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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-21-3015-2021</article-id><title-group><article-title>Automated time–height-resolved air mass source attribution for profiling remote sensing applications</article-title><alt-title>Automated air mass source attribution for profiling remote sensing applications</alt-title>
      </title-group><?xmltex \runningtitle{Automated air mass source attribution for profiling remote sensing applications}?><?xmltex \runningauthor{M. Radenz et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>Radenz</surname><given-names>Martin</given-names></name>
          <email>radenz@tropos.de</email>
        <ext-link>https://orcid.org/0000-0002-7771-033X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Seifert</surname><given-names>Patric</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-5626-3761</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Baars</surname><given-names>Holger</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-2316-8960</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Floutsi</surname><given-names>Athena Augusta</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-9662-8684</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2 aff3">
          <name><surname>Yin</surname><given-names>Zhenping</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-3270-534X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Bühl</surname><given-names>Johannes</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-0354-3487</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Leibniz Institute for Tropospheric Research (TROPOS), Leipzig, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>School of Electronic Information, Wuhan University, Wuhan, China</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Key Laboratory of Geospace Environment and Geodesy, Ministry of Education, Wuhan, China</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Martin Radenz (radenz@tropos.de)</corresp></author-notes><pub-date><day>1</day><month>March</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>4</issue>
      <fpage>3015</fpage><lpage>3033</lpage>
      <history>
        <date date-type="received"><day>11</day><month>September</month><year>2020</year></date>
           <date date-type="rev-request"><day>12</day><month>October</month><year>2020</year></date>
           <date date-type="rev-recd"><day>19</day><month>January</month><year>2021</year></date>
           <date date-type="accepted"><day>28</day><month>January</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 </copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e139">Height-resolved air mass source attribution is crucial for the evaluation of profiling ground-based remote sensing observations, especially when using lidar (light detection and ranging) to investigate different aerosol types throughout the atmosphere. Lidar networks, such as EARLINET (European Aerosol Research Lidar Network)  in the frame of ACTRIS (Aerosol, Clouds and Trace Gases), observe profiles of optical aerosol properties almost continuously, but usually, additional information is needed to support the characterization of the observed particles. This work presents an approach explaining how backward trajectories or particle positions from a dispersion model can be combined with geographical information (a land cover classification and manually defined areas) to obtain a continuous and vertically resolved estimate of an air mass source above a certain location. Ideally, such an estimate depends on as few as possible a priori information and auxiliary data.
An automated framework for the computation of such an air mass source is presented, and two applications are described. First, the air mass source information is used for the interpretation of air mass sources for three case studies with lidar observations from Limassol (Cyprus), Punta Arenas (Chile) and ship-borne off Cabo Verde. Second, air mass source statistics are calculated for two multi-week campaigns to assess potential observation biases of lidar-based aerosol statistics. Such an automated approach is a valuable tool for the analysis of short-term campaigns but also for long-term data sets, for example, acquired by EARLINET.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

