Abstract
Ideal and resistive ballooning modes are investigated for different
ratios of a two-layer stratified density region representing a model for
the photospheric/coronal boundary. Construction of the ballooning
equations using a WKB approach is justified by comparison between the
values of the growth rate obtained using Hain-Luest and ballooning
equations together with a WKB integral relation. Different values of the
density ratio, radius, and resistivity are considered. Sausage-type and
kink-type instabilities are found. One of these, depending on the value
of r, remained unstable for large density ratios. The other instability
tended to marginal stability as the density ratio was increased, and
allowed parallel and perpendicular flows across the boundary. This is
contrary to the predictions of both the 'rigid-wall' and 'flow-through'
conditions.
Original language | English |
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Pages (from-to) | 313-338 |
Journal | Solar Physics |
Volume | 133 |
DOIs | |
Publication status | Published - 1 Jun 1991 |
Keywords
- Ballooning Modes
- Boundary Conditions
- Magnetohydrodynamic Stability
- Solar Corona
- Solar Magnetic Field
- Magnetic Energy Storage
- Photosphere
- Solar Flares