NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
A partially collisional model of the Titan hydrogen torusOccasional collision effects are encompassed by the present numerical model of atomic hydrogen densities in Titan's hydrogen torus, which is noted to be azimuthally symmetric; the torus density peaks sharply at Titan's orbit, and rapidly decreases in the both radially outward and perpendicular directions. Collisions of Saturnian atoms with the torus population produce a corona. Without this coronal population, the torus model would not reproduce the Voyager 2 Lyman-alpha intensities. These observations may nevertheless be modelled by a torus-plus-corona model that also reconciles the Pioneer 11 torus observations with those of the two Voyager spacecraft.
Document ID
19880040762
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hilton, Douglas A.
(Arizona Univ. Tucson, AZ, United States)
Hunten, Donald M.
(Arizona, University Tucson, United States)
Date Acquired
August 13, 2013
Publication Date
February 1, 1988
Publication Information
Publication: Icarus
Volume: 73
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
88A27989
Funding Number(s)
CONTRACT_GRANT: NSG-7558
Distribution Limits
Public
Copyright
Other

Available Downloads

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