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- W4291383721 abstract "Abstract Jupiter is known to have a complex magnetosphere containing energetic (above 10s of keV) electrons, protons, and heavy ions. However, a global distribution of these energetic particles is not fully understood before the era of the polar‐orbiting Juno mission. In this study, we focus on the energetic proton distribution at M < 50 by taking advantage of Juno's measurement covering various magnetic latitudes and M ‐shells, and find that energetic proton fluxes are higher off‐equator than that near the equator at M > ∼20, and become comparable or lower at high latitudes than those near the equator at low M ‐shells. Pitch angle distributions of energetic protons are field‐aligned, isotropic, and weak pancake‐like from high to low M ‐shells. Proton phase space density shows a weak M ‐shell dependence at M > 30 and a large positive slope at M < 30, suggesting their potential source and loss processes." @default.
- W4291383721 created "2022-08-15" @default.
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- W4291383721 date "2022-08-26" @default.
- W4291383721 modified "2023-10-17" @default.
- W4291383721 title "Energetic Proton Distributions in the Inner and Middle Magnetosphere of Jupiter Using Juno Observations" @default.
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- W4291383721 doi "https://doi.org/10.1029/2022gl099832" @default.
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