Radiation parameters of an especially great radio microwave burst

Details Radiation parameters of an especially great radio microwave burst Radiation parameters of an especially great radio microwave burst

Mar 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.225...93z&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 225, no. 1, p. 93-99

Astronomy and Astrophysics

Astrophysics

1

Absorptivity, Emissivity, Energy Distribution, High Energy Electrons, Microwave Frequencies, Solar Radio Bursts, Synchrotron Radiation, Brightness Temperature, Coronal Loops, Electron Density (Concentration), Flux Density, Solar Magnetic Field

Scientific paper

By using the data of an especially great solar radio microwave burst occurring at 1700 UT on 30 October, 1992 in a 'very active' active region NOAA/USAF Region 7321, on the basis of the theoretical emission mechanism of nonthermal gyro-synchrotron radiation, we have derived the radiation parameters such as the energy distribution of energetic electrons in the source region of the burst, the emission coefficient, absorption coefficient and source function of the gyro-synchrotron radiation and made a simple analysis.

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