A study of Ratan-600 observations of solar S-component sources

Details A study of Ratan-600 observations of solar S-component sources A study of Ratan-600 observations of solar S-component sources

May 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..105..111k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 105, May 1986, p. 111-121.

Physics

24

Radio Telescopes, Solar Activity, Solar Magnetic Field, Bremsstrahlung, Circular Polarization, Gyromagnetism, Solar Flares

Scientific paper

A sample of 36 S-component sources observed by the radio telescope RATAN-600 was compared with calculations of gyromagnetic emission and bremsstrahung based on recent sunspot models. The diagnostic possibilities of the spectral distributions in the radio flux, the degree of polarization, and the source sizes for the estimation of magnetic scale heights and other source parameters were checked by different methods. Depending on the magnetic field structure, the observations show different types of polarization spectra. Most regular spectra and highest values of the degree of polarization were observed from sources above the leading part of the associated spot group. Magnetic scale heights were found to be intrinsically associated with the source size of the gyromagnetic emission. The flare producton rate of active regions appears to be related to their S-component flux and magnetic scale heights.

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