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  <front>
    <journal-meta>
<journal-id journal-id-type="publisher">AMT</journal-id>
<journal-title-group>
<journal-title>Atmospheric Measurement Techniques</journal-title>
<abbrev-journal-title abbrev-type="publisher">AMT</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">Atmos. Meas. Tech.</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub">1867-8548</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/amt-9-3391-2016</article-id><title-group><article-title>Comparison of aerosol properties retrieved using GARRLiC, LIRIC, and Raman algorithms applied to multi-wavelength lidar and sun/sky-photometer data</article-title>
      </title-group><?xmltex \runningtitle{Aerosol properties derived using some algorithms}?><?xmltex \runningauthor{V. Bovchaliuk et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Bovchaliuk</surname><given-names>Valentyn</given-names></name>
          <email>bovchaliukv@gmail.com</email>
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Goloub</surname><given-names>Philippe</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Podvin</surname><given-names>Thierry</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Veselovskii</surname><given-names>Igor</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Tanre</surname><given-names>Didier</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Chaikovsky</surname><given-names>Anatoli</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Dubovik</surname><given-names>Oleg</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3482-6460</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Mortier</surname><given-names>Augustin</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7724-3583</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Lopatin</surname><given-names>Anton</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff2">
          <name><surname>Korenskiy</surname><given-names>Mikhail</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-7374-6896</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Victori</surname><given-names>Stephane</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Laboratoire d'Optique Atmospherique, Lille1 University, Villeneuve d'Ascq, France</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Physics Instrumentation Center of the General Physics Institute, Troitsk, Moscow Region, Russia</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Institute of Physics, NAS of Belarus, Minsk, Belarus</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Norwegian Meteorological Institute, Oslo, Norway</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>Cimel advanced monitoring, Paris, France</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Valentyn Bovchaliuk (bovchaliukv@gmail.com)</corresp></author-notes><pub-date><day>28</day><month>July</month><year>2016</year></pub-date>
      
      <volume>9</volume>
      <issue>7</issue>
      <fpage>3391</fpage><lpage>3405</lpage>
      <history>
        <date date-type="received"><day>6</day><month>February</month><year>2016</year></date>
           <date date-type="rev-request"><day>9</day><month>March</month><year>2016</year></date>
           <date date-type="rev-recd"><day>3</day><month>July</month><year>2016</year></date>
           <date date-type="accepted"><day>5</day><month>July</month><year>2016</year></date>
      </history>
      <permissions>
<license license-type="open-access">
<license-p>This work is licensed under a Creative Commons Attribution 3.0 Unported License. To view a copy of this license, visit <ext-link ext-link-type="uri" xlink:href="http://creativecommons.org/licenses/by/3.0/">http://creativecommons.org/licenses/by/3.0/</ext-link></license-p>
</license>
</permissions><self-uri xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016.html">This article is available from https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016.html</self-uri>
<self-uri xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016.pdf">The full text article is available as a PDF file from https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016.pdf</self-uri>


