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

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-17-10937-2017</article-id><title-group><article-title>Particulate sulfur in the upper troposphere and lowermost stratosphere
– sources and climate forcing</article-title>
      </title-group><?xmltex \runningtitle{Particulate sulfur in the upper troposphere and lowermost stratosphere}?><?xmltex \runningauthor{B. G. Martinsson et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Martinsson</surname><given-names>Bengt G.</given-names></name>
          <email>bengt.martinsson@nuclear.lu.se</email>
        <ext-link>https://orcid.org/0000-0003-2230-5932</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Friberg</surname><given-names>Johan</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7971-4967</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sandvik</surname><given-names>Oscar S.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-9782-991X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Hermann</surname><given-names>Markus</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5124-1571</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>van Velthoven</surname><given-names>Peter F. J.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-7625-5753</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Zahn</surname><given-names>Andreas</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Division of Nuclear Physics, Lund University, Lund, Sweden</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Leibniz Institute for Tropospheric Research, Leipzig, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Royal Netherlands Meteorological Institute (KNMI), De Bilt, the
Netherlands</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Institute of Meteorology and Climate Research, Institute of
Technology, Karlsruhe, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Bengt G. Martinsson (bengt.martinsson@nuclear.lu.se)</corresp></author-notes><pub-date><day>15</day><month>September</month><year>2017</year></pub-date>
      
