Jupiter's polar auroral emissions

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

153 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/1e63e593b019735f92f94aa1e2415f79ff2f402f

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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. N. Lugaz

Citations in the corpus

• Simultaneous Chandra X ray, Hubble Space Telescope Ultraviolet, and Ulysses Radio Observations of Jupiter's Aurora (2005, background): “This region maps to the magnetic noon region just poleward of the main oval and is also where the UV active region [Grodent et al., 2003], showing UV flares apparently associated with X-ray flares, is observed.”
• 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 main auroral oval observed with HST-STIS (2003, background): “…[Pallier and Prangé, 2001] and, by contrast, these emissions vary rapidly, up to the extreme cases represented by the ‘‘flares’’ [Waite et al., 2001; Grodent et al., 2003], which can rise from the background level of a few kR to several megaRayleighs (MR) in brightness in tens of seconds.”