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<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing with OASIS Tables v3.0 20080202//EN" "journalpub-oasis3.dtd">
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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 GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-15-5229-2015</article-id><title-group><article-title>Emission factors of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
particles from ships in Neva Bay from ground-based and helicopter-borne
measurements and AIS-based modeling</article-title>
      </title-group><?xmltex \runningtitle{Emission factors of SO${}_{{2}}$, NO${}_{{x}}$ and particles from ships}?><?xmltex \runningauthor{J.~Beecken et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Beecken</surname><given-names>J.</given-names></name>
          <email>beecken@chalmers.se</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mellqvist</surname><given-names>J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Salo</surname><given-names>K.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-1017-4261</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ekholm</surname><given-names>J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Jalkanen</surname><given-names>J.-P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8454-4109</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Johansson</surname><given-names>L.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Litvinenko</surname><given-names>V.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Volodin</surname><given-names>K.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Frank-Kamenetsky</surname><given-names>D. A.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Chalmers University of Technology, Earth and Space Sciences, Gothenburg, Sweden</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Finnish Meteorological Institute, Helsinki, Finland</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>State Geological Unitary Company Mineral, St. Petersburg, Russia</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Committee for Nature Use, Environmental Protection and Ecological Safety, St. Petersburg, Russia</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">J. Beecken (beecken@chalmers.se)</corresp></author-notes><pub-date><day>11</day><month>May</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>9</issue>
      <fpage>5229</fpage><lpage>5241</lpage>
      <history>
        <date date-type="received"><day>17</day><month>September</month><year>2014</year></date>
           <date date-type="rev-request"><day>16</day><month>October</month><year>2014</year></date>
           <date date-type="rev-recd"><day>13</day><month>March</month><year>2015</year></date>
           <date date-type="accepted"><day>31</day><month>March</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>


      <abstract>
    <p>Emission factors of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and size-distributed particle numbers
were measured for approximately 300 different ships in the Gulf of Finland
and Neva Bay area during two campaigns in August/September 2011 and
June/July 2012. The measurements were carried out from a harbor vessel and
from an Mi-8 helicopter downwind of passing ships. Other measurements were
carried out from shore sites near the island of Kronstadt and along the
Neva River in the urban area of Saint Petersburg. Most ships were running at
reduced speed (10 kn), i.e., not at their optimal load. Vessels for
domestic and international shipping were monitored. It was seen that the
distribution of the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factors is bi-modal, with averages of
4.6 and 18.2 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> for the lower and the higher mode, respectively. The
emission factors show compliance with the 1 % fuel sulfur content Sulfur Emission Control Areas (SECA)
limit for 90 % of the vessels in 2011 and 97 % in 2012. The
distribution of the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factor is mono-modal, with an average
of 58 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. The corresponding emission
related to the generated power yields an average of
12.1 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kWh<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>. The distribution of the emission
factors for particulate number shows that nearly 90 % of all particles in
the 5.6 nm to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m size range were below 70 nm in diameter. The
distribution of the corresponding emission factors for the mass indicates
two separated main modes, one for particles between 30 and 300 nm and the other
for above 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m. The average particle emission factors were found to be in
the range from 0.7 to <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>2.7</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mn>16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> particles kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and
0.2 to 3.4 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PM</mml:mi></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, respectively. The NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and particulate emissions
are comparable with other studies. The measured emission factors were
compared, for individual ships, to modeled ones using the Ship Traffic
Emission Assessment Model (STEAM) of the Finnish Meteorological Institute. A
reasonably good agreement for gaseous sulfur and nitrogen emissions can be
seen for ships in international traffic, but significant deviations are
found for inland vessels. Regarding particulate mass, the values of the modeled data are
about 2–3 times higher than the measured results, which probably reflects
the assumptions made in the modeled fuel sulfur content. The sulfur contents
in the fuel retrieved from the measurements were lower than the previously
used assumptions by the City of Saint Petersburg when carrying out
atmospheric modeling, and using these measurements it was possible to better
assess the impact of shipping on air quality.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>Shipping is a major means of transport. In 2012, about 9 billion tons of
goods were transported by ships, corresponding to almost 80 % of the
worldwide merchandise trade by volume, with about 4 % growth as compared
to 2011 (UNCTAD, 2013). As much as shipping is important as a means of
transport it is also a source for air pollution. In earlier studies, it is
estimated that about 15 % of the anthropogenic NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions and
7 % of the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emissions are due to shipping. Of these emissions
around 70 % occur within 400 km from land (Corbett et al.,
1999). Gaseous and particle emissions from ships have significant impacts on
nature, climate and human health. Corbett et al. (2007) estimated the
number of humans dying prematurely due to emissions from ships to be 60 000
each year.</p>
      <p>The significance of air pollution by ships has been acknowledged by policy
makers on the global level. Under the umbrella of the International Maritime
Organization (IMO) international limits have been agreed upon with the aim
to reduce the emissions of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> as agreed in the MARPOL
Annex VI protocol. As a consequence, a global cap of 3.5 % fuel sulfur
content, by mass, has been in effect since 2012. This cap is intended to be
reduced to 0.5 % in 2020. However, there are stronger limits set for
Sulfur Emission Control Areas (SECA), like the North Sea and the Baltic Sea.
Here ships are not allowed to bunker fuel with more than 1 % sulfur
content since 2010, which was further reduced to 0.1 % in January
2015.</p>
      <p>For marine diesel engines, there are different regulations for the emission
of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> depending on the ships' construction dates. The caps defined
under Tier 1 are valid for ships with engines built between the years 2000
and 2010. These caps are reduced in Tier 2 by 20 % for ships with engines
built after 2011 and a further reduction of 80 % in Tier 3 is intended for
ships with engines built in the year 2016 and afterwards. For Tier 3, there will be
exceptions for smaller recreational vessels and certain countries.</p>
      <p>The coming requirements for low fuel sulfur content in the SECA areas will
be rather costly for the shipping industry, which has a strong concern,
together with policy makers, that the new rules will not be obeyed. It is
therefore suggested that the regulations are enforced by compliance
monitoring to promote a level playing field within the shipping industry.
Within the Swedish project Identification of Gross-Polluting Ships (IGPS)
(Mellqvist and Berg, 2010; Beecken et al., 2014) a
monitoring system has been developed for measuring gaseous and particulate
emissions of individual ships within harbor areas and on the open sea, with
the capability to check compliance with the new emission rules in the SECA
areas.</p>
      <p>Within the context above, measurements of ship emission factors were carried
out for various air pollutants during two campaigns in the Neva Bay area and
the Gulf of Finland in 2011 and 2012, respectively, as part of the
IGPS-project and the EU project BSR-Innoship.</p>
      <p>A new system for measuring ship emissions which was previously used on
airborne platforms (Beecken et al., 2014) was applied for
the first time for measurements from ground and boat. In this study, the
particulate measurements were extended to an upper particle size of 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, instead of 500 nm, and a more precise total number counter was
used. A considerable fraction of the ships measured in this study correspond
to river barges and other ships running only in the eastern part of the Gulf
of Finland and the Neva River, complementing the earlier study which
corresponded primarily to ocean-going ships, such as containers vessels, oil
tankers and ferry boats. The measurements in 2011 were carried out at the
transition period when Russia ratified the Annex VI protocol in April 2011
requiring maximum 1 % sulfur content in the fuel which came into effect
on 8 July 2011 (AMSA, 2014). Since very few real world emission
measurements of ships have been conducted worldwide, especially in the
eastern Baltic where to our knowledge no such studies have been carried out
before, there is a need for this type of data to be able to model ship
emissions more accurately and subsequently carry out air quality modeling.
The data derived in this study are compared to the STEAM model (Jalkanen
et al., 2009, 2012; Jalkanen and Johansson, 2013), which is
widely used, e.g., within the HELCOM (Baltic Marine Environment Protection Commission - Helsinki Commission) community to model individual ship
emissions and to estimate emissions on regional and global scale. The
objective of this study was to help to readjust and refine this model and
to demonstrate the performance of such a model.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
      <p>The results presented in this paper were obtained using an extended system
for the identification of gross-polluting ships (IGPS), (Mellqvist and
Berg, 2010). A short overview on the instrumentation is given in Sect. 2.1. The system's main components are described in
detail by Beecken et al. (2014). Additional components are
an optical particle sizer for particles up to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m and a
condensation particle counter.</p>
<sec id="Ch1.S2.SS1">
  <title>Instrumentation</title>
      <p>CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was measured with cavity ring-down spectroscopy (CRDS)
(O'Keefe and Deacon, 1988) using a modified flight
Picarro G2301-m greenhouse gas monitor with a response time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, of
less than 1 s, the time that is needed at a step change to reach 90 %
of the final value. The instrument produces a CO<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">2</mml:mn></mml:msub></mml:math></inline-formula>O and
CH<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> value once every second which is obtained by sequentially measuring
the three species for around 0.3 s per species.</p>
      <p>For determining the sulfur emission factor in the form of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, a modified
Thermo 43iTLE trace gas monitor was used. An internal UV flash lamp
stimulates fluorescence of the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> which is proportional to its volume
mixing ratio (VMR) (Luke, 1997). The instrument is custom-modified through
the elimination of a “hydrocarbon kicker”, and larger pump speed yielding a
response time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, of about 2 s to allow flow rates for the detection
of short and distinct plumes. The SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> instrument is cross-sensitive to
NO, with a SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> VMR reading corresponding to 1.5 % of the VMR of NO.
The removal of the kicker, which is simply a Teflon tube coil, also makes
the instrument cross sensitive to aromatic volatile organic compounds (VOC)
with about 1 % of the VOC VMR, but in most cases, ships emit very little
VOC (Williams et al., 2009), so this is only a problem when measuring in
proximity to large VOC sources, such as refineries, since this may cause
fluctuating background readings.</p>
      <p>The emission factor of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was obtained with a custom modified
Thermo 42TL trace gas monitor. A larger pump is used to obtain lower
instrument pressures, and a modification in the software allows for the
user to externally control whether NO, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> or the zero background
should be measured, instead of continuously switching between measurement
and zero background. The VMR of NO is determined by a chemiluminescent
reaction of NO with ozone. The intensity of the light emitted is
proportional to the VMR of NO (Kley and McFarland, 1980). The
instrument uses a catalytic converter that converts the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> to NO, so
the sum of NO and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>) is obtained. The instrument has a
response time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, of 1 s.</p>
      <p>An instrument based on electric mobility, the Engine Exhaust Particle Sizer
(EEPS, TSI 3090), was applied to analyze the number size distribution in the
range from 5.6 to 560 nm in 32 size channels. The particles in a stream
of sampled air are charged by a corona and then forced to move in an
electrical field which deflects them towards a column of electrodes
(Johnson et al., 2004). The EEPS is originally intended for
fast particle sizing of engine exhaust, and due to its fast simultaneous
sampling at 10 Hz and response time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, of 0.5 s it also was found
to be suitable for measurements of particulate ship emissions (Hallquist
et al., 2013; Jonsson et al., 2011), even from aircraft
(Beecken et al., 2014).</p>
      <p>The size distribution of bigger particles was measured with an Optical
Particle Sizer (OPS, TSI 3330). The OPS measures the backscattered intensity
of light pulses onto a stream of sample air with particles. The number and
size of the particles is determined from the detected backscattered light
flashes. The diameter of the detected particles ranges from 0.3 to
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m and is binned into 16 size channels. The instruments response
time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, is 2 s.</p>
      <p>The total number of particles was determined with TSI 3787 General Purpose
Water-Based Condensation Particle Counter (CPC) (Hering
et al., 2005). Sampled particles are grown in a supersaturated chamber and
afterwards optically counted. This CPC measures particles bigger than 5 nm
up to approximately 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m with a response time, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mn>90</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, of less
than 0.3 s. The CPC was only used during the 2012 campaign.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Example of plume evaluation on a typical plume, here from the Ro-Ro
(Roll-on/roll-off)
cargo ship <italic>Pauline Russ</italic>. The signal of three gas channels and one
particle channel are shown as a grey line. The black line is the found
background baseline to be subtracted from the plume. The plume's signal is
integrated over time (grey shaded area). The ratio of the areas of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> to CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is used for further calculation of the emission factors.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f01.png"/>

