Jupiter's main auroral oval observed with HST-STIS

By D. Grodent, J. Clarke, Jihyun Kim, J. Waite, S. Cowley. 2003

184 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/62c733be90b3a8539d6daf89e42fac73370ad64c

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In Astronomy and Astrophysics

1. Philippe Zarka
2. S. Cowley
3. E. Bunce
4. D. Grodent
5. J. Clarke
6. J. Waite
7. J. Duval
8. Jihyun Kim

Citations in the corpus

• Response of Jupiter's and Saturn's auroral activity to the solar wind (2009, background): “The overall brightness of the main oval has also been observed to vary from hour to hour, while generally stable in brightness on time scales of tens of minutes [Grodent et al., 2003a].”
• Jupiter's polar auroral emissions (2003, background): “The main oval emissions are observed to corotate with Jupiter [Ballester et al., 1996] and are relatively stable, exhibiting variations on time scales of tens of minutes to hours [Grodent et al., 2003].”