Abstract
The ideal magnetohydrodynamic (MHD) stability of the 2D twisted magnetic
flux tube prominence model of Cartledge and Hood (1993) is investigated.
The model includes a temperature profile that varies from realistic
prominence values up to typical coronal values. The prominence is
considered to be of finite-width and finite height. The stability
properties of the prominence models are studied by using a method that
generates a separate necessary condition and a sufficient condition.
These conditions give bounds on the parameters that define marginal
stability. In many cases these bounds are quite close so that further,
more detailed, stability calculations are not necessary. A number of
parameter regimes are examined, corresponding to different profiles of
the prominence temperatures, densities, and magnetic field shear. It is
found that the model admits realistic stable and unstable loop lengths
for observed prominence parameters when the axial magnetic field
component does not vanish.
Original language | English |
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Pages (from-to) | 51-68 |
Journal | Solar Physics |
Volume | 154 |
DOIs | |
Publication status | Published - 1 Sept 1994 |
Keywords
- Coronal Loops
- Current Density
- Current Sheets
- Force-Free Magnetic Fields
- Magnetic Field Configurations
- Magnetic Flux
- Magnetohydrodynamic Stability
- Mathematical Models
- Plasma Density
- Plasma Temperature
- Solar Corona
- Solar Magnetic Field
- Solar Prominences
- Boundary Conditions
- Coefficients
- Euler-Lagrange Equation
- Partial Differential Equations
- Potential Fields