        </fig>

</sec>
<sec id="Ch1.S2.SS2">
  <title>Calculation of emission factors</title>
      <p>The calculation of emission factors is similar for gas and particle data.
The evaluation of sampled plumes is illustrated in
Fig. 1. After the identification of a plume, a
baseline is determined and subtracted from the in-plume values. The
background-corrected data, given in mixing ratios units (here in ppb or
ppm), is integrated over the plume for each substituent <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula>, and then
normalized against the integrated CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values according to Eq. (1).
Furthermore, the calculated ratio is converted to a mass-based emission
factor, i.e., mass of pollutant versus mass of fuel, by scaling with the
molecular weights of the species <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> and fuel; the latter obtained as
molecular weight of carbon corrected with the assumed carbon content of the
fuel, i.e., 87 %. Note that for the calculation of fuel sulfur content the
species <inline-formula><mml:math display="inline"><mml:mi>X</mml:mi></mml:math></inline-formula> is replaced with pure sulfur, e.g., 20 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> corresponds to a fuel sulfur content (FSC) of 1 %.
In the case of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, its molecular weight is assumed to correspond to
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, following the IMO technical code MEPC.177(58) (MEPC, 2008).</p>
      <p>It is common to compare the performance of different engines, especially for
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, by using load-based emission factors, i.e., mass of pollutant
versus generated crank shaft power. In order to obtain this value (specific
emission factor) the mass-based emission factors is multiplied with the
brake-specific fuel consumption (BSFC), which relates the consumed fuel to
the generated power. This number, which varies between
160–250 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi></mml:msub></mml:math></inline-formula> kWh<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> depending on ship type, was in
this study obtained from the STEAM model data (Jalkanen et al.,
2009, 2012), which in turn is based on ship specific data
from the IHS Maritime ship register (IHS Global, 2014). In the cases of no
registered BSFC, a default value of 200 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kWh<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>
was assumed.
<?xmltex \hack{\newpage}?></p>
      <p><disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi mathvariant="normal">EF</mml:mi><mml:msub><mml:mfenced open="(" close=")"><mml:mi>X</mml:mi></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">kg</mml:mi><mml:mi mathvariant="normal">fuel</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>M</mml:mi><mml:msub><mml:mfenced close=")" open="("><mml:mi>X</mml:mi></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">mol</mml:mi></mml:mrow></mml:msub><mml:mo>×</mml:mo><mml:mo>∫</mml:mo><mml:msub><mml:mfenced close="]" open="["><mml:mi>X</mml:mi></mml:mfenced><mml:mi mathvariant="normal">ppb</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi>X</mml:mi><mml:mi mathvariant="normal">bgd</mml:mi></mml:msub></mml:mfenced><mml:mi mathvariant="normal">ppb</mml:mi></mml:msub><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow><mml:mrow><mml:mfrac><mml:mrow><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">C</mml:mi><mml:msub><mml:mo>)</mml:mo><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">mol</mml:mi></mml:mrow></mml:msub></mml:mrow><mml:mn>0.87</mml:mn></mml:mfrac><mml:mo>×</mml:mo><mml:mo>∫</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mi mathvariant="normal">ppm</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">bgd</mml:mi></mml:mrow></mml:msub></mml:mfenced><mml:mi mathvariant="normal">ppm</mml:mi></mml:msub><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle></mml:mrow></mml:math></disp-formula></p>
      <p>For the calculation of the particle number emission factor EF(PN) in
Eq. (2), the excess number concentration per volume unit in the plumes was
related to the excess mass concentration per volume unit of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
(assuming <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mi mathvariant="normal">avg</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 290 K, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">avg</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 101 325 Pa) using the ideal
gas law, with the ideal gas constant <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 8.314 J mol<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> K<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>. The emission factor of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> is
here calculated using Eq. (1).

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:mi mathvariant="normal">EF</mml:mi><mml:msub><mml:mfenced open="(" close=")"><mml:mi mathvariant="normal">PN</mml:mi></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">#</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">kg</mml:mi><mml:mi mathvariant="normal">fuel</mml:mi></mml:msub></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mo>∫</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:mi mathvariant="normal">PN</mml:mi></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">#</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mfenced close="]" open="["><mml:msub><mml:mi mathvariant="normal">PN</mml:mi><mml:mi mathvariant="normal">bgd</mml:mi></mml:msub></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">#</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:msub><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow><mml:mrow><mml:mo>∫</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">kg</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mfenced close="]" open="["><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>,</mml:mo><mml:mi mathvariant="normal">bgd</mml:mi></mml:mrow></mml:msub></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">kg</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:msub><mml:mi>d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E2"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><?xmltex \hack{\hspace*{2.05cm}}?><mml:mo>×</mml:mo><mml:mi mathvariant="normal">EF</mml:mi><mml:msub><mml:mfenced close=")" open="("><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">kg</mml:mi><mml:mo>/</mml:mo><mml:msub><mml:mi mathvariant="normal">kg</mml:mi><mml:mi mathvariant="normal">fuel</mml:mi></mml:msub></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

