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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ESSD</journal-id><journal-title-group>
    <journal-title>Earth System Science Data</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ESSD</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Earth Syst. Sci. Data</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1866-3516</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/essd-18-2799-2026</article-id><title-group><article-title>Tethered balloon-borne measurements to characterise the evolution of the Arctic atmospheric boundary layer at the Villum Research Station</article-title><alt-title>BELUGA measurements at Villum Research Station</alt-title>
      </title-group>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1 aff2">
          <name><surname>Dorff</surname><given-names>Henning</given-names></name>
          <email>henning.dorff@uni-leipzig.de</email>
        <ext-link>https://orcid.org/0000-0003-3238-1891</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Siebert</surname><given-names>Holger</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Navale</surname><given-names>Komal</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Ehrlich</surname><given-names>André</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-0860-8216</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Müller</surname><given-names>Joshua</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-6584-2581</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Schäfer</surname><given-names>Michael</given-names></name>
          
        <ext-link>https://orcid.org/0000-0003-1896-1574</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wu</surname><given-names>Fan</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1">
          <name><surname>Wendisch</surname><given-names>Manfred</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-4652-5561</ext-link></contrib>
        <aff id="aff1"><label>1</label><institution>Leipzig Institute for Meteorology, Leipzig University, Leipzig, Germany</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Meteorological Institute of University of Hamburg, University of Hamburg, Hamburg, Germany</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Leibniz Institute for Tropospheric Research e.V., Leipzig, Germany</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Henning Dorff (henning.dorff@uni-leipzig.de)</corresp></author-notes><pub-date><day>21</day><month>April</month><year>2026</year></pub-date>
      
      <volume>18</volume>
      <issue>4</issue>
      <fpage>2799</fpage><lpage>2817</lpage>
      <history>
        <date date-type="received"><day>30</day><month>October</month><year>2025</year></date>
           <date date-type="rev-request"><day>24</day><month>November</month><year>2025</year></date>
           <date date-type="rev-recd"><day>27</day><month>February</month><year>2026</year></date>
           <date date-type="accepted"><day>24</day><month>March</month><year>2026</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2026 Henning Dorff et al.</copyright-statement>
        <copyright-year>2026</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://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026.html">This article is available from https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026.html</self-uri><self-uri xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026.pdf">The full text article is available as a PDF file from https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026.pdf</self-uri>
      <abstract><title>Abstract</title>

      <p id="d2e157">We present a comprehensive balloon-borne measurement dataset collected during a dedicated Arctic observation campaign conducted from 19 March to 18 April 2024 in the transition from polar night to polar day at the Villum Research Station (VRS) at Station Nord in Greenland. The objective of the observations was to characterise the temporal evolution of the Arctic atmospheric boundary layer (ABL), focusing on key transition periods, including cloud development, low-level jet evolution, and day to night shifts. Data were collected by the Balloon-bornE moduLar Utility for profilinG the lower Atmosphere (BELUGA) tethered-balloon system performing in-situ measurements of temperature, relative humidity, wind speed, turbulence, and thermal infrared irradiance from the surface to several hundred meters altitude, with frequent profiling in high vertical resolution.  Twenty-eight research flights delivered more than 300 profiles, with up to 8 profiles per hour, complemented by daily radiosonde launches. This paper specifies the BELUGA instrumentation at VRS, data processing procedures, and the publicly available Level-2 data (BELUGA and radiosonde), provided in instrument-separated data subsets listed in a data collection (<ext-link xlink:href="https://doi.org/10.1594/PANGAEA.986431" ext-link-type="DOI">10.1594/PANGAEA.986431</ext-link>, <xref ref-type="bibr" rid="bib1.bibx14" id="altparen.1"/>). One possible major application of the data is to evaluate different model types (such as numerical weather prediction, single-column, large-eddy simulations) in representing processes controlling the Arctic ABL. To prepare such evaluations, we give an overview of the observations, environmental conditions during the campaign, and highlight specific events that are valuable for model comparison. We introduce an event in which temporal temperature changes influence the ABL inversion, radiative heating-rate profiles associated with transitions between cloudy and cloud-free conditions, and an observed Arctic low-level jet compared with reanalysis, offering insights into the Arctic ABL evolution.</p>
  </abstract>
    
<funding-group>
<award-group id="gs1">
<funding-source>Deutsche Forschungsgemeinschaft</funding-source>
<award-id>268020496</award-id>
</award-group>
</funding-group>
</article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d2e175">The Arctic climate system has experienced substantial changes in the past decades, including a dramatic increase in near-surface air temperature <xref ref-type="bibr" rid="bib1.bibx44" id="paren.2"/>. This warming is four times higher compared to the global average and is widely known as Arctic amplification <xref ref-type="bibr" rid="bib1.bibx48" id="paren.3"/>. This phenomenon results from local and remote feedback mechanisms driven by global warming <xref ref-type="bibr" rid="bib1.bibx64" id="paren.4"/>. The lapse rate and surface albedo feedbacks are considered the main drivers <xref ref-type="bibr" rid="bib1.bibx8" id="paren.5"/>. However, models are not perfect in representing the complex physical processes that cause Arctic amplification. Steering processes such as turbulent and radiative fluxes and transitions between cloudy and cloud-free states are limitedly represented in climate simulations, numerical weather predictions and also reanalyses (<xref ref-type="bibr" rid="bib1.bibx61" id="altparen.6"/>; <xref ref-type="bibr" rid="bib1.bibx41" id="altparen.7"/>; <xref ref-type="bibr" rid="bib1.bibx30" id="altparen.8"/>; <xref ref-type="bibr" rid="bib1.bibx4" id="altparen.9"/>; <xref ref-type="bibr" rid="bib1.bibx9" id="altparen.10"/>).</p>
      <p id="d2e206">A major problem of atmospheric models stems from the evolution of the Arctic atmospheric boundary layer (ABL), which significantly determines the lapse rate feedback. The ABL forms the shallow interface between the surface and the free atmosphere (<xref ref-type="bibr" rid="bib1.bibx57" id="altparen.11"/>; <xref ref-type="bibr" rid="bib1.bibx55" id="altparen.12"/>; <xref ref-type="bibr" rid="bib1.bibx10" id="altparen.13"/>; <xref ref-type="bibr" rid="bib1.bibx54" id="altparen.14"/>; <xref ref-type="bibr" rid="bib1.bibx63" id="altparen.15"/>). The typical near-surface temperature inversion in the Arctic ABL promotes amplified near-surface warming and relatively muted heating in the free troposphere, causing the ABL to play a dominant role in the lapse rate feedback <xref ref-type="bibr" rid="bib1.bibx31" id="paren.16"/>. However, the Arctic ABL is governed by complex processes that include radiative cooling, surface interaction, and advection.</p>
      <p id="d2e228">Of particular relevance for these processes are clouds within the Arctic ABL (<xref ref-type="bibr" rid="bib1.bibx34" id="altparen.17"/>; <xref ref-type="bibr" rid="bib1.bibx49" id="altparen.18"/>; <xref ref-type="bibr" rid="bib1.bibx28" id="altparen.19"/>). <xref ref-type="bibr" rid="bib1.bibx50" id="text.20"/> highlighted the impact of Arctic low-level clouds on the turbulent boundary layer structure, and they contribute to the surface radiative energy budget (<xref ref-type="bibr" rid="bib1.bibx63" id="altparen.21"/>; <xref ref-type="bibr" rid="bib1.bibx2" id="altparen.22"/>). However, the magnitude of this contribution is only partially understood <xref ref-type="bibr" rid="bib1.bibx26" id="paren.23"/>. <xref ref-type="bibr" rid="bib1.bibx60" id="text.24"/> and <xref ref-type="bibr" rid="bib1.bibx33" id="text.25"/> demonstrated that the vertical structure of the irradiance and radiative cooling rate profiles depends on the atmospheric state, especially the presence or absence of clouds. In a cloudfree atmosphere, thermal near-infrared (TIR) irradiance emission from the surface immediately results in cooling that promotes the formation of a surface-based temperature inversion. Furthermore, the presence of low-level jets (LLJs), characterised by a local maximum in the wind speed profile below 1.5 km <xref ref-type="bibr" rid="bib1.bibx59" id="paren.26"/>, can modulate the Arctic ABL properties through mixing induced by enhanced wind shear and subsequent turbulence below the LLJ core <xref ref-type="bibr" rid="bib1.bibx22" id="paren.27"/> and interactions with low-level cloud conditions <xref ref-type="bibr" rid="bib1.bibx35" id="paren.28"/>. All of these processes can lead to rapid transitions between states of the Arctic ABL with respect to atmospheric stability, turbulence, and cloud properties <xref ref-type="bibr" rid="bib1.bibx5" id="paren.29"/>, and become predominant in the evolution of near-surface inversions.</p>
      <p id="d2e272">Understanding the temporal evolution of the transitions between different Arctic ABL states is crucial for grasping changes in the surface energy budget, cloud formation, and the evolution of Arctic weather patterns (<xref ref-type="bibr" rid="bib1.bibx58" id="altparen.30"/>; <xref ref-type="bibr" rid="bib1.bibx34" id="altparen.31"/>). Transitions can be driven locally or by advection from different regions or altitudes through air mass exchange, or along air mass trajectories <xref ref-type="bibr" rid="bib1.bibx42" id="paren.32"/>. Despite extensive discussions on atmospheric states (e.g., <xref ref-type="bibr" rid="bib1.bibx49" id="altparen.33"/>; <xref ref-type="bibr" rid="bib1.bibx34" id="altparen.34"/>; <xref ref-type="bibr" rid="bib1.bibx41" id="altparen.35"/>), processes governing transitions between them, and the adjustment of the ABL are not fully understood. Numerical weather predictions, reanalyses, and climate simulations continue to face challenges in accurately representing relevant ABL transition processes (<xref ref-type="bibr" rid="bib1.bibx61" id="altparen.36"/>; <xref ref-type="bibr" rid="bib1.bibx30" id="altparen.37"/>; <xref ref-type="bibr" rid="bib1.bibx4" id="altparen.38"/>). To resolve ABL characteristics and their evolution – regarding near-surface heat fluxes, lapse rate feedback, and cloud properties – <xref ref-type="bibr" rid="bib1.bibx3" id="text.39"/> emphasized the importance of in situ data for all components of the surface energy budget.</p>
      <p id="d2e307">Tethered balloon measurements are a suitable tool for quantifying the characteristics and evolution of the lower ABL and can bridge the gap between continuous observations from surface stations <xref ref-type="bibr" rid="bib1.bibx47" id="paren.40"><named-content content-type="pre">e.g.,</named-content></xref> and measurements by research aircraft, which often have limited vertical resolution (<xref ref-type="bibr" rid="bib1.bibx56" id="altparen.41"/>; <xref ref-type="bibr" rid="bib1.bibx7" id="altparen.42"/>). Over the past decade, balloon-borne systems have been successfully deployed in the Arctic <xref ref-type="bibr" rid="bib1.bibx52" id="paren.43"><named-content content-type="pre">e.g.,</named-content></xref>, capable of carrying payloads of up to several tens of kilograms to altitudes of 1 km, with endurances of up to several hours. From vertical profiles of measured irradiances, heating rates in the Arctic ABL can be derived (<xref ref-type="bibr" rid="bib1.bibx18" id="altparen.44"/>; <xref ref-type="bibr" rid="bib1.bibx1" id="altparen.45"/>; <xref ref-type="bibr" rid="bib1.bibx33" id="altparen.46"/>). <xref ref-type="bibr" rid="bib1.bibx6" id="text.47"/> proved the feasibility of estimating turbulence from balloon-borne 3D wind measurements.</p>
      <p id="d2e339">The Balloon-bornE moduLar Utility for profilinG the lower Atmosphere (BELUGA; <xref ref-type="bibr" rid="bib1.bibx20" id="altparen.48"/>) was designed to combine measurements of thermodynamic (<xref ref-type="bibr" rid="bib1.bibx21" id="altparen.49"/>; <xref ref-type="bibr" rid="bib1.bibx40" id="altparen.50"/>), radiative (<xref ref-type="bibr" rid="bib1.bibx32" id="altparen.51"/>; <xref ref-type="bibr" rid="bib1.bibx33" id="altparen.52"/>), turbulent (<xref ref-type="bibr" rid="bib1.bibx21" id="altparen.53"/>; <xref ref-type="bibr" rid="bib1.bibx22" id="altparen.54"/>), and  aerosol properties <xref ref-type="bibr" rid="bib1.bibx38" id="paren.55"/>. With slow ascent rates, BELUGA can measure sharp gradients in Arctic near-surface inversions, thereby advancing our understanding of radiative and turbulent processes that sustain and modulate the ABL inversion and cloud formation. Recent BELUGA deployments (e.g. <xref ref-type="bibr" rid="bib1.bibx40" id="altparen.56"/>; <xref ref-type="bibr" rid="bib1.bibx33" id="altparen.57"/>) have focused on characterising different atmospheric states of the Arctic ABL.</p>
      <p id="d2e373">To study specific transition phases between different ABL states, BELUGA was adapted to a lightweight and reduced payload, facilitating continuous profiling of the ABL. BELUGA was deployed at the Villum Research Station (VRS) in Station Nord (Northeastern Greenland), for a 1-month period (19 March to 18 April 2024) within the framework of the Transregional Collaborative Research Center’s <inline-formula><mml:math id="M1" display="inline"><mml:mi mathvariant="script">A</mml:mi></mml:math></inline-formula>rcti<inline-formula><mml:math id="M2" display="inline"><mml:mi mathvariant="script">C</mml:mi></mml:math></inline-formula> <inline-formula><mml:math id="M3" display="inline"><mml:mi mathvariant="script">A</mml:mi></mml:math></inline-formula>mplification: <inline-formula><mml:math id="M4" display="inline"><mml:mi mathvariant="script">C</mml:mi></mml:math></inline-formula>limate Relevant <inline-formula><mml:math id="M5" display="inline"><mml:mi mathvariant="script">A</mml:mi></mml:math></inline-formula>tmospheric and Surfa<inline-formula><mml:math id="M6" display="inline"><mml:mi mathvariant="script">C</mml:mi></mml:math></inline-formula>e Processes and Feedback Mechanisms <inline-formula><mml:math id="M7" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">A</mml:mi><mml:mi mathvariant="script">C</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx64" id="paren.58"/>. This deployment was in parallel to the Vertical properties of aerosols in the Arctic lower atmosphere and their impact on cloud-radiative effects (VAERTICAL)/CleanCloud campaigns <xref ref-type="bibr" rid="bib1.bibx65" id="paren.59"/>. During the comprehensive measurement period, BELUGA performed intensive profiling of the ABL and captured multiple transitions between different atmospheric states. These transition phases were sampled with high temporal resolution.</p>
      <p id="d2e442">This paper presents the dataset collected by BELUGA at VRS and demonstrates potential applications. Section 2 introduces the measurement campaign, the BELUGA instrument setup and summarises the conducted research flights. Section 3 describes the data processing procedures, specifies the BELUGA Level-2 datasets and supplementary data from daily radiosonde profiles, and provides information on their accessibility. Section 4 provides an overview of the environmental conditions during the campaign that characterise the measurement data at VRS. To illustrate the potential of the BELUGA measurement data, Sect. 5 highlights exemplary scientific applications for analysing Arctic ABL transition events.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Tethered-balloon measurements at Villum Research Station</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>Villum Research Station at Station Nord</title>
      <p id="d2e460">Measurements with the BELUGA system were conducted at the Villum Research Station (operated by Aarhus University, Denmark) at Station Nord  from 24 March to 12 April 2024. VRS is located on the northeastern coast of Greenland at 81°36<sup>′</sup>9<sup>′′</sup> N, 16°40<sup>′</sup> 12<sup>′′</sup> W, close to a sea-ice-covered fjord in the vicinity of the Flade Isblink glacier (Fig. <xref ref-type="fig" rid="F1"/>). VRS is one of the northernmost manned stations in the world. It is equipped with an automatic weather station, cloud radar, lidar, and ceilometer measurements <xref ref-type="bibr" rid="bib1.bibx27" id="paren.60"/>. Furthermore, the parallel CleanCloud CLAVIER campaign, conducted by the EPFL at Lausanne, provided complementary aerosol data from the lower ABL using a Helikite system <xref ref-type="bibr" rid="bib1.bibx43" id="paren.61"/>.</p>

