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Magnetic field of solar prominences: The procedure of radio observations
Authors:G P Apushkinskij  N A Topchilo  A N Tsyganov  N S Nesterov
Abstract: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.
Keywords:prominences  magnetic field  radio measurements
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