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Dynamics of Triton's atmosphereIt is argued here that the facts about Triton's atmosphere discovered by the recent Voyager encounter can be explained if Triton, like Mars, has a global, well-structured atmosphere in equilibrium with surface frosts. The subliming frost cap produces a polar anticyclone at low altitudes, with northeastward winds of about 5 m/s within the Ekman boundary layer. The temperature contrast between the cold frost-covered pole and the warm unforested equator produces westward winds at high altitudes.
Document ID
19900042066
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Ingersoll, Andrew P.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
March 22, 1990
Publication Information
Publication: Nature
Volume: 344
ISSN: 0028-0836
Subject Category
Lunar And Planetary Exploration
Accession Number
90A29121
Distribution Limits
Public
Copyright
Other

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