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Geometry of solar prominences and magnetic fields in the corona

✍ Scribed by A. M. Zagnetko; B. P. Filippov; O. G. Den


Book ID
110141925
Publisher
Springer
Year
2005
Tongue
English
Weight
268 KB
Volume
49
Category
Article
ISSN
1063-7729

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πŸ“œ SIMILAR VOLUMES


Magnetic Fields in the Solar Corona
✍ ELLIS, G. R. A. πŸ“‚ Article πŸ“… 1967 πŸ› Nature Publishing Group 🌐 English βš– 356 KB
Atlas of magnetic fields in the solar co
✍ Gordon Newkirk; Dorothy E. Trotter; Martin D. Altschuler; Robert Howard πŸ“‚ Article πŸ“… 1972 πŸ› Springer 🌐 English βš– 105 KB

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 Prominence-Corona Transition Region
✍ Franca Chiuderi Drago; OddbjΓΈrn Engvold; Eberhart Jensen πŸ“‚ Article πŸ“… 1992 πŸ› Springer 🌐 English βš– 949 KB

An emission measure analysis is performed for the Prominence-Corona Transition Region (PCTR) under the assumption that the cool matter of quiescent filaments is contained in long, thin magnetic flux loops imbedded in hot coronal cavity gas. Consequently, there is a transition region around each thre