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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">ACPD</journal-id>
<journal-title-group>
<journal-title>Atmospheric Chemistry and Physics Discussions</journal-title>
<abbrev-journal-title abbrev-type="publisher">ACPD</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys. Discuss.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1680-7375</issn>
<publisher><publisher-name>Copernicus GmbH</publisher-name>
<publisher-loc>Göttingen, Germany</publisher-loc>
</publisher>
</journal-meta>

    <article-meta>
      <article-id pub-id-type="doi">10.5194/acpd-15-9507-2015</article-id><title-group><article-title>Aerosol vertical distribution, optical properties and transport over Corsica (western Mediterranean)</article-title>
      </title-group><?xmltex \runningtitle{Aerosol vertical distribution over Corsica}?><?xmltex \runningauthor{J.-F. L\'{e}on et~al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Léon</surname><given-names>J.-F.</given-names></name>
          <email>jean-francois.leon@aero.obs-mip.fr</email>
        <ext-link>https://orcid.org/0000-0002-1251-0361</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Augustin</surname><given-names>P.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0966-2468</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Mallet</surname><given-names>M.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Bourrianne</surname><given-names>T.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Pont</surname><given-names>V.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Dulac</surname><given-names>F.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Fourmentin</surname><given-names>M.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1385-2547</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lambert</surname><given-names>D.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Sauvage</surname><given-names>B.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3410-2139</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Laboratoire d'aérologie, CNRS, Université Paul Sabatier, Toulouse, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Laboratoire de physico-chimie de l'atmosphère, Université du Littoral Côte d'Opale, Dunkerque, France</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Centre National de la recherche météorologique, CNRS, Météo-France, Toulouse, France</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Laboratoire des sciences du climat et de l'environnement, UMR8212 CEA-CNRS-UVSQ, Gif-Sur-Yvette, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">J.-F. Léon (jean-francois.leon@aero.obs-mip.fr)</corresp></author-notes><pub-date><day>31</day><month>March</month><year>2015</year></pub-date>
      
      <volume>15</volume>
      <issue>6</issue>
      <fpage>9507</fpage><lpage>9540</lpage>
      <history>
        <date date-type="received"><day>26</day><month>January</month><year>2015</year></date>
           <date date-type="accepted"><day>13</day><month>March</month><year>2015</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015.html">This article is available from https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015.html</self-uri>
<self-uri xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015.pdf</self-uri>


