Group of type III bursts and its quasi-periodic pulsations in solar radio bursts

Details Group of type III bursts and its quasi-periodic pulsations in solar radio bursts Group of type III bursts and its quasi-periodic pulsations in solar radio bursts

Jun 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pbeio..37...88w&link_type=abstract

Astrophysics Reports. Publications of the Beijing Astronomical Observatory, No. 37, p. 88 - 92 (2001). In: Proceedings of the Ei

Astronomy and Astrophysics

Astrophysics

Solar Flare, Type Iii Burst, Pulsation

Scientific paper

A type III burst group event in solar microwave bursts observed with 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) on April 15, 1998 are analyzed in this paper. First the observational characteristics of the event including duration, frequency bandwidth, drift rate and quasi-periodicity are described. Then the space scale, brightness temperature and magnetic field strength of the emission sources were discussed. Finally we discuss the quasi-periods of the type III burst group using the magnetic coalescence model preliminarily.

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