The problem of using the moon as source with a reference intensity in the 0.1-30 CM wavelength range

Details The problem of using the moon as source with a reference intensity in the 0.1-30 CM wavelength range The problem of using the moon as source with a reference intensity in the 0.1-30 CM wavelength range

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987azh....64..417k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 64, Mar.-Apr. 1987, p. 417-423. In Russian.

Astronomy and Astrophysics

Astronomy

4

Brightness Temperature, Centimeter Waves, Lunar Radiation, Radio Sources (Astronomy), Heat Flux, Instrument Errors, Lunar Soil, Radio Antennas

Scientific paper

A spectrum has been calculated for the lunar brightness temperature in the wavelength range 0.1 to 30 cm. Calculations have been made taking into account the lunar interior heat and the temperature dependence of the lunar soil characteristics which are determined directly from radioastronomical observations. The errors of the spectrum calculated are ±4%, thus broadening the possibilities of the use of the moon as a source of comparison in measurements of the antenna parameters and calibration of the radio source intensity.

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