๐”– Bobbio Scriptorium
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Preflare activity of solar prominences

โœ Scribed by G. Simon; N. Mein; P. Mein; L. Gesztelyi


Publisher
Springer
Year
1984
Tongue
English
Weight
871 KB
Volume
93
Category
Article
ISSN
0038-0938

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๐Ÿ“œ SIMILAR VOLUMES


Kinematics of solar prominences
โœ J. L. Ballester; J. Kleczek ๐Ÿ“‚ Article ๐Ÿ“… 1983 ๐Ÿ› Springer ๐ŸŒ English โš– 434 KB
Physics of solar prominences
โœ Anton Bruzek; Max Kuperus ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 1011 KB
Prominence activity during the ascending
โœ V. N. Dermendjiev; K. Y. Stavrev; P. L. Andreeva ๐Ÿ“‚ Article ๐Ÿ“… 1992 ๐Ÿ› Springer ๐ŸŒ English โš– 414 KB

Longitude-latitude and time-latitude distributions of the number and area of prominences observed at Lomnick~ ~-tlt coronal station in the years IgStJ-lggO are studied using the method of contour rr~ps construction with different degree of smoothing. Special attention is paid to the bifurcation in t

The nature of quiescent solar prominence
โœ Max Kuperus; Einar Tandberg-Hanssen ๐Ÿ“‚ Article ๐Ÿ“… 1967 ๐Ÿ› Springer ๐ŸŒ English โš– 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