      <?xmltex \hack{\newpage}?>
<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e153">Tracing air mass transport through a turbulent atmosphere is (still) a complex problem, especially since the transport of aerosols and, consequently, the interactions with clouds, precipitation and radiation are required to capture the 4D history of an air parcel. When it comes to practical application, such as the analysis of aerosol observations or aerosol–cloud interaction studies, the ease of interpretation is often hindered by the amount of data that needs to be considered.</p>
      <p id="d1e156">The European Research Infrastructure on Aerosol, Clouds and Trace Gases (ACTRIS) aims at investigating short-lived components in the atmosphere, among them aerosols and clouds. As part of ACTRIS, the European Research Lidar Network, EARLINET <xref ref-type="bibr" rid="bib1.bibx43" id="paren.1"/>, operates lidar systems at more than 25 stations to observe atmospheric states and compositions up to 30 <inline-formula><mml:math id="M1" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. The complementary network of Cloudnet <xref ref-type="bibr" rid="bib1.bibx28" id="paren.2"/> utilizes continuous synergistic observations of ground based instruments such as ceilometers, cloud radars, microwave radiometers and Doppler wind lidars to provide comprehensive cloud observations within Europe and at key regions in the climate system.
Both networks, as part of ACTRIS, need additional, continuous information about air mass sources to interpret the observations.
Identifying the air mass source region supports the characterization of new particles, e.g., during volcanic eruptions <xref ref-type="bibr" rid="bib1.bibx42" id="paren.3"/> or strong wildfires injecting aerosol into the stratosphere <xref ref-type="bibr" rid="bib1.bibx9" id="paren.4"/>. Also, for aerosol typing <xref ref-type="bibr" rid="bib1.bibx1 bib1.bibx65 bib1.bibx41 bib1.bibx38 bib1.bibx37" id="paren.5"><named-content content-type="pre">e.g.,</named-content></xref>, air mass sources can<?pagebreak page3016?> provide an important constraint. Furthermore, operational height-resolved air mass source information could improve warning applications for hazardous events, as demonstrated for EARLINET in the frame of the European EUNADICS-AV exercise <xref ref-type="bibr" rid="bib1.bibx41" id="paren.6"><named-content content-type="pre">European Natural Disaster Coordination and Information System for Aviation;</named-content></xref>.</p>
      <p id="d1e190">Models that simulate air mass transport can be broadly grouped into trajectory models and particle dispersion models <xref ref-type="bibr" rid="bib1.bibx18" id="paren.7"><named-content content-type="pre">overview provided by</named-content></xref>. Trajectory models calculate the transport of a single air parcel imposed by the mean meteorological fields. The model simulations can be run either forward or backward in time, providing information about the source and the destination of the air mass, respectively, after a given transport time. Turbulence and vertical motion during the transport are usually parameterized on the grid scale. Commonly used models are HYSPLIT <xref ref-type="bibr" rid="bib1.bibx52" id="paren.8"><named-content content-type="pre">Hybrid Single-Particle Lagrangian Integrated Trajectory model;</named-content></xref>, FLEXTRA <xref ref-type="bibr" rid="bib1.bibx55" id="paren.9"><named-content content-type="pre">flexible trajectories;</named-content></xref> and LAGRANTO <xref ref-type="bibr" rid="bib1.bibx66 bib1.bibx59" id="paren.10"><named-content content-type="pre">Lagrangian analysis tool;</named-content></xref>.
Due to the rather simple approach, the results are quite uncertain <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx46" id="paren.11"/>, but computational requirements are comparably low. A straightforward approach for representing some of the variability is calculating spatial or temporal ensembles of the trajectories <xref ref-type="bibr" rid="bib1.bibx35 bib1.bibx30 bib1.bibx14" id="paren.12"/>.
Lagrangian particle dispersion models (LPDM), with a large number of particles, are set up to cover turbulent and diffusive transport even more realistically <xref ref-type="bibr" rid="bib1.bibx56" id="paren.13"/>. The fate of each particle is tracked individually, allowing more variability to be included into the transport simulation. A frequently used LPDM is FLEXPART <xref ref-type="bibr" rid="bib1.bibx45" id="paren.14"><named-content content-type="pre">FLEXible PARTicle dispersion model;</named-content></xref>.</p>
      <p id="d1e228">Generally, the representation of chaotic motion in the atmosphere improves with larger ensembles of trajectories or increasing numbers of particles. But, with dozens to hundreds of air parcel locations available, interpretation rapidly becomes cumbersome. A number of infinitesimally small air parcels grouped together gives an air mass, which is a larger volume of air with similar properties. Residence times are a well-established technique for attributing regional information to air mass properties, such as being laden with aerosols, moisture or trace gases <xref ref-type="bibr" rid="bib1.bibx5 bib1.bibx6" id="paren.15"/>.</p>
      <p id="d1e235">Using backward simulations of air parcel positions, analysis of the residence time yields useful information about the potential source region of an observed air mass. The basic assumption is that the longer an air parcel was present in a certain region, the more likely it will be influenced by the surface characteristics. Hence, the dimensionality of an air parcel's 4D location can be reduced to the residence time. Approaches for clustering backward trajectories by direction, source regions or latitude are widely used. The majority focus on the interpretation of time series observations at single heights – mostly close to ground <xref ref-type="bibr" rid="bib1.bibx16" id="paren.16"><named-content content-type="pre">e.g.,</named-content></xref>, for aircraft intersects <xref ref-type="bibr" rid="bib1.bibx44" id="paren.17"><named-content content-type="pre">e.g.,</named-content></xref>, or over a whole region <xref ref-type="bibr" rid="bib1.bibx31" id="paren.18"/>. More sophisticated approaches blend the residence time with actual concentration measurements <xref ref-type="bibr" rid="bib1.bibx53 bib1.bibx27" id="paren.19"/>.
However, these approaches require continuous concentration time series, which are generally not available for remote sensing observations. Furthermore, any profile information above the measurement site is neglected.</p>
      <p id="d1e254">When interpreting ground-based remote sensing observations, as obtained from aerosol lidars or cloud radars, the air mass sources have usually been assigned by manually selected periods (time and height above ground) that seem interesting for further investigation and calculation of backward transport for those specific cases <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx34" id="paren.20"><named-content content-type="pre">e.g.,</named-content></xref>. If air mass source estimates are required for longer time periods or multiple heights, calculating, visualizing and interpreting the results become tedious. Hence, a continuous, computationally efficient, easy to interpret and automated air mass source estimate is required. To be broadly and easily applicable, such a source estimate should not require extensive a priori information, such as clusters of trajectories or potential source contribution functions. The required approach is intended to also be simpler than using a coupled aerosol model, such as CAMS <xref ref-type="bibr" rid="bib1.bibx19" id="paren.21"><named-content content-type="pre">Copernicus Atmosphere Monitoring Service;</named-content></xref>, COSMO-MUSCAT <xref ref-type="bibr" rid="bib1.bibx13" id="paren.22"><named-content content-type="pre">COnsortium for Small-scale MOdeling MUltiScale Chemistry Aerosol Transport Model;</named-content></xref> or ICON-ART <xref ref-type="bibr" rid="bib1.bibx49" id="paren.23"><named-content content-type="pre">ICOsahedral Nonhydrostatic Aerosols and Reactive Trace gases;</named-content></xref>. Although these models can provide profiles of atmospheric composition, they usually do not provide information on the source.</p>
      <p id="d1e277">Herein, we propose a combination of automated backward trajectory calculations and geographical information for the setup of a simple, spatiotemporally resolved air mass source attribution scheme. As a proxy for geographical information, two products are used, namely a land cover classification mask and manually defined geographical areas. The methodology is described in Sect. 2. A comprehensive, easy-to-use software package is also provided. Earlier versions were already used in <xref ref-type="bibr" rid="bib1.bibx25" id="text.24"/>, <xref ref-type="bibr" rid="bib1.bibx21" id="text.25"/> and <xref ref-type="bibr" rid="bib1.bibx20" id="text.26"/>. Afterwards, two applications illustrate the potential use cases. In the first example, the temporal and vertical evolution of the air mass source is analyzed for three lidar observations of different aerosol conditions from Limassol (Cyprus), Punta Arenas (Chile) and on board R/V <italic>Polarstern</italic> off Cabo Verde. In the second example, vertically resolved air mass source statistics are used to assess potential observation biases of long-term lidar-based aerosol statistics. Two multi-week campaigns of the PollyNET <xref ref-type="bibr" rid="bib1.bibx7" id="paren.27"/>, as a part of EARLINET, are presented, namely Finokalia (Greece) and Krauthausen (Germany).</p>
</sec>
<?pagebreak page3017?><sec id="Ch1.S2">
  <label>2</label><title>Air mass source attribution method</title>
      <p id="d1e303">In a conceptualized view, properties of an air parcel arriving over a location of interest are characterized by a certain surface type if the air was close to the surface during its traveled path. The proximity to the surface can be parameterized as a reception height, which depends on the mixing state of the atmosphere at this location and on the type of aerosol particles that could potentially be emitted (i.e., mineral dust or sea salt). Conceivable choices for the reception height are the model-derived depth of the atmospheric boundary layer or fixed thresholds. As a first estimate for the identification of possible surface effects on an air parcel, 2 <inline-formula><mml:math id="M2" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> is widely used <xref ref-type="bibr" rid="bib1.bibx62" id="paren.28"/>. It is assumed that the longer an air parcel resides close to the surface, the more likely it will acquire the aerosol footprint of the surface. The residence time – the total time an air parcel spent over a certain surface and below the reception height – is a first hint of the aerosol characteristics of the air parcel.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F1" specific-use="star"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e319">Example of how the residence time profile is calculated. HYSPLIT ensemble backward trajectories <bold>(a)</bold> and FLEXPART particle positions <bold>(c)</bold> ending above Limassol on 14 September 2017, 00:00 UTC, at 3 <inline-formula><mml:math id="M3" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. The number of FLEXPART particles is reduced by a factor of 4 in this visualization (i.e., 10 000 instead of 40 000). A time-resolved version with all particles is provided in the Supplement. Air parcel height is color coded. The simplified MODIS land surface classification (Fig. <xref ref-type="fig" rid="Ch1.F2"/>) is shown in the background. The profiles of normalized residence time with a reception height threshold of <inline-formula><mml:math id="M4" display="inline"><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:mrow></mml:math></inline-formula> for HYSPLIT ensemble trajectories <bold>(b)</bold> and FLEXPART particle positions <bold>(d)</bold> are shown.</p></caption>
        <?xmltex \igopts{width=355.659449pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f01.png"/>

      </fig>

      <p id="d1e363">The transport pathway of an air mass arriving over the site can be computed using either mean-wind trajectories or a particle dispersion model. Both approaches can be used with the method proposed in this study. Mean wind trajectories for the past 10 d are calculated using HYSPLIT <xref ref-type="bibr" rid="bib1.bibx52" id="paren.29"/>. To account for variability, ensemble trajectories consisting of 27 members, spaced 0.3<inline-formula><mml:math id="M5" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontally and 220 <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> vertically around the end point, are used (Fig. <xref ref-type="fig" rid="Ch1.F1"/>a). Meteorological input data for HYSPLIT are obtained from the Global Data Assimilation System data set at 1<inline-formula><mml:math id="M7" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> horizontal resolution (GDAS1) and are provided by the Air Resources Laboratory (ARL) of the U.S. National Weather Service's National Centers for Environmental Prediction <xref ref-type="bibr" rid="bib1.bibx4" id="paren.30"><named-content content-type="pre">NCEP;</named-content></xref>. The location of the air parcel is stored in 1 h steps. A more realistic representation of turbulence and mixing can be achieved using a LPDM, which simulates the pathway of hundreds to thousands of particles. Here, the most recent version of FLEXPART <xref ref-type="bibr" rid="bib1.bibx57 bib1.bibx45" id="paren.31"/> is used. Meteorological data are obtained from the GFS (Global Forecast System) analysis at a horizontal resolution of 1<inline-formula><mml:math id="M8" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx40" id="paren.32"/>. For each height, 500 particles are used, with the particle positions being stored every 3 h. These simulations are run every 3 h, with height steps of 500 <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> for the whole period of interest.</p>

      <?xmltex \floatpos{p}?><fig id="Ch1.F2" specific-use="star"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e429">The simplified MODIS land cover classification. Details are given in the text.</p></caption>
        <?xmltex \igopts{width=312.980315pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f02.png"/>

