𝔖 Bobbio Scriptorium
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Origin of quiescent prominences

✍ Scribed by S. B. Pikel'ner

Publisher
Springer
Year
1971
Tongue
English
Weight
370 KB
Volume
17
Category
Article
ISSN
0038-0938

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✦ Synopsis

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

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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