Abstract
A necessary condition is derived for the ideal magnetohydrodynamic
stability of a class of three-dimensional laminated isothermal
equilibria presented by Chou, Low, & Bhattacharjee (1993). The
condition is derived by the use of a particular destabilizing trial
function known as a 'ballooning mode.' This choice of trial function
allows the necessary condition to be found by the solution of four
coupled first-order ordinary differential equations that may be
integrated along individual field lines. Here the boundary conditions
model the line-tying effect of the dense photosphere. The necessary
condition for stability together with the sufficient condition derived
by Chou gives a bound on marginal stability, the tightness of the bound
depending on the parameter regime. For the case of penumbral loops,
considered by Chou, an approximate lower and upper bound on the critical
value of the plasma beta for this model can be found. The upper bound on
Beta, however, is smaller than that determined from observations.
Original language | English |
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Pages (from-to) | 496-499 |
Journal | Astrophysical Journal |
Volume | 423 |
DOIs | |
Publication status | Published - 1 Mar 1994 |
Keywords
- Magnetohydrodynamic Stability
- Photosphere
- Solar Flares
- Solar Prominences
- Three Dimensional Models
- Ballooning Modes
- Boundary Conditions
- Isothermal Layers