      <volume>17</volume>
      <issue>18</issue>
      <fpage>10937</fpage><lpage>10953</lpage>
      <history>
        <date date-type="received"><day>21</day><month>December</month><year>2016</year></date>
           <date date-type="rev-request"><day>23</day><month>January</month><year>2017</year></date>
           <date date-type="rev-recd"><day>11</day><month>August</month><year>2017</year></date>
           <date date-type="accepted"><day>15</day><month>August</month><year>2017</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 3.0 Unported License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/3.0/">https://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>This study is based on fine-mode aerosol samples collected in the
upper troposphere (UT) and the lowermost stratosphere (LMS) of the Northern
Hemisphere extratropics during monthly intercontinental flights at
8.8–12 km altitude of the IAGOS-CARIBIC platform in the time period
1999–2014. The samples were analyzed for a large number of chemical elements
using the accelerator-based methods PIXE (particle-induced X-ray emission)
and PESA (particle elastic scattering analysis). Here the particulate sulfur
concentrations, obtained by PIXE analysis, are investigated. In addition, the
satellite-borne lidar aboard CALIPSO is used to study the stratospheric
aerosol load. A steep gradient in particulate sulfur concentration extends
several kilometers into the LMS, as a result of increasing dilution towards
the tropopause of stratospheric, particulate sulfur-rich air. The stratospheric air is diluted with tropospheric air, forming the extratropical transition layer (ExTL). Observed
concentrations are related to the distance to the dynamical tropopause. A
linear regression methodology handled seasonal variation and impact from
volcanism. This was used to convert each data point into stand-alone estimates
of a concentration profile and column concentration of particulate sulfur in
a 3 km altitude band above the tropopause. We find distinct responses to
volcanic eruptions, and that this layer in the LMS has a significant
contribution to the stratospheric aerosol optical depth and thus to its
radiative forcing. Further, the origin of UT particulate sulfur shows
strong seasonal variation. We find that tropospheric sources dominate during
the fall as a result of downward transport of the Asian tropopause aerosol
layer (ATAL) formed in the Asian monsoon, whereas transport down from the
Junge layer is the main source of UT particulate sulfur in the first half of
the year. In this latter part of the year, the stratosphere is the clearly
dominating source of particulate sulfur in the UT during times of volcanic
influence and under background conditions.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The global mean surface temperature has increased considerably in the last 2
years (NOAA, 2016), which followed on a 15-year period with
slow temperature evolution. CMIP5 (Coupled Model Intercomparison Project)
models predict stronger-than-observed temperature increases in this period
(Fyfe et al., 2013, 2016). Reasons for these differences were sought, and the
Interdecadal Pacific Oscillation connected with increased subduction and
upwelling (England et al., 2014; Meehl and Teng, 2014), variations in
volcanic aerosol (Solomon et al., 2011; Santer et al., 2014) and solar (Myhre
et al., 2013) forcings were identified as main causes of the discrepancies.
These phenomena are all elements of natural climate variability, thus
highlighting the importance of these influences for assessing the human
impact on the climate (Ramanathan and Feng, 2008).</p>
      <p>Air from the tropical troposphere containing aerosol precursor gases is
lifted into the tropical stratosphere in the Brewer–Dobson circulation.
Carbonyl sulfide (OCS) is the most abundant sulfur-containing gas in the
atmosphere. When lofted into the stratosphere, OCS is converted into sulfur
dioxide (SO<inline-formula><mml:math id="M1" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> at approximately 25 km altitude aided by UV radiation
(Crutzen, 1976) and next into sulfuric acid, giving rise to the
background stratospheric aerosol layer. The upward tropical flow is connected
with a downward flow in the extratropics, where stratospheric air flows back
to the troposphere.</p>
      <p>The stratospheric aerosol concentration varies strongly due to volcanic
influence, from events like the strong 1991 Mt. Pinatubo eruption, inducing
negative radiative forcing in excess of 1 W m<inline-formula><mml:math id="M2" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> (McCormick et al.,
1995), to close to background conditions at around the turn of the millennium
(Bauman et al., 2003; Martinsson et al., 2005). Overall, anthropogenic
influence on stratospheric aerosol is small compared to that from volcanism
(Neely III et al., 2013). Recent volcanic eruptions, such as in 2008 and 2009 of
the Kasatochi and Sarychev in the extratropics and in 2011 of the Nabro in
the tropics, significantly altered stratospheric aerosol (Vernier et al.,
2011a; Bourassa et al., 2012). These eruptions also had a profound impact on
the Northern Hemisphere lowermost stratosphere (LMS; Martinsson et al.,
2009) and the global aerosol optical depth (AOD) of the stratosphere
(Andersson et al., 2015). After reaching the LMS, stratospheric aerosol
is transported to the upper troposphere (UT). A recent study indicates that
volcanic aerosol also has an indirect climate effect by affecting the
reflectance of cirrus clouds in the UT (Friberg et al., 2015).</p>
      <p>Upper troposphere particulate sulfur, in addition, has tropospheric sources. In the
tropics, convection lofts aerosol and aerosol precursor gases from low
altitudes into the UT (Hess, 2005). During the monsoon season, primarily the
Asian monsoon, appreciable amounts of aerosol and gaseous aerosol precursors
are lifted to the tropopause region, extending from the UT to approximately
420 K potential temperature in the stratosphere, forming the Asian tropopause
aerosol layer (ATAL; Vernier et al., 2011b). The ATAL is a seasonal and
regional phenomenon which, according to atmospheric modeling, is strongly
connected with Asian pollution sources (Neely III et al., 2014). In the
extratropics, warm conveyor belts (WCBs; Stohl, 2001) and deep convection are
the main lofting channels, the latter especially in the summer season. Large
amounts of pollutants are transported long-range across the Pacific and
Atlantic oceans, where sources are affecting the background concentrations of
various species over remote continents. This transport is most efficient
above the boundary layer in the pressure interval 700–900 hPa (Luan and
Jaeglé, 2013). Warm conveyor belts reaching the UT have their maximum frequency in the
winter (Eckhardt et al., 2004) and transport of boundary layer air into the
LMS maximizes in the winter and spring (Škerlak et al., 2014), whereas deep
convection dominates in the summer (Kiley and Fuelberg, 2006).</p>
      <p>Aerosol particles in the UT and LMS contain a large fraction of sulfur
compounds, mostly sulfates (Dibb et al., 2000; Martinsson et al., 2001; Xu et
a., 2001; Kojima et al., 2004). These particles also contain a considerable
fraction of carbonaceous aerosol (Murphy et al., 1998; Nguyen et al., 2008;
Martinsson et al., 2009), of which a minor fraction is black carbon (Schwarz
et al., 2010; Friberg et al., 2014). In some periods, particularly during
spring, crustal particles are also found in this part of the atmosphere
(Papaspiropoulos et al., 2002).</p>
      <p>In this study the concentration of particulate sulfur in the UT and LMS is
investigated based on aerosol samples collected from the IAGOS-CARIBIC
platform in the time period 1999–2014. In this period the UT and LMS aerosol
was affected by volcanism from several eruptions as demonstrated in our
previous studies based on this data set (Martinsson et al., 2009, 2014;
Andersson et al., 2013, 2015; Friberg et al., 2014, 2015). The IAGOS-CARIBIC
aerosol elemental concentration measurements from the LMS are taken in strong
concentration gradients that are affected by mixing tropospheric air into the
lowest part of the LMS. Each measurement flight results in a small number of
samples, being insufficient to reconstruct the gradient. Therefore, we have
frequently relied on concurrent IAGOS-CARIBIC measurements, mostly by
relating the particulate sulfur measurements to ozone concentrations to
express, for example, volcanic influence on the aerosol concentration (Martinsson et
al., 2009). Satellite-based measurements do not usually provide specific
chemical information about aerosol particles. This lack of chemical
information in, for example, lidar measurements can cause a bias in LMS particle
concentrations close to the extratropical tropopause from non-volcanic
species such as crustal particles and enhanced signal caused by particle
hygroscopic growth. Here we present stand-alone estimates of the stratospheric
sulfur aerosol in terms of mass concentration profiles and column
concentrations based on a new method, which is then used to study the AOD of
the lowest part of Northern Hemisphere LMS and its radiative forcing. This
study also comprises a discussion on the relative importance of stratospheric
and the tropospheric sources to the UT of particulate sulfur, seasonal
dependences and different modes of tropospheric transport involved.</p>
</sec>
<sec id="Ch1.S2">
  <title>Methods</title>
<sec id="Ch1.S2.SS1">
  <title>Sampling, analysis and classification</title>
      <p>This study is based on measurements of particulate sulfur taken from the
IAGOS-CARIBIC platform (Brenninkmeijer et al., 2007;
<uri>www.caribic-atmospheric.com/</uri>), where the atmosphere is studied using
modified passenger aircraft (March 1999–April 2002: Boeing 767–300 ER from
LTU International Airways; May 2005–present: Airbus 340-600 from
Lufthansa) during monthly sets of usually four intercontinental flights. A
large number of trace gases and aerosol parameters are measured from this
platform during flights in the altitude range 8.8–12 km, including gaseous
and condensed water, O<inline-formula><mml:math id="M3" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:math></inline-formula>, CO, NO/NO<inline-formula><mml:math id="M4" display="inline"><mml:msub><mml:mi/><mml:mi>y</mml:mi></mml:msub></mml:math></inline-formula>, volatile organic compounds (VOCs), greenhouse gases,
halo-carbons, mercury, particle number concentrations, size distributions and
elemental concentrations (Brenninkmeijer et al., 2007; Hermann et al., 2003;
Schuck et al., 2009; Baker et al., 2010; Oram et al., 2012; Zahn et al.,
2012; Martinsson et al., 2014; Dyroff et al., 2015; Slemr et al., 2016;
Hermann et al., 2016).</p>
      <p>Aerosol sampling from the IAGOS-CARIBIC platform in the time period
1999–2014 resulted in 1198 samples analyzed for aerosol elemental
concentrations. The measurements were mainly taken in the Northern Hemisphere
(NH) extratropics and the tropics, while only a small fraction of the samples
were taken in the Southern Hemisphere. Here the focus is on the extratropical
LMS and UT of the NH. Aerosol particles with aerodynamic diameter in the
range 0.08–2 <inline-formula><mml:math id="M5" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m were collected with a multi-channel impactor with
a collection efficiency of 97 % <inline-formula><mml:math id="M6" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 4 % (Nguyen et al., 2006).
The typical time required to collect one sample is 100 min.
Accelerator-based methods were used to analyze the collected samples with
respect to elemental concentrations, using particle-induced X-ray emission
(PIXE) to analyze the concentration of elements with atomic number larger
than 15 (Martinsson et al., 2001). Concentrations of hydrogen, carbon,
nitrogen and oxygen were investigated using particle elastic scattering analysis
(PESA; Nguyen and Martinsson, 2007). Here the particulate sulfur
concentrations are used. The accuracy of the analyses is estimated to be
10 % and the combined uncertainty in sampling and analysis is estimated
to be 12 %. Further analytical details are found in Martinsson et
al. (2014). Finally, the concentration of particulate sulfur is mostly given
as a mixing ratio by normalization to STP (standard temperature, 273.15 K,
and pressure, 101 300 Pa). When computing column concentration and AOD of
the lowest 3 km of the LMS, the STP concentrations are converted into volume
concentrations using the pressure and temperature of the measurement, and the
altitude dependence in the LMS of the molar volume obtained from ECMWF
(European Centre for Medium-Range Weather Forecasts).</p>
      <p>The dynamical tropopause (Gettelman et al., 2011) at the potential vorticity
(PV) of 1.5 PVU (potential vorticity units;
1 PVU <inline-formula><mml:math id="M7" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 10<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> K m<inline-formula><mml:math id="M9" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> kg<inline-formula><mml:math id="M10" 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> s<inline-formula><mml:math id="M11" display="inline"><mml:mrow><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> was used to classify
samples with respect to tropospheric and stratospheric air. The PV along the
flight track was obtained from archived analyses from ECMWF with a resolution
of 1 <inline-formula><mml:math id="M12" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1<inline-formula><mml:math id="M13" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> in the horizontal and 91 vertical hybrid
sigma-pressure model levels. The PV was interpolated linearly by latitude,
longitude, log pressure and time to the position of the IAGOS-CARIBIC
aircraft.</p>
</sec>
<sec id="Ch1.S2.SS2">
  <title>Altitude</title>
      <p>The UT usually holds significantly lower particulate sulfur concentration
than the LMS. Combined with bi-directional exchange of tropospheric and
stratospheric air across the tropopause, this leads to a gradient of
increasing concentration in the LMS from the tropopause. In addition, the
concentration of particulate sulfur in the LMS varies due to the influence
from volcanism (Martinsson et al., 2009), which has been shown to cause
significant radiative forcing (Andersson et al., 2015). In order to study the
particulate sulfur gradient in the LMS, fine aerosol elemental concentration
measurements from the IAGOS-CARIBIC platform were used in relation to the
distance between measurement position and the tropopause (<inline-formula><mml:math id="M14" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>):
            <disp-formula id="Ch1.E1" content-type="numbered"><mml:math id="M15" display="block"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mtext>a</mml:mtext></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mtext>tp</mml:mtext></mml:msub><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M16" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mtext>a</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mtext>tp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> are the altitudes of the aircraft and
the tropopause. <inline-formula><mml:math id="M18" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mtext>tp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> refer to the dynamical tropopause of 1.5 PVU,
which is a low limit to ensure that very little LMS air will be considered as
tropospheric. The <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mtext>tp</mml:mtext></mml:msub></mml:mrow></mml:math></inline-formula> was obtained from the ERA-Interim data of
ECMWF, whereas the altitude of the aircraft was obtained from pressure
measurement which was converted into altitude using the ECMWF data. The
position of the tropopause was obtained using the aircraft as the starting
position. If the position is in the UT, i.e., it has a potential vorticity lower
than 1.5 PVU, then the tropopause is found by searching upwards in the potential
vorticity field. Tropopause folds in a small number of cases induce multiple
tropopauses in the vertical direction, complicating the analysis of the
stratospheric samples. In order to handle that problem, searches were
undertaken both upwards and downwards to find the tropopause closest to the
aircraft. That distance is assigned a positive value irrespective of whether
the tropopause is below or above the aircraft, because positive sign
indicates stratospheric air.</p>
      <p>The study of the aerosol concentration gradient deals primarily with the LMS.
The data set, however, contains observations both in the LMS and the UT and
one sample sometimes contains particles from both regions. These
concentrations are connected by the exchange across the tropopause. Figure 1
shows the samples that were taken in the UT during the entire sampling time.
It is clear that the dependence on the distance from the tropopause is
non-existent (<inline-formula><mml:math id="M20" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.02</mml:mn></mml:mrow></mml:math></inline-formula>). Further evaluation (not shown) by
normalization to seasonal average concentrations (<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.01</mml:mn></mml:mrow></mml:math></inline-formula>) or to
individual groups of concentration data that will be explained below (<inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.002</mml:mn></mml:mrow></mml:math></inline-formula>) did not reveal a dependence of the UT particulate sulfur
concentration on the distance from the tropopause either. It should be
noted that the variability in distance to the tropopause is mainly
caused by variability in the altitude of the tropopause because the altitude
of the measurement aircraft is fairly constant. This implies that the
distance from the tropopause in Fig. 1 does not reflect the sampling
altitude, and hence not an altitude-typical degree of cloud processing. The
distance to the tropopause for some summer measurements was very large due
to the seasonality of the position of the tropics. Approximately one-third of
all stratospheric air masses transported across the extratropical tropopause
reach the 500 hPa level of the atmosphere, corresponding to approximately
5000 m transport, in 4–5 days (Škerlak et al., 2014). This illustrates that
the exchange from the stratosphere goes deep into the troposphere in a rather short time. Based on
these observations and arguments, the UT particulate sulfur concentration is
considered independent of the distance from the tropopause under presented
conditions, and thus indicative of the particulate sulfur concentrations of
the air mixed into the LMS.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>Upper tropospheric particulate sulfur concentration related to
distance from the tropopause, where the symbols indicate sampling month.</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f01.jpg"/>

