Microwave M burst on May 3 1999

Details Microwave M burst on May 3 1999 Microwave M burst on May 3 1999

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...364..793n&link_type=abstract

Astronomy and Astrophysics, v.364, p.793-798 (2000)

Astronomy and Astrophysics

Astrophysics

10

Sun: Activity, Sun: Radio Radiation

Scientific paper

We present a remarkable fine structure of ``decimetric pulsation" event (DCIM), observed with the 2.60-3.80 GHz spectrometer in Beijing Astronomical Observatory on 3 May 1999; a ``M" dynamic spectrum has been detected, thanks to the high time and frequency resolutions. We call this fine structure a microwave M burst and propose a plausible model which treats the observed M burst as an emission produced by the same electron beam travelling along magnetic lines and mirrored; this beam might be originally formed from the plasmoid of a type IV-DCIM burst. The M burst could be another radio evidence of the mirror effect on electron beam after the N-burst. It is the first time that such a feature has been detected in type IV-DCIM bursts.

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