Analysis of the polarization of pulsating structures at m-dm wavelengths

Details Analysis of the polarization of pulsating structures at m-dm wavelengths Analysis of the polarization of pulsating structures at m-dm wavelengths

Sep 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..114..375z&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 114, no. 2, 1987, p. 375-384. Research supported by the Ministero della Pubblica Istruzione

Physics

15

Polarized Electromagnetic Radiation, Solar Flares, Solar Radio Emission, Decametric Waves, Stellar Models, Type 4 Bursts, Wave Propagation

Scientific paper

The polarization of 60 pulsating radio events, identified as type IV bursts, which were recorded in the m-dm band during solar cycle 21 have been analyzed. The results confirm that the emission is totally polarized at the source and that the source is itself unique. In contrast to previous work, it is found that, under the assumption of the leading-spot hypothesis, the emission occurs in the ordinary magnetoionic mode for most of the samples. A different polarization degree of the continuum may point to the contemporaneous presence of more than one source.

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