NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Plasma Densities in the Vicinity of Callisto from Galileo Plasma Wave ObservationsThe Galileo spacecraft has made seven close flybys of Jupiter's moon Callisto. During the closest of these (C22), which approached to within 535 km of the surface, the plasma wave instrument detected a very clear upper hybrid emission as the spacecraft passed near the moon. The peak electron density indicated by the upper hybrid resonance emission was 400/cc, almost one-thousand times the, electron density in the magnetosphere of Jupiter at the orbit of Callisto. These observations indicate that Callisto is probably surrounded by a dense ionospheric-like plasma.
Document ID
20000112957
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Gurnett, D. A.
(Iowa Univ. Iowa City, IA United States)
Persoon, A. M.
(Iowa Univ. Iowa City, IA United States)
Kurth, W. S.
(Iowa Univ. Iowa City, IA United States)
Roux, A.
(Centre des Etudes Terrestraire et Planetaire Velizy, France)
Bolton, S. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Date Acquired
August 19, 2013
Publication Date
July 1, 2000
Publication Information
Publication: Geophysical Research Letters
Publisher: American Geophysical Union
Volume: 27
Issue: 13
ISSN: 0094-8276
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
Paper 2000GL003751
Funding Number(s)
CONTRACT_GRANT: JPL-958779
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available