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  <front>
    <journal-meta><journal-id journal-id-type="publisher">ACP</journal-id><journal-title-group>
    <journal-title>Atmospheric Chemistry and Physics</journal-title>
    <abbrev-journal-title abbrev-type="publisher">ACP</abbrev-journal-title><abbrev-journal-title abbrev-type="nlm-ta">Atmos. Chem. Phys.</abbrev-journal-title>
  </journal-title-group><issn pub-type="epub">1680-7324</issn><publisher>
    <publisher-name>Copernicus Publications</publisher-name>
    <publisher-loc>Göttingen, Germany</publisher-loc>
  </publisher></journal-meta>
    <article-meta>
      <article-id pub-id-type="doi">10.5194/acp-21-10851-2021</article-id><title-group><article-title>The 2019 Raikoke volcanic eruption – Part 1: Dispersion model simulations and satellite retrievals of volcanic sulfur dioxide</article-title><alt-title><inline-formula><mml:math id="M1" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> dispersion model simulations and satellite retrievals for the 2019 Raikoke eruption</alt-title>
      </title-group><?xmltex \runningtitle{{$\chem{SO_{{2}}}$} dispersion model simulations and satellite retrievals for the 2019~Raikoke eruption}?><?xmltex \runningauthor{J.~de~Leeuw et al.}?>
      <contrib-group>
        <contrib contrib-type="author" corresp="yes" rid="aff1">
          <name><surname>de Leeuw</surname><given-names>Johannes</given-names></name>
          <email>jd876@cam.ac.uk</email>
        <ext-link>https://orcid.org/0000-0003-3062-9152</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff1 aff2">
          <name><surname>Schmidt</surname><given-names>Anja</given-names></name>
          
        <ext-link>https://orcid.org/0000-0001-8759-2843</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Witham</surname><given-names>Claire S.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff4">
          <name><surname>Theys</surname><given-names>Nicolas</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Taylor</surname><given-names>Isabelle A.</given-names></name>
          
        <ext-link>https://orcid.org/0000-0002-6824-893X</ext-link></contrib>
        <contrib contrib-type="author" corresp="no" rid="aff5">
          <name><surname>Grainger</surname><given-names>Roy G.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff6 aff7">
          <name><surname>Pope</surname><given-names>Richard J.</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff8">
          <name><surname>Haywood</surname><given-names>Jim</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3 aff8">
          <name><surname>Osborne</surname><given-names>Martin</given-names></name>
          
        </contrib>
        <contrib contrib-type="author" corresp="no" rid="aff3">
          <name><surname>Kristiansen</surname><given-names>Nina I.</given-names></name>
          
        </contrib>
        <aff id="aff1"><label>1</label><institution>Department of Chemistry, University of Cambridge, Cambridge, UK</institution>
        </aff>
        <aff id="aff2"><label>2</label><institution>Department of Geography, University of Cambridge, Cambridge, UK</institution>
        </aff>
        <aff id="aff3"><label>3</label><institution>Met Office, Exeter, UK</institution>
        </aff>
        <aff id="aff4"><label>4</label><institution>Royal Belgian Institute for Space Aeronomy (BIRA-IASB), Brussels, Belgium</institution>
        </aff>
        <aff id="aff5"><label>5</label><institution>COMET, Sub‐Department of Atmospheric, Oceanic and Planetary Physics, University of Oxford, Oxford, UK</institution>
        </aff>
        <aff id="aff6"><label>6</label><institution>School of Earth and Environment, University of Leeds, Leeds, UK</institution>
        </aff>
        <aff id="aff7"><label>7</label><institution>National Centre for Earth Observation, University of Leeds, Leeds, UK</institution>
        </aff>
        <aff id="aff8"><label>8</label><institution>College of Engineering, Mathematics, and Physical Sciences, University of Exeter, Exeter, UK</institution>
        </aff>
      </contrib-group>
      <author-notes><corresp id="corr1">Johannes de Leeuw (jd876@cam.ac.uk)</corresp></author-notes><pub-date><day>19</day><month>July</month><year>2021</year></pub-date>
      
      <volume>21</volume>
      <issue>14</issue>
      <fpage>10851</fpage><lpage>10879</lpage>
      <history>
        <date date-type="received"><day>25</day><month>August</month><year>2020</year></date>
           <date date-type="rev-request"><day>7</day><month>October</month><year>2020</year></date>
           <date date-type="rev-recd"><day>12</day><month>April</month><year>2021</year></date>
           <date date-type="accepted"><day>27</day><month>April</month><year>2021</year></date>
      </history>
      <permissions>
        <copyright-statement>Copyright: © 2021 </copyright-statement>
        <copyright-year>2021</copyright-year>
      <license license-type="open-access"><license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri" xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p></license></permissions><self-uri xlink:href="https://acp.copernicus.org/articles/.html">This article is available from https://acp.copernicus.org/articles/.html</self-uri><self-uri xlink:href="https://acp.copernicus.org/articles/.pdf">The full text article is available as a PDF file from https://acp.copernicus.org/articles/.pdf</self-uri>
      <abstract><title>Abstract</title>
    <p id="d1e222">Volcanic eruptions can cause significant disruption to society, and numerical models are crucial for forecasting the dispersion of erupted material. Here we assess the skill and limitations of the Met Office's Numerical Atmospheric-dispersion Modelling Environment (NAME) in simulating the dispersion of the sulfur dioxide (<inline-formula><mml:math id="M2" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) cloud from the 21–22 June 2019 eruption of the Raikoke volcano (48.3<inline-formula><mml:math id="M3" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153.2<inline-formula><mml:math id="M4" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E). The eruption emitted around <inline-formula><mml:math id="M5" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> Tg of <inline-formula><mml:math id="M6" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, which represents the largest volcanic emission of <inline-formula><mml:math id="M7" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the stratosphere since the 2011 Nabro eruption. We simulate the temporal evolution of the volcanic <inline-formula><mml:math id="M8" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud across the Northern Hemisphere (NH) and compare our model simulations to high-resolution <inline-formula><mml:math id="M9" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> measurements from the TROPOspheric Monitoring Instrument (TROPOMI) and the Infrared Atmospheric Sounding Interferometer (IASI) satellite <inline-formula><mml:math id="M10" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products.</p>
    <p id="d1e322">We show that NAME accurately simulates the observed location and horizontal extent of the <inline-formula><mml:math id="M11" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud during the first 2–3 weeks after the eruption but is unable, in its standard configuration, to capture the extent and precise location of the highest magnitude vertical column density (VCD) regions within the observed volcanic cloud. Using the structure–amplitude–location (SAL) score and the fractional skill score (FSS) as metrics for model skill, NAME shows skill in simulating the horizontal extent of the cloud for 12–17 d after the eruption where VCDs of <inline-formula><mml:math id="M12" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (in Dobson units, DU) are above 1 DU. For <inline-formula><mml:math id="M13" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above 20 DU, which are predominantly observed as small-scale features within the <inline-formula><mml:math id="M14" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud, the model shows skill on the order of 2–4 d only. The lower skill for these high-<inline-formula><mml:math id="M15" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>-VCD regions is partly explained by the model-simulated <inline-formula><mml:math id="M16" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud in NAME being too diffuse compared to TROPOMI retrievals. Reducing the standard horizontal diffusion parameters used in NAME by a factor of 4 results in a slightly increased model skill during the first 5 d of the simulation, but on longer timescales the simulated <inline-formula><mml:math id="M17" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud remains too diffuse when compared to TROPOMI measurements.</p>
    <p id="d1e403">The skill of NAME to simulate high <inline-formula><mml:math id="M18" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs and the temporal evolution of the NH-mean <inline-formula><mml:math id="M19" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden is dominated by the fraction of <inline-formula><mml:math id="M20" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass emitted into the lower stratosphere, which is uncertain for the 2019 Raikoke eruption. When emitting 0.9–1.1 Tg of <inline-formula><mml:math id="M21" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the lower stratosphere (11–18 km) and 0.4–0.7 Tg into the upper troposphere (8–11 km), the NAME simulations show a similar peak in <inline-formula><mml:math id="M22" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden to that derived from TROPOMI (1.4–1.6 Tg of <inline-formula><mml:math id="M23" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) with an average <inline-formula><mml:math id="M24" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <inline-formula><mml:math id="M25" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of 14–15 d in the NH.</p>
    <p id="d1e491">Our work illustrates how the synergy between high-resolution satellite retrievals and dispersion models can identify potential limitations of dispersion models like NAME,<?pagebreak page10852?> which will ultimately help to improve dispersion modelling efforts of volcanic <inline-formula><mml:math id="M26" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds.</p>
  </abstract>
    </article-meta>
  </front>
<body>
      

<sec id="Ch1.S1" sec-type="intro">
  <label>1</label><title>Introduction</title>
      <p id="d1e514">Volcanic activity can vary strongly in intensity, ranging from passive degassing volcanoes emitting sulfur into the lower troposphere to explosive eruptions that can release large amounts of ash and gases high into the stratosphere <xref ref-type="bibr" rid="bib1.bibx71" id="paren.1"><named-content content-type="pre">e.g.</named-content></xref>. It is well established that volcanic eruptions can impact Earth's climate system through changes in the energy balance <xref ref-type="bibr" rid="bib1.bibx87 bib1.bibx90 bib1.bibx93 bib1.bibx97" id="paren.2"><named-content content-type="pre">e.g.</named-content></xref>, which can affect the hydrological cycle <xref ref-type="bibr" rid="bib1.bibx103" id="paren.3"><named-content content-type="pre">e.g.</named-content></xref> and atmospheric dynamics <xref ref-type="bibr" rid="bib1.bibx95" id="paren.4"><named-content content-type="pre">e.g.</named-content></xref>. Furthermore, volcanic air pollution events can lead to a severe and spatially widespread health hazard and increase excess mortality <xref ref-type="bibr" rid="bib1.bibx89" id="paren.5"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d1e542">For the aviation industry, ash and gas emissions from volcanic eruptions can pose a flight safety hazard. Flying through volcanic ash is a well-recognised hazard as it can reduce visibility, damage the exterior of the aircraft and compromise the functionality of aircraft engines. Ingestion of volcanic ash can cause engine failure and permanently damage jet engines <xref ref-type="bibr" rid="bib1.bibx15 bib1.bibx78 bib1.bibx79 bib1.bibx26" id="paren.6"/>. When sulfur dioxide (<inline-formula><mml:math id="M27" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) oxidises to sulfuric acid and upon hydration forms sulfuric acid aerosol particles <xref ref-type="bibr" rid="bib1.bibx34 bib1.bibx43" id="paren.7"><named-content content-type="pre">see e.g.</named-content></xref>, damage to the exterior of aircraft can occur (e.g. window crazing) <xref ref-type="bibr" rid="bib1.bibx5" id="paren.8"/>. Through sulfidation, <inline-formula><mml:math id="M28" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> can also cause serious damage to the interior of the engines. Sulfuric acid aerosol particles have been recorded to corrode nickel alloys in engine components (e.g. compressor blades) when alkali metal salts, like mineral dust or sea salt, are co-present <xref ref-type="bibr" rid="bib1.bibx28 bib1.bibx33" id="paren.9"/>. While this effect has not been linked to immediate engine failures, it is a concern for the aviation industry as it increases maintenance costs. Apart from material damage, sulfurous odours can also cause distress of cabin passengers and aircrew.</p>
      <p id="d1e582">The Raikoke volcano is located in the Kuril Island chain, near the Kamchatka Peninsula in Russia (48.3<inline-formula><mml:math id="M29" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153.2<inline-formula><mml:math id="M30" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E; see Fig. <xref ref-type="fig" rid="Ch1.F1"/>), and had been dormant since 1924. On 21 June 2019 at 18:05 UTC Raikoke started erupting, and multiple explosions were reported until 05:40 UTC on 22 June 2019 <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx41" id="paren.10"/>. During this period, Raikoke released the largest amount of <inline-formula><mml:math id="M31" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the stratosphere since the Nabro eruption in 2011 <xref ref-type="bibr" rid="bib1.bibx30" id="paren.11"/>. The volcanic cloud (while a geographic distribution of <inline-formula><mml:math id="M32" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and/or sulfate aerosol is not technically a cloud in the meteorological sense, we use this term through our paper as it is common practice in the atmospheric dispersion community) dispersed across the Northern Hemisphere (NH) within the first few weeks after the eruption and was observed by various ground-based observational networks <xref ref-type="bibr" rid="bib1.bibx104 bib1.bibx61" id="paren.12"><named-content content-type="pre">e.g.</named-content></xref>, aircraft-based instruments <xref ref-type="bibr" rid="bib1.bibx9" id="paren.13"><named-content content-type="pre">e.g.</named-content></xref> and satellites <xref ref-type="bibr" rid="bib1.bibx67 bib1.bibx45 bib1.bibx80 bib1.bibx53 bib1.bibx31" id="paren.14"><named-content content-type="pre">e.g.</named-content></xref> in the following months.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F1"><?xmltex \currentcnt{1}?><?xmltex \def\figurename{Figure}?><label>Figure 1</label><caption><p id="d1e652">Example of daily TROPOMI overpasses (north of 25<inline-formula><mml:math id="M33" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, with a swath width of 2600 km). Time indicates the approximate central time for each overpass (each track takes approximately 1.5–2 h). Note the overlap of the swaths, resulting in a higher temporal resolution near the pole. Also shown is the location of the Raikoke volcano (triangle) and the radiosonde location at the Petropavlovsk-Kamchatsky Airport (square).</p></caption>
        <?xmltex \igopts{width=199.169291pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f01.png"/>

      </fig>

      <p id="d1e670">The International Airways Volcano Watch (IAVW) is responsible for the dissemination of information on the occurrence of volcanic eruptions and associated volcanic ash clouds <xref ref-type="bibr" rid="bib1.bibx46" id="paren.15"/> through nine Volcanic Ash Advisory Centres (VAACs). During a volcanic eruption the responsible VAAC disseminates relevant information to the aviation sector regarding the geographic location of volcanic ash present in the atmosphere. Currently, the VAACs are only required to provide forecasts of volcanic ash dispersion, and therefore less development has been achieved on the forecasting of volcanic gas clouds. There is, however, increasing consensus among the scientific community that monitoring and simulating <inline-formula><mml:math id="M34" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds could be of interest to stakeholders, as volcanic <inline-formula><mml:math id="M35" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> can pose a public health hazard and potentially affect the aviation industry (e.g. increase of aircraft maintenance costs) <xref ref-type="bibr" rid="bib1.bibx116 bib1.bibx91 bib1.bibx11 bib1.bibx32 bib1.bibx33" id="paren.16"/>. Volcanic <inline-formula><mml:math id="M36" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds are also frequently (but not always) co-located with ash clouds. Detecting ash clouds from satellites<?pagebreak page10853?> retrievals remains a challenging task, and in some circumstances <inline-formula><mml:math id="M37" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds may act as proxies for ash clouds <xref ref-type="bibr" rid="bib1.bibx12 bib1.bibx102 bib1.bibx94 bib1.bibx57" id="paren.17"><named-content content-type="pre">e.g.</named-content></xref>. As a result, the latest roadmap published by the IAVW <xref ref-type="bibr" rid="bib1.bibx47" id="paren.18"/> includes <inline-formula><mml:math id="M38" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> forecasts as a core item to be implemented in the future.</p>
      <p id="d1e743">The main tools used by VAACs to provide accurate forecasts of volcanic cloud characteristics are atmospheric dispersion models (ADMs), which are numerical models that simulate how air parcels disperse within the atmosphere. ADMs are used for a large variety of advection-related research, including dust transport, nuclear accidents, forest fires, air pollution, plant diseases and volcanic clouds <xref ref-type="bibr" rid="bib1.bibx14 bib1.bibx110 bib1.bibx52 bib1.bibx91 bib1.bibx92 bib1.bibx3 bib1.bibx62 bib1.bibx72" id="paren.19"/>. Because of the ash-focused task of VAACs, there has been a strong research focus on improving the simulation of volcanic ash in ADMs and measuring volcanic ash using in situ and satellite measurement techniques <xref ref-type="bibr" rid="bib1.bibx118 bib1.bibx17 bib1.bibx77 bib1.bibx66 bib1.bibx36 bib1.bibx112" id="paren.20"><named-content content-type="pre">e.g.</named-content></xref>. The skill of ADMs in simulating the evolution of <inline-formula><mml:math id="M39" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds has also been investigated <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx40 bib1.bibx6 bib1.bibx92" id="paren.21"><named-content content-type="pre">e.g.</named-content></xref> but to a much lesser extent as this has generally been the realm of global climate models interested in the climatic impacts of the periodic stratospheric injections from volcanoes <xref ref-type="bibr" rid="bib1.bibx39 bib1.bibx96 bib1.bibx93" id="paren.22"><named-content content-type="pre">e.g.</named-content></xref>.</p>
      <p id="d1e775">Observations are vital in determining the skill of the dispersion models. While in situ observations are available for several well-studied volcanoes <xref ref-type="bibr" rid="bib1.bibx75 bib1.bibx88 bib1.bibx114" id="paren.23"><named-content content-type="pre">e.g.</named-content></xref>, they are only available for a limited number of locations. In recent decades, many high-resolution remote-sensing measurements have become available, providing a great data source on activity at even the most remote volcanoes across the globe. A large number of satellites now measure atmospheric <inline-formula><mml:math id="M40" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, with each newly launched instrument having an increased accuracy (see for example Fig. 2 in <xref ref-type="bibr" rid="bib1.bibx100" id="altparen.24"/>). The TROPOspheric Monitoring Instrument (TROPOMI) has been operational since the end of 2017 and  retrieves atmospheric <inline-formula><mml:math id="M41" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> total column densities at an unprecedented spatial resolution for UV measurements (up to 3.5 km <inline-formula><mml:math id="M42" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5.5 km at nadir) <xref ref-type="bibr" rid="bib1.bibx98 bib1.bibx100" id="paren.25"/>. TROPOMI therefore provides a useful source of information to evaluate model simulations of <inline-formula><mml:math id="M43" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds using ADMs (and climate models).</p>
      <p id="d1e830">One major issue for the development of ADMs for volcanic clouds is the relatively small number of large-magnitude eruptions available since the start of the satellite era in 1979 in order to validate model output. While small-magnitude eruptions take place more frequently, large-magnitude eruptions that can emit large amounts of <inline-formula><mml:math id="M44" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the stratosphere are much more sporadic <xref ref-type="bibr" rid="bib1.bibx81 bib1.bibx63 bib1.bibx13 bib1.bibx93" id="paren.26"><named-content content-type="pre">e.g.</named-content></xref>. The 2019 Raikoke eruption is the first eruption with <inline-formula><mml:math id="M45" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions in excess of 1 Tg of <inline-formula><mml:math id="M46" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> that has been observed by the TROPOMI instrument. Due to the amount of <inline-formula><mml:math id="M47" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emitted into the stratosphere, it provides an ideal test case to validate the skill of the Numerical Atmospheric-dispersion Modelling Environment (NAME) <xref ref-type="bibr" rid="bib1.bibx49" id="paren.27"/>, which is the dispersion model used by the London VAAC <xref ref-type="bibr" rid="bib1.bibx117" id="paren.28"/>. In this paper we will focus on the evolution of the volcanic <inline-formula><mml:math id="M48" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud during the first 3 weeks after the 2019 Raikoke eruption and compare the output from NAME with the TROPOMI and the Infrared Atmospheric Sounding Interferometer (IASI) satellite <inline-formula><mml:math id="M49" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products. In the accompanying Part 2 paper <xref ref-type="bibr" rid="bib1.bibx73" id="paren.29"/>, a detailed assessment of the sulfate aerosol together with volcanic ash from this eruption is discussed as well as the effects from biomass burning aerosols that were emitted into the stratosphere from an unusually strong pyrocumulus event in continental North America.</p>
      <p id="d1e914">The paper is structured as follows: after discussing the TROPOMI and the IASI satellite <inline-formula><mml:math id="M50" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products in Sect. 2.1 and 2.2, we briefly introduce all the relevant aspects of the NAME dispersion model in Sect. 2.3, including the eruption source parameters. Using the introduced input parameters for our 25 d long NAME simulations, we obtain a good qualitative comparison of the simulated <inline-formula><mml:math id="M51" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud with the TROPOMI satellite <inline-formula><mml:math id="M52" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products during the first 3 weeks after the eruption, which we present in Sect. 3.1. A more detailed analysis of the model skill is presented in Sect. 3.2 and 3.3, where we show that the fractional skill score (FSS) and the structure, amplitude and location (SAL) metric (both metrics are introduced in Sect. 2.4) are powerful tools for assessing the skill of the model simulations in comparison to satellite measurements. The NAME simulation skill in terms of the NH-mean <inline-formula><mml:math id="M53" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden throughout the first 25 d after the Raikoke eruption is presented in Sect. 3.4, showing a large dependence of the mass burden evolution on the vertical emission profile. We finish with a discussion of our work (Sect. 4) and present the main conclusions in Sect. 5.</p>
</sec>
<sec id="Ch1.S2">
  <label>2</label><title>Data and methods</title>
<sec id="Ch1.S2.SS1">
  <label>2.1</label><title>TROPOspheric monitoring instrument</title>
      <?pagebreak page10854?><p id="d1e976">TROPOMI is part of the ESA's S5P satellite launched on 13 October 2017 <xref ref-type="bibr" rid="bib1.bibx105" id="paren.30"/> and is a polar-orbiting, sun-synchronous, hyperspectral spectrometer that measures Earth-reflected radiances in the ultraviolet (UV), visible, near-infrared and shortwave infrared parts of the spectrum. Atmospheric <inline-formula><mml:math id="M54" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> vertical column density (VCD, expressed in Dobson units with 1 DU  <inline-formula><mml:math id="M55" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> <inline-formula><mml:math id="M56" display="inline"><mml:mrow><mml:mn mathvariant="normal">2.69</mml:mn><mml:mo>×</mml:mo><mml:msup><mml:mn mathvariant="normal">10</mml:mn><mml:mn mathvariant="normal">16</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> molec cm<inline-formula><mml:math id="M57" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) is retrieved by applying differential optical absorption spectroscopy (DOAS) <xref ref-type="bibr" rid="bib1.bibx76" id="paren.31"/> to the measured ultraviolet spectra in three wavelength ranges (312–326, 325–335 and 360–390 nm). For a more detailed description of the <inline-formula><mml:math id="M58" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrieval, we refer the reader to <xref ref-type="bibr" rid="bib1.bibx98 bib1.bibx99" id="text.32"/>.</p>
      <p id="d1e1045">In our study we use the TROPOMI satellite retrievals across the NH (north of 25<inline-formula><mml:math id="M59" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>  N) that cover the Raikoke <inline-formula><mml:math id="M60" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud between 22 June and 15 July 2019. Figure <xref ref-type="fig" rid="Ch1.F1"/> shows an example of the TROPOMI daily overpasses over the NH. Compared to its predecessors OMI and SCIAMACHY, TROPOMI has a higher horizontal pixel resolution (up to 3.5 km <inline-formula><mml:math id="M61" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 5.5 km), allowing for a more detailed characterisation of the small-scale features in volcanic <inline-formula><mml:math id="M62" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds <xref ref-type="bibr" rid="bib1.bibx100" id="paren.33"/>. The retrieved TROPOMI <inline-formula><mml:math id="M63" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD product is calculated by accounting for a large number of parameters, such as meteorological cloud fraction, surface albedo and the vertical distribution of absorbing trace gases (e.g. ozone) <xref ref-type="bibr" rid="bib1.bibx98 bib1.bibx99" id="paren.34"/>. As a result, the <inline-formula><mml:math id="M64" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals from TROPOMI are sensitive to many assumptions, which can lead to uncertainties of up to <inline-formula><mml:math id="M65" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">50</mml:mn></mml:mrow></mml:math></inline-formula> %. For <inline-formula><mml:math id="M66" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the stratosphere, the sum of the various uncertainties can be approximated to be around <inline-formula><mml:math id="M67" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">30</mml:mn></mml:mrow></mml:math></inline-formula> % of the retrieved <inline-formula><mml:math id="M68" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. For a detailed discussion of the retrieval uncertainties, see <xref ref-type="bibr" rid="bib1.bibx98" id="text.35"/>.</p>
      <p id="d1e1163">One of the largest uncertainties of the TROPOMI <inline-formula><mml:math id="M69" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD product is the height of the <inline-formula><mml:math id="M70" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud. However, the sensitivity of the measurement with height is well characterised. To account for this sensitivity, the TROPOMI <inline-formula><mml:math id="M71" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD level 2 products are publicly available from the ESA website (<uri>https://s5phub.copernicus.eu</uri>, last access: 22 March 2021) for three different scenarios where the <inline-formula><mml:math id="M72" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> layer is assumed to be at either 1, 7 or 15 km a.s.l. (above sea level). The TROPOMI VCD data presented in this study are for an <inline-formula><mml:math id="M73" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> layer at 15 km a.s.l., as this is the height nearest to the estimated weight-averaged emission height for the Raikoke eruption (see e.g. Fig. <xref ref-type="fig" rid="Ch1.F2"/>).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F2"><?xmltex \currentcnt{2}?><?xmltex \def\figurename{Figure}?><label>Figure 2</label><caption><p id="d1e1230">Estimated total emitted <inline-formula><mml:math id="M74" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass for the Raikoke eruption between 21 June 2019 18:00 UTC and 22 June 2019 03:00 UTC. The initial emission profile was provided by the VolRes (Volcano Response) team, which is implemented in NAME for the 1.5 Tg <inline-formula><mml:math id="M75" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> simulation (VolRes1.5, orange). We also simulated the same profile for a 2.0 Tg <inline-formula><mml:math id="M76" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission (VolRes2.0, red). Also included is a new emission profile estimate (StratProfile, brown) based on the TROPOMI <inline-formula><mml:math id="M77" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD cloud on 23 June (see Sect. 2.3.4). This profile has a similar total mass emitted to VolRes1.5, but a larger fraction (69% instead of 43%) of its mass is emitted in the stratosphere (see Table <xref ref-type="table" rid="Ch1.T2"/>). The grey line represents the average tropopause height in the MetUM during the first 36 h after the eruption at the location of the Raikoke volcano. The blue line and shading represents the average and the range of measured tropopause heights by the radiosondes released from the Petropavlovsk-Kamchatsky Airport (square in Fig. <xref ref-type="fig" rid="Ch1.F1"/>) during the first 36 h after the eruption.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f02.png"/>

