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Magnetic field of solar prominences: The procedure of radio observations

✍ Scribed by G. P. Apushkinskij; N. A. Topchilo; A. N. Tsyganov; N. S. Nesterov


Publisher
John Wiley and Sons
Year
1996
Tongue
English
Weight
297 KB
Volume
317
Category
Article
ISSN
0004-6337

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✦ Synopsis


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 . lo-* 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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