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Topography of Apollinaris Patera and Ma'adim VallisDigital elevation models of the northern part of Ma'adim Vallis (603a41 607m/pix, 639a91 721m/pix), and Apollinaris Patera (603a42 612m/pix, 639a92 717m/pix), covering the area between 180 degrees to 190 degrees long and -2 degrees to -20 degrees lat. were obtained using a method described here. The results for the Ma'adim Vallis area show broad agreement with the United States Geological Survey (USGS) topographic map of the area with a channel depth of 1 to 2 km. A detailed study of the variations in the channel depth along its course and calculations of its discharge rate from channel cross section and slope are currently being undertaken. Results for Apollinaris Patera have been obtained, although the absolute heights relative to the Mars datum are not well constrained. However, the relative heights are sufficient for some analysis. Again, the topographic map is in reasonable agreement with the USGS map of the area, although there are significant differences.
Document ID
19920019826
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Thornhill, G. D.
(Open Univ. Milton Keynes, United Kingdom)
Rothery, D. A.
(Open Univ. Milton Keynes, United Kingdom)
Murray, J. B.
(Open Univ. Milton Keynes, United Kingdom)
Day, T.
(University Coll. London, United Kingdom)
Cook, A.
(University Coll. London, United Kingdom)
Muller, J.-P.
(University Coll. London, United Kingdom)
Iliffe, J. C.
(University Coll. London, United Kingdom)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time
Subject Category
Lunar And Planetary Exploration
Accession Number
92N29069
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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