Stability of solar coronal loops
โ Scribed by J.P. Goedbloed
- Book ID
- 107745413
- Publisher
- Elsevier Science
- Year
- 1990
- Tongue
- English
- Weight
- 983 KB
- Volume
- 59
- Category
- Article
- ISSN
- 0010-4655
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
In this paper solar coronal loops are regarded as regions of localized current flows. The main purpose is to investigate the consequences of current confinement rather than to produce a model. The physical and observational basis for this assumption are presented as well as the connection with previ
The theory of ideal magnetohydrodynamic turbulence in cylindrical geometry is used to study the steady-state structure of a coronal loop. The pressure profile is derived from MHD equations by representing the velocity and magnetic fields as the superposition of Chandrasekhar-Kendall functions. Such