry colname="col4">31.1</oasis:entry>  
         <oasis:entry colname="col5">Local and regional EC</oasis:entry>  
         <oasis:entry colname="col6">EC_Aged_L</oasis:entry>  
         <oasis:entry colname="col7">52 074</oasis:entry>  
         <oasis:entry colname="col8">23.8</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">EC_Aged_R</oasis:entry>  
         <oasis:entry colname="col3">202 227</oasis:entry>  
         <oasis:entry colname="col4">22.7</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">EC_Aged_R</oasis:entry>  
         <oasis:entry colname="col7">76 678</oasis:entry>  
         <oasis:entry colname="col8">35.1</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Secondary inorganic</oasis:entry>  
         <oasis:entry colname="col2">LRT-NIT</oasis:entry>  
         <oasis:entry colname="col3">102 909</oasis:entry>  
         <oasis:entry colname="col4">11.6</oasis:entry>  
         <oasis:entry colname="col5">Secondary inorganic</oasis:entry>  
         <oasis:entry colname="col6">LRT-NIT</oasis:entry>  
         <oasis:entry colname="col7">9982</oasis:entry>  
         <oasis:entry colname="col8">4.6</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Loc-NIT</oasis:entry>  
         <oasis:entry colname="col3">37 790</oasis:entry>  
         <oasis:entry colname="col4">4.2</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">Loc-NIT</oasis:entry>  
         <oasis:entry colname="col7">15 931</oasis:entry>  
         <oasis:entry colname="col8">7.3</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">LRT-SUL</oasis:entry>  
         <oasis:entry colname="col3">52 420</oasis:entry>  
         <oasis:entry colname="col4">5.9</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">LRT-SUL</oasis:entry>  
         <oasis:entry colname="col7">6635</oasis:entry>  
         <oasis:entry colname="col8">3.0</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Sea salt</oasis:entry>  
         <oasis:entry colname="col2">NaCl-NIT</oasis:entry>  
         <oasis:entry colname="col3">75 204</oasis:entry>  
         <oasis:entry colname="col4">8.4</oasis:entry>  
         <oasis:entry colname="col5">Sea salt</oasis:entry>  
         <oasis:entry colname="col6">NaCl-NIT</oasis:entry>  
         <oasis:entry colname="col7">8166</oasis:entry>  
         <oasis:entry colname="col8">3.7</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">NaCl</oasis:entry>  
         <oasis:entry colname="col3">8926</oasis:entry>  
         <oasis:entry colname="col4">1.0</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">NaCl</oasis:entry>  
         <oasis:entry colname="col7">31,853</oasis:entry>  
         <oasis:entry colname="col8">14.6</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Industry</oasis:entry>  
         <oasis:entry colname="col2">Fe</oasis:entry>  
         <oasis:entry colname="col3">7201</oasis:entry>  
         <oasis:entry colname="col4">0.8</oasis:entry>  
         <oasis:entry colname="col5">Industry</oasis:entry>  
         <oasis:entry colname="col6">Fe</oasis:entry>  
         <oasis:entry colname="col7">5564</oasis:entry>  
         <oasis:entry colname="col8">2.5</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Pb</oasis:entry>  
         <oasis:entry colname="col3">577</oasis:entry>  
         <oasis:entry colname="col4">0.1</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">Pb</oasis:entry>  
         <oasis:entry colname="col7">382</oasis:entry>  
         <oasis:entry colname="col8">0.2</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Combustion</oasis:entry>  
         <oasis:entry colname="col2">K-CN</oasis:entry>  
         <oasis:entry colname="col3">21 515</oasis:entry>  
         <oasis:entry colname="col4">2.4</oasis:entry>  
         <oasis:entry colname="col5">Combustion</oasis:entry>  
         <oasis:entry colname="col6">K-CN</oasis:entry>  
         <oasis:entry colname="col7">2778</oasis:entry>  
         <oasis:entry colname="col8">1.3</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Monitoring RS site</oasis:entry>  
         <oasis:entry colname="col2">Particle type</oasis:entry>  
         <oasis:entry colname="col3">Particle number</oasis:entry>  
         <oasis:entry colname="col4">%</oasis:entry>  
         <oasis:entry colname="col5">Monitoring UB site</oasis:entry>  
         <oasis:entry colname="col6">Particle type</oasis:entry>  
         <oasis:entry colname="col7">Particle number</oasis:entry>  
         <oasis:entry colname="col8">%</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">RS particles</oasis:entry>  
         <oasis:entry colname="col2">Amine (POA 58)</oasis:entry>  
         <oasis:entry colname="col3">6698</oasis:entry>  
         <oasis:entry colname="col4">0.8</oasis:entry>  
         <oasis:entry colname="col5">UB particles</oasis:entry>  
         <oasis:entry colname="col6">Soil-Saharan</oasis:entry>  
         <oasis:entry colname="col7">2842</oasis:entry>  
         <oasis:entry colname="col8">1.3</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Amine (SOA 114)</oasis:entry>  
         <oasis:entry colname="col3">3672</oasis:entry>  
         <oasis:entry colname="col4">0.4</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">Soil-Ca</oasis:entry>  
         <oasis:entry colname="col7">2482</oasis:entry>  
         <oasis:entry colname="col8">0.9</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Amine (SOA 59)</oasis:entry>  
         <oasis:entry colname="col3">2141</oasis:entry>  
         <oasis:entry colname="col4">0.2</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">Oil-V</oasis:entry>  
         <oasis:entry colname="col7">1875</oasis:entry>  
         <oasis:entry colname="col8">0.9</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Amine (EST 84)</oasis:entry>  
         <oasis:entry colname="col3">4888</oasis:entry>  
         <oasis:entry colname="col4">0.5</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6">Veg-KP</oasis:entry>  
         <oasis:entry colname="col7">3897</oasis:entry>  
         <oasis:entry colname="col8">1.7</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Org. (Lub Oil)</oasis:entry>  
         <oasis:entry colname="col3">16 273</oasis:entry>  
         <oasis:entry colname="col4">1.8</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Org. (OC-CHO)</oasis:entry>  
         <oasis:entry colname="col3">42 680</oasis:entry>  
         <oasis:entry colname="col4">4.8</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Org. (Aro-NIT)</oasis:entry>  
         <oasis:entry colname="col3">15 306</oasis:entry>  
         <oasis:entry colname="col4">1.7</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">Org. (OC-NIT)</oasis:entry>  
         <oasis:entry colname="col3">13 295</oasis:entry>  
         <oasis:entry colname="col4">1.5</oasis:entry>  
         <oasis:entry colname="col5"/>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Total RS</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3">890 873</oasis:entry>  
         <oasis:entry colname="col4">100</oasis:entry>  
         <oasis:entry colname="col5">Total UB</oasis:entry>  
         <oasis:entry colname="col6"/>  
         <oasis:entry colname="col7">221 139</oasis:entry>  
         <oasis:entry colname="col8">100</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
<sec id="Ch1.S3.SS1">
  <title>ATOFMS particle detection efficiency</title>
      <p>Overall, 890 873 particle mass spectra were apportioned at the RS and
221 139 at the UB. This large difference in detected particle numbers is
likely a result of the combined effects of the location and detection
efficiencies of both instruments. As shown in Fig. 1, the number and size
distribution of the particles detected by the two mass spectrometers is
quite different and reflects their expected performance characteristics
(Gard et al., 1997; Su et al., 2004). The instrument with the aerodynamic
lens detected considerably more particles below 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, while particles
larger than ca. 1.9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m were only detected with the converging nozzle
inlet. By running ART-2a, more than 300 clusters were found initially in
both UB and RS datasets. Many were merged when they presented similar temporal
trends, size distributions, and mass spectra (Dall'Osto and
Harrison, 2006). By merging similar clusters, the total number of particle
types describing the whole dataset was reduced to 18 and 14 at the RS and UB
sites, respectively. Despite the different inlet configurations and sampling
locations, the majority of the particles detected at both sites could be
