𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Plasma stability of quiescent prominences

✍ Scribed by Migliuolo, Stefano


Book ID
119714245
Publisher
American Geophysical Union
Year
1982
Tongue
English
Weight
635 KB
Volume
87
Category
Article
ISSN
0148-0227

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Origin of quiescent prominences
✍ S. B. Pikel'ner πŸ“‚ Article πŸ“… 1971 πŸ› Springer 🌐 English βš– 370 KB

For stable equilibrium, prominences must be supported with magnetic lines of force leaning

Dynamics of Quiescent Prominences
✍ Vladimir Ruzdjak, Einar Tandberg-Hanssen πŸ“‚ Library πŸ“… 1990 πŸ› Springer 🌐 English βš– 2 MB

For some time to come, this book should be the main source for research in prominences. It surveys the results of the past years, including the "Hvar Reference Atmosphere", which was developed by a panel as a model for quiescent prominences. The reader will find papers on the formation of and physic

The nature of quiescent solar prominence
✍ Max Kuperus; Einar Tandberg-Hanssen πŸ“‚ Article πŸ“… 1967 πŸ› Springer 🌐 English βš– 550 KB

Quiescent prominences occur as long-lasting cool sheets of matter in the surrounding hot corona at the base of coronal streamers. Seen on the disk they appear as dark filaments dividing regions of opposite magnetic polarity. In this paper a theoretical model is presented, which describes the genera

Numerical models of quiescent normal pol
✍ R. A. S. Fiedler; A. W. Hood πŸ“‚ Article πŸ“… 1992 πŸ› Springer 🌐 English βš– 800 KB

We present 2-D numerical models of quiescent solar prominences with normal magnetic polarity. These models represent an extension to the classical Kippenhahn-Schltiter model in that the prominence is treated as having finite width and height and the external coronal field is matched smoothly to the