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Pitch Angle Scattering of Upgoing Electron Beams in Jupiter's Polar Regions by Whistler Mode Waves
Journal article   Open access   Peer reviewed

Pitch Angle Scattering of Upgoing Electron Beams in Jupiter's Polar Regions by Whistler Mode Waves

S. S. Elliott, D. A. Gurnett, W. S. Kurth, G. Clark, B. H. Mauk, S. J. Bolton, J. E. P. Connerney and S. M. Levin
Geophysical research letters, Vol.45(3), pp.1246-1252
02/16/2018
DOI: 10.1002/2017GL076878
url
https://doi.org/10.1002/2017GL076878View
Published (Version of record) Open Access

Abstract

The Juno spacecraft's Jupiter Energetic-particle Detector Instrument has observed field-aligned, unidirectional (upgoing) electron beams throughout most of Jupiter's entire polar cap region. The Waves instrument detected intense broadband whistler mode emissions occurring in the same region. In this paper, we investigate the pitch angle scattering of the upgoing electron beams due to interactions with the whistler mode waves. Profiles of intensity versus pitch angle for electron beams ranging from 2.53 to 7.22 Jovian radii show inconsistencies with the expected adiabatic invariant motion of the electrons. It is believed that the observed whistler mode waves perturb the electron motion and scatter them away from the magnetic field line. The diffusion equation has been solved by using diffusion coefficients which depend on the magnetic intensity of the whistler mode waves.
Geology Geosciences, Multidisciplinary Physical Sciences Science & Technology

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