Abstract
The resistive tearing-mode instability of a current carrying plasma
sheet is investigated, including the stabilizing photospheric line-tying
boundary conditions. This end condition prohibits a single Fourier mode,
and so requires a series expansion in harmonics of the fundamental sheet
excitation. Equilibria in which there exist field lines that do not
connect to the photosphere are unstable provided that the ratio of the
sheet length to characteristic transverse scale is smaller than a
critical value that depends on the equilibrium profile. Line-tying has
strong stabilizing effect on the fundamental periodic mode. The tearing
mode harmonic which develops close to the instability threshold leads to
a configuration with one X point and one O point.
Original language | English |
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Pages (from-to) | 107-124 |
Journal | Solar Physics |
Volume | 119 |
DOIs | |
Publication status | Published - 1 Mar 1989 |
Keywords
- Magnetohydrodynamic Stability
- Solar Magnetic Field
- Tearing Modes (Plasmas)
- Current Sheets
- Force-Free Magnetic Fields
- Harmonics
- Reynolds Number
- Series Expansion