Geometry of solar prominences and magnetic fields in the corona
β 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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π SIMILAR VOLUMES
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'.
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
We determine magnetic fields and electric currents in three prominences without simplifications used in our previous papers.