Preflare activity of solar prominences
โ 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
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
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
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