Temporal and spectral characteristics of the circular polarization of solar microwave bursts

Details Temporal and spectral characteristics of the circular polarization of solar microwave bursts Temporal and spectral characteristics of the circular polarization of solar microwave bursts

Nov 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990a%26a...239..347b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 239, no. 1-2, Nov. 1990, p. 347-355.

Astronomy and Astrophysics

Astronomy

11

Circular Polarization, Solar Radio Bursts, Synchrotron Radiation, Radiation Spectra, Radio Astronomy, Solar Radiation, Temporal Distribution

Scientific paper

Observations and interpretations are presented of polarization time profiles of solar bursts at six different frequencies over the entire microwave range. The mean degree of polarization turns out to be significantly higher in the spectral maximum than in the other regions. Above the spectral maximum, rho(c) shows a power law decrease with harmonic number, a behavior which fits the predictions of a homogeneous source model very well. A variety of temporal structures are distinguished which can be explained by the influence of different parameters of a homogeneous source.

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