The radio brightness of the undisturbed outer solar corona in the presence of a radial magnetic field
โ Scribed by Kumar Golap; Ch. V. Sastry
- Publisher
- Springer
- Year
- 1994
- Tongue
- English
- Weight
- 425 KB
- Volume
- 150
- Category
- Article
- ISSN
- 0038-0938
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Daily images of the white light corona between 3 and 10 R| have been recorded by a coronagraph aboard the OSO-7 unmanned satellite since October 3, 1971. Images for the years 1972 and 1973 have been examined for persistent coronal forms. For most of 1972 there passed over the Sun's east limb a regul
Figs. la-b. An example of the weak field (a) and strong field (b) maps contained in the 'Atlas of Magnetic Fields in the Solar Corona'.
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 Astroph