Millisecond radio spikes occurring on may 16

Details Millisecond radio spikes occurring on may 16 Millisecond radio spikes occurring on may 16

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008acasn..49..282l&link_type=abstract

Acta Astronomica Sinica, vol. 49, no. 3, p. 282-287

Astronomy and Astrophysics

Astronomy

The Sun: Radio Radiation, Physical Data And Process: Polarization

Scientific paper

The duration, polarization degree and quasi-oscillation of the millisecond radio analyzed. Spikes at 2.5 and 2.6 GHz are statistically. The contributions of the left and right-hand circluar ploarizations on the spike emissions at 2.5, 2.6, and 3.1 GHz are reported in detail. In these three frequancies, a lot of radio spikes are superposed not only on the rising and maximum phases, but also on the decay phase. It is noticed that, the spike emissions continue for 17 minutes at 2.5 and 2.6 GHz, they are also superposed on the small bursts following the main burst. The reversals of polarization sense of the spike emissions at 2.5 and 2.6 GHz with different time scales are introduced. The statistical analysis shows that there are different the features of the polarization reversals of the spike emissions at 2.5 and 2.6 GHz. The polarization reversals of the spike emissions at 2.5 GHz is 1.5 minute later than those at 2.6 GHz, and there are more polarization reversals at 2.5 GHz than those at 2.6 GHz.

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