described by 10 common ATOFMS particle types, listed in Table 1. A number of
other particle types were found only at one of the monitoring sites (eight at
the RS site and four at the UB site), likely due to the different urban
environments as well as the different detection efficiency of the two
instruments (Table 1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Size distributions of collected ATOFMS particles at the two SAPUSS
monitoring sites.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f01.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p>Average mass spectra of the 10 single-particle types observed at
both the RS and UB sites.</p></caption>
          <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f02.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S3.SS2">
  <title>ATOFMS particle types observed at both sites</title>
<sec id="Ch1.S3.SS2.SSS1">
  <title>Elemental carbon</title>
      <p>Two main EC particle types, representing together more than 50 % of
detected particles (58.9 % at the UB, 53.8 % at the RS), were
identified at both sites. For reasons outlined below, they are named
EC_Aged_R (regional) and EC_Aged_L (local). Both EC particle
types presented a fine aerosol size distribution mode at both sites (about
300–500 nm; see Fig. S2 in the Supplement). Figure 2a shows the positive
mass spectrum of particle type EC_Aged_R. It is dominated by EC peaks
at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 12 [C]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 36 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 48 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and 60
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>. Cluster EC_Aged_L (see Fig. 2b) also shows a similar
EC positive mass spectrum pattern, although a strong signal at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39
dominates the positive mass spectrum. This peak is often associated with
potassium [K]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, although there may also be a contribution from the
organic ion [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> (Dall'Osto et al., 2009). The EC signals
present in the positive mass spectra, and the near-total absence of peaks in
the negative mass spectra suggests these EC particles are not freshly
emitted. Indeed, Giorio et al. (2012) reported for a regional background site
that strong EC peaks in the negative ion mass spectrum are more indicative of
fresh emissions while strong EC peaks in the positive mode represent aged
EC. This is consistent with observations which indicate that
particle composition affects the ionization and fragmentation pattern of EC
(Reinard and Johnson, 2008). The two EC-rich particle types were mainly
detected in stagnant air masses. As shown in Fig. S1a, an enhancement of
these particle types was observed during sulfate-rich air masses
(7–10 October 2010) and nitrate-rich stagnant regional air masses
(13–17 October 2010), as described in Dall'Osto et al. (2013a). The diurnal
profiles of these two aged EC particle types (Fig. 3a) can also help to
classify their origin. Whilst EC_Aged_R shows little diurnal variation,
particle type EC_Aged_L shows a gradual increase during the day, peaks
in the afternoon (15:00 local time, LT), and drops to a minimum during night-time. The
absence of sharp morning peaks indicates that these EC particle types are not
associated with primary emission from local traffic. Similarly, the absence
of a sharp evening peak also excludes the association with biomass burning,
which is not expected at this time of the year and is generally not important
in Barcelona (Dall'Osto et al., 2013a). Whilst the flat diurnal trend of
EC_Aged_R is typical of regional aerosol, particle type EC_Aged_L
suggests a local influence or an enhancement during the warmer part of the
day. This assignment is also supported by the observed correlation of the EC
types with some secondary inorganic particle types associated with local and
regional aerosol sources, described in the next section. Similar conclusions
were recently reported by Decesari et al. (2014), where most of the aged EC
particles detected with the ATOFMS were related to aged anthropogenic
aerosols accumulating in the lower layers of the Po Valley (Italy) overnight.
Overall, we did not find major differences in the diurnal profiles of similar
particle types detected simultaneously at the UB site and RS site. In other
words, there were not major differences that could have been affected by wind
speed and direction considering that the RS site is close to a large street
canyon (Dall'Osto et al., 2013a).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Diurnal profiles of the common particle types detected at both the
RS and UB sites. Differences between RS and UB sites were minor and average
diurnal profiles are presented.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f03.pdf"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS2.SSS2">
  <title>Secondary nitrate and sulfate</title>
      <p>The application of the ART-2a neural network algorithm to the ATOFMS data
apportioned two main distinct nitrate particle types, already previously
reported (Dall'Osto et al., 2009; Harrison et al., 2012; Decesari et al.,
2014). The first (local nitrate (Loc-NIT); 4.2–7.3 % of particles by
number) appears to be locally produced in urban locations during night-time,
whilst the second (long-range transport – nitrate (LRT-NIT); 4.2–7.3 %
of particles by number) is regionally transported within the Iberian
Peninsula and the rest of Europe. Briefly, particle type Loc-NIT is
characteristic of nitrate aerosol in small particles (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mtext>a</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> at about
300–500 nm; Fig. S2). The average mass spectrum (Fig. 2c) shows a peak at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39 that can be due to potassium, although previous studies (Dall'Osto
et al., 2009) suggested that an organic contribution may be also present
depending on the <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39 <inline-formula><mml:math display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> 41 ratio. The ATOFMS nitrate particle type
appears to be associated with local formation processes and occurred in the
main at times outside of the long-range transport episode (Fig. S2b). By
contrast, a second nitrate particle type (LRT-NIT) is regionally transported.
The average mass spectrum (Fig. 2d) shows that nitrate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62) is
internally mixed with sulfate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>97), ammonium (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 18) and both
elemental (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 36, 48, 60) and organic carbon (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 37, 39, 43). As
explained in Decesari et al. (2014) these aerosols likely originate from the
night-time condensation of nitric acid on EC-containing primary particles
(e.g. Shiraiwa et al., 2007). The LRT-NIT particle type is volatile, and
partially evaporates during the day leaving a core of about 300 nm mainly
composed also of sulfate, elemental and organic carbon (Dall'Osto et al.,
2009). Indeed, this can be seen in the LRT-SUL (long-range transport –
sulfate) particle type, whose average mass spectrum for this (Fig. 2e) shows
peaks due to nitrate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62), sulfate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>97), elemental carbon
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>36, 48, 60), and organic carbon (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>39, 43). The LRT-SUL and
LRT-NIT diurnal trends are anti-correlated, as previously described elsewhere
(Dall'Osto et al., 2009; Decesari et al., 2014), with LRT-SUL concentrations
peaking in the afternoon hours. Such behaviour is attributed to the effect of
the diel cycle of nitric acid and ammonia condensation/evaporation on the
same particle type: during night-time this regional particle type is seen
with nitrate, which evaporates during daytime, leaving a smaller aerosol core
composed of EC and sulfate (Decesari et al., 2014). These two particle types
were more abundant at the RS site, likely because of the improved focussing
of smaller particles provided by the aerodynamic lens inlet. However, this
study shows a novel aspect not found in the London local–regional nitrate
study (Dall'Osto et al., 2009) or in the Po Valley (Decesari et al., 2014).