      <abstract>
    <p>Aerosol particles are important and highly variable components of the
terrestrial atmosphere, and they affect both air quality and climate. In
order to evaluate their multiple impacts, the most important requirement is
to precisely measure their characteristics. Remote sensing technologies such
as lidar (light detection and ranging) and sun/sky photometers are powerful
tools for determining aerosol optical and microphysical properties. In our
work, we applied several methods to joint or separate lidar and
sun/sky-photometer data to retrieve aerosol properties. The Raman technique
and inversion with regularization use only lidar data. The LIRIC
(LIdar-Radiometer Inversion Code) and recently developed GARRLiC (Generalized
Aerosol Retrieval from Radiometer and Lidar Combined data) inversion methods
use joint lidar and sun/sky-photometer data. This paper presents a comparison
and discussion of aerosol optical properties (extinction coefficient profiles
and lidar ratios) and microphysical properties (volume concentrations,
complex refractive index values, and effective radius values) retrieved using
the aforementioned methods. The comparison showed inconsistencies in the
retrieved lidar ratios. However, other aerosol properties were found to be
generally in close agreement with the AERONET (AErosol RObotic NETwork)
products. In future studies, more cases should be analysed in order to
clearly define the peculiarities in our results.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <title>Introduction</title>
      <p>In situ and remote sensing measurements are the two main approaches used for
aerosol observations. The former involves measurements of particles using
instruments at the survey points. The latter involves measuring aerosol
properties from a distance without direct interaction with particles. Remote
sensing methods can be categorized into active and passive depending on the
kind of instrument used. Instruments belonging to the passive category
measure the modified solar radiation after interactions with particles and
terrestrial radiation. One of the most common instruments in this category, a
sun/sky photometer, measures both direct and diffuse solar radiation. These
data can be used in inversion algorithms <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx14" id="paren.1"/> to
retrieve several column-integrated aerosol properties such as the aerosol
optical depth (AOD), single scattering albedo (SSA), particle size
distribution (SD), effective radius (<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), and complex
refractive index (CRI, including real (RRI) and imaginary (IRI) parts of
refractive index). Instruments belonging to the active category of remote
sensing measurement scattered radiation emitted by themselves; one of the most
well-regarded and widely used instrument in this category is lidar (light
detection and ranging). Lidar instruments are used for profiling atmospheric variables
such as the temperature, pressure, humidity, wind speed and its direction,
and the amount of trace gases and aerosols. The main advantages of lidar
measurements include high vertical resolution and applicability during
nighttime and in cloudy environments. Current multi-wavelength lidar
observations can provide comprehensive and quantitative information regarding
aerosol properties <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx48 bib1.bibx49 bib1.bibx36 bib1.bibx21" id="paren.2"/>.</p>
      <p>Several methods, techniques, and algorithms can be used to obtain the optical
and microphysical characteristics of aerosols. These methods generally use
different sets of data. For instance, AERONET (AErosol RObotic NETwork)
inversion code uses only sun/sky-photometer data <xref ref-type="bibr" rid="bib1.bibx12" id="paren.3"/>. Similarly,
the Raman technique and regularization algorithm use only lidar data
<xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx53 bib1.bibx43" id="paren.4"/>. The LIRIC (LIdar-Radiometer
Inversion Code) and GARRLiC (Generalized Aerosol Retrieval from Radiometer
and Lidar Combined data) algorithms, in contrast, use both the
sun/sky-photometer and lidar data <xref ref-type="bibr" rid="bib1.bibx29 bib1.bibx9" id="paren.5"/>. Because
these methods use different datasets, they are applicable during different
observational times. For instance, while the Raman technique is most suitable
for nighttime observations, sun/sky photometers do not make measurements at
that time. Further, the GARRLiC algorithm, which is included in the GRASP
(Generalized Retrieval of Atmosphere and Surface Properties) inversion code
<xref ref-type="bibr" rid="bib1.bibx14" id="paren.6"/>, can separate the fine and coarse modes of aerosols, thus
resulting in the retrieval of particle characteristics separately for both
modes. While different methods retrieve different sets of aerosol
characteristics, all of them are aimed at obtaining detailed results. The
objective of our study is to discriminate and compare the common aerosol
characteristics obtained through different methods.</p>
      <p>Section 2 describes the observation sites where the measurements were carried
out. This section also describes a new lidar system, called LILAS (LIlle
Lidar AtmosphereS), which was used at the observation sites. Section 3
presents the methods considered in our study and discusses their potential,
applicability, and the common aerosol properties that were considered for
comparison. Section 4 presents three dust cases that were selected and
analysed by using the algorithms described in Sect. 3. The main conclusions
and perspectives are given in the last section.</p>
</sec>
<sec id="Ch1.S2">
  <title>Observational sites and the lidar system</title>
      <p>The lidar system LILAS used in this work belongs to Laboratoire d'Optique
Atmospherique (LOA). This system is operated at the campus of Lille
University, France. The campus area is influenced mainly by urban and
industrial pollutant emissions, marine aerosols, and  mineral dust and
aerosols from volcanic eruptions several times every year
<xref ref-type="bibr" rid="bib1.bibx30" id="paren.7"/>. Other remote sensing and in situ instruments are also
operational at this site. Among them is a lunar photometer for observing AOD
and Ångström exponent (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>) values on clear nights within the half
moon to full moon lunar phases. LOA is a permanent lidar site. However, for
the study of Saharan dust over West Africa (SHADOW2 campaign), LILAS was
moved to M'Bour city (Dakar site) in Senegal at the beginning of January
2015. The Dakar site is influenced by mineral dust during March–April and
biomass burning during December–January. The two main objectives of the
campaign were (i) to record the physical and chemical properties of
aerosols over the regions impacted by considerable amounts of dust particles
and
(ii) to study the aerosol dynamics. Seven laboratories with 18 instruments
took part in the campaign.</p>
      <p>The LILAS system was assembled and setup in December 2013, and observations
started in January 2014. The system is composed of a laser (Spectra-physics,
INDI-40) emitting at wavelengths of 1064, 532, and 355 nm (100 mJ/20 Hz),
a Newton telescope, a beam rotator, and a receiving module. The beam rotator
can be used for near- or far-range observations by changing the overlap
function. Several receiving modules were added in April 2014, and the system
now consists of five elastic channels (355 and 532 nm both parallel and
perpendicular for analog and photo-counting; 1064 nm for total analog)
and three Raman channels (387 nm for analog and photo-counting; 408
and 608 nm for photo-counting). During the SHADOW2 campaign, the vibrational
Raman channel at 608 nm was changed to a rotational channel at 530 nm. This
rotational Raman channel showed a good and stable performance
<xref ref-type="bibr" rid="bib1.bibx48 bib1.bibx49" id="paren.8"/>. The system can be remotely operated and is
coupled with a radar (radio detection and ranging) for reasons such as
automatic discontinuation control and airplane safety.</p>
      <p>The Lille site became an observation station of the European Aerosol Research
LIdar NETwork (EARLINET) in the summer of 2014. The main goal of the network
is to provide a comprehensive, quantitative, and statistically significant
database on aerosol distributions. The network has some special criteria for
data quality assurance, such as a telecover test, a trigger delay, dark
measurements, depolarization calibration, and regular check-ups of the
Rayleigh fits <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx16 bib1.bibx17 bib1.bibx18" id="paren.9"/>. LILAS has passed all the EARLINET tests and check-ups
except for depolarization calibration, which is currently in progress.</p>
</sec>
<sec id="Ch1.S3">
  <title>Retrieval algorithms</title>
      <p>Depending on the lidar characteristics, different techniques can be used for
obtaining optical and microphysical properties of aerosols. All the methods
and algorithms that were used for data processing are introduced in this
section.</p>
      <p>Elastic-backscatter lidar is considered to be a classic form of lidar
technology <xref ref-type="bibr" rid="bib1.bibx53" id="paren.10"/>. This technology is based on the measurement
of elastically scattered light in the backward direction. The common method
that derives aerosol optical characteristics is the Klett method
<xref ref-type="bibr" rid="bib1.bibx26 bib1.bibx27" id="paren.11"/>. This method is based on the relationship
between the extinction and backscatter coefficients. The algorithm called
BASIC <xref ref-type="bibr" rid="bib1.bibx30" id="paren.12"/> based on the Klett method has been developed at
LOA and is successfully implemented into routine for mono-wavelength lidar
data. This algorithm retrieves an extinction coefficient profile
(<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">aer</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) following an iterative procedure based on a dichotomy
where the lidar ratio (LR) can vary in the range from 10 to 140 sr. The
procedure ends when the integral of the extinction profile is close to the
AOD measured by a sun/sky photometer within <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">Δ</mml:mi></mml:math></inline-formula>AOD <inline-formula><mml:math display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.01 accuracy.</p>
      <p>The Raman lidar technique is a widely known technique in the lidar community
for obtaining aerosol optical properties (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>, LR)
<xref ref-type="bibr" rid="bib1.bibx1" id="paren.13"/>. This technique is based on the scattering of incident
lidar light with photon energy shifts due to vibrational or rotational modes
of the molecules. It is mostly used at nighttime when the signal-to-noise
ratio is the highest, owing to the absence of sunlight scattered into the
field of view of the lidar. Assuming that the aerosol extinction coefficient
depends on the wavelength through <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>, the former can be found
calculated as <xref ref-type="bibr" rid="bib1.bibx53" id="paren.14"/>
          <disp-formula id="Ch1.E1" content-type="numbered"><mml:math display="block"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">aer</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="normal">d</mml:mi><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced open="[" close="]"><mml:mi>ln⁡</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:msup><mml:mi>z</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>+</mml:mo><mml:msup><mml:mfenced open="(" close=")"><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle></mml:mfenced><mml:mi mathvariant="italic">α</mml:mi></mml:msup></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
        where <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>P</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the power received at the Raman wavelength <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> from
distance <inline-formula><mml:math display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the molecule number density,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">σ</mml:mi><mml:mi mathvariant="normal">mol</mml:mi></mml:msub><mml:mo>(</mml:mo><mml:msub><mml:mi mathvariant="italic">λ</mml:mi><mml:mi mathvariant="normal">R</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> are the
extinction coefficients due to absorption and Rayleigh scattering by
atmospheric molecules for emitting lidar and Raman wavelengths, respectively,
and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula> is the Ångström exponent. The aerosol backscatter coefficient
can be calculated from the ratio of the elastic signal to Raman signal by
using a coefficient determined at a reference point where no aerosol is
expected.</p>
      <p>A variety of methods can be used to retrieve aerosol microphysical properties
using lidar data. They can be divided into three main groups
<xref ref-type="bibr" rid="bib1.bibx53" id="paren.15"/>. The methods belonging to the first group combine
measurements from several instruments that provide enough information to
retrieve aerosol microphysical properties. For such methods, the collocation
of measurements by different instruments in space and time is necessary. The
LIRIC algorithm belongs to this group; it successfully retrieves
height-resolved aerosol optical and microphysical properties separately for
fine and coarse modes <xref ref-type="bibr" rid="bib1.bibx8 bib1.bibx9 bib1.bibx50 bib1.bibx21" id="paren.16"/>. The algorithm uses AERONET inversion products such as
column volume concentration, volume-specific backscatter, and extinction
coefficients as a priori information <xref ref-type="bibr" rid="bib1.bibx9" id="paren.17"/>. The specific
products include backscatter (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula>), extinction (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>), and volume
concentration (<inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>) profiles, Ångström exponent (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">α</mml:mi></mml:math></inline-formula>) values, and LR and depolarization (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>) ratios. A deeper synergy between the lidar
and sun/sky-photometer data is achieved in the GARRLiC algorithm developed at
LOA <xref ref-type="bibr" rid="bib1.bibx29" id="paren.18"/>. GARRLiC inverts the coincident lidar and
sun/sky-photometer radiometric data simultaneously. The other marked
distinction between GARRLiC and LIRIC is the inversion of two distinct
aerosol modes, which makes it possible to retrieve aerosol optical and
microphysical properties independently for both the fine and coarse modes.
Such differences in the algorithms can influence the results obtained by the
two systems. The GARRLiC method is based on the Dubovik inversion code
<xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx14" id="paren.19"/>, which has been previously used for processing
AERONET data. The synergistic retrieval is expected to improves aerosol
retrieval properties; the lidar observations are expected to improve the
observations of the columnar properties of aerosols in the backscattering
direction, and sun/sky photometers provide information on aerosol properties,
such as their amount or type, required for lidar retrievals without making
assumptions based on climatological data.</p>
      <p>GARRLIC has been designed to provide two independent vertical concentration
profiles for the fine and coarse modes of aerosols, since in most cases,
aerosols are believed to consist of two modes. However, it works for
single mode inversions as well. In such cases, a single value for the total
amount of particles is retrieved. The algorithm is quite flexible in this
regard; single or double mode inversion can be chosen by the user. Further,
single- or multi-wavelength lidar data can be used. In the case of
multi-wavelength lidar data, aerosol properties can be retrieved for fine and
coarse modes separately or together for the total amount of particles. In the
case of single-wavelength lidar data, the aerosol properties can be retrieved
only for the total amount of aerosols. Depending on the different
configurations of single or double mode inversion employed and the use of
single- or multi-wavelength lidar data, different sets of aerosol parameters
can be retrieved (see Fig. <xref ref-type="fig" rid="Ch1.F1"/>). Spectral information from
multiple wavelengths is used to distinguish the contribution of fine and
coarse aerosol modes. It should be noted that aerosol events characterized
mainly by one type of aerosols or a mixture of particles similar in size
(aerosol types are not distinguished inside the mode of particles) should be
retrieved by using the configuration of single mode inversion.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><caption><p>GARRLiC products derived by using single (unmarked) or double (both
unmarked and marked *) mode inversion. The latter can be applied only to
multi-wavelength lidar data. Common properties, which are compared in this
work, retrieved using GARRLiC, LIRIC, and Raman and regularization are
indicated by bold font. </p></caption>
        <?xmltex \igopts{width=170.716535pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f01.png"/>