        </fig>

      <p>The time required to collect one sample was subdivided into 10 time
intervals of equal length, where <inline-formula><mml:math id="M23" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> was computed along the flight route. For
samples taken in the LMS, the sample was represented by the average distance
to the tropopause of the 10 time intervals. Those time intervals when the
sampling was undertaken in the UT, i.e., with <inline-formula><mml:math id="M24" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M25" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0, <inline-formula><mml:math id="M26" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> was set to
zero, since no <inline-formula><mml:math id="M27" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> dependence of the UT particulate sulfur concentration
could be identified. This implies that samples collected entirely in the UT
are found at <inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>. Some of the samples were collected both in the LMS and
in the UT. In these cases, the average <inline-formula><mml:math id="M29" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> over the 10 time intervals of
each sample was computed with all UT parts of a sample set to <inline-formula><mml:math id="M30" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>. That
way all samples could be utilized to study the particulate sulfur
concentration in the LMS.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <title>Methodology to evaluate the particulate sulfur gradient around the
tropopause</title>
      <p>The particulate sulfur concentration in the LMS is investigated using linear
regression in two steps. To that end we need to consider that the LMS shows
a seasonal dependence induced by variability in stratospheric circulation
and exchange across the tropopause over the year. Within one season
differences between years can be large, mainly due to varying influence from
volcanism. Further, the onset of volcanic influence on the particulate
sulfur concentration can cause large variability within the season in the
same year, and patchiness of young volcanic clouds can further affect the
data analysis.</p>
      <p>This study was limited to samples taken north of 30<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, where in
total 765 samples are available. The highest latitude of sampling was
77<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and 90 % of the samples (5 % removed each side) were
taken in the range 32–64<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. Most of the LMS samples (95 %)
were taken within 3000 m from the tropopause. In terms of altitude, the
results of this study therefore can be considered representative of the range
0–3000 m above the tropopause.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2" specific-use="star"><caption><p><bold>(a)</bold> Cumulative frequency of the coefficient of determination
(<inline-formula><mml:math id="M34" 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:mrow></mml:math></inline-formula> of ordinary linear regression (OLR) between particulate sulfur
concentration and distance from the tropopause of the 52 data groups used in
this study. <bold>(b, c)</bold> Comparison of slope (Fig. 2b) and offset <bold>(c)</bold> between a
square root transformed dependent variable and both OLR and forced linear
regression.</p></caption>
          <?xmltex \igopts{width=392.648031pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f02.jpg"/>

        </fig>

      <p>A large number of measurements is needed to obtain high statistical
significance. For that, data averaged over 3 months were used. However,
to allow for exchange of data in the analyses in order to test the stability
of the results, as well as catch smooth seasonal variations in the upper troposphere–lower stratosphere (UTLS), a
seasonal overlapping technique is used. This technique uses 3-month seasons
shifted by 1 month; e.g., the season MAM is followed by a season
AMJ, where data from April and May are used in both “seasons”. Data from one
season were grouped with respect to concentration levels of the different
years, resulting in 4 to 5 groups of data for each season, and in total 52
groups of data from the 12 seasons were analyzed. Some data were excluded
from these analyses, which reduced the number of samples from 765 to 694. Of the
excluded 71 samples, 60 pertained to periods when fresh volcanism induced
strong patchiness in the particulate sulfur concentration. Eleven samples
were considered outliers for other reasons, e.g., single samples affected by
volcanism during a season or recent up-transport from strongly polluted
regions. The remaining data of each year were tested for systematical
differences. Those years where the data overlapped in particulate sulfur by
altitude above the tropopause space were grouped together. This way, groups
with varying degrees of volcanic influence were formed. Groups typical of
“background” conditions were primarily based on data obtained during the
1999–2002 period characterized by low volcanic influence on the
stratospheric aerosol (Bauman et al., 2003; Deshler, 2008) and data
from mid-2013 to mid-2014, when the LMS was back to near-background conditions
in the NH extratropics; see Table 1 for relevant volcanic eruptions. Another
period that we will return to later is mid-2005 to mid-2008, when the
stratosphere was affected by three tropical eruptions in 2005–2006: Manam,
Soufriere Hills and Rabaul (Vernier et al., 2009), which also affected the NH
LMS (Friberg et al., 2014). There was some variability during these years,
implying that years were not always grouped together. They could
be grouped with other years; e.g., 2011 and 2013 often had similar
concentrations and gradients during the winter and spring seasons. These
groups were handled individually in the regression procedures described next,
but in a context of the discussion section these groups of “moderate
influence from tropical volcanism” were averaged to describe the UT aerosol
along with the “background” group described above.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><caption><p>Most significant volcanic eruptions for the aerosol concentration in
the Northern Hemisphere LMS in the time period studied.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.97}[.97]?><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1">Volcano</oasis:entry>  
         <oasis:entry colname="col2">Date</oasis:entry>  
         <oasis:entry colname="col3">Lat, long</oasis:entry>  
         <oasis:entry colname="col4">SO<inline-formula><mml:math id="M41" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (Tg)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Manam</oasis:entry>  
         <oasis:entry colname="col2">27 Jan 2005</oasis:entry>  
         <oasis:entry colname="col3">4<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 145<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>  
         <oasis:entry colname="col4">0.1<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Soufriere Hills</oasis:entry>  
         <oasis:entry colname="col2">20 May 2006</oasis:entry>  
         <oasis:entry colname="col3">17<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 62<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>  
         <oasis:entry colname="col4">0.2<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Rabaul</oasis:entry>  
         <oasis:entry colname="col2">7 Oct 2006</oasis:entry>  
         <oasis:entry colname="col3">4<inline-formula><mml:math id="M48" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 152<inline-formula><mml:math id="M49" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>  
         <oasis:entry colname="col4">0.2<inline-formula><mml:math id="M50" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Jebel at Tair</oasis:entry>  
         <oasis:entry colname="col2">30 Sep 2007</oasis:entry>  
         <oasis:entry colname="col3">16<inline-formula><mml:math id="M51" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 42<inline-formula><mml:math id="M52" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>  
         <oasis:entry colname="col4">0.1<inline-formula><mml:math id="M53" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Okmok</oasis:entry>  
         <oasis:entry colname="col2">12 Jul 2008</oasis:entry>  
         <oasis:entry colname="col3">53<inline-formula><mml:math id="M54" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 168<inline-formula><mml:math id="M55" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>  
         <oasis:entry colname="col4">0.1<inline-formula><mml:math id="M56" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Kasatochi</oasis:entry>  
         <oasis:entry colname="col2">7 Aug 2008</oasis:entry>  
         <oasis:entry colname="col3">52<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 176<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>  
         <oasis:entry colname="col4">1.7<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Redoubt</oasis:entry>  
         <oasis:entry colname="col2">23 Mar 2009</oasis:entry>  
         <oasis:entry colname="col3">60<inline-formula><mml:math id="M60" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153<inline-formula><mml:math id="M61" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>  
         <oasis:entry colname="col4">0.1<inline-formula><mml:math id="M62" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Sarychev</oasis:entry>  
         <oasis:entry colname="col2">12 Jun 2009</oasis:entry>  
         <oasis:entry colname="col3">48<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153<inline-formula><mml:math id="M64" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>  
         <oasis:entry colname="col4">1.2<inline-formula><mml:math id="M65" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">e</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Grimsvötn</oasis:entry>  
         <oasis:entry colname="col2">21 May 2011</oasis:entry>  
         <oasis:entry colname="col3">64<inline-formula><mml:math id="M66" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 17<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W</oasis:entry>  
         <oasis:entry colname="col4">0.4<inline-formula><mml:math id="M68" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">f</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Nabro</oasis:entry>  
         <oasis:entry colname="col2">12 Jun 2011</oasis:entry>  
         <oasis:entry colname="col3">13<inline-formula><mml:math id="M69" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 42<inline-formula><mml:math id="M70" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E</oasis:entry>  
         <oasis:entry colname="col4">1.5<inline-formula><mml:math id="M71" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">f</mml:mi></mml:msup></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table><?xmltex \begin{scaleboxenv}{.97}[.97]?><table-wrap-foot><p><inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">a</mml:mi></mml:msup></mml:math></inline-formula> Prata and Bernardo (2007).
<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">b</mml:mi></mml:msup></mml:math></inline-formula> Carn and Prata (2010).
<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">c</mml:mi></mml:msup></mml:math></inline-formula> Thomas et al. (2011).
<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">d</mml:mi></mml:msup></mml:math></inline-formula> Brühl et al. (2015).
<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">e</mml:mi></mml:msup></mml:math></inline-formula> Haywood et al. (2010).
<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">f</mml:mi></mml:msup></mml:math></inline-formula> Clarisse et al. (2012).</p></table-wrap-foot><?xmltex \end{scaleboxenv}?></table-wrap>

