A new expression for cylindrically-symmetric magnetic fields in coronal magnetic loops
β Scribed by Suresh Chandra; Lalan Prasad
- Publisher
- Springer Netherlands
- Year
- 1993
- Tongue
- English
- Weight
- 714 KB
- Volume
- 204
- Category
- Article
- ISSN
- 0004-640X
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The equilibrium and non-equilibrium properties of a coronal loop embedded in a stratified isothermal atmosphere are investigated. The shape of the loop is determined by a balance between magnetic tension, buoyancy, and external pressure gradients. The footpoints of the loop are anchored in the photo
The Very Large Array (VLA) has been used at 20 cm wavelength to study the evolution of a burst loop with 4" resolution on timescales as short as 10 s. The VLA observations show that the coronal loop began to heat up and change its structure about 15 rain betbre the eruption of two impulsive bursts.