      <abstract>
    <p>This paper presents the aerosol vertical distribution observed in the western Mediterranean between February and April 2011 and between February 2012 and August 2013.
An elastic backscattering lidar was continuously operated at a coastal site in the northern part of Corsica Island (Cap Corse) for a total of more than 14 000 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> of observations.
The aerosol extinction coefficient retrieved from cloud-free lidar profiles are analyzed along with the SEVIRI satellite aerosol optical depth (AOD).
The SEVIRI AOD was used to constrain the retrieval of the aerosol extinction profiles from the lidar range-corrected signal and to detect the presence of dust or pollution aerosols.
The daily average AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is 0.16 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math></inline-formula>) and ranges between 0.05 and 0.80.
A seasonal cycle is observed with minima in winter and maxima in spring–summer.
High AOD days (above 0.3 at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>) represent less than 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the totality of daily observations and correspond to the large scale advection of desert dust from Northern Africa or pollution aerosols from Europe.
The respective origin of the air masses is confirmed using FLEXPART simulations in the backward mode.
Dust events are characterized by a large turbid layer between 2 and 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height while pollution events show a lower vertical development with a thick layer below 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> in altitude.
However low level dust transport is also reported during spring while aerosol pollution layer between 2 and 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height has been also observed.
We report an effective lidar ratio at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> for pollution aerosols 68 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>13</mml:mn></mml:mrow></mml:math></inline-formula>) Sr while it is 63 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>18</mml:mn></mml:mrow></mml:math></inline-formula>) Sr for dust.
The daily mean AOD at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> for dust events is 0.61 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.14</mml:mn></mml:mrow></mml:math></inline-formula>) and 0.71 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.16</mml:mn></mml:mrow></mml:math></inline-formula>) for pollution aerosols events.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\allowdisplaybreaks}?>
<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>The Mediterranean area has been identified as a “hot-spot” in terms of vulnerability to climate change <xref ref-type="bibr" rid="bib1.bibx20" id="paren.1"/>.
The hydrological cycle of the basin is particularly vulnerable to global warming, showing a 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> decrease in the availability of land surface water and a 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> increase in the loss of fresh water over the Mediterranean sea due to precipitation reduction and warming-enhanced evaporation <xref ref-type="bibr" rid="bib1.bibx33" id="paren.2"/>.
It has been recognized that tropospheric aerosol interact significantly on the climate system and the hydrological cycle <xref ref-type="bibr" rid="bib1.bibx30 bib1.bibx44" id="paren.3"/>.
Moreover the type and abundance of atmospheric aerosols is one of the key issue regarding regional climate change over the Mediterranean (<xref ref-type="bibr" rid="bib1.bibx40" id="altparen.4"/>).
Indeed aerosols scatter and absorb solar light and thermal radiation and thus perturb the radiative balance <xref ref-type="bibr" rid="bib1.bibx19" id="paren.5"><named-content content-type="pre">e.g.</named-content></xref>.
Aerosols also interact with the water cycle because they act as cloud condensation nuclei <xref ref-type="bibr" rid="bib1.bibx46" id="paren.6"><named-content content-type="pre">e.g.</named-content></xref>.
Moreover, they can also significantly impact the vertical stability of the atmosphere by modifying the heating rate profile and reducing the solar irradiance at the surface <xref ref-type="bibr" rid="bib1.bibx45" id="paren.7"/>.
Because of their short lifetime in the atmosphere compared to greenhouse gases, their radiative impact has a pronounced regional pattern <xref ref-type="bibr" rid="bib1.bibx31" id="paren.8"><named-content content-type="pre">e.g.</named-content></xref>.
In the Mediterranean region, such variability has been shown to have
significant effects on the variability in surface radiation and consequently
on sea surface evaporation and climate variability
<xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx40" id="paren.9"/>.
The aerosol concentration, types and optical properties are highly variable over the Mediterranean because of the large diversity in the sources, which are both from natural and anthropogenic origins.
The vertical distribution is also complex and often shows several layers with different types of particles.
The marine boundary layer is under the influence of primary and secondary marine aerosols and anthropogenic emissions from major coastal urban or industrial areas.
The free troposphere above the basin is often affected by the transport of mineral dust from North Africa <xref ref-type="bibr" rid="bib1.bibx41" id="paren.10"/> and occasionaly by biomass burning aerosols from Europe <xref ref-type="bibr" rid="bib1.bibx7" id="paren.11"/> and North America <xref ref-type="bibr" rid="bib1.bibx18" id="paren.12"/>.
Many studies based on lidar soundings have been dedicated to the characterization of the aerosol vertical distribution over the Mediterranean
<xref ref-type="bibr" rid="bib1.bibx24 bib1.bibx22 bib1.bibx23 bib1.bibx15 bib1.bibx51 bib1.bibx16 bib1.bibx53 bib1.bibx7 bib1.bibx41 bib1.bibx10" id="paren.13"/>.
Those studies show that the transport of mineral dust from North Africa has a significant impact on the vertical distribution of aerosols in the Mediterranean region <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx14" id="paren.14"><named-content content-type="pre">e.g.,</named-content></xref>.
Over Lampedusa Island (35.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 12.6<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) <xref ref-type="bibr" rid="bib1.bibx14" id="text.15"/> have shown that the maximum of altitude of desert dust reaches 8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> in spring while non-desert dust aerosols are confined below 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.
Such high altitude has been also observed over Potenza (40.6<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 15.7<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) by <xref ref-type="bibr" rid="bib1.bibx36" id="text.16"/>.
<xref ref-type="bibr" rid="bib1.bibx2" id="text.17"/> report lower altitude at about 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> over Thessaloníki (40.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 22.9<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) as well as <xref ref-type="bibr" rid="bib1.bibx42" id="text.18"/>  and <xref ref-type="bibr" rid="bib1.bibx53" id="text.19"/> in the western basin.</p>
      <p>In this paper, we focus on the northern part of the western basin. As shown
by satellite analysis <xref ref-type="bibr" rid="bib1.bibx9 bib1.bibx6" id="paren.20"/> this area is on
average at the northern bound of the desert dust influence zone while it is
also directly affected by the emissions of the large industrial and urban
areas of southern France, eastern Spain and northern Italy. We present in
this paper the observations on aerosol vertical profiles performed in Corsica
Island from 2011 to 2013 using a backscatter lidar located in the north of
the island. The northern tip of Corsica has already been identified as an
adequate location for atmospheric chemistry measurements
<xref ref-type="bibr" rid="bib1.bibx28" id="paren.21"/>. The system was operated continuously from
February 2011 to April 2011 and from February 2012 up to August 2013. The
lidar data are analyzed together with concurrent sun photometer and satellite
data that are presented in the next section. We present the methods used for
retrieving the profile of aerosol extinction coefficient from lidar signal
and we analyse the time series of aerosol layer altitude and optical
properties. Significant events in terms of their contribution to the total
aerosol depth are then discussed.</p>
</sec>
<sec id="Ch1.S2">
  <title>Aerosol optical depth from sun photometer and satellite</title>
      <p>An automated CIMEL-318 sun photometer <xref ref-type="bibr" rid="bib1.bibx25" id="paren.22"/> was set up for the first time in June 2008 in Ersa (43.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E).
However due to large gap in the data during the lidar operation period, we didn't use this database in the present paper.
Another sun photometer has been set up on 14 July 2012 in the outskirt of Bastia (42.67<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.43<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), a town of approx. 50 000 inhabitants.
The sun photometer measured the direct sun irradiance in spectral channels at 440, 675, 860, 1020 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> at 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> intervals.
A channel at 940 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>  is used to retrieve the water vapor columnar content.
We have used in this study the level 1.5 aerosol optical depth (AOD) delivered by the version 2 of the direct sun algorithm of the AERONET project.
The AOD is extrapolated to 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> from measurements at 440 and 675 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> using a power law <xref ref-type="bibr" rid="bib1.bibx4" id="paren.23"/>.</p>
      <p>There is a remaining gap in the sun photometer time series in spring 2012. To
fill this gap we have collected the AOD retrieved from the Spinning Enhanced
Visible and Infrared Imager (SEVIRI) aboard Meteosat Second Generation
geostationnary satellite. SEVIRI measures radiances in three spectral solar
channels useful for aerosol study (0.6, 0.8 and 1.6 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) every
15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> with a spatial resolution of 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> at nadir. The
physical background and validation of the algorithm for the AOD and
Ångström exponent retrieval is described in <xref ref-type="bibr" rid="bib1.bibx50" id="text.24"/>.
The AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> and the Ångström exponent maps can be
downloaded from the ICARE center database
(<uri>http://www.icare.univ-lille1.fr</uri>). The aerosol parameters are retrieved
only over the sea and for cloud free pixels. We have selected and averaged
all the pixels within a range of 25 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> from the lidar site for each
of the 15 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula> slots. The AOD at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is extrapolated from
550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> by using a power law and the corresponding Ångström
coefficient. The hourly average AOD is computed for hours with at least 2
observations.</p>
      <p>We have performed a validation of the SEVIRI AOD by comparing the  hourly mean SEVIRI AOD to the AOD measured by the sun photometer in Bastia from July 2012 to August 2013 corresponding to a total of 1574 data.
Figure <xref ref-type="fig" rid="App1.Ch1.F1"/> shows that the extrapolated AOD fits very well the sun photometer measured ones with a correlation coefficient of <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>R</mml:mi><mml:mo>=</mml:mo><mml:mn>0.91</mml:mn></mml:mrow></mml:math></inline-formula>.
The intercept of 0.01 is within the error generaly admitted for the sun photometer AOD.
The slope (<inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.97</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>) indicates a slight underestimation of the satellite retrieved AOD that could be due to the fact that the photometer is situated inland in a peri-urban area whereas SEVIRI marine pixels are several km off from the coast.</p>
      <p>Figure <xref ref-type="fig" rid="App1.Ch1.F2"/> shows the time series of the daily mean
SEVIRI AOD and derived Ångström exponent from February 2011 to August
2013. AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> ranges between 0.05 and 0.8 and Ångström
exponent between 0.04 and 1.78 respectively. The AOD remains close to 0.1
from October to March while during spring and summer we observe a much higher
variability. 90 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the daily mean AOD remains below 0.26. The
times series indicate that the atmosphere over Corsica Island is hardly
affected by turbid events with large AOD.</p>
</sec>
<sec id="Ch1.S3">
  <title>Lidar observations</title>
      <p>We performed in situ soundings with a Rayleigh–Mie
backscatter lidar ALS 300 manufactured by Leosphere <xref ref-type="bibr" rid="bib1.bibx32" id="paren.25"/>. The
lidar uses a tripled, pulsed Nd : YAG laser source at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> with
an output energy of 16 mJ and a pulse repetition of 20 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Hz</mml:mi></mml:math></inline-formula>.</p>
      <p>The time acquisition for each profile is about 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">min</mml:mi></mml:math></inline-formula>, corresponding to an average of 1000 shots.
The raw signals are range-corrected.
The sky background signal is estimated in the far field and subtracted to the raw signal.
The correcting overlap factor for short-range heights where the field of view of the telescope does not overlap the laser beam is estimated from a series of horizontal shots when the atmosphere is stable.
This factor is over 0.8 at 120 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> above the telescope and close to 1 at 360 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>.
The lidar was tilted by a zenith angle of 15<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> to the North so the step in altitude is 14.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>.
We consider only the altitude levels above 145 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>
The lidar was set up  for the first time from 15 February to 14 April 2011 at the sun photometer site in Bastia.
It was reinstalled at the same place on 15 February 2012 and was operating until 28 August 2013.
The lidar was moved 50 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> southward in San-Giuliano (42.28<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.51<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) from the 22 June to the 11 July 2012.
This dataset is included in the present study.
The overall data base contains more than 170 000 profiles.
In the following, we consider only hourly average, leading to about 14 000 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> of observations.</p>
<sec id="Ch1.S3.SS1">
  <title>Cloud screening</title>
      <p>The aerosol extinction coefficient is not retrieved in case of clouds below
the reference level. Indeed, clouds will drastically decrease the
signal-to-noise ratio or even prevent the laser beam to reach clear air. The
retrieval of aerosol extinction coefficient requires avoiding any
contamination of the profiles by low clouds. Low clouds can be detected in
the lidar profiles because they are associated with a sharp increase in the
return signal that is highly variable from one shot to the other. The cloudy
profiles are automatically detected using a simple procedure commonly used in
satellite image processing <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx37" id="paren.26"/>.
We select a set of 3 consecutive profiles over a period of 24 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula>. The
profiles are standardized. For each altitude and each set of 3 consecutive
hourly profiles we compute the <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> neighborhood mean and standard
deviation. Cloudy structures have an abnormal mean and standard deviation. We
retain a threshold of 1.0 for the mean and 0.5 for the standard deviation,
i.e. above such thresholds the profile is flagged as cloudy.
Figure <xref ref-type="fig" rid="App1.Ch1.F3"/> is an example of cloud masking obtained between
24 and 27 May 2012. Gray areas correspond to the cloud mask. During this
period, all the clouds between 2 and 6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> are detected
(Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>a) and the corresponding contaminated profiles
are automatically discarded (Fig. <xref ref-type="fig" rid="App1.Ch1.F3"/>b).</p>
      <p>Such a procedure removes 52 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the total number of the 14 370 hourly acquired profiles.
On a monthly basis, the screening ranges between a minimum of 26 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of cloudy data in August 2012 to a maximum of 72 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> in March 2013.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <title>Extinction coefficient</title>
      <p>The aerosol extinction coefficient is retrieved from the range-corrected attenuated backscattering signal following the Klett's method <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx17 bib1.bibx5" id="paren.27"/> and considering both molecules and aerosols.
The calibration of the lidar profiles is given as the initial condition used for solving the differential form of the lidar equation for the range corrected signal <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>.
The solution for the aerosol backscattering coefficient <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is