      </fig>

      <p id="d1e438">In this work, the surface is classified by two methods. The first method is based on a simplified version of the MODIS land cover classification <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx10" id="paren.33"/>. The 17 categories of the original data set are grouped into seven categories according to Table <xref ref-type="table" rid="Ch1.T1"/> in order to allow for robust statistics in the output (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). Additionally, the horizontal resolution is reduced to 0.1<inline-formula><mml:math id="M10" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>. The categories do not resolve the annual cycles, for example, due to growing seasons. The second method involves custom defined areas as polygons, named according to their geographical context (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). These areas can be tailored to the measurement location and/or scientific interest.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Table}?><label>Table 1</label><caption><p id="d1e462">Overview of how the MODIS land surface categories translate into the simplified categories used in this study. MODIS category numbers as in <xref ref-type="bibr" rid="bib1.bibx10" id="text.34"/>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="2">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">MODIS category</oasis:entry>
         <oasis:entry colname="col2">Simplified category</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">0</oasis:entry>
         <oasis:entry colname="col2">Water</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">1, 2, 3, 4, 5, 6</oasis:entry>
         <oasis:entry colname="col2">Forest</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">7, 8, 9</oasis:entry>
         <oasis:entry colname="col2">Savanna/shrubland</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">10, 11, 12, 14</oasis:entry>
         <oasis:entry colname="col2">Grassland and/or cropland</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">13</oasis:entry>
         <oasis:entry colname="col2">Urban</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">15</oasis:entry>
         <oasis:entry colname="col2">Snow</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">16</oasis:entry>
         <oasis:entry colname="col2">Barren</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e558">The custom defined geographical areas for Limassol, Finokalia, Krauthausen (all shown in <bold>a</bold>), Punta Arenas <bold>(b)</bold> and the Atlantic transit <bold>(c)</bold>. Locations of the sites are also marked on the respective maps.</p></caption>
        <?xmltex \igopts{width=213.395669pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f03.png"/>

      </fig>

      <p id="d1e576"><?xmltex \hack{\newpage}?>The residence times at each time and height step are summed for each land cover class or polygon, where the air parcel was below the reception height.
Within this study, the widely applicable reception height threshold of 2 <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> is used <xref ref-type="bibr" rid="bib1.bibx62" id="paren.35"/>. Different settings can be easily applied to study events which are entrained at greater heights, such as wildfire smoke emission or volcanic eruptions. The vertical air mass transport during such events is usually not accurately covered by atmospheric models. Setting the reception height to the maximum emission height of such events (as can be estimated, e.g., from satellite observations) can bypass the uncertainties in the modeled vertical motion. The residence times for each category and each height can then be visualized as a profile (Fig. <xref ref-type="fig" rid="Ch1.F1"/>b). Where the residence time is <inline-formula><mml:math id="M12" display="inline"><mml:mn mathvariant="normal">0</mml:mn></mml:math></inline-formula>, no air parcels were observed below the reception height during the duration of the backward simulation. In the example shown in  Fig. <xref ref-type="fig" rid="Ch1.F1"/>b, above 5 <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, no air masses resided at heights below 2 <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> above the ground in the previous 10 d.
The theoretical maximum residence time (in hours) depends on the number of trajectories or particles <inline-formula><mml:math id="M15" display="inline"><mml:mi>n</mml:mi></mml:math></inline-formula>, the duration of backward calculation <inline-formula><mml:math id="M16" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> in days and the interval of output <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>o</mml:mi></mml:mrow></mml:math></inline-formula> in hours as follows:
          <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M18" display="block"><mml:mrow><mml:msub><mml:mi>t</mml:mi><mml:mtext>max</mml:mtext></mml:msub><mml:mo>=</mml:mo><mml:mi>n</mml:mi><mml:mi>d</mml:mi><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">24</mml:mn><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>o</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>.</mml:mo></mml:mrow></mml:math></disp-formula></p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e673"><bold>(a)</bold> Quasi particle backscatter coefficient at 1064 <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> observed by Polly<inline-formula><mml:math id="M20" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> on board R/V <italic>Polarstern</italic> close to Cabo Verde on 30 and 31 May 2018. Moving average smoothing of eight range bins (60 <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) and 10 temporal bins (5 min) was applied. The red overlays show the Klett-derived particle backscatter coefficient from the automated algorithm at 532 <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>. The time period of manual analysis (see text) is marked by a horizontal orange bar. <bold>(b)</bold> Volume depolarization ratio at 532 <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> for the same period. No smoothing was applied.</p></caption>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f04.png"/>

      </fig>

      <p id="d1e732">To illustrate the temporal evolution, successive air mass source profiles can be shown one after another. This visualization condenses the 4D history of a multitude of trajectories (or thousands of particle positions) to a quickly understandable summary, which structures information on air mass source into a time–height cross section. Such a format is usually obtained from vertically or nadir-pointed active ground-based remote sensing observations (e.g., Fig. <xref ref-type="fig" rid="Ch1.F4"/>).</p>
</sec>
<sec id="Ch1.S3">
  <label>3</label><?xmltex \opttitle{Polly${}^{\mathrm{XT}}$ lidar observations}?><title>Polly<inline-formula><mml:math id="M24" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> lidar observations</title>
      <?pagebreak page3019?><p id="d1e755">The air mass source estimate is used to interpret observations conducted with the Polly<inline-formula><mml:math id="M25" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> lidar <xref ref-type="bibr" rid="bib1.bibx15" id="paren.36"/>.
Polly<inline-formula><mml:math id="M26" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> is equipped with backscatter channels at 1064, 532 and 355 <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> and Raman and depolarization channels at the shorter two wavelengths. The optical properties are derived using the automated PollyNET retrieval <xref ref-type="bibr" rid="bib1.bibx7 bib1.bibx8 bib1.bibx69" id="paren.37"/> and manual analysis of single profiles. One product of the PollyNET retrieval is the quasi backscatter coefficient, where the attenuated backscatter is corrected for molecular extinction. For this approach, the background, range and dead-time-corrected lidar profiles are normalized by the so-called lidar calibration parameter (also sometimes called the lidar constant even though it is not constant) which is derived from Raman or Klett retrievals <xref ref-type="bibr" rid="bib1.bibx7" id="paren.38"><named-content content-type="pre">see</named-content></xref>. This normalization gives the attenuated backscatter coefficient from ground (note that, for the same atmospheric scene, the attenuated backscatter measured from ground is different to the one measured from space as it is not corrected for attenuation by molecules and particles). The molecular contribution to the atmospheric backscattering and extinction can be calculated from pressure and temperature profiles; the attenuated backscatter coefficient is corrected for the molecular scattering. Furthermore, an assumption of a fixed lidar ratio is applied on the attenuated backscatter corrected for molecular contribution to account for a first guess of the particulate attenuation. This procedure gives the quasi particle backscatter coefficient, which is a good proxy for the real particle backscatter coefficient that cannot yet be obtained at a high temporal resolution for all atmospheric scenes. More details are covered in <xref ref-type="bibr" rid="bib1.bibx8" id="text.39"/>.</p>
      <p id="d1e799">Polly<inline-formula><mml:math id="M28" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> was deployed to various field campaigns and longer-term measurements during the last 15 years <xref ref-type="bibr" rid="bib1.bibx7" id="paren.40"/>. A broad variety of meteorological conditions and aerosol regimes was covered. The multi-wavelength observations of Polly<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> contain unique fingerprints of the observed aerosol types from different source regions <xref ref-type="bibr" rid="bib1.bibx29" id="paren.41"/>.</p>
      <p id="d1e826">In Sects. 4 and 5, the air mass source attribution will be applied to selected case studies and measurement campaigns in order to demonstrate its applicability for determinating the air mass source regions and for the estimate of potential observation biases. The case studies are chosen from deployments of Polly<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> to Limassol (Cyprus; 34.7<inline-formula><mml:math id="M31" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 33.0<inline-formula><mml:math id="M32" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E; 12 m above sea level (a.s.l.); October 2016 to March 2018), Punta Arenas (Chile; 53.1<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> S, 70.9<inline-formula><mml:math id="M34" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W; 10 m a.s.l.; November 2018 and ongoing) and the Atlantic transit of R/V <italic>Polarstern</italic> in 2018 when passing Cabo Verde (18.1<inline-formula><mml:math id="M35" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 21.3<inline-formula><mml:math id="M36" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W to 21.3<inline-formula><mml:math id="M37" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 20.8<inline-formula><mml:math id="M38" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W).
The estimate of potential observation biases is done for two multi-week campaigns. One at Krauthausen (Germany; 50.9<inline-formula><mml:math id="M39" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 6.4<inline-formula><mml:math id="M40" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E; 99 m a.s.l.) took place for 8 weeks in April–May 2013 and the second one was at Finokalia (Greece; 35.3<inline-formula><mml:math id="M41" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N 25.7<inline-formula><mml:math id="M42" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E; 250 m a.s.l.) for 6.5 weeks in June–July 2014.</p>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Application to lidar case studies</title>
<sec id="Ch1.S4.SS1">
  <label>4.1</label><title>Saharan dust off the coast of West Africa</title>
      <p id="d1e967">A lofted layer of dust was observed on 30 and 31 May 2018 by a Polly<inline-formula><mml:math id="M43" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> system on board R/V <italic>Polarstern</italic> <xref ref-type="bibr" rid="bib1.bibx58" id="paren.42"/> as the ship steamed between Cabo Verde and the African mainland (18.1<inline-formula><mml:math id="M44" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 21.3<inline-formula><mml:math id="M45" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W to 21.3<inline-formula><mml:math id="M46" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 20.8<inline-formula><mml:math id="M47" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> W) on her transit north from Punta Arenas (Chile) to Bremerhaven (Germany). A detailed description of the event and optical properties of the observed aerosol were already reported by <xref ref-type="bibr" rid="bib1.bibx70" id="text.43"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e1027">Profiles of optical properties on 30 May 2018, between 22:00 and 22:59 UTC, manually derived with the Raman method. A vertical smoothing of 35 bins (262.5 <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) was applied.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f05.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e1046">Air mass source estimate from 06:00 UTC on 30 May 2018 to 06:00 UTC on 31 May 2018 for the land surface classification <bold>(a, b)</bold> and the named geographical areas <bold>(b, d)</bold>, based on HYSPLIT ensemble trajectories <bold>(a, c)</bold> and FLEXPART particle positions <bold>(b, d)</bold>.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f06.png"/>