                <disp-formula specific-use="align" content-type="numbered"><mml:math display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd/><mml:mtd><mml:mrow><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mrow><mml:mi mathvariant="normal">kg</mml:mi><mml:mo>/</mml:mo><mml:msup><mml:mi mathvariant="normal">cm</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mfenced open="[" close="]"><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mfenced><mml:mi mathvariant="normal">ppm</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>M</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="normal">CO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mo>)</mml:mo><mml:mrow><mml:mi mathvariant="normal">g</mml:mi><mml:mo>/</mml:mo><mml:mi mathvariant="normal">mol</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd/><mml:mtd/><mml:mtd><mml:mrow><?xmltex \hack{\hspace*{1.75cm}}?><mml:mo>×</mml:mo><mml:mfrac><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">Pa</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mrow><mml:mi mathvariant="normal">J</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="normal">mol</mml:mi><mml:mo>×</mml:mo><mml:mi mathvariant="normal">K</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:msub><mml:mo>×</mml:mo><mml:msub><mml:mi>T</mml:mi><mml:mi>K</mml:mi></mml:msub></mml:mrow></mml:mfrac><mml:mo>×</mml:mo><mml:msup><mml:mn>10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn>15</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula></p>
      <p>The calculation of the emission factor of the particle mass is done
analogously to Eq. (1) by substituting particle number (PN) with particle mass (PM). A
unity density of 1 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> was arbitrarily assumed for the
sake of qualitative comparison, although diesel particle density varies with
composition and size between 0.5 and 1.23 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> for
particles between 50 and 150 nm (Barone et al., 2011; Virtanen et al.,
2002; Petzold et al., 2008). For the estimation of the emission factor of the
particle mass, the particle sized data from the EEPS and OPS instruments were
used. The results for the particle sizers were additionally compensated for
by
the actual size dependent diffusion losses under laminar flow conditions
(Hinds, 1999).</p>
      <p>The geometric mean diameter (GMD) was calculated using Eq. (4) (Hinds,
1999). It should be noted that the EEPS measures the particle diameter
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> depending on the electro-mobility of the particles while the OPS
measures diameters depending on the optical properties of the particles.
            <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi mathvariant="normal">GMD</mml:mi><mml:mi mathvariant="normal">nm</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced close=")" open="("><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mo>∑</mml:mo><mml:mfenced open="[" close="]"><mml:msub><mml:mi>n</mml:mi><mml:mi>i</mml:mi></mml:msub><mml:mo>×</mml:mo><mml:mi>ln⁡</mml:mi><mml:mfenced open="(" close=")"><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>i</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:msub></mml:mfenced></mml:mfenced></mml:mrow><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle></mml:mfenced></mml:mrow></mml:math></disp-formula></p>
      <p>The symbols <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>n</mml:mi><mml:mi>i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> denote the number of particles in the respective
size bin and the total number of particles of all size bins, respectively.
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi>p</mml:mi><mml:mi>i</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is the center diameter of the respective size bin.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Calibrations</title>
      <p>Calibrations of the gas-phase instruments were performed repeatedly during
the measurement campaigns. The calibration gases were obtained from the
Russian D.I. Mendeleyev Institute for Metrology (VNIIM) Standard Materials
Service.</p>
      <p>In 2011, cylinders with known gas mixtures were used for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
(401 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 %, 356 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 %) and NO (250 ppb <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 10 %). SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was calibrated with a dynamic gas calibrator, based on
mass flow controller GGS-03-03 from OOO Monitoring, that mixes a high
concentrated SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (53.4 ppm) with zero air by controlling the respective
mass flow. SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was calibrated in several steps up to 529 ppb. Because
the maximum flow of the gas calibrator was less than the flow of the
measurement system, the calibration gas was filled in Tedlar gas sampling
bags which were subsequently used in the calibration. This procedure was
only carried out twice during the campaign.</p>
      <p>In 2012, a high-flow dynamic gas calibrator (Thermo 146i), in conjunction with
a zero-air supply (Thermo 1160), was used to dilute SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> at
63.7 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % and NO at 64 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 5 % in several calibration
steps to volume mixing ratios between 0 and 300 ppb for both gases. For
CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> two calibration mixtures of 365 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % and
418 ppm <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 3 % were used. This gas calibrator eliminated the need
for
Tedlar bags and therefore the calibration could be done several times each
measurement day.</p>
      <p>The measurement precision of the gas-phase instruments was estimated from
the standard deviation during the calibrations, over a period between 30 and
120 s. The measurement precision of the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> instrument was recorded as
3.6 % in 2012, while for 2011 it was assumed to be 5 % due to fewer
calibrations. For the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> analyzer, the standard deviation of the
response was recorded to be 0.5 % in 2011 and 1.3 % in 2012,
respectively.</p>
      <p>The plume samples were corrected using calibration factors. The uncertainty
due to the interpolation of the calibration factors is estimated by
evaluating the mean standard deviation between two adjacent calibration
points. It was 0.2 and 0.7 % for CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> respectively for 2011 and
2012. For SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, it was 4.7 and 2.0 % and for NO, 4.0 and
2.1 % for these years.</p>
      <p>The size response of the particle sizers was validated for both campaigns
with vaporized Diethylhexyl Sebacate (DEHS) with particle diameters,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, between 200 and 300 nm during the campaigns with good agreement.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Uncertainties</title>
      <p>The results of repeatedly measured plumes from the same ship were used to
estimate the precision, i.e., random uncertainty, of the emission factor
measurements from the helicopter. The 1 <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>×</mml:mo><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> precision
values were 19.5 % for SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 23.7 % for NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, respectively,
based on the mean precision of 12 ships that were measured at least three times.</p>
      <p>For the ground-based measurements, the random uncertainty is expected to be
smaller, since the plumes were present for a considerably longer time, and the
random uncertainties above are therefore considered as an upper level.</p>
      <p>The systematic uncertainties consist of the calibration uncertainties and the
uncertainty by the model-based retrieval of the BSFC. Furthermore, other
studies indicate that the sulfur content may be systematically underestimated
by 1–19 % when applying ratio measurement of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> over CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
hence assuming that all sulfur is emitted in the form of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Schlager
et al., 2006; Agrawal et al., 2008; Moldanová et al., 2009, 2013; Balzani
Lööv et al., 2014). Since the conclusions from these studies are
quite inconsistent, this potential uncertainty is not included in the error
estimation here.</p>
      <p>Following the IMO guidelines, the carbon mass fraction in fuel varies between
85 and 87.5 % (MEPC, 2005). The carbon mass fraction of
heavy fuel oil is closer to the lower end and diesel oil closer to the
higher end of this interval. In this study a carbon mass fraction of 87 %
was assumed in the calculation of the emission factors. The maximum error
due to this assumption is approximately 2.4 %.</p>
      <p>The overall measurement uncertainty is calculated as the root of sum of
squares (RSS) of the systematic and random uncertainties. Where the
uncertainties of the two campaigns were combined, the higher uncertainty was
taken into account. This yields the total uncertainties of 21 and
26 % for the mass-based emission factors of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>,
respectively. For the calculation of the specific emission factor for
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> an additional uncertainty of 11 % for the BSFC data is added,
yielding a total uncertainty of 29 %.</p>
      <p>The uncertainties above are comparable to estimates that were done in a
previous study using the same system (Beecken et al., 2014),
where the uncertainties in the mass-based emission factors were 20 % for
SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 24 % for NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. Alföldy et al. (2013) report similar uncertainties of 23 % for SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and 26 %
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. It should be noted that the uncertainty for emission factor of
SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> of 20 % was found for FSCs of around 1 %. In a study by
Mellqvist et al. (2015), the emission of a ship which was known to
run voluntarily on marine gas oil and hence with FSC of 0.1 % or below
was repeatedly measured, yet at different occasions, using the same system
at a fixed site. The measurements indicate an average FSC of 0.06 % with
a standard deviation of about 0.03 %. Under the assumption that the FSC
used by the ship would be the same during all measurements, this would indicate
an uncertainty of about 50 % for the EF(SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>) for ships running on
low FSC around 0.1 %.</p>
      <p>According to the instrument certificate, the EEPS was analyzed by the
manufacturer (TSI) against a scanning mobility particle sizer (SMPS) system
for particle size distribution accuracy and a CPC (TSI CPC 3022,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>D</mml:mi><mml:mrow><mml:mi mathvariant="normal">p</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">min</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 7 nm) for total number accuracy using both 100 nm classified
and polydisperse emery oil. According to the manufacturer's certificate, the
deviation of particle size distribution was found to be less than 7 % and
the deviation in total number less than 20 %.</p>
      <p>Cross-comparison measurements of the EEPS were performed at our laboratory
with a SMPS (TSI DMA 3081 and TSI CPC 3787) with ammonium sulfate at
concentrations between 1.85 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>11</mml:mn></mml:msup></mml:math></inline-formula> and 8.36 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>11</mml:mn></mml:msup></mml:math></inline-formula> particles m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. It was found that the GMDs in a
size region around 30 nm measured with the EEPS are around 14 % below
those measured with the SMPS. In this study it is assumed that the CPC
counts all particles. The SMPS System which was used in this comparison was
validated with standardized polystyrene latex spheres (PLS) of known sizes
between 70 and 500 nm. From the deviations, it was seen that the particle
diameters were underestimated by the SMPS by less than 1 % at an offset
of less than 7 nm. A comparison with the CPC indicated an underestimation of
the total particle number of about 30 % by the EEPS. A similar
discrepancy has been observed in another study (Jonsson et al.,
2011), when comparing the same type of instruments.</p>
      <p>In this study it was not possible to perform any cross validations for the
OPS. Instead the manufacturer's quality assurance certificates have to be
relied on for error estimation, corresponding to an uncertainty in size
resolution of 3.5 % and in number better than 10 % for particles
around 0.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m.</p>
</sec>
<sec id="Ch1.S2.SS5">
  <title>Ship emission modeling</title>
      <p>The STEAM model generates ship specific emissions of CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and particulates at the time and location of the actual ships
(Jalkanen et al., 2009, 2012; Jalkanen and Johansson,
2013). The model uses as input values the position reports generated by the
automatic identification system (AIS), this system is on-board
every vessel that weighs more than 300 t throughout the globe. The AIS system provides
automatic updates of the positions and instantaneous speeds of ships at
intervals of a few seconds. The model requires as input also the detailed
technical specifications of all fuel consuming systems on-board and other
relevant technical details of the ships, taken from the IHS Maritime ship
register (IHS Global, 2014), for all the ships.</p>
      <p>The propelling power of each ship is predicted as a function of its speed.
In STEAM, the fuel type and sulfur content for different engines are
assigned on a per vessel basis and for main and auxiliary engines
separately. If the sulfur content of the fuel is known explicitly, it is
used by the model. In any other case the sulfur content is determined by
engine properties (engine power, angular velocity and stroke type) according
to the classification proposed by Kuiken (2008). The NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions
are modeled according to IMO three tier approach as a function of engine
angular velocity (revolutions per minute; rpm). For vessels built before the year
2000, the so-called Tier 0 ships, the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factors 10 %
above the Tier 1 level are assigned (Starcrest, 2012). Emission factors
for PM are determined based on the FSC as described in
Jalkanen et al. (2012). This approach assumes a
linear relationship between sulfate aerosol formation and fuel sulfur
content, but engine load level changes to sulfur–sulfate conversion
efficiency were not modeled. Note that when comparing the results of modeled data with the measured data, in STEAM the gas-phase emissions of sulfur were calculated as SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, which is the sum of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, while during the campaigns just SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> was measured. However, in the comparison it is assumed that the abundance of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula> is negligible.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Map overview of the measurement sites. Most of the measurements from
the harbor boat <italic>Redut</italic> were performed from the main <italic>Redut</italic> sites. Some
during the passage between these sites and the port. (Map
data<sup>©</sup> OpenStreetMap)</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f02.png"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Measurements</title>
      <p>Measurements in the Neva Bay were conducted from land and ship while the
measurements in the Gulf of Finland were carried out from a Mi-8 helicopter.
The locations of the measurements are presented in
Fig. 2. The measurements with the helicopter were
mostly performed on ships at open sea to the west of the St. Petersburg Dam.
The measurement campaigns took place in August/September 2011 and June/July 2012. Most measurements were carried out from a harbor vessel, but for
3 days in 2011, measurements were also conducted from a vehicle parked along
the Neva River and at the St. Petersburg Dam. For 5 days in
July 2012, measurements were carried out from a Mi-8 helicopter.</p>
      <p>Most of the measurements were conducted onboard the work vessel <italic>Redut</italic>,
Fig. 3, while anchoring downwind the main ship
passage trail in the Neva Bay between the island of Kronstadt and Saint Petersburg. This ship passage is used by all commercial ships going to and
from Saint Petersburg and by river ships that sail further up the Neva River.
In 2011, these measurements took place between 22 August and 5 September, and in
2012 from 26 June to 5 July. In Neva Bay, vessel speed is restricted to
10 kn, with an exception for fast ferries running up to 30 kn, and
many ships were hence running at half their design speed, with low engine
loads. This impacts, in particular, the emission factors of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and
particles (Lack et al., 2011; Cappa et al., 2014). The ships on the open
sea had speeds up to 20 kn.</p>
      <p>The sample inlets themselves were mounted to the front of the vessel at
6.5 m above sea level in 2011 and 8.5 m in 2012, far away from the
smokestack at the aft.</p>
      <p>Stationary measurements were carried out from a van on 18 and 19 August
2011, close to the storm surge gates at the Saint Petersburg Dam. The sample
inlets were mounted onto a mast at around 7 m above sea level. In addition,
similar measurements were performed during the night from 20 to 21 August
2011, studying the traffic on the Bolshaya Neva river arm near the
Blagoveshchensky Bridge, while the bridges were open for ship traffic. The
sample inlets were 6.5 m above sea level.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Top: work vessel <italic>Redut</italic> with sample inlets (photo of
<italic>Redut</italic> taken by M. Pingoud); bottom: Mi-8 helicopter with sample inlet.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f03.jpg"/>

