The relation between brightness fluctuations and polarization of solar metre-wave emission

Details The relation between brightness fluctuations and polarization of solar metre-wave emission The relation between brightness fluctuations and polarization of solar metre-wave emission

May 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984soph...92..363d&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 92, May 1984, p. 363-373.

Physics

Brightness Temperature, Polarized Electromagnetic Radiation, Solar Radio Bursts, Polarization Characteristics, Solar Spectra

Scientific paper

Solar 80-MHz emission recorded by the Culgoora radioheliograph over a number of years (no matter what its spectral type) has followed a persistent pattern. Emission with average polarization less than 40 percent, even if bursty, shows constant polarization: the polarization remains weak during both lulls and bursts of brightness. By contrast, if emission with average polarization more than 40 percent is bursty, it shows fluctuating polarization: the polarization decreases during the bursts. The effect is discussed in terms of 'streaming' versus 'gyrating' electrons.

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