Mini-U bursts and fine structures in microwave bursts.

Details Mini-U bursts and fine structures in microwave bursts. Mini-U bursts and fine structures in microwave bursts.

Jun 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999ppmto..18..157f&link_type=abstract

Publ. Purple Mt. Obs., Vol. 18, No. 2, p. 157 - 160

Computer Science

Solar Microwave Bursts: Fine Structure

Scientific paper

The mini-U bursts have been found with the 2.6 - 3.8 GHz microwave radiospectrograph with time resolution of as short as 8 msec in the microwave bursts on Apr 15, 1998 and Nov 3, 1997. The study demonstrates: 1. According to high frequency drift rate and high polarization degree, it seems likely that the nature of mini-U bursts prefers spike emissions rather than type III bursts. 2. These phenomena are mini-scale loops, compatible with the duration of spike emissions.

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