      </fig>

      <p>Measurements from onboard the Mi-8 helicopter,
Fig. 3, were conducted between 5 and 10 July
2012, with about 17 flight hours in total. In the helicopter, a probe was
used that was pointed straight out, with 50 cm distance from the fuselage. To
minimize the influence of downwash from the rotor, the helicopter was
operated at a steady forward motion, usually between 40 and 70 kn. This
minimized variations in the CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> values that were interpreted as
turbulence caused by the rotor. The typical flight altitude was around 65 m
above sea surface to be able to sample the ship plumes and the helicopter
generally flew outside the Neva Bay, as illustrated in
Fig. 2.</p>
      <p>During the helicopter measurements, larger ships were predominantly chosen
for the measurements while for the ground-based measurements, plumes of any
of the passing ships were measured, since the latter were done in a passive
manner.</p>
      <p><?xmltex \hack{\newpage}?>The domestic vessels are divided into cargo boats (Nevsky vessels) and
tankers (Volgoneft), operating on the Neva River and the east part of the
Gulf of Finland and fast hydrofoil ferries traveling between the city of St. Petersburg and Peterhof.</p>
      <p>The measured data was compared to the modeled data using the STEAM ship
emission model.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>The frequency distribution of the measured emission factors of
SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Two main modes can be identified for the ground-based measurements;
one for small SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factors below and around
4 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, and the other one for
20 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> in 2011 and
16 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> in 2012.</p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f04.png"/>

      </fig>

</sec>
<sec id="Ch1.S4">
  <title>Results and discussion</title>
      <p>In total 466 plumes from 311 different vessels were observed, of which
434 plumes were observed during the ground-based measurements and 32 plumes were observed from
the helicopter. Most of the plumes which were measured from the helicopter
were sampled repeatedly for the same vessel. Results from individual
measurements can be found in the Supplement.</p>
<sec id="Ch1.S4.SS1">
  <title>Sulfur dioxide</title>
      <p>The frequency distribution of the measured SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factors is
shown in Fig. 4. The distributions of the
ground-based measurements show that there are two prominent modes separated
by the gap at 12 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> with about 50 %
of the measurements on either side. The median emission in the lower mode is
about 4.6 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> while the first and
third quartiles can be found at 2.7 and 7.5 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>,
respectively. The corresponding median in the higher mode is
18.2, and
15.4 and
21.3 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> for the first and
third quartiles. The distribution of the helicopter-borne measured
emission factors are almost entirely located around 20 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and particle emission factors over different ship
types and comparison to results from the literature. The number close to the
boxes denotes the number of sampled plumes from this ship type; numbers in
brackets, the fraction of plumes that were measured from the helicopter. Ship types Nevsky, Volgoneft and Fast Ferry are shown separately from their
main groups.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f05.png"/>

        </fig>

      <p>The emission factors of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> for different ship types are shown in
Fig. 5. Nearly all values are below
20 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. However, a clear difference in
the sulfur emission can be seen for the different types. Vessels which are
operated mostly in domestic waters, i.e., fast ferries, Nevsky class cargo
vessels, Volgoneft tankers and tugs, emitted less than
10 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, indicating low fuel sulfur
content, while the internationally operating ships had higher fuel sulfur
contents.</p>
      <p>The measured SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factors indicate that there was a reduction
of 13 % in the sulfur emission factors between 2011 and 2012, with
80 % of the plumes corresponding to emission factors below
21.2 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> in 2011 and below 18.4 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> in 2012. The
results obtained from ground-based measurement in Neva Bay in 2011 and 2012
indicate that 90 and 97 %, respectively, of the ships complied with
IMO FSC limit of 1 %, when taking the measurement uncertainty into
account. The 32 ships measured outside Neva Bay from the helicopter all
complied with the IMO sulfur limits.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6"><caption><p>The frequency distribution of the measured emission factors of
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. It can be seen that there is a distinct peak around
60 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> which can be seen for all
campaigns. For helicopter-borne measurements, no samples were seen with
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factors above
75 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f06.png"/>

