Abstract
Some results concerning two-dimensional (∂/∂y = 0) magnetohydrodynamic equilibria in the presence of an X-type neutral line are presented. It is shown that in the framework of ideal MHD the latter is structurally unstable: shearing of an initial potential poloidal magnetic field results in the splitting of an X-point into a current sheet with cusp-points (or Y-points for some particular cases) at its ends. At the same time, one finds the formation of current sheets all along the separatrices even for a footpoint shearing displacement that is finite as the separatrix is approached. Scale-invariant or similarity solutions for the poloidal magnetic field inside the cusp are found. They are valid in the vicinity of a cusp-point on lengths much smaller than the global scale. These solutions predict fractional power-law singularities in the current density at the separatrix as well as a universal behavior for the poloidal magnetic field strength Bp near a cusp point, namely Bp ~∼ r1-3. Discussion is presented regarding the global geometry of the poloidal magnetic field produced by different types of footpoint shearing motions.
Original language | English |
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Pages (from-to) | 333-340 |
Number of pages | 8 |
Journal | Astrophysical Journal |
Volume | 384 |
Issue number | 1 |
DOIs | |
Publication status | Published - 1992 |
Keywords
- MHD
- Sun: Corona