        </fig>

      <p id="d1e1068">Figure <xref ref-type="fig" rid="Ch1.F4"/> illustrates the temporal evolution of the observed aerosol plume by means of a time–height cross section of the 1064 <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> quasi particle backscatter coefficient for the time period from 30 May 06:00 UTC to 31 May 06:00 UTC.
<xref ref-type="bibr" rid="bib1.bibx70" id="text.44"/> already discussed this case, especially the period from 16:00 to 17:00 UTC (their Fig. 14). Optical parameters from the Raman analysis during the following night from 22:00 to 23:00 UTC are shown in Fig. <xref ref-type="fig" rid="Ch1.F5"/> (period marked in Fig. <xref ref-type="fig" rid="Ch1.F4"/>a with a horizontal orange bar). According to the optical properties, Yin et al. (2019) argued that the lowest 1 <inline-formula><mml:math id="M50" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> was dominated by marine particles and a certain contribution from European continental aerosol. Patchy, liquid clouds were observed at the boundary layer top, especially around 09:00 and 19:00 UTC.
At larger heights, between 1.8 and 5.2 <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, a Saharan dust plume with extinction values as large as 700 <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">Mm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> was present. Lidar ratios were 60 <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula> and particle linear depolarization ratios at 532 <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> of 0.35. The low Ångström exponent between the 532 and 355 <inline-formula><mml:math id="M55" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> backscatter coefficients is consistent with values reported by <xref ref-type="bibr" rid="bib1.bibx64" id="text.45"/> and <xref ref-type="bibr" rid="bib1.bibx50" id="text.46"/>. <xref ref-type="bibr" rid="bib1.bibx70" id="text.47"/> corroborate their findings by ensemble calculations of HYSPLIT backward trajectories for selected arrival heights and times. However, this way of presentation is rather selective, as information for different heights and times can hardly be shown. This is where the benefit of the continuous air mass source estimate becomes evident. Figure <xref ref-type="fig" rid="Ch1.F6"/> presents the results of the air mass source estimate for the land surface classification and geographical areas for both the HYSPLIT (Fig. <xref ref-type="fig" rid="Ch1.F6"/>a, c) and the FLEXPART simulations (Fig. <xref ref-type="fig" rid="Ch1.F6"/>b, d).
The estimates based on HYSPLIT and FLEXPART show a good general agreement. The heights and times of certain surface types and geographical regions agree qualitatively. Before 12:00 UTC on 30 May 2018, FLEXPART derived a lower residence time from barren and grassland regions or Africa, respectively. With respect to Fig. <xref ref-type="fig" rid="Ch1.F4"/>, this seems to be reasonable as the layer was rather faint at the beginning of the shown measurement period. Besides this difference, both the HYSPLIT and FLEXPART approaches provide a concise picture of the likely source regions of the observed aerosol. Below 1.5 <inline-formula><mml:math id="M56" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, the air mass was marine dominated, with a small contribution of European grass and/or cropland. At heights between 2 and 4 <inline-formula><mml:math id="M57" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>, barren areas from Africa are the main source, but a considerable fraction is also attributed to African grass/cropland and savanna. This finding supports the observations presented by <xref ref-type="bibr" rid="bib1.bibx70" id="text.48"/>, who already discussed that there was likely a small non-dust fraction in the upper layer as the particle depolarization ratio profile was not constant at all heights. A potential reason for the observed discrepancy in the observations from pure dust conditions could be the presence of wildfire smoke stemming from the crop/grassland and savanna. In comparison to the lidar observations, the top of the layer was slightly<?pagebreak page3022?> underestimated by the air mass source estimate.
The temporal extent is also fully captured. Variability in backscatter within the layer is not represented by the air mass source estimate because the strength of dust mobilization is insufficiently parameterized by the reception height. However, the air mass transport is correctly covered by both estimates. Interestingly, the air mass source estimation for this case provides some information with an added value with respect to the lidar observations. As both HYSPLIT and FLEXPART approaches indicate, North American air masses were present in the upper troposphere during the time of the observation, which, however, had too low an aerosol load to be detectable by the Polly<inline-formula><mml:math id="M58" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> lidar.</p>
</sec>
<sec id="Ch1.S4.SS2">
  <label>4.2</label><title>Saharan and Arabian dust at Limassol, Cyprus</title>
      <p id="d1e1198">On 14 September 2017 an upper level shortwave trough moved eastward from the Aegean Sea towards Cyprus. Above 1 <inline-formula><mml:math id="M59" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, the wind turned from southwest to south during the course of the day, with velocities ranging between 5–15 m s<inline-formula><mml:math id="M60" 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>, whereas, below the 1 <inline-formula><mml:math id="M61" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, wind velocity was lower and the direction was more variable.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e1231"><bold>(a)</bold> Quasi particle backscatter coefficient at 1064 <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> observed by Polly<inline-formula><mml:math id="M63" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> at Limassol on 14 September 2017. Moving average smoothing of eight range bins (60 <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) and 10 temporal bins (5 min) was applied. The red overlays show the Klett-derived particle backscatter coefficient at 532 <inline-formula><mml:math id="M65" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>. The time periods of manual analysis (Figs. <xref ref-type="fig" rid="Ch1.F8"/> and <xref ref-type="fig" rid="Ch1.F9"/>) are marked by horizontal orange bars. <bold>(b)</bold> Volume depolarization ratio at 532 <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> for the same period. No smoothing was applied.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f07.png"/>