                <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced open="[" close="]"><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msubsup><mml:mo>∫</mml:mo><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>R</mml:mi></mml:msubsup><mml:mo>[</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>]</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">d</mml:mi><mml:mi>r</mml:mi></mml:mfenced></mml:mrow><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:msubsup><mml:mo>∫</mml:mo><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>R</mml:mi></mml:msubsup><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mspace linebreak="nobreak" width="0.25em"/><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">d</mml:mi><mml:mi>r</mml:mi></mml:mrow></mml:mfrac></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is molecular backscattering coefficient, and

                <disp-formula id="Ch1.E2" content-type="numbered"><mml:math display="block"><mml:mrow><mml:mi>T</mml:mi><mml:mo>(</mml:mo><mml:mi>r</mml:mi><mml:mo>,</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi>exp⁡</mml:mi><mml:mfenced open="[" close="]"><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:munderover><mml:mo movablelimits="false">∫</mml:mo><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>r</mml:mi></mml:munderover><mml:mo>[</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msup><mml:mi>r</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>)</mml:mo><mml:mspace width="0.25em" linebreak="nobreak"/><mml:mi mathvariant="normal">d</mml:mi><mml:msup><mml:mi>r</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are the particulate and molecular
lidar ratio, respectively. The extinction coefficient is given by

                <disp-formula id="Ch1.E3" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo><mml:mo>⋅</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></disp-formula></p>
      <p>The initial condition <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> (Eq. <xref ref-type="disp-formula" rid="Ch1.E4"/>) is taken in the far range <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and above 7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height where the aerosol contribution is negligible compared to the molecular one.