      <p>First linear vertical concentration gradients of particulate sulfur in the
lower LMS was calculated. Ordinary linear regression (OLR) was undertaken for
the 52 groups of data mentioned above of particulate sulfur concentration as
a function of the altitude above the tropopause. Figure 2a shows the
cumulative frequency of the coefficient of determination (<inline-formula><mml:math id="M72" 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:mrow></mml:math></inline-formula> of the 52
OLRs undertaken. <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> spans 0.48 to 0.95, 72 % of the groups having
<inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:msup><mml:mi>R</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> exceeding 0.6 and 50 % exceeding 0.66. The deviations from the
OLR models consists of scatter that does not show any trends.</p>
      <p>When investigating the variance of the dependent variable (the particulate
sulfur concentration, <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> along the independent variable
(altitude above the tropopause, <inline-formula><mml:math id="M76" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>) it is clear that the variance of
<inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> increases with increasing <inline-formula><mml:math id="M78" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>. This heteroscedastic nature
of the data, which is shared by most natural science data sets, could
unfavorably affect in particular the offset of the OLR. In order to further
investigate the effects of this problem, two variable transformations of the
dependent variable were tested: logarithmic and square root transformations.
The logarithmic transformation turned the problem around,
i.e., the logarithm of <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> has large variance for small <inline-formula><mml:math id="M80" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> and
small variance for large <inline-formula><mml:math id="M81" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>. The square root transformation of
<inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, on the other hand, shows rather constant variance along the
<inline-formula><mml:math id="M83" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> axis, thus making this transformation more suitable for regression. The
transformation <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msubsup><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:msqrt></mml:mrow></mml:math></inline-formula> was applied
to the data. As mentioned, <inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M86" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula> have a linear
relationship implying that the following expression should be minimized with
respect to slope (<inline-formula><mml:math id="M87" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>) and offset (<inline-formula><mml:math id="M88" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>): <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:msubsup><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>-</mml:mo><mml:msqrt><mml:mrow><mml:mi>a</mml:mi><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:msqrt><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula>. This results in rather tedious expressions that we solved numerically
for all the 52 data groups. Figure 2b and c show comparisons between the
slopes and the offsets obtained by the square root transformed regression
results and the OLRs. It is clear that the heteroscedastic nature of the data
causes large deviations, especially in the offset.</p>
      <p>Yet another transformation, based on forcing the regression to comply with
the data for small <inline-formula><mml:math id="M90" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>, was investigated. To that end, the average
concentration (<inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> of the data points closest to the
tropopause at the average distance <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the tropopause was formed.
<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> of the 52 data groups is on average based on 13
measurements, the minimum being 5, and the average <inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is 88 m and the
largest is 273 m. The data were transformed linearly to place
<inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the origin by forming
<inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msubsup><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M98" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M99" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M100" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M101" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M102" display="inline"><mml:mrow><mml:msup><mml:mi>Z</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>=</mml:mo><mml:mi>Z</mml:mi><mml:mo>-</mml:mo><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> followed by linear regression forced through the origin,
i.e., C<inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msubsup><mml:mi/><mml:mi mathvariant="normal">S</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:msup><mml:mi>Z</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>. Finally, the regression results are
transformed back to the form <inline-formula><mml:math id="M104" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula>, where the slope <inline-formula><mml:math id="M105" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> is
not changed by the translation, and the offset is obtained by <inline-formula><mml:math id="M106" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. These results of the forced linear regressions
are compared with the square root transformed regressions in Fig. 2b and c.
As can be seen, the forced linear regressions, in contrast to the OLRs, show
only small deviations from the square root transformed data. Due to the more
direct determination of the offset as well as the simplicity of forced linear
regression compared with square root transformation, the forced linear
regression method is chosen for the analyses. Thus, for each season (<inline-formula><mml:math id="M107" display="inline"><mml:mi>s</mml:mi></mml:math></inline-formula>) and
year (<inline-formula><mml:math id="M108" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula>) in total 52 forced linear regressions were undertaken:
            <disp-formula id="Ch1.E2" content-type="numbered"><mml:math id="M109" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>,</mml:mo><mml:mi>Z</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M110" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M111" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> varies with season and the strength of the volcanic
influence.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><caption><p>Weighted regression between slopes and offsets of all groups of
each season. The offset indicates the tropopause (and UT) concentration of
tropospheric origin (<inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the slope of the fit (<inline-formula><mml:math id="M113" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) expresses
the sensitivity of the UT concentration to changes in the stratospheric
concentration slope (<inline-formula><mml:math id="M114" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>). The error bars show Student <inline-formula><mml:math id="M115" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> 70 and 95 %
confidence interval, respectively.</p></caption>
          <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f03.jpg"/>