        </fig>

      <p id="d1e1291">The time–height cross section of quasi particle backscatter observed by Polly<inline-formula><mml:math id="M67" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> at Limassol shows two pronounced aerosol layers above the boundary layer (Fig. <xref ref-type="fig" rid="Ch1.F7"/>). The first layer was observed between 1 and 2 <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height from 00:00 to 09:00 UTC and a second, thicker layer after 03:00 UTC. Until nighttime, this layer increases in thickness from bases at 3 <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> and tops at 4.5 <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height to bases at 1.2 <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> and tops at 6.5 <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height.
The boundary layer itself is also laden with aerosols and shows significant backscatter below 1 <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e1357">Profiles of optical properties on 14 September 2017, between 02:59 and 04:02 UTC, manually derived with the Raman method. A smoothing of 99 range bins (742.5 <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) was applied. The abbreviation NR indicates the profiles observed with the larger field of view near-range telescope.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f08.png"/>

        </fig>

      <p id="d1e1374">The optical parameters of the aerosol plume were analyzed for two periods, namely 02:59–04:02 UTC in the morning and 21:41–22:39 UTC in the evening (periods marked in Fig. <xref ref-type="fig" rid="Ch1.F7"/>a with horizontal orange bars). The profiles from the morning period (Fig. <xref ref-type="fig" rid="Ch1.F8"/>) show, for the lower layer at 1.8 <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, particle depolarization ratios of 0.25 (355 and 532 <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>) and low Ångström values and lidar ratios around 40 <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M78" display="inline"><mml:mn mathvariant="normal">355</mml:mn></mml:math></inline-formula> and  532 <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>). These optical parameters and their independence of wavelength are typical for aerosol mixtures with a high dust fraction. Extinction in this layer peaks at 72 <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Mm</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M81" 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> (355 and  532 <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>). The second layer, above 2.5 <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, has particle backscatter values of less than 2 <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Mm</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M85" 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> <inline-formula><mml:math id="M86" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M87" 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> (at 355 <inline-formula><mml:math id="M88" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>) and 0.5 <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">Mm</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M90" 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> <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula><inline-formula><mml:math id="M92" 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> (at 532 <inline-formula><mml:math id="M93" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>). Ångström values are slightly higher than in the lower layer, varying between one and two. The particle depolarization ratios, at both the 355 and 532 <inline-formula><mml:math id="M94" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> wavelength, are between <inline-formula><mml:math id="M95" display="inline"><mml:mn mathvariant="normal">0.05</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math id="M96" display="inline"><mml:mn mathvariant="normal">0.10</mml:mn></mml:math></inline-formula>. This upper layer during the morning is already the leading edge of the second plume that increased in thickness during the day (both geometrically and optical). As shown in Fig. <xref ref-type="fig" rid="Ch1.F7"/>b, the volume depolarization ratio increased only slowly during the averaging period.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9" specific-use="star"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e1577">Profiles of optical properties on 14 September 2017, between 21:41 and 22:39 UTC, manually derived with the Raman method. A smoothing of 99 range bins (742.5 <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) was applied. The abbreviation of NR indicates profiles observed with the larger field of view near-range telescope.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f09.png"/>

        </fig>

      <p id="d1e1594">During the evening (Fig. <xref ref-type="fig" rid="Ch1.F9"/>), the upper layer extended from <inline-formula><mml:math id="M98" display="inline"><mml:mn mathvariant="normal">1.3</mml:mn></mml:math></inline-formula> to 6 <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height and shows homogeneous and mostly wavelength-independent optical properties throughout. Particle depolarization ratios were between <inline-formula><mml:math id="M100" display="inline"><mml:mn mathvariant="normal">0.10</mml:mn></mml:math></inline-formula> and <inline-formula><mml:math id="M101" display="inline"><mml:mn mathvariant="normal">0.15</mml:mn></mml:math></inline-formula>, with 532 <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> values slightly higher than those at 355 <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>. Lidar ratios in that layer were 35 <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula>, typical for Middle Eastern dust <xref ref-type="bibr" rid="bib1.bibx32 bib1.bibx39" id="paren.49"/>, while the particle depolarization ratio hints towards a mixture of mineral dust and anthropogenic pollution <xref ref-type="bibr" rid="bib1.bibx60" id="paren.50"><named-content content-type="pre">e.g.,</named-content></xref>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e1663">Air mass source estimate on 14 September 2017 for the land surface classification <bold>(a, b)</bold> and the named geographical areas <bold>(b, d)</bold>, based on HYSPLIT ensemble trajectories <bold>(a, c)</bold> and FLEXPART particle positions <bold>(b, d)</bold>.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f10.png"/>

        </fig>

      <p id="d1e1685">The air mass source estimate (Fig. <xref ref-type="fig" rid="Ch1.F10"/>) identifies transport from barren-ground-influenced air from the Sahara until 09:00 UTC. Later, corresponding to the change in wind direction, the source for the air aloft is identified as Arabian Peninsula but is still in the barren class.
Below 1 <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, a mixture of surfaces was observed, originating mostly form Europe. Comparing the source estimate based on HYSPLIT (Fig. <xref ref-type="fig" rid="Ch1.F10"/>a, c) with the one from FLEXPART (Fig. <xref ref-type="fig" rid="Ch1.F10"/>b, d), both models agree qualitatively well again. While the general transition was captured by the source estimate, the leading edge of the Arabian Peninsula plume was observed over Limassol earlier than indicated. The increase in the thickness of this plume is represented in the source estimate as well.</p>
</sec>
<sec id="Ch1.S4.SS3">
  <label>4.3</label><title>Biomass burning aerosol at Punta Arenas, Chile</title>
      <p id="d1e1710">Punta Arenas is located in a region where the atmosphere is known to be clean and one of the least affected by anthropogenic influences <xref ref-type="bibr" rid="bib1.bibx26" id="paren.51"/>. Nevertheless, events of aerosol long-range transport occur occasionally <xref ref-type="bibr" rid="bib1.bibx21 bib1.bibx20" id="paren.52"/>. Due to the large distance between Punta Arenas and the aerosol source regions, an attribution of observed aerosol events is, in general, rather complicated. The application of air mass source estimates for the characterization of an aerosol long-range transport event is presented here. An upper-level ridge was located off the Chilean coast on 20 May 2019, which also supported a surface high-pressure system. At Punta Arenas, the flow was zonal throughout the troposphere. Within that flow, long-range transport from across the Pacific Ocean occurred.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e1721">Quasi particle backscatter coefficient at 1064 <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> observed by Polly<inline-formula><mml:math id="M107" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> at Punta Arenas on 20 May 2019. Moving average smoothing of eight range bins (60 <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) and 10 temporal bins (5 min) was applied. The red overlay shows the Klett-derived particle backscatter coefficient at 532 <inline-formula><mml:math id="M109" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula>. The time period of the manual analysis (Fig. <xref ref-type="fig" rid="Ch1.F12"/>) is marked by a horizontal orange bar.</p></caption>
          <?xmltex \igopts{width=338.587795pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f11.png"/>

        </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F12" specific-use="star"><?xmltex \currentcnt{12}?><?xmltex \def\figurename{Figure}?><label>Figure 12</label><caption><p id="d1e1767">Profiles of optical properties on 20 May 2019, between 02:50 and 04:30 UTC, manually derived with the Raman method. A smoothing of range 153 bins (1147.5 <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula>) was applied. The abbreviation NR indicates profiles observed with the larger field of view near-range telescope.</p></caption>
          <?xmltex \igopts{width=332.897244pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f12.png"/>

