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Plasma waves in Jupiter's high-latitude regions: Observations from the Juno spacecraft
Journal article   Open access   Peer reviewed

Plasma waves in Jupiter's high-latitude regions: Observations from the Juno spacecraft

S. S. Tetrick, D. A. Gurnett, W. S. Kurth, M. Imai, G. B. Hospodarsky, S. J. Bolton, J. E. P. Connerney, S. M. Levin and B. H. Mauk
Geophysical research letters, Vol.44(10), pp.4447-4454
05/28/2017
DOI: 10.1002/2017GL073073
url
https://doi.org/10.1002/2017GL073073View
Published (Version of record) Open Access

Abstract

The Juno Waves instrument detected a new broadband plasma wave emission (similar to 50 Hz to 40 kHz) on 27 August 2016 as the spacecraft passed over the low-altitude polar regions of Jupiter. We investigated the characteristics of this emission and found similarities to whistler mode auroral hiss observed at Earth, including a funnel-shaped frequency-time feature. The electron cyclotron frequency is much higher than both the emission frequency and local plasma frequency, which is assumed to be similar to 20-40 kHz. The E/cB ratio was about three near the start of the event and then decreased to one for the rest of the period. A correlation of the electric field spectral density with the flux of an upgoing 20 to 800 keV electron beam was found, with a correlation coefficient of 0.59. We conclude that the emission is propagating in the whistler mode and is driven by the energetic upgoing electron beam.
Geology Geosciences, Multidisciplinary Physical Sciences Science & Technology

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