        </fig>

      <p>The sulfur concentration at the tropopause and in the UT, expressed by <inline-formula><mml:math id="M116" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> in
Eq. (2), is dependent on the stratospheric concentration which is affected by
volcanism (Friberg et al., 2015). This means that the offset of the
regressions is affected. This is expressed here by
            <disp-formula id="Ch1.E3" content-type="numbered"><mml:math id="M117" display="block"><mml:mrow><mml:mi>b</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UT</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mfenced close=")" open="("><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi></mml:mfenced><mml:mi>k</mml:mi><mml:mfenced open="(" close=")"><mml:mi>s</mml:mi></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mfenced close=")" open="("><mml:mi>s</mml:mi></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where the first term expresses the contribution from stratospheric sources
and the second expresses that of tropospheric sources. This results in the combined
equation:
            <disp-formula id="Ch1.E4" content-type="numbered"><mml:math id="M118" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>,</mml:mo><mml:mi>Z</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
          where <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> reflects stratospheric influence on the UT particulate sulfur
concentration and <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the particulate sulfur
concentration of tropospheric origin.</p>
      <p>In order to obtain estimates of <inline-formula><mml:math id="M121" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, a second
regression for each season is undertaken where the offsets (<inline-formula><mml:math id="M123" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula>) are related to
the slopes (<inline-formula><mml:math id="M124" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>); see Fig. 3. The relative variance of the slopes was much
smaller than that of the offsets (average variance ratio of 0.19). For
simplicity, the variance of the slope was therefore neglected in these
regressions. The groups of data of a season differ in <inline-formula><mml:math id="M125" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M126" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> mainly due
to volcanic influence. A zero slope (<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) would be obtained should the
stratospheric concentration become as low as the UT concentration. The UT
aerosol of tropospheric origin (<inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> thus can be estimated
as the offset of the <inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>-</mml:mo><mml:mi>a</mml:mi></mml:mrow></mml:math></inline-formula> regression. The slope of that regression shows
how the offset <inline-formula><mml:math id="M130" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> changes with increased slope <inline-formula><mml:math id="M131" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>, hence expressing the
sensitivity (<inline-formula><mml:math id="M132" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) of the UT concentration to changes in stratospheric
concentration. With access to these two parameters, <inline-formula><mml:math id="M133" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
and <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, the LMS concentration gradient and tropopause concentration can
be estimated based on a single measurement of the particulate sulfur
concentration.</p>
      <p>The uncertainties of the forced regression results of a given season vary
among the data groups. In order to account for this variability, weights are
used in the regression between the offsets and slopes of a season. The
weights are based on 70 % double-sided Student <inline-formula><mml:math id="M135" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula> distribution
(<inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> %) estimates because some of the estimated <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and
<inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> rely on few observations. The <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % estimate of <inline-formula><mml:math id="M140" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> (<inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mi>b</mml:mi><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mtext>S</mml:mtext><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:mi>a</mml:mi><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>; see above) is obtained by combining the upper
<inline-formula><mml:math id="M142" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % limit of <inline-formula><mml:math id="M143" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> with the weakest <inline-formula><mml:math id="M144" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % slope
(<inline-formula><mml:math id="M145" display="inline"><mml:mi>a</mml:mi></mml:math></inline-formula>) and the strongest <inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % slope at the lower limit multiplied with
<inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. The inverse of the squared <inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mn mathvariant="normal">70</mml:mn></mml:mrow></mml:math></inline-formula> % estimates of <inline-formula><mml:math id="M149" display="inline"><mml:mi>b</mml:mi></mml:math></inline-formula> obtained in
this way are then used as weights in the second step regressions.</p>
</sec>
<sec id="Ch1.S2.SS4">
  <title>Lidar data from the CALIPSO satellite</title>
      <p>The evaluation of the particulate sulfur concentrations from the
IAGOS-CARIBIC aircraft was aided by the use of lidar data from the CALIOP
sensor aboard the CALIPSO (Cloud-aerosol lidar and infrared pathfinder
satellite observation) satellite from NASA (Winker et al., 2010), performing
15 orbits per day covering the globe from 82<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S to 82<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N
with a repeat cycle of 16 days during night and day. The data evaluation
was based on the methodology developed by Vernier et al. (2009). Here only
the nighttime data of the 532 nm wavelength lidar signals were used. The
level 1 data of version 4–10 (averaged in a grid of 180 m vertically and
1 <inline-formula><mml:math id="M152" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 1 horizontally) were used to obtain scattering ratios, i.e., the ratio of
the measured, combined air and aerosol scattering to the modeled air
scattering based on molecule and ozone number concentrations from the GMAO
(Global Modeling and Assimilation Office). Cloud pixels were removed by
rejecting pixels of a depolarization ratio greater than 5 %. This cloud
mask was extended 360 m upwards to remove faint cloud residues, and pixels
from underneath clouds were removed to avoid bias from cloud absorption; see
Andersson et al. (2015) for further details. Removal of cloud pixels as well
as periods of instrument failure sometimes resulted in few observations in
these pixels. In order to avoid statistical noise, at least 20 % of the
maximum possible observation data was required for any given pixel (latitude,
altitude). The pixels were generated by averaging in the longitude interval
60 to 120<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, the main longitude region of the ATAL (Vernier et al.,
2015).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><caption><p>Examples of first step forced linear regression between the
particulate sulfur concentration and the altitude above the tropopause for
the data groups of two seasons: <bold>(a)</bold> FMA (February, March and April) and
<bold>(b)</bold> OND (October, November and December). The legend shows which years are
included in the respective data groups followed by the coefficient of
determination in parentheses.</p></caption>
          <?xmltex \igopts{width=335.74252pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f04.jpg"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S3">
  <title>Results</title>
      <p>The linear regression methodology described in the previous section was
applied to particulate sulfur concentrations (<inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> as a function
of the distance from the tropopause (<inline-formula><mml:math id="M155" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>) for seasons comprising 3 months.
Data from different years of one season were grouped according to their
concentrations, resulting in four or five groups differing with respect to
the <inline-formula><mml:math id="M156" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:mi>Z</mml:mi></mml:mrow></mml:math></inline-formula> relationship. The resulting groups of data from each
season were modeled by forced linear regression. These model results are used
in a second regression step to model seasonal influences from transport,
which in turn are used to obtain the response of the LMS and UT particulate
sulfur concentrations to changes induced mainly by volcanic eruptions.</p>
      <p>This methodology was applied to all seasons, having a duration of 3
months. The final product of the regression methodology, i.e., the second
regression step, of all 12 overlapping seasons is shown in Fig. 3. It is
clear that slopes and offsets of the season groups obtained in the first step
of forced linear regression, differing in particulate sulfur concentration
related to distance from the tropopause, can readily be described by linear
regressions for all twelve 3-month seasons. The relationship between slopes
and offsets has a very strong seasonal dependence. In some seasons small
changes in the LMS sulfur concentration slope is connected with a strong
change in tropopause sulfur concentration. This is most pronounced for the
seasons centered in February, March and April. At the other end we find the
seasons centered in September, October and November, where a change in the
slope of the first regression step due to varying influence from volcanism
has little effect on the tropopause concentration. To further illustrate the
connection to the measurements, Fig. 4 shows the four data groups of the
seasons most (Fig. 3: FMA) and least (Fig. 3: OND) susceptible to change in
the tropopause concentration due to changed stratospheric concentrations. In
Fig. 4a the data group of least volcanic influence includes years 1999–2002
and 2014, and the most influenced years are 2009 and 2012 which are the
springs after the Kasatochi (7 August 2008) and Nabro (12 June 2011)
eruptions (we have no late winter/spring data after the most powerful
eruption of the period studied, Sarychev, 12 June 2009, due to maintenance
of the measurement aircraft). The season centered in November has the
weakest volcanic influence years 1999–2001, 2012 and 2013 (Fig. 4b),
whereas the group with strongest slope includes the three strongest eruptions
of the period studied (Kasatochi, Sarychev and Nabro), a few months after
respective eruption. Despite the very strong volcanic influence of the latter
group, the tropopause concentration (<inline-formula><mml:math id="M157" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) remains close to that of the
closely distributed tropopause concentrations of the other groups of that
season.</p>
      <p>The sensitivity of the tropopause and UT concentration to changes in LMS
concentration slope is denoted <inline-formula><mml:math id="M158" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula> in Eqs. (3) and (4), which thus is obtained for
each regression depicted in Fig. 3. These results are collected in Fig. 5a.
The salient features of the seasonal dependence can be described by two
Gaussian distributions (Fig. 5a). The maximum sensitivity appears in
late winter and early spring when the seasonal variation in tropopause
altitude has its maximum rate of upward motion (Appenzeller et al.,
1996). The maximum in rate of downward motion of the tropopause appears in
the fall. This delays transport from the stratosphere to the troposphere,
which is reflected by a low-sensitivity <inline-formula><mml:math id="M159" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>. This sensitivity can, in
addition, be affected by the residence time of particulate sulfur in the UT.
Interestingly, the downward transport in association with the Brewer–Dobson
circulation from deeper, aerosol-rich stratospheric layers through the LMS
takes place in the same season as the maximum in <inline-formula><mml:math id="M160" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>, thus further enhancing
the stratospheric influence on the UT by the term <inline-formula><mml:math id="M161" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>(</mml:mo><mml:mi>y</mml:mi><mml:mo>,</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>×</mml:mo><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> in
Eq. (4).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Seasonal variation of <bold>(a)</bold> the sensitivity of the UT particulate
sulfur concentration to the concentration slope in the LMS (<inline-formula><mml:math id="M162" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>) and <bold>(b)</bold> the
UT particulate sulfur concentration of tropospheric origin (<inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=176.407087pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f05.jpg"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>Estimated <bold>(a)</bold> slopes and <bold>(b)</bold> offsets based on individual
measurements (dots) and monthly averages (magenta bars). <bold>(c)</bold> Sulfur aerosol
column of the lowest 3000 m of the LMS with standard errors, assuming
particles of 75 % sulfuric acid and 25 % water, and AOD (right <inline-formula><mml:math id="M164" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis)
assuming stratospheric background aerosol particle size distribution.</p></caption>
        <?xmltex \igopts{width=298.753937pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f06.jpg"/>

      </fig>

      <p>The offsets of the regression lines shown in Fig. 3 (when <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:mi>a</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula>) expresses
the case when the stratospheric and tropospheric concentrations are equal,
implying that this offset expresses the particulate sulfur concentration of
tropospheric origin (<inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> that is mixed into the LMS; see
Fig. 5b. Two Gaussian distributions were used as fits to the seasonal
variation of <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. As for <inline-formula><mml:math id="M168" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>, the seasonal variation of
<inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> is strong. The seasonal variation of
<inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> will be elaborated in the discussion section.</p>
      <p>After obtaining <inline-formula><mml:math id="M171" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M172" display="inline"><mml:mi>k</mml:mi></mml:math></inline-formula>, the data that are needed for
conversion of every measurement of the concentration to an estimate of the
slope and offset of the LMS concentration are available. Thus, for each
individual measurement (i) in the LMS, consisting of the particulate sulfur
concentration (<inline-formula><mml:math id="M173" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">i</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and the altitude <inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> above the
tropopause, the slope and offset of Eqs. (3) and (4) are obtained from

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M175" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E5"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>a</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">i</mml:mi></mml:mrow></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>+</mml:mo><mml:mi>k</mml:mi><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E6"><mml:mtd/><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi>b</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>a</mml:mi><mml:mi mathvariant="normal">i</mml:mi></mml:msub><mml:mi>k</mml:mi><mml:mfenced close=")" open="("><mml:mi>s</mml:mi></mml:mfenced><mml:mo>+</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>(</mml:mo><mml:mi>s</mml:mi><mml:mo>)</mml:mo><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          The estimated slopes and offsets are shown in Fig. 6a and b, where the dots
are individual measurements and the histogram monthly averages. Here
measurements taken at an altitude of less than 50 m above the tropopause are
not shown, because they were judged to have too small a stratospheric character
for an estimate of the concentration slope in the LMS. Both the slope and the
tropopause concentration are affected by volcanism (Table 1), but the
relative response of the slope is much stronger than that of the tropopause
concentration; see, for example, the falls of 2008 and 2009 affected by the Kasatochi
and Sarychev eruptions.</p>
      <p><?xmltex \hack{\newpage}?>Observations at various altitudes above the tropopause are difficult to
compare, due to the concentration gradient in the LMS. With the estimates of
the tropopause concentration and the slope in the particulate sulfur LMS
concentration, each measurement becomes an estimate of the total amount of
particulate sulfur in the altitude interval investigated through the integration of
Eq. (4). However, first the STP concentrations (<inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">STP</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mi mathvariant="normal">S</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mi>a</mml:mi><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi></mml:mrow></mml:math></inline-formula>) need to be converted into volume concentrations
(<inline-formula><mml:math id="M177" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">V</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, which are related by <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">V</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">STP</mml:mi></mml:mrow></mml:msub><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">STP</mml:mi></mml:msub><mml:mo>/</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>Z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M179" display="inline"><mml:mi>Q</mml:mi></mml:math></inline-formula> is molar
volumes. For that purpose, the altitude dependence of the molar volume from
the tropopause up to 5 km above the tropopause was extracted from
temperatures and pressures obtained from ECMWF for each sample. The molar
volume can be expressed as <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mi>Z</mml:mi></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mi>w</mml:mi><mml:mi>Z</mml:mi></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, where the tropopause is at <inline-formula><mml:math id="M181" display="inline"><mml:mrow><mml:mi>Z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M182" display="inline"><mml:mrow><mml:mi>w</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.0001535</mml:mn></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M183" 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> obtained as the average of all samples. For a
measurement the molar volume is <inline-formula><mml:math id="M184" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> obtained at distance
<inline-formula><mml:math id="M185" display="inline"><mml:mrow><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from the tropopause, and the tropopause molar volume is
computed by <inline-formula><mml:math id="M186" display="inline"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mfenced close=")" open="("><mml:mn mathvariant="normal">0</mml:mn></mml:mfenced><mml:mo>=</mml:mo><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mi>w</mml:mi><mml:msub><mml:mi>Z</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>. Finally,
the column concentration of particulate sulfur for the first 3 km above the
dynamical tropopause of 1.5 PVU is obtained by integration of the volume
concentration:

              <disp-formula specific-use="align" content-type="numbered"><mml:math id="M187" display="block"><mml:mtable displaystyle="true"><mml:mtr><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">col</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mn mathvariant="normal">3000</mml:mn></mml:munderover><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">STP</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mfenced open="(" close=")"><mml:mi>Z</mml:mi></mml:mfenced></mml:mrow></mml:mfrac></mml:mstyle><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">STP</mml:mi></mml:mrow></mml:msub><mml:mfenced open="(" close=")"><mml:mi>Z</mml:mi></mml:mfenced><mml:mi mathvariant="normal">d</mml:mi><mml:mi>Z</mml:mi></mml:mrow></mml:mtd></mml:mtr><mml:mlabeledtr id="Ch1.E7"><mml:mtd/><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mo>=</mml:mo><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mn mathvariant="normal">3000</mml:mn></mml:munderover><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">STP</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>Q</mml:mi><mml:mi mathvariant="normal">V</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mn mathvariant="normal">0</mml:mn><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle><mml:msup><mml:mi>e</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mi>w</mml:mi><mml:mi>Z</mml:mi></mml:mrow></mml:msup><mml:mfenced open="(" close=")"><mml:mi>a</mml:mi><mml:mi>Z</mml:mi><mml:mo>+</mml:mo><mml:mi>b</mml:mi></mml:mfenced><mml:mi mathvariant="normal">d</mml:mi><mml:mi>Z</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

          The particulate sulfur column is calculated for altitudes above the
tropopause (<inline-formula><mml:math id="M188" display="inline"><mml:mi>Z</mml:mi></mml:math></inline-formula>) in the range of 0 to 3000 m, the upper limit set where too few
measurements (5 %) were taken above that level. After integrating the
column, it is also interesting to estimate the total amount of
sulfur-connected aerosol. To that end, it was assumed that the aerosol
consists of 75 % sulfuric acid and 25 % water, which is a commonly
used stratospheric composition (Rosen, 1971; Arnold et al., 1998). This means
that the total sulfur column was multiplied by a stoichiometric factor of <inline-formula><mml:math id="M189" display="inline"><mml:mrow><mml:mi>h</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">4.084</mml:mn></mml:mrow></mml:math></inline-formula> to obtain the column of the sulfuric acid–water aerosol:
          <disp-formula id="Ch1.E8" content-type="numbered"><mml:math id="M190" display="block"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">A</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">col</mml:mi></mml:mrow></mml:msub><mml:mo>=</mml:mo><mml:mi>h</mml:mi><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">col</mml:mi></mml:mrow></mml:msub><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>
        The measurements were taken in the Northern Hemisphere latitudes higher than
30<inline-formula><mml:math id="M191" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> with the highest latitude of 77<inline-formula><mml:math id="M192" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>, with 90 % of the
data in the latitude range 32–64<inline-formula><mml:math id="M193" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and 70 % of the data
between 37 and 57<inline-formula><mml:math id="M194" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. The northern midlatitudes sulfur aerosol
columns are shown in Fig. 6c as monthly averages with standard errors (the
few months with only one measurement available are shown without error
bars). The sulfur aerosol column of the LMS shows large variability primarily
caused by volcanism. The lowest columns are found in the period 1999–2002,
when the volcanic influence on the stratospheric aerosol was small (see
Table 1 for relevant volcanic eruptions). The time period mid-2005 to mid-2008
was affected by tropical volcanism (Vernier et al., 2011a), which also caused
elevated concentrations in the NH LMS (Friberg et al., 2014). The eruptions
of the extratropical volcano Kasatochi in August 2008 placed two volcanic
clouds in the stratosphere (Andersson et al., 2015), one in the LMS causing
strongly elevated aerosol column of the LMS that ceased by November the same
year, and the other above the LMS. The latter cloud was transported downward,
causing a rise of the lower LMS aerosol column in December 2008. After some
influence from several eruptions of the extratropical volcano Redoubt in the
spring of 2009, the eruption of Sarychev strongly affected the Northern Hemisphere stratosphere from June 2009. The eruption of the Icelandic
volcano Grimsvötn in May 2011 had a strong and short impact on the
northern LMS, which is reflected by a peak in June to July 2011 (Fig. 6c),
before the tropical volcano Nabro reached the northern LMS in the early fall
of the same year. After that eruption a gradual decrease of the aerosol load
can be seen. The concentrations after mid-2013 approach those of the period
1999–2002, which was close to stratospheric background conditions.</p>
      <p>The LMS aerosol contains a significant fraction of carbonaceous material
(Martinsson et al., 2009), mainly organic in nature (Friberg et al., 2014),
which adds to the aerosol columns of Fig. 6c and affect the refractive
index of the particles. However, this work is dealing with the sulfurous
fraction, the main fraction of the stratospheric aerosol. To put the results
presented in Fig. 6c into perspective, the AOD is estimated using a
simplified aerosol (which thus likely is an underestimation of the AOD).
Thus, the “standard” stratospheric 75 % sulfuric acid, 25 % water
composition, 1.669 g cm<inline-formula><mml:math id="M195" 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> particle density and 1.44 refractive
index will be used. Furthermore, particle size distribution measurements
from IAGOS-CARIBIC have been taken since 2010 (Hermann et al., 2016). The
changes of the size distribution induced by the moderate 2011 eruptions of
Grimsvötn and Nabro were small (Martinsson et al., 2014), and agree well
with previous measurements (Andersson et al., 2015) of the stratospheric
background particle size distribution by Jäger and Deshler (2002). Thus,
for the estimation of the AOD the latter particle size distribution was used
for the entire time period studied. For fixed composition and particle size
distribution the AOD is obtained as a fixed relationship to aerosol column:
<inline-formula><mml:math id="M196" display="inline"><mml:mrow><mml:mi mathvariant="normal">AOD</mml:mi><mml:mo>=</mml:mo><mml:mi>f</mml:mi><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">A</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">col</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>, where <inline-formula><mml:math id="M197" display="inline"><mml:mi>f</mml:mi></mml:math></inline-formula> contains the relationships
between mass and area/extinction, in this case <inline-formula><mml:math id="M198" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">3.29</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> m<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> <inline-formula><mml:math id="M200" display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g<inline-formula><mml:math id="M201" 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>. Finally, converting the AOD into radiative forcing (RF) using the
global average relation (Hansen et al., 2005; Solomon et al., 2011) of
          <disp-formula id="Ch1.E9" content-type="numbered"><mml:math id="M202" display="block"><mml:mrow><mml:mi mathvariant="normal">RF</mml:mi><mml:mo>=</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">25</mml:mn><mml:mo>×</mml:mo><mml:mi mathvariant="normal">AOD</mml:mi><mml:mo>;</mml:mo><mml:mspace width="1em" linebreak="nobreak"/><mml:mi mathvariant="normal">in</mml:mi><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        to obtain an estimate of the climate influence of the sulfate aerosol of the
lower LMS. The peak AOD of the Kasatochi and Sarychev eruptions is
approximately 0.006, corresponding to <inline-formula><mml:math id="M203" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.15 W m<inline-formula><mml:math id="M204" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in regional
radiative forcing of the lowest 3000 m of the Northern Hemisphere LMS.
Although no detailed comparisons will be made here, we find that the AOD and
radiative forcing obtained from the particulate sulfur measurements show
similar tendencies to satellite-based measurements (Andersson et al., 2015).
The findings presented here also corroborate the findings of Andersson et
al. (2015) on the importance of the LMS for the total stratospheric AOD and
radiative impact.</p><?xmltex \hack{\newpage}?>
</sec>
<sec id="Ch1.S4">
  <title>Discussion</title>
      <p>The results presented here are based on measurements in the extratropical UT
and the LMS of the NH, where the latter includes the extratropical transition
layer (ExTL). Bi-directional exchange across the tropopause affects strong
gradients in the ExTL for species having clearly different stratospheric and
tropospheric concentrations (Hoor et al., 2002), such as particulate sulfur
(Martinsson et al., 2005). In the previous section, the UT concentration, the
gradient in the LMS and column amount of particulate sulfur in the ExTL were
investigated, with seasonal dependence (Fig. 5) and influence from
volcanism (Fig. 6). In the processing of the data to obtain these results, one feature stands out in
particular: the seasonal dependence of the particulate
sulfur concentration from tropospheric sources that is mixed into the ExTL
(Fig. 5b). It shows a broad maximum from August to December, peaking in
September to November and a deep minimum in the late winter and early spring
(February and March).</p>
      <p>Let us now compare these concentrations in the UT of tropospheric origin
(<inline-formula><mml:math id="M205" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> with average concentrations of particulate sulfur in
the UT for two cases: “background conditions” dominated by data from
mid-1999 to mid-2002 and “moderate influence from tropical volcanism”
dominated by data from mid-2005 to mid-2008; see Sect. 2.3 for details. The
seasonal dependence of these two categories are shown in Fig. 7a together
with <inline-formula><mml:math id="M206" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula>. It is clear that, in line with the findings of
Friberg et al. (2015), the UT particulate sulfur concentration is affected by
volcanism. In Fig. 7a we see that the main differences in UT concentrations
of the two cases appears from January to July, coinciding with the season of
transport down from the Junge layer into to the LMS and the shrinkage of the
LMS due to tropopause upward motion (Appenzeller et al., 1996; Gettelman et
al., 2011). In the period September to November the influence from volcanism
on the UT particulate sulfur concentrations is small (compare the background
and moderate volcanism cases; Fig. 7a). When comparing these cases to the
concentration of particulate sulfur found to be of tropospheric origin, it is
clear that there is strong agreement between all three categories in the
fall months, whereas differences are large during the remainder of the year.
The UT particulate sulfur concentration of stratospheric origin can be
estimated by subtracting <inline-formula><mml:math id="M207" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> from the two cases of UT
concentrations. The results are shown in Fig. 7b, where peak stratospheric
influences of 19 and 36 ng m<inline-formula><mml:math id="M208" 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> STP are found in the spring, and
minimum contributions of approximately 1 ng m<inline-formula><mml:math id="M209" 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> STP are found in the fall for
the “background” and “moderate volcanism” cases. Summing the observations
up (Fig. 7c), a clear seasonal dependence in the fraction of the UT
particulate sulfur concentration originating in the stratosphere was found,
from close to 100 % in late winter/spring to approximately 10 % in
the fall. On a yearly average the fraction of the UT particulate sulfur that
originates in the stratosphere is approximately 50 % during background
conditions and 70 % during moderate influence from tropical volcanism.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>Seasonal variation of <bold>(a)</bold> the UT particulate sulfur concentration
during LMS background conditions and moderate volcanic influence, together
with the estimated UT particulate sulfur concentration of tropospheric
origin (<inline-formula><mml:math id="M210" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <bold>(b)</bold> UT particulate sulfur concentration of
stratospheric origin (<inline-formula><mml:math id="M211" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTstrat</mml:mi></mml:mrow></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> obtained by subtracting the
<inline-formula><mml:math id="M212" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> from the two UT concentration cases in <bold>(a)</bold> and the
ratio <inline-formula><mml:math id="M213" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTstrat</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M214" display="inline"><mml:mo>/</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M215" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UT</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> for the two cases <bold>(c)</bold>.</p></caption>
        <?xmltex \igopts{width=176.407087pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f07.jpg"/>