        </fig>

      <p id="d1e1288">In order to compare the available satellite retrievals with any atmospheric dispersion model output, one needs to apply the column averaging kernel (AK) operators to the model data, thereby matching the model-simulated <inline-formula><mml:math id="M78" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs to the TROPOMI products. The pre-calculated AKs for the 15 km scenario <xref ref-type="bibr" rid="bib1.bibx99" id="paren.36"/> have been applied to the NAME model output. We have repeated the analysis using the AKs and TROPOMI VCDs assuming the <inline-formula><mml:math id="M79" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> layer at 7 km a.s.l., which affects the absolute <inline-formula><mml:math id="M80" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs (not shown) but not our interpretation of the results or our overall conclusions.</p>
      <p id="d1e1327">To obtain a daily <inline-formula><mml:math id="M81" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimate from the TROPOMI measurements, we grid the satellite data and combine all the overpasses during a 24 h period starting at 12:00 UTC of any given day. In the case of multiple overpasses over a single location, we average the <inline-formula><mml:math id="M82" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud at these grid locations to avoid double counting. For the mass estimate from TROPOMI we have used a detection threshold of 0.3 DU <xref ref-type="bibr" rid="bib1.bibx101" id="paren.37"/>. The resulting <inline-formula><mml:math id="M83" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD (in DU) is then converted into a mass (Tg) by using the area of each individual grid point and the molar mass of <inline-formula><mml:math id="M84" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. Due to the high spatial resolution of the TROPOMI retrieval (on average 9 TROPOMI pixels per output grid cell for the resolution used in the dispersion model), we have downscaled the final TROPOMI retrievals to the output grid resolution of the NAME dispersion model by averaging the <inline-formula><mml:math id="M85" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs of all pixels within each NAME grid cell (0.2<inline-formula><mml:math id="M86" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude <inline-formula><mml:math id="M87" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 0.4<inline-formula><mml:math id="M88" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude). Unless otherwise specified, we refer to the sulfur dioxide mass burden as the total <inline-formula><mml:math id="M89" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass within the NH, north of 25<inline-formula><mml:math id="M90" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p>
      <p id="d1e1434">During the initial stage of the eruption, it is likely that TROPOMI underestimates the <inline-formula><mml:math id="M91" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs due to the presence of volcanic ash <xref ref-type="bibr" rid="bib1.bibx119" id="paren.38"><named-content content-type="pre">e.g.</named-content></xref>. To understand if ash interference is likely to have affected our <inline-formula><mml:math id="M92" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> estimates, we also retrieve the absorbing aerosol index (AAI) from the TROPOMI instrument <xref ref-type="bibr" rid="bib1.bibx120" id="paren.39"/>. Although the TROPOMI AAI product should be used with care due to its sensitivity to for example cloud height and optical thickness <xref ref-type="bibr" rid="bib1.bibx23 bib1.bibx55" id="paren.40"><named-content content-type="pre">see e.g.</named-content></xref>, high index values (<inline-formula><mml:math id="M93" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>) indicate the presence of aerosol plumes from dust outbreaks, volcanic ash and biomass burning. During the first 48 h after the eruption we found high peak AAI values within the volcanic cloud (<inline-formula><mml:math id="M94" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">18.9</mml:mn></mml:mrow></mml:math></inline-formula> on the 22 June and <inline-formula><mml:math id="M95" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">3.5</mml:mn></mml:mrow></mml:math></inline-formula> on the 23 June), indicating that volcanic ash had an impact on the <inline-formula><mml:math id="M96" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrieval during this period.</p>
</sec>
<?pagebreak page10855?><sec id="Ch1.S2.SS2">
  <label>2.2</label><title>The infrared atmospheric sounding interferometer</title>
      <p id="d1e1522">The second satellite <inline-formula><mml:math id="M97" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> dataset used in our analysis is acquired using IASI aboard the MetOp-A and MetOp-B satellites. These satellites operate in tandem on a polar orbit with a field of view (FOV) consisting of four circular footprints of 12 km diameter (at nadir) inside a square of
50 km <inline-formula><mml:math id="M98" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 50 km and provide a global coverage twice a day. For our analysis we use the <inline-formula><mml:math id="M99" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> plume height estimates based on the IASI data, which are produced by applying the retrieval algorithm presented in <xref ref-type="bibr" rid="bib1.bibx10 bib1.bibx11" id="text.41"/>. The IASI instrument also retrieves the <inline-formula><mml:math id="M100" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs within the volcanic plume but uses a different set of assumptions in the retrieval algorithm compared to TROPOMI (e.g. IASI retrieves the plume height which affects the <inline-formula><mml:math id="M101" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD; the retrieved IASI plume height can be different from the plume heights assumed in the TROPOMI product, and therefore the <inline-formula><mml:math id="M102" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from the two methods are not equivalent). To compare <inline-formula><mml:math id="M103" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from NAME to the IASI data, one would therefore also need to apply a different scaling (i.e. AK). As the TROPOMI and IASI retrieval assumptions and limitations are satellite-specific (for example, TROPOMI might detect <inline-formula><mml:math id="M104" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> closer to the surface than IASI due to the presence of water vapour), a comparison between the two <inline-formula><mml:math id="M105" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD products is not straightforward and is not attempted here. While it would be an interesting exercise to apply our analysis also to the IASI data, we focus on the comparison of NAME with the TROPOMI <inline-formula><mml:math id="M106" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> estimates, and therefore no further analysis is done for the IASI <inline-formula><mml:math id="M107" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD retrievals.</p>
</sec>
<sec id="Ch1.S2.SS3">
  <label>2.3</label><title>Numerical Atmospheric-dispersion Modelling Environment (NAME)</title>
      <p id="d1e1655">The Numerical Atmospheric-dispersion Modelling Environment (NAME) is a Lagrangian model developed by the Met Office <xref ref-type="bibr" rid="bib1.bibx49" id="paren.42"/> and is the operational dispersion model used by the London VAAC to forecast the dispersion of volcanic clouds within European airspace (e.g. the Icelandic eruptions of Eyjafjallajökull in 2010 and Holuhraun in 2014–2015). For our work we use NAME version 8.1. The model can trace both ash particles and gases through the atmosphere and includes chemistry parameterisations that allow the conversion of <inline-formula><mml:math id="M108" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into sulfate aerosols (<inline-formula><mml:math id="M109" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) within the volcanic cloud (see Sect. 2.3.3). There is no radiative or chemical interaction between the ash particles and the sulfur species in NAME; the ash particles and sulfate aerosols are thus considered to be externally mixed. In this section we focus on the dispersion of <inline-formula><mml:math id="M110" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and highlight the important aspects of NAME for this part of the research. More details on the modelling of ash particles within the model are discussed in the accompanying Part 2 paper <xref ref-type="bibr" rid="bib1.bibx73" id="paren.43"/>.</p><?xmltex \hack{\newpage}?>
<sec id="Ch1.S2.SS3.SSS1">
  <label>2.3.1</label><title>Simulating volcanic cloud dispersion using NAME</title>
      <p id="d1e1705">Simulating the dispersion of a volcanic cloud with NAME relies on the tracing of air parcels through the atmosphere, each containing an ash, <inline-formula><mml:math id="M111" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and/or <inline-formula><mml:math id="M112" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass. These air parcels are released from the source location (volcano), where the user has to define the eruption source parameters (see Sect. 2.3.4). NAME is an offline model; therefore, each parcel is advected by an externally obtained wind field (e.g. a high-resolution Numerical Weather Prediction (NWP) model). In our simulations, we use the wind fields from the latest global analysis of the Met Office Unified Model (MetUM), which have a horizontal resolution of around 10 km at mid-latitudes, 59 levels between the surface and 30 km a.s.l. (decreasing vertical resolution with altitude, with approximately 600 m resolution at tropopause height), and a 3-hourly temporal resolution. The path of each trajectory is calculated using the following equation:
              <disp-formula id="Ch1.E1" content-type="numbered"><label>1</label><mml:math id="M113" display="block"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>=</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:mo>[</mml:mo><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>+</mml:mo><mml:msup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo><mml:mo>]</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M114" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the location of the parcel at time <inline-formula><mml:math id="M115" display="inline"><mml:mi>t</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M116" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the new location of the parcel at time <inline-formula><mml:math id="M117" display="inline"><mml:mrow><mml:mi>t</mml:mi><mml:mo>+</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:math></inline-formula>, <inline-formula><mml:math id="M118" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> is the 3D-wind vector at location <inline-formula><mml:math id="M119" display="inline"><mml:mrow><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M120" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>′</mml:mo></mml:msup><mml:mo>(</mml:mo><mml:mi mathvariant="bold-italic">x</mml:mi><mml:mo>(</mml:mo><mml:mi>t</mml:mi><mml:mo>)</mml:mo><mml:mo>)</mml:mo></mml:mrow></mml:math></inline-formula> represents a stochastic perturbation to the parcel trajectory representing turbulence and unresolved sub-grid mesoscale wind variations in the dispersion model. In NAME, <inline-formula><mml:math id="M121" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mo>′</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> consists of two parts representing atmospheric turbulence (<inline-formula><mml:math id="M122" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mi mathvariant="normal">turb</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>) and sub-grid mesoscale diffusion (<inline-formula><mml:math id="M123" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mi mathvariant="normal">meso</mml:mi><mml:mo>′</mml:mo></mml:msubsup></mml:mrow></mml:math></inline-formula>). The turbulence part represents the stochastic motions from the air parcels due to small-scale perturbations. The mesoscale diffusion represents the horizontal mesoscale motions in the atmosphere that are not captured by the resolution of the used NWP model. Each NWP model has a limited spatial and temporal resolution, and as a result part of the mesoscale features (e.g. eddies) are not captured by the NWP wind field provided. Both the turbulence and mesoscale diffusion within the free atmosphere (excluding the planetary boundary layer, which has a more detailed scheme; <xref ref-type="bibr" rid="bib1.bibx111" id="altparen.44"/>) are calculated using

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M124" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E2"><mml:mtd><mml:mtext>2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msubsup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mi mathvariant="normal">turb</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mi>d</mml:mi><mml:msqrt><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msqrt><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E3"><mml:mtd><mml:mtext>3</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msubsup><mml:mi mathvariant="bold-italic">u</mml:mi><mml:mi mathvariant="normal">meso</mml:mi><mml:mo>′</mml:mo></mml:msubsup><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi><mml:mo>=</mml:mo><mml:mi>d</mml:mi><mml:msqrt><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub><mml:mo>⋅</mml:mo><mml:mi mathvariant="normal">Δ</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:msqrt><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E4"><mml:mtd><mml:mtext>4</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi>x</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mfenced open="(" close=")"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>u</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>u</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>v</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>v</mml:mi></mml:msub><mml:mo>,</mml:mo><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              where <inline-formula><mml:math id="M125" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi>x</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is a 3D-diffusion vector defined separately for both components, using typical values for the standard deviation of the velocity (<inline-formula><mml:math id="M126" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula>) and typical time length scales (<inline-formula><mml:math id="M127" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula>). <inline-formula><mml:math id="M128" display="inline"><mml:mi>d</mml:mi></mml:math></inline-formula> represents a random number from a top-hat distribution within the range [<inline-formula><mml:math id="M129" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>, 1]. The values for <inline-formula><mml:math id="M130" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M131" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> are dependent on the NWP model used, as they are impacted by the resolution of the model <xref ref-type="bibr" rid="bib1.bibx36 bib1.bibx111" id="paren.45"/>. The values for <inline-formula><mml:math id="M132" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M133" display="inline"><mml:mi mathvariant="italic">τ</mml:mi></mml:math></inline-formula> used in this study are obtained from the analysis done by <xref ref-type="bibr" rid="bib1.bibx111" id="text.46"/> and are shown in Table <xref ref-type="table" rid="Ch1.T1"/>. Note that for <inline-formula><mml:math id="M134" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> the vertical component (<inline-formula><mml:math id="M135" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) is zero.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T1"><?xmltex \currentcnt{1}?><label>Table 1</label><caption><p id="d1e2225">The values for the diffusion parameter <inline-formula><mml:math id="M136" display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> used in NAME. Values are NWP dependent and are given here for the Met Office Unified Model global analysis (10 km horizontal resolution, 59 levels) with a 3-hourly temporal resolution. Values for <inline-formula><mml:math id="M137" display="inline"><mml:mrow><mml:msup><mml:mi mathvariant="italic">σ</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:mrow></mml:math></inline-formula> are given instead of <inline-formula><mml:math id="M138" display="inline"><mml:mi mathvariant="italic">σ</mml:mi></mml:math></inline-formula> to be consistent with the values presented by <xref ref-type="bibr" rid="bib1.bibx111" id="text.47"/>. Values are given for both the turbulence <inline-formula><mml:math id="M139" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> and the mesoscale diffusion <inline-formula><mml:math id="M140" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> that are used in NAME for the free atmosphere (i.e. excluding the boundary layer).</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.92}[.92]?><oasis:tgroup cols="6">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry namest="col1" nameend="col6" align="center">Global MetUM analysis (<inline-formula><mml:math id="M141" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.140625</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.09375</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>, 59 levels, </oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col6" align="center">3-hourly resolution) </oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"><inline-formula><mml:math id="M142" display="inline"><mml:mi>K</mml:mi></mml:math></inline-formula> (m<inline-formula><mml:math id="M143" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M144" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col3"><inline-formula><mml:math id="M145" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi></mml:mrow><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col4"><inline-formula><mml:math id="M146" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mrow><mml:mi>u</mml:mi><mml:mo>,</mml:mo><mml:mi>v</mml:mi></mml:mrow></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M147" display="inline"><mml:mrow><mml:msubsup><mml:mi mathvariant="italic">σ</mml:mi><mml:mi>w</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col6"><inline-formula><mml:math id="M148" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="italic">τ</mml:mi><mml:mi>w</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2"/>
         <oasis:entry colname="col3">(m<inline-formula><mml:math id="M149" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M150" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col4">(s)</oasis:entry>
         <oasis:entry colname="col5">(m<inline-formula><mml:math id="M151" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M152" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>)</oasis:entry>
         <oasis:entry colname="col6">(s)</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M153" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">(18.75, 18.75, 1)</oasis:entry>
         <oasis:entry colname="col3">0.0625</oasis:entry>
         <oasis:entry colname="col4">300</oasis:entry>
         <oasis:entry colname="col5">0.01</oasis:entry>
         <oasis:entry colname="col6">100</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1"><inline-formula><mml:math id="M154" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">(6400, 6400, 0)</oasis:entry>
         <oasis:entry colname="col3">0.64</oasis:entry>
         <oasis:entry colname="col4">10 000</oasis:entry>
         <oasis:entry colname="col5">0</oasis:entry>
         <oasis:entry colname="col6">0</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