      </fig>

      <p>As for the second group of methods, optical properties (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>
profiles) are calculated using Mie theory and are compared with the results
obtained by using the Raman technique <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx5" id="paren.20"/>. In
these methods, aerosol microphysical properties such as SD and CRI are
assumed as a priori information. Such methods are used in case of atmospheric
layers with single, well-known type of particles. For instance, such methods
can characterize the particles of polar stratospheric clouds, volcanic
ejecta, and some stratospheric particles. However, owing to the presence of a
variety of particles and rapid changes in the atmospheric conditions, such
methods are not applicable to the troposphere.</p>
      <p>The third group consists of mathematical approaches that use <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">β</mml:mi></mml:math></inline-formula> and
<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> coefficient profiles at multiple wavelengths (only lidar
measurements). Such methods were developed from the methods of the second
group, but they require a lower number of a priori parameters
<xref ref-type="bibr" rid="bib1.bibx31 bib1.bibx43 bib1.bibx44 bib1.bibx41" id="paren.21"/>. The algorithm called
inversion with regularization  developed by <xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx44 bib1.bibx47" id="normal.22"/> has also been considered in this work. A simplified set
of lidar data (three backscatter (355, 532, and 1064 nm) and two extinction
(355 and 532 nm) coefficients – the so-called <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="italic">β</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> dataset)
allows the retrieval of the main aerosol microphysical properties
<xref ref-type="bibr" rid="bib1.bibx45" id="paren.23"/>. Aerosol optical properties that are required for the
regularization algorithm can be derived using the Raman technique. The main
aerosol microphysical products of the regularization algorithm are the CRI,
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, number, surface area, and volume concentrations
<xref ref-type="bibr" rid="bib1.bibx43 bib1.bibx47" id="paren.24"/>.</p>
      <p>These groups of retrieval methods use different types of measurements and,
also, different amounts of information. For instance, while regularization
uses the <inline-formula><mml:math display="inline"><mml:mrow><mml:mn mathvariant="normal">3</mml:mn><mml:mi mathvariant="italic">β</mml:mi><mml:mo>+</mml:mo><mml:mn mathvariant="normal">2</mml:mn><mml:mi mathvariant="italic">σ</mml:mi></mml:mrow></mml:math></inline-formula> set of optical data, AERONET uses up to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 30
measurements (direct and diffuse almucantar measurements) at each wavelength.
Hence, it is important to compare the particle properties retrieved with
these methods for these different groups. If different algorithms retrieve
similar aerosol properties, it will mean that they are in agreement and can
complement each other for data processing during long-term day–night
observations.</p>
      <p>Aerosol characteristics that are common to LIRIC, GARRLiC, and regularization
algorithms are <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, LR, CRI, <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The challenging
issue here is that no perfectly coincident measurements exist that can be
used by these algorithms. The standard Raman technique preferably uses lidar
measurements during nighttime, while the sun/sky photometers require
sunlight. Consequently, for a comparison of the retrieved aerosol properties
by using the GARRLiC/LIRIC and regularization algorithms, early morning or
late evening data under stable atmospheric conditions should be selected.
Three events fulfilling these requirements were selected and analysed.</p>
</sec>
<sec id="Ch1.S4">
  <title>Applications</title>
      <p>Several dust events were selected from the LILAS measurements over the Lille
and Dakar sites. These days had moderate (AOD <inline-formula><mml:math display="inline"><mml:mo>≃</mml:mo></mml:math></inline-formula> 0.5 at 440 nm) to high
(AOD <inline-formula><mml:math display="inline"><mml:mo>≃</mml:mo></mml:math></inline-formula> 1.5 at 440 nm) aerosol loads. Back trajectories
<xref ref-type="bibr" rid="bib1.bibx11 bib1.bibx40" id="paren.25"/> and the NMMB/BSC-Dust model (Non-hydrostatic
Multiscale/Barcelona Supercomputing Centre Dust model <xref ref-type="bibr" rid="bib1.bibx37 bib1.bibx23" id="paren.26"/> confirmed the origin of mineral dust from Sahara and showed the
source locations. In the case of local dust events, the back-trajectory analysis
was not used. More details and results of the comparison of each event are
presented below.</p>
      <p>The AERONET products are presented herein for comparison. As it is used as a
priori information for the LIRIC algorithm, the LRs retrieved by LIRIC are
presented along with the AERONET characteristics (marked by ** in Tables <xref ref-type="table" rid="Ch1.T2"/> and <xref ref-type="table" rid="Ch1.T3"/>). Mass concentration profiles were obtained
simply by multiplying the volume concentration profiles, <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, with the mass
density of fine and coarse mode particles. The densities of the fine and
coarse modes are 1.5 and 2.6 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, respectively
<xref ref-type="bibr" rid="bib1.bibx6 bib1.bibx2 bib1.bibx3 bib1.bibx23" id="paren.27"/>. This density
for the coarse mode is also considered in the NMMB/BSC-Dust model.</p>
      <p>The GARRLiC and LIRIC algorithms produce uncertainties with the retrieved
aerosol properties. For the GARRLiC algorithm, systematic and random errors
are presented. For the LIRIC algorithm, only the dispersion of aerosol volume
concentration profiles is presented. This work presents only the
uncertainties regarding the directly retrieved aerosol properties.
Uncertainties on the derived aerosol properties (<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>, LR, SSA profiles)
are not presented due to their high values as derived by GARRLiC (rough
estimations were about 100 % and more). The uncertainties in the volume
concentration profiles retrieved using the regularization algorithm are
assumed to be about 20 % <xref ref-type="bibr" rid="bib1.bibx44 bib1.bibx45 bib1.bibx49" id="paren.28"/>.</p>
      <p>As this work mainly deals with mineral dust sometimes mixed with marine
aerosol particles, it will be useful to consider the particle properties
obtained from previous studies. According to <xref ref-type="bibr" rid="bib1.bibx53" id="normal.29"/>, <xref ref-type="bibr" rid="bib1.bibx32" id="normal.30"/>,
<xref ref-type="bibr" rid="bib1.bibx35" id="normal.31"/>, <xref ref-type="bibr" rid="bib1.bibx39" id="normal.32"/>, and <xref ref-type="bibr" rid="bib1.bibx13" id="normal.33"/>, the typical values of <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for
desert dust vary within the range of 1.2–2.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>
for the coarse mode of sea salt is close to 2.7 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m <xref ref-type="bibr" rid="bib1.bibx13" id="paren.34"/>. The
SSA for dust particles increases from 0.80 to 0.99 in the
ultraviolet–near-infrared range <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx13" id="paren.35"/>. The SSA for
marine aerosols is high, at <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0.98, and the value remains stable at all
wavelengths. The RRI varies from 1.5 to 1.6 for dust particles and is close
to 1.36 for marine particles. The IRI decreases from 0.02 to 0.001 in the
ultraviolet–near-infrared range for dust particles and is close to 0.001
for marine particles. For Saharan dust, the LR varies within the range of
50–80 sr at a wavelength of 532 nm, and it is significantly lower, at
20–35 sr, for marine particles <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx33 bib1.bibx34 bib1.bibx22" id="paren.36"/>. The depolarization ratio is high, being close to 30–35 % for
dust particles, whereas marine particles have a significantly lower <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">δ</mml:mi></mml:math></inline-formula>,
i.e. close to 5 % <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx22" id="paren.37"/>.</p>
<sec id="Ch1.S4.SS1">
