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Physics of solar prominences

โœ Scribed by Anton Bruzek; Max Kuperus


Publisher
Springer
Year
1972
Tongue
English
Weight
1011 KB
Volume
24
Category
Article
ISSN
0038-0938

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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