Microwave emission from hot X-ray kernels in solar flares

Details Microwave emission from hot X-ray kernels in solar flares Microwave emission from hot X-ray kernels in solar flares

Nov 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982soph...81..121z&link_type=abstract

Solar Physics, vol. 81, Nov. 1982, p. 121-135.

Physics

8

Microwave Spectra, Polarization Characteristics, Solar Flares, Solar Radio Bursts, Solar X-Rays, Bremsstrahlung, Brightness Temperature, Cyclotron Radiation, Plasma Frequencies, Solar Magnetic Field, Thermal Radiation

Scientific paper

Spectral and polarization characteristics of radio emission from hot X-ray kernels are considered. It is shown that thyfrequency spectrum of thermal cyclotron radio emission and bremsstrahlung from these regions may contain a set of lines at cyclotron harmonics and the maximum at plasma frequency. This makes possible the diagnostics of the X-ray kernel plasma and magnetic fields according to spectral and polarization observations of microwave radio emission in solar flares

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