  <title>Analysis of a moderate dust event in Lille on 30 March 2014</title>
      <p>The dust event detected over Lille on 30 March 2014 was characterized as
heavy for Lille site in terms of the aerosol load (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.52</mml:mn></mml:mrow></mml:math></inline-formula>;
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.27</mml:mn></mml:mrow></mml:math></inline-formula> for 440/870 nm). The back-trajectory analysis showed
that aerosols, which were located in the altitude range of 3 to 6 km, had
their origin in the Saharan region (Fig. <xref ref-type="fig" rid="Ch1.F2"/>), and aerosols
located up to 2 km travelled from south and south-east France. According to
lidar measurements, very thin and homogeneous cirrus clouds with negligible
effect on AOD were present at 11 km. Cross-examination was done using
almucantar sky radiance measurements in order to prevent cloud contamination.
The relative deviation between the left/right sky radiance measurements in
almucantar geometry was found to be less than 20 %. Cirrus clouds were
identified by neither us nor  AERONET criteria <xref ref-type="bibr" rid="bib1.bibx25" id="paren.38"/>; the
exact time of the sun/sky-photometer measurements was 07:42 UTC. The
NMMB/BSC-Dust model (operated by the Barcelona Supercomputing Center,
<uri>www.bsc.es/projects/earthscience/NMMB-BSC-DUST/</uri>) confirmed dust
emissions over Algeria that travelled towards Lille (Fig. <xref ref-type="fig" rid="Ch1.F3"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><caption><p>Backward trajectories of air masses observed over Lille during the morning of 30 March 2014.
</p></caption>
          <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f02.png"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1" specific-use="star"><caption><p>Aerosol properties retrieved by GARRLiC, BASIC, and AERONET. The LR
values marked by ** were linearly interpolated to lidar wavelength. The
abbreviations f, c, and t correspond to fine, coarse, and total aerosol
modes, respectively (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.52</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.27</mml:mn></mml:mrow></mml:math></inline-formula> for
440/870 nm).</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="10">
     <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:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="left"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col6" align="center">GARRLiC </oasis:entry>  
         <oasis:entry colname="col7">BASIC</oasis:entry>  
         <oasis:entry rowsep="1" namest="col8" nameend="col10" align="center">AERONET </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (nm)</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)</oasis:entry>  
         <oasis:entry colname="col3">Sph %</oasis:entry>  
         <oasis:entry colname="col4">RRI</oasis:entry>  
         <oasis:entry colname="col5">IRI</oasis:entry>  
         <oasis:entry colname="col6">LR (sr)</oasis:entry>  
         <oasis:entry colname="col7">LR (sr)</oasis:entry>  
         <oasis:entry colname="col8">RRI</oasis:entry>  
         <oasis:entry colname="col9">IRI</oasis:entry>  
         <oasis:entry colname="col10">LR (sr)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">440</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.50</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">53</oasis:entry>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8">1.48</oasis:entry>  
         <oasis:entry colname="col9">0.002</oasis:entry>  
         <oasis:entry colname="col10">57</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">532</oasis:entry>  
         <oasis:entry colname="col2">f: 0.1</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.50</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">48</oasis:entry>  
         <oasis:entry colname="col7">53</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10">52**</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">675</oasis:entry>  
         <oasis:entry colname="col2">c: 2.0</oasis:entry>  
         <oasis:entry colname="col3">1 %</oasis:entry>  
         <oasis:entry colname="col4">1.51</oasis:entry>  
         <oasis:entry colname="col5">0.001</oasis:entry>  
         <oasis:entry colname="col6">43</oasis:entry>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8">1.52</oasis:entry>  
         <oasis:entry colname="col9">0.001</oasis:entry>  
         <oasis:entry colname="col10">43</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">870</oasis:entry>  
         <oasis:entry colname="col2">t: 0.9</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.50</oasis:entry>  
         <oasis:entry colname="col5">0.001</oasis:entry>  
         <oasis:entry colname="col6">45</oasis:entry>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8">1.51</oasis:entry>  
         <oasis:entry colname="col9">0.001</oasis:entry>  
         <oasis:entry colname="col10">43</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1020</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.51</oasis:entry>  
         <oasis:entry colname="col5">0.001</oasis:entry>  
         <oasis:entry colname="col6">45</oasis:entry>  
         <oasis:entry colname="col7"/>  
         <oasis:entry colname="col8">1.51</oasis:entry>  
         <oasis:entry colname="col9">0.001</oasis:entry>  
         <oasis:entry colname="col10">43</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>The configuration of LILAS was changed from three channels (355 nm parallel and
perpendicular and 532 nm total) to eight channels (355 and 532 nm parallel and
perpendicular; 387, 408, 608, and 1064 nm total) in April 2014. Hence,
the Saharan dust event could not be analysed by the Raman and regularization
algorithms. Unfortunately, depolarization calibration of 355 nm have not been
done for the event. Hence, only data at 532 nm channel were used for analysis.
LIRIC inversion had not been applied to this event. Consequently, only the
GARRLiC and BASIC algorithms were considered in our analysis. Single mode
GARRLiC inversions were considered due to only lidar signal at 532 nm. The
lidar elevation angle during the measurements was 56<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p>Aerosol properties retrieved by the GARRLiC and BASIC algorithms and AERONET
products are presented in Table <xref ref-type="table" rid="Ch1.T1"/> and Figs. <xref ref-type="fig" rid="Ch1.F4"/> and
<xref ref-type="fig" rid="Ch1.F5"/>. The columnar-integrated GARRLiC SSA values increase with the
wavelength, i.e. from 0.94 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 at 440 nm to 0.98 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 at
1020 nm. The RRI is close to 1.50 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02, the IRI decreases from 0.002 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.001 to 0.001 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.001. The CRI values retrieved by GARRLiC are in
agreement with the AERONET retrievals. The GARRLiC LR values are lower in
comparison to the ones retrieved by AERONET at wavelengths of 440 and 532 nm,
while they are almost equal at others. The BASIC LR value at 532 nm are close
to the value interpolated by AERONET values. The effective radius for the
coarse mode of particles is high and is close to 2.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, and the
<inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> for the fine mode is close to the value of urban particles.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><caption><p>Dust event over Algeria on 29 March 2014.
</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f03.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4"><caption><p>Volume size distribution retrieved by GARRLiC (pink) and AERONET
(black) on 30 March 2014 (07:40 UTC) in Lille (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.52</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.27</mml:mn></mml:mrow></mml:math></inline-formula> for 440/870 nm). </p></caption>
          <?xmltex \igopts{width=207.705118pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f04.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5"><caption><p>Aerosol extinction profiles at a wavelength 532 nm retrieved by the
GARRLiC (green) and the BASIC (black) algorithms for dust event over Lille on
30 March 2014.</p></caption>
          <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f05.pdf"/>