      <?pagebreak page10856?><p id="d1e2557"><?xmltex \hack{\newpage}?>Accurately describing atmospheric dispersion due to mixing is a complex three-dimensional problem <xref ref-type="bibr" rid="bib1.bibx108 bib1.bibx37 bib1.bibx38 bib1.bibx42 bib1.bibx107" id="paren.48"><named-content content-type="pre">e.g.</named-content></xref>. TROPOMI satellite retrievals provide <inline-formula><mml:math id="M155" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs, and therefore our information on mixing effects of the <inline-formula><mml:math id="M156" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud is limited to their horizontal impact. Studies by <xref ref-type="bibr" rid="bib1.bibx4" id="text.49"/> and <xref ref-type="bibr" rid="bib1.bibx37" id="text.50"/> have shown that the vertical and horizontal components of stratospheric mixing are related, which allowed them to derive an effective horizontal diffusion from observations. Values reported in the literature for horizontal diffusion coefficients in the lower stratosphere vary over an order of magnitude (10<inline-formula><mml:math id="M157" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">3</mml:mn></mml:msup></mml:math></inline-formula>–10<inline-formula><mml:math id="M158" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">5</mml:mn></mml:msup></mml:math></inline-formula> m<inline-formula><mml:math id="M159" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> s<inline-formula><mml:math id="M160" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and also depend on the resolution of the NWP data used  <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx108 bib1.bibx36 bib1.bibx107" id="paren.51"><named-content content-type="pre">e.g.</named-content></xref>. To investigate the importance of the horizontal mesoscale diffusion parameter, we present two sensitivity simulations with two different <inline-formula><mml:math id="M161" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions profiles (see Sect. 2.3.4 for discussion of these profiles) and a reduced value for <inline-formula><mml:math id="M162" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> (see Table <xref ref-type="table" rid="Ch1.T2"/>). We decided to only change the <inline-formula><mml:math id="M163" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> parameter, as the horizontal <inline-formula><mml:math id="M164" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">turb</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> components (see Table <xref ref-type="table" rid="Ch1.T1"/>) are at least an order of magnitude smaller than the <inline-formula><mml:math id="M165" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> components, and thus changing them would not show any significant impact on our initial results that is not captured by changing <inline-formula><mml:math id="M166" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>. The simulations with a reduced value for <inline-formula><mml:math id="M167" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> are indicated by the subscript <inline-formula><mml:math id="M168" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> throughout this study. Due to the large range of potential realistic <inline-formula><mml:math id="M169" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values, we have stepwise reduced the parameter and found the best results for a 75 % reduction, which is the value presented in this paper and is similar to the values reported by <xref ref-type="bibr" rid="bib1.bibx4" id="text.52"/> and <xref ref-type="bibr" rid="bib1.bibx108" id="text.53"/>.</p>

<?xmltex \floatpos{t}?><table-wrap id="Ch1.T2"><?xmltex \currentcnt{2}?><label>Table 2</label><caption><p id="d1e2752">Overview of the NAME simulations performed using different emission profiles and a reduced mesoscale diffusion (values for <inline-formula><mml:math id="M170" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> can be found in Table <xref ref-type="table" rid="Ch1.T1"/>). Also shown is the estimated mass emitted into the stratosphere. For the actual vertical emission profiles, see Fig. <xref ref-type="fig" rid="Ch1.F2"/>. All the simulations use the same NWP data input (Global MetUM), the same emission location (48.3<inline-formula><mml:math id="M171" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153.2<inline-formula><mml:math id="M172" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), and duration between 21 June 2019 18:00 UTC–22 June 2019 03:00 UTC. The simulation domain is the NH between 25–90<inline-formula><mml:math id="M173" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N and the simulation length is 25 d.</p></caption><oasis:table frame="topbot"><?xmltex \begin{scaleboxenv}{.92}[.92]?><oasis:tgroup cols="5">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="right"/>
     <oasis:colspec colnum="3" colname="col3" align="left"/>
     <oasis:colspec colnum="4" colname="col4" align="center"/>
     <oasis:colspec colnum="5" colname="col5" align="left"/>
     <oasis:thead>
       <oasis:row>
         <oasis:entry colname="col1">Simulation</oasis:entry>
         <oasis:entry colname="col2">Mass</oasis:entry>
         <oasis:entry colname="col3">Profile</oasis:entry>
         <oasis:entry colname="col4">Mass</oasis:entry>
         <oasis:entry colname="col5">Mesoscale</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">name</oasis:entry>
         <oasis:entry colname="col2">emitted</oasis:entry>
         <oasis:entry colname="col3">used</oasis:entry>
         <oasis:entry colname="col4">stratosphere</oasis:entry>
         <oasis:entry colname="col5">diffusion</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5</oasis:entry>
         <oasis:entry colname="col2">1.5 Tg</oasis:entry>
         <oasis:entry colname="col3">VolRes1.5</oasis:entry>
         <oasis:entry colname="col4">0.64 Tg</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M174" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes2.0</oasis:entry>
         <oasis:entry colname="col2">2.0 Tg</oasis:entry>
         <oasis:entry colname="col3">VolRes2.0</oasis:entry>
         <oasis:entry colname="col4">0.85 Tg</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M175" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile</oasis:entry>
         <oasis:entry colname="col2">1.57 Tg</oasis:entry>
         <oasis:entry colname="col3">StratProfile</oasis:entry>
         <oasis:entry colname="col4">1.09 Tg</oasis:entry>
         <oasis:entry colname="col5"><inline-formula><mml:math id="M176" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5<inline-formula><mml:math id="M177" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.5 Tg</oasis:entry>
         <oasis:entry colname="col3">VolRes1.5</oasis:entry>
         <oasis:entry colname="col4">0.64 Tg</oasis:entry>
         <oasis:entry colname="col5">0.25 <inline-formula><mml:math id="M178" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile<inline-formula><mml:math id="M179" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">1.57 Tg</oasis:entry>
         <oasis:entry colname="col3">StratProfile</oasis:entry>
         <oasis:entry colname="col4">1.09 Tg</oasis:entry>
         <oasis:entry colname="col5">0.25 <inline-formula><mml:math id="M180" display="inline"><mml:mrow><mml:msub><mml:mi>K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula></oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup><?xmltex \end{scaleboxenv}?></oasis:table></table-wrap>

</sec>
<sec id="Ch1.S2.SS3.SSS2">
  <label>2.3.2</label><?xmltex \opttitle{Calculating {$\protect\chem{SO_{{2}}}$} mass estimates from NAME}?><title>Calculating <inline-formula><mml:math id="M181" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimates from NAME</title>
      <p id="d1e3029">In our simulations, the <inline-formula><mml:math id="M182" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations (kg m<inline-formula><mml:math id="M183" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) from all the individual air parcels in NAME are presented as hourly means on a regular latitude–longitude grid by calculating the total mass of the <inline-formula><mml:math id="M184" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> of all parcels in each grid box every hour. The NAME output is calculated using a grid size of 0.2<inline-formula><mml:math id="M185" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude and 0.4<inline-formula><mml:math id="M186" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude (approximately 20 km <inline-formula><mml:math id="M187" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> 20 km at the latitude of the Raikoke volcano). The vertical resolution of the output is 500 m up to 15 km a.s.l. and 1 km resolution up to 20 km a.s.l., giving a total of 35 levels.</p>
      <p id="d1e3092">To compare the daily <inline-formula><mml:math id="M188" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimates from NAME and TROPOMI, we select the hourly NAME output corresponding to each individual TROPOMI overpass time and select only the grid boxes in NAME that are in the domain scanned by TROPOMI during that overpass. To calculate the <inline-formula><mml:math id="M189" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD, we apply the corresponding column AK operators obtained from TROPOMI (see Sect. 2.1) to each grid cell of the NAME output. Then for each column on the NAME output grid, the <inline-formula><mml:math id="M190" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations (kg m<inline-formula><mml:math id="M191" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in each grid cell are vertically integrated to obtain the <inline-formula><mml:math id="M192" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD estimate from NAME.</p>
      <p id="d1e3151">In all our NAME simulations we found that the <inline-formula><mml:math id="M193" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud is more diffuse than observed by TROPOMI. Therefore, removing all <inline-formula><mml:math id="M194" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs <inline-formula><mml:math id="M195" display="inline"><mml:mo>&lt;</mml:mo></mml:math></inline-formula> 0.3 DU in NAME (which is the detection threshold we have used for TROPOMI; see Sect. 2.1) from the simulations would result in a negative bias within the NAME simulation mass estimates that are not related to the evolution of the cloud but due to the stronger diffusion within the model. Therefore we have not included a detection threshold when determining the <inline-formula><mml:math id="M196" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimates for the NAME simulations. Similarly to the TROPOMI estimate, the daily mass estimates from NAME are calculated during a 24 h period starting at 12:00 UTC on any given day. The <inline-formula><mml:math id="M197" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden is defined as the total <inline-formula><mml:math id="M198" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass (Tg) within the NH, north of 25<inline-formula><mml:math id="M199" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS3">
  <label>2.3.3</label><title>Chemistry within NAME</title>
      <?pagebreak page10857?><p id="d1e3235">NAME contains an atmospheric chemistry scheme <xref ref-type="bibr" rid="bib1.bibx83" id="paren.54"/>. The relevant chemistry for volcanic clouds is related to the conversion of <inline-formula><mml:math id="M200" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into sulfate (<inline-formula><mml:math id="M201" display="inline"><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow></mml:math></inline-formula>). NAME accounts for the oxidation of <inline-formula><mml:math id="M202" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the gas phase using the following reaction:

              <disp-formula id="Ch1.R5" content-type="numbered reaction"><label>R1</label><mml:math id="M203" display="block"><mml:mrow><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mi>M</mml:mi><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mi>M</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:math></disp-formula>
            where <inline-formula><mml:math id="M204" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is then rapidly oxidised to <inline-formula><mml:math id="M205" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> on formation. When water is present in the atmosphere, the oxidation can happen in the aqueous phase by both <inline-formula><mml:math id="M206" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M207" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through the following reaction:

                  <disp-formula specific-use="align" content-type="numbered reaction"><mml:math id="M208" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R6"><mml:mtd><mml:mtext>R2</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>⇌</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R7"><mml:mtd><mml:mtext>R3</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>⇌</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              which is followed by

                  <disp-formula specific-use="align" content-type="numbered reaction"><mml:math id="M209" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.R8"><mml:mtd><mml:mtext>R4</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:mi mathvariant="normal">O</mml:mi></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R9"><mml:mtd><mml:mtext>R5</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">HSO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mo>-</mml:mo></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msup><mml:mi mathvariant="normal">H</mml:mi><mml:mo>+</mml:mo></mml:msup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.R10"><mml:mtd><mml:mtext>R6</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">3</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow><mml:mo>→</mml:mo><mml:mrow class="chem"><mml:msubsup><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn><mml:mrow><mml:mn mathvariant="normal">2</mml:mn><mml:mo>-</mml:mo></mml:mrow></mml:msubsup></mml:mrow><mml:mo>+</mml:mo><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              Reactions (R2)–(R6) dominate in cloudy conditions and only occur in model grid boxes when both the meteorological cloud fraction and liquid water content are non-zero. The concentrations of <inline-formula><mml:math id="M210" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">H</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M211" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">O</mml:mi><mml:mn mathvariant="normal">3</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the atmosphere are pre-defined in the NAME model by using monthly mean background fields obtained from a historical Unified Model coupled to the United Kingdom Chemistry and Aerosol model (UM-UKCA model) simulation that have been smoothed between months using interpolation.</p>
      <p id="d1e3666">In NAME the <inline-formula><mml:math id="M212" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and sulfate aerosol particles can be removed through dry and wet deposition. For our simulations we found that the dry deposition had limited importance for the 2019 Raikoke eruption as most of the volcanic clouds are at high altitudes. Wet deposition in NAME is calculated using a standard depletion equation:


                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M213" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E11"><mml:mtd><mml:mtext>5</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>C</mml:mi></mml:mrow><mml:mrow><mml:mi mathvariant="normal">d</mml:mi><mml:mi>t</mml:mi></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>=</mml:mo><mml:mi mathvariant="normal">Λ</mml:mi><mml:mi>C</mml:mi><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E12"><mml:mtd><mml:mtext>6</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:mi mathvariant="normal">Λ</mml:mi><mml:mo>=</mml:mo><mml:mi>A</mml:mi><mml:msup><mml:mi>r</mml:mi><mml:mi>B</mml:mi></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              with <inline-formula><mml:math id="M214" display="inline"><mml:mi>C</mml:mi></mml:math></inline-formula> representing the <inline-formula><mml:math id="M215" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration (kg m<inline-formula><mml:math id="M216" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and <inline-formula><mml:math id="M217" display="inline"><mml:mi mathvariant="normal">Λ</mml:mi></mml:math></inline-formula> the scavenging coefficient, which is calculated based on the rainfall rate <inline-formula><mml:math id="M218" display="inline"><mml:mi>r</mml:mi></mml:math></inline-formula> (in mm h<inline-formula><mml:math id="M219" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and two scavenging parameters <inline-formula><mml:math id="M220" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M221" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula>. The parameters <inline-formula><mml:math id="M222" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M223" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> vary for different types of precipitation (i.e. large-scale/convective and rain/snow) and for different wet deposition processes (i.e. rainout, washout and the seeder–feeder process). For more detailed information, including the specific values for <inline-formula><mml:math id="M224" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M225" display="inline"><mml:mi>B</mml:mi></mml:math></inline-formula> for <inline-formula><mml:math id="M226" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and sulfate aerosols, we refer to <xref ref-type="bibr" rid="bib1.bibx109" id="text.55"/>, <xref ref-type="bibr" rid="bib1.bibx59" id="text.56"/> and references therein.</p>
</sec>
<sec id="Ch1.S2.SS3.SSS4">
  <label>2.3.4</label><title>Eruption source parameters</title>
      <p id="d1e3864">When simulating a volcanic eruption, the NAME dispersion model needs eruption source parameters (ESPs) consisting of (1) location, (2) timing, (3) mass eruption rate (kg s<inline-formula><mml:math id="M227" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) and (4) vertical emission profile, and for simulating volcanic ash also (5) particle density, shape and particle size distribution. Here we will discuss ESP 1–4. For information about the set-up of the simulations including ash, we refer to the Part 2 paper <xref ref-type="bibr" rid="bib1.bibx73" id="paren.57"/>. For all simulations described in this paper, we released a total of 10 million air parcels in NAME within a column above the volcano, with each parcel representing an equal amount of <inline-formula><mml:math id="M228" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass. All simulations are run for 25 d until 15 July 2019, and the simulation domain is the NH (north of 25<inline-formula><mml:math id="M229" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N).</p>
      <p id="d1e3902">In all our simulations (see Table <xref ref-type="table" rid="Ch1.T2"/> for overview), we release the <inline-formula><mml:math id="M230" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the location of the volcano (48.3<inline-formula><mml:math id="M231" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, 153.2<inline-formula><mml:math id="M232" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E) between 21 June 18:00 UTC and 22 June 03:00 UTC. The timing of the <inline-formula><mml:math id="M233" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> release is in line with the source term provided by the Volcano Response (VolRes) team (<uri>https://wiki.earthdata.nasa.gov/display/volres</uri>, last access:  6 July 2021). The VolRes team is an international research collaboration to coordinate a response plan after large volcanic eruptions using observational and modelling tools. No information on the temporal variation in the mass eruption rate was provided by VolRes; thus we assume a constant mass eruption rate throughout the entire eruption period.</p>
      <p id="d1e3951">The Raikoke eruption injected most <inline-formula><mml:math id="M234" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass near the tropopause height (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>), but the precise emission profile is uncertain <xref ref-type="bibr" rid="bib1.bibx41 bib1.bibx53" id="paren.58"><named-content content-type="pre">e.g.</named-content></xref>. Small changes in the <inline-formula><mml:math id="M235" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profile could lead to a large change in the amount of mass emitted into the stratosphere, which will strongly influence the evolution of the <inline-formula><mml:math id="M236" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud. Therefore, in our study we use three different <inline-formula><mml:math id="M237" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profiles that vary in terms of the <inline-formula><mml:math id="M238" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass that is emitted into the stratosphere as shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>. The VolRes1.5 <inline-formula><mml:math id="M239" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profile is based on the vertical mass distribution obtained from the VolRes team using IASI retrievals on 22 June, as shown by the orange bars in Fig. <xref ref-type="fig" rid="Ch1.F2"/>. The total <inline-formula><mml:math id="M240" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass emitted based on the VolRes estimate, which is also the mass emission used in the VolRes1.5 profile, was approximately <inline-formula><mml:math id="M241" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> Tg of <inline-formula><mml:math id="M242" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>.</p>
      <p id="d1e4067">To determine what fraction of the total <inline-formula><mml:math id="M243" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass was emitted into the stratosphere, we calculated the tropopause height in the MetUM global analysis using the World Meteorological Organization (WMO) temperature lapse rate definition. Using the spread in the 150 nearest grid points to the volcano location in the model, we get an average tropopause height of <inline-formula><mml:math id="M244" display="inline"><mml:mrow><mml:mn mathvariant="normal">11.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> km during the first 36 h after the eruption. To verify this tropopause height, we used radiosonde data from the Petropavlovsk-Kamchatsky Airport (see Fig. <xref ref-type="fig" rid="Ch1.F1"/>), which is the nearest radiosonde location to the Raikoke volcano (data can be retrieved from <uri>http://weather.uwyo.edu/upperair/sounding.html</uri>, last access: 6 July 2021). Using the same tropopause height criteria for the radiosondes released from this location, we estimate an average tropopause altitude of <inline-formula><mml:math id="M245" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> km during the first 36 h, showing that the MetUM simulated the tropopause height within the expected range. Using the MetUM tropopause height estimate, the VolRes1.5 profile emits 0.86 Tg into the upper<?pagebreak page10858?> troposphere (UT) with a peak at 10 km altitude and emits 0.64 Tg into the lower stratosphere (LS, defined as the layer between the tropopause and 18 km a.s.l.) with a secondary peak at 14 km a.s.l.</p>
      <p id="d1e4111">In the case of a multi-phase plume like Raikoke (multi-phase here refers to the mixture of ash, sulfate aerosols and gas present in the cloud, not the number of eruption phases), high ash concentrations within the volcanic cloud can interfere with satellite <inline-formula><mml:math id="M246" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals <xref ref-type="bibr" rid="bib1.bibx119 bib1.bibx11 bib1.bibx98" id="paren.59"/>, leading to an underestimation of the <inline-formula><mml:math id="M247" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. Furthermore it is known that, in the stratosphere, ash and sulfate aerosols can have a local heating effect due to their interactions with radiation, resulting in lofting of the <inline-formula><mml:math id="M248" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, sulfate aerosols and ash <xref ref-type="bibr" rid="bib1.bibx69 bib1.bibx50 bib1.bibx67 bib1.bibx8" id="paren.60"><named-content content-type="pre">e.g.</named-content></xref>. NAME does not account for radiative lofting of volcanic species due to changes in heating rates as it is an offline model driven by NWP wind fields that are not affected by any volcanic ash or aerosols radiative effects.</p>
      <p id="d1e4155">The fact that Raikoke was an eruption that produced a multi-phase plume that emitted 1.5 Tg of <inline-formula><mml:math id="M249" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and 15 Tg of ash <xref ref-type="bibr" rid="bib1.bibx73" id="paren.61"/> near the tropopause (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>) justifies simulations using different initial <inline-formula><mml:math id="M250" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profiles and warrants a closer investigation of the emission profile provided by the VolRes team. To understand potential uncertainties on the VolRes emission profile, we have run an initial 36 h NAME simulation with the VolRes1.5 vertical emission profile input and compared the <inline-formula><mml:math id="M251" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD estimates (Fig. <xref ref-type="fig" rid="Ch1.F3"/>a) with the TROPOMI retrieval on 23 June (Fig. <xref ref-type="fig" rid="Ch1.F3"/>b). The comparison reveals that the VolRes1.5 simulation has a different longitudinal distribution compared to the TROPOMI satellite retrievals. Figure <xref ref-type="fig" rid="Ch1.F3"/>d shows the averaged <inline-formula><mml:math id="M252" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs between 48–52<inline-formula><mml:math id="M253" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N along section I–II (black box in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a) for the clouds shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a–c. This shows that along the northern part of the cloud between 170–175<inline-formula><mml:math id="M254" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E, the VolRes1.5 simulation underestimates the <inline-formula><mml:math id="M255" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from TROPOMI by up to a factor of 8.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F3" specific-use="star"><?xmltex \currentcnt{3}?><?xmltex \def\figurename{Figure}?><label>Figure 3</label><caption><p id="d1e4250">The <inline-formula><mml:math id="M256" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD estimates for 23 June 2019 for <bold>(a)</bold> the VolRes1.5 simulation, <bold>(b)</bold> the TROPOMI retrievals and <bold>(c)</bold> the StratProfile simulation. The TROPOMI retrievals are downscaled to the NAME simulation resolution, (i.e. averaged per grid box; see Sect. 2.1). The black contours show the pressure at the 10 km a.s.l. in the MetUM analysis used for both NAME simulations. Panel <bold>(d)</bold> shows the latitudinal <inline-formula><mml:math id="M257" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs from panels <bold>(a)</bold>–<bold>(c)</bold> along section I–II in panel <bold>(a)</bold>, averaged over the black box between 48 and 52<inline-formula><mml:math id="M258" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. Shading represents the standard error estimate for the TROPOMI estimate.</p></caption>
            <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f03.png"/>

