Abstract
An analytical solution to the magnetohydrostatic equations is presented
that generalizes a solution due to Birn et al. (1978) to include the
effect of gravity. There exist two solutions to the same boundary
conditions for small base pressures. If the base pressure exceeds a
critical value, then 'non-equilibrium' may occur and initiate a
two-ribbon flare.
Original language | English |
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Pages (from-to) | 301-307 |
Journal | Solar Physics |
Volume | 87 |
DOIs | |
Publication status | Published - 1 Sept 1983 |
Keywords
- Coronal Loops
- Gravitational Effects
- Magnetohydrostatics
- Solar Corona
- Solar Magnetic Field
- Beta Factor
- Boundary Conditions
- Boundary Value Problems
- Equilibrium Equations
- Photosphere
- Solar Atmosphere
- Solar Physics