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\begin{document}

\title{Characterising the magnetic and plasma environment upstream of Ganymede}



\author[1]{Alexandre Santos}%
\author[1]{Nicholas Achilleos}%
\author[2]{Dimitrios Millas}%
\author[1]{William Richard Dunn}%
\author[1]{Patrick Guio}%
\author[3]{Christopher Stephen Arridge}%
\affil[1]{University College London}%
\affil[2]{Royal Observatory of Belgium}%
\affil[3]{Lancaster University}%


\vspace{-1em}



  
  \date{May 25, 2024}


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\begin{abstract}
We present an application of the latest UCL-AGA magnetodisc model
(MDISC) to the study of the magnetic and plasma conditions in the
near-Ganymede space. By doing this, we provide a comparison with
measurements from Juno's most recent flyby of the Jovian moon, perijove
34 (PJ34). We find good agreement between the model results and the
magnetometer data, pointing towards a hot plasma index value \$K\_h =
\textbackslash{}SI\{2.719(24)e7\}\{\textbackslash{}pascal\textbackslash{},\textbackslash{}meter\textbackslash{},\textbackslash{}tesla\^{}\{-1\}\}\$
and an effective magnetodisc radius \$r\_\{\textbackslash{}text\{max\}\}
= \textbackslash{}SI\{79.5(11)\}\{\}\$ Jupiter radii for the Jovian
magnetosphere, for the duration of the trajectory, suggesting a
configuration with middling levels of expansion. We also predict the
plasma conditions observed by Juno during the same flight-path, as well
as the typical conditions over the orbit of Ganymede, with the magnetic
and hot plasma pressures assuming dominant roles. Finally, these results
are compared with functional fits of a compilation of Galileo flyby data
obtained in the vicinity of Ganymede's orbit, suggesting Juno
experienced somewhat similar conditions, despite a systematic
overestimation in magnetic field intensity in the near-Ganymede space.%
\end{abstract}%



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