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Radiation parameters of an especially great radio microwave burst

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Abstract

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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Authors and Affiliations

  1. Beijing Observatory, Academia Sinica, Beijing, China

    Ren-Yang Zhao

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  1. Ren-Yang Zhao
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Zhao, RY. Radiation parameters of an especially great radio microwave burst. Astrophys Space Sci 225, 93–99 (1995). https://doi.org/10.1007/BF00657846

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  • DOI: https://doi.org/10.1007/BF00657846

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