      <fig id="F1" specific-use="star"><label>Figure 1</label><caption><p id="d2e516">Location of Villum Research Station (VRS) at Station Nord on the northeastern tip of Greenland (purple cross), with the CARRA reanalysis (western) domain indicated by the orange rectangle <bold>(a)</bold>. The mean sea ice concentration from ASMR-2 <xref ref-type="bibr" rid="bib1.bibx53" id="paren.62"/>, averaged over the BELUGA measurement period from 24 March to 12 April 2024, is also shown. Panel <bold>(b)</bold> provides a zoomed view of the coastal region around Station Nord. Dots illustrate the grid spacing of the commonly used reanalysis datasets ERA5 (black) and CARRA (orange), which can be evaluated by the BELUGA observations. The background map was created with Natural Earth. </p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f01.png"/>

        </fig>

      <p id="d2e534">The tethered balloon-borne measurements were operated next to the air laboratory Flyger's Hut, in a distance of roughly 2 km from the base of VRS. The surrounding of Flyger's hut is mostly flat and snow-covered, elevated glaciers are located further to the south (Fig. <xref ref-type="fig" rid="F1"/>b), and permanent inland ice is sufficiently distant (<inline-formula><mml:math id="M12" display="inline"><mml:mo lspace="0mm">&gt;</mml:mo></mml:math></inline-formula> 100 km southwest of VRS). However, the meteorological conditions at VRS are frequently influenced by katabatic flows induced by the complex orography in the hinterland of VRS (e.g. <xref ref-type="bibr" rid="bib1.bibx36" id="altparen.63"/>; <xref ref-type="bibr" rid="bib1.bibx29" id="altparen.64"/>).  The location of VRS is within the grid domain of the Copernicus Arctic Regional Reanalysis (CARRA), which provides a high horizontal resolution of 2.5 km for characterising local Arctic effects. CARRA adequately incorporates complex orography and sea ice conditions in the vicinity of VRS (Fig. <xref ref-type="fig" rid="F1"/>b).</p>
</sec>
<sec id="Ch1.S2.SS2">
  <label>2.2</label><title>BELUGA setup: balloon and instrument payload</title>
      <p id="d2e562">The BELUGA system consists of a helium-filled tethered balloon that carries a set of dedicated in-situ measurement devices. Different balloons and sensors have been used in the past. For the VRS measurement campaign (19 March to 18 April 2024), a 9 m<sup>3</sup> balloon was used (Fig. <xref ref-type="fig" rid="F2"/>a). The BELUGA instrument payload was configured to measure thermodynamic conditions, terrestrial broadband irradiance, and three-dimensional (3D) wind vectors, and was equipped with two instrument probes (summarised in Table <xref ref-type="table" rid="T1"/>) that rely on three of the previous probes described by <xref ref-type="bibr" rid="bib1.bibx40" id="text.65"/>. The two main probes are: (i) the turbulence meteorological probe (TMP), which contains a hot-wire anemometer for turbulence measurements at different scales, and a modified radiosonde complemented by an ultrasonic anemometer to measure standard meteorological quantities (temperature, relative humidity, pressure) as well as the 3D wind vector (Fig. <xref ref-type="fig" rid="F2"/>b), and (ii) the broadband radiation probe (BP, Fig. <xref ref-type="fig" rid="F2"/>c), which measures the broadband thermal infrared up- and downward irradiances. Since these probes are similar to the instrumentation detailed in <xref ref-type="bibr" rid="bib1.bibx20" id="text.66"/>, <xref ref-type="bibr" rid="bib1.bibx32" id="text.67"/>, and <xref ref-type="bibr" rid="bib1.bibx40" id="text.68"/>, here we only summarize their characteristics during the VRS campaign.</p>

      <fig id="F2" specific-use="star"><label>Figure 2</label><caption><p id="d2e597">Tethered balloon at VRS and instrumentation. <bold>(a)</bold> Photo of the tethered balloon system (BELUGA) at Station Nord, here fixed before launch. <bold>(b)</bold>  The turbulent meteorological probe, consisting of a modified radiosonde (<inline-formula><mml:math id="M14" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and a hot-wire anemometer used for turbulence measurements (<inline-formula><mml:math id="M15" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), <bold>(c)</bold> The broadband radiometer package, which includes nadir- and zenith-pointing pyrgeometers.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f02.jpg"/>