        </fig>

      <p id="d1e1785">In the Polly<inline-formula><mml:math id="M111" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> observations from 20 May 2019 a layer of increased backscatter is present from 02:00 UTC to roughly 10:00 UTC. This layer extends from 3 <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> to above 6 <inline-formula><mml:math id="M113" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height (Fig. <xref ref-type="fig" rid="Ch1.F11"/>). From 14:00 to 18:00 UTC a low-level liquid cloud was observed at 1.5 <inline-formula><mml:math id="M114" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. The cloud was optically thick enough to significantly attenuate the laser beam, causing a lack of signal above the cloud's top. Occasional cirrus clouds also enhanced the backscatter in the free troposphere, e.g., at 12:00 UTC, between <inline-formula><mml:math id="M115" display="inline"><mml:mn mathvariant="normal">4</mml:mn></mml:math></inline-formula> and 5 <inline-formula><mml:math id="M116" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>. The values of particle backscatter peaked at 0.3 <inline-formula><mml:math id="M117" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">Mm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M118" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">sr</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>  (Fig. <xref ref-type="fig" rid="Ch1.F12"/>), which are significantly lower values than reported for the prior cases. In the period analyzed, extinction values were approximately 15 <inline-formula><mml:math id="M119" display="inline"><mml:mrow class="unit"><mml:msup><mml:mi mathvariant="normal">Mm</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, giving lidar ratios well above 50 <inline-formula><mml:math id="M120" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">sr</mml:mi></mml:mrow></mml:math></inline-formula> and rather low linear particle depolarization ratios. Altogether, these optical parameters agree with prior findings of wildfire smoke in the troposphere <xref ref-type="bibr" rid="bib1.bibx61 bib1.bibx11 bib1.bibx24 bib1.bibx63" id="paren.53"/>.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F13" specific-use="star"><?xmltex \currentcnt{13}?><?xmltex \def\figurename{Figure}?><label>Figure 13</label><caption><p id="d1e1897">Air mass source estimate on 20 May 2019 for the land surface classification <bold>(a, b)</bold> and the named geographical areas <bold>(b, d)</bold>, based on HYSPLIT ensemble trajectories <bold>(a, c)</bold> and FLEXPART particle positions <bold>(b, d)</bold>.</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f13.png"/>

        </fig>

      <?pagebreak page3023?><p id="d1e1918">The air mass source estimate is also able to capture this faint aerosol layer. Fig. <xref ref-type="fig" rid="Ch1.F13"/> shows that air masses from Australia were present between 03:00 and 09:00 UTC from <inline-formula><mml:math id="M121" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula> to 6 <inline-formula><mml:math id="M122" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. In terms of land cover class, these air masses were characterized by savanna/shrubland and grass. Wildfires were active in southwestern Australia between 10 and 16 May 2019, which is also the region where the backward simulations end (Fig. <xref ref-type="fig" rid="App1.Ch1.S1.F16"/>).
Apart from the described period, the air masses were solely influenced by the Southern Ocean (i.e., the water class). FLEXPART simulations (Fig. <xref ref-type="fig" rid="Ch1.F13"/>b, d) agree with the HYSPLIT results; however, the computed temporal extent and the residence times are slightly longer for the latter. Hence, the air mass source scheme is also capable of capturing aerosol transport at hemispheric (i.e., more than 10 000 <inline-formula><mml:math id="M123" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>) scales.</p>
</sec>
</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Assessing potential observation biases</title>
      <p id="d1e1960">Vertically resolved aerosol statistics are prone to observation biases, as they usually depend on cloud-free conditions. When clouds or precipitation are present, no aerosol properties can be obtained from optical techniques.
However, respective statistics, for example, obtained from lidar observations, provide key quantities for the determination of the environmental conditions at a certain site <xref ref-type="bibr" rid="bib1.bibx33 bib1.bibx68 bib1.bibx7" id="paren.54"/>. It is therefore an open question whether the data from suitable (cloud-free) measurement periods are representative for the full observational period. Chances are that cloudy conditions are related to certain air masses which would stay unidentified in the lidar-based statistics of aerosol optical properties. One way<?pagebreak page3024?> to assess this bias is to compare the air mass residence time statistics of the full observational period with the one subsampled to the times when aerosol information is available.</p>
      <p id="d1e1966">When applied to lidar data, the automatically analyzed profiles of particle backscatter at 532 <inline-formula><mml:math id="M124" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">nm</mml:mi></mml:mrow></mml:math></inline-formula> from <xref ref-type="bibr" rid="bib1.bibx7" id="text.55"/> are used.
In their work, the raw profiles are grouped into 30 min chunks, cloud screened, averaged and analyzed by either the Klett or the Raman method to see if signal-to-noise ratio is high enough for a reference height to be set.
All profiles that pass a basic quality control are then included in the backscatter statistics. Obviously, this statistic will only be intermittent, due to overcast cloud conditions or interruptions in the measurement. Subsampling the air mass source statistics is done by selecting only the air mass source profiles that are temporally close to a valid lidar profile. A time threshold of 1.5 <inline-formula><mml:math id="M125" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> is used for the following statistics. However, covering representative air mass conditions is only a necessary condition and not a sufficient for obtaining representative aerosol statistics.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F14" specific-use="star"><?xmltex \currentcnt{14}?><?xmltex \def\figurename{Figure}?><label>Figure 14</label><caption><p id="d1e1990">Statistics of particle backscatter coefficient (<bold>a</bold>, as in <xref ref-type="bibr" rid="bib1.bibx7" id="altparen.56"/>) and air mass source estimate, based on FLEXPART particle positions for the Finokalia campaign of Polly<inline-formula><mml:math id="M126" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> in June and July 2014. The land surface classification <bold>(b)</bold> and the named geographical areas <bold>(c)</bold> are shown for the full duration (solid lines) and subsampled only for the periods with available lidar data (dotted lines). The subsampled residence times are divided by the fraction of the time covered. The reception height threshold is 2 <inline-formula><mml:math id="M127" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f14.png"/>

      </fig>

      <?xmltex \floatpos{t}?><fig id="Ch1.F15" specific-use="star"><?xmltex \currentcnt{15}?><?xmltex \def\figurename{Figure}?><label>Figure 15</label><caption><p id="d1e2032">Statistics of particle backscatter coefficient (<bold>a</bold>, as in <xref ref-type="bibr" rid="bib1.bibx7" id="altparen.57"/>) and air mass source estimate, based on FLEXPART particle positions for the Krauthausen campaign of Polly<inline-formula><mml:math id="M128" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> in April and May 2013. The land surface classification <bold>(b)</bold> and the named geographical areas <bold>(c)</bold> are shown for the full duration (solid lines) and subsampled only for the periods with available lidar data (dotted lines). The subsampled residence times are divided by the fraction of time covered. The reception height threshold is 2 <inline-formula><mml:math id="M129" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>.</p></caption>
        <?xmltex \igopts{width=384.112205pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f15.png"/>

