Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....8771n&link_type=abstract
EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #8771
Astronomy and Astrophysics
Astronomy
Scientific paper
We present three special solar radio bursts or fine structures on the frequency band of 1.00-7.60Ghz. Firstly, we study the type III burst pair, which was recorded by spectrometer 1.00-2.00GHz at National Astronomical Observatory of China on Jan. 05, 1994. A plausible model might be thought that this event could be the observational evidence of two electron beams traveling bi-directions simultanuously due to the acceleration of magnetic reconnection in the corona. Secondly, a fine structure of microwave type IV bursts is microwave type M-burst on May 03 1999. Partial N-burst, which is a fine structure of solar III-V bursts recorded on August 251999 by both separated spectrometers 4.50-7.50 GHz at Purple Mountain observatory and 5.20-7.60GHz at NAO respectively, is the third phenomenon studied here. As the N-burst documented before, the last two fine structures are thought to the new observational evidences of electron beam reflected by magnetic mirror in the corona.
Fu Qi Jun
Lu K. Q.
Ning Zong-Jun
Yan Yiguang
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