During the period 12–14 October, under rainy conditions and with air masses
arriving from Europe (Dall'Osto et al., 2013a), the transport of LRT-SUL was
detected without the nitrate component (LRT-NIT, Fig. S1b). This could be due
to a different source of LRT-SUL not linked with LRT-NIT and previously
unobserved.</p>
</sec>
<sec id="Ch1.S3.SS2.SSS3">
  <title>Potassium organonitrogen (K-CN) particles</title>
      <p>The K-CN particle type was a minor one, representing only 1.3–2.4 % of
the total particles analysed. Figure 2f shows the average mass spectrum,
which features a strong peak at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39 [K]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>in the positive mode, as
well as peaks at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 113 [K<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>Cl]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 [Cl]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>,
suggesting a biomass-burning source (Pastor et al., 2003; Dall'Osto and
Harrison, 2006). K-rich particles similar to K-CN have previously been
attributed to biomass burning (Silva et al., 1999; Guazzotti et al., 2003)
and were found to correlate with gas-phase measurements of acetonitrile, a
good biomass-burning tracer. The negative ion mass spectrum shows strong
peaks at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> 26 [CN]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>42 [CNO]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, indicating
that the potassium and chloride are internally mixed with organonitrogen
species. The size distribution, centred at about 350 nm (Fig. S2), also
points to a combustion source. Overall, this particle type represented only
about 2 % of the total particles sampled (Table 1) and its temporal
variation is presented in Fig. S2d. Its diurnal trend (Fig. 3) tracks the
anthropogenic activities of the city of Barcelona, suggesting general minor
urban combustion processes. It should be noted that biogenic plant debris
also has a similar single-particle mass spectrum, with strong signals at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>26, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>42 (Silva and Prather, 2000). However, vegetative dust is
usually internally mixed with sodium and phosphate and presents aerodynamic
diameters above 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m (see Sect. 3.3).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS4">
  <title>Fresh and aged sea salt particles</title>
      <p>Two sea salt particle types (fresh and aged) were detected at both sites,
accounting for 9.4 and 18.3 % of the total particles sampled at RS and
UB, respectively (Table 1). The higher percentage detected at the UB is
likely due to the instrument configuration given that the nozzle inlet
enables more efficient detection of coarser particles. The average mass
spectrum (Fig. 2g) for the particle type assigned to fresh sea salt (labelled
NaCl) shows peaks typical of sodium chloride clusters ([Na]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23), [K]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39), [Na<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 46),
[Na<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>Cl]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 81 and 83), [NaCl<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 93, 95 and
97)), whilst aged sea salt (NaCl-NIT, Fig. 2h) also exhibited nitrate peaks
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62) reflecting the reaction between NaCl and HNO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
and the replacement of chloride by nitrate (Gard et al., 1998). Both particle
types had mean size distributions above 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m (Fig. S2c). NaCl was
mainly detected during air masses that had travelled over Mediterranean
regions (7–10 and 11–13 October), as shown in Fig. S2e. Interestingly, the
diurnal variation of the two NaCl particle types is quite different (Fig. 3).
Whilst NaCl-NIT does not show a clear trend, NaCl shows an enhancement in the afternoon, associated with the sea
breeze, peaking at 15:00 (Dall'Osto et
al., 2013c).</p>
</sec>
<sec id="Ch1.S3.SS2.SSS5">
  <title>Iron- and lead-containing particles</title>
      <p>Two common ATOFMS particle types have average mass spectra that were
dominated by metals. The first was rich in iron (type Fe, 1.4 % of the
total particles) and has a spectrum (Fig. 2i) characterized by a strong
signal at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 56 and weaker features at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 73 (iron oxide,
[FeOH]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 54 (isotope [<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>54</mml:mn></mml:msup></mml:math></inline-formula>Fe]). The negative
spectrum has strong features at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62, indicating that the
iron is internally mixed with nitrate. During SAPUSS, the Fe particle type
was found to correlate (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.75) with LRT-NIT, which is associated
with long-range transport of pollutants. The small mode of the Fe particle
type (Fig. S2) reflects the fact that only fine particles were likely to
travel long distances relative to the coarser ones which were lost during
transport. This is in line with previous ATOFMS field studies showing the
transport of iron-containing particles internally mixed with nitrate from
continental Europe (Harrison et al., 2012). The flat diurnal profile for the
Fe particle type (Fig. 3) also suggests a regional origin. The long-range
transport of fine Fe-containing particles (internally mixed with nitrate) is
discussed further elsewhere (Dall'Osto et al., 2016).</p>
      <p>The average mass spectrum of the second metal-rich particle type is shown in
Fig. 2j. This particle type is labelled Pb since lead is one of the largest
contributors in the positive mode, occurring at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>206, 207, and 208.
Other peaks in the positive ion spectrum include <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23 [Na]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>,
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 56 [Fe]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39 and 113 ([K]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and [K<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>Cl]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mo>+</mml:mo></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.
In addition to nitrate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46 [NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>] and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62
[NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, chloride (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>35 ([Cl]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was one of the most abundant species in the negative
ion mode. Further information can be found in Dall'Osto et al. (2013b), where
this ATOFMS particle type was found highly correlated with hourly elemental
concentrations determined by PIXE analysis (Dall'Osto et al., 2013b), showing
that this source of lead and
chloride (Pb–Cl) is a major (82 %) source of fine Cl in the
urban agglomerate of Barcelona. A similar particle type containing Pb–Cl was detected by ATOFMS in Mexico City and attributed to a
waste incinerator source (Moffet et al., 2008), although other studies in the
same area attributed lead-containing particles to multiple sources, including
trash burning (Salcedo et al., 2010; Hodzic et al., 2012). It is worth noting
that whilst the regional particle type Fe was mainly distributed in the fine
mode (about 300–500 nm), a much larger mode (about 700–900 nm) was
observed for this local ATOFMS Pb particle type (see Fig. S2d). Finally, the
temporal trend (Fig. S1d) and the diurnal profile (Fig. 3) of the Pb particle
type also suggests a local origin, likely related to emissions from urban
combustion.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Average mass spectra of the four single-particle types only observed
at the UB site.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f04.pdf"/>

          </fig>

</sec>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Particle types observed at UB</title>
      <p>The ATOFMS fitted with converging nozzle inlet located at the UB site
detected four particle types that were not observed at the RS site. Each of
the particle types make a minor contribution (0.9–1.7 %) and overall
they represented less than 5 % of the total particles sampled at the UB
site.</p>
<sec id="Ch1.S3.SS3.SSS1">
  <title>Vanadium (V)-containing particles</title>
      <p>A particle type containing vanadium (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 51 [V]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 67
[VO]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> Na (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23) and Fe (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 56), along with minor peaks due to
EC at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 36, 48, and 60, was observed at the UB site. A negative ion mass
spectrum was not acquired for this particle type (Fig. 4a). It has been shown
that the condensation of secondary material on soot particles (Moffet and
Prather, 2009) and the consequent change in aerosol hygroscopicity (Spencer
et al., 2006) can suppress the formation of negative ions in real-time laser
desorption/ionization mass spectrometry, causing many aged EC-containing
particles to lack negative mass spectra (Neubauer et al., 1998). The V
particle type accounted for only 1 % of the particles characterized at
the UB, with a unimodal distribution peaking at about 350 nm pointing to a
fresh combustion emission source. Field observations have confirmed that
ships produce significant amounts of soot, vanadium, nickel, and sulfate
(Pattanaik et al., 2007). Previous ATOFMS field measurements also reported
that single particles containing organic carbon, vanadium, and sulfate
(OC-V-sulfate) resulted from residual fuel combustion (i.e. bunker fuel),
whereas high quantities of fresh soot particles represented distinct markers
for plumes from distillate fuel combustion (i.e. diesel fuel) from ships as
well as trucks in the port area (Healy et al., 2009; Ault et al., 2010).
