Magnetic field of solar prominences: the procedure of radio observations

Details Magnetic field of solar prominences: the procedure of radio observations Magnetic field of solar prominences: the procedure of radio observations

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996an....317..417a&link_type=abstract

Astronomische Nachrichten, vol. 317, no. 6, p. 417.

Astronomy and Astrophysics

Astrophysics

Scientific paper

The first successful radio astronomical results of measurements of the magnetic field of solar prominences are presented. The accuracy of polarization and magnetic field observations is 3* 10(-4) and 2 G, respectively. The observations were made by the 22-meter radio telescope of the Crimean Astrophysical Observatory at wavelengths of 8 and 13.5 mm. It has been found that the value of the magnetic fields coincides with the optical one (from 7 to 30 G), but the image of radio polarization differs from the intensity.

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