Figs. la-b. An example of the weak field (a) and strong field (b) maps contained in the 'Atlas of Magnetic Fields in the Solar Corona'.
Bounds on the stability of 3D magnetic equilibria in the solar corona
โ Scribed by A. W. Longbottom; J. P. Melville; A. W. Hood
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 998 KB
- Volume
- 146
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
The conditions required for the stability of a steady-state electron beam propagating in the solar corona are determined using the quasi-linear theory. The growth rate for electron plasma waves in a magnetized plasma is evaluated, with the electron distribution function being given by an analytic so
This paper elucidates the topological relationship between the distribution of polarity neutral lines on the solar surface and the interspersion of closed field lines among open field lines in the corona. The solar surface contains polarity neutral lines, that are spatially nested in a series-and-pa