      </fig>

      <p id="d1e2071">Polly<inline-formula><mml:math id="M130" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> observations at Krauthausen (Germany; April–May 2013) and Finokalia (Greece; June–July 2014) are used here.
At Finokalia, 940 profiles could be analyzed with the<?pagebreak page3025?> Klett method. Hence, the particle backscatter statistic covers 457.7 <inline-formula><mml:math id="M131" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula>, which is 42 % of the campaign duration. The statistics of particle backscatter are shown in Fig. <xref ref-type="fig" rid="Ch1.F14"/>a. For the Krauthausen deployment, 315 profiles could be analyzed with the Klett method, covering 154.2 <inline-formula><mml:math id="M132" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">h</mml:mi></mml:mrow></mml:math></inline-formula> or 11 % of the campaign. Figure <xref ref-type="fig" rid="Ch1.F15"/>a shows the particle backscatter statistics.</p>
      <p id="d1e2103">Profiles of air mass source for the Finokalia deployment are shown in Fig. <xref ref-type="fig" rid="Ch1.F14"/>b and c, again with a reception height threshold of 2 <inline-formula><mml:math id="M133" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>. The summed residence time of the subsampled profiles is divided by the fraction of time covered to make them comparable to the full residence time. Most dominant land surface categories are water, barren ground<?pagebreak page3026?> and grass-/cropland. The residence time of air masses from barren ground shows a pronounced maximum between <inline-formula><mml:math id="M134" display="inline"><mml:mn mathvariant="normal">2</mml:mn></mml:math></inline-formula> and 6 <inline-formula><mml:math id="M135" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. The residence time of all other categories decreases monotonically. Air masses from urban and snow- or ice-covered areas are 10–100 times less frequent than the other categories.</p>
      <p id="d1e2131">In terms of geographical areas (Fig. <xref ref-type="fig" rid="Ch1.F14"/>c), Europe is the most dominant source up to 3 <inline-formula><mml:math id="M136" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> and again above 9 <inline-formula><mml:math id="M137" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. Between <inline-formula><mml:math id="M138" display="inline"><mml:mn mathvariant="normal">3</mml:mn></mml:math></inline-formula> and 6 <inline-formula><mml:math id="M139" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, the Sahara is the most dominant air mass source.
During the campaign period, no air masses from the Arabian Peninsula, that fulfilled the <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M141" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> criterion were transported to Finokalia.</p>
      <?pagebreak page3027?><p id="d1e2186">The dominant sources are well covered by the lidar profiles in terms of land surface; only the barren class is subsampled by a factor of 10 above 6.5 <inline-formula><mml:math id="M142" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height (Fig. <xref ref-type="fig" rid="Ch1.F14"/>b). This agrees with the Sahara also being subsampled above that height. Air masses originating over Europe were also subsampled at heights above 5 <inline-formula><mml:math id="M143" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>.
An undersampling of potentially aerosol-laden air masses by the lidar statistics will cause the backscatter statistics to be biased as low values.</p>
      <?pagebreak page3028?><p id="d1e2207">During the Krauthausen campaign, air masses originating over water were the most frequent ones, followed by grass-/cropland, forest, shrubland and barren ground (Fig. <xref ref-type="fig" rid="Ch1.F15"/>b). Again, the residence times of the barren class show a distinct peak between <inline-formula><mml:math id="M144" display="inline"><mml:mn mathvariant="normal">6</mml:mn></mml:math></inline-formula> and 8 <inline-formula><mml:math id="M145" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height.
Air masses from the Sahara area agree with the barren class (Fig. <xref ref-type="fig" rid="Ch1.F15"/>c). As expected, Europe is the dominant air mass source in the lowest 6 <inline-formula><mml:math id="M146" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, but due to increasing residence times with height for the Sahara source, both appear with equal frequency in the upper troposphere. In the lidar observations, Europe is potentially undersampled by 70 % between <inline-formula><mml:math id="M147" display="inline"><mml:mn mathvariant="normal">1</mml:mn></mml:math></inline-formula> and 10 <inline-formula><mml:math id="M148" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, which is consistent with the grass/cropland and forest class also being undersampled. Barren land surfaces and the Sahara are oversampled by approximately 20 % up to 7 <inline-formula><mml:math id="M149" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height. In the lowermost 2 <inline-formula><mml:math id="M150" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, the land surface classes urban and snow/ice also contribute to the air mass mixture and are slightly oversampled.</p>
</sec>
<sec id="Ch1.S6" sec-type="conclusions">
  <label>6</label><title>Discussion and conclusions</title>
      <p id="d1e2277">In this study, we propose an easy-to-use method for a continuous, height-resolved automated air mass source estimate. With the combination of air mass transport modeling and geographical information, the dimensionality can be reduced, and straightforward visualizations accelerate the interpretation of air mass origin. The air mass source estimate can be used to assist (profiling) aerosol observations, as aerosol load and characteristics are strongly controlled by surface properties and atmospheric transport. Three case studies illustrated the applicability at different sites and under different large-scale flow conditions. In a second application, we showed how the source estimate supports the interpretation of lidar case studies and how potential observation biases can be investigated for longer-term campaigns.</p>
      <p id="d1e2280">The major constraints of the proposed method are discussed in the following.
While the air mass transport itself is generally covered well by trajectory models or LPDMs, linking it to aerosol properties has to be done with care.
First, the reception height is modeled by using the mixing depth of the input fields or fixed values for all surfaces and aerosol particles, where differences could be expected for dust, smoke or wildfire smoke. Nevertheless, the assumption for a general reception height might be valid and can be improved in future. The 2 <inline-formula><mml:math id="M151" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height used in this work was also reported by other studies <xref ref-type="bibr" rid="bib1.bibx62" id="paren.58"><named-content content-type="pre">e.g., for wildfires</named-content></xref> and seem to be applicable over wide ranges of climates and meteorological conditions. In summary, a high residence time over a certain class is only a necessary, not a sufficient, condition for the aerosol load of an air parcel.</p>
      <p id="d1e2296">Second, aerosol particles might be removed by (wet) deposition between the source and observation site. Currently, such processes are not sufficiently reproduced in trajectory models or LPDMs as they require detailed representation of aerosol microphysics and precipitation amount. Some improvements in this regard incorporated in the most recent version of FLEXPART <xref ref-type="bibr" rid="bib1.bibx45" id="paren.59"/>. However, deposition changes only the aerosol load of an air parcel and not the air mass source itself. Judging from the air mass source residence times alone, this process cannot be distinguished from cases in which no emission happened in the first place.
These questions could be addressed in future with a fully fledged aerosol transport model that also includes a tracer of the air mass origin, similar to the scheme shown here.</p>
      <p id="d1e2302">Some uncertainty is caused by the turbulent nature of the transport. For HYSPLIT, a first estimate for the uncertainty of a single parcel location is 20 % of the distance from the trajectory's origin <xref ref-type="bibr" rid="bib1.bibx54" id="paren.60"/>. Hence, for HYSPLIT, a 27-member ensemble was used to attribute this uncertainty. Compared to HYSPLIT, the LPDM FLEXPART allows for a more realistic representation of turbulent transport and better sampling when using hundreds or thousands of particles. However, a qualitatively good agreement between both simulations suggests that the presented air mass source estimate is rather robust, considering uncertainty in the models.</p>
      <p id="d1e2309">In summary, the described compromises are necessary to obtain a continuous, height-resolved, automated air mass source estimate. The provided source code allows us to use FLEXPART particle positions and HYSPLIT trajectories as input. User-defined named geographical areas can be easily added. The runtime environment is provided as a docker container, including FLEXPART v10.4. With that setup, 1 d of air mass source estimate, with the resolution used in this study, can be processed in less than 1 h on a standard desktop computer (2.1 GHz processor; 4 GB RAM; single-threaded).</p>
      <p id="d1e2312">Such an automated air mass source estimate can provide valuable auxiliary information for the analysis of long-term data sets of profiling aerosol observations, such as those collected in the network of EARLINET <xref ref-type="bibr" rid="bib1.bibx43" id="paren.61"/>. The methodology could also be adapted to existing and future space-borne lidar observations, e.g., CALIPSO <xref ref-type="bibr" rid="bib1.bibx67" id="paren.62"><named-content content-type="pre">Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation;</named-content></xref>, Aeolus <xref ref-type="bibr" rid="bib1.bibx48" id="paren.63"/> or EarthCARE <xref ref-type="bibr" rid="bib1.bibx29" id="paren.64"><named-content content-type="pre">Earth Clouds, Aerosols and Radiation Explorer;</named-content></xref>. A first estimate of air mass source could be used to constrain retrievals of optical parameters by narrowing the assumed lidar ratio, as in the case of CALIPSO, or guide subsequent aerosol typing based on intensive aerosol optical properties, as in the case of Aeolus and EarthCARE. But, simulating enough air parcels with sufficient along-track resolution might require further development.</p>
      <p id="d1e2331">With respect to aerosol typing, downstream products, such as estimates of concentration of cloud condensation nuclei or ice nucleating particles <xref ref-type="bibr" rid="bib1.bibx2 bib1.bibx3" id="paren.65"/>, will benefit from the air mass source estimate. Having air mass source information available will advance the implementation of such retrievals into automatic processing, such as the single calculus chain <xref ref-type="bibr" rid="bib1.bibx12" id="paren.66"/> for EARLINET from the ground or for EarthCARE from space. Also, further synergy between lidar target categorizations, such as <xref ref-type="bibr" rid="bib1.bibx8" id="text.67"/> and the source estimate, remain subject to further investigation.</p>
      <p id="d1e2343">Apart from the shown applications, the presented methodology can be utilized to assess profiles of air mass sources when planning field campaigns. Questions on where, when or how long to measure in order to capture a certain mix of aerosol scenarios can easily be answered. In future, the proposed method can be extended further by source maps, for example, by dust source maps derived by the approach of <xref ref-type="bibr" rid="bib1.bibx17" id="text.68"/> or temporally varying information on wildfires and snow and ice cover or biological productivity.</p><?xmltex \hack{\clearpage}?>
</sec>

