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\begin{document}

\title{Juno Plasma Wave Observations at Ganymede}



\author[1,1]{William S Kurth}%
\author[1,1]{Ali H. Sulaiman}%
\author[1,1]{George Blair Hospodarsky}%
\author[1,1]{John Douglas Menietti}%
\author[2,2]{Barry H. Mauk}%
\author[3,3]{George Clark}%
\author[4,4]{Frederic Allegrini}%
\author[4,4]{Philip Valek}%
\author[5,5]{John E. P. Connerney}%
\author[4,4]{Jack Hunter Waite}%
\author[4,4]{Scott J Bolton}%
\author[1,1]{Masafumi Imai}%
\author[6,6]{Ondrej Santolik}%
\author[7,7]{Wen Li}%
\author[8,8]{Stefan Duling}%
\author[8,8]{Joachim Saur}%
\author[9,9]{Corentin Kenelm Louis}%
\affil[1]{University of Iowa}%
\affil[2]{Johns Hopkins University}%
\affil[3]{Johns Hopkins University Applied Physics Laboratory}%
\affil[4]{Southwest Research Institute}%
\affil[5]{NASA Goddard Space Flight Center}%
\affil[6]{Department of Space Physics, Institute of Atmospheric Physics of the Czech Academy of Sciences}%
\affil[7]{Boston University}%
\affil[8]{University of Cologne}%
\affil[9]{Dublin Institute for Advanced Studies (DIAS)}%


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  \date{May 27, 2024}


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\begin{abstract}
The Juno Waves instrument measured plasma waves associated with
Ganymede's magnetosphere during its flyby on 7 June, day 158, 2021.
Three distinct regions were identified including a wake, and nightside
and dayside regions in the magnetosphere distinguished by their electron
densities and associated variability. The magnetosphere includes
electron cyclotron harmonic emissions including a band at the upper
hybrid frequency, as well as whistler-mode chorus and hiss. These waves
likely interact with energetic electrons in Ganymede's magnetosphere by
pitch angle scattering and/or accelerating the electrons. The wake is
accentuated by low-frequency turbulence and electrostatic solitary
waves. Radio emissions observed before and after the flyby likely have
their source in Ganymede's magnetosphere.%
\end{abstract}%



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