<?xml version="1.0" encoding="UTF-8"?>
<!DOCTYPE article PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "https://jats.nlm.nih.gov/nlm-dtd/publishing/3.0/journalpublishing3.dtd">
<article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" article-type="research-article" specific-use="SMUR" dtd-version="3.0" xml:lang="en">
<front>
<journal-meta>
<journal-id journal-id-type="publisher">EGUsphere</journal-id>
<journal-title-group>
<journal-title>EGUsphere</journal-title>
<abbrev-journal-title abbrev-type="publisher">EGUsphere</abbrev-journal-title>
<abbrev-journal-title abbrev-type="nlm-ta">EGUsphere</abbrev-journal-title>
</journal-title-group>
<issn pub-type="epub"></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/egusphere-2026-2572</article-id>
<title-group>
<article-title>A deep learning-driven emission estimator utilizing a mixture of experts for local wind speed situations applied to high-resolution methane imagery</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Plewa</surname>
<given-names>Thomas</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Butz</surname>
<given-names>André</given-names>
<ext-link>https://orcid.org/0000-0003-0593-1608</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Frankenberg</surname>
<given-names>Christian</given-names>
<ext-link>https://orcid.org/0000-0002-0546-5857</ext-link>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Thorpe</surname>
<given-names>Andrew K.</given-names>
<ext-link>https://orcid.org/0000-0001-7968-5433</ext-link>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Marshall</surname>
<given-names>Julia</given-names>
<ext-link>https://orcid.org/0000-0003-2648-128X</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
<xref ref-type="aff" rid="aff7">
<sup>7</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Institute of Environmental Physics (IUP), Heidelberg University, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Deutsches Zentrum für Luft- und Raumfahrt, Institut für Physik der Atmosphäre, Oberpfaffenhofen, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Heidelberg Center for the Environment (HCE), Heidelberg University, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Interdisciplinary Center for Scientific Computing (IWR), Heidelberg University, Heidelberg, Germany</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125, USA</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91125, USA</addr-line>
</aff>
<aff id="aff7">
<label>7</label>
<addr-line>Leipzig Institute for Meteorology, Leipzig University, Leipzig, Germany</addr-line>
</aff>
<pub-date pub-type="epub">
<day>28</day>
<month>05</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>27</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Thomas Plewa et al.</copyright-statement>
<copyright-year>2026</copyright-year>
<license license-type="open-access">
<license-p>This work is licensed under the Creative Commons Attribution 4.0 International License. To view a copy of this licence, visit <ext-link ext-link-type="uri"  xlink:href="https://creativecommons.org/licenses/by/4.0/">https://creativecommons.org/licenses/by/4.0/</ext-link></license-p>
</license>
</permissions>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2572/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2572/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2572/egusphere-2026-2572.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2572/egusphere-2026-2572.pdf</self-uri>
<abstract>
<p>Methane (CH&lt;sub&gt;4&lt;/sub&gt;) is the anthropogenic greenhouse gas with the second-highest impact on the Earth&apos;s radiative budget since pre-industrial times. A substantial amount of CH&lt;sub&gt;4&lt;/sub&gt; emissions are from the fossil fuel industry and are emitted from point-like sources that can be measured using airborne or space-based spectrometers. The precise quantification of point-source emissions has proven to be difficult, with uncertainties driven by the lack of local wind speed measurements and the task of estimating the effective wind speed of the plume. Here, we continue the development of deep learning-based methods using convolutional neural networks (CNN) to estimate emissions without the need for auxiliary wind speed information. We use a library of plumes obtained from large-eddy-simulations (LES) and realistic background noise scenes from the Airborne Visible/Infrared Imaging Spectrometer (AVIRIS-NG), used in previous studies, to generate realistic synthetic data. We suggest a mixture of experts (MoE) architecture, that is able to extract the wind speed forcing used in the LES and to estimate emission rates conditional on the wind speed present in the scenes. This allows us to integrate the concept of different wind speed scenarios into the network architecture, making the performance of the network more transparent and explainable and, while still being independent of external wind speed information, makes it possible to use external wind speed information to validate or improve emission estimates. The MoE-based network, without any external wind speed information, provides a mean absolute percentage error (MAPE) of 5.65 % for scenes with CH&lt;sub&gt;4&lt;/sub&gt; emission rates exceeding 100 kg h&lt;sup&gt;-1&lt;/sup&gt;, which is a 40 % improvement compared to previous implementations. The proposed network is also able to address biases at high wind speed situations, leading to almost unbiased estimates over the entire emission and wind speed domain.</p>
</abstract>
<counts><page-count count="27"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>Bundesministerium für Wirtschaft und Klimaschutz</funding-source>
<award-id>FZK50EE2212</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
<body/>
<back>
</back>
</article>