Survey of whistler mode chorus intensity at Jupiter

Whistler mode chorus emission is important in the acceleration of electrons and filling of the radiation belts at Jupiter. In this work chorus magnetic intensity levels (frequency‐integrated spectral density, PB) at Jupiter are comprehensively binned and parameterized. The frequency range of chorus...

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Bibliographic Details
Published in:Journal of geophysical research. Space physics 2016-10, Vol.121 (10), p.9758-9770
Main Authors: Menietti, J. D., Groene, J. B., Averkamp, T. F., Horne, R. B., Woodfield, E. E., Shprits, Y. Y., Soria‐Santacruz Pich, M., Gurnett, D. A.
Format: Article
Language:English
Subjects:
Acceleration
Astrophysics
Chorus waves
Earth
Emissions
Geophysics
Jupiter
Jupiter (planet)
Latitude
Magnetic fields
planetary magnetospheres
Radiation
Radiation belts
Sampling
whistler mode emission
Whistlers
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Summary:Whistler mode chorus emission is important in the acceleration of electrons and filling of the radiation belts at Jupiter. In this work chorus magnetic intensity levels (frequency‐integrated spectral density, PB) at Jupiter are comprehensively binned and parameterized. The frequency range of chorus under study extends from the lower hybrid frequency, flh, to fceq/2 and fceq/2 
ISSN:2169-9380
2169-9402
DOI:10.1002/2016JA022969