        </fig>

<?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Nitrogen oxides</title>
      <p>In Fig. 6 it can be seen that the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emission factors are distributed around a single peak. The median of the
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission related to the amount of consumed fuel can be found at
58 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and the first and third
quartiles at 44 and 70 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. The
measured median NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factor in this study is 12 % below the
average value found by Williams et al. (2009), probably due the fact that
most ships were running at low speed with relatively low loads
(Borkowski et al., 2011). These lower values are consistent with
other studies (Alföldy et al., 2013; Pirjola et al., 2014) also taking
place in harbor areas or channels where ships were running at reduced speed
(Cappa et al., 2014).</p>
      <p>For the power related emission the corresponding median is at
12.1 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kWh<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> and the first and third
quartiles at 9.1 and 14.4 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kWh<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>. The NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>
emission factors are shown for different ship types in
Fig. 5.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Averaged normalized size distribution of the EF(PN) and the
cumulative sum of the median EF(PM) distribution over particle size. Around
77 % of the particles in the range 5.6 nm to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m were found
to be between 7 and 65 nm in size. Around 70 % of the EF(PM) is from
particles below 300 nm.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f07.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <title>Particulate matter</title>
      <p>The normalized size distributions in number, EF(PN), and mass units, EF(PM),
for individual plume measurements are shown in
Fig. 7. Ninety percent of the measured particles
were smaller than 70 nm. It can be seen that the 10th to the 90th
percentile range of the GMDs is between 24 and 53 nm. In a similar study
(Jonsson et al., 2011), in the harbor of Gothenburg, Sweden,
measurements were carried out from about the same distance as in this study,
and in this case the GMD values were between 21 and 39 nm for six selected
ships, consistent with the data given in this paper. The graph showing
EF(PN) also indicates the presence of a second smaller particle mode with
diameters of about 10 nm, probably corresponding to fresh particles produced
in the flue gas, which is also observed in other studies (Hallquist et
al., 2013; Moldanová et al., 2013). Around 70 % of the total measured
EF(PM) particulate mass below 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m consists of particles smaller
than 300 nm. In the distribution of the particle mass emission factor, two
separate size regions were identified to contribute to the mass, one for
particles from 30 to 300 nm and the other for particles above 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m.
This is based on the assumption that all measured particles have spherical
shape and unit density.</p>
      <p>A comparison of the total particle numbers from measurements with the CPC
and the combined measurements with the EEPS and OPS shows high correlation
(<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>0.98</mml:mn></mml:mrow></mml:math></inline-formula>) and a root mean square error (RMSE) of 0.17 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula> particles kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. However, the CPC
results show 34 % higher values than the combined particle sizers.</p>
      <p>In Fig. 8, the frequency distributions of the
measured emission factors of total particle numbers for each instrument are
presented, whereas the result for the frequency distribution for particulate
mass, EF(PM), is shown in Fig. 9. The statistical
distributions of the particle emission factors for number and mass are shown
for the different ship types in Fig. 5.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Frequency distribution of emission factors for particle number shown
for <bold>(a)</bold> CPC (&gt; 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m), <bold>(b)</bold> EEPS (5.6
to 560 nm) and <bold>(c)</bold> OPS (0.3 to 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m).</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f08.png"/>

        </fig>

      <p>Altogether, the number and mass emission factors measured by the particle
sizers lie within the ranges of 0.7 to 2.7 <inline-formula><mml:math display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mn>16</mml:mn></mml:msup></mml:math></inline-formula> particles kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and of 0.2 to
3.4 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PM</mml:mi></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>, respectively. These ranges
compare well with the results found in other studies (Petzold et al.,
2008; Murphy et al., 2009; Jonsson et al., 2011; Lack et al., 2011; Alföldy
et al., 2013; Beecken et al., 2014; Pirjola et al., 2014) between 0.3 and
2.55 particles kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> or accordingly for
particulate mass, between 0.4 and 3.77 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">PM</mml:mi></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>.</p>
</sec>
<sec id="Ch1.S4.SS4">
  <title>Comparison of modeled to measured data</title>
      <p>The differences between measured and modeled emission factors by STEAM are
summarized for each ship type in Fig. 10. The
data for each ship was modeled considering the actual ship speed at the time
of the plume measurement to estimate the engine load.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Frequency distribution of emission factors for particle mass. The
data bases on the particle sizer measurements from the EEPS and the OPS. The
size distribution of the OPS was truncated for size channels below 560 nm
i.e., the upper size limit of the EEPS. Since no more data is available at
this stage, the particles are assumed to be of spherical shape with a density
of 1 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f09.png"/>

        </fig>

      <p>When comparing modeled and measured SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factors, it can be
seen that there is good agreement for passenger ships in international
traffic and only a slight positive bias for the model for cargo and tanker
ships. This hence indicates that the assigned model FSC for these ships is
approximately correct. However, there are also many inland vessels for which
there is a large positive bias in the model, indicating that the assigned
model FSC of 1 % is much too high since the domestically running cargo
and tanker ships actually had a measured FSC of around 0.4 % or less.
This reflects the restrictions of fuel used in inland waterway traffic,
which to our knowledge prohibit the use of heavy fuel oil within the city
borders due to ship-operation safety reasons. Improvements to the FSC
predictions of especially inland vessels needs local knowledge and
geographical restrictions. In future modeling work, the fuel assignment
of inland waterway traffic must be considered in a more realistic manner
because fuel type and sulfur content assignment will have an impact on both
SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and PM emission factors.</p>
      <p>This fact was pointed out to the air quality authorities of the City of
Saint Petersburg (Krylov et al., 2012), who assumed a
FSC of 1 and 1.5 % for the primary fuel of 70 and 30 % of
the ships, respectively, when carrying out air quality modeling. They later
adapted the emission factors in their modeling to 0.17 and 1 %,
based on the FSC data given in this paper with the consequence that shipping
area had considerably less impact on air quality in the Saint Petersburg
than originally estimated, especially for sulfur but also particles.</p>
      <p>The modeled emission factors of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> match well with the measurements
for passenger ships and domestic tankers, as shown in
Fig. 10. The average difference is around
3 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>4 % relative to average)
and the spread for individual ships is in the order of the measurement
uncertainty for NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>. For domestic cargo ships, the average difference
between the model and measurement results is 9 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>11 %) lower than the measured emissions.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p>Comparison between modeled data by STEAM and measured data. The
differences of the emission factors are shown group-wise for individual ships
at same speed. Thus it is shown in the graphs by how much the STEAM model
statistically exceeds the measured data. It should be considered that the
modeled SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> was compared to the measured SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>. Furthermore, the sum
of the modeled emissions of organic carbon, elemental carbon, ash and SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:math></inline-formula> are compared to the
measured size-distributed data between 5.6 nm and 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m under the
assumption of a particle density of 1 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, which were calculated
using the FSCs originally assumed by the model and the FSCs obtained from the
measurements. The number of the compared plumes for each type and species is
presented by the number values in the legend.</p></caption>
          <?xmltex \igopts{width=241.848425pt}?><graphic xlink:href="https://www.atmos-chem-phys.net/15/5229/2015/acp-15-5229-2015-f10.png"/>

