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The Spectrohelioscope and Direct Telescopic View of Solar Prominences

โœ Scribed by BUSS, ALBERT ALFRED

Book ID
109486814
Publisher
Nature Publishing Group
Year
1927
Tongue
English
Weight
288 KB
Volume
119
Category
Article
ISSN
0028-0836

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๐Ÿ“œ SIMILAR VOLUMES

The structure of coronal arcades and the
The structure of coronal arcades and the formation of solar prominences
โœ E. R. Priest; E. A. Smith ๐Ÿ“‚ Article ๐Ÿ“… 1979 ๐Ÿ› Springer ๐ŸŒ English โš– 869 KB

The temperature and density are obtained for coronal plasma in thermal and hydrostatic equilibrium and located in a force-free magnetic arcade. The isotherms are found to be inclined to the magnetic field lines and so care should be taken in inferring the magnetic structure from observed emission.

Magnetic field of solar prominences: The
Magnetic field of solar prominences: The procedure of radio observations
โœ G. P. Apushkinskij; N. A. Topchilo; A. N. Tsyganov; N. S. Nesterov ๐Ÿ“‚ Article ๐Ÿ“… 1996 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 297 KB ๐Ÿ‘ 2 views

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