Indeed, the V particle type presented a temporal variation showing a maximum
on 3 October 2010, when strong wind was blowing from the port of Barcelona
(North African tropical air masses from the west (NAF_W); Fig. S1e). This
Vanadium particle type is therefore most likely associated with fuel oil and
ship emissions from the port. However, it was not detected at the RS site,
possibly due to local street canyon effects which restrict transport and
mixing in the area (Solazzo et al., 2008).</p>
</sec>
<sec id="Ch1.S3.SS3.SSS2">
  <title>Soil rich in Ca (Soil-Ca)</title>
      <p>The average ATOFMS mass spectrum of a dust particle type rich in calcium is
shown in Fig. 4b, where peaks for calcium (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 40 [Ca]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 56
[CaO]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 57 [CaOH]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and 96 [Ca<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are present. Peaks
associated with sodium (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23), magnesium (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 24, 25), and potassium
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39) can also be seen. The Soil-Ca particle class represented
0.9 % of the particles sampled at the UB site and was found to moderately
correlate (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.6</mml:mn></mml:mrow></mml:math></inline-formula>) with the urban dust (Ca) factor obtained by PIXE-PMF
analysis (Dall'Osto et al., 2013b). The large aerosol size mode above
1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m (Fig. S1e) also points to a dust origin. Enhanced levels of the
Ca ATOFMS particle type were observed during ATL air masses
(Dall'Osto et al., 2013a), likely due to extra resuspension of dust caused by
the high wind speeds during these periods. Urban areas in the south of Europe
are known to have high dust loadings and three different types of dust were
previously reported in the SAPUSS PIXE study (Dall'Osto et al., 2013b),
representing ca. 25 % of the PM<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>2.5</mml:mn></mml:msub></mml:math></inline-formula> mass concentrations measured. It
should be noted that this particle type did not possess a negative ion mass
spectrum and was also not detected at the RS site, likely for the same
reasons explained above (Sect. 3.3.1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><caption><p>Average mass spectra of the four amine-containing single-particle
types only observed at the RS site.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f05.pdf"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS3.SSS3">
  <title>Saharan dust particles (Saharan-dust)</title>
      <p>A rarely observed particle type with peaks due to titanium at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 48 and
64 ([Ti]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and [TiO]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, respectively) was found to represent
0.9 % of the particles sampled at the UB site (Fig. 4c). Additional peaks
are associated with other metals including Na (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23), Al (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 27), Ca
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 40, 56, 96), and Fe (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 56), as well as minor peaks of silicate at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60 [SiO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>76 [SiO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>. These particles
presented an aerosol size coarse mode (1–3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m; Fig. S2) and were
detected mainly during the period 8–10 October, when Barcelona experienced
air masses originating in the North African Saharan region (Dall'Osto et al.,
2013a). It is likely that the Art-2a algorithm did not apportion this minor
particle type of regional origin in the RS site. With regard to secondary
species, it is interesting to note that the dust was internally mixed only
with nitrate and not with sulfate (Fig. 4c). Previous studies (Dall'Osto et
al., 2010) showed that Saharan dust particles collected near the Cape Verde
Islands contained internally mixed nitrate but no sulfate, whilst Saharan
dust particles collected on the coast of Ireland showed a very high degree of
internally mixed secondary species including nitrate, sulfate, and
methanesulfonate (Dall'Osto et al., 2004).</p>
</sec>
<sec id="Ch1.S3.SS3.SSS4">
  <title>Vegetative debris (Veg-KP)</title>
      <p>The ATOFMS has already proven to be a good tool for identifying and
separating dust (mainly Ca-rich or Al-Si-rich) and biological particles
(Fergenson et al., 2004). A particle type dominated by K (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39) and
phosphate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>63 and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>79) in the average mass spectrum (Fig. 4d)
accounted for 1.7 % of the total particles sampled at the UB site. Strong
signals at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 26 and 42, due to [CN]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and [CNO]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, are also
present, as well as peaks due to Na (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23) and Fe (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 56). A coarse
aerosol size mode of about 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m (Fig. S2) is likely again the
reason why this particle type was not detected by the ATOFMS at the RS site.
The size and chemical composition suggest a source such as vegetative debris
and the particle type is thus labelled Veg K-P. A previous ATOFMS study
reported a very similar particle type from samples of leaves collected from a
roadside (Schofield, 2004). It is interesting to note that an increase of
this vegetative debris particle type was detected under NAF_W air masses
in concomitance with Saharan dust particles. Previous atmospheric
measurements have shown that the concentration of bacteria over the sea may
be much lower than over land but that higher concentrations of aerosolized
microorganisms are generated during dust events compared to clean background
marine conditions (Kellog and Griffin, 2006; Prospero et al., 2005).</p>
</sec>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Particle types observed at RS</title>
      <p>The ATOFMS fitted with an aerodynamic focussing lens located at the RS site
detected eight particle types that were not observed at the UB site.</p>
<sec id="Ch1.S3.SS4.SSS1">
  <title>Amines</title>
      <p>Amines are ubiquitous in the atmospheric environment and have been detected
in marine, urban, and rural atmosphere in the gas and particle phases as well
as aqueous fog and rain water (Ge et al., 2011). The ATOFMS is a particularly
good aerosol instrument for studying amines because the LDI laser wavelength
(266 nm) ionizes them very efficiently (Angelino et al., 2001; Healy et al.,
2015). During the SAPUSS measurement campaign, four amine particle types were
detected at the RS. To the best of our knowledge, this is the first time such
a variety of organonitrogen particle types has been detected at the single-particle level in real time in urban air.
<list list-type="custom"><list-item><label>a.</label><p><italic>Amine (POA 58</italic>): Fig. 5a shows the ATOFMS mass spectra of a
particle type called amine-58, which accounted for 0.8 % of the total
particles classified at RS. The strongest peak in the positive mass spectra
at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 58 is likely due to [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>NH <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>. In
general, the most important primary fragmentation process occurring for
aliphatic amines involves the removal of one of the electrons from the lone
pair on N and cleavage of the C–C bond to the nitrogen, with loss of the
heavier alkyl group favoured. This cleavage explains the presence of the
fragments at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 58 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>NH <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 72
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>NH <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 86
[(C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>N <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and 114
[(C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>N <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>. The minor peak at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 86 was
found to correlate (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn>0.8</mml:mn></mml:mrow></mml:math></inline-formula>) with <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 58. <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 86 was suggested as
amine species associated with fresh mobile emissions (Angelino et al., 2001).