        </fig>

<table-wrap id="T1" specific-use="star"><label>Table 1</label><caption><p id="d2e640">Instrument specifications of the probes deployed at BELUGA during the campaign at Station Nord.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="4">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="left"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="left"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">Probe</oasis:entry>
         <oasis:entry colname="col2">Instrument</oasis:entry>
         <oasis:entry colname="col3">Measured Quantities</oasis:entry>
         <oasis:entry colname="col4">Uncertainty</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Radiosonde</oasis:entry>
         <oasis:entry colname="col3">Air temperature (<inline-formula><mml:math id="M16" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>), relative humidity (RH)</oasis:entry>
         <oasis:entry colname="col4">0.2 K, 3 %–5 %</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">TMP</oasis:entry>
         <oasis:entry colname="col2">Mini-ultrasonic anemomenter</oasis:entry>
         <oasis:entry colname="col3">3D wind vector</oasis:entry>
         <oasis:entry colname="col4">7.5 <inline-formula><mml:math id="M17" display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</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>, 1.5 °</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">Hot-wire anemometer</oasis:entry>
         <oasis:entry colname="col3">Wind speed at 250 Hz</oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M18" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 1 <inline-formula><mml:math id="M19" display="inline"><mml:mrow><mml:mi mathvariant="normal">cm</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">BP</oasis:entry>
         <oasis:entry colname="col2">2<inline-formula><mml:math id="M20" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> Pyrgeometers</oasis:entry>
         <oasis:entry colname="col3">Upward, downward thermal infrared irradiance (TIR)</oasis:entry>
         <oasis:entry colname="col4">5<inline-formula><mml:math id="M21" display="inline"><mml:mrow><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">BME280 sensor</oasis:entry>
         <oasis:entry colname="col3">Air temperature, relative humidity</oasis:entry>
         <oasis:entry colname="col4">0.3 K, 2 %</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d2e821">The meteorological parameters recorded by the TMP, hereafter referred to as <inline-formula><mml:math id="M22" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, are obtained using a modified (lightweight) radiosonde, with the accuracies specified in Table <xref ref-type="table" rid="T1"/>. A miniature ultrasonic anemometer (sonic) provides the three wind vector components (<inline-formula><mml:math id="M23" display="inline"><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi><mml:mo>,</mml:mo><mml:mi>w</mml:mi></mml:mrow></mml:math></inline-formula>), the virtual temperature derived from sound speed, as well as static pressure and relative humidity – though this humidity data proved unreliable and are not used. Note that the uncertainties listed for the minisonic in Table <xref ref-type="table" rid="T1"/> are manufacturer specifications, not including the probe attitude correction; these could be verified for a horizontally aligned sonic in a wind tunnel. A small navigation module supplies the three attitude angles (roll, pitch, and yaw). All the selected parameters are transmitted to the ground with 1 Hz. In the turbulence measurement component, which we define as the <inline-formula><mml:math id="M24" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, a single-component hot-wire anemometer measures high-resolution wind speed, sampled natively at 250 Hz.</p>
      <p id="d2e866">The broadband radiation probe (BP) measures downward and upward thermal infrared (TIR) radiative flux densities (irradiances, <inline-formula><mml:math id="M25" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M26" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) using two identical pyrgeometers oriented in the nadir and zenith direction (Fig. <xref ref-type="fig" rid="F2"/>). Each pyrgeometer is sensitive to the broadband TIR irradiance in a wavelength range of 4.5–42 <inline-formula><mml:math id="M27" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> (<xref ref-type="bibr" rid="bib1.bibx20" id="altparen.69"/>; <xref ref-type="bibr" rid="bib1.bibx40" id="altparen.70"/>). In addition to radiation measurements, the BP is equipped with a BME sensor to monitor standard meteorological parameters, including air pressure, temperature, and relative humidity.</p>
      <p id="d2e910">This BELUGA payload is designed to minimize instrument weight while ensuring stable horizontal sensor alignment during operation. The system was also equipped with GPS and attitude sensors to account for any horizontal misalignment of the probes. Furthermore, a similar ground-based radiation probe, additionally equipped with an upward-pointing pyranometer, was operated simultaneously to measure downward solar radiative flux densities in conjunction with the BELUGA observations.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Flight strategy and research flights</title>
      <p id="d2e921">The strategy of the measurement flights at VRS aimed to characterise the vertical structure of the ABL, including near-surface inversions where low-level clouds can occur, with a temporal resolution sufficient to capture the evolution of the atmospheric parameters during transition events. The lightweight payload of BELUGA allows such high-resolution profiling of the ABL. Consequently, most flights involved continuous ascent and descent profiling, as illustrated in  Fig. <xref ref-type="fig" rid="F3"/>. The maximum altitude of the profiles was adjusted to the actual conditions. To gain an overview of the ABL, higher profiles up to at least 500 m height were implemented at the beginning of the flights.</p>

      <fig id="F3"><label>Figure 3</label><caption><p id="d2e928">Schematic sketch of the typical flight strategy with instrument probes along the rope recording data in several profiles throughout the ABL. Shadings qualitatively show the temperature structure within the ABL, with increased values (orange) around a near-surface inversion above which clouds commonly formed during the campaign.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f03.png"/>

        </fig>

      <p id="d2e937">In total, BELUGA conducted 28 research flights (RFs) during the VRS campaign in spring 2024. All flights are listed in Table <xref ref-type="table" rid="T2"/>, which includes their respective duration, instrument status, number and maximum altitude of profiles, and atmospheric transitions observed during flight. The 28 RFs of BELUGA accumulated measurement data over about 76 flight hours, with individual flights lasting between 1 and 6 h. In general, the instruments performed reliable and continuous measurements, except for the turbulence probe (<inline-formula><mml:math id="M28" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>), which experienced data acquisition problems during the first half of the campaign. The aforementioned flight strategy resulted in a large number of 336 profiles (ascent or descent) with a depth of more than 200 m. Most flights included more than ten profiles, with a maximum of 34 profiles during RF26. Profiling of the ABL was performed quasi-continuously, with ascent and descent cycles at intervals of <inline-formula><mml:math id="M29" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> min, to optimally capture both large-scale ABL structures and small-scale temporal fluctuations. The vertical movement of the balloon along the profiles corresponds to a mean vertical resolution of about 0.8 m, based on the averaged 1 Hz data.</p>

<table-wrap id="T2" specific-use="star"><label>Table 2</label><caption><p id="d2e967">BELUGA research flights (RFs) with specified start and end times, data quality, and profile information (number of profiles <inline-formula><mml:math id="M30" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 200 m,  maximum peak height). The RFs are categorised with respect to ABL transition types that we specify in Sect. <xref ref-type="sec" rid="Ch1.S5"/>.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="10">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="center"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:colspec colnum="6" colname="col6" align="left"/>
     <oasis:colspec colnum="7" colname="col7" align="left"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="left"/>
     <oasis:colspec colnum="10" colname="col10" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">RF</oasis:entry>
         <oasis:entry colname="col2">Date</oasis:entry>
         <oasis:entry colname="col3">Start</oasis:entry>
         <oasis:entry colname="col4">End</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M31" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M32" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col7">BP</oasis:entry>
         <oasis:entry colname="col8">No. of</oasis:entry>
         <oasis:entry colname="col9">Max</oasis:entry>
         <oasis:entry colname="col10">Transition</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">(yyyy/mm/dd)</oasis:entry>
         <oasis:entry colname="col3">time</oasis:entry>
         <oasis:entry colname="col4">time</oasis:entry>
         <oasis:entry colname="col5">data</oasis:entry>
         <oasis:entry colname="col6">data</oasis:entry>
         <oasis:entry colname="col7">data</oasis:entry>
         <oasis:entry colname="col8">profiles</oasis:entry>
         <oasis:entry colname="col9">height</oasis:entry>
         <oasis:entry colname="col10">types</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">RF01</oasis:entry>
         <oasis:entry colname="col2">2024/03/24</oasis:entry>
         <oasis:entry colname="col3">12:32:56</oasis:entry>
         <oasis:entry colname="col4">14:38:13</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">8</oasis:entry>
         <oasis:entry colname="col9">378 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF02</oasis:entry>
         <oasis:entry colname="col2">2024/03/24</oasis:entry>
         <oasis:entry colname="col3">15:33:41</oasis:entry>
         <oasis:entry colname="col4">16:41:32</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">4</oasis:entry>
         <oasis:entry colname="col9">450 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF03</oasis:entry>
         <oasis:entry colname="col2">2024/03/25</oasis:entry>
         <oasis:entry colname="col3">10:09:08</oasis:entry>
         <oasis:entry colname="col4">13:56:33</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">18</oasis:entry>
         <oasis:entry colname="col9">487 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF04</oasis:entry>
         <oasis:entry colname="col2">2024/03/25</oasis:entry>
         <oasis:entry colname="col3">15:05:26</oasis:entry>
         <oasis:entry colname="col4">16:25:43</oasis:entry>
         <oasis:entry colname="col5">unavailable</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
         <oasis:entry colname="col9">406 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF05</oasis:entry>
         <oasis:entry colname="col2">2024/03/26</oasis:entry>
         <oasis:entry colname="col3">16:07:39</oasis:entry>
         <oasis:entry colname="col4">18:25:35</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">482 m</oasis:entry>
         <oasis:entry colname="col10">night <inline-formula><mml:math id="M33" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> day</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF06</oasis:entry>
         <oasis:entry colname="col2">2024/03/26</oasis:entry>
         <oasis:entry colname="col3">19:09:02</oasis:entry>
         <oasis:entry colname="col4">21:57:37</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">465 m</oasis:entry>
         <oasis:entry colname="col10">night <inline-formula><mml:math id="M34" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> day</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF07</oasis:entry>
         <oasis:entry colname="col2">2024/03/27</oasis:entry>
         <oasis:entry colname="col3">16:11:40</oasis:entry>
         <oasis:entry colname="col4">17:42:30</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
         <oasis:entry colname="col9">480 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M35" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF08</oasis:entry>
         <oasis:entry colname="col2">2024/03/28</oasis:entry>
         <oasis:entry colname="col3">09:56:12</oasis:entry>
         <oasis:entry colname="col4">12:48:06</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">494 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M36" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF09</oasis:entry>
         <oasis:entry colname="col2">2024/03/28</oasis:entry>
         <oasis:entry colname="col3">13:41:48</oasis:entry>
         <oasis:entry colname="col4">17:02:12</oasis:entry>
         <oasis:entry colname="col5">unavailable</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">unavailable</oasis:entry>
         <oasis:entry colname="col8">–</oasis:entry>
         <oasis:entry colname="col9">–</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF10</oasis:entry>
         <oasis:entry colname="col2">2024/03/29</oasis:entry>
         <oasis:entry colname="col3">14:41:38</oasis:entry>
         <oasis:entry colname="col4">16:05:56</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">4</oasis:entry>
         <oasis:entry colname="col9">474 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M37" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF11</oasis:entry>
         <oasis:entry colname="col2">2024/03/30</oasis:entry>
         <oasis:entry colname="col3">10:45:28</oasis:entry>
         <oasis:entry colname="col4">14:09:54</oasis:entry>
         <oasis:entry colname="col5">unavailable</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">10</oasis:entry>
         <oasis:entry colname="col9">489 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M38" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF12</oasis:entry>
         <oasis:entry colname="col2">2024/04/01</oasis:entry>
         <oasis:entry colname="col3">09:35:37</oasis:entry>
         <oasis:entry colname="col4">11:49:08</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">688 m</oasis:entry>
         <oasis:entry colname="col10">LLJ</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF13</oasis:entry>
         <oasis:entry colname="col2">2024/04/01</oasis:entry>
         <oasis:entry colname="col3">12:13:25</oasis:entry>
         <oasis:entry colname="col4">14:48:22</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">549 m</oasis:entry>
         <oasis:entry colname="col10">LLJ</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF14</oasis:entry>
         <oasis:entry colname="col2">2024/04/01</oasis:entry>
         <oasis:entry colname="col3">15:17:39</oasis:entry>
         <oasis:entry colname="col4">16:59:37</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
         <oasis:entry colname="col9">502 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF15</oasis:entry>
         <oasis:entry colname="col2">2024/04/02</oasis:entry>
         <oasis:entry colname="col3">09:31:52</oasis:entry>
         <oasis:entry colname="col4">12:35:30</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">20</oasis:entry>
         <oasis:entry colname="col9">475 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M39" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF16</oasis:entry>
         <oasis:entry colname="col2">2024/04-02</oasis:entry>
         <oasis:entry colname="col3">13:08:47</oasis:entry>
         <oasis:entry colname="col4">14:27:02</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">6</oasis:entry>
         <oasis:entry colname="col9">543 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M40" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF17</oasis:entry>
         <oasis:entry colname="col2">2024/04/03</oasis:entry>
         <oasis:entry colname="col3">13:31:30</oasis:entry>
         <oasis:entry colname="col4">16:17:28</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">10</oasis:entry>
         <oasis:entry colname="col9">616 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF18</oasis:entry>
         <oasis:entry colname="col2">2024/04/04</oasis:entry>
         <oasis:entry colname="col3">10:47:22</oasis:entry>
         <oasis:entry colname="col4">13:47:51</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">20</oasis:entry>
         <oasis:entry colname="col9">507 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF19</oasis:entry>
         <oasis:entry colname="col2">2024/04/04</oasis:entry>
         <oasis:entry colname="col3">14:25:02</oasis:entry>
         <oasis:entry colname="col4">17:07:03</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">20</oasis:entry>
         <oasis:entry colname="col9">549 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M41" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF20</oasis:entry>
         <oasis:entry colname="col2">2024/04/05</oasis:entry>
         <oasis:entry colname="col3">09:36:28</oasis:entry>
         <oasis:entry colname="col4">14:59:31</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">unavailable</oasis:entry>
         <oasis:entry colname="col8">24</oasis:entry>
         <oasis:entry colname="col9">599 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF21</oasis:entry>
         <oasis:entry colname="col2">2024/04/06</oasis:entry>
         <oasis:entry colname="col3">14:44:10</oasis:entry>
         <oasis:entry colname="col4">17:12:06</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">16</oasis:entry>
         <oasis:entry colname="col9">572 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF22</oasis:entry>
         <oasis:entry colname="col2">2024/04/07</oasis:entry>
         <oasis:entry colname="col3">12:40:48</oasis:entry>
         <oasis:entry colname="col4">15:52:54</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">18</oasis:entry>
         <oasis:entry colname="col9">717 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF23</oasis:entry>
         <oasis:entry colname="col2">2024/04/08</oasis:entry>
         <oasis:entry colname="col3">09:33:23</oasis:entry>
         <oasis:entry colname="col4">12:48:46</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">14</oasis:entry>
         <oasis:entry colname="col9">734 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M42" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF24</oasis:entry>
         <oasis:entry colname="col2">2024/04/08</oasis:entry>
         <oasis:entry colname="col3">13:53:34</oasis:entry>
         <oasis:entry colname="col4">16:26:09</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">12</oasis:entry>
         <oasis:entry colname="col9">769 m</oasis:entry>
         <oasis:entry colname="col10">cloudfree <inline-formula><mml:math id="M43" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF25</oasis:entry>
         <oasis:entry colname="col2">2024/04/09</oasis:entry>
         <oasis:entry colname="col3">09:12:10</oasis:entry>
         <oasis:entry colname="col4">13:36:16</oasis:entry>
         <oasis:entry colname="col5">missing parts</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">25</oasis:entry>
         <oasis:entry colname="col9">855 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF26</oasis:entry>
         <oasis:entry colname="col2">2024/04/10</oasis:entry>
         <oasis:entry colname="col3">09:56:37</oasis:entry>
         <oasis:entry colname="col4">15:41:44</oasis:entry>
         <oasis:entry colname="col5">good</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">34</oasis:entry>
         <oasis:entry colname="col9">829 m</oasis:entry>
         <oasis:entry colname="col10">LLJ</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF27</oasis:entry>
         <oasis:entry colname="col2">2024/04/11</oasis:entry>
         <oasis:entry colname="col3">09:38:26</oasis:entry>
         <oasis:entry colname="col4">14:08:32</oasis:entry>
         <oasis:entry colname="col5">gaps</oasis:entry>
         <oasis:entry colname="col6">good</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">24</oasis:entry>
         <oasis:entry colname="col9">897 m</oasis:entry>
         <oasis:entry colname="col10">LLJ</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">RF28</oasis:entry>
         <oasis:entry colname="col2">2024/04/12</oasis:entry>
         <oasis:entry colname="col3">13:58:35</oasis:entry>
         <oasis:entry colname="col4">16:29:16</oasis:entry>
         <oasis:entry colname="col5">unavailable</oasis:entry>
         <oasis:entry colname="col6">unavailable</oasis:entry>
         <oasis:entry colname="col7">good</oasis:entry>
         <oasis:entry colname="col8">16</oasis:entry>
         <oasis:entry colname="col9">819 m</oasis:entry>
         <oasis:entry colname="col10">–</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

