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Ganymede‐Induced Decametric Radio Emission: In Situ Observations and Measurements by Juno
Journal article   Open access   Peer reviewed

Ganymede‐Induced Decametric Radio Emission: In Situ Observations and Measurements by Juno

C. Louis, P. Louarn, F. Allegrini, W. Kurth and J. Szalay
Geophysical research letters, Vol.47(20), e2020GL090021
10/28/2020
DOI: 10.1029/2020GL090021
url
https://hal.science/hal-03048192View
Open Access

Abstract

At Jupiter, part of the auroral radio emissions are induced by the Galilean moons Io, Europa and Ganymede. Until now, they have been remotely detected, using ground-based radio-telescopes or electric antennas aboard spacecraft. The polar trajectory of the Juno orbiter allows the spacecraft to cross the magnetic flux tubes connected to these moons, or their tail, and gives a direct measure of the characteristics of these decametric moon–induced radio emissions. In this study, we focus on the detection of a radio emission during the crossing of magnetic field lines connected to Ganymede’s tail. Using electromagnetic waves (Juno/Waves) and in-situ electron measurements (Juno/JADE-E), we estimate the flux tube width to be a few 100 km, a radio emission growth rate > 3×10−4, an electron population of energy E = 4 − 15 keV and an emission beaming angle of θ = 76◦ − 83◦ , at a frequency ∼ 1.005 − 1.021 × fce. We also confirmed that radio emission is associated with Ganymede’s down-tail far-ultraviolet emission
Astrophysics Sciences of the Universe

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