The negative mass spectrum shows nitrate and sulfate internally mixed with
this particle type, although the former has a stronger signal than the
latter. A size distribution peaking at about 300–400 nm was associated with
this particle type. The diurnal variation of amine (POA 58) (Fig. 6a) shows
a peak about 1 h later than morning and evening rush hour traffic and
thus points to relatively fresh vehicular source. In conclusion, both the
mass spectra (similar to previous traffic emissions; Angelino et al., 2001)
and the temporal trend of this particle type point to traffic emission as a
main source.</p></list-item></list></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>Diurnal trend of amines <bold>(a)</bold> and organic-rich <bold>(b)</bold> particle types
detected at the RS site. Differences between RS and UB sites were minor
and average diurnal profiles are presented.</p></caption>
            <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f06.pdf"/>

          </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><caption><p>Average mass spectra of the four OC-rich single-particle types only
observed at the RS site.</p></caption>
            <?xmltex \igopts{width=369.885827pt}?><graphic xlink:href="https://acp.copernicus.org/articles/16/9693/2016/acp-16-9693-2016-f07.pdf"/>

          </fig>

      <p><list list-type="custom">
              <list-item><label>b.</label>

                <p><italic>Amine (ETS 84)</italic>: Fig. 5b shows the average mass spectrum of a
particle type associated with environment tobacco smoke (ETS) called
amine-84, which represented 0.5 % of the total particles classified at
RS. In the positive mass spectrum, the peak at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 161 is assigned to
nicotine, with the main fragment being at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 84 (methyl-pyrrole
fragment). The negative mass spectrum shows nitrate and sulfate internally
mixed with this particle type. The amine-84 mass spectrum is very similar to
that previously reported in Athens (<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.9; Dall'Osto et al.,
2007) and also attributed to tobacco smoke. This particle type generally
followed human activity within the city (Fig. 6a), with a main peak in the
morning (10:00) and a broader one during the evening
(18:00–22:00 LT). It should be noted that an
afternoon peak – potentially related to lunch activities – was not noticed.
The ATOFMS cluster amine (ETS 84) attributed to tobacco smoke was compared to
the measured nicotine value described in Alier et al. (2013). Briefly, much
higher nicotine concentrations (58 ng m<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> were observed at the RS
site than at UB site (7 ng m<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. This 8-fold difference pointed to
a very high level of outdoor cigarette consumption near the RS site, which is
situated next to a busy street and an exit of an underground metro station
(Alier et al., 2013). Moreover, nicotine concentrations were more affected by
daytime working activities during weekdays rather than during the weekends.
ATOFMS cluster amine (ETS 84) was temporally correlated with nicotine
concentrations available at 12 h resolution, and an <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> of 0.65 was
found, confirming the tobacco smoke source suggested. Spain ranks among the
countries with the highest levels of cigarette consumption in the European
Union and in the World (WHO, 2004; Alier et al., 2013). High outdoor
gas-phase nicotine concentrations (0.5 and 1.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> have
been previously measured in Barcelona in summer 2010 (Sureda et al., 2012).</p>
              </list-item>
              <list-item><label>c.</label>

                <p><italic>Amine (SOA 59)</italic>: Fig. 5c shows the average mass spectrum of
a particle type called amine-59, which accounted for 0.2 % of the total
particles classified at RS. Based on previous studies, the strong peak at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 59 ([N(CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is attributed to trimethylamine (TMA)
(Angelino et al., 2001; Healy et al., 2015). Amine (SOA 59) concentration was
found particularly enhanced under regional air masses (13–17 October 2010,
Fig. S1h) and exhibited a diurnal trend (Fig. 6a) showing maximum
concentrations at 15:00 and 22:00. TMA plays an important role in atmospheric
chemistry, yet its pathway towards aerosol is not clear. Rehbein et
al. (2011) demonstrated that cloud/fog processing could enhance
gas-to-particle partitioning of TMA. TMA can also participate in the
formation of secondary organic aerosol. Several studies have shown that
gas-phase TMA could form non-salt organic aerosol products through reaction
with oxidizing agents (Murphy et al., 2007).</p>
              </list-item>
              <list-item><label>d.</label>

                <p><italic>Amine (SOA 114)</italic>: Fig. 5d shows the average mass spectrum for
a particle type called amine (SOA 114). The main peak is at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 114, which
may be assigned to dipropylamine or tripropylamine (Angelino et al., 2001;
Healy et al., 2015). Minor peaks can also be seen at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 58, 74, and 128,
which were previously attributed to alkyl ammonium nitrate salt particles
formed by reaction of nitric acid and amines (Angelino et al., 2001). The
negative ion mass spectrum for amine (SOA 114) shows a strong peak at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62, confirming the presence of nitrate. Figure 6a shows that the
diurnal profile is similar to that reported for amine (SOA 59), although with
a much stronger peak at 15:00, during the warmest part of the day for the
measurement period (Dall'Osto et al., 2013a). This is in line with recent
measurements of gaseous amines by ambient pressure proton transfer reaction mass
spectrometry (Hanson et al., 2011) which also showed an enhancement of TEA
(triethylamine) during the afternoon. Amine (SOA 59) and amine (SOA 114)
presented similar diurnal profiles but their temporal occurrence was not
similar. Whilst amine (SOA 59) was detected mainly during the period of
nitrate-rich regional air masses (13–17 October), amine (SOA 114) was
detected mainly under NAF_E air masses rich in sulfate
(7–10 October 2010). This observation is discussed further in Sect. 4.</p>
              </list-item>
            </list></p>
      <p>Overall, the four amine-containing particle types were found distributed
mainly in the sub-micron mode. Amine (POA 58) and amine (ETS 84), which are
attributed to primary emissions from traffic and ETS respectively, have
similar size distributions which peak around 400–500 nm (Fig. S2). Amine
(SOA 59) and amine (SOA 114) were also found in the same size range, but
presented a broader shape, suggesting partial condensation of SOA material on
existing particles. Previous work of Angelino et al. (2001) used the peak at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 118 to track a marker for the oxidation products of alkylamines
observed in the condensed phase of aerosol particles, specifically attributed
to the oxidation of triethylamine (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 118;
[(C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>NCH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. The analysis of the ATOFMS dataset
for the RS site shows that the majority (about 80 %) of amine particle
types containing a peak at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 118 were found in the tobacco-related ATOFMS
amine (ETS 84) class, whereas the remaining 20 % was associated with
amine (POA 58). This suggests – at least in our study – that <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 118
cannot be used as a marker for amines produced by secondary processes. Other
possible identification of higher mass ions detected and associated with
organic nitrate include <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 74 ([C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, 88
([C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> or (([C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>NO]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, 104
([C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, and
191([C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn>11</mml:mn></mml:msub></mml:math></inline-formula>N<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. Overall, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 104 was found to
be to be linked to  amine (POA 58), whereas <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 74 and 191 were related to amine (SOA 114).