        </fig>

      <p>The size distribution (see Fig. <xref ref-type="fig" rid="Ch1.F4"/>) clearly shows the
predominance of coarse mode particles with two maxima. The first one with
lower radii likely indicates dust particles, and the second one with larger
radii also indicates dust particles or can refer to the particles of thin
cirrus clouds <xref ref-type="bibr" rid="bib1.bibx42 bib1.bibx24" id="paren.39"/>. The sphericity parameter
retrieved by GARRLiC is in agreement with the one from AERONET, both being
close to 1 %. The extinction profiles retrieved by BASIC and GARRLiC are
close (Fig. <xref ref-type="fig" rid="Ch1.F5"/>).</p>
      <p>The back-trajectory analysis indicates two layers. This mixture of dust and
some fine particles results in lower LR and CRI and higher SSA (at 440 and
532 nm) values than for aerosols from mineral dust only <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx20 bib1.bibx38" id="paren.40"/>. Consequently, if the higher layer consisted of
mineral dust particles, it is possible to assume that lower aerosol layer
with lower LR, CRI, higher SSA and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> of fine mode close to 0.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m would consist of urban particles <xref ref-type="bibr" rid="bib1.bibx13 bib1.bibx53" id="paren.41"/>.
Unfortunately, no mass concentration profiles could be obtained by the
NMMB/BSC-Dust model.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><caption><p>NMMB/BSC-Dust model over Africa and Europe on 29 March 2015. AOD
values forecasted by the model ranged from 0.8 to 1.6 at 550 nm. <bold>(a)</bold> 18:00
UTC, 29 March; <bold>(b)</bold> 00:00 UTC, 30 March. </p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f06.png"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS2">
  <title>Analysis of a heavy dust event in Dakar on 29 March 2015</title>
      <p>The second event considered in this work was also a dust event, but it
occurred over the Dakar site during the SHADOW2 campaign. Three time ranges
were selected for the analysis. Daytime data from 15:50 to 19:00 were
selected for the Raman technique. For the GARRLiC and LIRIC algorithms, lidar
signals were averaged for 20 min at the time of measurement by the
sun/sky photometer (16:49 UTC). A third data range was selected for the
regularization and Raman methods from 23:30 to 01:10 during nighttime
measurements. All aerosols were found in the boundary layer for all time
ranges. During the daytime measurements, the altitude of the boundary layer
was 2.5 km, and it came down to 2 km at night. The daytime event was
characterized by a high aerosol load (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.35</mml:mn><mml:mo>±</mml:mo><mml:mn>0.20</mml:mn></mml:mrow></mml:math></inline-formula>;
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mn>0.04</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula> for 440/870 nm), and the nighttime event was
characterized by a lower aerosol load (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.83</mml:mn><mml:mo>±</mml:mo><mml:mn>0.03</mml:mn></mml:mrow></mml:math></inline-formula>;
<inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.08</mml:mn><mml:mo>±</mml:mo><mml:mn>0.02</mml:mn></mml:mrow></mml:math></inline-formula> for 440/870 nm). The NMMB/BSC-Dust model
showed a local dust event over the Dakar site with an AOD range of 0.8–1.6
at the 550 nm wavelength (Fig. <xref ref-type="fig" rid="Ch1.F6"/>) for both day- and nighttime
measurements. A wind lidar instrument was installed on the site during the
SHADOW2 campaign <xref ref-type="bibr" rid="bib1.bibx52" id="paren.42"/>, and it captured vertically
resolved wind speeds and the direction of wind at the site for up to 2 km.
The lidar data showed the wind direction to be north–north-east with a speed
of 5 to 10 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the full altitudinal range for the daytime measurements;
the wind direction was north-east with a speed of 10 to 15 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> in the
altitudinal range of up to 1.5 km, and lower speeds of 5 to 10 m s<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> were
present in upper altitudes for the nighttime measurements. Therefore, while
presumably the atmospheric conditions in terms of aerosol types should have
remained the same during the event, the aerosol load decreased over the day-
to nighttime measurement time frame. Also, the presence of marine particles
was not expected because of the lower wind speeds and their northwardly
direction during the day.</p>
      <p>The aerosol properties retrieved by the GARRLiC and regularization algorithms
for the day- and nighttime measurements, respectively, are presented in
Table <xref ref-type="table" rid="Ch1.T2"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2" specific-use="star"><caption><p>Aerosol properties during the dust event over the Dakar site on 29
March 2015. Here and further, the LR values marked by ** were retrieved by
using the LIRIC algorithm. Only the values given for all the wavelengths
refer to the column-integrated property. Day: AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.35</mml:mn><mml:mo>±</mml:mo><mml:mn>0.20</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mn>0.04</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>. Night: AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.83</mml:mn><mml:mo>±</mml:mo><mml:mn>0.03</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.08</mml:mn><mml:mo>±</mml:mo><mml:mn>0.02</mml:mn></mml:mrow></mml:math></inline-formula>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="12">
     <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:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="left"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:colspec colnum="11" colname="col11" align="left"/>
     <oasis:colspec colnum="12" colname="col12" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col6" align="center">GARRLiC </oasis:entry>  
         <oasis:entry colname="col7">AERONET</oasis:entry>  
         <oasis:entry colname="col8">Raman (day)</oasis:entry>  
         <oasis:entry rowsep="1" namest="col9" nameend="col12" align="center">Raman and regularization (night) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (nm)</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)</oasis:entry>  
         <oasis:entry colname="col3">Sph %</oasis:entry>  
         <oasis:entry colname="col4">RRI</oasis:entry>  
         <oasis:entry colname="col5">IRI</oasis:entry>  
         <oasis:entry colname="col6">LR (sr)</oasis:entry>  
         <oasis:entry colname="col7">LR (sr)</oasis:entry>  
         <oasis:entry colname="col8">LR (sr)</oasis:entry>  
         <oasis:entry colname="col9"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)</oasis:entry>  
         <oasis:entry colname="col10">RRI</oasis:entry>  
         <oasis:entry colname="col11">IRI</oasis:entry>  
         <oasis:entry colname="col12">LR (sr)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">355</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.59</oasis:entry>  
         <oasis:entry colname="col5">0.003</oasis:entry>  
         <oasis:entry colname="col6">37</oasis:entry>  
         <oasis:entry colname="col7">82**</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 57</oasis:entry>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 70</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">440</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.59</oasis:entry>  
         <oasis:entry colname="col5">0.003</oasis:entry>  
         <oasis:entry colname="col6">33</oasis:entry>  
         <oasis:entry colname="col7">74</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">532</oasis:entry>  
         <oasis:entry colname="col2">f: 0.2</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.59</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">28</oasis:entry>  
         <oasis:entry colname="col7">58**</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 53</oasis:entry>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 58</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">675</oasis:entry>  
         <oasis:entry colname="col2">c: 2.2</oasis:entry>  
         <oasis:entry colname="col3">20 %</oasis:entry>  
         <oasis:entry colname="col4">1.58</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">25</oasis:entry>  
         <oasis:entry colname="col7">43</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9">1.1</oasis:entry>  
         <oasis:entry colname="col10">1.53</oasis:entry>  
         <oasis:entry colname="col11">0.010</oasis:entry>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">870</oasis:entry>  
         <oasis:entry colname="col2">t: 1.9</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.57</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">24</oasis:entry>  
         <oasis:entry colname="col7">37</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1020</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.56</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">22</oasis:entry>  
         <oasis:entry colname="col7">35</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1064</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.56</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">22</oasis:entry>  
         <oasis:entry colname="col7">34**</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p>Single mode GARRLiC inversions were considered and performed in this event
because of the huge predominance of coarse mode particles. The effective
radius value is high and close to 1.9 during the daytime and decreases to
1.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m at night. The RRI values are high, being close to 1.58 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02
during the daytime measurements; then, values become lower and close to
1.53 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.05 at night. The IRI values decrease from 0.003 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.002 to
0.002 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.001 in the UV–near-infrared range during the daytime and are
higher at all wavelengths and close to 0.010 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.005 at night. For both
the day and night cases, the Ångström exponent is close to 0. Regarding
absorption, the SSA values obtained by GARRLiC increase from 0.87 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02
to 0.97 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 in the UV–near-infrared range. The daytime LR values are
similar at 532 nm, whereas the ones retrieved by GARRLiC are much lower. The
LR values at 355 nm during the daytime measurements differ for all the
algorithms, being close to 57, 82, and 37 sr for the Raman, LIRIC, and
GARRLiC algorithms, respectively. The Raman LR values slightly increase from
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 53 to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 58 sr at 532 nm, and it significantly increases from
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 57 to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 70 sr at 355 nm over the day- to nighttime measurement
time frame. Such a behaviour could be explained by the influence of marine
aerosols during daytime. However, the depolarization ratio (Fig. <xref ref-type="fig" rid="Ch1.F10"/>)
shows that there was at most very little contribution of marine aerosol
during daytime. Hence, such a behaviour of retrieved aerosol properties
points
to inconsistency between the different methods.</p>
      <p>It was observed that the IRI, SSA, SD, and <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> retrieved by
GARRLiC were in good agreement with AERONET products. However, RRI values and
parameter of particle sphericity differed. While the AERONET RRI is equal to
1.53 and the sphericity is equal to 0 %, the RRI retrieved by GARRLiC is
close to 1.58 and the sphericity is <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 20 %. The differences in the LR
values are presented in Table <xref ref-type="table" rid="Ch1.T2"/> and are discussed above.</p>
      <p>Figure <xref ref-type="fig" rid="Ch1.F7"/> shows that the SD values obtained from GARRLiC and
AERONET are in good agreement. Figure <xref ref-type="fig" rid="Ch1.F8"/> presents the aerosol
volume concentrations, <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula>, retrieved with the GARRLiC, LIRIC, and
regularization algorithms. Because of the use of single mode inversion by
GARRLiC, only the overall <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> profile was obtained; however, the LIRIC
algorithm provided both fine and coarse mode volume concentrations. Because
of a high background noise, the regularization algorithm was not applied to
daytime measurements; only nighttime <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> is presented with this algorithm.
The GARRLiC and LIRIC volume concentrations are in good agreement.
Unfortunately, obtaining close <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> values using GARRLiC, LIRIC, and
regularization algorithms between the day- and nighttime is not possible
because of a significant decrease in the AOD values. The relative uncertainty
in <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> obtained from the regularization method was expected to be about 20 %;
the GARRLiC and LIRIC uncertainties are plotted in Fig. <xref ref-type="fig" rid="Ch1.F8"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7"><caption><p>GARRLiC (pink) and AERONET (black) SD on 29 March 2015 (16:49 UTC)
over the Dakar site (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.35</mml:mn><mml:mo>±</mml:mo><mml:mn>0.20</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mn>0.04</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>). </p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f07.pdf"/>