                <disp-formula id="Ch1.E4" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msup><mml:mi>S</mml:mi><mml:mo>*</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mfrac><mml:mrow><mml:mi>S</mml:mi><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msub><mml:mi mathvariant="italic">β</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi>R</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mrow></mml:math></disp-formula></p>
      <p>The choice of an adequate aerosol lidar ratio (ratio of aerosol extinction to
backscattering coefficient) is a key issue in the analysis of single
wavelength backscattering lidar data. This parameter may vary between 27 Sr
for maritime aerosol and 71 Sr for urban/industrial pollution at
550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx11" id="paren.28"/>. The lidar ratio is a function of the
altitude as it depends on the vertical stratification of the atmosphere, and
on the aerosol optical properties transported in the different layers, their
hygroscopicity, and the profile of relative humidity. In case of a single
wavelength backscattering lidar, we can't derive any information on the
vertical variability of this parameter so the lidar ratio is first assumed to
be constant as a function of the altitude. The AOD is used as a constrain for
the lidar ratio selection in the extinction retrieval
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx29" id="paren.29"/>. Different values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are
tested until the vertical integration of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
(Eq. <xref ref-type="disp-formula" rid="Ch1.E3"/>) is equal to the sun photomoter AOD. When no AOD
value is available (nighttime or clouds) we use the same <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>
as the previous retrieval. It means that during nighttime, the extinction
profiles are retrieved using the <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mi mathvariant="normal">a</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> given by the lastest
inversion on the preceding day. Post-processing of daily mean AOD indicates
that AOD above 1.2 corresponds to remaining cloud contamination and so the
lidar extinction coefficient profiles are removed from the data set.</p>
      <p>The fix lidar ratio retrieved when constraining the retrieval of the hourly extinction profiles with the satellite AOD ranges between 22 and 108 Sr with an average value of <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>54</mml:mn><mml:mo>±</mml:mo><mml:mn>23</mml:mn></mml:mrow></mml:math></inline-formula> Sr.
This estimation is made over the 1836 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">h</mml:mi></mml:math></inline-formula> of simultaneous satellite and lidar observations during daytime.
There is a slight increase in the lidar ratio as a function of the AOD.
Considering AOD below 0.05 the average lidar ratio is 42 Sr while it is 62 Sr in high aerosol condition, i.e. when AOD is above 0.5.</p>
      <p>Figure <xref ref-type="fig" rid="App1.Ch1.F4"/> presents the comparison between sun photometer, lidar and satellite AOD at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> on a monthly basis.
There is an excellent consistency for the months were all the measurements are available.
A seasonal cycle is clearly observed with minima in winter and maxima in spring–summer.
Local maxima are observed in July 2012 (0.4), July 2013 (0.44) and in March 2012 (0.28).
However no clear maximum is observed in spring 2013.</p>
      <p>The monthly mean aerosol extinction profiles (Fig. <xref ref-type="fig" rid="App1.Ch1.F5"/>) shows a weak variability.
The extinction coefficient tends to increase above 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> from April to June and in September which probably corresponds to the overpass of dust events.
The extinction coefficient below 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> is maximum from June to September which correponds in majority to the period of polluted photochemical or smoke aerosol events.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <title>Comparison with ground-level data</title>
      <p>A TSI 3-wavelength integrating nephelometer was operated at the Ersa station
(43.0<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 9.35<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, 530 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula>) since
May 2012. The nephelometer is located 37 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> away from the lidar on
a North–South axis. The pseudo-total backscattering (integration of the
scattering function for scattering angles between 7<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">a</mml:mi></mml:math></inline-formula>nd
170<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>) is measured at 450, 550 and 700 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>. The
error due to the truncation in the phase function is corrected following
<xref ref-type="bibr" rid="bib1.bibx3" id="text.30"/>. The aerosol scattering coefficient is extrapolated
to 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> from the measurements at 450 and 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> following
the Ångström law.</p>
      <p>Figure <xref ref-type="fig" rid="App1.Ch1.F6"/> shows the comparison between the daily mean total aerosol scattering coefficient derived from the integrating nephelometer and the mean aerosol extinction coefficient between 450 and 550 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> derived from the lidar.
The extinction coefficient is the sum of the scattering and absorption coefficient and so it has to be higher or egal to the scattering coefficient.
Since the measurement sites are not collocated it is not possible to estimate the single scattering albedo, that is the ratio between scattering and extinction coefficient.
However we have a similar trend showing low scattering, respectively extinction coefficient during winter period and a maximum value in July 2013.
When considering the coincident data the correlation coefficient is 0.63 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn>302</mml:mn></mml:mrow></mml:math></inline-formula> data).</p>
</sec>
<sec id="Ch1.S3.SS4">
  <title>Layer altitude</title>
      <p>The variation in the aerosol concentration and optical properties between the
different layer induces gradients in the attenuated range corrected lidar
signal. In the lower part of the atmosphere where the signal to noise ratio
is the higher, we classify at least two layers using the second derivative of
the lidar signal <xref ref-type="bibr" rid="bib1.bibx35" id="paren.31"/>. In the upper part of the atmosphere where
the gradients and the signal to noise ratio are smaller the derivative of the
signal doesn't lead a clear detection of the dust layer. As an indicator of
the vertical development of the aerosol layer, we compute the AOD scale
height, i.e. the altitude at which <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>/</mml:mo><mml:mi>e</mml:mi></mml:mrow></mml:math></inline-formula> of the total AOD is below that point
<xref ref-type="bibr" rid="bib1.bibx52 bib1.bibx29" id="paren.32"/>.</p>
      <p>We detect a shallow marine boundary layer on most of the profiles.
The average altitude is <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>380</mml:mn><mml:mo>±</mml:mo><mml:mn>260</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>.
A weak seasonal cycle is observed with a summer maximum at 460 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> in July and a winter minimum at 250 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> in December.
The daytime variability is also lower during winter months (November to March).
We also detect a secondary maximum in the derivative of the lidar signal located between 700 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula> and 3.5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> and on average at <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>1.3</mml:mn><mml:mo>±</mml:mo><mml:mn>0.5</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>.
This secondary gradient in the lidar signal can be due to the complex local atmospheric circulation because of the proximity of both the sea shore and the high topography of the island.
The mean scale height is  <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>4.1</mml:mn><mml:mo>±</mml:mo><mml:mn>1.6</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>.
The scale height reaches 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> during the dust outbreak in March 2013.
Below the scale height the mean hourly aerosol extinction coefficient is <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.07</mml:mn><mml:mo>±</mml:mo><mml:mn>0.17</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.
It is <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>0.05</mml:mn><mml:mo>±</mml:mo><mml:mn>0.08</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> in the marine boundary layer.</p>
</sec>
<sec id="Ch1.S3.SS5">
  <title>Synthesis</title>
      <p>The two main phenomena leading to strong AODs over Corsica are dust outbreaks
from Northern Africa and advection of pollution or biomass burning from
Europe. The AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> and the Ångström coefficient are
