Observations of the polarization of the radio emission of a prominence with the RT-22 radio telescope of the Crimean Astrophysical Observatory

Details Observations of the polarization of the radio emission of a prominence with the RT-22 radio telescope of the Crimean Astrophysical Observatory Observations of the polarization of the radio emission of a prominence with the RT-22 radio telescope of the Crimean Astrophysical Observatory

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990azh....67.1053a&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 67, Sept.-Oct. 1990, p. 1053-1056. In Russian.

Astronomy and Astrophysics

Astronomy

4

Solar Magnetic Field, Solar Prominences, Solar Radio Emission, Magnetic Measurement, Polarized Electromagnetic Radiation, Radio Telescopes

Scientific paper

The first measurements of weak magnetic fields in solar prominences by
radio techniques were carried out with the RT-22 telescope. A field
value of about 10 G was measured.

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