      
      </body>
    <back><app-group>

<?pagebreak page3029?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title/>

      <?xmltex \floatpos{h!}?><fig id="App1.Ch1.S1.F16"><?xmltex \currentcnt{A1}?><?xmltex \def\figurename{Figure}?><label>Figure A1</label><caption><p id="d1e2362">HYSPLIT ensemble backward trajectories ending above Punta Arenas on 20 May 2019, 06:00 UTC, at 5 <inline-formula><mml:math id="M152" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula> height, together with the MODIS-derived fire radiative power <xref ref-type="bibr" rid="bib1.bibx23" id="paren.69"/>. Dots along the trajectories indicate the height of the air parcel in 12 h intervals. MODIS-derived fire radiative power of fires between 10 and 16 May 2019 is gridded to 2<inline-formula><mml:math id="M153" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p></caption>
        <?xmltex \hack{\hsize\textwidth}?>
        <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/3015/2021/acp-21-3015-2021-f16.png"/>

      </fig>

<?xmltex \hack{\clearpage}?>
</app>
  </app-group><notes notes-type="codedataavailability"><title>Code and data availability</title>

      <p id="d1e2399">The processing software, as used for this publication, is available under <ext-link xlink:href="https://doi.org/10.5281/zenodo.4438051" ext-link-type="DOI">10.5281/zenodo.4438051</ext-link> <xref ref-type="bibr" rid="bib1.bibx47" id="paren.70"/>. The most recent version is available via GitHub at <uri>https://github.com/martin-rdz/trace_airmass_source</uri> (last access: 14 January 2021). A Docker configuration is provided for a straightforward replication of the programming environment, including all dependencies. Meteorological fields for the backward simulations were obtained from  <uri>https://www.ready.noaa.gov/gdas1.php</uri> <xref ref-type="bibr" rid="bib1.bibx4" id="paren.71"/> and <ext-link xlink:href="https://doi.org/10.5065/D6M043C6" ext-link-type="DOI">10.5065/D6M043C6</ext-link> <xref ref-type="bibr" rid="bib1.bibx40" id="paren.72"/>. The data for the fire radiative power map are available at <ext-link xlink:href="https://doi.org/10.5067/FIRMS/MODIS/MCD14ML" ext-link-type="DOI">10.5067/FIRMS/MODIS/MCD14ML</ext-link> <xref ref-type="bibr" rid="bib1.bibx23" id="paren.73"/>. The analyzed Polly<inline-formula><mml:math id="M154" display="inline"><mml:msup><mml:mi/><mml:mi mathvariant="normal">XT</mml:mi></mml:msup></mml:math></inline-formula> and air mass source data are available on request.</p>
  </notes><app-group>
        <supplementary-material position="anchor"><p id="d1e2439">The supplement related to this article is available online at: <inline-supplementary-material xlink:href="https://doi.org/10.5194/acp-21-3015-2021-supplement" xlink:title="zip">https://doi.org/10.5194/acp-21-3015-2021-supplement</inline-supplementary-material>.</p></supplementary-material>
        </app-group><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e2448">MR developed the algorithm and drafted the paper. PS and JB supported the implementation and supervised the work. HB, AAF and ZY analyzed the lidar data. All authors jointly contributed to the paper and the scientific discussion.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e2454">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e2461">This article is part of the special issue “EARLINET aerosol profiling: contributions to atmospheric and climate research”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e2467">We thank the Alfred Wegener Institute as well as the captain and crew of R/V <italic>Polarstern</italic> for their support (grant no. AWI_PS113_00). Many improvements to the Polly instruments, both in terms of hardware and software, were triggered by the fruitful discussions and network activities within EARLINET <xref ref-type="bibr" rid="bib1.bibx43" id="paren.74"/>. We thank Lucia Mona for serving as an editor and gratefully acknowledge the constructive comments from the two anonymous referees.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e2478">This research has been supported by the European Union's Horizon 2020 (ACTRIS; grant no. 654109), the Seventh Framework Programme (BACCHUS; grant no. 603445), the Federal Ministry of Education and Research in Germany (grant nos. 01LK1503F, 01LK1502I, 01LK1209C and 01LK1212C), the Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research (grant no. AWI_PS113_00), and the German Federal Ministry for Economic Affairs and Energy (BMWi; grant no. 50EE1721C.<?xmltex \hack{\newline}?><?xmltex \hack{\newline}?>The publication of this article was funded by the <?xmltex \hack{\newline}?> Open Access Fund of the Leibniz Association.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e2489">This paper was edited by Lucia Mona and reviewed by two anonymous referees.</p>
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  </ref-list></back>
    <!--<article-title-html>Automated time–height-resolved air mass source attribution for profiling remote sensing applications</article-title-html>
<abstract-html><p>Height-resolved air mass source attribution is crucial for the evaluation of profiling ground-based remote sensing observations, especially when using lidar (light detection and ranging) to investigate different aerosol types throughout the atmosphere. Lidar networks, such as EARLINET (European Aerosol Research Lidar Network)  in the frame of ACTRIS (Aerosol, Clouds and Trace Gases), observe profiles of optical aerosol properties almost continuously, but usually, additional information is needed to support the characterization of the observed particles. This work presents an approach explaining how backward trajectories or particle positions from a dispersion model can be combined with geographical information (a land cover classification and manually defined areas) to obtain a continuous and vertically resolved estimate of an air mass source above a certain location. Ideally, such an estimate depends on as few as possible a priori information and auxiliary data.
An automated framework for the computation of such an air mass source is presented, and two applications are described. First, the air mass source information is used for the interpretation of air mass sources for three case studies with lidar observations from Limassol (Cyprus), Punta Arenas (Chile) and ship-borne off Cabo Verde. Second, air mass source statistics are calculated for two multi-week campaigns to assess potential observation biases of lidar-based aerosol statistics. Such an automated approach is a valuable tool for the analysis of short-term campaigns but also for long-term data sets, for example, acquired by EARLINET.</p></abstract-html>
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Baars, Engelmann, Foth, Jimenez, Seifert, and Barja</label><mixed-citation>
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