High-energy electrons in solar microwave sources

Details High-energy electrons in solar microwave sources High-energy electrons in solar microwave sources

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978pazh....4..323k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 4, July 1978, p. 323-325.) Soviet Astronomy Letters, vol. 4, July-Aug. 1978, p. 175, 17

Astronomy and Astrophysics

Astronomy

High Energy Electrons, Microwave Emission, Solar Electrons, Solar Radio Bursts, Brightness Temperature, Plasma-Particle Interactions, Synchrotron Radiation

Scientific paper

The role of synchrotron radiation emitted by an ensemble of high-energy electrons having a temperature of 10 million to 100 million K in the regions above sunspots with a strong magnetic field is discussed in an effort to explain the energetic processes observed in the microwave range. Changes in the electron ensemble parameters could serve to reverse the sign of circular polarization and to produce a distinctive peak in the polarization curve during the phase of rising burst intensity.

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