Constraints on Jupiter's hydrogen corona from Galileo UVS observations

Planetary and Space Science

Volumn 52, Issue 5-6, 2004, Pages 415-421

  Gladstone, G R ^a   Pryor, W R ^b   Tobiska, W K ^c   Stewart, A I F ^d   Simmons, K E ^d   Ajello, J M ^e  

^a SOUTHWEST RESEARCH INSTITUTE   (United States)

^b Central Arizona University   (United States)

^c Space Environment Technologies ^*  (United States)

^d UNIVERSITY OF COLORADO   (United States)

^e CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

Author keywords

Airglow; Jupiter; Lyman alpha

Indexed keywords

ASTROPHYSICS; EXTRATERRESTRIAL ATMOSPHERES; HYDROGEN; ORBITS; RADIATION EFFECTS; SOLAR ENERGY; SPACE RESEARCH; ULTRAVIOLET SPECTROMETERS;

AIRGLOW; JUPITER; LYMAN ALPHA;

PLANETS;

EID: 1442311846     PISSN: 00320633     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pss.2003.06.012     Document Type: Conference Paper

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