      </fig>

      <p>The tropospheric source of UT particulate sulfur could be transported from
the planetary boundary layer either in the form of particulate sulfur or
precursor gases, in the latter case primarily sulfur dioxide (SO<inline-formula><mml:math id="M216" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>. In
fall, winter and spring, with maximum in the winter, vertical transport by
WCBs from the boundary layer to the UT is strong (Eckhardt et al., 2004),
whereas in the summer deep convection is the most important mode (Hess,
2005; Kiley and Fuelberg, 2006) in the extratropics. For sulfate, the most
common chemical form of particulate sulfur, the concentration usually shows
a rapid decline with altitude in the troposphere (Heald et al., 2011)
associated with formation of precipitation. Cloud processing also tends to
strongly reduce SO<inline-formula><mml:math id="M217" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentrations with altitude, where the relative
availability of SO<inline-formula><mml:math id="M218" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and hydrogen peroxide (H<inline-formula><mml:math id="M219" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>O<inline-formula><mml:math id="M220" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is important
for the SO<inline-formula><mml:math id="M221" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> lifetime in the cloud.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><caption><p>Latitude and altitude distribution of scattering from aerosol in
the stratosphere and the UT. Two series, from 2013 (upper row, <bold>a–e</bold>) and
2011 (lower row, <bold>f–j</bold>), show the monthly mean 532 nm wavelength scattering
ratio from June to October without and with, respectively, fresh volcanic
influence. The former series allows identification of the comparably weak
ATAL in July to September. The lower series includes two volcanic eruptions:
the high-altitude cloud from the tropical volcano Nabro (eruption in 12 June 2011) and the low-altitude and midlatitude faint volcanic cloud from
Grimsvötn (21 May 2011). The two white lines in every graph show the
monthly averaged positions of 380 K potential temperature (upper line) and
the 1.5 PVU dynamical tropopause.</p></caption>
        <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/17/10937/2017/acp-17-10937-2017-f08.png"/>

