A group of microwave type bursts on 1998 April 15

Details A group of microwave type bursts on 1998 April 15 A group of microwave type bursts on 1998 April 15

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001acasn..42..382d&link_type=abstract

Acta Astronomica Sinica, vol.42, no.4, p. 382-389

Astronomy and Astrophysics

Astronomy

1

Sun, Microwave Type Bursts, Plasma Radiation, Sun, Microwave Type Bursts, Plasma Radiation

Scientific paper

A group of microwave type-III bursts observed by the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) on 1998 April 15 is introduced in detail in this paper. They have the characteristics of broad bandwidth (>100MHz), short durations (<100ms), very high polarization degrees (~100%), positive frequency drift rates (>1 GHz/s), and fast pulsations (with a period of about 100 ms). Their time profiles are also analyzed. According to these characteristics, we suggest that these microwave type III bursts are due to the plasma fundamental emission.

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