used to classify 3 types of aerosol conditions: maritime, dust and pollution
aerosols. Maritime situations correspond to AOD below 0.3
<xref ref-type="bibr" rid="bib1.bibx9" id="paren.33"/> whatever values of the Ångström coefficient.
Pollution aerosol conditions are identified with AOD above 0.3 and
Ångström coefficient above 1.2 while dust cases correspond to AOD
above 0.3 and Ångström coefficient below 0.9 <xref ref-type="bibr" rid="bib1.bibx24" id="paren.34"/>.
From February 2012 to August 2013, only 28 out of 341 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula> of
observation have an AOD above 0.3, i.e. 8 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the observations.
Among those 28 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>, 43 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> (12 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>) are identified
as dust and 32 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> (9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>) as pollution events.</p>
      <p>In Table <xref ref-type="table" rid="App1.Ch1.T1"/> we give the daily average aerosol properties
according to the previous classification. Low AOD denomination corresponds to
maritime situation for which the AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is below 0.1. The
average AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is higher for the dust than for the pollution
cases. However because of the high Ångström exponent for polluted
fine particles, it is the opposite at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>. Considering cases with
a low AOD, the Ångström exponent is 0.52 indicating a main
contribution of large sea salt particles. The lidar ratio at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>
for those cases is 49 Sr. The effective lidar ratio found for dust is 63
(<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>18</mml:mn></mml:mrow></mml:math></inline-formula>) Sr. This value is higher than the one retrieved by
<xref ref-type="bibr" rid="bib1.bibx38" id="text.35"/> but in the range of previously
published values in the Mediterranean <xref ref-type="bibr" rid="bib1.bibx8" id="paren.36"/>. However, in
our case the lidar ratio is not vertically resolved and thus is biased by the
contribution of marine and pollution aerosols in the marine boundary layer.
In the case of the long range transport of pollution aerosols which occurs at
a lower altitude as it is shown by the lower scale height, the lidar ratio of
69 Sr is more reliable and in a better agreement with previously published
values <xref ref-type="bibr" rid="bib1.bibx1" id="paren.37"/>. The high scale height
for low AOD is due to the weak contribution of the clean boundary layer to
the total AOD. The difference in the altitude of the transport for dust and
pollution aerosols is highlighted by a higher scale height for dust than for
pollution particles. In the next section, we focus on this difference by
analyzing selected case studies.</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <title>Discussion on specific events</title>
<sec id="Ch1.S4.SS1">
  <title>Analysis of satellite data</title>
      <p>Figure <xref ref-type="fig" rid="App1.Ch1.F7"/> shows the daily mean AOD over the western
Mediterranean basin during the dust events which affected Cap Corse during
2012–2013 period. The major dust event in terms of AOD occurred in
April–May 2013 (Fig. <xref ref-type="fig" rid="App1.Ch1.F7"/>d) with a paroxysm on 30 April
when the AOD reached 0.89 (daily mean at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>). SEVIRI
Ångström exponent is 0.27 indicating a large contribution of coarse
particles to the AOD. Such corridor is a well known feature of the dust
transport in the Mediterranean <xref ref-type="bibr" rid="bib1.bibx24" id="paren.38"/> and forms when
low-pressure systems enter the northwestern part of the basin
<xref ref-type="bibr" rid="bib1.bibx21" id="paren.39"/> in spring or autumn <xref ref-type="bibr" rid="bib1.bibx53" id="paren.40"/>. The dust storm is
associated with clouds that prevent from retrieving AOD over large parts of
the plume and lead to a patchy structure when averaging during the whole dust
event between 30 April to 4 May 2012. The second dust event in magnitude
observed over the site occurred in June–July 2012
(Fig. <xref ref-type="fig" rid="App1.Ch1.F7"/>b) with a SEVIRI AOD at 0.8 on 30 June 2012
<xref ref-type="bibr" rid="bib1.bibx39" id="paren.41"/>. In this case the advection pattern is different. The
saharan air layer advected over north-east Atlantic and western Spain during
the dust event is recirculated to the northwestern part of the basin by
westerly winds. A larger SEVIRI Ångström exponent of 0.6 is observed
for this dust outbreak which can be linked to a smaller contribution of large
particles to the AOD than in the case of spring event. A similar pattern is
observed for the 19 June 2012 (Fig. <xref ref-type="fig" rid="App1.Ch1.F7"/>a). Finally, the
Fig. <xref ref-type="fig" rid="App1.Ch1.F7"/>d shows the case of a dust storm in the western
basin on July 2012 where the core of the dust plume doesn't reach the Cap
Corse and the gulf of Genova so the AOD remains rather weak in this area.</p>
      <p>The highest pollution event observed occurred on July 2013.
Figure <xref ref-type="fig" rid="App1.Ch1.F8"/>d shows the mean daily SEVIRI AOD between
13–20 July 2013. The SEVIRI AOD reached 0.53 (daily mean) on 14 July and
increased to 0.6 on 15 July. The Ångström exponent is 1.33 so leading
to an AOD of 0.95 at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> on 14 July 2013. During this period, the
pollution plume is observed all along the northern coast of the basin
including the Balearic islands and Corsica (Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/>d)
while a local maximum at 0.4 is observed in the gulf of Genova. A rather
similar case was observed on 6 September 2012
(Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/>c). However the plume is limited to the gulf of
Genova. The geographic position of the low pressure system in the northern
basin affects the extent of the plume. In this case the low is located in the
gulf of Genova, while in July 2013 it is located westward over Spain. The
second major pollution event in term of AOD occurs on 26 March 2012. SEVIRI
observations indicate a large plume crossing the northern part of the western
basin (Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/>a). The corresponding daily mean AOD at
355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is 0.75 and the Ångström exponent is 1.25. This
moderate value tends to indicate a possible contribution of large particles.
In this case the low is southward over Sicily bringing more continental air
from central Europe to the basin. The case of August 2012
(Fig. <xref ref-type="fig" rid="App1.Ch1.F8"/>b) is ambiguous because despite an
Ångström exponent of 1.3 the satellite pictures indicates a possible
contribution of dust particles from northern Africa.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <title>Vertical profiles and air mass origin</title>
      <p>We further analyze the stratification of the aerosol layers and their possible origin and transport pathway.
The air mass origins for the aforementioned specific events are analyzed using the Lagrangian particle dispersion model FLEXPART <xref ref-type="bibr" rid="bib1.bibx49" id="paren.42"/>.
The model is run in backward mode <xref ref-type="bibr" rid="bib1.bibx47" id="paren.43"/> over 10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">days</mml:mi></mml:math></inline-formula>.
The meteorological forcing is given by ECMWF operational analysis at 0.5<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.
The plume is computed using 1 000 000 particles released for a given range of altitudes and arriving in <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">1</mml:mn><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> box centered on the Cap Corse station.
The ranges of altitudes are selected to highlight some particular features of the aloft aerosol transport.
The residence time is computed for the whole duration of the simulation and integrated between the surface level and the top altitude of the release.
The retroplume residence times (in seconds) gives the density of probability of the origin of the air mass that arrived at the station in the given altitude range from below altitudes.</p>
      <p>Figure <xref ref-type="fig" rid="App1.Ch1.F9"/> presents the vertical profiles of the aerosol extinction coefficient obtained during the aforementioned events.
Lidar data were not available on 19 June 2012.
Figure <xref ref-type="fig" rid="App1.Ch1.F9"/>a to <xref ref-type="fig" rid="App1.Ch1.F9"/>e is for dust events and Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>f to <xref ref-type="fig" rid="App1.Ch1.F9"/>i is for pollution events.
The main feature corresponding to the pollution cases profiles is the low level of altitude in the transport of aerosols.
The 26 March 2012 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>f) and 6 September 2012 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>h) are very similar in terms of vertical distribution showing a thick layer between 1 and 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height.
The backward simulations of the air masses arriving at the station between 500