        </fig>

      <p><?xmltex \hack{\newpage}?>Significant differences between the model and the measurement results can be
seen for international running tankers (<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>40 %) and tug boats
(<inline-formula><mml:math display="inline"><mml:mo>+</mml:mo></mml:math></inline-formula>84 %). Even though only three tug boats were measured, they showed
significantly lower NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions than other ship types in the low-load
conditions in the ship channel of Neva Bay.</p>
      <p>The low values of measured NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factors for certain, very new,
vessels were observed already at IMO Tier 3 level. The measurements indicate
that certain, recently built vessels already operate following the IMO
tier 3 regulations. Other ships showing low NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions are known to
run with engines capable of using both gas and diesel. In the case of dual-fuel engines, low-load operation in STEAM leads to switch from gas mode to
diesel mode. The speed limit of 10 kn is already low enough to trigger
this behavior in the model and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factors defined by engine
rpm and IMO NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> curve is then applied.
<?xmltex \hack{\newpage}?></p>
      <p>The modeling of particulate matter emissions is complex due to the
uncertainties in assumptions about the FSC, engine load and the mass and
composition of the emitted particles used. Large differences between modeled and
measured emissions can be seen for particles in Fig. 10. The deviations found might be partly due to the assumed unity density
(see for example Virtanen et al., 2002, Petzold et al., 2008, Murphy et al., 2009, Barone et al., 2011, Kuwata et al., 2012, and
Pennington et al., 2013, for the typical range of
densities), the limited size range for the measured data and assumptions
made in STEAM. With respect to the latter, there are several uncertainty
sources regarding the modeling of the particulate matter emissions.</p>
      <p>First, the instantaneous main and auxiliary engine power level predictions
will have an impact on modeled engine loads. Load levels of engines, in
turn, will have an impact on calculated emission factors and instantaneous
values of specific fuel consumption, thus changing the mass-based emission
factors in the model. For the model, engine load and load balancing is more
straightforward for a single two-stroke main engine than for a setup of
several four-stroke main engines, in the case of which the number of active
main engines may vary depending on variable power needs of the vessel. A
comparison of the model and measured results for EF(PM) of ships using two-stroke engines did not show a significant improvement in this study.
Unfortunately, the lack of observations from the ships' engine rooms
regarding the operational state of the engines hinders a more detailed
analysis. However, it is unlikely that these uncertainties are the single
cause for the deviations between measured and modeled results of more than
100 %.</p>
      <p>Second, the FSC will have a major impact on the modeled PM emission factor.
In STEAM, the cheapest possible fuel (with higher sulfur content) is
assigned to vessels, defined by geographical limitations (SECA/non-SECA,
local legislation for port areas) and technical feasibility of using
residual fuel. A recalculation with the model using FSC from the
measurement of the individual ships as shown in the bottom plot in
Fig. 10 did not lead to a major improvement.</p>
      <p>Third, some differences between the modeled and measured results can be
explained by unknown parameters for certain domestic ships, for which
standard parameters for small vessels were used. Small vessels in domestic
operations do not need to undergo the IMO registry procedure and the level
of technical details of these vessels in STEAM database is low. For this
reason, small vessels are assigned the generic tugboat type, which is bound
to lead to inaccuracies in vessel performance and emissions calculations.</p>
      <p>Fourth, the conditions of experimental measurements, on which STEAM emission
factors for PM are based (see Jalkanen et al., 2012, for details), do not
necessarily correspond to the measurement conditions used in the plume
chasing approach used in the current work. The emission factors of fresh
exhaust are quite different from those of the aged plume and sample analysis
in laboratory conditions may have an impact on PM mass determination when
compared to in situ measurements. The aerosol chemistry after the emission
of the plume is not trivial, and considering that the plumes are already aged
by several minutes there are significant changes in number and mass of the
emitted particles. Direct comparison of PM results from plume chasing studies
with emission modeling would necessitate the use of PM emission factors
which represent fresh exhaust, and consecutive modeling should be done using
a plume model with a detailed description of aerosol processes. This was not
done during the current work, however, and it requires further study. It may
be necessary to develop separate ship emission modeling schemes for short-range studies (both in space and time) of aerosols and for regional scale
modeling, unless regional transport models can include relevant aerosol
physics modules describing gas/particle partitioning in a short timescale
(Robinson et al., 2007; Tian et al., 2014).</p>
      <p>It was clearly observed in the modeling results that the misallocation of
FSC for ships, especially for domestic traffic using low sulfur fuel, will
easily lead to SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and PM emission factors of which the latter are over
twice higher than what was measured in this work. However, the model does
not allow for higher fuel sulfur content for vessels than what is
allowed by current legislation unless the user assigns the fuel sulfur
content manually. Currently, there is no centralized registry for the
properties of fuel used in each vessel, making emission modeling
challenging for SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and PM. In this regard, the work reported improves
the knowledge of the fuel sulfur content of Baltic Sea shipping.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Summary and conclusions</title>
      <p>During two campaigns in summer 2011 and summer 2012, ship emissions in the
Gulf of Finland, especially in the Neva Bay area, were measured from various
platforms: boat, helicopter and from shore. Altogether 466 plumes of 311
individual vessels were sampled.</p>
      <p>The sampled plumes showed a bi-modal distribution of the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission
factors. Ships in the lower mode emitted in average
4.6 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula> and in the higher mode
18.2 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. It was observed that
locally operating ships like the fast ferries, Nevsky cargo ships,
Volgoneft tanker vessels and tugs generally emit less SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> than
domestically operating passenger and cargo ships. Passenger ships appeared
to be located significantly towards the upper end on the SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> emission factor scale
and entirely running on fuel with higher sulfur contents, around 1 %.
Measurements in 2011 showed compliance with the 1 % SECA sulfur limit in
90 % of the 255 observed plumes. In 2012, 97 % of the measurements of
211 plumes indicated compliance.</p>
      <p>The distribution of the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emission factor indicated a mono-modal
distribution around an average of 58 g<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mrow><mml:msub><mml:mi mathvariant="normal">NO</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:msub></mml:math></inline-formula> kg<inline-formula><mml:math display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">fuel</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>. This average was found to be around 12 % below the
values found in other studies, probably because of the low speed with low
engine loads which impact the emissions rate.</p>
      <p>The emission factor uncertainties of 21 % for SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and around 25 %
for NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> found are comparable to similar studies
(Alföldy et al., 2013).</p>
      <p>The particle measurements show that the main contribution to the particle
number for particle sizes between 5.6 nm and 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m comes from
particles below 65 nm. Around 70 % of the particle mass appears to be due
to particles below 300 nm.</p>
      <p>The conducted ground-based measurements provide a good overview about the
distribution of all passing vessels and about the general distribution of