          </fig>

      <p id="d1e4312">Figure <xref ref-type="fig" rid="Ch1.F4"/> shows the vertical cross section from the VolRes1.5 simulation through the <inline-formula><mml:math id="M259" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud along section I–II in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a, together with the available estimated cloud heights from IASI for all pixels between 49–50<inline-formula><mml:math id="M260" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N. The cloud height from the IASI retrieval is estimated using the method described in <xref ref-type="bibr" rid="bib1.bibx11" id="text.62"/>. Figure <xref ref-type="fig" rid="Ch1.F4"/> shows that the <inline-formula><mml:math id="M261" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud between 170–175<inline-formula><mml:math id="M262" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E is simulated in NAME between 11–14 <inline-formula><mml:math id="M263" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>, which coincides with the UT/LS in the MetUM Global model (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>). The altitude of the <inline-formula><mml:math id="M264" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud for the NAME VolRes1.5 simulation along the cross section shown in Fig. <xref ref-type="fig" rid="Ch1.F4"/> is within the uncertainty range of the IASI height estimates and gives us confidence that the NAME simulated cloud height range is realistic. However, the underestimated <inline-formula><mml:math id="M265" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs in the latitude range 170–175<inline-formula><mml:math id="M266" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E for the VolRes1.5 simulation compared to TROPOMI (Fig. <xref ref-type="fig" rid="Ch1.F3"/>) could indicate an underestimation of the mass fraction of <inline-formula><mml:math id="M267" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> present in the stratosphere, which could be due to the lack of radiative lofting of the <inline-formula><mml:math id="M268" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> during the first 36 h after the eruption. The study by <xref ref-type="bibr" rid="bib1.bibx67" id="text.63"/> shows that after the Raikoke eruption, most of the radiative lofting of the ash layers occurred over these timescales, and we assume similar timescales to be applicable for the lofting of the <inline-formula><mml:math id="M269" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds. Reducing the horizontal diffusion <inline-formula><mml:math id="M270" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> in the VolRes1.5<inline-formula><mml:math id="M271" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> simulation (not shown) resulted in a similar underestimate as shown in Fig. <xref ref-type="fig" rid="Ch1.F3"/>d for VolRes1.5, excluding that overdispersion in the stratosphere is the main source for the underestimate.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F4" specific-use="star"><?xmltex \currentcnt{4}?><?xmltex \def\figurename{Figure}?><label>Figure 4</label><caption><p id="d1e4472">Vertical cross section of <inline-formula><mml:math id="M272" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass concentrations (<inline-formula><mml:math id="M273" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">µ</mml:mi></mml:mrow></mml:math></inline-formula>g m<inline-formula><mml:math id="M274" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">3</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>) in the VolRes1.5 simulation and the IASI height estimate along the line I–II in Fig. <xref ref-type="fig" rid="Ch1.F3"/>a on 22 June 2019 at 22:00 UTC. This time corresponds with the IASI overpass over the volcanic cloud, thereby minimising displacement errors due to timing. The black dots represent the available height estimates including error bars from the IASI retrieval of the <inline-formula><mml:math id="M275" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud for all pixels between 49–50<inline-formula><mml:math id="M276" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N, and it is estimated following the method described in <xref ref-type="bibr" rid="bib1.bibx11" id="text.64"/>. The blue arrow on the right of the figure indicates the range of cruise altitudes for long-haul aircraft (11.9–13.7 km).</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f04.png"/>

          </fig>

      <p id="d1e4539">Based on the initial findings from the VolRes1.5 simulation, we also conduct a simulation in which we released a total of 2 Tg of <inline-formula><mml:math id="M277" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, using the same relative mass distribution in the vertical, termed VolRes2.0. The experiment emits a larger amount of <inline-formula><mml:math id="M278" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the LS (1.15 Tg in the UT and 0.85 Tg in the LS). In chemistry transport models (including NAME), the chemical conversion and the rate of wet and dry deposition of <inline-formula><mml:math id="M279" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> depends on the <inline-formula><mml:math id="M280" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration. Therefore this simulation is not a simple scaling of the VolRes1.5 results.</p>
      <p id="d1e4586">In addition, we derive a different vertical profile based on the TROPOMI <inline-formula><mml:math id="M281" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD retrievals (StratProfile; for derivation see Appendix A) in which we use a different relative mass distribution in the vertical. In contrast to the VolRes1.5 profile (which is based on the IASI satellite overpasses on 22 June), our StratProfile emission profile is based on the 23 June overpasses of TROPOMI. These overpasses are approximately 30 h after the onset of the eruption and show a reduced ash interference (as seen by the strongly reduced AAI values; see Sect. 2.1); thus we expect the <inline-formula><mml:math id="M282" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals to be more accurate. Furthermore, this effective emission profile <xref ref-type="bibr" rid="bib1.bibx84 bib1.bibx54" id="paren.65"/> will take into account any lofting of the <inline-formula><mml:math id="M283" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds resulting from the radiation interactions which may be enhanced by the presence of ash during the first 30 h after the eruption. The derived StratProfile emission profile releases similar amounts of <inline-formula><mml:math id="M284" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the atmosphere as the VolRes1.5 run (1.57 Tg) but has the main peak in <inline-formula><mml:math id="M285" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass at 12–13 km altitude. As a result, the StratProfile emits a much higher fraction (69 % or 1.09 Tg) of the mass into the LS (VolRes emission profile emits 43 % or 0.64 Tg into the LS).</p>
</sec>
</sec>
<sec id="Ch1.S2.SS4">
  <label>2.4</label><title>Metrics to determine the skill of the NAME simulations</title>
      <p id="d1e4657">Assessing the model's skill in representing satellite measurements of <inline-formula><mml:math id="M286" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> requires appropriate metrics. Similar comparisons should be possible in almost near-real time for VAACs when investigating future eruptions. Therefore, apart from being able to show the details of the model–satellite comparison, it is also important that the metric is easily interpretable by end users. In the following subsections we introduce two metrics for identifying the skill of the simulations: (1) the FSS and (2) the SAL score.</p><?xmltex \hack{\newpage}?>
<?pagebreak page10859?><sec id="Ch1.S2.SS4.SSS1">
  <label>2.4.1</label><title>Fractional skill score (FSS)</title>
      <?pagebreak page10860?><p id="d1e4679">The FSS was originally developed to determine the skill of weather forecast models to represent radar rainfall observations <xref ref-type="bibr" rid="bib1.bibx85 bib1.bibx86 bib1.bibx64" id="paren.66"/> but has been since used to also describe the skill of dispersion models in representing volcanic clouds <xref ref-type="bibr" rid="bib1.bibx22 bib1.bibx35" id="paren.67"/>. For volcanic <inline-formula><mml:math id="M287" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds, the FSS is calculated using the ratio between the model-simulated (<inline-formula><mml:math id="M288" display="inline"><mml:mrow><mml:msub><mml:mi>M</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) and observed (<inline-formula><mml:math id="M289" display="inline"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>) fractional coverage of the <inline-formula><mml:math id="M290" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud at each location (neighbourhood) in the domain investigated. When considering <inline-formula><mml:math id="M291" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> neighbourhoods, the FSS is calculated using
<?xmltex \hack{\newpage}?><?xmltex \hack{\vspace*{-6mm}}?>

                  <disp-formula specific-use="align" content-type="numbered"><mml:math id="M292" display="block"><mml:mtable displaystyle="true"><mml:mlabeledtr id="Ch1.E13"><mml:mtd><mml:mtext>7</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">FSS</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn><mml:mo>-</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mi mathvariant="normal">FBS</mml:mi><mml:mrow><mml:msub><mml:mi mathvariant="normal">FBS</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub></mml:mrow></mml:mfrac></mml:mstyle><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E14"><mml:mtd><mml:mtext>8</mml:mtext></mml:mtd><mml:mtd><mml:mstyle displaystyle="true" class="stylechange"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle class="stylechange" displaystyle="true"/><mml:mi mathvariant="normal">FBS</mml:mi><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msup><mml:mfenced open="(" close=")"><mml:mrow><mml:msub><mml:mi>O</mml:mi><mml:mi>k</mml:mi></mml:msub><mml:mo>-</mml:mo><mml:msub><mml:mi>M</mml:mi><mml:mi>k</mml:mi></mml:msub></mml:mrow></mml:mfenced><mml:mn mathvariant="normal">2</mml:mn></mml:msup><mml:mo>,</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr><mml:mlabeledtr id="Ch1.E15"><mml:mtd><mml:mtext>9</mml:mtext></mml:mtd><mml:mtd><mml:mstyle class="stylechange" displaystyle="true"/></mml:mtd><mml:mtd><mml:mrow><mml:mstyle displaystyle="true" class="stylechange"/><mml:msub><mml:mi mathvariant="normal">FBS</mml:mi><mml:mi mathvariant="normal">ref</mml:mi></mml:msub><mml:mo>=</mml:mo><mml:mstyle displaystyle="true"><mml:mfrac style="display"><mml:mn mathvariant="normal">1</mml:mn><mml:mi>N</mml:mi></mml:mfrac></mml:mstyle><mml:mfenced open="[" close="]"><mml:mrow><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msubsup><mml:mi>O</mml:mi><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup><mml:mo>-</mml:mo><mml:munderover><mml:mo movablelimits="false">∑</mml:mo><mml:mrow><mml:mi>k</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow><mml:mi>N</mml:mi></mml:munderover><mml:msubsup><mml:mi>M</mml:mi><mml:mi>k</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msubsup></mml:mrow></mml:mfenced><mml:mo>.</mml:mo></mml:mrow></mml:mtd></mml:mlabeledtr></mml:mtable></mml:math></disp-formula>

              The FSS is calculated from the fractions Brier score (FBS), which is a variation on the Brier score <xref ref-type="bibr" rid="bib1.bibx7" id="paren.68"/>, and FBS<inline-formula><mml:math id="M293" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">ref</mml:mi></mml:msub></mml:math></inline-formula> is the largest FBS score one can obtain from multiple non-zero fractions within the domain when there is no overlap between the two fields. In the case that observations and simulation are perfectly aligned, FSS is equal to one. In the case of a total mismatch FSS is equal to zero. In general for the FSS, a model simulation is considered to have skill when FSS <inline-formula><mml:math id="M294" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5 <xref ref-type="bibr" rid="bib1.bibx35" id="paren.69"><named-content content-type="pre">see e.g.</named-content></xref>.</p>
      <p id="d1e4919">The FSS metric is very suitable for studying the skill of a model in capturing the volcanic cloud's spatial extent. One advantage of using the FSS metric is that it relaxes the requirement for exact matching of the spatial features in the simulations with the observations. Instead when the fractional coverage of the <inline-formula><mml:math id="M295" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud within a studied region (i.e. a neighbourhood of size <inline-formula><mml:math id="M296" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>) is the same for the observations and the simulation, this metric counts it as a correct forecast. By using different sizes of neighbourhoods, one can also determine at which spatial resolution the simulation is skilful (i.e. for which <inline-formula><mml:math id="M297" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> is FSS <inline-formula><mml:math id="M298" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5) at any given time, which helps to determine at which spatial scale features of the <inline-formula><mml:math id="M299" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud can be considered realistic. However the method does not consider differences in <inline-formula><mml:math id="M300" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs values – it only considers a “hit” or “miss” for each location. By applying the same FSS metric to increasing <inline-formula><mml:math id="M301" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD thresholds (i.e. subregions of the cloud), one can obtain information about model skill at simulating volcanic <inline-formula><mml:math id="M302" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud structures with varying vertical column densities.</p>
</sec>
<sec id="Ch1.S2.SS4.SSS2">
  <label>2.4.2</label><title>Structure, amplitude and location score (SAL score)</title>
      <p id="d1e5007">The SAL score is a metric that is composed of three components, which describe the structure (<inline-formula><mml:math id="M303" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>), amplitude (<inline-formula><mml:math id="M304" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula>) and location (<inline-formula><mml:math id="M305" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>) of an investigated feature within a specified domain. The metric was originally developed to compare the structure of model-simulated precipitation fields with observations <xref ref-type="bibr" rid="bib1.bibx113" id="paren.70"/> but has since been adapted to also describe other fields, including volcanic clouds <xref ref-type="bibr" rid="bib1.bibx19 bib1.bibx115 bib1.bibx82" id="paren.71"><named-content content-type="pre">e.g.</named-content></xref>. Here we will adopt this metric to describe the evolution of the <inline-formula><mml:math id="M306" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud. For a detailed description of the equations used to calculate each individual component, we refer the reader to <xref ref-type="bibr" rid="bib1.bibx115" id="text.72"/>.</p>
      <p id="d1e5054">Briefly, to calculate the <inline-formula><mml:math id="M307" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M308" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> scores (not needed for the <inline-formula><mml:math id="M309" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score), we have to identify all the individual simulated and observed <inline-formula><mml:math id="M310" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds. In our analysis each cloud is identified as a group of adjacent grid cells which have a <inline-formula><mml:math id="M311" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD value above a certain threshold. From <xref ref-type="bibr" rid="bib1.bibx100" id="text.73"/> we deduce that the detection limit of the satellite measurements for individual pixels is approximately 1 DU. All of the analysis in our study is done at the highest resolution that is available for all fields, which is the NAME model output (0.2<inline-formula><mml:math id="M312" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude and 0.4<inline-formula><mml:math id="M313" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude). Due to the higher spatial resolution of the satellite product, we have to average the TROPOMI output of multiple pixels within each NAME grid box (on average 9 TROPOMI pixels per NAME output grid box at each given time step) to get both datasets on the same output grid. As a result, we have used a lower detection threshold of 0.3 DU when identifying all grid points that are part of a <inline-formula><mml:math id="M314" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud for the (re-gridded) TROPOMI retrievals and the NAME simulations. To remove additional spurious data from the TROPOMI satellite product, we also include a minimum size of each identified <inline-formula><mml:math id="M315" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud to be 100 km<inline-formula><mml:math id="M316" display="inline"><mml:msup><mml:mi/><mml:mn mathvariant="normal">2</mml:mn></mml:msup></mml:math></inline-formula> (approximately the NAME grid box size at 50<inline-formula><mml:math id="M317" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> N) before considering in our analysis. Simulated and observed <inline-formula><mml:math id="M318" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values below either of these thresholds are excluded from all <inline-formula><mml:math id="M319" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M320" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M321" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> calculations. SAL scores have been calculated by comparing the <inline-formula><mml:math id="M322" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD estimates from each NAME simulation with the individual TROPOMI overpasses, as well as the daily averages. When calculating the individual overpass SAL score values, we only included the NAME simulation data within the region covered by the TROPOMI overpass.</p>
      <p id="d1e5206">To interpret the SAL score, we first assume a single idealised 2D-Gaussian-shaped cloud for both the simulated and observed <inline-formula><mml:math id="M323" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. Looking at the schematic cross section presented in Fig. <xref ref-type="fig" rid="Ch1.F5"/>, three characteristics are represented by the <inline-formula><mml:math id="M324" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>, <inline-formula><mml:math id="M325" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M326" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> scores. The <inline-formula><mml:math id="M327" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score compares the shapes of each individual <inline-formula><mml:math id="M328" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud in terms of the horizontal extent (width) and maximum concentrations within the cloud, by comparing the normalised shape of the clouds (i.e. total mass of the simulated and the observed clouds are made equal; see Fig. <xref ref-type="fig" rid="Ch1.F5"/>a). A negative <inline-formula><mml:math id="M329" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score indicates that the simulated <inline-formula><mml:math id="M330" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds are too narrow or have peak <inline-formula><mml:math id="M331" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values that are too high when compared to the observed cloud (leptokurtic). When the simulated <inline-formula><mml:math id="M332" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds are too wide spread or have peak <inline-formula><mml:math id="M333" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values that are too low, this is indicated by a positive <inline-formula><mml:math id="M334" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score (platykurtic).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F5" specific-use="star"><?xmltex \currentcnt{5}?><?xmltex \def\figurename{Figure}?><label>Figure 5</label><caption><p id="d1e5326">Schematic overview of the SAL score and its interpretation, using two cross sections of idealised Gaussian-shaped <inline-formula><mml:math id="M335" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds. Each panel shows the impact of an individual component of the SAL score: <bold>(a)</bold> structure, <bold>(b)</bold> amplitude and <bold>(c)</bold> location (only the <inline-formula><mml:math id="M336" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> part). A negative <inline-formula><mml:math id="M337" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score indicates that the simulated <inline-formula><mml:math id="M338" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds are too narrow or have peak <inline-formula><mml:math id="M339" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values that are too high when compared to the observed cloud (leptokurtic). When the simulated <inline-formula><mml:math id="M340" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds are too wide spread or have peak <inline-formula><mml:math id="M341" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values that are too low, this is indicated by a positive <inline-formula><mml:math id="M342" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score (platykurtic). Panel <bold>(d)</bold> shows an example of the SAL score diagram with the scores of the three cases in panels <bold>(a)</bold>–<bold>(c)</bold> included. The horizontal axis represents the <inline-formula><mml:math id="M343" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score, the vertical axis represents the <inline-formula><mml:math id="M344" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score and the colour of each point represents the <inline-formula><mml:math id="M345" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score. When the simulation and observations compare perfectly, the score of each of the components is 0. The simulation and observations compare best when all the points are near the origin and have the dark purple colour.</p></caption>
            <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f05.png"/>