Finally, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 88 was found associated with both amine (POA 58) and amine
(SOA 114). In summary, organic nitrate peaks were associated with both
primary and secondary amine particle types.</p>
</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <title>Organic carbon (OC) particle types</title>
      <p>The high efficiency of the ATOFMS equipped with the aerodynamic lens and
deployed at the RS allowed us to characterize four particle types rich in
organic compounds.
<list list-type="custom"><list-item><label>a.</label><p><italic>Org (Lub. Oil)</italic>: Fig. 7a shows the average mass spectrum of a
particle type named “Lub. Oil” (1.8 %). The positive ion mass spectrum
shows strong peaks for [Ca]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 40) and minor ones for OC
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 27, 43, 57) and EC (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 12, 24, 36, 48, 60). The negative mass
spectrum shows the presence of nitrate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62) and EC (<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>36,
<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>48, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>60). This particle type was only detected in the lower size range
of the ATOFMS (ca. 150–400 nm), was found to spike during traffic rush hour
times (Fig. 6b), and is attributed to lubricating oil from traffic emissions
(Spencer et al., 2006; Drewnick et al., 2008).</p></list-item><list-item><label>b.</label><p>Org. (<italic>Aro-NIT)</italic>: a particle type rich in aromatic compounds
and internally mixed with nitrate (Org. (Aro-NIT)) was found to account for
1.7 % of the particles classified at the RS. The average mass spectrum
shown in Fig. 7b features strong signals due to organic fragments at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 27, 29, 39, 43, 51, 57, and 63. <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 51 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 63
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 77 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and 91
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> are indicative of a strong aromatic signature
(McLafferty, 1993). Common peaks due to nitrate (i.e. <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46
[NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62 [NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are found in the negative
mass spectrum. Figure 6b shows a daily maximum of this particle type at about
19:00–20:00. Two previous ATOFMS studies in Athens (Dall'Osto and Harrison,
2006) and London (Dall'Osto and Harrison, 2012) reported very similar
particle types (called C-SEC_2 and Na-EC-OC, respectively), which were
attributed to condensation of organic compounds onto the particle phase as
air temperatures dropped. The secondary particles showed clear internal
mixing of organic and inorganic constituents. The size distribution of the
Aro-NIT particle type shows a broad mode at about 500–700 nm (Fig. S2),
also suggesting condensation of species on existing aerosols.</p></list-item><list-item><label>c.</label><p>Org. (<italic>OC-NIT)</italic>: A third organic-rich particle type, called
OC-NIT (1.5 % of the particles classified), was also detected at the RS
site. Figure 7c shows the average positive ion mass spectrum, which contains
a strong peak at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 39 (K and/or C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and minor peaks due to
OC and EC, as well as Na (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 23). Perhaps the most interesting part of the
negative spectrum for this particle type is the presence of signals due to
organic nitrogen species (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>26 [CN]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>42
[CNO]<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, not seen in other organic-rich particle types shown in Fig. 7.
Finally, strong peaks for nitrate (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>46, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>62) dominate the negative
mass spectra. Figure 6b shows a daily maximum concentration of OC-NIT at
15:00. The presence of an organonitrogen component in this particle type,
as well as its maximum at 15:00, is similar to that for the amine (SOA 59)
particle type described in the previous section.</p></list-item><list-item><label>d.</label><p>Org. (<italic>OC-CHO)</italic>: This particle type presents a positive mass
spectrum (Fig. 7d), with strong peaks at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 27 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 43 [(CH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>CO]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> usually associated with oxidized secondary
organic aerosol. Peaks at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 29
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 41 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> confirm the
strong hydrocarbon-like nature of the particles (Spencer et al., 2006), while
weak peaks at <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> 51 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 63 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, 77
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">6</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula>, and 91 [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>+</mml:mo></mml:msup></mml:math></inline-formula> also indicate an
aromatic contribution (McLafferty, 1993). A negative ion mass spectrum was
often not recorded for this particle type. However, some of the particles did
generate one and an example is shown in Fig. S3d. The presence of peaks at
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>m</mml:mi><mml:mo>/</mml:mo><mml:mi>z</mml:mi></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>45, <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>59, and <inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>71 are likely to be due to the formate
[CHO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, acetate [C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula>, and propionate
[C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>H<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>]<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>-</mml:mo></mml:msup></mml:math></inline-formula> ions, respectively. Figure 6b shows that in
contrast to the other three OC-rich particle types, OC-CHO shows a complex
diurnal profile. The number of counts per hour increases from 06:00 to 08:00 and
then remains stable for about 5 h. A peak is observed around 15:00, the
hottest part of the day, followed by a second peak at about 22:00–23:00. This
diurnal profile is similar to that of amine (SOA 114), which is also of
secondary origin. Cluster OC-CHO could also be associated with oxidation of
aromatics by the OH radical (Platt et al., 2013; Giorio et al., 2015).</p></list-item></list>
Overall these four OC-rich particle types indicate that a number of processes
and sources are likely producing oxidized organic aerosols. There are at
least four main peaks during the day: a morning traffic rush hour
(09:00–10:00), an afternoon one during the hottest part of the day (15:00),
and two evening ones at 20:00 (sunset) and at about 22:00–23:00. This is
likely to be governed by a combination of emissions from local sources during
rush hour periods, as well as by meteorological parameters such as
atmospheric wind speed, wind direction, relative humidity, and temperature.</p>
</sec>
</sec>
</sec>
<sec id="Ch1.S4" sec-type="conclusions">
  <title>Discussion and conclusions</title>
      <p>During the SAPUSS intensive field study two ATOFMS instruments were deployed
simultaneously. The ATOFMS deployed at the RS site was equipped with an
aerodynamic lens inlet system, allowing characterization of primary traffic
aerosols as well as other primary and secondary aerosols affecting this
heavily urbanized area of Barcelona. This type of ATOFMS (Su et al., 2004)
has a very high efficiency in sampling aerosols (more than 1 000 000 single-particle mass spectra were collected at the RS), particularly for sub-micron
particles in the size range 300–700 nm. The ATOFMS deployed at the UB site
was equipped with a converging nozzle inlet system (Gard et al., 1997), which
has a low aerosol collection efficiency (Dall'Osto et al., 2006), but it is
particularly well suited for sampling coarser aerosols in the size range
800–2000 nm.</p>
      <p>Overall, 10 particles types were detected at both sites (Table 1). Two of
these particle types, composed of EC internally mixed with secondary
inorganic species, described more than half of the classified single-particle
mass spectra. EC_aged_R was found accumulating within stagnant air
masses, with a flat diurnal profile and suggesting a certain physico-chemical
stability. In contrast, a more local but processed form of EC
(EC_aged_L) was found to possess a finer submicron mode and enhanced
concentrations during afternoon periods.</p>
      <p>Two different types of nitrate-dominated aerosols were observed, in line with
a previous ATOFMS study in London (Dall'Osto et al., 2009). The first
(LRT_NIT) was attributed to regional nitrate (accumulation mode, volatile,
more NH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula>NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>/(NH<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> type) and the second
(Loc_NIT) was assigned to local nitrate (ultrafine mode, less volatile,
more OC-NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> type). An enhancement of local nitrate was found under warm
and humid NAF_E air masses, indicating that meteorological conditions
(i.e. high relative humidity) or aerosol composition (i.e. sea salt, Saharan dust) could
affect local urban nitrate aerosol production.</p>
      <p>Two types of sea salt particles were also identified at both sites. NaCl particles showed a peak in the diurnal profile at 15:00,
related to the sea breeze and enhanced under NAF_E air masses. NaCl-NIT were mainly observed during more anthropogenically
influenced air masses.</p>
      <p>Two types of particles rich in metallic elements were found at both
monitoring sites. One, rich in iron and internally mixed with nitrate, was
found to be distributed in the fine accumulation mode at about 400 nm and
related to regional air masses. This observation supports previous findings
(Dall'Osto et al., 2010; Harrison et al., 2012) that showed fine
iron-containing aerosols are able to travel long distances and are thus
related to aged air masses. Other studies have reported anthropogenic
Fe-containing particles internally mixed with secondary species such as
sulfate (Furutani et al., 2011; Moffet et al., 2012) originating from coal
combustion in Asian continental outflows. This study shows that – within the
European continental outflow – Fe-containing particles are instead
internally mixed with nitrate. This observed difference is likely due to
emissions from coal combustion in Asia which are rich in SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, as opposed
to European air masses which are relatively higher in NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and lower in
SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Bio-available iron from atmospheric aerosol is an essential
nutrient that can control ocean productivity (Baker and Croot, 2010). Hence,
it can impact the global carbon budget and climate. There are also large
uncertainties in the origin of the aerosol nitrogen matter which may be
enhancing ocean productivity (Duce et al., 2008). The fact that iron is internally
mixed with nitrate points to an urban source (i.e. more traffic than
industrial activities) suggests that transported submicron urban particles can
be a source of both iron and nitrogen nutrients for the oceans. However, it
is worth noting that Cu-rich traffic-related aerosols can also have a
negative effect on marine phytoplankton over a vast region of the western
Mediterranean Sea (Jordi et al., 2012).</p>
      <p>A second metallic particle type rich in lead and chloride was identified.
