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Secular changes and dark-area regeneration on Mars.Martian secular changes and dark area regeneration attributed to movement of sand, dust and wind caused by elevation and slope differences
Document ID
19670052260
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pollack, J. B.
Sagan, C.
Date Acquired
August 3, 2013
Publication Date
May 1, 1967
Publication Information
Publication: ICARUS
Subject Category
Space Sciences
Accession Number
67A30989
Funding Number(s)
CONTRACT_GRANT: NGR-09-015-023
Distribution Limits
Public
Copyright
Other
Keywords
MARS SURFACE
SECULAR PERTURBATION
SEASONAL VARIATION
SLOPE

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