          </fig>

      <p id="d1e5456">The <inline-formula><mml:math id="M346" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score represents the comparison between the simulated and the observed total mass of <inline-formula><mml:math id="M347" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> within the entire studied domain and is independent on the number of individual <inline-formula><mml:math id="M348" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds. Negative
<inline-formula><mml:math id="M349" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> scores represent an underestimate of the total <inline-formula><mml:math id="M350" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass in the simulation when compared to the observations (Fig. <xref ref-type="fig" rid="Ch1.F5"/>b), while a positive value shows that the simulation is overestimating the total <inline-formula><mml:math id="M351" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass in the domain.</p>
      <p id="d1e5520">Finally the <inline-formula><mml:math id="M352" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score represents the distribution of the individual simulated and observed <inline-formula><mml:math id="M353" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds within the domain and consists of two parts: <inline-formula><mml:math id="M354" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M355" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> <xref ref-type="bibr" rid="bib1.bibx113" id="paren.74"/>. <inline-formula><mml:math id="M356" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> represents the normalised distance between the domain-averaged centre of mass of all the simulated and observed <inline-formula><mml:math id="M357" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds, where a higher positive value represents a<?pagebreak page10861?> larger distance between the simulated and observed domain-averaged centres of mass (see Fig. <xref ref-type="fig" rid="Ch1.F5"/>c). In the case of multiple <inline-formula><mml:math id="M358" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds, <inline-formula><mml:math id="M359" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> represents the differences in the distribution of individual clouds around the domain-averaged total centre of mass. <inline-formula><mml:math id="M360" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is calculated by considering the distance between the centre of mass of each individual cloud and the total domain-averaged centre of mass. In the case of a single object, <inline-formula><mml:math id="M361" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is equal to 0, as the centre of mass in the domain is the same as the centre of mass of the individual object.</p>
      <p id="d1e5636">When the simulation and observations compare perfectly, the score of each of the components is 0. For the <inline-formula><mml:math id="M362" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M363" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score the values are all between <inline-formula><mml:math id="M364" display="inline"><mml:mrow><mml:mo>±</mml:mo><mml:mn mathvariant="normal">2</mml:mn></mml:mrow></mml:math></inline-formula>, where a value of <inline-formula><mml:math id="M365" display="inline"><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> represents a factor of 3 underestimate of the simulation compared to the observations and <inline-formula><mml:math id="M366" display="inline"><mml:mrow><mml:mo>+</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> represents a factor of 3 overestimate of the simulation. For the <inline-formula><mml:math id="M367" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M368" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> scores, values are between [0, 1], with the worst possible score being 1, representing a distance equal to the maximum distance within the domain. Similar to <xref ref-type="bibr" rid="bib1.bibx113" id="text.75"/>, we will present the three components of this metric in a SAL diagram (Fig. <xref ref-type="fig" rid="Ch1.F5"/>d), where the horizontal axis represents the <inline-formula><mml:math id="M369" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score, the vertical axis represents the <inline-formula><mml:math id="M370" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score and the colour of each point represents the <inline-formula><mml:math id="M371" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score (sum of <inline-formula><mml:math id="M372" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">1</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M373" display="inline"><mml:mrow><mml:msub><mml:mi>L</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>). The simulation and observations compare best when all the points are near the origin and have the dark purple colour.</p><?xmltex \hack{\newpage}?>
</sec>
</sec>
</sec>
<sec id="Ch1.S3">
  <label>3</label><title>Results</title>
      <p id="d1e5766">First we qualitatively discuss the spatial pattern of the <inline-formula><mml:math id="M374" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud and its dispersion across the NH during the first week after the eruption. We then discuss the FSS and the SAL scores for the <inline-formula><mml:math id="M375" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud, followed by a discussion of the <inline-formula><mml:math id="M376" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden evolution during the first 25 d after the eruption. A video of the volcanic <inline-formula><mml:math id="M377" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M378" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs as simulated by NAME for the VolRes1.5 and StratProfile emission profiles can be found in the video supplements <xref ref-type="bibr" rid="bib1.bibx24" id="paren.76"/>.</p>
<sec id="Ch1.S3.SS1">
  <label>3.1</label><title>Spatial pattern of the sulfur dioxide cloud</title>
      <p id="d1e5835">Qualitatively, the general structure of the <inline-formula><mml:math id="M379" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud simulated by the NAME VolRes1.5 and the StratProfile simulations compare well with the retrieved TROPOMI <inline-formula><mml:math id="M380" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs during the first week after the eruption. On 23 June 2019 the TROPOMI retrievals show a split between the northern and southern branch of the <inline-formula><mml:math id="M381" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud, as seen in Fig. <xref ref-type="fig" rid="Ch1.F3"/>. This observed <inline-formula><mml:math id="M382" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud structure was strongly influenced by a low-pressure cyclone approximately 1500 km to the east of the volcano. As a result of the low-pressure system, the volcanic cloud within the troposphere (below 11 km) moved predominantly in a south-eastward direction along the south flank of the cyclone until it started to wrap around the centre on<?pagebreak page10862?> 23 June. For the cloud layers at higher altitudes within the stratosphere, the main wind direction was more zonal, resulting in the observed split in Fig. <xref ref-type="fig" rid="Ch1.F3"/>. The VolRes1.5 and the StratProfile simulations show the same spatial pattern but have different <inline-formula><mml:math id="M383" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs within the cloud (see e.g. Fig. <xref ref-type="fig" rid="Ch1.F3"/>d). The StratProfile (Fig. <xref ref-type="fig" rid="Ch1.F3"/>c) simulation shows a better agreement with the TROPOMI <inline-formula><mml:math id="M384" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values for this day, which is expected based on its derivation.</p>
      <p id="d1e5913">By 25 June 2019, a large part of the cloud moves in a north-western direction, spreading over the Asian continent as seen in Fig. <xref ref-type="fig" rid="Ch1.F6"/>a and b for both the VolRes1.5 simulation and TROPOMI. Due to the variation in emission heights between the VolRes1.5 and the StratProfile simulations (Fig. <xref ref-type="fig" rid="Ch1.F2"/>), we can identify the parts of the cloud in the NAME simulations that are mainly within the troposphere and the stratosphere by comparing their differences. The results are shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>c, which shows that the north-western part of the cloud is mainly within the troposphere, while the stratospheric parts of the cloud remain centred around the low-pressure system. Calculating the difference between the VolRes1.5 simulation and the TROPOMI retrievals in Fig. <xref ref-type="fig" rid="Ch1.F6"/>d, we find that the pattern is very similar to Fig. <xref ref-type="fig" rid="Ch1.F6"/>c. This shows that the VolRes1.5 simulation mainly overestimates the <inline-formula><mml:math id="M385" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass of the cloud in the troposphere and underestimates the stratospheric part of the cloud.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F6" specific-use="star"><?xmltex \currentcnt{6}?><?xmltex \def\figurename{Figure}?><label>Figure 6</label><caption><p id="d1e5940">The spatial pattern of the volcanic cloud on 25 June 2019. The colours in panels <bold>(a)</bold> and <bold>(b)</bold> represent the <inline-formula><mml:math id="M386" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD for the VolRes1.5 simulation and TROPOMI retrievals respectively. The black contours in panel <bold>(a)</bold> show the pressure at 10 km a.s.l. Panel <bold>(c)</bold> shows the difference between the VolRes1.5 and the StratProfile simulations, and the black contours show the pressure at 12 km a.s.l. The negative (blue) values indicate the part of the cloud within the stratosphere, while the positive (red) values highlight the cloud within the UT. Panel <bold>(d)</bold> shows the difference between panels <bold>(a)</bold> and <bold>(b)</bold>, where the contour shows the 1 DU contour for the <inline-formula><mml:math id="M387" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud retrieved by TROPOMI in panel <bold>(b)</bold>.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f06.png"/>

        </fig>

      <p id="d1e5997">On 27 June 2019, the <inline-formula><mml:math id="M388" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud starts to spread also at higher altitudes, leading to a complex spatial pattern as shown in Fig. <xref ref-type="fig" rid="Ch1.F7"/>. While the large-scale structure of the cloud on 27 June has become much more complex, both the VolRes1.5 and the StratProfile simulations capture the general <inline-formula><mml:math id="M389" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD structure of the retrieved TROPOMI cloud well. Note that the small-scale eddies observed by TROPOMI in the centre of the cloud are not simulated by NAME as a result of the limited (spatial and temporal) resolution of the NWP input. Therefore, the small-scale variability cannot be captured by the model but instead is parameterised by the diffusion parameters as a random perturbation on the wind field (see Sect. 2.3.1). This results in the spreading of the <inline-formula><mml:math id="M390" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud with a smoother pattern in the NAME simulations without the high peak values. This also explains the patchy variations shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>b and c within the centre of the cloud. Averaging the <inline-formula><mml:math id="M391" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs over the whole domain shown in Fig. <xref ref-type="fig" rid="Ch1.F7"/> (thereby removing the small-scale features from TROPOMI), the average <inline-formula><mml:math id="M392" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values for the VolRes1.5 simulation are 20 % lower than measured by TROPOMI. This is also evident from the dominant blue colours in Fig. <xref ref-type="fig" rid="Ch1.F7"/>b. For the StratProfile simulation (Fig. <xref ref-type="fig" rid="Ch1.F7"/>c) the domain-average mass is within 0.01 Tg of <inline-formula><mml:math id="M393" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> of the TROPOMI <inline-formula><mml:math id="M394" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimate (i.e. StratProfile <inline-formula><mml:math id="M395" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimate is <inline-formula><mml:math id="M396" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> % lower than TROPOMI).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F7" specific-use="star"><?xmltex \currentcnt{7}?><?xmltex \def\figurename{Figure}?><label>Figure 7</label><caption><p id="d1e6112">The spatial pattern of the volcanic <inline-formula><mml:math id="M397" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud as retrieved by the TROPOMI satellite for the 27 June 2019 (panel <bold>a</bold>). Panels <bold>(b)</bold> and <bold>(c)</bold> show the difference (in DU) with the VolRes1.5 and the StratProfile simulation respectively. Only <inline-formula><mml:math id="M398" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values above 1 DU are shown. The contour shows the outline of the <inline-formula><mml:math id="M399" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud in TROPOMI for a <inline-formula><mml:math id="M400" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD of 1 DU.</p></caption>
          <?xmltex \igopts{width=455.244094pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f07.png"/>

        </fig>

      <p id="d1e6175">Finally, we also find a larger spread of the cloud in both the VolRes1.5 and StratProfile simulations as seen in Fig. <xref ref-type="fig" rid="Ch1.F7"/>b and c by the red values outside the 1 DU TROPOMI contour. We only included the values <inline-formula><mml:math id="M401" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1 DU in this plot for clarity of the figure. When including lower values (0.3–1 DU), the overestimation of the spread of the cloud in NAME is even larger (not shown here).</p>
</sec>
<sec id="Ch1.S3.SS2">
  <label>3.2</label><title>Fractional skill score (FSS)</title>
      <p id="d1e6195">The VolRes1.5 and the StratProfile simulations are generally able to capture the large-scale structure of the <inline-formula><mml:math id="M402" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud, but differences between the simulations and the satellite retrievals occur after 4–5 d of simulation (see for example Fig. <xref ref-type="fig" rid="Ch1.F6"/>). To determine the timescales for which the simulations show skill compared to the TROPOMI retrievals, we calculate the FSS score for each individual overpass for a range of <inline-formula><mml:math id="M403" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD contours (ranging between 0.3 and 100 DU). The results for the smallest neighbourhood size <inline-formula><mml:math id="M404" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> (i.e. the NAME output grid box size 0.2<inline-formula><mml:math id="M405" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> latitude and 0.4<inline-formula><mml:math id="M406" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> longitude) are shown in Fig. <xref ref-type="fig" rid="Ch1.F8"/> for (a) the VolRes1.5 and (b) the StratProfile simulation.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F8" specific-use="star"><?xmltex \currentcnt{8}?><?xmltex \def\figurename{Figure}?><label>Figure 8</label><caption><p id="d1e6257">Time evolution of the FSS (<inline-formula><mml:math id="M407" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula>) and the <inline-formula><mml:math id="M408" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass for each individual overpass of the TROPOMI satellite over the Raikoke cloud for <bold>(a)</bold> the VolRes1.5 simulation and <bold>(b)</bold> StratProfile simulation. Each annotated date represents 00:00 UTC. Grey dots represent all concentrations between 0.3 and 100 DU, with the highest skill score for the lowest concentrations. The horizontal dashed line shows a value of FSS <inline-formula><mml:math id="M409" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0.5, which is the cut-off value for determining the skill of the simulations.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f08.png"/>

        </fig>

      <p id="d1e6302">The VolRes1.5 simulation is able to capture the overall outline of the cloud well for this period but struggles to simulate the peak <inline-formula><mml:math id="M410" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values within the retrieved TROPOMI <inline-formula><mml:math id="M411" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud. Focussing on the <inline-formula><mml:math id="M412" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD <inline-formula><mml:math id="M413" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 1 DU points in Fig. <xref ref-type="fig" rid="Ch1.F8"/>a, the simulation has skill (FSS <inline-formula><mml:math id="M414" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.5) for up to 12.5 d after the eruption onset. This shows that the simulation captures the overall dispersion of the cloud well, as it is able to distinguish between areas with and without any <inline-formula><mml:math id="M415" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> across the NH. For <inline-formula><mml:math id="M416" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs greater than 30 DU, which correspond to small-scale features within the volcanic cloud, the simulation has no significant skill beyond 2.5 d after the start of the eruption. This agrees with the fact that the VolRes1.5 simulation was not able to capture the peak values on the 25 June 2019 observed by TROPOMI as shown in Fig. <xref ref-type="fig" rid="Ch1.F6"/>.</p>
      <p id="d1e6380">The FSS values for the StratProfile simulation (Fig. <xref ref-type="fig" rid="Ch1.F8"/>b) reveal that this simulation performs better than VolRes1.5 and has skill on a longer timescale for all of the <inline-formula><mml:math id="M417" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. For the lower <inline-formula><mml:math id="M418" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs (<inline-formula><mml:math id="M419" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> DU), the StratProfile simulation remains skilful 2 d longer than the VolRes1.5 simulation (12.5 d versus 14.5 d). For the <inline-formula><mml:math id="M420" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above 30 DU, the FSS skill timescale has doubled compared to the VolRes1.5 simulation, showing again the importance of the emission profile on the skill of the simulation.</p>
      <p id="d1e6428">The timescales for which the NAME simulations show skill (compared to the TROPOMI retrievals) in terms of FSS are shown in Fig. <xref ref-type="fig" rid="Ch1.F9"/> and Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>. Independent of the neighbourhood size, the StratProfile simulation has the highest skill for all <inline-formula><mml:math id="M421" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. Figure <xref ref-type="fig" rid="Ch1.F9"/> shows that the StratProfile simulation is skilful on timescales twice as long for <inline-formula><mml:math id="M422" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values above 10 DU compared to the VolRes1.5 and VolRes2.0 simulations. Interestingly the change in neighbourhood size (i.e. averaging region) has only a limited impact on the skill timescales for low <inline-formula><mml:math id="M423" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs  (below 5 DU). This shows that all of the simulations are able to capture the horizontal extent of the <inline-formula><mml:math id="M424" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud well on spatial scales similar to our smallest output grid used (<inline-formula><mml:math id="M425" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.2</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula>) and on timescales of 2–3 weeks after the start of the eruption.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F9"><?xmltex \currentcnt{9}?><?xmltex \def\figurename{Figure}?><label>Figure 9</label><caption><p id="d1e6504">The timescales for which the NAME model shows skill based on the FSS, when compared with TROPOMI retrievals. The results are shown for the three simulations as discussed in Sect. 2.3.4 and for two different neighbourhood sizes (value in brackets represent the corresponding resolution). The FSS metric is calculated only for the first 17 d of the simulation (up to 10 July), as the <inline-formula><mml:math id="M426" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values become too small after to give a good estimate of the FSS from the TROPOMI measurements.</p></caption>
          <?xmltex \igopts{width=236.157874pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f09.png"/>

        </fig>

      <?pagebreak page10863?><p id="d1e6524"><?xmltex \hack{\newpage}?>The reduction in FSS scores for high <inline-formula><mml:math id="M427" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs is influenced by two factors. (1) Does the simulation capture high <inline-formula><mml:math id="M428" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs. And if so
(2) is the location of the high VCD features in the <inline-formula><mml:math id="M429" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud (see e.g. Fig. <xref ref-type="fig" rid="Ch1.F7"/>c) correct? Due to the dispersion of the <inline-formula><mml:math id="M430" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud with time, we expect a decrease in the FSS values in time for the higher <inline-formula><mml:math id="M431" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs as these concentrations are not present anymore in either the TROPOMI retrievals or the NAME simulations (resulting in FSS <inline-formula><mml:math id="M432" display="inline"><mml:mo>=</mml:mo></mml:math></inline-formula> 0). The skill timescales are therefore expected to reduce as the <inline-formula><mml:math id="M433" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs increase. The StratProfile simulation contains higher <inline-formula><mml:math id="M434" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs throughout the simulation period compared to the VolRes1.5 and VolRes2.0 simulations, resulting in higher FSS values and longer relative skill.</p>
      <p id="d1e6615">For high <inline-formula><mml:math id="M435" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs, the FSS metric depends more on the used neighbourhood sizes as the corresponding <inline-formula><mml:math id="M436" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud features get smaller. Using a larger neighbourhood size<?pagebreak page10864?> compares the presence of small-scale features over a larger region, reducing the impact of any misplacement, and results in a higher FSS. The <inline-formula><mml:math id="M437" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values at which model skill increases for different neighbourhood sizes is therefore linked to a displacement error. In Fig. <xref ref-type="fig" rid="Ch1.F9"/>, a doubling in skill timescales is found for the larger neighbourhood size (hashed versus non-hashed) at <inline-formula><mml:math id="M438" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs <inline-formula><mml:math id="M439" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 10 DU for the VolRes1.5 and VolRes2.0 simulations, while for the StratProfile similar differences are evident for <inline-formula><mml:math id="M440" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above 30 DU. This shows that the VolRes1.5 and VolRes2.0 simulations are able to represent observed small-scale features within the <inline-formula><mml:math id="M441" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud for VCDs up to 10 DU at timescales less than 5 d. For <inline-formula><mml:math id="M442" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs <inline-formula><mml:math id="M443" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 20 DU these two simulations gain no additional skill with an increased neighbourhood size and show a strong reduction in skill timescales. This indicates that the high <inline-formula><mml:math id="M444" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs (<inline-formula><mml:math id="M445" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> DU) observed by TROPOMI are not simulated anywhere in the <inline-formula><mml:math id="M446" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud at timescales longer than 5 d. For the StratProfile simulation, features with <inline-formula><mml:math id="M447" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above 30 DU are still present up to 4 d. However, these features are slightly displaced, as evident from the increase in the FSS skill timescales from increasing the neighbourhood size from 0.2 to 1<inline-formula><mml:math id="M448" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>.</p>
      <p id="d1e6766">On timescales longer than 5 d, all the NAME simulations show a strong diffusion in the <inline-formula><mml:math id="M449" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud (related to the diffusion parameterisations). As a result none are capturing the high <inline-formula><mml:math id="M450" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs retrieved by TROPOMI, which reduces the FSS for these high values quickly to 0. This shows that high <inline-formula><mml:math id="M451" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs within the <inline-formula><mml:math id="M452" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud are only skilfully simulated on timescales less than 5 d.</p>
</sec>
<sec id="Ch1.S3.SS3">
  <label>3.3</label><title>The SAL score</title>
      <p id="d1e6821">Figure <xref ref-type="fig" rid="Ch1.F10"/> shows the SAL scores for all the individual TROPOMI overpasses and the daily average values for four different NAME simulations. This comparison shows the strength of the SAL diagram to determine what aspects of the <inline-formula><mml:math id="M453" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud are captured well by the NAME simulations and where the simulations are struggling to match the TROPOMI<?pagebreak page10865?> retrievals. At the start of the eruption, all simulations are in the top half of the diagram (positive <inline-formula><mml:math id="M454" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score). This indicates that the simulations have a larger total <inline-formula><mml:math id="M455" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass than the TROPOMI retrievals during the first days after the eruption. This can be partly explained by the presence of ash interfering with the TROPOMI retrievals (see Sect. 3.4). Furthermore the <inline-formula><mml:math id="M456" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> values are close to 0, indicating that the shape of the cloud is captured well within the simulations. The low <inline-formula><mml:math id="M457" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> values throughout all the simulation indicate that the location of the <inline-formula><mml:math id="M458" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds is well captured.</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F10" specific-use="star"><?xmltex \currentcnt{10}?><?xmltex \def\figurename{Figure}?><label>Figure 10</label><caption><p id="d1e6883">Time evolution of the SAL values for four different NAME simulations: <bold>(a)</bold> VolRes1.5, <bold>(b)</bold> VolRes2.0, <bold>(c)</bold> StratProfile and <bold>(d)</bold> StratProfile<inline-formula><mml:math id="M459" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula>. The black dashed line shows the daily average evolution of the <inline-formula><mml:math id="M460" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M461" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> parameters between 22 June and 10 July, while the coloured squares show the daily average values of <inline-formula><mml:math id="M462" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula>. The coloured dots represent the SAL values for each individual TROPOMI overpass as shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/>. To obtain the <inline-formula><mml:math id="M463" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> parameter, we have excluded the <inline-formula><mml:math id="M464" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs of TROPOMI below 0.3 DU to reduce noise but included all mass for the NAME simulations (see Sect. 2.3.2).</p></caption>
          <?xmltex \igopts{width=497.923228pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f10.png"/>