This particle type was related to more local sources, presenting sharp
spikes in concentration. It is interesting to note this particle type was
found correlated with hourly elemental mass concentrations determined by
PIXE analysis (Dall'Osto et al., 2013b), showing that this particle
type can be a major source of submicron chloride in the urban area of
Barcelona.</p>
      <p>The ATOFMS equipped with the converging nozzle inlet at the UB site detected
four further different particle types. Two types of dust particles were
found, both occurring mainly in the coarse mode (<inline-formula><mml:math display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m): one
type, as attributed to Saharan Dust, was characterized by an
aluminium/silicon signature, while the other type, with a more local origin
(Ca dust), was characterized by a Ca-rich composition. Two other minor coarse
particle types were characterized: Veg-KP (rich in
potassium and phosphate), found enhanced during tropical NAF_E air masses,
and vanadium-containing particles (Oil-V), related to shipping/oil
combustion activities in the port of Barcelona. Overall, high concentrations
of vanadium were only observed on 1 day (3 October), indicating that
shipping emissions were a minor source of aerosol at the UB site.</p>
      <p>Eight particle types were detected by the ATOFMS with aerodynamic focussing
lens at the RS site. Overall, these particle types described less than
10 % of the aerosol population, but their mass spectra, as well as their
peculiar diurnal profiles, allow us to advance our understanding of the
OC-ON-nitrate mixing state of urban aerosols.</p>
      <p>Four particle types contain amines, which, in addition to ammonia, are
important atmospheric bases (Ge et al., 2011). Urban concentrations of
ammonia in Barcelona are higher than those reported in similar urban
background sites in Europe, especially in summer (Reche et al., 2012).
Conversely, in winter, levels of ammonia were higher at traffic-affected
sites, suggesting a contribution from vehicle emissions (Reche et al., 2012).
Emissions of ammonia from vehicular traffic have been widely reported and
they may increase in the future because it is not a regulated pollutant
(Suarez-Bertoa et al., 2015). In comparison, the sources, atmospheric
transformation, and sinks of amines are more poorly characterized. Overall,
both primary (amine POA 58 and amine ETS 84) and secondary (amine SOA 59
and amine SOA 114) sources of amine-containing particles were identified
during SAPUSS. The most abundant amine particle type (amine POA 58,
0.8 % of total particles at RS) was attributed to traffic activities and
the second-most abundant (amine ETS 84, 0.5 % of the total particles at
RS) was also associated with environmental tobacco smoke. Concurrent SAPUSS
measurements (Alier et al., 2013) of nicotine concentrations were much higher
at the RS site (58 ng m<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> than at UB (7 ng m<inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, pointing to a
significant outdoor cigarette consumption in the city centre. A recent study
(Sleiman et al., 2010) found that nicotine can contribute significantly to
the formation of urban SOA though reaction with ozone. The results of this
study therefore suggest that third-hand cigarette smoke may be a source of
nitrogen-containing particles in Barcelona and similar cities in southern
Europe where smoking is prominent.</p>
      <p>Amines were also related to secondary aerosol production, although a very
complex dynamic was found associated with their occurrences. They were found
to peak during the warmest part of the day (15:00) and during evening times
(22:00–23:00). Amine (SOA 59) was found particularly enhanced in regional
air masses (13–17 October 2010) when nitrate concentrations were also high
(Dall'Osto et al., 2013b). By contrast, amine (SOA114) was more abundant in
NAF_E humid air masses (7–11 October 2010). This latter type of SOA
was internally mixed with nitrate, suggesting aminium salt formation under
such specific conditions. Previous ATOFMS studies reported that most of the
amines volatilized during cold seasons, whereas during summer most were in
the form of low-volatility aminium nitrate and sulfate salts when particle
acidity was higher (Pratt et al., 2009). This observation supports previous
laboratory studies which reported that aerosol-containing non-salt organic
amines are more stable and less volatile than nitrate salts (Murphy et al.,
2007). Overall, amines can undergo oxidation by OH, O<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, and/or NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>
to form amides, nitramines, and imines, which can also partition to the
particle phase (Murphy et al., 2007; Silva et al., 2008; Healy et al., 2015).
Rehbein et al. (2011) combined field and laboratory work to demonstrate that
high relative humidity greatly enhances the gas-to-particle partitioning and
subsequent aqueous acid–base reaction of amines. High relative humidity favours aqueous
processing in general because aerosol is more likely to be in a deliquescent
or partly deliquescent form (Saukko et al., 2015). During the SAPUSS study,
we find aminium nitrate salts on coarse particles containing sulfate,
suggesting that heterogeneous reactions occur during the warmest part of the
day. This observation is in contrast to the study of Day et al. (2010), who
reported organonitrates when sulfate aerosols and humidity were low,
although the study site was less urbanized than the one used in this study.</p>
      <p>Finally, some consideration should be given to the four specific organic
particle types detected at the RS. One (Org. (Lub. Oil)) was found to be
related to primary lubricating oil traffic emissions. More difficult is the
attribution of the remaining three, which each contain an internal mixture
of OC and nitrate. This is not surprising given the fact that the urban
atmosphere is heavily contaminated by traffic emissions, the main producers
of the two chemical species (Dall'Osto et al., 2013a).</p>
      <p>Two different types of organic carbon/nitrate particle types were found. One
(OC-NIT) was found spiking in the afternoon. By contrast, a nitrate with a
strong aromatic signature (OC-Aro-NIT) was found mainly during night-time
(80 % of the time) and showing a sharp concentration peak at
19:00–20:00.
