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
β¦ LIBER β¦
Energy balance in the prominence-corona transition region
β Scribed by C. Chiuderi; F. Chiuderi Drago
- Publisher
- Springer
- Year
- 1991
- Tongue
- English
- Weight
- 656 KB
- Volume
- 132
- Category
- Article
- ISSN
- 0038-0938
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The energy balance equation for a general solar atmosphere without assuming the planeparallel approximation is solved analytically. This leads to models for both the transition region and inner corona as well as for the outer corona. The form of the latter is very similar to that of the hydrostatic