By expressing the magnetic field and fluid velocity in terms of two Chandrasekhar-Kendall functions (n = 0, m = 0; n = 1, m = 0) we investigated the steady-state pressure profile inside a solar coronal loop. For constant density loops, we found a two-dimensional (radial and axial) structure of press
A two-dimensional MHD global coronal model: Steady-state streamers
β Scribed by A. -H. Wang; S. T. Wu; S. T. Suess; G. Poletto
- Publisher
- Springer
- Year
- 1993
- Tongue
- English
- Weight
- 928 KB
- Volume
- 147
- Category
- Article
- ISSN
- 0038-0938
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