      </fig>

      <p>We have found some very distinctive characteristics of the particulate sulfur
concentration of tropospheric origin in the UT, with low concentrations in
February and March, increasing concentrations during the summer and maximum
in the sources of tropospheric origin in the fall. Carbon monoxide (CO) is
often used as a tracer of air pollution. Zbinden et al. (2013) found
winter/spring maximum in the CO concentration in the UT of the NH in contrast
to the tropospheric component of the UT particulate sulfur. This contrast
can, at least in part, be explained by the oxidizing capacity in the UT. The
summer abundance of the hydroxyl (OH) radical (Bahm and Khalil, 2004) induces
a decline in CO (Bergamaschi et al., 2000; Osman et al., 2016). High
abundance of this radical, on the other hand, and availability of SO<inline-formula><mml:math id="M222" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula>
can lead to production of particulate sulfur. SO<inline-formula><mml:math id="M223" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> measurements by the
satellite-based instrument MIPAS have recently become available (Höpfner
et al., 2015). These data have large uncertainties (Höpfner et al.,
2015), and likely overestimate the SO<inline-formula><mml:math id="M224" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> concentration (Rollins et al.,
2017). However, here we only qualitatively use the seasonal variation. The
MIPAS results indicate a UT seasonal variation in the NH midlatitudes with
low concentrations in December to March and the highest concentrations in
June to September (Höpfner et al., 2015). Deep convection provides a
rapid route upwards in the atmosphere, favoring transport of short-lived
species like SO<inline-formula><mml:math id="M225" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> (TF-HTAP-2010, 2010; Dickerson et al., 2007). Low abundance
of both SO<inline-formula><mml:math id="M226" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and OH in the NH UT thus could explain the weak tropospheric
contribution to the UT particulate sulfur during late winter and early
spring. The increase in <inline-formula><mml:math id="M227" display="inline"><mml:mrow><mml:msub><mml:mi>C</mml:mi><mml:mrow><mml:mi mathvariant="normal">S</mml:mi><mml:mo>,</mml:mo><mml:mi mathvariant="normal">UTtrop</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> during the spring and summer
months coincides with increases in convective activity as well as in the
concentration of both SO<inline-formula><mml:math id="M228" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> and OH, thus offering a plausible explanation.
However, the quantitative understanding of the SO<inline-formula><mml:math id="M229" display="inline"><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:math></inline-formula> transport paths and UT
seasonality requires further study. Still, we need to consider the late
maximum in the fall of the tropospheric source of UT particulate sulfur.</p>
      <p>The Asian monsoon is an important feature of global circulation in June
to September, which has been found to reach deep into the lower stratosphere.
This intrusion of tropospheric air into the tropical transition layer
(Sunilkumar et al., 2017) has been manifested by gas-phase components
including water and ozone (Gettelman et al., 2004; Randel and Park, 2006) and
hydrogen cyanide (Randel et al., 2010). Later an aerosol layer extending from
the UT to the potential temperature of 420 K in the lower stratosphere was
found at 14 to 18 km altitude (Vernier et al., 2011b; Thomason and Vernier,
2013; Vernier et al., 2015). Figure 8a–e show monthly means of the
scattering ratio obtained from the CALIPSO sensor CALIOP for the months June
to October 2013, when the volcanic influence was low. Formation of the ATAL
can be identified in July (Fig. 8b) with maximum intensity in August
(Fig. 8c). Even in September can a weakened ATAL be identified (Fig. 8d),
whereas in June and October the scattering in the ATAL region at 14–18 km
altitude is very weak (Fig. 8a and e).</p>
      <p>The altitude range of the ATAL is above the measurement altitudes of
IAGOS-CARIBIC (9–12 km). However, the poleward circulation along isentropes
bending downwards, further amplified by an extratropical cross-isentrope,
downward component, brings the ATAL down to lower altitudes. The ATAL is too
weak to be traced by CALIOP in the downward transport (Fig. 8a–e). We
therefore illustrate the subsidence using the eruption of the tropical
volcano Nabro in summer 2011 (Table 1), with effluents that occupied
approximately the same region as the ATAL (see Fig. 3 in Bourassa et
al., 2012). The effluents of this eruption were rapidly transported to the
north in the tropical tropopause layer. Figure 8f–j actually includes two volcanic eruptions;
besides the tropical volcano Nabro, the Icelandic volcano Grimsvötn
injected a volcanic cloud into the tropopause region at midlatitudes which is
visible in June and July 2011. The time series of the Nabro volcanic cloud in
Fig. 8f–j unambiguously demonstrates the transport down to the IAGOS-CARIBIC
flight altitudes in the season of the ATAL. In Fig. 6c we see a clear
increase in the particulate sulfur column in September 2011, following the
decline of the June–July 2011 short peak from the of Grimsvötn eruption
in May 2011, thus demonstrating agreement between CALIOP and IAGOS-CARIBIC
measurements of particulate sulfur. The volcanic cloud from Nabro initially
resided at somewhat higher altitude than the ATAL, implying that the ATAL can
be expected to reach IAGOS-CARIBIC flight altitudes somewhat earlier in the
year. The transport in this season contains little particulate sulfur during
periods without fresh volcanic aerosol; compare Fig. 7 “tropical
volcanism” (the “tropical volcanism” category of Fig. 7 does not include the Nabro eruption – see
Sect. 2.3) with “background” and the particulate sulfur of tropospheric
origin.</p>
      <p>The downward transport allows delayed detection of the ATAL in the fall from
altitudes above the measurement altitude range of IAGOS-CARIBIC in the same
way as the spring detection of aerosol transported from the Junge layer, with
or without volcanic influence, as shown in Fig. 7. A difference between these
two seasons is that in the spring the strong source of particulate sulfur is
stratospheric, whereas in the fall the source is tropospheric extending from
the UT into the stratosphere. We therefore conclude that the UT particulate
sulfur concentration of tropospheric origin that starts to increase rapidly
in August, peaking in September to November, and is back at low concentration
in January (Fig. 5b) is most likely caused by the ATAL formation from the
Asian monsoon.</p>
      <p>Model studies find similar UT/stratosphere distribution of the ATAL as the
experimental studies, that Asian pollution sources strongly
contribute to the ATAL and that sulfate is an important component of that
aerosol layer (Neely III et al., 2014). Besides this component, primary and
secondary organic aerosol constituents are predicted to be important
components of the ATAL (Yu et al., 2015). The present study is, as far as we
know, the first observation of a chemical component of the ATAL. In agreement
with modeling results we find that particulate sulfur is a component of the
Asian tropopause aerosol layer. This component affects the tropopause region
from July to September at 14 to 18 km altitude (Fig. 8) and the
extratropical tropopause region from August to December (Fig. 5b).</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>Particulate sulfur (usually sulfate) in the upper troposphere (UT) and the
lowermost stratosphere (LMS) obtained from the IAGOS-CARIBIC platform was
investigated at northern midlatitudes in the time period 1999–2014, which
covers several tropical and extratropical volcanic eruptions. The study is
based on the use of linear regression models, where individual measurements
in the strong gradient of the extratropical transition layer (ExTL) can be
converted into an estimate of the column of particulate sulfur in a layer 3000 m
above the dynamical tropopause (here defined at 1.5 PVU). The obtained time series in particulate sulfur column concentration
shows distinct response to extratropical volcanism and delayed elevation of
the column concentration following tropical eruptions. Assuming the
stratospheric background particle size distribution and composition (75 %
sulfuric acid and 25 % water) the AOD and radiative forcing were
estimated; e.g., the peak values following the 2009 Sarychev eruptions were
estimated to be 0.006 and <inline-formula><mml:math id="M230" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>0.15 W m<inline-formula><mml:math id="M231" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, respectively. These estimates
refer mainly to the ExTL, i.e., lowest part of the LMS, thus highlighting the
importance of the lowest part of the stratosphere for the overall climate
impact of volcanism.</p>
      <p>As part of this investigation the sources of UT particulate sulfur were
explored. A distinct pattern emerges where tropospheric sulfur sources
dominate the supply of particulate sulfur to the UT in the fall, whereas
stratospheric sources dominate in January to July, the main season of
transport from the Junge layer into the LMS. The smallest contributions from
the troposphere are found in February and March in conjunction with low
sulfur dioxide (SO<inline-formula><mml:math id="M232" display="inline"><mml:mrow><mml:msub><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and oxidant concentrations. As the concentrations
of these species increase, the UT particulate sulfur concentration of
tropospheric origin increases somewhat in April to July. The particulate
sulfur concentration shows a threefold increase during the fall, with maximum
concentration in September to November. Making use of lidar data from the
CALIPSO satellite together with the in situ measurements we find that the
Asian tropopause aerosol layer (ATAL) resulting from the Asian monsoon is the
cause of the increase. The ATAL is formed at 14–18 km altitude and extends
from the UT to approximately 420 K potential temperature in the
stratosphere, with main extension in July to September. The ATAL is
transported downwards and affects the extratropical tropopause region in
August to December. As far as we know, this is the first measurement of a
chemical species in particles connected with the ATAL. The stratospheric and
tropospheric contributions to the UT particulate sulfur concentrations thus
have strong and opposite seasonal dependences. On annual average the
stratospheric contribution to the UT particulate sulfur is estimated to be
50 % during stratospheric background conditions. During influence from
moderate tropical volcanism the stratospheric fraction rises to 70 %. The
particulate sulfur concentration in the UT is thus to a large degree governed
by the stratosphere and volcanism.</p>
</sec>

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

      <p>Data are available upon request from the corresponding
author.</p>
  </notes><notes notes-type="competinginterests">

      <p>The authors declare that they have no conflict of
interest.</p>
  </notes><ack><title>Acknowledgements</title><p>We acknowledge all members of the IAGOS-CARIBIC project, Lufthansa and
Lufthansa Technik for enabling the IAGOS-CARIBIC observatory. Financial
support from the Swedish National Space Board (contract 130/15) and the
Swedish Research Council for Environment, Agricultural Sciences and Spatial
Planning (contract 942-2015-995) is gratefully acknowledged. Moreover, the
German Federal Ministry of Education and Research (BMBF) is acknowledged for
financing the instruments' operation as part of the joint project IAGOS-D.
Aerosol measurements from CALIPSO were produced by NASA Langley Research
Center.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?> Edited by: Kostas
Tsigaridis<?xmltex \hack{\newline}?> Reviewed by: four anonymous referees</p></ack><ref-list>
    <title>References</title>

      <ref id="bib1.bib1"><label>1</label><mixed-citation>Andersson, S. M., Martinsson, B. G., Friberg, J., Brenninkmeijer, C. A. M.,
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    </app></app-group></back>
    <!--<article-title-html>Particulate sulfur in the upper troposphere and lowermost stratosphere – sources and climate forcing</article-title-html>
<abstract-html><p class="p">This study is based on fine-mode aerosol samples collected in the
upper troposphere (UT) and the lowermost stratosphere (LMS) of the Northern
Hemisphere extratropics during monthly intercontinental flights at
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several kilometers into the LMS, as a result of increasing dilution towards
the tropopause of stratospheric, particulate sulfur-rich air. The stratospheric air is diluted with tropospheric air, forming the extratropical transition layer (ExTL). Observed
concentrations are related to the distance to the dynamical tropopause. A
linear regression methodology handled seasonal variation and impact from
volcanism. This was used to convert each data point into stand-alone estimates
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radiative forcing. Further, the origin of UT particulate sulfur shows
strong seasonal variation. We find that tropospheric sources dominate during
the fall as a result of downward transport of the Asian tropopause aerosol
layer (ATAL) formed in the Asian monsoon, whereas transport down from the
Junge layer is the main source of UT particulate sulfur in the first half of
the year. In this latter part of the year, the stratosphere is the clearly
dominating source of particulate sulfur in the UT during times of volcanic
influence and under background conditions.</p></abstract-html>
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