Circular Polarization of Solar Bursts at 22-GHZ

Details Circular Polarization of Solar Bursts at 22-GHZ Circular Polarization of Solar Bursts at 22-GHZ

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993soph..148..341s&link_type=abstract

Solar Physics, Vol.148, NO. 2/DEC, P.341, 1993

Physics

Scientific paper

The circular polarization of complex solar bursts was measured at short microwaves (22 GHz, A = 1.35 cm) with high sensitivity (0.03 s.f.u. r.m.s.) and high time resolution (5 ms). The polarization shows up as soon as an excess burst emission is measured. Two components are found in the time development of the degree of circular polarization: (1) a steady level, sometime changing smoothly with time; (2) superimposed faster polarization time structures, small compared to the basic steady degree of polarization, and often not clearly related to the burst flux time structures. The observed degrees may range from 10% to more than 85%

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