An analysis of five solar microwave Type-III bursts

Details An analysis of five solar microwave Type-III bursts An analysis of five solar microwave Type-III bursts

Feb 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998cha%26a..22..245x&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 22, Issue 2, p. 245-245.

Astronomy and Astrophysics

Astrophysics

Scientific paper

Five Type-III microwave bursts observed with our high temporal resolution, four-frequency (1.42, 2.13, 2.84, 4.26 GHz) system are presented. They show the following features: a broad frequency band, long and short lives, inward and outward fast frequency drifts. The indications are that both plasma emission by nonthermal electron beams and electron cyclotron maser are possible. The observed features are not entirely the same as the Type-III events in decimetre or high-frequency microwave ranges and double features or transitions are indicated.

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