        </fig>

      <p id="d1e6955">All four simulations shown in Fig. <xref ref-type="fig" rid="Ch1.F10"/> show a tendency of increasing positive <inline-formula><mml:math id="M465" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score values with time, with a strong increase on 27 June, which is 5 d after the start of the eruption. An increase in the <inline-formula><mml:math id="M466" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score represents an <inline-formula><mml:math id="M467" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud which is more widespread (platykurtic) in the simulations compared to the <inline-formula><mml:math id="M468" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs obtained from TROPOMI. The largest changes in the <inline-formula><mml:math id="M469" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score around 5 d into the simulation are consistent with our FSS analysis where we identified that this is also the time where the VolRes1.5 and the StratProfile simulations are losing the skill to represent high <inline-formula><mml:math id="M470" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs retrieved by TROPOMI (i.e. not capturing the peak values in the cloud).</p>
      <p id="d1e7016">Focussing on the VolRes1.5 and the VolRes2.0 simulations (Fig. <xref ref-type="fig" rid="Ch1.F10"/>a and b), both SAL diagrams show a similar pattern (moving from the top left towards the bottom right in the diagram). Due to the total emitted <inline-formula><mml:math id="M471" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass being greater in the VolRes2.0 simulation, Fig. <xref ref-type="fig" rid="Ch1.F10"/>b shows a more positive <inline-formula><mml:math id="M472" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score during the first 4 d after the eruption (22–26 June) than the VolRes1.5 simulation as the former overestimates the total <inline-formula><mml:math id="M473" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass retrieved by TROPOMI. After 26 June, the <inline-formula><mml:math id="M474" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score for VolRes2.0 remains close to the <inline-formula><mml:math id="M475" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> line in Fig. <xref ref-type="fig" rid="Ch1.F10"/>b, showing that the total <inline-formula><mml:math id="M476" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass compares better with TROPOMI for the VolRes2.0 simulation than the VolRes1.5 simulation after 5 d. For the StratProfile simulation (Fig. <xref ref-type="fig" rid="Ch1.F10"/>c), the comparison with TROPOMI is better throughout the entire simulation than for the VolRes1.5 and the VolRes2.0 simulations, as is evident by the low <inline-formula><mml:math id="M477" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score as well as the low <inline-formula><mml:math id="M478" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score. The comparison between the StratProfile simulation and TROPOMI for each individual TROPOMI overpass (i.e. each dot in Fig. <xref ref-type="fig" rid="Ch1.F10"/>c) is close to the <inline-formula><mml:math id="M479" display="inline"><mml:mrow><mml:mi>A</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0</mml:mn></mml:mrow></mml:math></inline-formula> line in the diagram, showing that NAME is able to capture the total <inline-formula><mml:math id="M480" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass very well. Also a lower <inline-formula><mml:math id="M481" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score (darker colour of the squares and circles) indicates that the model captures the location of the cloud more accurately than both the VolRes simulations. These results are consistent with the results shown in Figs. <xref ref-type="fig" rid="Ch1.F6"/>–<xref ref-type="fig" rid="Ch1.F9"/>.</p>
      <p id="d1e7139">Reducing the horizontal diffusion parameter by 75 % (<inline-formula><mml:math id="M482" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula>; see Table <xref ref-type="table" rid="Ch1.T2"/>) in the StratProfile<inline-formula><mml:math id="M483" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> simulation (Fig. <xref ref-type="fig" rid="Ch1.F10"/>d) reveals a relative decrease in the <inline-formula><mml:math id="M484" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score during the first week (e.g. <inline-formula><mml:math id="M485" display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.5</mml:mn></mml:mrow></mml:math></inline-formula> for StratProfile versus <inline-formula><mml:math id="M486" display="inline"><mml:mrow><mml:mi>S</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">0.1</mml:mn></mml:mrow></mml:math></inline-formula> for StratProfile<inline-formula><mml:math id="M487" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> on 25 June) and no change in the <inline-formula><mml:math id="M488" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> and <inline-formula><mml:math id="M489" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> scores when compared to Fig. <xref ref-type="fig" rid="Ch1.F10"/>c. This behaviour is expected, as a decreased diffusion will not alter the total mass (<inline-formula><mml:math id="M490" display="inline"><mml:mi>A</mml:mi></mml:math></inline-formula> score) or the centre of mass of the individual <inline-formula><mml:math id="M491" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds (<inline-formula><mml:math id="M492" display="inline"><mml:mi>L</mml:mi></mml:math></inline-formula> score), but it will result in more concentrated <inline-formula><mml:math id="M493" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds (reduction of <inline-formula><mml:math id="M494" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula>). As a result, the StratProfile<inline-formula><mml:math id="M495" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> simulation shows the best comparison with the TROPOMI retrievals for the first 4 d of the eruption (up to 26 June). After that the <inline-formula><mml:math id="M496" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score quickly increases for all the simulations independent of the diffusion parameterisation, as diffusion related to uncertainties from the large-scale meteorological conditions (i.e. synoptic-scale uncertainties) starts to dominate the signal.</p>
</sec>
<sec id="Ch1.S3.SS4">
  <label>3.4</label><title>Sulfur dioxide mass burden</title>
      <p id="d1e7293">Figure <xref ref-type="fig" rid="Ch1.F11"/>a shows the <inline-formula><mml:math id="M497" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden evolution calculated from the TROPOMI satellite retrievals and three NAME simulations (VolRes1.5, VolRes2.0 and the StratProfile) for the 25 d between the start of the eruption and 15 July 2019. The best comparison is obtained using the StratProfile simulation, which captures both the peak value and the long-term evolution remarkably well and falls well within the uncertainty range of the TROPOMI estimate. To obtain the mass burden, we have excluded the <inline-formula><mml:math id="M498" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs of TROPOMI below 0.3 DU to reduce noise but included all mass for NAME simulations as discussed in the methods section. It is likely that TROPOMI underestimates the <inline-formula><mml:math id="M499" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs and thus <inline-formula><mml:math id="M500" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass during the initial phase of the eruption due to the presence of volcanic ash, which is supported by large values of AAI obtained from TROPOMI during the first 2 d after the eruption (see grey bars Fig. <xref ref-type="fig" rid="Ch1.F11"/>a and also Sect. 2.1).</p>

      <?xmltex \floatpos{t}?><fig id="Ch1.F11" specific-use="star"><?xmltex \currentcnt{11}?><?xmltex \def\figurename{Figure}?><label>Figure 11</label><caption><p id="d1e7347">The daily evolution of <bold>(a)</bold> the total <inline-formula><mml:math id="M501" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass (Tg of <inline-formula><mml:math id="M502" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) and <bold>(b)</bold> the total <inline-formula><mml:math id="M503" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass (Tg of <inline-formula><mml:math id="M504" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>) for the 2019 Raikoke eruption for different ESPs in NAME. We have included the TROPOMI <inline-formula><mml:math id="M505" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass estimate (blue dashed line) as well as the evolution of three NAME runs: VolRes1.5, VolRes2.0 and StratProfile (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>). The dotted lines in the figures show the corresponding daily deposition of <inline-formula><mml:math id="M506" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M507" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the simulations. The peak values in the NAME <inline-formula><mml:math id="M508" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass distribution are slightly higher than the mentioned total emission values in Table <xref ref-type="table" rid="Ch1.T2"/>, which is the result from applying the 15 km AKs to the dispersion model data. The total <inline-formula><mml:math id="M509" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden for TROPOMI is calculated using all locations where the vertical column densities are above 0.3 DU, while for the NAME simulations we include all mass. The blue shading represents the standard error estimate for the TROPOMI product. The grey bars show the TROPOMI estimated 0.1 <inline-formula><mml:math id="M510" display="inline"><mml:mo>×</mml:mo></mml:math></inline-formula> max(AAI) value inside the volcanic cloud for the first 5 d after the eruption. The high AAI values during the first 48 h indicate high concentrations of ash, thereby affecting the TROPOMI <inline-formula><mml:math id="M511" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals during this period.</p></caption>
          <?xmltex \igopts{width=341.433071pt}?><graphic xlink:href="https://acp.copernicus.org/articles/21/10851/2021/acp-21-10851-2021-f11.png"/>