emission factors at the measurement sites. Most ground-based measurements
were conducted at the ship passage between St. Petersburg and Kronstadt.
Many of the domestic and all of the international shipping vessels that travel between St. Petersburg and the Baltic pass this way.
Furthermore, these measurements were conducted over several days, where
both day and night traffic were observed.</p>
      <p>The strength of the helicopter-based measurements was that a greater sea
area could be covered and the emissions of more ships could be measured
within a short time period. The ships could be arbitrarily selected and inspected.
Further, it was possible to cross the same plume several times to decrease
uncertainty.</p>
      <p>The measured data was compared to modeled data using the STEAM model of the
Finnish Meteorological Institute. The result indicated that the assumed FSC
might be overestimated by the model for certain ship types, especially those
engaging in domestic traffic. Overall, the NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> emissions compared well
with the modeled results, while there is a significant difference concerning
the particle emissions which is only partially due to uncertainties in fuel
sulfur content assumptions made in STEAM and requires further evaluation.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/acp-15-5229-2015-supplement" xlink:title="zip">doi:10.5194/acp-15-5229-2015-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>The Swedish innovation agency Vinnova and the Swedish Environmental
Protection agency are acknowledged for financial support for the development
of the IGPS measurement system through the projects IGPS-2005-01835 and
IGPS-plius-2008-03884. The measurements campaigns in Russia were financially
supported by the Baltic Sea cooperation for reducing ship and port
emissions project, BSR InnoShip.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: R. Harley</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>Agrawal, H., Malloy, Q. G. J., Welch, W. A., Wayne Miller, J., and Cocker, D.
R.: In-use gaseous and particulate matter emissions from a modern ocean goingvessel, Atmos. Environ., 42, 5504–5510,
<ext-link xlink:href="http://dx.doi.org/10.1016/j.atmosenv.2008.02.053" ext-link-type="DOI">10.1016/j.atmosenv.2008.02.053</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib2"><label>2</label><mixed-citation>Alföldy, B., Lööv, J. B., Lagler, F., Mellqvist, J., Berg, N.,
Beecken, J., Weststrate, H., Duyzer, J., Bencs, L., Horemans, B., Cavalli,
F., Putaud, J.-P., Janssens-Maenhout, G., Csordás, A. P., Van Grieken,
R., Borowiak, A., and Hjorth, J.: Measurements of air pollution emission
factors for marine transportation in SECA, Atmos. Meas. Tech., 6, 1777–1791,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-1777-2013" ext-link-type="DOI">10.5194/amt-6-1777-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib3"><label>3</label><mixed-citation>AMSA (Australian Maritime Safety Authority): Protocol of 1997 to amend the
International Convention for the Prevention of Pollution from Ships, 1973, as
modified by the Protocol of 1978 relating thereto (MARPOL PROT 1997) Annex
VI, available at: <uri>https://imo.amsa.gov.au/public/parties/marpol97prot.html</uri> (last
access: 30 January 2015), 2014.</mixed-citation></ref>
      <ref id="bib1.bib4"><label>4</label><mixed-citation>Balzani Lööv, J. M., Alfoldy, B., Gast, L. F. L., Hjorth, J., Lagler,
F., Mellqvist, J., Beecken, J., Berg, N., Duyzer, J., Westrate, H., Swart, D.
P. J., Berkhout, A. J. C., Jalkanen, J.-P., Prata, A. J., van der Hoff, G.
R., and Borowiak, A.: Field test of available methods to measure remotely SOx
and NOx emissions from ships, Atmos. Meas. Tech., 7, 2597–2613,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-7-2597-2014" ext-link-type="DOI">10.5194/amt-7-2597-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib5"><label>5</label><mixed-citation>
Barone, T. L., Lall, A. A., Storey, J. M. E., Mulholland, G. W., Prikhodko,
V. Y., Frankland, J. H., Parks, J. E., and Zachariah, M. R.: Size-resolved
density measurements of particle emissions from an advanced combustion diesel
engine: Effect of aggregate morphology, Energy and Fuels, 25, 1978–1988,
2011.</mixed-citation></ref>
      <ref id="bib1.bib6"><label>6</label><mixed-citation>Beecken, J., Mellqvist, J., Salo, K., Ekholm, J., and Jalkanen, J.-P.:
Airborne emission measurements of SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> , NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> and particles from
individual ships using a sniffer technique, Atmos. Meas. Tech., 7,
1957–1968, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-7-1957-2014" ext-link-type="DOI">10.5194/amt-7-1957-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib7"><label>7</label><mixed-citation>
Borkowski, T., Kasyk, L., and Kowalak, P.: Assessment of ship's engine
effective power, fuel consumption and emission using the vessel speed,
Journal of KONES, 18, 31–39, 2011.</mixed-citation></ref>
      <ref id="bib1.bib8"><label>8</label><mixed-citation>Cappa, C. D., Williams, E. J., Lack, D. A., Buffaloe, G. M., Coffman, D.,
Hayden, K. L., Herndon, S. C., Lerner, B. M., Li, S.-M., Massoli, P.,
McLaren, R., Nuaaman, I., Onasch, T. B., and Quinn, P. K.: A case study into
the measurement of ship emissions from plume intercepts of the NOAA ship
<italic>Miller Freeman</italic>, Atmos. Chem. Phys., 14, 1337–1352,
<ext-link xlink:href="http://dx.doi.org/10.5194/acp-14-1337-2014" ext-link-type="DOI">10.5194/acp-14-1337-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib9"><label>9</label><mixed-citation>
Corbett, J. J., Fischbeck, P. S., and Pandis, S. N.: Global nitrogen and
sulfur inventories for oceangoing ships, J. Geophys. Res.-Atmos., 104,
3457–3470, 1999.</mixed-citation></ref>
      <ref id="bib1.bib10"><label>10</label><mixed-citation>
Corbett, J. J., Winebrake, J. J., Green, E. H., Kasibhatla, P., Eyring, V.,
and Lauer, A.: Mortality from ship emissions: A global assessment, Environ.
Sci. Technol., 41, 8512–8518, 2007.</mixed-citation></ref>
      <ref id="bib1.bib11"><label>11</label><mixed-citation>
Hallquist, Å. M., Fridell, E., Westerlund, J., and Hallquist, M.: Onboard
measurements of nanoparticles from a SCR-equipped marine diesel engine,
Environ. Sci. Technol., 47, 773–780, 2013.</mixed-citation></ref>
      <ref id="bib1.bib12"><label>12</label><mixed-citation>
Hering, S. V., Stolzenburg, M. R., Quant, F. R., O'Berreit, D. R., and Keady,
P. B.: A laminar-flow, water-based condensation particle counter (WCPC),
Aerosol. Sci. Tech., 39, 659–672, 2005.</mixed-citation></ref>
      <ref id="bib1.bib13"><label>13</label><mixed-citation>
Hinds, W. C.: Aerosol technology : properties, behavior, and measurement of
airborne particles, Wiley, New York, 1999.</mixed-citation></ref>
      <ref id="bib1.bib14"><label>14</label><mixed-citation>
IHS Global: IHS Maritime, Chemin de la Mairie, Perly, Geneva, Switzerland,
2014.</mixed-citation></ref>
      <ref id="bib1.bib15"><label>15</label><mixed-citation>Jalkanen, J. P. and Johansson,L.: Emissions from Baltic Sea shipping in 2012,
available at: <uri>http://www.helcom.fi/baltic-sea-trends/environment-fact-sheets/hazardous-substances/emissions-from-baltic-sea-shipping/</uri>
(last access: 28 August 2014), 2013.</mixed-citation></ref>
      <ref id="bib1.bib16"><label>16</label><mixed-citation>Jalkanen, J.-P., Brink, A., Kalli, J., Pettersson, H., Kukkonen, J., and
Stipa, T.: A modelling system for the exhaust emissions of marine traffic and
its application in the Baltic Sea area, Atmos. Chem. Phys., 9, 9209–9223,
<ext-link xlink:href="http://dx.doi.org/10.5194/acp-9-9209-2009" ext-link-type="DOI">10.5194/acp-9-9209-2009</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib17"><label>17</label><mixed-citation>Jalkanen, J.-P., Johansson, L., Kukkonen, J., Brink, A., Kalli, J., and
Stipa, T.: Extension of an assessment model of ship traffic exhaust emissions
for particulate matter and carbon monoxide, Atmos. Chem. Phys., 12,
2641–2659, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-12-2641-2012" ext-link-type="DOI">10.5194/acp-12-2641-2012</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib18"><label>18</label><mixed-citation>
Johnson, T., Caldow, R., Pöcher, A., Mirme, A., and Kittelson, D.: A new
electrical mobility particle sizer spectrometer for engine exhaust particle
measurements, SAE Technical Paper 2004-1-1341, 2004 SAE World Congress
Detroit (MI), United States, 2004.</mixed-citation></ref>
      <ref id="bib1.bib19"><label>19</label><mixed-citation>Jonsson, A. M., Westerlund, J., and Hallquist, M.: Size-resolved particle
emission factors for individual ships, Geophys. Res. Lett., 38, L13809,
<ext-link xlink:href="http://dx.doi.org/10.1029/2011GL047672" ext-link-type="DOI">10.1029/2011GL047672</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bib20"><label>20</label><mixed-citation>Kley, D. and McFarland, M.: Chemiluminescence detector for NO and NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>,
Atmos. Technol., 12, 63–69, 1980.</mixed-citation></ref>