and 2000 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> (Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>a and b) indicates a most probable transport from Eastern Europe.
The aerosol extinction coefficient in the pollution layer reached 0.15 and 0.25 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> on 26 March and 6 September 2012, respectively.
The value of extinction coefficient encountered during those events might be explained by the advection of air masses contaminated by biomass burning by-products originating from southeast Europe.
Indeed for both events,  Global Fire Assimilation System <xref ref-type="bibr" rid="bib1.bibx26" id="paren.44"/> biomass burning emission inventory shows biomass burning emissions on the pathways of air masses arriving to the Cap Corse (not shown here).</p>
      <p>The case of summer 2012 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>g) and summer 2013 shows
additional elevated layers. The extinction coefficient below 700 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">m</mml:mi></mml:math></inline-formula>
increased from 0.09 to 0.19 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> from 20 to 25 August 2012 showing
the build up of the pollution event during this period. Below 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>
height, the air mass was originating from the gulf of Genova and coastal
areas of Italy. The aerosol layer observed between 2.5 and 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>
height was originating from Spain and Southern France
(Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>c) and passed over the Pyrenees mountain range.
The backward plume shows also a possible northwestern African origin and thus
possibly carrying dust that might explains the rather low value for the
Ångström exponent.</p>
      <p>During the month of July 2013 we observed a large increase in the AOD (Fig. <xref ref-type="fig" rid="App1.Ch1.F2"/>).
This increase was also well observed in the aerosol scattering coefficient measured at the Ersa station (Fig. <xref ref-type="fig" rid="App1.Ch1.F6"/>).
Below 1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> the aerosols are originating from the Pô valley (northern Italy) and we observed a large variability in the extinction coefficient ranging between 0.1 on the 15 July (<xref ref-type="fig" rid="App1.Ch1.F9"/>i, black solid line) and almost 0.2 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (<xref ref-type="fig" rid="App1.Ch1.F9"/>g, red solid line) on the 19 July.
A large aerosol layer was observed aloft between 2 and 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>i).
The air mass backtrajectory (Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>d)  indicated that the air mass was originating from northern Europe and underwent an ascent over the Alps before arriving above Cap Corse.
An additional aerosol layers was also observed between 1 and 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height during the pollution event.</p>
      <p>The dust events observed during summer 2012 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>a and b) are rather similar in terms of vertical distribution.
We observed a thick dust layer with a top located at 5 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height.
The maximum extinction coefficient in the dust layer is 0.12 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.
The bottom of the layer is located between 2 and 3 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.
The air mass origin simulations indicate a transport of dust from North western Africa.
In late June (Figs. <xref ref-type="fig" rid="App1.Ch1.F9"/>a and <xref ref-type="fig" rid="App1.Ch1.F10"/>e) the plume is first advected over the Atlantic and then transported to the east over the strait of Gibraltar.
While the dust case in July (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>b) shows an advection of the plume east of the coast of Spain (Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>f).
The event observed in July 2013 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>d) has a lower extinction coefficient at 0.06 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> but with a similar vertical structure than the previous cases.
The advection pattern of the dust (not shown) was the same as for the case in June 2012.
On August 2013 (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>e) the profile shows a dust layer up to 7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula>.
The extinction coefficient is 0.1 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> however such a high altitude event has an impact on the estimation of the extinction coefficient as the reference zone is affected by aerosols.
The air mass backward simulations show the advection of the dust from the northwestern Sahara with an ascent over the Atlas mountain range (Fig. <xref ref-type="fig" rid="App1.Ch1.F10"/>g).</p>
      <p>A large dust layer arrived on the 30 April (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>c, black solid line) between 1 and 4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height with extinction coefficient over 0.3 <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>.
To highlight the variability in the aerosol vertical distribution during the dust event in April–May 2013  (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>c) we plotted the aerosol extinction on the 30 April and the 2 May.
As the dust event passed over the site (Fig. <xref ref-type="fig" rid="App1.Ch1.F9"/>c, red solid line), we observed an increase in the extinction coefficient below 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> while the aloft layer vanished.
Figure <xref ref-type="fig" rid="App1.Ch1.F10"/>h highlights an advection pattern that is different to the summer cases.
The dust is transported in a southerly flow across north-western Sahara and then over Tunisia before reaching the station.
This kind of synoptic situation favors first the transport in altitude of air masses uplift in northwestern Sahara and then the low level transport of dust from closest sources in southern Tunisia.</p>
</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>We present for the first time lidar observations in
the north of Corsica Island during more than a year. The combined analysis of
satellite and lidar observation shows that the aerosol optical depth in the
northern part of the western basin remains moderate most of the time. The AOD
has a clear seasonal cycle with minima during winter and maxima in spring and
summer. The increase in the AOD is linked to the large scale advection of
polluted air masses from Europe or dusty air masses from North Africa.
However large AOD events (above 0.3 at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>) represent less than
10 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">%</mml:mi></mml:math></inline-formula> of the observation days. The average low influence of desert
dust events in this area has also been observed by <xref ref-type="bibr" rid="bib1.bibx43" id="text.45"/>
using ground level <inline-formula><mml:math display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">PM</mml:mi><mml:mn>10</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass concentration. For the observed
aerosol events the average AOD at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is 0.61 for dust and 0.71
for pollution aerosols, respectively. The higher AOD for pollution aerosols
at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> is associated to a high Ångström exponent, 1.38
compared to 0.60 for dust.</p>
      <p>During pollution events, the large increase in the extinction coefficient below 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> is due to the build up of pollution into the gulf of Genova.
We have also observed the transport of polluted air masses above 2 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height either from northern or southwestern Europe and reaching the measurement site after been advected over mountainous areas.
Saharan dust transport can be stratified in different layers located between the ground level and up to 7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">km</mml:mi></mml:math></inline-formula> height, which is an upper detection limit for the lidar system.
The largest dust event in term of AOD is observed during spring and corresponds to a south-north advection of dusty air masses over north-western Africa with an outlet over Tunisia.
Other cases are observed in summer and show that the dust is advected to Corsica by westerly winds after being uplifted in Morocco and Algeria and ejected in the western part of the basin.</p>
      <p>Our observations corroborate previous studies on the vertical distribution and properties of Mediterranean aerosols <xref ref-type="bibr" rid="bib1.bibx48" id="paren.46"/>.
The complex stratification of the aerosol transport over the western basin is due to the various origins of the particles, including pollution and biomass burning aerosols from Europe and mineral dust from Northern Africa, and the effect of the topography surrounding the basin.
This new dataset obtained in Cap Corse provides a new insight in the vertical distribution of aerosols in the Mediterranean and offers the opportunity to better understand the origin and transport pathways of those particles.</p>
</sec>

