Statistics and analysis of microwave type III bursts

Details Statistics and analysis of microwave type III bursts Statistics and analysis of microwave type III bursts

Jun 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004pnaoc...1...84m&link_type=abstract

Astronomical Research and Technology. Publications of National Astronomical Observatories of China (ISSN 1672-7673), Vol. 1, No.

Astronomy and Astrophysics

Astronomy

Sun, Solar Radio Radiation, Microwave Type Iii Burst, Solar Activities

Scientific paper

87 groups of type III bursts recorded with the dynamic spectrograph (from 5.7 to 7.6 GHz) during the 23rd solar cycle (from August 1999 to January 2002) at the National Astronomical Observatories are statistically analysed in this article, especially with the frequency drift, duration, bandwidth and polarization of each of these events being analysed in detail. From the observational characteristics the authors hold that the microwave type III bursts may be caused by the harmonic plasma radiation nonthermal electronic beams and the electron gyro-maser radiation.

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