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=1985cha%26a...9..232l&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 9, Issue 3, p. 232-240.

Astronomy and Astrophysics

Astrophysics

Scientific paper

We construct a magnetic loop model for the slowly varying radio sources on the Sun based on the gyro-radiation mechanism and the radio data at 2.0, 3.2, 8.2 and 21 cm obtained during the total eclipse of 1980 Feb. 16. The model explains several detail features of the observed emission, especially the minimum brightness temperature and the high frequency cutoff.

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