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Strain Histories Among Alba and Syria Planum, MarsThe centers work of Anderson et al. (2001) [1] identified two prominent centers in the Tharsis region, Syria Planum and Alba Patera (Stage 2 and Stage 4 respectively). Because of their perceived influence on the geologic and possible paleoclimatic histories of Mars, Mars Orbiter Laser Altimetry (MOLA) along with published stratigraphic and paleotectonic information (including the centers information) were analyzed using Geographic Information Systems (GIS) to perform a comparative investigation of their strain histories through time. This investigation highlights their similarities and distinctions, including their topographic and morphologic signatures, deformational extent, and intensities and durations of activity.
Document ID
20030110899
Document Type
Conference Paper
Authors
Anderson, R. C. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Dohm, J. M. (Arizona Univ. AZ, United States)
Hare, T. (Geological Survey Flagstaff, AZ, United States)
Haldemann, A. F. C. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Baker, V. (Arizona Univ. AZ, United States)
Date Acquired
August 21, 2013
Publication Date
January 1, 2003
Publication Information
Publication: Lunar and Planetary Science XXXIV
Subject Category
Lunar and Planetary Science and Exploration
Distribution Limits
Public
Copyright
Public Use Permitted.

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