Combined radiation mechanism in the sun's active region no. 75 during the eclipse of 16 February, 1980

Details Combined radiation mechanism in the sun's active region no. 75 during the eclipse of 16 February, 1980 Combined radiation mechanism in the sun's active region no. 75 during the eclipse of 16 February, 1980

Feb 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.200..239j&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 200, no. 2, p. 239-250.

Astronomy and Astrophysics

Astrophysics

Solar Activity, Solar Eclipses, Solar Radiation, Brightness Temperature, Electron Energy, Field Strength, Photosphere, Radio Spectra, Solar Magnetic Field

Scientific paper

A 3D distribution of the electron temperature and density based on the radio spectrum of active region No. 75 obtained from the solar eclipse observation made on February 16 1980 is calculated. The magnetic field above the active region is calculated in terms of the solar photospheric magnetic field under the assumption of a potential field. Results show that the gyro-resonance radiation is overwhelmingly dominant in the slowly varying radiation of the active region. Bremsstrahlung radiation can reach from 5 to 20 percent of the gyro-resonance.

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