Spaceborne measurement of the radio emission of the Galaxy at a frequency of 37 GHz

Details Spaceborne measurement of the radio emission of the Galaxy at a frequency of 37 GHz Spaceborne measurement of the radio emission of the Galaxy at a frequency of 37 GHz

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pazh...13..469s&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 13, June 1987, p. 469-473. In Russian. In Russian.

Astronomy and Astrophysics

Astronomy

Galactic Radiation, Milky Way Galaxy, Radiation Measurement, Radio Emission, Satellite-Borne Instruments, Angular Resolution, Atmospheric Attenuation, Nonthermal Radiation, Radio Frequencies, Thermal Emission

Scientific paper

A Prognoz-9 survey of the Galactic plane was carried out at a frequency of 37 GHz with an angular resolution of 5.5 deg and a temperature resolution of 0.6 mK in the framework of the Relikt experiment. Excess radiation was observed in Galactic quadrants I and IV. Portions of the thermal and nonthermal emission of extended components in the 408-MHz survey are estimated.

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