      <p id="d2e2130">The maximum altitude attainable for BELUGA is determined by wind conditions, as stronger winds increase horizontal drift, requiring a longer tether that adds weight and consequently reduces the achievable height. For the VRS campaign, Fig. <xref ref-type="fig" rid="F4"/> shows the maximum heights of all profiles exceeding 200 m for each RF. Most profiles exceeded 400 m, with the highest flight altitude reaching nearly 900 m during RF27. Beyond wind requirements, the flight strategy was slightly adapted throughout the campaign. During the first 15 RFs, the maximum profile heights reached by the balloon were mostly slightly below 500 m and occurred at similar altitudes. In subsequent RFs, maximum profile heights varied more, both between and within individual RFs, and frequently exceeded 500 m. The change was motivated by higher variability of near-surface temperature inversions in the second half, which also resulted in a higher number of profiles.</p>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Level-2 data</title>
      <p id="d2e2144">For the measurements of the devices described in Sect. <xref ref-type="sec" rid="Ch1.S2.SS2"/>, we published the post-processed Level-2 (L2) data  at the World Data Center PANGAEA <xref ref-type="bibr" rid="bib1.bibx24" id="paren.71"/>, under an open access licence (CC-BY 4.0). The L2 measurements are compiled in a data collection titled <italic>Balloon-borne profile L2-data characterising the Arctic boundary layer and troposphere at Villum Research Station</italic> <xref ref-type="bibr" rid="bib1.bibx14" id="paren.72"/>, accessible via the link <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.986431" ext-link-type="DOI">10.1594/PANGAEA.986431</ext-link>. Table <xref ref-type="table" rid="T3"/> summarises the access to the individual instrument probe and radiosonde datasets. For each probe and research flight, single Network Common Data Format (netCDF) files (version netCDF-4) are provided, referencing the UTC time (from probe-included GPS modules). The file naming convention includes the measurement platform (BELUGA or Radiosonde), the instrument probe type (<inline-formula><mml:math id="M44" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M45" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, BP), the RF label (RFxy) and the date. Following the Climate and Forecast (CF) Metadata Conventions version 1.12 <xref ref-type="bibr" rid="bib1.bibx19" id="paren.73"/>, global attributes provide general data information, while variable attributes specify units and long names for each variable. Here, we describe the common altitude reference, the segmentation of flight sections, data quality control procedures, and give an overview of the post-calibrated L2 observations.</p>

      <fig id="F4"><label>Figure 4</label><caption><p id="d2e2191">Maximum heights of profiles for each research flight (RF) of the tethered-balloon. Markers are colour-coded with respect to the ABL transition types during which the flight were performed.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f04.png"/>

      </fig>

<table-wrap id="T3" specific-use="star"><label>Table 3</label><caption><p id="d2e2203">Specifications of published L2 BELUGA data sets from Station Nord.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="3">
     <oasis:colspec colnum="1" colname="col1" align="justify" colwidth="2cm"/>
     <oasis:colspec colnum="2" colname="col2" align="justify" colwidth="7cm"/>
     <oasis:colspec colnum="3" colname="col3" align="justify" colwidth="6cm"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left">Probe</oasis:entry>
         <oasis:entry colname="col2" align="left">Provided quantities</oasis:entry>
         <oasis:entry colname="col3" align="left">Reference</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left"><inline-formula><mml:math id="M46" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2" align="left">barometric pressure, air temperature, relative humidity, hor. wind speed and direction, lateral and longitudinal wind vector components, barometric altitude</oasis:entry>
         <oasis:entry colname="col3" align="left"><xref ref-type="bibr" rid="bib1.bibx17" id="text.74"/>: <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987003" ext-link-type="DOI">10.1594/PANGAEA.987003</ext-link></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left"><inline-formula><mml:math id="M47" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2" align="left">static pressure, temperature, raw hot-wire signal, air density, calibrated wind speed and barometric altitude</oasis:entry>
         <oasis:entry colname="col3" align="left"><xref ref-type="bibr" rid="bib1.bibx16" id="text.75"/>: <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987008" ext-link-type="DOI">10.1594/PANGAEA.987008</ext-link></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1" align="left">BP</oasis:entry>
         <oasis:entry colname="col2" align="left">downward and upward terrestrial irradiances (<inline-formula><mml:math id="M48" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M49" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), net terrestrial irradiance <inline-formula><mml:math id="M50" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, air pressure, temperature and relative humidity, and barometric altitude</oasis:entry>
         <oasis:entry colname="col3" align="left"><xref ref-type="bibr" rid="bib1.bibx13" id="text.76"/>: <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987001" ext-link-type="DOI">10.1594/PANGAEA.987001</ext-link></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1" align="left">Radiosonde</oasis:entry>
         <oasis:entry colname="col2" align="left">air pressure, air temperature, capacitor temperature,  relative humidity, speed of the sonde, <inline-formula><mml:math id="M51" display="inline"><mml:mi>u</mml:mi></mml:math></inline-formula>- and <inline-formula><mml:math id="M52" display="inline"><mml:mi>v</mml:mi></mml:math></inline-formula> wind, distance, altitude</oasis:entry>
         <oasis:entry colname="col3" align="left"><xref ref-type="bibr" rid="bib1.bibx12" id="text.77"/>: <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987053" ext-link-type="DOI">10.1594/PANGAEA.987053</ext-link></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Common altitude reference</title>
      <p id="d2e2372">The L2-data for each BELUGA probe component are referenced to the barometric altitude in metres, as all probes are equipped with appropriate sensors measuring static barometric pressure <inline-formula><mml:math id="M53" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. Barometric values used as altitude reference are more reliable in the high Arctic than GPS-based values. From <inline-formula><mml:math id="M54" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, we calculate the barometric altitude <inline-formula><mml:math id="M55" display="inline"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in metres as follows:

            <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M56" display="block"><mml:mrow><mml:msub><mml:mi>z</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>⋅</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:msup><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mi mathvariant="normal">b</mml:mi></mml:msub></mml:mrow><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle scriptlevel="+1"><mml:mfrac><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow><mml:mi>g</mml:mi></mml:mfrac></mml:mstyle></mml:msup></mml:mrow></mml:mfenced></mml:mrow></mml:math></disp-formula>

          using the standard adiabatic lapse rate <inline-formula><mml:math id="M57" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 6.5 <inline-formula><mml:math id="M58" display="inline"><mml:mrow><mml:mi mathvariant="normal">K</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">km</mml:mi><mml:mrow><mml:mi mathvariant="normal">−</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> and the specific gas constant for dry air <inline-formula><mml:math id="M59" display="inline"><mml:mrow><mml:msub><mml:mi>R</mml:mi><mml:mi mathvariant="normal">L</mml:mi></mml:msub><mml:mo>=</mml:mo></mml:mrow></mml:math></inline-formula> 287 <inline-formula><mml:math id="M60" display="inline"><mml:mrow><mml:mi mathvariant="normal">J</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">kg</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">K</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx62" id="paren.78"/>. The calculation method of Eq. (1), which uses a standard temperature gradient to determine barometric altitude, is commonly applied in aviation and has been shown to  correspond well with GPS-derived altitude in recent BELUGA datasets (e.g., <xref ref-type="bibr" rid="bib1.bibx39" id="altparen.79"/>). To ensure consistency across all BELUGA datasets, this method was also applied in the dataset reported here. For users aiming at higher precision of the altitude, reprocessing is recommended using the actual gradients of the locally measured temperature.</p>
      <p id="d2e2545">To correct for synoptic pressure tendencies and to ensure comparability in barometric altitude estimates, surface pressure <inline-formula><mml:math id="M61" display="inline"><mml:mrow><mml:msub><mml:mi>p</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and temperature <inline-formula><mml:math id="M62" display="inline"><mml:mrow><mml:msub><mml:mi>T</mml:mi><mml:mn mathvariant="normal">0</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, along with their tendencies during each flight were obtained from a ground-based pyrgeometer equipped with a BME-sensor. These measurements were time-synchronised with the balloon data.</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Flight segmentation</title>
      <p id="d2e2578">The BELUGA datasets listed in Table <xref ref-type="table" rid="T3"/> are provided with flight segmentation. The segmentation is stored as a one-dimensional, time-dependent flag that specifies distinct periods of flight segments. Data from specific segments can be easily accessed via the data variable <italic>flight_segments</italic>. For RF01, Fig. <xref ref-type="fig" rid="F5"/> illustrates the categories of flight segments identified by our segmentation. BELUGA ascents and descents are defined as periods with absolute vertical movement rates exceeding 0.3 <inline-formula><mml:math id="M63" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</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> (averaged over 30 s). Ascents and descents that are continuous over more than 100 m are flagged as profiles and marked with individual integer IDs with <inline-formula><mml:math id="M64" display="inline"><mml:mrow><mml:mn mathvariant="normal">100</mml:mn><mml:mo>+</mml:mo></mml:mrow></mml:math></inline-formula> number of ascent and <inline-formula><mml:math id="M65" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>100 – number of decent (not specified in Fig. <xref ref-type="fig" rid="F5"/>). More than 80  % of the flight duration for all RFs is assigned to profiles due to the observational focus on vertical conditions in the Arctic ABL. Additionally, the data include periods where BELUGA maintained a relatively constant altitude for several minutes (Fig. <xref ref-type="fig" rid="F5"/>; green). These periods are identified by mean vertical movement rates below 0.3 <inline-formula><mml:math id="M66" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</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> when averaged over 30 s. Such height-constant segments provide a statistical basis for turbulent flux estimates and help characterise the temporal evolution of radiative cloud properties at a given altitude.  Measurement periods near the surface, such as at the beginning of RF01 (Fig. <xref ref-type="fig" rid="F5"/>), result from the installation of the probes along the balloon tether, or, in other cases, aim to compare the balloon-borne instruments with ground-based near-surface measurements from VRS.</p>

      <fig id="F5"><label>Figure 5</label><caption><p id="d2e2648">Flight altitude over time during flight (RF01) with all flagged flight segments. Vertical profiling is distinguished by ascent and descent. Peaks are flagged for 15 s before and after maximum profile heights (red dots, with the highest profile depicted as darked dot).</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f05.png"/>

        </fig>


</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>Quality control</title>
      <p id="d2e2667">The L2-data have been quality-checked and appropriately flagged. Outliers were removed and spike filtering was performed for each quantity. For meteorological quantities, physically implausible values were identified. Specifically, temperature values above <inline-formula><mml:math id="M67" display="inline"><mml:mn mathvariant="normal">0</mml:mn></mml:math></inline-formula> °C were set to NaN. During the campaign, wind speeds were generally low, so values above 20 <inline-formula><mml:math id="M68" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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> were considered unrealistic and thus excluded. Values of RH were capped at 120 %. In the data quality flag, these cases were labeled as <italic>missing</italic> and <italic>bad</italic> accordingly. Sensor tilt of the BP can significantly affect the accuracy of irradiance values; data for sensor pitch angles <inline-formula><mml:math id="M69" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">15</mml:mn><mml:mi mathvariant="italic">°</mml:mi></mml:mrow></mml:math></inline-formula> were treated as <italic>bad</italic>, with uncertainties in the irradiance values greater than 5 %. This amounts to less than 5 % of the total data and is often for measurements only shortly after launch. For users interested in considering these strongly titled data, correction routines as described by <xref ref-type="bibr" rid="bib1.bibx37" id="text.80"/> are suggested. Data gaps up to 10 s were interpolated and flagged accordingly. For available data, the quality flag assigns <italic>good</italic> quality for almost 95 % of all flight periods.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Level-2 data overview</title>
<sec id="Ch1.S3.SS4.SSS1">
  <label>3.4.1</label><title>Meteorological data from the TMP</title>
      <p id="d2e2737">The meteorological L2-data for the <inline-formula><mml:math id="M70" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (<xref ref-type="bibr" rid="bib1.bibx17" id="altparen.81"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987003" ext-link-type="DOI">10.1594/PANGAEA.987003</ext-link>) are provided at 1 Hz resolution and contain the following quantities: barometric pressure, air temperature (radiosonde and sonic), relative humidity, horizontal wind speed, wind direction, longitudinal and lateral wind vector components and barometric altitude (Table <xref ref-type="table" rid="T3"/>). The three attitude angles (roll, pitch, and yaw) from the navigation module were used to transform the 3D wind vector into a ground-fixed coordinate system. However, the design of the sonic system does not allow for a precise determination of the vertical wind component. Furthermore, changes of the tether inclination and a related drift of the instrument probes can affect the measured wind speeds. Past BELUGA campaigns have shown that the drift speeds of the probes are up to about one order of magnitude smaller than wind speeds. Therefore, these effects have been neglected in the data processing.</p>
      <p id="d2e2759">Figure <xref ref-type="fig" rid="F6"/> summarises the distribution of meteorological values from the <inline-formula><mml:math id="M71" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> data as a function of height, which were observed throughout the measurement period. The distributions correspond to a total measurement duration of more than 10 h for profile data at the lowest levels, decreasing with height due to varying profile heights; however, data still accumulate to about 1 h above 500 m (Fig. <xref ref-type="fig" rid="F6"/>a). Temperature values are predominantly below <inline-formula><mml:math id="M72" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>10 °C throughout the ABL (Fig. <xref ref-type="fig" rid="F6"/>b) with two notable nodes at inversion heights below 200 m. Overall, quite dry conditions were observed, with RH mainly ranging between 40 % and 60 % in the lowest hundred metres. As altitude increases, the spread of the RH distributions widens (Fig. <xref ref-type="fig" rid="F6"/>c), indicating a higher variability of moisture conditions with height and the sporadic presence of clouds. The wind was generally calm (below 8 <inline-formula><mml:math id="M73" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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> at all heights, and particularly below 4 <inline-formula><mml:math id="M74" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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> close to the surface). Between 50 to 200 m, there is an increasing frequency of wind speeds exceeding 4 <inline-formula><mml:math id="M75" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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>, associated with the occurrence of low-level jets (LLJs).</p>

      <fig id="F6" specific-use="star"><label>Figure 6</label><caption><p id="d2e2842">Summary of meteorological data from the <inline-formula><mml:math id="M76" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> package recorded during the measurement period. <bold>(a)</bold> shows the distribution of the measurement heights and respective flight duration in each height bin. For these data, <bold>(b)</bold> illustrates the statistics of measured temperature values as a function of height. <bold>(c)</bold> and <bold>(d)</bold> analogously depict the values of relative humidity and wind speed, respectively.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f06.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS4.SSS2">
  <label>3.4.2</label><title>Turbulence data from the TMP</title>
      <p id="d2e2882">The L2-data of the turbulence component (<inline-formula><mml:math id="M77" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; <xref ref-type="bibr" rid="bib1.bibx16" id="altparen.82"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987008" ext-link-type="DOI">10.1594/PANGAEA.987008</ext-link>) are provided at a temporal resolution of 50 Hz and include the following quantities: static pressure, temperature, raw hot-wire signal, air density, barometric height and calibrated wind velocity with 50 Hz resolution (Table <xref ref-type="table" rid="T3"/>). The raw data sampled at 250 Hz was averaged over 5 data points to reduce noise levels. The hot-wire anemometer wind speed was calibrated individually for each flight using the horizontal wind measurements from the sonic anemometer. For calibration, we applied a least-squares method similar to that described in <xref ref-type="bibr" rid="bib1.bibx25" id="text.83"/>, which accounts for dependencies on air temperature and density. Static pressure, air temperature and density values are included in the <inline-formula><mml:math id="M78" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> data. For consistency, these were upsampled from initially 1 to 50 Hz.</p>
      <p id="d2e2919">The calibrated wind speed values enable the resolution of turbulence at small scales through the calculation of power spectra of wind velocities. Figure <xref ref-type="fig" rid="F7"/> shows the power spectral density of the high-resolution wind speed derived from an exemplary 20 min measurement period conducted at a constant height of 10 m. The raw spectrum was additionally averaged over logarithmically equidistant bins, and referenced to a model spectrum for an inertial range with a slope of <inline-formula><mml:math id="M79" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula>. Up to frequencies slightly above 10 Hz, the averaged spectrum in Fig. <xref ref-type="fig" rid="F7"/> has not yet transitioned to white noise (a flat spectrum), implying that spatial structures of about 2 cm can still be well resolved. Since the spectrum is normalised such that its integral yields the variance, the sensor resolution can be estimated as <inline-formula><mml:math id="M80" display="inline"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>U</mml:mi><mml:mo>=</mml:mo><mml:msqrt><mml:mrow><mml:msub><mml:mi mathvariant="italic">ψ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mn mathvariant="normal">50</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">Hz</mml:mi></mml:mrow></mml:msqrt><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">7</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">mm</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</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> for the noise level of the spectrum <inline-formula><mml:math id="M81" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">ψ</mml:mi><mml:mi mathvariant="normal">n</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">6</mml:mn></mml:mrow></mml:msup><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">Hz</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>.</p>

      <fig id="F7"><label>Figure 7</label><caption><p id="d2e3031">Power spectral density of calibrated hot-wire wind data measured during a 20 min sampling period at approximately 10 m above the surface during RF22 (7 April 2024). The raw spectrum (lightgreen), the spectrum averaged over logarithmically equidistant bins (dark-green dashed), and a slope of <inline-formula><mml:math id="M82" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">5</mml:mn><mml:mo>/</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:math></inline-formula> for the inertia subrange (brown) are shown.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f07.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS4.SSS3">
  <label>3.4.3</label><title>Broadband radiation probe (BP)</title>
      <p id="d2e3062">The L2-data of the broadband radiation probe (BP; <xref ref-type="bibr" rid="bib1.bibx13" id="altparen.84"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987001" ext-link-type="DOI">10.1594/PANGAEA.987001</ext-link>) are provided at a temporal resolution of 1 Hz. We calibrated the broadband irradiance measurements following the methods introduced by <xref ref-type="bibr" rid="bib1.bibx20" id="text.85"/>, <xref ref-type="bibr" rid="bib1.bibx32" id="text.86"/>, and <xref ref-type="bibr" rid="bib1.bibx40" id="text.87"/>. The sensor senstivity specified in the manufacturer's certification was applied. Additionally, the effects of sensor inertia due to the finite response times of the radiometers were corrected using the method by <xref ref-type="bibr" rid="bib1.bibx23" id="text.88"/>. Subsequently, a low-pass filter was applied to reduce noise, employing a moving-window average with a period of 7 s. From the calibrated downward and upward irradiances, the net TIR irradiance, <inline-formula><mml:math id="M83" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, was calculated as <inline-formula><mml:math id="M84" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup><mml:mo>-</mml:mo><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, which quantifies the infrared radiative energy budget at flight altitude. Accordingly, the BP L2-dataset includes the following quantities: downward and upward terrestrial irradiances (<inline-formula><mml:math id="M85" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M86" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>), the net terrestrial irradiance <inline-formula><mml:math id="M87" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, measurements of air pressure, temperature, and relative humidity from the BME-280, as well as barometric altitude (Table <xref ref-type="table" rid="T3"/>).</p>
      <p id="d2e3156">Summarising all flights, Fig. <xref ref-type="fig" rid="F8"/> displays the frequency distribution of <inline-formula><mml:math id="M88" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values, comparing data measured at approximately 30 m height (near-surface) and around the profile peak heights, which range from 200 to 900 m (Fig. <xref ref-type="fig" rid="F4"/>). Both frequency distributions reveal <inline-formula><mml:math id="M89" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values spanning from <inline-formula><mml:math id="M90" display="inline"><mml:mo>-</mml:mo></mml:math></inline-formula>100 <inline-formula><mml:math id="M91" display="inline"><mml:mrow><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> (net upward radiation) to 0 <inline-formula><mml:math id="M92" display="inline"><mml:mrow><mml:mi mathvariant="normal">W</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">m</mml:mi><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula>, with barely positive values (net downward radiation). Significant differences can be identified between the two distributions and heights, highlighting the relevance of vertical profiling the radiative energy budget. In particular, there is a marked negative shift in the distribution curve toward more negative <inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values at profile peak heights. These differences between the near-surface and upper-level irradiance distributions are the result of vertical variation in cloud cover, with low-level clouds causing negative irradiance values.</p>

