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<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-2026-2054</article-id>
<title-group>
<article-title>First results from the Juice magnetometer during the Lunar-Earth Gravity Assist</article-title>
</title-group>
<contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>LaMoury</surname>
<given-names>Adrian T.</given-names>
<ext-link>https://orcid.org/0000-0003-1551-5325</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Schulz</surname>
<given-names>Leonard</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Betzler</surname>
<given-names>Alexander</given-names>
</name>
<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>Hercik</surname>
<given-names>David</given-names>
</name>
<xref ref-type="aff" rid="aff5">
<sup>5</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Auster</surname>
<given-names>Hans-Ulrich</given-names>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Brown</surname>
<given-names>Patrick</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Magnes</surname>
<given-names>Werner</given-names>
<ext-link>https://orcid.org/0000-0003-0086-6288</ext-link>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Amtmann</surname>
<given-names>Christoph</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Baughen</surname>
<given-names>Richard</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Cao</surname>
<given-names>Hao</given-names>
</name>
<xref ref-type="aff" rid="aff6">
<sup>6</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Jernej</surname>
<given-names>Irmgard</given-names>
</name>
<xref ref-type="aff" rid="aff3">
<sup>3</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Lammegger</surname>
<given-names>Roland</given-names>
</name>
<xref ref-type="aff" rid="aff4">
<sup>4</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Masters</surname>
<given-names>Adam</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Plaschke</surname>
<given-names>Ferdinand</given-names>
<ext-link>https://orcid.org/0000-0002-5104-6282</ext-link>
</name>
<xref ref-type="aff" rid="aff2">
<sup>2</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Yu</surname>
<given-names>Xun</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Pomfret</surname>
<given-names>Taylor</given-names>
<ext-link>https://orcid.org/0009-0009-9121-3063</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Strickland</surname>
<given-names>Alex</given-names>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Garg</surname>
<given-names>Vaibhav</given-names>
<ext-link>https://orcid.org/0000-0002-9242-7962</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
<contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Dougherty</surname>
<given-names>Michele K.</given-names>
<ext-link>https://orcid.org/0000-0002-9658-8085</ext-link>
</name>
<xref ref-type="aff" rid="aff1">
<sup>1</sup>
</xref>
</contrib>
</contrib-group><aff id="aff1">
<label>1</label>
<addr-line>Blackett Laboratory, Imperial College London, London, UK</addr-line>
</aff>
<aff id="aff2">
<label>2</label>
<addr-line>Institut für Geophysik und extraterrestrische Physik, Technische Universität Braunschweig, Braunschweig, Germany</addr-line>
</aff>
<aff id="aff3">
<label>3</label>
<addr-line>Space Research Institute, Austrian Academy of Sciences, Graz, Austria</addr-line>
</aff>
<aff id="aff4">
<label>4</label>
<addr-line>Institute of Experimental Physics, Graz University of Technology, Graz, Austria</addr-line>
</aff>
<aff id="aff5">
<label>5</label>
<addr-line>Institute of Atmospheric Physics, Czech Academy of Sciences, Prague, Czechia</addr-line>
</aff>
<aff id="aff6">
<label>6</label>
<addr-line>Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles, Los Angeles, USA</addr-line>
</aff>
<pub-date pub-type="epub">
<day>15</day>
<month>04</month>
<year>2026</year>
</pub-date>
<volume>2026</volume>
<fpage>1</fpage>
<lpage>19</lpage>
<permissions>
<copyright-statement>Copyright: &#x000a9; 2026 Adrian T. LaMoury 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-2026-2054/">This article is available from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2054/</self-uri>
<self-uri xlink:href="https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2054/egusphere-2026-2054.pdf">The full text article is available as a PDF file from https://egusphere.copernicus.org/preprints/2026/egusphere-2026-2054/egusphere-2026-2054.pdf</self-uri>
<abstract>
<p>Before reaching the Jovian system in 2031, the ESA Jupiter Icy Moons Explorer (Juice) spacecraft will perform three Earth flybys. As well as providing gravitational assistance, these flybys are prime opportunities to assess performance and undertake in-flight calibration of the science payload in a well-understood environment. The first such interval occurred in August 2024, dubbed the Lunar-Earth gravity assist (LEGA) as it included a pass by the Moon in advance of the approach to Earth. The unique spacecraft trajectory allowed for sampling of various regions of the magnetosphere before exiting into the solar wind. In this paper, we report on the performance of the Juice magnetometer instrument (J-MAG) during the LEGA. J-MAG comprises three sensors&amp;mdash;two fluxgate vector sensors and one Coupled Dark State Magnetometer (CDSM) scalar sensor&amp;mdash;all of which were operational during the LEGA period. This represents the first time in the mission that the scalar sensor has operated in its nominal state. Here, we analyse J-MAG observations during key periods of the flyby. As well as inter-sensor comparison, we assess J-MAG data against geomagnetic field models during the approach to Earth, and compare with measurements from other spacecraft at the Moon and in the solar wind, which allow us to make suggestions for future calibration activities. Overall, the three sensors showed excellent performance at this early stage in the mission and confirmed that the scalar sensor meets the requirements for in-flight calibration of the fluxgate sensors at Ganymede. The LEGA also demonstrates the potential value of using cruise phase measurements for scientific exploration and solar wind monitoring.</p>
</abstract>
<counts><page-count count="19"/></counts>
<funding-group>
<award-group id="gs1">
<funding-source>UK Space Agency</funding-source>
<award-id>ST/X002357/1</award-id>
</award-group>
<award-group id="gs2">
<funding-source>Deutsches Zentrum für Luft- und Raumfahrt</funding-source>
<award-id>50 QJ 2402</award-id>
</award-group>
<award-group id="gs3">
<funding-source>Österreichische Forschungsförderungsgesellschaft</funding-source>
<award-id>FO999911907</award-id>
</award-group>
</funding-group>
</article-meta>
</front>
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<back>
</back>
</article>