        </fig>

      <p>The extinction profiles (Fig. <xref ref-type="fig" rid="Ch1.F9"/>) at all the wavelengths were
found to be in reasonable agreement. The nighttime values of <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> are
lower in accordance with the lower AOD values. The top boundary of the dust
layer decreases from 2.5 km during the day to 2 km at night. The GARRLiC
extinction profiles are much smoother because lidar signals were reduced by
averaging into 60 points during the data preparation phase. The daytime
Raman LR values (Fig. <xref ref-type="fig" rid="Ch1.F10"/>) increase with altitude and, therefore,
correct <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profiles; however, GARRLiC and LIRIC retrieved only the
column-integrated LRs in this case (GARRLiC retrieved vertically resolved LRs
in the case of fine and coarse modes inversion). The particle depolarization,
presented in Fig. <xref ref-type="fig" rid="Ch1.F10"/>, is lower during daytime (close to 29 %)
and higher at nighttime when no marine particles are expected (close to
34 %). These LRs and particle depolarization values are common for mineral
dust, especially at nighttime. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> profile retrieved by
regularization is close to 1.1 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m at the 0.9–1.6 km altitudinal range,
and higher values up to 1.4 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m were observed below 0.9 km, whereas lower
values close to 0.8 were observed above 1.6 km. The regularization CRI
profiles are stable at all altitudes; the averaged values are presented in
Table <xref ref-type="table" rid="Ch1.T2"/> as column-integrated values. The <inline-formula><mml:math display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msup></mml:mrow></mml:math></inline-formula> profile
for 355/532 nm is close to 0 at all altitudes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8"><caption><p>Volume (Vol conc) and mass (Mass conc) concentration profiles for an
event over the Dakar site on 29 March 2015. The abbreviation RR corresponds
to <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> retrieved by using Raman and regularization algorithms.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f08.pdf"/>

        </fig>

      <p>For the comparison with NMMB/BSC-Dust model, the mass concentration profiles
were obtained (Fig. <xref ref-type="fig" rid="Ch1.F8"/>). To keep the figure clear, uncertainties of
mass concentration profiles are not presented. In the case of GARRLiC because of
high predominance of coarse aerosol mode, particle density was taken to be
equal to 2.6 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>. In the case of LIRIC, both particle densities 1.5 and
2.6 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> were taken for fine and coarse aerosol modes respectively.
To keep the figure clear and similar to other parameters, only total LIRIC
values are presented in Fig. <xref ref-type="fig" rid="Ch1.F8"/>. The mass concentration profiles
obtained by GARRLiC and LIRIC algorithms are 1280 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 500 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
and 1170 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 180 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> respectively at 1.5 km, which is slightly
higher in comparison with the NMMB/BSC-Dust model result (<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 900 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).
The nighttime mass concentration is close to 500 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 100 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>, whereas the modelled value is close to 1700 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> at the
same altitude of 1.5 km.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><caption><p>Raman, LIRIC, and GARRLiC extinction profiles during the day (AOD
440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.35</mml:mn><mml:mo>±</mml:mo><mml:mn>0.20</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mo>-</mml:mo><mml:mn>0.04</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>) and night (AOD
440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.83</mml:mn><mml:mo>±</mml:mo><mml:mn>0.03</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.08</mml:mn><mml:mo>±</mml:mo><mml:mn>0.02</mml:mn></mml:mrow></mml:math></inline-formula>) on 29 March
2015.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f09.pdf"/>

        </fig>

</sec>
<sec id="Ch1.S4.SS3">
  <title>Analysis of a heavy dust event in Dakar on 10 April 2015</title>
      <p>The third and the last dust event considered in our study was observed on 10
April 2015 over Dakar (11 days later). Three time ranges were selected for
the analysis: the first two during daytime (15:00–19:00 for Raman and
16:01–16:19 for GARRLiC and LIRIC) and the third during nighttime
(21:00–04:00 on 11 April 2015 for regularization). The atmospheric
conditions were stable, but the height of the aerosol layer containing almost
all the aerosols increased from 3 to 4.5 km from the day- to nighttime
measurements. The daytime event was characterized by a high aerosol load
(AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.53</mml:mn><mml:mo>±</mml:mo><mml:mn>0.04</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.02</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula> for
440/870 nm). Unfortunately, there were no lunar-photometer measurements
because of the lunar phase. However, AOD derived by the integration of the
<inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profile obtained by the Raman method at 532 nm wavelength is equal
to 0.83. It should be noted that such an estimation of AOD does not include
aerosols located in incomplete overlap zone of lidar. The NMMB/BSC-Dust model
forecasted a dust event over the Dakar site with AOD values ranging from 0.8
to 1.6 at 550 nm for both day- and nighttime (Fig. <xref ref-type="fig" rid="Ch1.F11"/>).
Unfortunately, no measurements could be obtained from the wind lidar.
However, a sea breeze was observed at the ground level during daytime
measurements. Back-trajectory analysis showed that during the daytime event,
the sources of air masses that came to the observational site changed from
north (coast of Mauritania) at 0.5 km to east (north-west of Mali) at 2.5 km
(Fig. <xref ref-type="fig" rid="Ch1.F12"/>). Additionally, during the night, air masses were coming from
the northeast direction (Sahara region) at all altitudes. The GARRLiC and
Raman plus regularization aerosol retrievals for the day- and nighttime
measurements are presented in Table <xref ref-type="table" rid="Ch1.T3"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10"><caption><p>Lidar ratio and depolarization ratio during day- and nighttime
measurements for an event on 29 March 2015 over the Dakar site. GARRLiC and
LIRIC LR column-integrated values are shown at the beginning of the
profiles. </p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f10.pdf"/>

