The inversion of the sign of the circular polarization of active region microwave emission at a 5.2 CM wavelength

Astronomy and Astrophysics – Astronomy

Scientific paper

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Circular Polarization, Emission Spectra, Microwaves, Solar Flares, Sunspots, Correlation Coefficients, Magnetic Field Configurations, Radio Telescopes, Solar Corona, Solar Magnetic Field

Scientific paper

Using data from the Siberian Solar Radio Telescope, a study has been made of the dependence of temporal characteristics of the phenomenon of sign inversion of the circular polarization of the microwave emission at a wavelength of 5.2 cm on the active-region parameters in the optical emission: latitude, inclination angle of the sunspot group axis with respect to the equator, extent and area of sunspot groups, magnetic configuration, and flare activity. The obtained empirical dependences can serve as reference points for model calculations of the magnetic field structure in the corona above the active region and for predicting large solar flares.

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