Determination of the polarized emission from local sources and the structure of coronal magnetic fields

Details Determination of the polarized emission from local sources and the structure of coronal magnetic fields Determination of the polarized emission from local sources and the structure of coronal magnetic fields

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981azh....58.1070p&link_type=abstract

Astronomicheskii Zhurnal, vol. 58, Sept.-Oct. 1981, p. 1070-1077. In Russian.

Astronomy and Astrophysics

Astronomy

5

Polarized Electromagnetic Radiation, Solar Corona, Solar Magnetic Field, Solar Radio Emission, Sunspots, Circular Polarization, Faculae, Magnetic Field Configurations, Magnetic Flux, Mathematical Models, Radiation Sources

Scientific paper

The structure of solar coronal magnetic fields is studied on the basis of the sign inversion of polarized radio emission from active regions. Attention is given to the case of the asymmetric distribution of magnetic flux in sunspot groups, and a simple numerical model is presented which agrees with radio observations if faculae magnetic fields are taken into account.

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