DocumentCode
978476
Title
Thermal radio radiation from the moon and planets
Author
Mayer, Cowtell H.
Author_Institution
Naval Research Laboratory, Washington, DC, USA
Volume
12
Issue
7
fYear
1964
fDate
12/1/1964 12:00:00 AM
Firstpage
902
Lastpage
913
Abstract
Thermal radio radiation has been observed from the moon, Mercury, Venus, Mars, Jupiter, and Saturn. The most important result of the observations is the discovery that the temperature at the surface of Venus, beneath the clouds, is greater than
K. The thermal radio radiation from the moon comes from beneath the surface and gives information about the temperature distribution and variation which can be interpreted in terms of the physical characteristics of the subsurface material. This also should apply to the planets with thin atmospheres. The thermal radio radiation from Jupiter should give information about the temperature distribution in the extensive absorbing atmosphere, but the intensity of the thermal radiation is confused by the nonthermal radiation of the radiation belts and cannot be accurately specified until more observational data are available.
K. The thermal radio radiation from the moon comes from beneath the surface and gives information about the temperature distribution and variation which can be interpreted in terms of the physical characteristics of the subsurface material. This also should apply to the planets with thin atmospheres. The thermal radio radiation from Jupiter should give information about the temperature distribution in the extensive absorbing atmosphere, but the intensity of the thermal radiation is confused by the nonthermal radiation of the radiation belts and cannot be accurately specified until more observational data are available.Keywords
Extraterrestrial radio sources; Radio sources, extraterrestrial; Atmosphere; Belts; Clouds; Jupiter; Mars; Moon; Planets; Saturn; Temperature distribution; Venus;
fLanguage
English
Journal_Title
Antennas and Propagation, IEEE Transactions on
Publisher
ieee
ISSN
0018-926X
Type
jour
DOI
10.1109/TAP.1964.1138325
Filename
1138325
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