        </fig>

      <?pagebreak page10866?><p id="d1e7485">Consistent with Figs. <xref ref-type="fig" rid="Ch1.F3"/>, <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F7"/>, the VolRes1.5 simulation captures the peak in total <inline-formula><mml:math id="M512" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass within the uncertainty of the TROPOMI estimate but underestimates the TROPOMI <inline-formula><mml:math id="M513" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass between 27 June and 15 July 2019 by 0.3 Tg on average. Based on the data shown in Fig. <xref ref-type="fig" rid="Ch1.F11"/>, we calculated an <inline-formula><mml:math id="M514" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M515" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> d for the VolRes1.5 simulation and an <inline-formula><mml:math id="M516" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M517" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">21</mml:mn></mml:mrow></mml:math></inline-formula> d for TROPOMI during the first 6 d after the eruption (23–27 June 2019), showing that the VolRes1.5 simulation loses <inline-formula><mml:math id="M518" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass at a much faster rate than that calculated based on TROPOMI. As a result, this leads to an underestimation of 25 % (0.33 Tg) of the VolRes1.5 simulation compared to TROPOMI on 28 June. From 27 June the loss rate for both TROPOMI and VolRes1.5 is similar, with an <inline-formula><mml:math id="M519" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M520" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">14</mml:mn></mml:mrow></mml:math></inline-formula>–15 d, which is within the range reported in the literature for extratropical summer eruptions of similar magnitude (e.g. <inline-formula><mml:math id="M521" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of 9–18 d for Kasatochi 2008 and 11–14 d for Sarychev 2009) <xref ref-type="bibr" rid="bib1.bibx51 bib1.bibx58 bib1.bibx39 bib1.bibx48 bib1.bibx44 bib1.bibx13" id="paren.77"/>.</p>
      <p id="d1e7593">After 27 June 2019, the total <inline-formula><mml:math id="M522" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden evolution from TROPOMI is best captured by the VolRes2.0 and the StratProfile simulations, related to a larger amount of mass emitted into the stratosphere. From the total <inline-formula><mml:math id="M523" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass emitted into the stratosphere calculated in Table <xref ref-type="table" rid="Ch1.T2"/>, we see that both the VolRes2.0 and the StratProfile respectively emit 0.2 and 0.45 Tg more <inline-formula><mml:math id="M524" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass into the stratosphere than the VolRes1.5 simulation. For the VolRes2.0 simulation the overall evolution of the <inline-formula><mml:math id="M525" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass profile is similar to that obtained from the VolRes1.5 simulation (<inline-formula><mml:math id="M526" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M527" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> d during the first week and <inline-formula><mml:math id="M528" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of 14–15 d afterwards). However, due to the increased total <inline-formula><mml:math id="M529" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emissions (0.5 Tg more than VolRes1.5), the <inline-formula><mml:math id="M530" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass evolution of VolRes2.0 also overestimates the TROPOMI peak mass by more than 0.5 Tg on 23 June. Given that TROPOMI is used as our baseline metric for initialising our StratProfile simulations, it is not surprising that the best comparison with TROPOMI during the start of the eruption is obtained for the StratProfile simulations. However, on longer timescales the influence of other factors (e.g. simulated wind field, radiative heating, mixing) on the dispersion of the <inline-formula><mml:math id="M531" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud means that the model simulation could easily diverge from the observations. That the StratProfile continues to best match the TROPOMI data gives confidence that NAME captures the main processes needed to represent the <inline-formula><mml:math id="M532" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> dispersion well.</p>
      <?pagebreak page10867?><p id="d1e7712">A possible cause for the strong reduction in total <inline-formula><mml:math id="M533" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass during the first week for the VolRes1.5 and VolRes2.0 simulations might be too strong a conversion of <inline-formula><mml:math id="M534" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into sulfate aerosols during the start of the simulation. To test this hypothesis, we also calculated the mass evolution of <inline-formula><mml:math id="M535" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in NAME, which is shown in Fig. <xref ref-type="fig" rid="Ch1.F11"/>b. From this we can conclude that the chemical conversion into <inline-formula><mml:math id="M536" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is realistic within the NAME simulations. The daily rate of production of <inline-formula><mml:math id="M537" display="inline"><mml:mrow class="unit"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is small (less than 0.03 Tg d<inline-formula><mml:math id="M538" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>), which is a factor of 3 lower than the average daily decrease in <inline-formula><mml:math id="M539" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass in the VolRes1.5 and VolRes2.0 simulations during the first week (0.1 Tg d<inline-formula><mml:math id="M540" display="inline"><mml:msup><mml:mi/><mml:mrow><mml:mo>-</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:msup></mml:math></inline-formula>).</p>
      <p id="d1e7808">The daily total <inline-formula><mml:math id="M541" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass deposition from the NAME simulations is shown by the dotted lines in Fig. <xref ref-type="fig" rid="Ch1.F11"/>a. For 23 and 24 June, the total daily wet deposition dominates the removal of <inline-formula><mml:math id="M542" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> from the atmosphere, as it is responsible for 89 %–90 % of the <inline-formula><mml:math id="M543" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass reduction for the VolRes1.5, the VolRes2.0 and the StratProfile simulations. Atmospheric conditions during the first week of the eruption can explain this relatively large contribution from wet deposition. During the first week of the eruption, the <inline-formula><mml:math id="M544" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud is moving within a region of moist air in the warm conveyor belt on the southern edge of the cyclone (see Fig. <xref ref-type="fig" rid="Ch1.F3"/>). This favours the chemical conversion of <inline-formula><mml:math id="M545" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into <inline-formula><mml:math id="M546" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through aqueous-phase chemistry and also the removal of <inline-formula><mml:math id="M547" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> through wet deposition, resulting in the peak deposition values in Fig. <xref ref-type="fig" rid="Ch1.F11"/>a. The cyclone is mainly a tropospheric phenomenon, and as a result wet deposition occurs mostly in the tropospheric part of the <inline-formula><mml:math id="M548" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud. As the VolRes2.0 simulation emits the largest amount of <inline-formula><mml:math id="M549" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the troposphere (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>), this also explains the highest removal rate (red dotted line Fig. <xref ref-type="fig" rid="Ch1.F11"/>a peaks at 12 % of the NH-mean daily <inline-formula><mml:math id="M550" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden on 23 June) and also the highest conversion rate during the first week of the simulation (evident from the largest <inline-formula><mml:math id="M551" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden in Fig. <xref ref-type="fig" rid="Ch1.F11"/>b in this period). The wet deposition is lowest for the StratProfile simulation during 23 and 24 June (peaks at 4 %–5 % of the NH-mean daily <inline-formula><mml:math id="M552" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden on 23 June), as less mass is emitted into the troposphere for this profile.</p>
      <p id="d1e7958">The results from Fig. <xref ref-type="fig" rid="Ch1.F11"/> show that there is a high sensitivity of the mass burden evolution in NAME to the vertical emission profile used for this particular eruption, which straddled the tropopause. Due to different atmospheric conditions within the troposphere and stratosphere, the <inline-formula><mml:math id="M553" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden evolution is different within the two layers, resulting in significant differences in the total <inline-formula><mml:math id="M554" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden evolution in our simulations. The average <inline-formula><mml:math id="M555" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M556" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> in the UT is <inline-formula><mml:math id="M557" display="inline"><mml:mrow><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> d <xref ref-type="bibr" rid="bib1.bibx58 bib1.bibx13" id="paren.78"><named-content content-type="pre">e.g.</named-content></xref>, which is consistent with the <inline-formula><mml:math id="M558" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time simulated during the first days of the VolRes1.5 and VolRes2.0 simulations. However, the longer <inline-formula><mml:math id="M559" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time obtained for TROPOMI for the first 10 d suggests that the bulk of the <inline-formula><mml:math id="M560" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass was not emitted into the UT.</p>
      <?pagebreak page10868?><p id="d1e8044">After 10 d a large fraction of the tropospheric <inline-formula><mml:math id="M561" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass is removed from the atmosphere through wet deposition or converted into <inline-formula><mml:math id="M562" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, and the remaining signal in Fig. <xref ref-type="fig" rid="Ch1.F11"/> is dominated by the stratospheric component of the cloud. This part of the cloud is much less affected by the cyclone, and the stratosphere contains much less moisture. Therefore <inline-formula><mml:math id="M563" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> is removed at a much lower rate (<inline-formula><mml:math id="M564" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> deposition is <inline-formula><mml:math id="M565" display="inline"><mml:mrow><mml:mo>&lt;</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> %) and is mainly converted through the gas-phase reaction with <inline-formula><mml:math id="M566" display="inline"><mml:mrow class="chem"><mml:mi mathvariant="normal">OH</mml:mi></mml:mrow></mml:math></inline-formula>, resulting in the longer <inline-formula><mml:math id="M567" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of approximately 14–15 d. The similarity in <inline-formula><mml:math id="M568" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time obtained from TROPOMI and all the simulations between 27 June and 15 July suggests that the chemistry scheme in NAME is realistic.</p>
      <p id="d1e8126">Overall, the total <inline-formula><mml:math id="M569" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden obtained using the StratProfile emission profiles (both StratProfile and StratProfile<inline-formula><mml:math id="M570" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> give the same mass evolution) compares best with TROPOMI. Based on this comparison, we estimate that the 2019 eruption of Raikoke emitted approximately 0.9–1.1 Tg of <inline-formula><mml:math id="M571" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the lower stratosphere (11–18 km a.s.l.). With a maximum <inline-formula><mml:math id="M572" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden of 1.5–1.6 Tg in the atmosphere, it follows that approximately 0.4–0.7 Tg was emitted into the UT (8–11 km a.s.l.).</p>
</sec>
</sec>
<sec id="Ch1.S4">
  <label>4</label><title>Discussion</title>
      <p id="d1e8180">Our study shows that the NAME simulations compare very well with the TROPOMI satellite retrievals of the <inline-formula><mml:math id="M573" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud during the first 3 weeks after the 2019 Raikoke eruption. Despite the increasing complexity of the <inline-formula><mml:math id="M574" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud's horizontal structure over time, all our simulations are able to capture the outermost extent of the cloud within an accuracy of approximately 0.4<inline-formula><mml:math id="M575" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula>(50 <inline-formula><mml:math id="M576" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>) during the first 2 weeks of the simulations and for up to 25 d with an accuracy of approximately 1<inline-formula><mml:math id="M577" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> (100 <inline-formula><mml:math id="M578" display="inline"><mml:mrow class="unit"><mml:mi mathvariant="normal">km</mml:mi></mml:mrow></mml:math></inline-formula>) (see Figs. <xref ref-type="fig" rid="Ch1.F8"/> and <xref ref-type="fig" rid="Ch1.F9"/> and Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>). While simulated <inline-formula><mml:math id="M579" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations within the cloud are strongly dependent on the ESPs, the general dispersion patterns of the <inline-formula><mml:math id="M580" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud are captured very well in both the troposphere and the stratosphere for all the NAME simulations performed (see Figs. <xref ref-type="fig" rid="Ch1.F3"/>, <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F7"/>). Combining this information with the comparison of the vertical profile from IASI (Fig. <xref ref-type="fig" rid="Ch1.F4"/>) and the included representation of the sulfur chemistry in the NAME simulations (Fig. <xref ref-type="fig" rid="Ch1.F11"/>) gives us confidence that the NAME model is able to simulate the 3D structure of the volcanic <inline-formula><mml:math id="M581" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud (and consequently the <inline-formula><mml:math id="M582" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud) for the 2019 Raikoke eruption.</p>
      <p id="d1e8302">While the NAME model was not developed specifically to simulate stratospheric volcanic <inline-formula><mml:math id="M583" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds, our results show that the model is suitable to be used by VAACs to issue forecasts on the evolution of volcanic <inline-formula><mml:math id="M584" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds in the upper troposphere/lower stratosphere. Currently after a volcanic eruption, VAACs provide information on the areas in the atmosphere where volcanic ash is forecasted up to 18 h into the future. In the case of the Raikoke 2019 eruption, we have shown that a similar approach to produce a forecast for the presence of a <inline-formula><mml:math id="M585" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud would have been accurate on this and even longer timescales. However, future <inline-formula><mml:math id="M586" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud forecasts will more likely be based on designated <inline-formula><mml:math id="M587" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration thresholds. From our simulations we found that NAME is able to capture the horizontal extent of the 1 DU <inline-formula><mml:math id="M588" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD contour on a spatial resolution of <inline-formula><mml:math id="M589" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.2</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>×</mml:mo><mml:mn mathvariant="normal">0.4</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:mrow></mml:math></inline-formula> during the first 17 d after the eruption. Assuming that the obtained <inline-formula><mml:math id="M590" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values are from a cloud at 12 km altitude with a thickness of 2 km (e.g. estimated from Fig. <xref ref-type="fig" rid="Ch1.F4"/>), 1 DU would correspond to an average <inline-formula><mml:math id="M591" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentration of 0.02 ppm within this cloud. As reference, based on sulfur dioxide acute exposure guideline levels (AEGL) <xref ref-type="bibr" rid="bib1.bibx68" id="paren.79"/>, an extended exposure (<inline-formula><mml:math id="M592" display="inline"><mml:mrow><mml:mo>&gt;</mml:mo><mml:mn mathvariant="normal">10</mml:mn></mml:mrow></mml:math></inline-formula> min) to <inline-formula><mml:math id="M593" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> concentrations of 0.2 ppm (lowest AEGL) can lead to some respiratory irritation, while concentrations above 0.75 ppm can lead to long-lasting adverse health effects. For our example, the lowest AEGL threshold would therefore correspond to <inline-formula><mml:math id="M594" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs above 10 DU. We find that NAME is capable of capturing the spatial distribution of the features within the <inline-formula><mml:math id="M595" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud where the <inline-formula><mml:math id="M596" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs are larger than 10 DU on the order of 7–10 d (see Fig. <xref ref-type="fig" rid="Ch1.F9"/>).</p>
      <p id="d1e8476">Our work highlights that accurate information on ESPs is key when comparing model simulations to satellite retrievals. In reality it can be difficult to obtain this information, especially in near-real time. For example, observations show that the Raikoke eruption was actually characterised by a series of explosive eruptions that emitted <inline-formula><mml:math id="M597" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at varying heights <xref ref-type="bibr" rid="bib1.bibx18 bib1.bibx41 bib1.bibx67 bib1.bibx53" id="paren.80"/>. Furthermore a study by <xref ref-type="bibr" rid="bib1.bibx80" id="text.81"/> suggests that activity continued until 10:00 UTC on 22 June rather than 03:00 UTC as reported by the VolRes team. These examples indicate how hard it is to obtain a “correct” time-dependent emission profile for the eruption in near-real time. Instead, the profiles used in this study try to capture the time-averaged emission profiles of these “pulses” during the eruption. To test the importance of the emission duration, we conducted some additional simulations where we increased the duration of the eruption to 10:00 UTC on 22 June. The results of these new simulations (not shown) were very similar to the results presented in this paper, with the main difference that the structure of the cloud is slightly more diffuse.</p>
      <p id="d1e8496">For all the simulations we find that small changes in the vertical emission profile lead to a large change in the amount of mass emitted into the stratosphere, due to the emissions spanning the tropopause. In our analysis the mass-averaged emission height in the VolRes and StratProfile emission profiles differs by only 1 km (10.5 km in VolRes versus 11.5 km in StratProfile). But in the StratProfile emission profile we emit 69 % (1.09 Tg) of the total <inline-formula><mml:math id="M598" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass above the tropopause (as defined by the MetUM NWP), compared to 43 % (0.64 Tg) in the VolRes1.5 simulation.</p>
      <p id="d1e8511">NAME does not account for any radiative lofting effect and thus an emission profile derived during the first hours after the eruption could lead to <inline-formula><mml:math id="M599" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> at the wrong altitudes. <xref ref-type="bibr" rid="bib1.bibx67" id="text.82"/> show that for the Raikoke 2019 multi-phase plume, the radiative lofting effect for ash is on the order of 2–3 km during the first days after the eruption. While the precise impact of such a lofting effect on the <inline-formula><mml:math id="M600" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2<?pagebreak page10869?></mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud is difficult to quantify (<xref ref-type="bibr" rid="bib1.bibx8" id="altparen.83"/>; owing to lack of knowledge of the details of the relative vertical position on the <inline-formula><mml:math id="M601" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and the ash, and the lack of knowledge of the mixing state between the resulting sulfate aerosol and ash), it could help to explain the differences seen between the emission profiles used in this study. For the VolRes1.5 emission profile, which was derived during the first hours after the eruption, the radiative lofting effect is still limited. Instead for the StratProfile, which is derived 30 h after the eruption onset, the radiative lofting has very likely impacted the <inline-formula><mml:math id="M602" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud vertical structure as <xref ref-type="bibr" rid="bib1.bibx67" id="text.84"/> show that most of the lofting took place during the first 36 h after the Raikoke eruption. Therefore, we get a better comparison between the NAME simulations and observations by determining an effective emission profile from 1–2 d after the initial emission time to account for potential radiative lofting effects. Our study results show that the potential impact of radiative lofting should be considered by VAACs when producing forecasts for multi-phase plumes near the tropopause.</p>
      <p id="d1e8568">Interestingly while the fractional split of the mass between the stratosphere and troposphere is important, the detailed vertical distribution of <inline-formula><mml:math id="M603" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> within each of these two layers has only a minor effect on model performance. To test the sensitivity of the model results to the details of the vertical distribution of the emissions within the troposphere and stratosphere, we performed a simulation where we emitted 1 Tg evenly between 11–14 km and 0.5 Tg evenly between 9–11 km (not shown). The general conclusions were the same as shown for the StratProfile, illustrating that, for the 2019 Raikoke eruption, it is key to establish the fraction of the <inline-formula><mml:math id="M604" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass that was emitted into the stratosphere.</p>
      <p id="d1e8593">Also an error in the definition of the tropopause height within the MetUM (or any other NWP) model can have a large influence on the skill of the dispersion simulations. If, for example, the MetUM model-estimated tropopause height is 2 km above the actual observed tropopause height, this would lead to a wrong placement of the majority of the <inline-formula><mml:math id="M605" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass in the troposphere in our VolRes1.5 simulation. Using a different NWP model with a lower tropopause height in the NAME simulations would result in a higher fraction of the <inline-formula><mml:math id="M606" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass of the VolRes1.5 profile being emitted into the stratosphere and potentially give a better comparison with TROPOMI than the StratProfile estimate (which would overestimate the stratospheric <inline-formula><mml:math id="M607" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass in that case). However, we found the average tropopause height of <inline-formula><mml:math id="M608" display="inline"><mml:mrow><mml:mn mathvariant="normal">11.2</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> km diagnosed in the model at the eruption site is in good agreement with the observed tropopause height of <inline-formula><mml:math id="M609" display="inline"><mml:mrow><mml:mn mathvariant="normal">10.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.7</mml:mn></mml:mrow></mml:math></inline-formula> km from a nearby radiosonde location (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>), which gives us confidence that our StratProfile emission estimates for the stratosphere and troposphere are suitable and that the NAME results are not strongly biased by a wrong tropopause height within the NWP fields.</p>
      <p id="d1e8656">While we have investigated the impact of changing the vertical <inline-formula><mml:math id="M610" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profile (see Fig. <xref ref-type="fig" rid="Ch1.F2"/>), we have not investigated the effect of any uncertainty related to the atmospheric conditions in the NWP wind fields used as input for the NAME simulation. A study by <xref ref-type="bibr" rid="bib1.bibx20" id="text.85"/> shows that the impact of the atmospheric conditions on the NAME simulations can be large, especially in conditions of large horizontal flow separation in the atmosphere. The specific atmospheric conditions for this particular eruption (i.e. the low-pressure system east of the eruption site) show isobars that are parallel to each other during the first days after the eruption in the region of the cloud (Fig. <xref ref-type="fig" rid="Ch1.F3"/>). Therefore, it is expected that the impact of flow separation is limited during the initial stages of the cloud evolution. After several days, the flow separation becomes more pronounced in various regions in the domain (see Fig. <xref ref-type="fig" rid="Ch1.F6"/>). This effect is also reflected in the decrease in the <inline-formula><mml:math id="M611" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score value of the SAL diagram shown in Fig. <xref ref-type="fig" rid="Ch1.F10"/>, as trajectories start diverging in these regions of enhanced flow separation enhancing dispersion in the model. To better understand the impact of the NWP wind field variability on our results presented here, the analysis would need to be repeated using an ensemble of NWP wind field forecasts as input for the NAME simulations.</p>
      <p id="d1e8689">Our study of the 2019 Raikoke eruption demonstrates the strength of the SAL diagram for performing a comparison of model simulations with satellite observations and can help to determine potential issues. In this particular case, the NAME model simulations generally tend to show increasing positive <inline-formula><mml:math id="M612" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score values for all the simulations. Partly this is related to the diffusion parameterisation in the model, which smooths the signal (i.e. random perturbation) of the small-scale eddies within the cloud that are not present in the input wind field (see Sect. 2.3.1). As uncertainties from the meteorological conditions used as input for the simulations gradually accumulate, this leads to a larger spread in the <inline-formula><mml:math id="M613" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud over time than is observed in reality. This gives the tendency for the model to be more diffuse on longer timescales, as revealed by the <inline-formula><mml:math id="M614" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score increase in Fig. <xref ref-type="fig" rid="Ch1.F10"/>a–c.</p>
      <?pagebreak page10870?><p id="d1e8719">We find that the key reason for the increasing <inline-formula><mml:math id="M615" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score values on shorter timescales (i.e. 1–5 d) is related to the horizontal diffusion parameter <inline-formula><mml:math id="M616" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> used for the model simulations. NAME v8.1 uses a single value for the diffusion coefficient within the free atmosphere (see Table <xref ref-type="table" rid="Ch1.T1"/>). From literature it is known that mixing in the atmosphere can be highly variable and seasonally dependent  <xref ref-type="bibr" rid="bib1.bibx38 bib1.bibx2 bib1.bibx60 bib1.bibx1" id="paren.86"><named-content content-type="pre">e.g.</named-content></xref>. Furthermore, the diffusion parameter values currently used in NAME have been determined using observational datasets near the surface <xref ref-type="bibr" rid="bib1.bibx111" id="paren.87"/>. It is therefore possible that the mesoscale diffusion values used in the model might be unsuitable for the higher levels in the atmosphere, especially in the stratosphere, and thereby cause too much diffusion from the start of the eruption. To test this hypothesis, we investigated several simulations with a smaller horizontal diffusion coefficient (see Table <xref ref-type="table" rid="Ch1.T2"/>), where we reduce the mesoscale diffusion value <inline-formula><mml:math id="M617" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> by 75 % for the whole atmosphere above the boundary layer. The resulting values for the FSS score and SAL diagram for the StratProfile<inline-formula><mml:math id="M618" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> simulation are shown in Fig. <xref ref-type="fig" rid="Ch1.F10"/>d and Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/> and indicate that the simulations are better able to capture the structure (i.e. peak values and horizontal extent) of the cloud during the first 5 d of the simulations. It is currently impossible to determine a more precise value for the diffusion parameters, due to the lack of case studies and limited available observations for these high altitudes. Part of ongoing work is to investigate the impact of a new space and time-varying free-atmospheric turbulence scheme that is included in the latest version of NAME <xref ref-type="bibr" rid="bib1.bibx21" id="paren.88"/>, which was not available for the simulations presented in this paper.</p>
      <p id="d1e8781">A previous study by <xref ref-type="bibr" rid="bib1.bibx36" id="text.89"/> used a multi-level emulation approach to better understand the influence of model parameters on the accuracy of NAME output for volcanic ash concentration during the 2010 Eyjafjallajökull eruption. Their study showed a limited impact of the mesoscale diffusion parameter <inline-formula><mml:math id="M619" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> on their ash simulations for the 2010 Eyjafjallajökull eruption. This limited effect of <inline-formula><mml:math id="M620" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> is partly explained by the lower resolution (<inline-formula><mml:math id="M621" display="inline"><mml:mrow><mml:mn mathvariant="normal">40</mml:mn><mml:mo>×</mml:mo><mml:mn mathvariant="normal">40</mml:mn></mml:mrow></mml:math></inline-formula> km) of their model output. This leads to an averaging of small-scale eddies and a reduced impact of the diffusion parameterisation, something we also observed in our study when using a larger neighbourhood size <inline-formula><mml:math id="M622" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> in our calculations of the FSS score (see Fig. <xref ref-type="fig" rid="Ch1.F10"/> and Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>). Furthermore, the 2010 Eyjafjallajökull emissions were at lower altitude than for the Raikoke eruption, and <xref ref-type="bibr" rid="bib1.bibx36" id="text.90"/> only investigated the diffusion of the ash clouds, so a larger <inline-formula><mml:math id="M623" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> might be more appropriate. However, the reduced <inline-formula><mml:math id="M624" display="inline"><mml:mrow><mml:msub><mml:mi mathvariant="bold-italic">K</mml:mi><mml:mi mathvariant="normal">meso</mml:mi></mml:msub></mml:mrow></mml:math></inline-formula> values in our StratProfile<inline-formula><mml:math id="M625" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula> simulations are within the range of realistic values for the free atmosphere (see Table 1 in <xref ref-type="bibr" rid="bib1.bibx36" id="altparen.91"/>), and so this motivates more research to investigate the potential improvement of the model by having a more detailed representation of the mesoscale diffusion in the model at higher altitudes.</p>
      <p id="d1e8871">The results from our work are for a single case study, as 2019 Raikoke is the first eruption of this magnitude that has been observed by the high-spatial-resolution TROPOMI instrument. Nonetheless, our work shows the large potential of using TROPOMI <inline-formula><mml:math id="M626" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrievals (in combination with the correct AKs) to identify and rectify issues in dispersion modelling efforts of volcanic eruptions. Comparing high-resolution satellite measurements and dispersion model simulations is a valuable exercise that can help improve both the volcanic dispersion modelling tools and the satellite retrievals of volcanic plumes. By combining the information obtained from NAME, TROPOMI and IASI for Raikoke 2019, we are able to give a more detailed picture of the eruption source parameters and the dispersion of the volcanic <inline-formula><mml:math id="M627" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud than ever before. Even though we only considered this one case study, it becomes clear that improvements in ADMs simulating volcanic eruptions can be expected when more volcanic eruptions are investigated using this or similar frameworks.</p>
      <p id="d1e8896">While this study has focussed almost entirely on representing the evolution of the gas-phase sulfur in the form of <inline-formula><mml:math id="M628" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>, it is acknowledged that this is only part of the story. The Part 2 companion paper <xref ref-type="bibr" rid="bib1.bibx73" id="paren.92"/> focusses on assessing the fidelity of the NAME model in representing the resulting sulfate aerosol together with volcanic ash and any confounding effects from biomass burning aerosol that were emitted into the stratosphere from an unusually strong pyrocumulus event in continental North America.</p>
</sec>
<sec id="Ch1.S5" sec-type="conclusions">
  <label>5</label><title>Conclusions</title>
      <p id="d1e8922">Volcanic eruptions can pose a large threat to society and in particular the aviation industry. In this study we simulated the 2019 Raikoke eruption using the Met Office's Numerical Atmospheric-dispersion Modelling Environment (NAME). The 21–22 June 2019 Raikoke eruption emitted <inline-formula><mml:math id="M629" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.5</mml:mn><mml:mo>±</mml:mo><mml:mn mathvariant="normal">0.2</mml:mn></mml:mrow></mml:math></inline-formula> Tg of <inline-formula><mml:math id="M630" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the UT/LS. We evaluated the skill and limitations of NAME to simulate the dispersion of the resulting volcanic <inline-formula><mml:math id="M631" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud by comparing our simulations to high-spatial-resolution satellite measurements from the TROPOspheric Monitoring Instrument (TROPOMI). Based on our analysis we conclude the following.
<list list-type="bullet"><list-item>
      <p id="d1e8961">NAME accurately simulates the observed location and horizontal extent of the <inline-formula><mml:math id="M632" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud during the first 2–3 weeks after the eruption (Figs. <xref ref-type="fig" rid="Ch1.F6"/> and <xref ref-type="fig" rid="Ch1.F7"/>). Based on the fractional skill score (FSS), we find that our simulations have skill out to 12–17 d when considering the 1 DU <inline-formula><mml:math id="M633" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD contour (Fig. <xref ref-type="fig" rid="Ch1.F10"/> and Table <xref ref-type="table" rid="App1.Ch1.S1.T3"/>). For <inline-formula><mml:math id="M634" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs larger than 20 DU, the model performs less well and has skill on the order of 2–4 d only (Fig. <xref ref-type="fig" rid="Ch1.F9"/>).</p></list-item><list-item>
      <?pagebreak page10871?><p id="d1e9009">Based on both the FSS score and structure, amplitude and location (SAL) metric (Fig. <xref ref-type="fig" rid="Ch1.F10"/>), we find that the model-simulated <inline-formula><mml:math id="M635" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud in NAME is more diffuse than in the TROPOMI measurements, in particular for <inline-formula><mml:math id="M636" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCDs exceeding 20 DU. The diffusion parameterisation in NAME, which is developed for the lower free troposphere, results in too much horizontal spread in the lower stratosphere and therefore leads to a fast reduction of <inline-formula><mml:math id="M637" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass concentrations in the densest parts of the eruption cloud right from the start of the eruption. This is reflected by the high positive <inline-formula><mml:math id="M638" display="inline"><mml:mi>S</mml:mi></mml:math></inline-formula> score of the SAL diagram shown in Fig. <xref ref-type="fig" rid="Ch1.F10"/> when compared to TROPOMI. Reducing the horizontal diffusion parameters in NAME results in a better agreement during the first 5 d of the simulation (Fig. <xref ref-type="fig" rid="Ch1.F10"/>d) but has no significant impact on timescales longer than that. We therefore suggest that the horizontal diffusion parameters currently used in NAME are potentially too large in the UT and LS, and different values should be considered when investigating dispersion processes near the tropopause and in the stratosphere. Our reduced horizontal diffusion parameter values are within the range of values found in the literature for LS mixing <xref ref-type="bibr" rid="bib1.bibx4 bib1.bibx108" id="paren.93"><named-content content-type="pre">e.g.</named-content></xref>. However, we are not able to determine exact values for the diffusion parameters on the basis of this single volcanic eruption case study with one NWP representation and one set of detailed observations. In the future, as more eruption case studies become available, there is a potential to constrain the values of these diffusion parameters in order to better represent the diffusion of upper tropospheric and stratosphere volcanic <inline-formula><mml:math id="M639" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> clouds in NAME and other ADMs.</p></list-item><list-item>
      <p id="d1e9076">For the 2019 Raikoke eruption, we find that the skill of the model strongly depends on the eruption source parameter used for the simulation. Using the Volcanic Response team profile (VolRes1.5 Fig. <xref ref-type="fig" rid="Ch1.F2"/>), we find that NAME removes too much <inline-formula><mml:math id="M640" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass from the atmosphere during the first week of the simulations (Fig. <xref ref-type="fig" rid="Ch1.F11"/>), resulting in a shorter <inline-formula><mml:math id="M641" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time in the simulation than estimated based on TROPOMI data (<inline-formula><mml:math id="M642" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of 9 d for VolRes1.5 versus 21 d in TROPOMI between 23–27 June). A large fraction of the tropospheric <inline-formula><mml:math id="M643" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass is removed from the atmosphere in the warm conveyor belt region of the cyclone east of the eruption site during the first week of the simulation. NAME performs better with the StratProfile emission profile, where a larger fraction of the total <inline-formula><mml:math id="M644" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass is emitted into the stratosphere (1.09 Tg versus 0.64 Tg; see Fig. <xref ref-type="fig" rid="Ch1.F2"/> and Table <xref ref-type="table" rid="Ch1.T2"/>). When emitting 0.9–1.1 Tg of <inline-formula><mml:math id="M645" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> into the LS and 0.4–0.7 Tg into the UT, we obtain the best agreement with TROPOMI, both in terms of the peak <inline-formula><mml:math id="M646" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass burden and the <inline-formula><mml:math id="M647" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of <inline-formula><mml:math id="M648" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M649" display="inline"><mml:mi>e</mml:mi></mml:math></inline-formula>-folding time of 14–15 d).</p></list-item></list></p>
      <p id="d1e9183">Determining the vertical <inline-formula><mml:math id="M650" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profile for any volcanic eruption from observations is one of the most difficult and challenging tasks the community faces. Our analysis shows that determining the details of the vertical profiles is essential in particular for eruptions that only just straddle the stratosphere in order to accurately forecast the dispersion of volcanic <inline-formula><mml:math id="M651" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula>. This study demonstrates that combining observational datasets with dispersion model estimates can be beneficial to obtain a more detailed estimate of the volcanic <inline-formula><mml:math id="M652" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> emission profile. The attempts in this paper to give more details on the vertical emission profile are basic, and more sophisticated near-real-time estimates are currently being developed by the scientific community <xref ref-type="bibr" rid="bib1.bibx56 bib1.bibx6 bib1.bibx65 bib1.bibx106 bib1.bibx74" id="paren.94"><named-content content-type="pre">e.g.</named-content></xref>. With the current efforts, we expect that estimates of volcanic <inline-formula><mml:math id="M653" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> fluxes will become more detailed and will very likely lead to a significant improvement of model simulations of future eruptions.</p>
      <p id="d1e9235"><?xmltex \hack{\newpage}?>Finally, the average cruise altitudes for long-haul aircraft (11.9–13.7 km) fall well within the altitudes where the volcanic <inline-formula><mml:math id="M654" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> cloud for the 2019 Raikoke eruption was observed (see Fig. <xref ref-type="fig" rid="Ch1.F4"/>); thus eruptions like the 2019 Raikoke eruption may pose a hazard to the aviation industry. Having reliable dispersion models to simulate volcanic clouds is crucial to better understand and mitigate their potential impacts. We have shown that the FSS and the SAL score metrics are potentially very powerful tools when assessing the skill of the model simulations in comparison with satellite measurements. The FSS score gives insight into the timescales over which the model has skill and also shows at what resolution results are significant. The SAL score gives a more detailed overview on three different aspects of the cloud properties (shape, location and mass) and helps to identify what aspects of the eruption cloud are well represented in a model. Using the two metrics in tandem gives a good overview of the strengths and weaknesses of the simulation and helps to interpret the results of the forecast model in more detail. While we have applied the metrics to the NAME model and the TROPOMI retrievals, they can also be easily applied to any combination of dispersion models and spatial observations. It could therefore also be a useful tool to inter-compare skills of satellite observation products and/or multiple dispersion models.</p><?xmltex \hack{\clearpage}?>
</sec>

