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Irrotational motion in quiescent prominences

✍ Scribed by M. C. Pande; K. R. Bondal

Publisher
Springer Netherlands
Year
1991
Tongue
English
Weight
256 KB
Volume
182
Category
Article
ISSN
0004-640X

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πŸ“œ SIMILAR VOLUMES

The rotational motion in quiescent promi
The rotational motion in quiescent prominences
✍ M. C. Pande; K. R. Bondal πŸ“‚ Article πŸ“… 1991 πŸ› Springer Netherlands 🌐 English βš– 227 KB

On the basis of Kippenhahn and Schltiter's magnetohydrostatic model of a quiescent prominence we have attempted to study the effect of a rotational velocity field in it. We find that a physically plausible solution is not possible in the vertical plane. A possibility, however, is shown in the horizo

Fine structure of motions in a quiescent
Fine structure of motions in a quiescent prominence
✍ M. Sh. Gigolashvili; Yu. D. Zhugzhda πŸ“‚ Article πŸ“… 1982 πŸ› Springer 🌐 English βš– 513 KB

The Ca Β§ K line of the quiescent prominence of 15 October 1969 observed at the Abastumani Astrophysical Observatory of the Academy of Sciences of Georgia, U.S.S.R. is studied in detail. The behaviour of various fragments of the prominence with the line-of-sight Doppler velocities is investigated for

Velocity fields in quiescent prominences
Velocity fields in quiescent prominences
✍ Eberhart Jensen πŸ“‚ Article πŸ“… 1982 πŸ› Springer 🌐 English βš– 532 KB

Three quiescent prominences were observed in the Ca ~I K-line and a fourth one also in the H-line at Oslo Solar Observatory, Harestua, and reduced by Rustad (1974) and by Engvold et al. (1980). These data are used to study the distribution of the line-of-sight velocity component, N(uo). It is pointe