        </fig>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T3" specific-use="star"><caption><p>Aerosol properties during the dust event over the Dakar site on 10
April 2015. The LR values marked by ** were retrieved by the LIRIC algorithm.
Only the values given for all the wavelengths refer to the column-integrated
property. Day: AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.53</mml:mn><mml:mo>±</mml:mo><mml:mn>0.04</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.02</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>. Night: AOD 532 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.83</mml:mn></mml:mrow></mml:math></inline-formula>; <inline-formula><mml:math display="inline"><mml:mrow><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> by Raman.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="12">
     <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:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="left"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:colspec colnum="11" colname="col11" align="left"/>
     <oasis:colspec colnum="12" colname="col12" align="left"/>
     <oasis:thead>
       <oasis:row>  
         <oasis:entry colname="col1"/>  
         <oasis:entry rowsep="1" namest="col2" nameend="col6" align="center">GARRLiC </oasis:entry>  
         <oasis:entry colname="col7">AERONET</oasis:entry>  
         <oasis:entry colname="col8">Raman (day)</oasis:entry>  
         <oasis:entry rowsep="1" namest="col9" nameend="col12" align="center">Raman and regularization (night) </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">  
         <oasis:entry colname="col1"><inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">λ</mml:mi></mml:math></inline-formula> (nm)</oasis:entry>  
         <oasis:entry colname="col2"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)</oasis:entry>  
         <oasis:entry colname="col3">Sph %</oasis:entry>  
         <oasis:entry colname="col4">RRI</oasis:entry>  
         <oasis:entry colname="col5">IRI</oasis:entry>  
         <oasis:entry colname="col6">LR (sr)</oasis:entry>  
         <oasis:entry colname="col7">LR (sr)</oasis:entry>  
         <oasis:entry colname="col8">LR (sr)</oasis:entry>  
         <oasis:entry colname="col9"><inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m)</oasis:entry>  
         <oasis:entry colname="col10">RRI</oasis:entry>  
         <oasis:entry colname="col11">IRI</oasis:entry>  
         <oasis:entry colname="col12">LR (sr)</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>  
         <oasis:entry colname="col1">355</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.60</oasis:entry>  
         <oasis:entry colname="col5">0.004</oasis:entry>  
         <oasis:entry colname="col6">20</oasis:entry>  
         <oasis:entry colname="col7">70**</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25</oasis:entry>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 59</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">440</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.60</oasis:entry>  
         <oasis:entry colname="col5">0.003</oasis:entry>  
         <oasis:entry colname="col6">17</oasis:entry>  
         <oasis:entry colname="col7">62</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">532</oasis:entry>  
         <oasis:entry colname="col2">f: 0.2</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.60</oasis:entry>  
         <oasis:entry colname="col5">0.003</oasis:entry>  
         <oasis:entry colname="col6">14</oasis:entry>  
         <oasis:entry colname="col7">49**</oasis:entry>  
         <oasis:entry colname="col8"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 23</oasis:entry>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"><inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50</oasis:entry>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">675</oasis:entry>  
         <oasis:entry colname="col2">c: 2.4</oasis:entry>  
         <oasis:entry colname="col3">57 %</oasis:entry>  
         <oasis:entry colname="col4">1.60</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">13</oasis:entry>  
         <oasis:entry colname="col7">39</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9">0.9</oasis:entry>  
         <oasis:entry colname="col10">1.54</oasis:entry>  
         <oasis:entry colname="col11">0.008</oasis:entry>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">870</oasis:entry>  
         <oasis:entry colname="col2">t: 2.0</oasis:entry>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.59</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">12</oasis:entry>  
         <oasis:entry colname="col7">32</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1020</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.58</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">13</oasis:entry>  
         <oasis:entry colname="col7">31</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
       <oasis:row>  
         <oasis:entry colname="col1">1064</oasis:entry>  
         <oasis:entry colname="col2"/>  
         <oasis:entry colname="col3"/>  
         <oasis:entry colname="col4">1.58</oasis:entry>  
         <oasis:entry colname="col5">0.002</oasis:entry>  
         <oasis:entry colname="col6">13</oasis:entry>  
         <oasis:entry colname="col7">30**</oasis:entry>  
         <oasis:entry colname="col8"/>  
         <oasis:entry colname="col9"/>  
         <oasis:entry colname="col10"/>  
         <oasis:entry colname="col11"/>  
         <oasis:entry colname="col12"/>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><caption><p>NMMB/BSC-Dust model results over Africa and Europe on 10 April 2015.
AOD values forecasted by the model ranged from 0.8 to 1.6 at 550 nm.
<bold>(a)</bold>
18:00 UTC, 10 April; <bold>(b)</bold> 00:00 UTC, 11 April.</p></caption>
          <?xmltex \igopts{width=398.338583pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f11.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12"><caption><p>Backward trajectories of air masses for an event over the Dakar site on 10 April 2015.
</p></caption>
          <?xmltex \igopts{width=227.622047pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f12.png"/>

        </fig>

      <p>GARRLiC single mode inversion was used because of the huge predominance of
coarse mode particles. As in the previous event, daytime <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is
high and equal to 2.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m, and the value decreases to 0.9 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m at
night. The daytime column-integrated RRI is close to 1.59 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.02 and
stays rather stable at nighttime (1.54 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.06). The IRI slightly decreases
during the daytime from 0.004 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.002 to 0.002 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.001 in the
UV–near-infrared range and is close to 0.008 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.004 at the nighttime.
The GARRLiC SSA increases from 0.85 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.03 to 0.95 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 0.01 in
UV–near-infrared range. The maximum of SD is shifted to higher radii (Fig. <xref ref-type="fig" rid="Ch1.F13"/>). However, in general, RRI, IRI, SSA, and SD retrieved by
GARRLiC are quite comparable to AERONET values. However, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and
particle sphericity differ. AERONET <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is equal to 1.6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m
and sphericity <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 0 %, while the GARRLiC algorithm retrieved 2.0 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m
for <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and 57 % of sphericity particles.</p>
      <p>Volume concentration profiles are presented in Fig. <xref ref-type="fig" rid="Ch1.F14"/>. Because
of different AOD values and altitudes of the boundary layer, day- and
nighttime <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> obtained using different methods are not comparable. The LIRIC
and GARRLiC daytime <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> are different, especially below 2 km, which can be
explained by LIRIC usage of both 532 nm parallel and perpendicular signals
whereas GARRLiC used total backscattered signal only. However, obtained
uncertainties are high and data are overlapped. Extinction profiles (Fig. <xref ref-type="fig" rid="Ch1.F15"/>) at all wavelengths are close to each other in respect to the
retrieval algorithm. Differences between LRs retrieved by the algorithms are
very high, but, nevertheless, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profiles of different algorithms do not
have such high differences. The GARRLiC LRs for 355 and 532 nm are 20 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 11
and 14 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 21 respectively. The Raman LR values at 532 nm increase from
<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 23 to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 50 sr over the day- to nighttime measurement time frame,
and LR at 355 nm also increases from <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 25 to <inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 59 sr (Fig. <xref ref-type="fig" rid="Ch1.F16"/>). Such an increase in LR from day- to nighttime measurements
can be explained by the contribution of marine particles during the daytime
(i.e. sea-breeze effect). Particle depolarization is lower during daytime
(29 %) than during nighttime (32 %). The Raman <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">α</mml:mi><mml:mi mathvariant="normal">ext</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> profile at
355/532 nm is close to 0 and does not change with altitude (this is not shown
in the figures). The profile of the effective radius retrieved with
regularization decreases from 1.2 to 0.6 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>m at the altitude
range of 1–4.5 km. Regularization RRI and IRI profiles remain stable through
all altitudes, and column-integrated values, which are presented in Table <xref ref-type="table" rid="Ch1.T3"/>, have been taken as averaged values.</p>
      <p>The volume concentration profile at 2 km is much higher during the daytime
measurements than the one obtained at night. For comparison with
NMMB/BSC-Dust model results, the mass concentration profiles were obtained
(Fig. <xref ref-type="fig" rid="Ch1.F14"/>). Similar to the previous event, the particle density
was taken to be equal to 2.6 g cm<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula> according to the NMMB/BSC-Dust
model for GARRLiC result. And total LIRIC mass concentration defined as sum
of fine and coarse aerosol modes values. The obtained mass concentration
profiles at 2 km are close to 1225 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 400 and 1020 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 90 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>
for GARRLiC and LIRIC, respectively. This is at least 2 times higher in
comparison with the value produced by the NMMB/BSC-Dust model (<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 550 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>). The calculated Raman nighttime mass concentration
(310 <inline-formula><mml:math display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula> 60 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) shows good agreement with the NMMB/BSC-Dust model
(<inline-formula><mml:math display="inline"><mml:mo>∼</mml:mo></mml:math></inline-formula> 300 <inline-formula><mml:math display="inline"><mml:mi mathvariant="normal">µ</mml:mi></mml:math></inline-formula>g m<inline-formula><mml:math display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) at 2 km.</p>
      <p>Raman and GARRLiC daytime LRs indicate very likely the measurements of marine
particles, but at the same time the depolarization ratio indicates at
mineral dust. The GARRLiC results are more consistent with mineral dust, but
at the same time the retrieved sphericity (57 %) is too high for dust and LR
values at all wavelengths are too low.</p>
      <p>Such a complex event, which includes several types of particles with similar
radii, can cause difficulties in retrieving, interpreting, and comparing the
results. The GARRLiC and LIRIC height-resolved aerosol properties are
incompatible with the NMMB/BSC-Dust <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> and Raman <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profiles. That is
why, to avoid inconsistencies between the results of different methods,
GARRLiC should be only implemented in cases (i) where a single
aerosol type is present or (ii) when the investigated aerosols can
be separated into two different types of fine and coarse modes.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13"><caption><p>GARRLiC (pink) and AERONET (black) SD for 10 April 2015 (16:11 UTC)
over the Dakar site (AOD 440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.53</mml:mn><mml:mo>±</mml:mo><mml:mn>0.04</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.02</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>). </p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f13.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14"><caption><p>Volume (Vol conc) and mass (Mass conc) concentration profiles for an
event over the Dakar site on 10 April 2015. The abbreviation RR corresponds
to <inline-formula><mml:math display="inline"><mml:mi>V</mml:mi></mml:math></inline-formula> retrieved by using Raman and regularization algorithms.
</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f14.pdf"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15"><caption><p>Raman, LIRIC, and GARRLiC extinction profiles during the day (AOD
440 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>1.53</mml:mn><mml:mo>±</mml:mo><mml:mn>0.04</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn>0.02</mml:mn><mml:mo>±</mml:mo><mml:mn>0.01</mml:mn></mml:mrow></mml:math></inline-formula>) and night (AOD
532 nm <inline-formula><mml:math display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn>0.83</mml:mn><mml:mo>;</mml:mo><mml:mi mathvariant="italic">α</mml:mi><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> by Raman) on 10 April 2015.
</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f15.pdf"/>

