A magnetic loop model for the slowly varying radio source observed during the solar eclipse of 1980 February 16

Details A magnetic loop model for the slowly varying radio source observed during the solar eclipse of 1980 February 16 A magnetic loop model for the slowly varying radio source observed during the solar eclipse of 1980 February 16

Sep 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985acasn..26...51l&link_type=abstract

(Acta Astronomica Sinica, vol. 26, 1985, p. 51-61) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 9, Sept. 1985, p. 2

Astronomy and Astrophysics

Astrophysics

1

Solar Eclipses, Solar Magnetic Field, Solar Radio Emission, Brightness Temperature, Electron Density (Concentration), Gyrofrequency, Sunspots, Temperature Gradients

Scientific paper

A magnetic loop model for the slowly varying radio sources on the sun is constructed based on the gyroradiation mechanism and the radio data at 2.0, 3.2, 8.2 and 21 cm obtained during the total eclipse of February 16, 1980. The model explains several detail features of the observed emission, especially the minimum brightness temperature and the high frequency cutoff.

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