      
      </body>
    <back><ack><title>Acknowledgements</title><p>The project was supported financially by INSU, ADEME and IRD through MISTRAL/CHARMEX program.
The authors want to thank AERONET/PHOTONS team for providing and calibrating the sun photometer.
ICARE data center is also acknowledged for providing a free access to SEVIRI aerosol products.
The authors thank Qualitair Corse, DREAL Corse and INRA at San-Giuliano for providing local facilities and support.
This work is within the frame of CORSICA (Corsican Observatory for Research and Studies on climate and Atmosphere-ocean environment) sponsored by Communauté Territoriale de Corse and FEDER.</p></ack><ref-list>
    <title>References</title>

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  </ref-list><app-group content-type="float"><app><title/>

<?xmltex \floatpos{t}?><table-wrap id="App1.Ch1.T1"><caption><p>Mean aerosol optical depth (AOD) at 355 and 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>, Ångström
exponent, lidar ratio at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> and scale height.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.90}[.90]?><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"/>  
         <oasis:entry colname="col2">AOD  550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> (–)</oasis:entry>  
         <oasis:entry colname="col3">AOD 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> (–)</oasis:entry>  
         <oasis:entry colname="col4">Ang. Exp. (–)</oasis:entry>  
         <oasis:entry colname="col5">Lr 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> (Sr)</oasis:entry>  
         <oasis:entry colname="col6"><inline-formula><mml:math display="inline"><mml:mi>H</mml:mi></mml:math></inline-formula> (km)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">Total</oasis:entry>  
         <oasis:entry colname="col2">0.16 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col3">0.25 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.16</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">0.88 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.41</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col5">55 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>21</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col6">3.9 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>1.0</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Dust</oasis:entry>  
         <oasis:entry colname="col2">0.47 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.13</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col3">0.61 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.14</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">0.60 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.17</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col5">63 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>18</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col6">4.0 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.8</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">Anthrop.</oasis:entry>  
         <oasis:entry colname="col2">0.39 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col3">0.71 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.16</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">1.38 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.09</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col5">68 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>13</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col6">3.2 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.6</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">low AOD</oasis:entry>  
         <oasis:entry colname="col2">0.08 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col3">0.10 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col4">0.52 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.27</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col5">49 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>20</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>  
         <oasis:entry colname="col6">4.6 (<inline-formula><mml:math display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn>0.7</mml:mn></mml:mrow></mml:math></inline-formula>)</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <fig id="App1.Ch1.F1"><caption><p>Comparison between sun photometer and SEVIRI AOD. The wavelength is 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula>.</p></caption>
      <?xmltex \igopts{width=284.527559pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f01.pdf"/>

