Observational evidence for solar radio microflares with unusual characteristics.

Details Observational evidence for solar radio microflares with unusual characteristics. Observational evidence for solar radio microflares with unusual characteristics.

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pyuno....s.396x&link_type=abstract

Publications of the Yunnan Observatory, Suppl. 1999, p. 396 - 399

Physics

Solar Flares: Radio Radiation

Scientific paper

A very rare type of solar radio microflares occurring during 0645 - 0720 UT on Jan. 5, 1994 is introduced. The radio and optical characteristics of the solar microflares of a short decimetric wave (1.42 GHz) are discussed. The authors try to discuss the generation mechanism qualitatively and find it is in consistence with the model of current loop explosive coalescence: the explosive coalescence of the multiple of cross magnetic flux loops causes the plasma disturbance and so rapidly transform the magnetic energy into the kinetic energy of electrons.

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