Abstract
A general method for studying the resistive MHD stability of plasma
configurations where boundary effects are of crucial importance and can
be expressed as additional constraints on a periodic system is presented
and applied to the case of line-tied cylindrically symmetric coronal
loops. The eigenvalue equations obtained are a generalization of the
Freidberg and Hewett equations, to which they reduce when the loop
length is made infinite. An application to tearing modes is described
which shows that in a finite geometry, tearing takes place at the center
of the configuration, corresponding to the vertex of coronal loops.
Applications to other configurations of astrophysical interest are
described.
| Original language | English |
|---|---|
| Pages (from-to) | 419-427 |
| Journal | Astrophysical Journal |
| Volume | 350 |
| DOIs | |
| Publication status | Published - 1 Feb 1990 |
Keywords
- Coronal Loops
- Magnetohydrodynamic Stability
- Solar Corona
- Solar Magnetic Field
- Tearing Modes (Plasmas)
- Boundary Value Problems
- Cylindrical Plasmas
- Fourier Series
- Photosphere
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