๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

Magnetic fields in two active prominences

โœ Scribed by J. McKim Malville


Publisher
Springer
Year
1968
Tongue
English
Weight
558 KB
Volume
5
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


๐Ÿ“œ SIMILAR VOLUMES


Magnetic fields in flares and active pro
โœ J. McKim Malville; E. Tandberg-Hanssen ๐Ÿ“‚ Article ๐Ÿ“… 1969 ๐Ÿ› Springer ๐ŸŒ English โš– 583 KB

The locations of flarcs and chromospheric absorption features on May 21 and 23, 1967, are compared with a series of ]-Ia magnetograms. Each of the four major flares included in the study developcd as double emission ribbons lying at positions of steep field gradient on opposite sides of the boundary

Analysis of two active prominences
โœ Marcos E. Machado ๐Ÿ“‚ Article ๐Ÿ“… 1972 ๐Ÿ› Springer ๐ŸŒ English โš– 931 KB
The orientation of magnetic fields in qu
โœ E. Tandberg-Hanssen; Ulrich Anzer ๐Ÿ“‚ Article ๐Ÿ“… 1970 ๐Ÿ› Springer ๐ŸŒ English โš– 322 KB

We have measured the longitudinal component, Bll, of the magnetic field in quiescent prominences and obtained a relationship between BII and 0, where 0 is the angle between the long axis of the prominence and the north-s0uth direction on the sun. From this relationship we deduce a distribution funct

Velocity fields in quiescent prominences
โœ Eberhart Jensen ๐Ÿ“‚ Article ๐Ÿ“… 1982 ๐Ÿ› Springer ๐ŸŒ English โš– 532 KB

Three quiescent prominences were observed in the Ca ~I K-line and a fourth one also in the H-line at Oslo Solar Observatory, Harestua, and reduced by Rustad (1974) and by Engvold et al. (1980). These data are used to study the distribution of the line-of-sight velocity component, N(uo). It is pointe