Distribution of the solar radio brightness temperature at 8.6 mm wavelength.

Details Distribution of the solar radio brightness temperature at 8.6 mm wavelength. Distribution of the solar radio brightness temperature at 8.6 mm wavelength.

Jun 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994acasn..35..195z&link_type=abstract

Acta Astron. Sin., Vol. 35, No. 2, p. 195 - 203

Astronomy and Astrophysics

Astronomy

Solar Radio Radiation: Brightness Temperature, Solar Radio Radiation: Solar Eclipses, Solar Eclipses: 1980 February 16

Scientific paper

The radial distribution of the solar radio brightness temperature at 8.6 mm wavelength is calculated, based on the total eclipse observation on Feb. 16, 1980. The results obtained by the first, second and third contacts show that there is an evident brightening structure with a single spike in the 2' range on the inner side of the optical limb. The average brightening value is about 18% of the central brightness temperature. Radiation from the brightening region is about 4% of total radiation from the solar disk. The average brightness temperature is 9727K at 8.6 mm wavelength on Feb. 16, 1980.

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