A method of reduction of the solar radio flux density observed with a large paraboloid

Details A method of reduction of the solar radio flux density observed with a large paraboloid A method of reduction of the solar radio flux density observed with a large paraboloid

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996cha%26a..20q.380z&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 20, Issue 3, p. 380-380.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We use the observed solar antenna temperature to make a correction for the K-factor of antenna power pattern. For quiet sun, the conversion between the antenna temperature Ta and the flux S is found to be is S = 0.15Ta. The sum of SVC fluxes of radio sources on the solar disk on 1990 July 2 is 20 sfu, about 2.4% of the total emission at 22 GHz.

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