The distribution of hot hydrogen atoms produced by electron and proton precipitation in the Jovian aurora

Journal of Geophysical Research: Planets

Volumn 101, Issue E9, 1996, Pages 21157-21168

  Bisikalo, D V ^a   Shematovich, V I ^a   Gerard J C ^b   Gladstone, G R ^c   Waite, J H ^c  

^a INSTITUTE OF ASTRONOMY   (Russian Federation)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c SOUTHWEST RESEARCH INSTITUTE   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0003196891     PISSN: 01480227     EISSN: None     Source Type: Journal    
DOI: 10.1029/96JE01952     Document Type: Article

References (11)

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6. Bisikalo, D.V., V.I. Shematovich, and J.C. Gérard, A kinetic model of the formation of the hot oxygen geocorona, II, Disturbed geomagnetic conditions, J. Geophys. Res., 100, 3715, 1995.
7. Broadfoot, A.L., et al., Extreme ultraviolet observations from Voyager 1 encounter with Jupiter, Science, 204, 979, 1979.
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11. 2 rotational spectra of Jupiter's aurora, Astrophys. J., 430, L73, 1994.