      <fig id="F8"><label>Figure 8</label><caption><p id="d2e3240">Frequency distribution of net thermal infrared irradiance values (<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) for near-surface data recorded at around 30 m height (purple), and for the profile peaks (orange), if their maximum heights were higher than 200 m. All flight periods with BP measurements are included.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f08.png"/>

          </fig>

</sec>
<sec id="Ch1.S3.SS4.SSS4">
  <label>3.4.4</label><title>Daily radiosondes</title>
      <p id="d2e3268">Profile measurements by radiosondes that were launched each morning before the first BELUGA ascent were published (<xref ref-type="bibr" rid="bib1.bibx12" id="altparen.89"/>, <ext-link xlink:href="https://doi.org/10.1594/PANGAEA.987053" ext-link-type="DOI">10.1594/PANGAEA.987053</ext-link>) to complement BELUGA observations of ABL profiles. These radiosonde profiles cover the full troposphere and thus facilitate further analysis by providing information about the background meteorological (synoptic) state above the ABL and above the BELUGA observations. The radiosondes used were of type DFM-17 (GRAW), measuring air pressure, temperature, relative humidity, wind speed, and wind direction. The upper-tropospheric profiles, especially regarding relative humidity are particularly relevant for locating clouds and moist areas above the ABL. Consequently, these profiles contributed to the identification of clear-to-cloudy transition events. The radiosonde data have been post-processed by quality checking the physical plausibility of the measurement values.</p>
      <p id="d2e3277">Figure <xref ref-type="fig" rid="F9"/> illustrates the meteorological standard quantities measured by all radiosonde launches during the campaign period at VRS (spring 2024). For a few days (27 and 30 March, 3 April), the radiosonde data were limited to below 5 km altitude due to data transfer issues. Overall, the radiosonde profiles indicate a predominantly stable stratified and mostly dry troposphere throughout the campaign. Winds remained generally calm, but they significantly intensified in the middle of the campaign.</p>

      <fig id="F9" specific-use="star"><label>Figure 9</label><caption><p id="d2e3284">Radiosonde profiles of <bold>(a)</bold> potential temperature, <bold>(b)</bold> relative humidity, <bold>(c)</bold> wind speed for the entire balloon-borne measurement campaign period in spring 2024 at VRS.  Profiles are only shown up to heights of 10 km.</p></caption>
            <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f09.png"/>

          </fig>

</sec>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Meteorological conditions during campaign</title>
      <p id="d2e3312">During the measurement period, Arctic sea ice extended along nearly the entire Greenland coast (Fig. <xref ref-type="fig" rid="F1"/>a), including the coastline near VRS (Fig. <xref ref-type="fig" rid="F1"/>b). Marine air masses reaching VRS and their thermodynamic vertical structure are influenced by their traversal over the sea-ice-covered ocean. The synoptic situation at VRS, and by this the thermodynamic BELUGA measurements, are furthermore often influenced by katabatic flows, driven by the complex orography in the hinterland of Station Nord.</p>
      <p id="d2e3319">We use the CARRA reanalysis data <xref ref-type="bibr" rid="bib1.bibx46" id="paren.90"/> to briefly describe the synoptic conditions.  Maps of the equivalent potential temperature <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at 850 hPa and the 500 hPa geopotential heights in Fig. <xref ref-type="fig" rid="F10"/> illustrate how the synoptic patterns changed considerably over the measurement campaign period. During the first week of the measurement period (20–27 March 2024, Fig. <xref ref-type="fig" rid="F10"/>a), an expansive high-pressure ridge over the North Atlantic advected rather cold and dry air masses from the pole towards VRS. Nevertheless, the flow remained weak because the geopotential gradients were relatively small. The synoptic situation changed during the second week when the northeastern part of Greenland and the Fram Strait became increasingly influenced by a low-pressure system northeast of Svalbard (Fig. <xref ref-type="fig" rid="F10"/>b). Although southwestern Greenland remained under the influence of the high-pressure ridge, the geopotential gradients over VRS substantially increased, favoring intensified northwestern winds and the advection of cold polar air masses. The approaching low pressure system also increased the likelihood of cloud formation at VRS.</p>

      <fig id="F10" specific-use="star"><label>Figure 10</label><caption><p id="d2e3344">CARRA-based synoptic overview of campaign period depicting four days (23 and 30 March 2024, 5 and 10 April 2024). For each day, filled contours show equivalent potential temperature <inline-formula><mml:math id="M96" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mi mathvariant="normal">e</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> at 850 hPa. Isolines show geopotential metre at the 500 hPa level.</p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f10.jpg"/>

      </fig>

      <p id="d2e3365">In the first week of April (Fig. <xref ref-type="fig" rid="F10"/>c), this pattern persisted in general; however, the geopotential dipoles declined, reducing the pressure gradients over northeast Greenland and surface winds. The decrease in advection of polar air masses caused <inline-formula><mml:math id="M97" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">Θ</mml:mi><mml:mrow><mml:mi mathvariant="normal">e</mml:mi><mml:mo>,</mml:mo><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mn mathvariant="normal">850</mml:mn><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">hPa</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula> to rise to approximately 265 K at VRS. In the last week of the campaign, particularly on 10 April (Fig. <xref ref-type="fig" rid="F10"/>d), a significant change occurred in the synoptic pattern due to the formation of a low-pressure system over central North Greenland (with <inline-formula><mml:math id="M98" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 5000 gpdm at the 500 hPa level in its core). This resulted in southerly winds over northeastern Greenland and a weak intrusion of warm, moist air south of the Fram Strait.</p>
      <p id="d2e3399">These large-scale synoptic patterns are reflected in the local conditions at VRS, as illustrated over the entire measurement period using CARRA data in Fig. <xref ref-type="fig" rid="F11"/>. During the first week, when weak pressure gradients prevailed, winds were calm at VRS, favoring stable stratification, as indicated by the spread of <inline-formula><mml:math id="M99" display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> between 50 and 500 m altitude (Fig. <xref ref-type="fig" rid="F11"/>a, b). High RH values near the surface highlight the potential presence of a near-surface inversion, which conserves moisture close to the ground (Fig. <xref ref-type="fig" rid="F11"/>c). The approaching low pressure system in the second week led to a significant increase in wind speeds exceeding 10 <inline-formula><mml:math id="M100" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">s</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> at VRS (Fig. <xref ref-type="fig" rid="F11"/>b). Notably, when the upper-level wind speeds decreased at the beginning of April, a LLJ persisted with a strong reduction in relative humidity, which was associated with significant warming of the ABL (Fig. <xref ref-type="fig" rid="F11"/>a). For the rest of the campaign, <inline-formula><mml:math id="M101" display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> values remained relatively constant; however, around 10 April, the vertical profiles of wind speed indicate another LLJ event (Fig. <xref ref-type="fig" rid="F11"/>b), with higher relative humidity located below this jet (Fig. <xref ref-type="fig" rid="F11"/>c). The radiosonde profiles, which were shown for the entire troposphere in Fig. <xref ref-type="fig" rid="F9"/>, also generally confirm the synoptic development in the ABL indicated by CARRA in Fig. <xref ref-type="fig" rid="F11"/>, highlighting the rather dry conditions at VRS.</p>

      <fig id="F11" specific-use="star"><label>Figure 11</label><caption><p id="d2e3455">Meteorological conditions during the measurement campaign period (24 March to 10 April 2024) as represented by CARRA reanalysis data interpolated onto the measurement station location. <bold>(a)</bold> shows potential temperature values for 50 and 500 m height above ground over the measurement period, together wind speed values at 50 m on the additional right <inline-formula><mml:math id="M102" display="inline"><mml:mi>y</mml:mi></mml:math></inline-formula> axis. <bold>(b)</bold> depicts the vertical profiles of wind speed for the lowest 500 m. <bold>(c)</bold> represents the vertical profiles of relative humidity. </p></caption>
        <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f11.png"/>

      </fig>

</sec>
<sec id="Ch1.S5">
  <label>5</label><title>Data potential to investigate transition events</title>
      <p id="d2e3489">While the thermal stratification of the ABL, as well as moisture and wind conditions, changed considerably throughout the measurement period (Sect. <xref ref-type="sec" rid="Ch1.S4"/>), numerous transitions between the ABL states occurred. We classified three major categories of transition events based on visual data inspection: (1) changes in cloud conditions between clear and cloudy states, (2) LLJ evolution, and (3) day-to-night transitions. When these transitions occurred during flight, they are documented in Table <xref ref-type="table" rid="T2"/> and Fig. <xref ref-type="fig" rid="F11"/>, and are also marked as attributes in the L2-data. Accordingly, fifteen RFs recorded significant transitions that modulated the Arctic ABL conditions.</p>
      <p id="d2e3499">The following section sketches how BELUGA L2-data from VRS during such transitions can enhance our understanding of Arctic ABL steering processes, for example, regarding temporal temperature changes and radiative heating rates under varying cloud conditions. To fully exploit the BELUGA data and draw robust conclusions about the observed processes, future work will also rely on joint analysis with numerical weather prediction models or reanalysis data. An important aspect in this context is the comparability of the BELUGA data to the model data, particularly with respect to the vertical resolution, which we introduce here for one of the LLJ events and reanalysis data.</p>
<sec id="Ch1.S5.SS1">
  <label>5.1</label><title>Temperature tendencies in near-surface inversions</title>
      <p id="d2e3509">Among the transitions between Arctic ABL states, changes in cloud conditions have significant impact on the ABL structure, particularly evident in variations of the vertical temperature gradient (lapse-rate) at small temporal and vertical scales. The repetitive BELUGA profile observations, with their high temporal resolution, enable us to resolve such thermodynamic impacts.</p>
      <p id="d2e3513">Figure <xref ref-type="fig" rid="F12"/> shows exemplary vertical potential temperature profiles from 2 April 2024 (RF15), sampled under varying cloud and moisture conditions. High RH values above 5 km, measured by the radiosonde (Fig. <xref ref-type="fig" rid="F9"/>), suggest the presence of mid- to high-level (cirrus) clouds, as confirmed by local ceilometer data (not shown) showing that they were descending and gradually dissipating during flight. At the start of the profiling sequence, a pronounced near-surface temperature inversion was present within the lowest 100 m. The inversion weakened in successive profiles, likely due to enhanced turbulent mixing associated with increasing surface heating. Later profiles reveal a smoother potential temperature variation with height (Fig. <xref ref-type="fig" rid="F12"/>b).</p>

