Analysis of an extra large Type-IV microwave burst

Details Analysis of an extra large Type-IV microwave burst Analysis of an extra large Type-IV microwave burst

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997cha%26a..21..352c&link_type=abstract

Chinese Astronomy and Astrophysics, Volume 21, Issue 3, p. 352-359.

Astronomy and Astrophysics

Astrophysics

Scientific paper

An extra large Type-IV microwave burst was observed at Yunnan Observatory with our fast sampling radio telescopes on 1988-12-16, over a 70-min period between 0831-0941 UT. The burst consisted of 5 main peaks with a quasi-period of 12.5 min. Within the first main peak there were 8 secondary peaks with a quasi-period of 92 s (at 4.00 GHz), 72 s (2.84 GHz) and 60 s (1.42 GHz). A semi-quantitative explanation is given for the variation of the quasi-period with frequency in terms of MHD modulated oscillations in the magnetic flux tube.

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