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Surface and airborne evidence for plumes and winds on TritonAeolian features on Triton that were imaged during the Voyager Mission have been grouped. The term 'aeolian feature' is broadly defined as features produced by or blown by the wind, including surface and airborne materials. Observations of the latitudinal distributions of the features probably associated with current activity (known plumes, crescent streaks, fixed terminator clouds, and limb haze with overshoot) all occur from latitude -37 deg to latitude -62 deg. Likely indicators of previous activity (dark surface streaks) occur from latitude -5 deg to -70 deg, but are most abundant from -15 deg to -45 deg, generally north of currently active features. Those indicators which give information on wind direction and speed have been measured. Wind direction is a function of altitude. The predominant direction of the surface wind streaks is found to be between 40 deg and 80 deg measured clockwise from north. The average orientation of streaks in the northeast quadrant is 59 deg. Winds at 1- to 3-kilometer altitude are eastward, while those at more than 8 kilometers blow west.
Document ID
19910027594
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hansen, C. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Terrile, R. J.
(JPL Pasadena, CA, United States)
Mcewen, A.
(USGS Flagstaff, AZ, United States)
Ingersoll, A.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
October 19, 1990
Publication Information
Publication: Science
Volume: 250
ISSN: 0036-8075
Subject Category
Lunar And Planetary Exploration
Accession Number
91A12217
Distribution Limits
Public
Copyright
Other

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