Investigation of the structure of coronal irregularities according to the Faraday rotation of a radio signal

Details Investigation of the structure of coronal irregularities according to the Faraday rotation of a radio signal Investigation of the structure of coronal irregularities according to the Faraday rotation of a radio signal

Feb 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ge%26ae..30..163b&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 30, Jan.-Feb. 1990, p. 163-165. In Russian.

Physics

1

Electron Density Profiles, Faraday Effect, Radio Signals, Solar Corona, Solar Electrons, Helios 2, Nonuniform Plasmas, Satellite Observation

Scientific paper

Data on the Faraday rotation of a radio signal that has passed through the solar corona are analyzed. Helios-2 data are examined in the framework of a solar-corona model with a bubble-type transient, taking into account the sector structure of the solar magnetic field. Calculation results agree well with experimental data, which indicates that the transient model used here is valid.

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