𝔖 Bobbio Scriptorium
✦   LIBER   ✦

Ballooning Instability in Coronal Flare Loops

✍ Scribed by Y. T. Tsap; Y. G. Kopylova; A. V. Stepanov; V. F. Melnikov; K. Shibasaki


Publisher
Springer
Year
2008
Tongue
English
Weight
461 KB
Volume
253
Category
Article
ISSN
0038-0938

No coin nor oath required. For personal study only.


πŸ“œ SIMILAR VOLUMES


Kink instability of solar coronal loops
✍ A. W. Hood; E. R. Priest πŸ“‚ Article πŸ“… 1979 πŸ› Springer 🌐 English βš– 789 KB

Solar coronal loops are observed to be remarkably stable structures. A magnetohydrodynamic stability analysis of a model loop by the energy method suggests that the main reason for stability is the fact that the ends of the loop are anchored in the dense photosphere. In addition to such line-tying,

X-ray observations of limb flare loops a
✍ ZdenΓ©k Ε vestka; Kermit L. Smith; Keith T. Strong πŸ“‚ Article πŸ“… 1992 πŸ› Springer 🌐 English βš– 374 KB

We present observations of another post-flare arch following an eruptive flare, detected in X-ray lines above the western solar limb on 2 May 1985.

Thermal trigger for solar flares and cor
✍ B. V. Somov; S. I. Syrovatskii πŸ“‚ Article πŸ“… 1982 πŸ› Springer 🌐 English βš– 351 KB

A longitudinal stability is considered for the quasi-steady current sheet which is uniform along the current. In the MHD approximation, the stability problem is solved for the plane neutral sheet and small disturbances propagating along the current. The current sheet is shown to break-up into the sy