Intermittent heating in a model of solar coronal loops
โ Scribed by R.W. Walsh; S. Galtier
- Book ID
- 111564238
- Publisher
- Springer
- Year
- 2000
- Tongue
- English
- Weight
- 846 KB
- Volume
- 197
- Category
- Article
- ISSN
- 0038-0938
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๐ SIMILAR VOLUMES
We investigate the limits of applicability of the Spitzer-Harm thermal conductivity in solar coronal loops and show that the ratio 2o/1. r of electron mean-free path to temperature scale height in large-scale structures can approach the limits of the Spitzer-Harm theory. We use a non-local formulati
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