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

<?pagebreak page10872?><app id="App1.Ch1.S1">
  <?xmltex \currentcnt{A}?><label>Appendix A</label><title>Derivation of StratProfile vertical emission profile</title>
      <p id="d1e9264">To investigate the sensitivity of the results to the <inline-formula><mml:math id="M655" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass fraction that is emitted into the stratosphere, we derive a new emission profile based on the TROPOMI <inline-formula><mml:math id="M656" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD on 23 June in combination with the 36 h NAME VolRes1.5 simulation. Using Fig. <xref ref-type="fig" rid="Ch1.F3"/>d, we scale the VolRes1.5 <inline-formula><mml:math id="M657" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD estimates at each longitude to represent the TROPOMI <inline-formula><mml:math id="M658" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD values along cross section I–II, and using Fig. <xref ref-type="fig" rid="Ch1.F4"/> we simultaneously derive the corresponding cloud height for the VolRes1.5 vertical profile at each point along the cross section. The obtained scaling and altitude of the cloud at each longitude are then combined to apply a scaling to the VolRes1.5 emission profile (Fig. <xref ref-type="fig" rid="Ch1.F2"/>). We only determine the scaling where the modelled cloud thickness is less than 4 km (between 157 and 176<inline-formula><mml:math id="M659" display="inline"><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup></mml:math></inline-formula> E), resulting in a scaling factor for the emission profile levels between 9 and 18 km. The resulting StratProfile shown in Fig. <xref ref-type="fig" rid="Ch1.F2"/> emits 1.57 Tg of <inline-formula><mml:math id="M660" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> mass, which is very similar to the mass emitted by VolRes1.5. However, this new profile emits a much higher fraction of the mass into the stratosphere (1.09 Tg versus 0.64 Tg; see Table <xref ref-type="table" rid="Ch1.T2"/>). The results for the StratProfile simulations on 23 June are presented in Fig. <xref ref-type="fig" rid="Ch1.F3"/>c and d and, as expected, show a better comparison with the TROPOMI satellite <inline-formula><mml:math id="M661" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> VCD retrievals at this particular time. A more detailed vertical emission profile could be constructed using sophisticated inverse modelling techniques <xref ref-type="bibr" rid="bib1.bibx27 bib1.bibx56 bib1.bibx65" id="paren.95"><named-content content-type="pre">e.g.</named-content></xref>, but this is beyond the scope of this paper and is not attempted here.</p><?xmltex \hack{\clearpage}?><?xmltex \floatpos{h!}?><table-wrap id="App1.Ch1.S1.T3"><?xmltex \hack{\hsize\textwidth}?><?xmltex \currentcnt{A1}?><label>Table A1</label><caption><p id="d1e9365">The FSS-based timescales estimates for which the NAME simulations have skill compared to TROPOMI at the given spatial resolution <inline-formula><mml:math id="M662" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula>. The given values represent the number of days after start of eruption (rounded by 0.5 d) where the FSS comparison between the NAME simulations and the TROPOMI retrievals drops below 0.5 for various neighbourhood <inline-formula><mml:math id="M663" display="inline"><mml:mi>N</mml:mi></mml:math></inline-formula> sizes (value in brackets shows the corresponding model resolution for which the values would be valid), maximum included vertical column density contours and NAME simulations. When calculating the daily FSS value, we only include overpasses where the satellite-retrieved total mass was above 0.2 Tg to remove noise. When the model still has skill FSS <inline-formula><mml:math id="M664" display="inline"><mml:mo>&gt;</mml:mo></mml:math></inline-formula> 0.6 on the last day where we could determine FSS (17 d), we represent this with a bold number, indicating that the value could be higher than what is presented here.</p></caption><oasis:table frame="topbot"><oasis:tgroup cols="9">
     <oasis:colspec colnum="1" colname="col1" align="left"/>
     <oasis:colspec colnum="2" colname="col2" align="center"/>
     <oasis:colspec colnum="3" colname="col3" align="right"/>
     <oasis:colspec colnum="4" colname="col4" align="right"/>
     <oasis:colspec colnum="5" colname="col5" align="right"/>
     <oasis:colspec colnum="6" colname="col6" align="right"/>
     <oasis:colspec colnum="7" colname="col7" align="right"/>
     <oasis:colspec colnum="8" colname="col8" align="right"/>
     <oasis:colspec colnum="9" colname="col9" align="right"/>
     <oasis:thead>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1"/>
         <oasis:entry colname="col2">0.3 DU</oasis:entry>
         <oasis:entry colname="col3">1 DU</oasis:entry>
         <oasis:entry colname="col4">5 DU</oasis:entry>
         <oasis:entry colname="col5">10 DU</oasis:entry>
         <oasis:entry colname="col6">20 DU</oasis:entry>
         <oasis:entry colname="col7">30 DU</oasis:entry>
         <oasis:entry colname="col8">40 DU</oasis:entry>
         <oasis:entry colname="col9">50 DU</oasis:entry>
       </oasis:row>
     </oasis:thead>
     <oasis:tbody>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col9"><inline-formula><mml:math id="M665" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">1</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M666" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.2</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">20</mml:mn></mml:mrow></mml:math></inline-formula> km) </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5</oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">12.5</oasis:entry>
         <oasis:entry colname="col4">9</oasis:entry>
         <oasis:entry colname="col5">2.5</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">1</oasis:entry>
         <oasis:entry colname="col8">1</oasis:entry>
         <oasis:entry colname="col9">1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes2.0</oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">12</oasis:entry>
         <oasis:entry colname="col4">9.5</oasis:entry>
         <oasis:entry colname="col5">2.5</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">1.5</oasis:entry>
         <oasis:entry colname="col8">1</oasis:entry>
         <oasis:entry colname="col9">1</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile</oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">14.5</oasis:entry>
         <oasis:entry colname="col4">10.5</oasis:entry>
         <oasis:entry colname="col5">9.5</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5<inline-formula><mml:math id="M667" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">12.5</oasis:entry>
         <oasis:entry colname="col4">9</oasis:entry>
         <oasis:entry colname="col5">3</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">1.5</oasis:entry>
         <oasis:entry colname="col8">1</oasis:entry>
         <oasis:entry colname="col9">1</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">StratProfile<inline-formula><mml:math id="M668" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">14.5</oasis:entry>
         <oasis:entry colname="col4">10.5</oasis:entry>
         <oasis:entry colname="col5">9.5</oasis:entry>
         <oasis:entry colname="col6">5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col9"><inline-formula><mml:math id="M669" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">9</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M670" display="inline"><mml:mrow><mml:mn mathvariant="normal">0.6</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">60</mml:mn></mml:mrow></mml:math></inline-formula> km) </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5</oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">13</oasis:entry>
         <oasis:entry colname="col4">9</oasis:entry>
         <oasis:entry colname="col5">4.5</oasis:entry>
         <oasis:entry colname="col6">2</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes2.0</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">14</oasis:entry>
         <oasis:entry colname="col4">10</oasis:entry>
         <oasis:entry colname="col5">5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">15</oasis:entry>
         <oasis:entry colname="col4">11</oasis:entry>
         <oasis:entry colname="col5">9.5</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4</oasis:entry>
         <oasis:entry colname="col8">2.5</oasis:entry>
         <oasis:entry colname="col9">2</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5<inline-formula><mml:math id="M671" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2">17</oasis:entry>
         <oasis:entry colname="col3">13.5</oasis:entry>
         <oasis:entry colname="col4">9.5</oasis:entry>
         <oasis:entry colname="col5">4</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">StratProfile<inline-formula><mml:math id="M672" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">15</oasis:entry>
         <oasis:entry colname="col4">11.5</oasis:entry>
         <oasis:entry colname="col5">10</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4</oasis:entry>
         <oasis:entry colname="col8">2.5</oasis:entry>
         <oasis:entry colname="col9">2</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col9"><inline-formula><mml:math id="M673" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">25</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M674" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.0</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">100</mml:mn></mml:mrow></mml:math></inline-formula> km) </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">13.5</oasis:entry>
         <oasis:entry colname="col4">9</oasis:entry>
         <oasis:entry colname="col5">5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes2.0</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">14</oasis:entry>
         <oasis:entry colname="col4">10.5</oasis:entry>
         <oasis:entry colname="col5">5.5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col4">11</oasis:entry>
         <oasis:entry colname="col5">9.5</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4</oasis:entry>
         <oasis:entry colname="col8">3</oasis:entry>
         <oasis:entry colname="col9">2.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5<inline-formula><mml:math id="M675" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">13.5</oasis:entry>
         <oasis:entry colname="col4">9.5</oasis:entry>
         <oasis:entry colname="col5">5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">1.5</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry colname="col1">StratProfile<inline-formula><mml:math id="M676" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col4">11.5</oasis:entry>
         <oasis:entry colname="col5">10</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4.5</oasis:entry>
         <oasis:entry colname="col8">3</oasis:entry>
         <oasis:entry colname="col9">2.5</oasis:entry>
       </oasis:row>
       <oasis:row rowsep="1">
         <oasis:entry namest="col1" nameend="col9"><inline-formula><mml:math id="M677" display="inline"><mml:mrow><mml:mi>N</mml:mi><mml:mo>=</mml:mo><mml:mn mathvariant="normal">49</mml:mn></mml:mrow></mml:math></inline-formula> (<inline-formula><mml:math id="M678" display="inline"><mml:mrow><mml:mn mathvariant="normal">1.4</mml:mn><mml:msup><mml:mi/><mml:mo>∘</mml:mo></mml:msup><mml:mo>≈</mml:mo><mml:mn mathvariant="normal">140</mml:mn></mml:mrow></mml:math></inline-formula> km) </oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">13.5</oasis:entry>
         <oasis:entry colname="col4">9</oasis:entry>
         <oasis:entry colname="col5">5.5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes2.0</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">14.5</oasis:entry>
         <oasis:entry colname="col4">10.5</oasis:entry>
         <oasis:entry colname="col5">7</oasis:entry>
         <oasis:entry colname="col6">3</oasis:entry>
         <oasis:entry colname="col7">2.5</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile</oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col4">11.5</oasis:entry>
         <oasis:entry colname="col5">10</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4.5</oasis:entry>
         <oasis:entry colname="col8">3</oasis:entry>
         <oasis:entry colname="col9">2.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">VolRes1.5<inline-formula><mml:math id="M679" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3">14</oasis:entry>
         <oasis:entry colname="col4">9.5</oasis:entry>
         <oasis:entry colname="col5">5</oasis:entry>
         <oasis:entry colname="col6">2.5</oasis:entry>
         <oasis:entry colname="col7">2</oasis:entry>
         <oasis:entry colname="col8">2</oasis:entry>
         <oasis:entry colname="col9">1.5</oasis:entry>
       </oasis:row>
       <oasis:row>
         <oasis:entry colname="col1">StratProfile<inline-formula><mml:math id="M680" display="inline"><mml:msub><mml:mi/><mml:mi mathvariant="normal">rd</mml:mi></mml:msub></mml:math></inline-formula></oasis:entry>
         <oasis:entry colname="col2"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col3"><bold>17</bold></oasis:entry>
         <oasis:entry colname="col4">11.5</oasis:entry>
         <oasis:entry colname="col5">10.5</oasis:entry>
         <oasis:entry colname="col6">5.5</oasis:entry>
         <oasis:entry colname="col7">4.5</oasis:entry>
         <oasis:entry colname="col8">3</oasis:entry>
         <oasis:entry colname="col9">2.5</oasis:entry>
       </oasis:row>
     </oasis:tbody>
   </oasis:tgroup></oasis:table></table-wrap>

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

      <p id="d1e10293">Code and simulation data used in this paper may be requested from the corresponding author and can be downloaded from <ext-link xlink:href="https://doi.org/10.5281/zenodo.4729991" ext-link-type="DOI">10.5281/zenodo.4729991</ext-link> <xref ref-type="bibr" rid="bib1.bibx25" id="paren.96"/>. The TROPOMI satellite data can be downloaded from the ESA website (<uri>https://s5phub.copernicus.eu</uri>, last access: 9 December 2020) <xref ref-type="bibr" rid="bib1.bibx16" id="paren.97"/>. Isabelle A. Taylor and Roy G. Grainger plan to archive the Oxford IASI <inline-formula><mml:math id="M681" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> products for the Raikoke eruption; in the meantime these can made available on request from Isabelle A. Taylor (isabelle.taylor@physics.ox.ac.uk). Radiosonde data are available at <uri>http://weather.uwyo.edu/upperair/sounding.html</uri>  <xref ref-type="bibr" rid="bib1.bibx70" id="paren.98"/>. The NAME code is available under license from the Met Office.</p>
  </notes><notes notes-type="videosupplement"><title>Video supplement</title>

      <p id="d1e10329">Videos of the <inline-formula><mml:math id="M682" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> and <inline-formula><mml:math id="M683" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">4</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> NAME VCD simulations for the VolRes1.5 and the StratProfile emission profiles can be found at <ext-link xlink:href="https://doi.org/10.5281/zenodo.3992052" ext-link-type="DOI">10.5281/zenodo.3992052</ext-link> <xref ref-type="bibr" rid="bib1.bibx24" id="paren.99"/>.</p>
  </notes><notes notes-type="authorcontribution"><title>Author contributions</title>

      <p id="d1e10363">JdL, AS and CSW designed the project. JdL set up and performed all the NAME simulations and analysed the results. AS, CSW, MO and JH contributed to the scientific discussion and interpretation of the results. NK provided model input files for the initial NAME simulations. JdL, NT and RJP were responsible for the preparation of the TROPOMI data for the comparison with the NAME output. IT and RG processed the IASI data for the comparison. AS, CSW and RGG obtained the funding for this work. JdL, AS and CSW prepared the manuscript. All the authors reviewed the manuscript.</p>
  </notes><notes notes-type="competinginterests"><title>Competing interests</title>

      <p id="d1e10369">The authors declare that they have no conflict of interest.</p>
  </notes><notes notes-type="sistatement"><title>Special issue statement</title>

      <p id="d1e10375">This article is part of the special issue “Satellite observations, in situ measurements and model simulations of the 2019 Raikoke eruption (ACP/AMT/GMD inter-journal SI)”. It is not associated with a conference.</p>
  </notes><ack><title>Acknowledgements</title><p id="d1e10381">Johannes de Leeuw, Anja Schmidt, Claire S. Witham, Roy G. Grainger and Isabelle A. Taylor acknowledge funding from the Natural Environment Research Council (NERC) V-PLUS grants NE/S00436X/1 and NE/S004025/1. Isabelle A. Taylor and Roy G. Grainger are supported by the NERC Centre for Observation and Modelling of Earthquakes, Volcanoes, and Tectonics (COMET). Nicolas Theys acknowledges financial support from ESA S5P MPC (4000117151/16/I-LG) and Belgium Prodex TRACE-S5P (PEA 4000105598) projects. Funding for PhD work for Martin Osborne was provided by NERC through the University of Exeter, grant NE/M009416/1. Contributions from Jim Haywood and Anja Schmidt benefitted from support by the NERC ADVANCE (Aerosol-cloud-climate interactions derived from Degassing VolcANiC Eruptions), grant NE/T006897/1. The authors would like to thank Helen Webster (Met Office) for helpful discussions on the NAME diffusion parameterisations and Peter Haynes for our discussions on stratospheric mixing. We also like to acknowledge Andrew Prata  and the anonymous reviewer for their comments and suggestions. This work used JASMIN, the UK collaborative data analysis facility (<ext-link xlink:href="https://doi.org/10.1109/BigData.2013.6691556" ext-link-type="DOI">10.1109/BigData.2013.6691556</ext-link>), to run all the simulations and to run the IASI <inline-formula><mml:math id="M684" display="inline"><mml:mrow class="chem"><mml:msub><mml:mi mathvariant="normal">SO</mml:mi><mml:mn mathvariant="normal">2</mml:mn></mml:msub></mml:mrow></mml:math></inline-formula> retrieval. We would like to acknowledge EUMETSAT for providing the IASI spectra, as well as ECMWF and CEDA for the meteorological profiles used in the IASI retrievals <xref ref-type="bibr" rid="bib1.bibx29" id="paren.100"/>.</p></ack><notes notes-type="financialsupport"><title>Financial support</title>

      <p id="d1e10403">This research has been supported by the Natural Environment Research Council (grant nos. NE/S00436X/1, NE/M009416/1, NE/T006897/1 and NE/S004025/1), ESA S5P MPC (grant no. 4000117151/16/I-LG) and Belgium Prodex TRACE-S5P (grant no. PEA 4000105598).</p>
  </notes><notes notes-type="reviewstatement"><title>Review statement</title>

      <p id="d1e10409">This paper was edited by Yves Balkanski and reviewed by Andrew Prata and one anonymous referee.</p>
  </notes><ref-list>
    <title>References</title>

      <ref id="bib1.bibx1"><?xmltex \def\ref@label{{Abalos et~al.(2016)Abalos, Legras, and Shuckburgh}}?><label>Abalos et al.(2016)Abalos, Legras, and Shuckburgh</label><?label abalos2016?><mixed-citation>Abalos, M., Legras, B., and Shuckburgh, E.: Interannual variability in
effective diffusivity in the upper troposphere/lower stratosphere from
reanalysis data, Q. J. Roy. Meteorol. Soc., 142, 1847–1861,
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    <!--<article-title-html>The 2019 Raikoke volcanic eruption – Part 1: Dispersion model simulations and satellite retrievals of volcanic sulfur dioxide</article-title-html>
<abstract-html><p>Volcanic eruptions can cause significant disruption to society, and numerical models are crucial for forecasting the dispersion of erupted material. Here we assess the skill and limitations of the Met Office's Numerical Atmospheric-dispersion Modelling Environment (NAME) in simulating the dispersion of the sulfur dioxide (SO<sub>2</sub>) cloud from the 21–22 June 2019 eruption of the Raikoke volcano (48.3°&thinsp;N, 153.2°&thinsp;E). The eruption emitted around 1.5±0.2&thinsp;Tg of SO<sub>2</sub>, which represents the largest volcanic emission of SO<sub>2</sub> into the stratosphere since the 2011 Nabro eruption. We simulate the temporal evolution of the volcanic SO<sub>2</sub> cloud across the Northern Hemisphere (NH) and compare our model simulations to high-resolution SO<sub>2</sub> measurements from the TROPOspheric Monitoring Instrument (TROPOMI) and the Infrared Atmospheric Sounding Interferometer (IASI) satellite SO<sub>2</sub> products.</p><p>We show that NAME accurately simulates the observed location and horizontal extent of the SO<sub>2</sub> cloud during the first 2–3 weeks after the eruption but is unable, in its standard configuration, to capture the extent and precise location of the highest magnitude vertical column density (VCD) regions within the observed volcanic cloud. Using the structure–amplitude–location (SAL) score and the fractional skill score (FSS) as metrics for model skill, NAME shows skill in simulating the horizontal extent of the cloud for 12–17&thinsp;d after the eruption where VCDs of SO<sub>2</sub> (in Dobson units, DU) are above 1&thinsp;DU. For SO<sub>2</sub> VCDs above 20&thinsp;DU, which are predominantly observed as small-scale features within the SO<sub>2</sub> cloud, the model shows skill on the order of 2–4&thinsp;d only. The lower skill for these high-SO<sub>2</sub>-VCD regions is partly explained by the model-simulated SO<sub>2</sub> cloud in NAME being too diffuse compared to TROPOMI retrievals. Reducing the standard horizontal diffusion parameters used in NAME by a factor of 4 results in a slightly increased model skill during the first 5&thinsp;d of the simulation, but on longer timescales the simulated SO<sub>2</sub> cloud remains too diffuse when compared to TROPOMI measurements.</p><p>The skill of NAME to simulate high SO<sub>2</sub> VCDs and the temporal evolution of the NH-mean SO<sub>2</sub> mass burden is dominated by the fraction of SO<sub>2</sub> mass emitted into the lower stratosphere, which is uncertain for the 2019 Raikoke eruption. When emitting 0.9–1.1&thinsp;Tg of SO<sub>2</sub> into the lower stratosphere (11–18&thinsp;km) and 0.4–0.7&thinsp;Tg into the upper troposphere (8–11&thinsp;km), the NAME simulations show a similar peak in SO<sub>2</sub> mass burden to that derived from TROPOMI (1.4–1.6&thinsp;Tg of SO<sub>2</sub>) with an average SO<sub>2</sub> <i>e</i>-folding time of 14–15&thinsp;d in the NH.</p><p>Our work illustrates how the synergy between high-resolution satellite retrievals and dispersion models can identify potential limitations of dispersion models like NAME, which will ultimately help to improve dispersion modelling efforts of volcanic SO<sub>2</sub> clouds.</p></abstract-html>
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