The number of energetic electrons deduced from a type C microwave burst.

Details The number of energetic electrons deduced from a type C microwave burst. The number of energetic electrons deduced from a type C microwave burst.

Apr 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acaps..12..148z&link_type=abstract

Acta Astrophys. Sin., Vol. 12, No. 2, p. 148 - 155

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

A type C microwave burst is analysed. It occurred at 1353 UT on 6 March 1989 in the active region 5395. The number of electrons Nr in the radio emission source is calculated using a proper value of magnetic field (100G), assuming the source to be homogeneous and to be located on the coronal part of magnetic loops. The author has also calculated the number of electrons, Nx, which is required for interpreting the hard X-ray flare emission in the standard thin-target model. He finds that Nr (5.6×1037) is similar to Nx (2.8×1037). So it is reasonable to conclude that both emissions may be produced by the same population of electrons.

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