Jupiter's Whistler‐Mode Belts and Electron Slot Region

The spatial distribution of whistler‐mode wave emissions in the Jovian magnetosphere measured during the first 45 perijove orbits of Juno is investigated. A double‐belt structure in whistler‐mode wave intensity is revealed. Between the two whistler‐mode belts, there exists a region devoid of 100 s k...

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Bibliographic Details
Published in:Journal of geophysical research. Space physics 2024-12, Vol.129 (12), p.n/a
Main Authors: Hao, Y.‐X., Shprits, Y. Y., Menietti, J. D., Liu, Z. Y., Averkamp, T., Wang, D. D., Kollmann, P., Hospodarsky, G. B., Drozdov, A., Roussos, E., Krupp, N., Horne, R. B., Woodfield, E. E., Bolton, S. J.
Format: Article
Language:English
Subjects:
Auroral hiss
Chorus waves
Electron distribution
Electrons
Emission
Emission measurements
Equatorial regions
galileon moons
Hiss
Jupiter
Jupiter atmosphere
Jupiter probes
Magnetic equator
Orbits
Planetary magnetospheres
Polar environments
Polar regions
Propagation modes
radiation belt
Radiation belts
Solar cycle
Space missions
Spatial distribution
Wave propagation
wave‐particle interaction
Whistlers
whistler‐mode waves
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Summary:The spatial distribution of whistler‐mode wave emissions in the Jovian magnetosphere measured during the first 45 perijove orbits of Juno is investigated. A double‐belt structure in whistler‐mode wave intensity is revealed. Between the two whistler‐mode belts, there exists a region devoid of 100 s keV electrons near the magnetic equator at 9
ISSN:2169-9380
2169-9402
DOI:10.1029/2024JA032850