The study of temperature variations of the lunar surface at short centimeter wavelengths with the RATAN-600

Details The study of temperature variations of the lunar surface at short centimeter wavelengths with the RATAN-600 The study of temperature variations of the lunar surface at short centimeter wavelengths with the RATAN-600

Jun 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988pazh...14..553n&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 14, June 1988, p. 553-563. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

1

Brightness Temperature, Centimeter Waves, Lunar Radiation, Lunar Surface, Temperature Profiles, Radio Emission, Surface Temperature

Scientific paper

Observations of the intrinsic emission of the moon at short centimeter wavelengths with high resolution and sensitivity show that the lunar brightness temperature distribution is extremely inhomogeneous. The dimensions of these inhomogeneities range from 0.5 arcmin to 0.4 lunar radii. The brightness temperature variations are analyzed as a function of lunar phase. It is found that differences in the temperature regime in the radio range can be attributed to differences in chemical composition as well as to geometrical factors.

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