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The internal motion of quiescent prominences

✍ Scribed by Oddbjörn Engvold

Publisher
Springer
Year
1972
Tongue
English
Weight
1021 KB
Volume
23
Category
Article
ISSN
0038-0938

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📜 SIMILAR VOLUMES

The rotational motion in quiescent promi
The rotational motion in quiescent prominences
✍ M. C. Pande; K. R. Bondal 📂 Article 📅 1991 🏛 Springer Netherlands 🌐 English ⚖ 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

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The Ca § 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

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✍ S. B. Pikel'ner 📂 Article 📅 1971 🏛 Springer 🌐 English ⚖ 370 KB

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

The nature of quiescent solar prominence
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✍ Max Kuperus; Einar Tandberg-Hanssen 📂 Article 📅 1967 🏛 Springer 🌐 English ⚖ 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