      <ref id="bib1.bib21"><label>21</label><mixed-citation>
Krylov, B. S., Novikov, L. A., and Frank-Kamenetsky, D. A.: Opredeleniye
massy vrednykh (zagryaznyayushchikh) veshchestv, vybrasyvayemykh vodnym
transportom v atmosferu Sankt-Peterburga [Determining the mass of harmful
substances (pollutants) emitted into the atmosphere waterways of
St. Petersburg], Okhrana atmosfernogo vozdukha, Atmosfera [Air Protection.
Atmosphere], SRI Atmosphere, St. Petersburg, Russia, 1, 21, 2012.</mixed-citation></ref>
      <ref id="bib1.bib22"><label>22</label><mixed-citation>
Kuiken, K.: Diesel Engines for Ship Propulsion and Power Plants Vol 1, Target
Global Energy Training, Onnen, the Netherlands, 2008.</mixed-citation></ref>
      <ref id="bib1.bib23"><label>23</label><mixed-citation>Kuwata, M., Zorn, S. R., and Martin, S. T.: Using elemental ratios to predict
the density of organic material composed of carbon, hydrogen, and oxygen,
Environ. Sci. Technol., 46, 787–794, <ext-link xlink:href="http://dx.doi.org/10.1021/es202525q" ext-link-type="DOI">10.1021/es202525q</ext-link>, 2012.</mixed-citation></ref>
      <ref id="bib1.bib24"><label>24</label><mixed-citation>Lack, D. A., Cappa, C. D., Langridge, J., Bahreini, R., Buffaloe, G., Brock,
C., Cerully, K., Coffman, D., Hayden, K., Holloway, J., Lerner, B., Massoli,
P., Li, S. M., McLaren, R., Middlebrook, A. M., Moore, R., Nenes, A.,
Nuaaman, I., Onasch, T. B., Peischl, J., Perring, A., Quinn, P. K., Ryerson,
T., Schwartz, J. P., Spackman, R., Wofsy, S. C., Worsnop, D., Xiang, B., and
Williams, E.: Impact of fuel quality regulation and speed reductions on
shipping emissions: implications for climate and air quality, Environ. Sci.
Technol., 45, 9052–9060, <ext-link xlink:href="http://dx.doi.org/10.1021/es2013424" ext-link-type="DOI">10.1021/es2013424</ext-link>, 2011.</mixed-citation></ref>
      <ref id="bib1.bib25"><label>25</label><mixed-citation>Luke, W. T.: Evaluation of a commercial pulsed fluorescence detector for the
measurement of low-level SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations during the gas-phase sulfur
intercomparison experiment, J. Geophys. Res.-Atmos., 102, 16255–16265, 1997.</mixed-citation></ref>
      <ref id="bib1.bib26"><label>26</label><mixed-citation>
Mellqvist, J. and Berg, N.: Final Report to Vinnova: Identification of gross
polluting ships, RG Report No. 4, ISSN 1653 333X, Chalmers University of
Technology, Göteborg, Sweden, 2010.</mixed-citation></ref>
      <ref id="bib1.bib27"><label>27</label><mixed-citation>
Mellqvist, J., Beecken, J., Ekholm, J., and Salo, K.: Remote Compliance
Monitoring of Gas Emissions from Shipping to Enforce International Policies,
in preparation, 2015.</mixed-citation></ref>
      <ref id="bib1.bib28"><label>28</label><mixed-citation>MEPC: Marine Environment Protection Committee, Interim Guidelines for
Voluntary Ship CO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> Emission Indexing for Use in Trials, IMO, London,
United Kingdom, 2005.</mixed-citation></ref>
      <ref id="bib1.bib29"><label>29</label><mixed-citation>MEPC: Marine Environment Protection Committee, Amendments to the technical
code on control of emission of nitrogen oxides from marine diesel engines –
NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula> Technical Code, IMO, London, United Kingdom, 2008.</mixed-citation></ref>
      <ref id="bib1.bib30"><label>30</label><mixed-citation>Moldanová, J., Fridell, E., Popovicheva, O., Demirdjian, B., Tishkova,
V., Faccinetto, A., and Focsa, C.: Characterisation of particulate matter and
gaseous emissions from a large ship diesel engine, Atmos. Environ., 43,
2632–2641, <ext-link xlink:href="http://dx.doi.org/10.1016/j.atmosenv.2009.02.008" ext-link-type="DOI">10.1016/j.atmosenv.2009.02.008</ext-link>, 2009.</mixed-citation></ref>
      <ref id="bib1.bib31"><label>31</label><mixed-citation>Moldanová, J., Fridell, E., Winnes, H., Holmin-Fridell, S., Boman, J.,
Jedynska, A., Tishkova, V., Demirdjian, B., Joulie, S., Bladt, H., Ivleva, N.
P., and Niessner, R.: Physical and chemical characterisation of PM emissions
from two ships operating in European Emission Control Areas, Atmos. Meas.
Tech., 6, 3577–3596, <ext-link xlink:href="http://dx.doi.org/10.5194/amt-6-3577-2013" ext-link-type="DOI">10.5194/amt-6-3577-2013</ext-link>, 2013.</mixed-citation></ref>
      <ref id="bib1.bib32"><label>32</label><mixed-citation>
Murphy, S., Agrawal, H., Sorooshian, A., Padró, L. T., Gates, H., Hersey,
S., Welch, W. A., Jung, H., Miller, J. W., Cocker III, D. R., Nenes, A.,
Jonsson, H. H., Flagan, R. C., and Seinfeld, J. H.: Comprehensive
simultaneous shipboard and airborne characterization of exhaust from a modern
container ship at sea, Environ. Sci. Technol., 43, 4626–4640, 2009.</mixed-citation></ref>
      <ref id="bib1.bib33"><label>33</label><mixed-citation>
O'Keefe, A. and Deacon, D. A. G.: Cavity ring-down optical spectrometer for
absorption measurements using pulsed laser sources, Rev. Sci. Instrum., 59,
2544–2551, 1988.</mixed-citation></ref>
      <ref id="bib1.bib34"><label>34</label><mixed-citation>Pennington, M. R., Bzdek, B. R., DePalma, J. W., Smith, J. N., Kortelainen,
A.-M., Hildebrandt Ruiz, L., Petäjä, T., Kulmala, M., Worsnop, D. R.,
and Johnston, M. V.: Identification and quantification of particle growth
channels during new particle formation, Atmos. Chem. Phys., 13, 10215–10225,
<ext-link xlink:href="http://dx.doi.org/10.5194/acp-13-10215-2013" ext-link-type="DOI">10.5194/acp-13-10215-2013</ext-link>, 2013.
</mixed-citation></ref><?xmltex \hack{\newpage}?>
      <ref id="bib1.bib35"><label>35</label><mixed-citation>Petzold, A., Hasselbach, J., Lauer, P., Baumann, R., Franke, K., Gurk, C.,
Schlager, H., and Weingartner, E.: Experimental studies on particle emissions
from cruising ship, their characteristic properties, transformation and
atmospheric lifetime in the marine boundary layer, Atmos. Chem. Phys., 8,
2387–2403, <ext-link xlink:href="http://dx.doi.org/10.5194/acp-8-2387-2008" ext-link-type="DOI">10.5194/acp-8-2387-2008</ext-link>, 2008.</mixed-citation></ref>
      <ref id="bib1.bib36"><label>36</label><mixed-citation>Pirjola, L., Pajunoja, A., Walden, J., Jalkanen, J.-P., Rönkkö, T.,
Kousa, A., and Koskentalo, T.: Mobile measurements of ship emissions in two
harbour areas in Finland, Atmos. Meas. Tech., 7, 149–161,
<ext-link xlink:href="http://dx.doi.org/10.5194/amt-7-149-2014" ext-link-type="DOI">10.5194/amt-7-149-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib37"><label>37</label><mixed-citation>Robinson, A. L., Donahue, N. M., Shrivastava, M. K., Weitkamp, E. A., Sage,
A. M., Grieshop, A. P., Lane, T. E., Pierce, J. R., and Pandis, S. N.:
Rethinking organic aerosols: Semivolatile emissions and photochemical aging,
Science, 315, 1259–1262, <ext-link xlink:href="http://dx.doi.org/10.1126/science.1133061" ext-link-type="DOI">10.1126/science.1133061</ext-link>, 2007.</mixed-citation></ref>
      <ref id="bib1.bib38"><label>38</label><mixed-citation>
Schlager, H., Baumann, R., Lichtenstern, M., Petzold, A., Arnold, F.,
Speidel, M., Gurk, C., and Fischer, H.: Aircraft-based Trace Gas Measurements
in a Primary European Ship Corridor, TAC-Conference, Oxford, UK, 26–29 June 2006, 83–88,
2006.</mixed-citation></ref>
      <ref id="bib1.bib39"><label>39</label><mixed-citation>
Starcrest: Starcrest Consulting Group LLC, Port of Long Angeles: Inventory
Air Emissions – 2011, Long Beach (CA), USA, 2012.</mixed-citation></ref>
      <ref id="bib1.bib40"><label>40</label><mixed-citation>Tian, J., Riemer, N., West, M., Pfaffenberger, L., Schlager, H., and Petzold,
A.: Modeling the evolution of aerosol particles in a ship plume using
PartMC-MOSAIC, Atmos. Chem. Phys., 14, 5327–5347,
<ext-link xlink:href="http://dx.doi.org/10.5194/acp-14-5327-2014" ext-link-type="DOI">10.5194/acp-14-5327-2014</ext-link>, 2014.</mixed-citation></ref>
      <ref id="bib1.bib41"><label>41</label><mixed-citation>
UNCTAD: Review of Maritime Transport 2012, United Nations Publication,
ISSN 0566-7682, ISBN: 978-92-1-112860-4, e-ISBN: 978-92-1-055950-8, 2013.</mixed-citation></ref>
      <ref id="bib1.bib42"><label>42</label><mixed-citation>
Virtanen, A., Ristimäki, J., Marjamäki, M., Vaaraslahti, K.,
Keskinen, J., and Lappi, M.: Effective density of diesel exhaust particles
as a function of size, SAE Technical Paper 2002-01-0056, 2002 SAE World
Congress Detroit (MI), United States, 2002.</mixed-citation></ref>
      <ref id="bib1.bib43"><label>43</label><mixed-citation>Williams, E. J., Lerner, B. M., Murphy, P. C., Herndon, S. C., and Zahniser,
M. S.: Emissions of NO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mi>x</mml:mi></mml:msub></mml:math></inline-formula>, SO<inline-formula><mml:math display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>, CO, and HCHO from commercial marine
shipping during Texas Air Quality Study (TexAQS) 2006, J. Geophys.
Res.-Atmos., 114, D21306, <ext-link xlink:href="http://dx.doi.org/10.1029/2009JD012094" ext-link-type="DOI">10.1029/2009JD012094</ext-link>, 2009.</mixed-citation></ref>

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    </article>
