Extraction of Solar Coronal Magnetic Loops with
โ Scribed by S. Biskri; J.-P. Antoine; B. Inhester; F. Mekideche
- Publisher
- Springer
- Year
- 2010
- Tongue
- English
- Weight
- 681 KB
- Volume
- 262
- Category
- Article
- ISSN
- 0038-0938
No coin nor oath required. For personal study only.
๐ SIMILAR VOLUMES
We present here a model, based on observations, for the magnetic-field equilibrium of a cool coronal loop. The pressure structure, taken from the Harvard/Skylab EUV data, is used to modify the usual force-free-field form in quasi-cylindrical symmetry. The resulting field, which has the same directio
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