Part of the OC-Aro-NIT could be associated with products from the reaction of
aromatic components with NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> radicals (Benton et al.,
2010). These two ATOFMS particle types add complexity to the local–regional
inorganic nitrate-containing particle types, and further studies are needed
to correctly apportion the local urban nitrate component.</p>
      <p>The fourth organic particle type (OC-CHO) was found rich in oxidized organic
carbon and associated with nitrate from a traffic source. In a previous
ATOFMS study, considerable effort was made to apportion cooking-related
particle types (Dall'Osto and Harrison, 2012). However, only a particle type
exhibiting maximum frequency during the warmest part of the day and
associated with secondary aerosol production from traffic-related
semi-volatile aromatic compounds was found. During this study, we were again
not able to associate a specific particle type with cooking activities. In a
companion SAPUSS study, Alier et al. (2013) reported an aerosol source formed
mainly by C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">7</mml:mn></mml:msub></mml:math></inline-formula>–C<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">9</mml:mn></mml:msub></mml:math></inline-formula> dicarboxylic acids and detected especially during
daytime, which is highly dynamic, dependent on air masses, and pointing to a secondary
organic component driven by primary urban sources including cooking and
traffic (mainly gasoline) activities. O'Brien et al. (2013) reported a
detailed mass spectrometry characterization of the urban aerosol in an urban
background environment. Compounds containing only carbon, hydrogen, and
oxygen (CHO) and nitrogen-containing organic compounds (NOC) were found,
showing that both photo-oxidation and ammonia chemistry may play a role in
forming the compounds observed in the mixed urban–rural environment. NOC had
precursor product pairs consistent with imidization and cyclization
reactions, suggesting that part of the aromatic compounds detected during
SAPUSS may also be formed by cyclization and not only by condensation of
aromatic volatile organic compounds.</p>
      <p>In summary, the two ATOFMS instruments deployed during the SAPUSS field
measurement study showed that the urban atmosphere contains a complex
mixture of aerosol particles emitted from a variety of sources and formed
via numerous atmospheric processes. We have identified 22 different particle
types, characterized by specific single-particle mass spectra and temporal
trends. European Union abatement of traffic-related NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> levels is still
required to maintain levels within international standards (EEA, 2007).
Higher NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> levels (due to the high vehicle density and the high percentage
of diesel vehicles) are often seen in urban background locations in
Barcelona (and southern Europe) relative to other northern and central
European cities (Eeftens et al., 2012). Latitude variations within Europe
influence secondary nitrate aerosol formation (Revuelta et al., 2012).
Organic nitrogen species represent a considerable fraction of fine
particulate matter (Kiendler-Scharr et al., 2016). The present work shows a
number of unique particle types detected mainly at the traffic-dominated RS
site containing organic nitrogen and presenting different diurnal profiles,
likely originating from different sources and different processes. Further
studies are needed at high time resolution, emphasizing the need to better
understand the sources and properties of particulate organic nitrogen. The
ATOFMS measurements also provided some novel information on the mixing state
of organic carbon and nitrate in urban aerosols, again highlighting the
complex nature of the roles played by both primary sources and in situ
chemical processing in affecting aerosol composition.</p>
</sec>
<sec id="Ch1.S5">
  <title>Data availability</title>
      <p>Data are available by contacting the corresponding author.</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-16-9693-2016-supplement" xlink:title="pdf">doi:10.5194/acp-16-9693-2016-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>Financial support for this study was provided by the Marie Curie FP7 SAPUSS
(FP7-PEOPLE-2009-IEF, Project number 254773) and previously supported by
research projects from the D. G. de Calidad y Evaluacion Ambiental (Spanish
Ministry of the Environment) and the Plan Nacional de IyD (Spanish Ministry
of Science and Innovation) CGL2010-19464-VAMOS, CTQ2009-11572 and
CTQ2009-377-14777-C02-01-AERTRANS). The SAPUSS team is also
acknowledged.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by:
S. Decesari<?xmltex \hack{\newline}?> Reviewed by: two anonymous referees</p></ack><ref-list>
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an urban background and a roadside site during SAPUSS</article-title-html>
<abstract-html><p class="p">The aerosol time-of-flight mass spectrometer (ATOFMS) provides size-resolved
information on the chemical composition of single particles with high time
resolution. Within SAPUSS (Solving Aerosol Problems by Using Synergistic
Strategies), continuous ATOFMS measurements of ambient particles were made
simultaneously at two urban locations: urban background (UB) site and roadside (RS) site in the city of Barcelona (Spain) from 17 September to
18 October 2010. Two different instrumental configurations were used:
ATOFMS (TSI 3800) with a converging nozzle inlet (high efficiency at about
800–2000 nm) at the UB site and ATOFMS (TSI 3800-100) with an aerodynamic
lens inlet (high efficiency at about 300–700 nm) at the RS site. This is the
first time, to our knowledge, that two ATOFMS instruments have been deployed
in the same field study. The different instrument configurations had an
impact on the observed particle types at the two sites. Nevertheless,
10
particle types were detected at both locations, including local and regional
elemental carbon (22.7–58.9 % of total particles), fresh and aged sea salt
(1.0–14.6 %), local and regional nitrate-containing aerosols (3–11.6 %),
local lead-containing metallic particles (0.1–0.2 %), and transported
Fe-nitrate particles (0.8–2.5 %). The ATOFMS at the UB also characterized
four particle types: calcium-containing dust (0.9 %), Saharan dust
(1.3 %), vanadium-containing particles (0.9 %), and vegetative debris
(1.7 %). By contrast, the high statistical counts of fine particles
detected at the RS allowed identification of eight particle types. Four of
these contained organic nitrogen of primary and secondary origin, which
highlights the complex nature of the sources and processes that contribute
to this aerosol chemical component. Aminium salts were found related to
coarse sulfate-rich particle types, suggesting heterogeneous reaction
mechanisms for their formation. The other four particle types mainly
containing organic carbon were found spiking at different types of the day,
also showing a complex single-particle mixing state relationship between
organic carbon and nitrate. This ATOFMS study clearly shows that the
composition of atmospheric fine particles in Barcelona, and likely other
Mediterranean urban areas, is complex, with a wide range of local and
regional sources combining with chemical processing to produce at least
22 different particle types exhibiting different temporal behaviour.
The advantage of using two ATOFMS instruments is also demonstrated, with the
nozzle-skimmer configuration enabling detection of coarse dust particles and
the aerodynamic lens configuration allowing better identification of
particles rich in organic carbon and amines. Overall, we find that organic
nitrogen is a considerable fraction of the single particles detected,
especially at the traffic-dominated RS site. Further studies are needed,
especially at high time resolution, to better understand the sources and
properties of particulate organic nitrogen.</p></abstract-html>
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