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Journal Article

Jupiter's Whistler‐Mode Belts and Electron Slot Region

Authors
/persons/resource/yixinhao

Hao,  Yixin
2.7 Space Physics and Space Weather, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;
Submitting Corresponding Author, Deutsches GeoForschungsZentrum;

/persons/resource/yshprits

Shprits,  Yuri
2.7 Space Physics and Space Weather, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Menietti,  J. D.
External Organizations;

Liu,  Z. Y.
External Organizations;

Averkamp,  T.
External Organizations;

/persons/resource/dedong

Wang,  D.
2.7 Space Physics and Space Weather, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Kollmann,  P.
External Organizations;

Hospodarsky,  G. B.
External Organizations;

/persons/resource/adrozdov

Drozdov,  A.
2.7 Space Physics and Space Weather, 2.0 Geophysics, Departments, GFZ Publication Database, Deutsches GeoForschungsZentrum;

Roussos,  E.
External Organizations;

Krupp,  N.
External Organizations;

Horne,  R. B.
External Organizations;

Woodfield,  E. E.
External Organizations;

Bolton,  S. J.
External Organizations;

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Fulltext (public)

5029163.pdf
(Publisher version), 3MB

Supplementary Material (public)
There is no public supplementary material available
Citation

Hao, Y., Shprits, Y., Menietti, J. D., Liu, Z. Y., Averkamp, T., Wang, D., Kollmann, P., Hospodarsky, G. B., Drozdov, A., Roussos, E., Krupp, N., Horne, R. B., Woodfield, E. E., Bolton, S. J. (2024): Jupiter's Whistler‐Mode Belts and Electron Slot Region. - Journal of Geophysical Research: Space Physics, 129, 12, e2024JA032850.
https://doi.org/10.1029/2024ja032850


Cite as: https://gfzpublic.gfz-potsdam.de/pubman/item/item_5029163
Abstract
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 . Insufficient source electron population in such an electron “slot” region is a possible explanation for the relatively lower wave activity compared to the whistler-mode belts. The wave intensity of the outer whistler-mode belt measured in the dusk-premidnight sector is significantly stronger than in the postmidnight-dawn sector. We suggest that the inherent dawn-dusk asymmetries in source electron distribution and/or auroral hiss emission rather than the modulation of solar cycle are more likely to result in the azimuthal variation of outer whistler-mode belt intensity during the first 45 Juno perijove orbits.