      <fig id="F12"><label>Figure 12</label><caption><p id="d2e3524">Near-surface thermal structure and its temporal evolution during RF15 (2 April 2024) based on <inline-formula><mml:math id="M103" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="normal">TMP</mml:mi><mml:mi mathvariant="normal">met</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> data. <bold>(a)</bold> Flight altitude, with colour-coded progression over time. <bold>(b)</bold> Vertical profiles of potential temperature (<inline-formula><mml:math id="M104" display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula>), with each profile colour-matched to the corresponding time segment in <bold>(a)</bold>. <bold>(c)</bold> Calculated  potential temperature tendency in <inline-formula><mml:math id="M105" display="inline"><mml:mrow><mml:mi mathvariant="normal">K</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">h</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> as vertical profile, referring to the difference between the first and last <inline-formula><mml:math id="M106" display="inline"><mml:mi mathvariant="normal">Θ</mml:mi></mml:math></inline-formula> profiles in <bold>(b)</bold>. Positive (negative) values indicate warming (cooling).</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f12.png"/>

        </fig>

      <p id="d2e3592">For the sequence of temperature profiles, we calculated the temperature tendencies, which are, as displayed in Fig. <xref ref-type="fig" rid="F12"/>c, based on first and last profiles (with a time gap of approximately 2.75 h). The tendencies indicate modest cooling above 300 m, slight warming between 200 and 300 m, and near-surface cooling or reduced heating. The tendencies are statistically significant and robust, as indicated by the calculated uncertainty ranges (Fig. <xref ref-type="fig" rid="F12"/>c). We estimated the uncertainties using Gaussian error propagation, assuming a constant temperature measurement uncertainty of <inline-formula><mml:math id="M107" display="inline"><mml:mo>±</mml:mo></mml:math></inline-formula>0.2 K, as specified for the sensor in Table <xref ref-type="table" rid="T1"/>.</p>
      <p id="d2e3608">Taking uncertainties into account, the results demonstrate that even subtle thermal tendencies can be detected with confidence by the BELUGA observations. This example highlights the capability of BELUGA's high-resolution profiling to investigate ABL inversion thermodynamics, particularly during transitions under varying cloud conditions.</p>
</sec>
<sec id="Ch1.S5.SS2">
  <label>5.2</label><title>Evolution of heating rates in cloudfree <inline-formula><mml:math id="M108" display="inline"><mml:mo>↔</mml:mo></mml:math></inline-formula> cloudy transitions</title>
      <p id="d2e3627">In addition to advection (horizontal exchange of different air masses), phase transitions, and vertical mixing by turbulence, the divergence of the local radiative fluxes can induce the temperature tendencies in the near-surface inversion during transitions between cloud-free and cloudy states described in Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/>. The divergence of radiative energy flux, measured by BELUGA with the BP, can be translated into radiative heating rates. The local radiative heating rate is defined as the temporal change in temperature resulting from variations in net irradiance <inline-formula><mml:math id="M109" display="inline"><mml:mrow><mml:mi mathvariant="italic">δ</mml:mi><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> with altitude <inline-formula><mml:math id="M110" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx20" id="paren.91"/>. Following <xref ref-type="bibr" rid="bib1.bibx33" id="text.92"/> and using the downward and upward terrestrial irradiance (<inline-formula><mml:math id="M111" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M112" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula>) measured by the BP at a given height <inline-formula><mml:math id="M113" display="inline"><mml:mi>z</mml:mi></mml:math></inline-formula>, the radiative heating rates <inline-formula><mml:math id="M114" display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula> are calculated as:

            <disp-formula id="Ch1.E2" content-type="numbered"><label>2</label><mml:math id="M115" display="block"><mml:mrow><mml:mi mathvariant="italic">ζ</mml:mi><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mrow><mml:mi mathvariant="italic">ρ</mml:mi><mml:mo>⋅</mml:mo><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="normal">Δ</mml:mi><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mfenced close=")" open="("><mml:mrow><mml:munder><mml:munder class="underbrace"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo><mml:mo>-</mml:mo><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi>z</mml:mi><mml:mo>)</mml:mo></mml:mrow><mml:mo mathvariant="normal">︸</mml:mo></mml:munder><mml:mstyle scriptlevel="+1"><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mstyle></mml:munder></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>

          where <inline-formula><mml:math id="M116" display="inline"><mml:mi mathvariant="italic">ρ</mml:mi></mml:math></inline-formula> represents the air density and <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:msub><mml:mi>c</mml:mi><mml:mi mathvariant="normal">p</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is the specific heat capacity of air at constant pressure. For the calculations, a single BELUGA profile is used, assuming that the environment remains in a steady state during vertical profiling of the ABL. A layer thickness of <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>z</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">10</mml:mn><mml:mspace linebreak="nobreak" width="0.125em"/><mml:mi mathvariant="normal">m</mml:mi></mml:mrow></mml:math></inline-formula> was chosen.</p>

      <fig id="F13" specific-use="star"><label>Figure 13</label><caption><p id="d2e3823">BELUGA observed net irradiance <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> as a function of height showing the first and last profile of RF15 <bold>(a)</bold>. From these profiles, heating rates <inline-formula><mml:math id="M120" display="inline"><mml:mi mathvariant="italic">ζ</mml:mi></mml:math></inline-formula> are calculated using Eq. (<xref ref-type="disp-formula" rid="Ch1.E2"/>) and their mean is derived.</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f13.png"/>

        </fig>

      <p id="d2e3855">Reconsidering the thermal inversion under changing cloud conditions during RF15, we, similar to Sect. <xref ref-type="sec" rid="Ch1.S5.SS1"/> and Fig. <xref ref-type="fig" rid="F12"/>, analyse the first and last profile to demonstrate the capabilities of BELUGA to study heating rate profiles during a transition event. Their net irradiances and calculated heating rates are shown in Fig. <xref ref-type="fig" rid="F13"/>. While the intensification of the net upward irradiance remains relatively consistent between both profiles up to 150 m, the last profile exhibits a much stronger vertical decay of <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>, even though <inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msub><mml:mi>F</mml:mi><mml:mi mathvariant="normal">net</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values become less negative around the inversion bottom (Fig. <xref ref-type="fig" rid="F13"/>a). The calculated heating rates (Fig. <xref ref-type="fig" rid="F13"/>b) are approximately half the magnitude of the (potential) temperature tendencies identified in Fig. <xref ref-type="fig" rid="F12"/>. The negative heating rates (cooling) suggest that advection somewhat overcompensates radiative effects on the lapse rate, especially near the inversion at around 200 m. This inversion height corresponds to the vertical level with the strongest cooling and heating rates. This vertical variability of radiative heating rates, as shown in Fig. <xref ref-type="fig" rid="F13"/>, emphasizes the importance of quantifying thermal irradiance as a function of height to better understand the evolution of the ABL with respect to the thermodynamic and radiative effects modulating the ABL structure.</p>
</sec>
<sec id="Ch1.S5.SS3">
  <label>5.3</label><title>Low-level jet evolution</title>
      <p id="d2e3905">LLJs play a significant role in modulating the structure of the Arctic ABL due to their influence on vertical entrainment. Balloon-borne observations are well suited for studying LLJ events. Previous balloon-borne studies have demonstrated that LLJs can effectively enhance near-surface horizontal transport of passive tracers <xref ref-type="bibr" rid="bib1.bibx22" id="paren.93"/>.</p>
      <p id="d2e3911">During the measurement campaign at VRS, BELUGA sampled several LLJ events, as listed in Table <xref ref-type="table" rid="T2"/> and shown in Fig. <xref ref-type="fig" rid="F11"/>. A prominent LLJ example is presented in Fig. <xref ref-type="fig" rid="F14"/>, illustrating vertical profiles of potential temperature, wind speed, and specific humidity observed from RF12 on 1 April 2024. The BELUGA observations reveal a pronounced LLJ with a maximum wind speed approaching 5 <inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msup><mml:mtext>m s</mml:mtext><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:mrow></mml:math></inline-formula> above a stably stratified Arctic ABL extending up to 100 m (Fig. <xref ref-type="fig" rid="F14"/>a, b). Over the course of the flight, the LLJ intensity increased by approximately 1 <inline-formula><mml:math id="M124" display="inline"><mml:mrow><mml:mi mathvariant="normal">m</mml:mi><mml:mspace linebreak="nobreak" width="0.125em"/><mml:msup><mml:mi mathvariant="normal">s</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="F14"/>b). Apart from a decrease in the near-surface layer (<inline-formula><mml:math id="M125" display="inline"><mml:mo lspace="0mm">&lt;</mml:mo></mml:math></inline-formula> 50 m), moisture conditions remained fairly homogeneous throughout the lowest 500 m  with <inline-formula><mml:math id="M126" display="inline"><mml:mi>q</mml:mi></mml:math></inline-formula> between 0.4 and 0.5<inline-formula><mml:math id="M127" display="inline"><mml:mrow><mml:mspace width="0.125em" linebreak="nobreak"/><mml:mi mathvariant="normal">g</mml:mi><mml:mspace width="0.125em" linebreak="nobreak"/><mml:msup><mml:mi mathvariant="normal">kg</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="F14"/>c).</p>

      <fig id="F14" specific-use="star"><label>Figure 14</label><caption><p id="d2e3992">Flight pattern of RF12 during 1 April 2024 <bold>(a)</bold>, with measured vertical profiles of potential temperature <bold>(b)</bold>, horizontal wind speed <bold>(c)</bold>, and specific humidty <bold>(d)</bold> by BELUGA. The observations are compared to the corresponding CARRA data (bold dots) which are interpolated onto the VRS location and considers the model time steps that correspond to the flight duration. All data is shown as a function of height above ground level (a.g.l.).</p></caption>
          <graphic xlink:href="https://essd.copernicus.org/articles/18/2799/2026/essd-18-2799-2026-f14.png"/>

