Observations of Microwave Type-U Bursts

Details Observations of Microwave Type-U Bursts Observations of Microwave Type-U Bursts

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001soph..199..157w&link_type=abstract

Solar Physics, v. 199, Issue 1, p. 157-164 (2001).

Physics

2

Scientific paper

Two microwave type-U bursts observed with the 2.6-3.8 GHz spectrometer of Beijing Astronomical Observatory (BAO) are described and analysed in this paper. The microwave type-U bursts have very short durations (about 200 ms), narrow bandwidth, high-frequency drift rates of the ascending and descending branches, and a high degree of circular polarization (80%). The sense of polarization remains the same from the ascending to the descending branch.

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