Study of the structure of coronal inhomogeneities by the Faraday rotation of a radio signal.

Details Study of the structure of coronal inhomogeneities by the Faraday rotation of a radio signal. Study of the structure of coronal inhomogeneities by the Faraday rotation of a radio signal.

Aug 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..138b&link_type=abstract

Geomagn. Aeron., Vol. 30, No. 1, p. 138 - 139

Computer Science

Solar Corona: Structure

Scientific paper

According to Helios-2 data, in the context of a model of the solar corona with a "bubble"-type transient, and considering the sector structure of the magnetic field of the Sun, an analysis is made of the Faraday rotation of a radio signal Λ traversing the solar corona. The electron distribution in the model considered is presented. Calculations are made of the dependence of Λ on a sighting parameter p and compared with the experimental data. The calculations of Λ(p) are in good agreement with the experimental data. This result is indicative of a realistic choice of the transient model.

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