    </fig>

      <fig id="App1.Ch1.F2"><caption><p>SEVIRI daily mean <bold>(a)</bold> aerosol optical depth and <bold>(b)</bold>
Ångström exponent close to the lidar site.</p></caption>
      <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f02.pdf"/>

    </fig>

      <fig id="App1.Ch1.F3"><caption><p>Time series of the range corrected lidar signal between 24 and 27 May 2012. <bold>(a)</bold> Low level clouds and <bold>(b)</bold> corresponding profiles are shaded in gray.</p></caption>
      <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f03.pdf"/>

    </fig>

      <fig id="App1.Ch1.F4"><caption><p>Monthly mean AOD at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> for the lidar (averaged during day and night), Sun photometer and SEVIRI (only daytime) from January 2011 to December 2013.</p></caption>
      <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f04.pdf"/>

    </fig>

      <fig id="App1.Ch1.F5"><caption><p>Monthly mean aerosol extinction profiles at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> for (blue) 2012 and (black) 2013.</p></caption>
      <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f05.pdf"/>

    </fig>

      <fig id="App1.Ch1.F6"><caption><p>Nephelometer total scattering coefficient at Ersa station and mean extinction coefficient between 450 and 550 <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">a</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">s</mml:mi><mml:mo>.</mml:mo><mml:mi mathvariant="normal">l</mml:mi><mml:mo>.</mml:mo></mml:mrow></mml:math></inline-formula> derived from the lidar.</p></caption>
      <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f06.pdf"/>

    </fig>

      <fig id="App1.Ch1.F7"><caption><p>Mean daily SEVIRI AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> corresponding to identified dust
episodes at Cap Corse <bold>(a)</bold> for 19 June 2012, <bold>(b)</bold> from
29 June to 1 July 2012, <bold>(c)</bold> from 27 to 28 July 2012,
<bold>(d)</bold> from 30 April to 4 May 2013, <bold>(e)</bold> 28 July 2013 and
<bold>(f)</bold> 4 to 6 August 2013.</p></caption>
      <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f07.pdf"/>

    </fig>

      <fig id="App1.Ch1.F8"><caption><p>Mean daily SEVIRI AOD at 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> corresponding to identified pollution episodes at Cap Corse <bold>(a)</bold> for 26 March 2012, <bold>(b)</bold> 23 August 2012, <bold>(c)</bold> 6 September 2012, <bold>(d)</bold> from 13 to 20 July 2013.</p></caption>
      <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f08.pdf"/>

    </fig>

      <fig id="App1.Ch1.F9"><caption><p>Vertical profiles of the aerosol extinction coefficient at 355 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">nm</mml:mi></mml:math></inline-formula> for
selected events: <bold>(a)</bold> 29 June to 1 July 2012, <bold>(b)</bold>
27–28 July 2012, <bold>(c)</bold> 30 April (black solid line) and 2 May 2013
(red solid line), <bold>(d)</bold> 28 July 2013, <bold>(e)</bold> 4 August 2013,
<bold>(f)</bold> 26 March 2012, <bold>(g)</bold> 23 August 2012, <bold>(h)</bold> 6
September 2012, and <bold>(i)</bold> 15 (black solid line) and 19 (red solid
line) July 2013.</p></caption>
      <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f09.pdf"/>

    </fig>

      <fig id="App1.Ch1.F10"><caption><p>Backward simulations of the residence time for air masses (in seconds) arriving at Cap Corse using the Lagrangien particle dispersion model FLEXPART.
The range of altitude for each release and the time period of the simulation
are given at the top of each subplot labeled from <bold>(a)</bold> to <bold>(h)</bold>.</p></caption>
      <?xmltex \igopts{height=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/preprints/15/9507/2015/acpd-15-9507-2015-f10.pdf"/>

    </fig>

    </app></app-group></back>
    </article>