        </fig>

      <p id="d2e4014">These measurements allow the structure of LLJs in Arctic ABLs to be compared with reanalysis-based profiles. As an example, Fig. <xref ref-type="fig" rid="F14"/> includes the corresponding CARRA reanalysis profiles for the duration of the flight. The overall agreement between BELUGA and CARRA, particularly regarding potential temperature (Fig. <xref ref-type="fig" rid="F14"/>a) and the general shape of the LLJ, places the observations in a broader meteorological context. The high-resolution vertical profiles of meteorological, radiative, and turbulence conditions obtained with BELUGA provide valuable case-study material for future evaluations of high-resolution reanalyses such as those provided by CARRA. The observations support efforts to better understand limitations in the model-based representation of transition events. The differences in specific humidity and maximum wind speed at the LLJ height for this case in CARRA (Fig.<xref ref-type="fig" rid="F14"/>b, c) illustrate aspects to be examined in more detail across additional LLJ events.</p>
</sec>
</sec>
<sec id="Ch1.S6">
  <label>6</label><title>Code and data availability</title>
      <p id="d2e4032">All processed BELUGA and radiosonde Level-2 data are publicly available at the World Data Center PANGAEA under CC-BY 4.0 (Table <xref ref-type="table" rid="T3"/>). The entire data set is compiled in the data collection entitled <italic>Balloon-borne profile L2-data characterising the Arctic boundary layer and troposphere at Villum Research Station</italic> (<ext-link xlink:href="https://doi.org/10.1594/PANGAEA.986431" ext-link-type="DOI">10.1594/PANGAEA.986431</ext-link>, <xref ref-type="bibr" rid="bib1.bibx14" id="altparen.94"/>). All included netCDF files follow the Climate and Forecast (CF) Metadata Conventions version 1.12 (<ext-link xlink:href="https://doi.org/10.5281/zenodo.14275599" ext-link-type="DOI">10.5281/zenodo.14275599</ext-link>, <xref ref-type="bibr" rid="bib1.bibx19" id="altparen.95"/>). Details about the raw and Level-1 measurement files can be obtained upon request.</p>
      <p id="d2e4053">We strongly encourage the use of balloon-borne L2-data from VRS as a continuation of a series of previous BELUGA measurement campaigns with similar instrumental setups, such as during the Physical feedbacks of Arctic planetary boundary level Sea ice, Cloud and AerosoL (PASCAL)  campaign (<xref ref-type="bibr" rid="bib1.bibx63" id="altparen.96"/>; <xref ref-type="bibr" rid="bib1.bibx20" id="altparen.97"/>; <xref ref-type="bibr" rid="bib1.bibx21" id="altparen.98"/>), the Multidisciplinary drifting Observatory for the Study of Arctic Climate (MOSAiC) expedition (<xref ref-type="bibr" rid="bib1.bibx51" id="altparen.99"/>; <xref ref-type="bibr" rid="bib1.bibx32" id="altparen.100"/>;  <xref ref-type="bibr" rid="bib1.bibx40" id="altparen.101"/>), and at Ny-Ålesund, Svalbard <xref ref-type="bibr" rid="bib1.bibx33" id="paren.102"/>.</p>
      <p id="d2e4078">The CARRA data used to analyse the meteorological conditions are publicly available, provided by <xref ref-type="bibr" rid="bib1.bibx46" id="text.103"/> at <ext-link xlink:href="https://doi.org/10.24381/CDS.8679900D" ext-link-type="DOI">10.24381/CDS.8679900D</ext-link>. This CARRA dataset includes eleven specific height levels, ranging from 15 m up to 500 m.</p>
      <p id="d2e4087">The CARRA data corresponding to the campaign period and the nearest grid cell of Station Nord are provided with slight post-proccesing and plotting routines in <xref ref-type="bibr" rid="bib1.bibx11" id="text.104"/> at <ext-link xlink:href="https://doi.org/10.5281/zenodo.17660389" ext-link-type="DOI">10.5281/zenodo.17660389</ext-link>.</p>
      <p id="d2e4097">The python-based code for processing the balloon-borne measurements from Level-0 (raw) to Level-2 (published) is accessible via Zenodo (<ext-link xlink:href="https://doi.org/10.5281/zenodo.18763860" ext-link-type="DOI">10.5281/zenodo.18763860</ext-link>, <xref ref-type="bibr" rid="bib1.bibx15" id="altparen.105"/>). The processing code framework employs an object-oriented architecture, with the main class <italic>BELUGA</italic> composed of three subclasses specific to the instrument probes. These subclasses contain all routines required for the post-processing of measurements, complemented by plotting functions to visualise processing steps and data analysis.</p>
</sec>
<sec id="Ch1.S7" sec-type="conclusions">
  <label>7</label><title>Summary and conclusions</title>
      <p id="d2e4117">As part of the <inline-formula><mml:math id="M128" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">A</mml:mi><mml:mi mathvariant="script">C</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> project, this paper presents an observation-based dataset comprising balloon-borne measurements within the Arctic boundary layer, obtained using the Balloon-bornE moduLar Utility for profilinG the lower Atmosphere (BELUGA) system. BELUGA is a tethered balloon equipped with multiple atmospheric sensors, enabling high-resolution vertical profiling of temperature, humidity, wind fields, turbulence, and broadband thermal-infrared irradiance. The dataset described herein originates from a comprehensive measurement campaign conducted at the Villum Research Station (VRS) at Station Nord (81°36<sup>′</sup> 9<sup>′′</sup> N, 16°40<sup>′</sup>12<sup>′′</sup> W), Greenland, from 19 March to 18 April 2024. The processed Level-2 measurement data are publicly available and are compiled in a PANGAEA data bibliography <xref ref-type="bibr" rid="bib1.bibx14" id="paren.106"/>, organized into probe-separated subsets providing netCDF files for each individual research flight (RF).</p>
      <p id="d2e4183">Overall, a total of 28 BELUGA RFs were conducted during the measurement period in spring 2024 at VRS.  The measurement strategy aimed to perform continuous profiling throughout the Arctic atmospheric boundary layer (ABL). The RFs collected measurement data over approximately 76 flight hours and yielded 336 deep vertical profiles, sampling thermodynamic (<inline-formula><mml:math id="M133" display="inline"><mml:mi>T</mml:mi></mml:math></inline-formula>, RH, <inline-formula><mml:math id="M134" display="inline"><mml:mi>p</mml:mi></mml:math></inline-formula>), radiation (up- and downward terrestrial near-infrared irradiance; <inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↑</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M136" display="inline"><mml:mrow><mml:msup><mml:mi>F</mml:mi><mml:mo>↓</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) and turbulence parameters (eddy dissipation rate <inline-formula><mml:math id="M137" display="inline"><mml:mi mathvariant="italic">ϵ</mml:mi></mml:math></inline-formula>) within the Arctic ABL. Some profiles reached altitudes of up to 900 m. During each flight, measurements were performed mainly in a continuous manner for several hours, limited only by battery constraints.</p>
      <p id="d2e4229">This BELUGA data from VRS enable the investigation of the temporal evolution of the ABL with near-surface inversions under various atmospheric transitions, including the day-to-night transitions, cloud cover variations, and low-level jet (LLJ) formation. We presented examples of observed transitions and highlighted the scientific applicability of the published balloon-borne observations for understanding temperature and heating rates occurring in near-surface inversions,  as well as the radiative energy budget during Arctic low-level cloudfree-cloudy transitions, and thermodynamic characteristics during LLJ formation.</p>
      <p id="d2e4232">These observations offer valuable insights into Arctic ABL transitions, emphasizing the roles of near-surface thermal inversions, cloud-radiative effects and wind structure evolution. By shedding light on these processes, BELUGA data significantly enhance the understanding and quantification of surface warming via the lapse rate feedback, which is driven by temperature lapse rate (stability), inversion height and strength, vertical humidity, air mass circulation, and cloud processes. Current climate models still face challenges in adequately resolving the relevant small-scale processes within the ABL, although the lapse-rate feedback is recognised as the primary driver of Arctic amplification (<xref ref-type="bibr" rid="bib1.bibx41" id="altparen.107"/>; <xref ref-type="bibr" rid="bib1.bibx45" id="altparen.108"/>).</p>
      <p id="d2e4242">For this reason, we encourage synergy studies that combine the BELUGA observations with various modeling frameworks to examine the ABL evolution and their impact on the lapse-rate feedback at different scales. Single column models (SCMs) can quantify the influence of clouds on ABL evolution, also for heights unreachable for the balloon.  SCMs are computationally efficient and suitable for inexpensive parameterization testing and sensitivity experiments, using BELUGA measurements as input. Large-eddy simulations (LES) can elucidate horizontal cloud scenarios and resolve dynamical boundary layer processes on larger scales, but are associated with high computational costs. Comparing the observations with NWP models can assess how accurately transitions between different states of the Arctic ABL and their influence on surface warming via the lapse-rate feedback are represented in longer-term projections. Additionally, BELUGA data are crucial for evaluating reanalyses such as the ECMWF Reanalysis v5 (ERA5) and the Copernicus Arctic Regional Reanalysis (CARRA).</p>
      <p id="d2e4245">Together with the supplementary observational platforms installed at VRS during spring 2024 (Sect. <xref ref-type="sec" rid="Ch1.S2.SS1"/>) and the aforementioned model configurations, the BELUGA L2-data are embedded within a manifold framework, which enhances the ability to simulate Arctic ABL processes under varying atmospheric conditions and to understand how their contributions to Arctic amplification via feedback mechanisms. The synergy of these datasets will provide an unprecedented and comprehensive characterisation of the Arctic ABL. This enables greater insight into the role of surface warming driven by the lapse-rate feedback, with balloon-borne observations serving as benchmarks for model-based,  process-oriented sensitivity studies.</p>
</sec>

      
      </body>
    <back><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d2e4254">MW and HS were the main initiators for the conceptualisation of the measurement approach and its acquisition. HS and MS conducted the balloon-borne measurements at Station Nord. HD was in charge for post-processing the balloon-borne data with fundamental support for the TMP data by HS and KN, and support for the BP data by MS, AE, FW, and JM, and support for the radiosonde data by JM. The publication of the post-processed data was led by HD. HD conceptualised and drafted the manuscript and visualisations, while HS and KN were responsible for specific sections concerning turbulence measurements (HS) and scientific analysis of temperature rates (KN). All authors were involved in revising the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d2e4260">The contact author has declared that none of the authors has any competing interests.</p>
  </notes><notes notes-type="disclaimer"><title>Disclaimer</title>

      <p id="d2e4266">Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. The authors bear the ultimate responsibility for providing appropriate place names. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.</p>
  </notes><ack><title>Acknowledgements</title><p id="d2e4272">We gratefully acknowledge the funding by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – project no. 268020496 – within the Transregional Collaborative Research Center TRR 172, “ArctiC Amplification: Climate Relevant Atmospheric and SurfaCe Processes”, and Feedback Mechanisms <inline-formula><mml:math id="M138" display="inline"><mml:mrow><mml:mo>(</mml:mo><mml:mi mathvariant="script">A</mml:mi><mml:mi mathvariant="script">C</mml:mi><mml:msup><mml:mo>)</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> in sub-project A02 “Balloon-borne observations and dedicated simulations of the transitions between typical states of the Arctic atmospheric boundary layer”. We also thank Henrik Skov, head of the Villum Research Station, for his support during our stay. Without Jørgen Skafte and Bjarne Jensen, the work on site and logistics would not have been possible. The staff of Station Nord provided logistical support for our work. Thanks to Johannes Röttenbacher and Amelie Driemel for their support during data publication and additional manuscript comments, as well as to Andreas Walbröl.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d2e4294">This research has been supported by the Deutsche Forschungsgemeinschaft (grant no. 268020496).Supported by the Open Access Publishing Fund  of Leipzig University.</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d2e4306">This paper was edited by Fan Mei and reviewed by Christof Lüpkes and one anonymous referee.</p>
  </notes><ref-list>
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