        </fig>

</sec>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <title>Conclusions</title>
      <p>As  mentioned previously, the main objective of this article is to compare
aerosol properties retrieved by different algorithms. This helps to know to
what extent these algorithms can be used in a complementary way for long-term
day–night aerosol observations and data processing.</p>
      <p>Three dust events were selected from LILAS measurements. The first event over
Lille on 30 March 2014 was characterized by transported mineral dust
particles from the Saharan region. Three different layers of aerosols were
observed: (i) assumed urban particles up to 2.5 km, (ii)
dust layer in the altitude range of 2.5 to 6 km, and (iii) cirrus
clouds with a negligible AOD impact at heights of 11 to 12 km.</p>
      <p>The second and third events over Dakar were characterized by a layer
consisting of a dust and marine (small contribution) aerosol mixture during
the daytime and only dust particles during the nighttime. In both cases,
AOD values decrease over the day- to nighttime measurement time frame, and,
therefore, it was not possible to compare the day- and nighttime <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>.
GARRLiC, LIRIC, and Raman daytime <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profiles are in agreement on 29
March. However, <inline-formula><mml:math display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> profiles retrieved by the same algorithms on 10
April differ. The latter was a more complex event with different types of
particles in the same size range. Development, such as introducing
depolarization profile into the GARRLiC algorithm, should enhance the
algorithm and make it possible to distinguish aerosols with different shapes
inside one mode. In both dust cases, <inline-formula><mml:math display="inline"><mml:mrow><mml:msub><mml:mi>r</mml:mi><mml:mi mathvariant="normal">eff</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> were found to be higher
during daytime in comparison with the nighttime cases. Raman LRs increased
over the day- to nighttime measurement time frame, which could be caused by
the absent of marine particles at night. However, depolarization ratios were
always indicative of dust particles. GARRLiC LR values were always lower than
the ones obtained by LIRIC and Raman. Also, GARRLiC sphericity was always
higher than the one obtained by AERONET. Also, the presence of marine
particles should decrease RRI values during the day, but daytime RRI values
were higher in comparison with the nighttime ones. However, daytime IRI
values were lower in comparison with the ones obtained at night, which agrees
with the presence of marine particles, which absorb less than dust particles.
These features indicate the challenges in description of optical properties
of non-spherical particles in backscattering, on top of possible
inconsistencies between the retrieval algorithms used herein. The studies by
<xref ref-type="bibr" rid="bib1.bibx35" id="normal.43"/>,  <xref ref-type="bibr" rid="bib1.bibx54" id="normal.44"/>, and <xref ref-type="bibr" rid="bib1.bibx28" id="normal.45"/> suggest that the difficulties
with reproduction of the observations relate to inaccuracies in the
spheroidal model in reproduction of scattering properties in backwards
direction. However, those studies are focused on observations of desert dust
particle depolarization that were not used in GARRLiC and LIRIC analysis of
this study. At the same time, it is worth mentioning that recent research by
<xref ref-type="bibr" rid="bib1.bibx49" id="normal.46"/> has reported very encouraging agreement of spheroidal model
with dust observations. More events should be analysed in order to
distinguish the inconsistencies between the algorithms. The second phase of
the SHADOW2 campaign will be taking place in December–January 2016.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F16"><caption><p>Lidar ratio and depolarization ratio during day- and nighttime
measurements for an event on 10 April 2015 over the Dakar site. GARRLiC and
LIRIC LR column-integrated values are shown at the beginning of the
profiles. </p></caption>
        <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://amt.copernicus.org/articles/9/3391/2016/amt-9-3391-2016-f16.pdf"/>

      </fig>

      <p>In future studies, it will be interesting to select morning measurements
excluding see-breeze and marine particles. GARRLiC development (for instance,
by incorporating the Raman technique and/or depolarization profile into the
code) will make it possible to distinguish vertically resolved aerosol
optical properties more accurately, i.e. improved extinction and volume
concentration profiles. After such improvements, similar studies should be
carried out and, again, the algorithm results should be compared to determine
whether they are able to complement each other for long-term day–night
measurements.</p>
</sec>
<sec id="Ch1.S6">
  <title>Data availability</title>
      <p>AERONET data for Dakar and Lille instrumentation sites are available at <uri>http://aeronet.gsfc.nasa.gov/</uri>.
Lidar data available at <uri>http://www-loa.univ-lille1.fr/index.php/observation/lidar.html</uri>.</p>
</sec>

      
      </body>
    <back><app-group>
        <supplementary-material position="anchor"><p><bold>The Supplement related to this article is available online at <inline-supplementary-material xlink:href="http://dx.doi.org/10.5194/amt-9-3391-2016-supplement" xlink:title="pdf">doi:10.5194/amt-9-3391-2016-supplement</inline-supplementary-material>.</bold></p></supplementary-material>
        </app-group><ack><title>Acknowledgements</title><p>The research leading to these results has received funding from European
Union's Horizon 2020 research and innovation programme under grant
agreement no. 654109 within the ACTRIS project. The authors acknowledge Diaollo
Aboubacry and Thierno Ndiaye from IRD (Institute pour la Recherche et le
Développement) at Mbour, Dakar, Senegal, and the CaPPA project for the its
support. The authors acknowledge Sara Basart and the BSC-CNS (Barcelona
Supercomputing Center/Centro Nacional de Supercomputación) team for
providing modelled dust concentration profiles.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>
Edited by: V. Amiridis<?xmltex \hack{\newline}?>
Reviewed by: three anonymous referees</p></ack><ref-list>
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    <!--<article-title-html>Comparison of aerosol properties retrieved using GARRLiC, LIRIC, and Raman algorithms applied to multi-wavelength lidar and sun/sky-photometer data</article-title-html>
<abstract-html><p class="p">Aerosol particles are important and highly variable components of the
terrestrial atmosphere, and they affect both air quality and climate. In
order to evaluate their multiple impacts, the most important requirement is
to precisely measure their characteristics. Remote sensing technologies such
as lidar (light detection and ranging) and sun/sky photometers are powerful
tools for determining aerosol optical and microphysical properties. In our
work, we applied several methods to joint or separate lidar and
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Aerosol Retrieval from Radiometer and Lidar Combined data) inversion methods
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and lidar ratios) and microphysical properties (volume concentrations,
complex refractive index values, and effective radius values) retrieved using
the aforementioned methods. The comparison showed inconsistencies in the
retrieved lidar ratios. However, other aerosol properties were found to be
generally in close agreement with the AERONET (AErosol RObotic NETwork)
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