Determination of the solar radio brightness temperature distribution at 8.6 mm wavelength based on the observations of the annular solar eclipse.

Details Determination of the solar radio brightness temperature distribution at 8.6 mm wavelength based on the observations of the annular solar eclipse. Determination of the solar radio brightness temperature distribution at 8.6 mm wavelength based on the observations of the annular solar eclipse.

Jun 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ppmto..14...95s&link_type=abstract

Publ. Purple Mt. Obs., Vol. 14, No. 2, p. 95 - 103

Physics

Solar Eclipses: 1987 September 23, Solar Radio Radiation: Brightness Temperature, Solar Radio Radiation: Solar Eclipses

Scientific paper

The radial distribution of the solar radio brightness temperature at 8.6 mm wavelength is calculated, based on the annular eclipse observation of Sept 23, 1987. The results obtained show that the limb brightening is about 5.1% above the brightness of the central part of the disk. The total flux density, the percentage of residual flux density at the moment of maximum eclipse phase and the radius of the radio sun are determined.

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