Solar radio observation with large paraboloid antenna and reduction method of the radio flux density.

Details Solar radio observation with large paraboloid antenna and reduction method of the radio flux density. Solar radio observation with large paraboloid antenna and reduction method of the radio flux density.

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996acasn..37...60z&link_type=abstract

Acta Astron. Sin., Vol. 37, No. 1, p. 60 - 67

Astronomy and Astrophysics

Astronomy

Solar Radio Radiation: Methods Of Observation

Scientific paper

The author presented a reduction method of solar radio emission flux at 22 GHz with a resolution of 4'. According to observed solar antenna temperatues, the author makes a correction for the K-factor of the antenna power pattern, then he can obtain values of solar radio flux. In addition, according to models of different temperature distributions of the quiet sun and radio sources, he deduced the expression of the K-factor of the antenna power pattern, and calculated the fluxes of the quiet sun and SVC emission of radio sources.

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