Dawn-dusk asymmetry in the main auroral emissions at Jupiter observed with Juno-UVS-Reference-Cited by-同舟云学术

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Dawn-dusk asymmetry in the main auroral emissions at Jupiter observed with Juno-UVS

Published:2024-05 Issue: Volume:413 Page:116005
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Groulard A.,Bonfond B.,Grodent D.,Gérard J.-C.,Greathouse T.K.,Hue V.,Gladstone G.R.,Versteeg M.H.

Funder

NASA

FRS-FNRS

Publisher

Elsevier BV

Reference39 articles.

1. The Juno mission;Bolton;Space Sci. Rev.,2017

2. Auroral evidence of Io’s control over the magnetosphere of Jupiter;Bonfond;Geophys. Res. Lett.,2012

3. The far-ultraviolet main auroral emission at Jupiter – part 1: dawn–dusk brightness asymmetries;Bonfond;Ann. Geophys.,2015

4. Six pieces of evidence against the corotation enforcement theory to explain the main aurora at Jupiter;Bonfond;J. Geophys. Res. Space Physics,2020

5. Are dawn storms Jupiter’s auroral substorms?;Bonfond;AGU Adv.,2021

Cited by 1 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Effect of magnetospheric conditions on the morphology of Jupiter’s ultraviolet main auroral emission as observed by Juno-UVS;Astronomy & Astrophysics;2024-08

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