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Effect of haze absorption and scattering on radiative-convective-conductive heat flux divergence in Martian CO2 atmosphere and groundThe paper presents some guidelines of an improved numerical modeling effort developed to investigate the effect of an absorbing and scattering particulate phase on the temperature field of the Mars atmosphere and soil in its diurnal cycle and in response to a time-dependent convective heat transfer. Some guidelines are also formulated for the re-evaluation of Mariner 9 infrared radiometer or spectrometer inverted temperature measurements of the dust-laden atmosphere.
Document ID
19770044367
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Pallmann, A. J.
(St. Louis University St. Louis, Mo., United States)
Date Acquired
August 8, 2013
Publication Date
April 1, 1977
Publication Information
Publication: Rivista Italiana di Geofisica e Scienze Affini
Volume: 4
Subject Category
Lunar And Planetary Exploration
Accession Number
77A27219
Funding Number(s)
CONTRACT_GRANT: NGR-26-006-042
Distribution Limits
Public
Copyright
Other

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