On current sheets in two‐dimensional ideal magnetohydrodynamics caused by pressure perturbations

In this paper it is shown that in ideal magnetohydrodynamics (IMHD) a two‐dimensional equilibrium with an X‐shaped neutral point (X‐point) configuration reacts to small and smooth perturbations of the plasma pressure by the development of sheets with singular current density while the X‐point structure is replaced by a different kind of configuration containing either cusp‐like or T‐shaped singularities. This behavior is demonstrated by computing the time dependent response to a suitable initial perturbation using a relaxation method within ideal MHD. The two‐dimensional configurations considered in this paper are motivated by models of space plasma systems like, e.g. the Earth’s magnetotail containing a distant X‐point where perturbations caused by the solar wind may force the formation of current sheets and the subsequent occurrence of magnetic reconnection.

[1]  J. Birn,et al.  On the cause of thin current sheets in the near-Earth magnetotail and their possible significance for magnetospheric substorms , 1993 .

[2]  E. Priest,et al.  Magnetostatic equilibria and current sheets in a sheared magnetic field with an X-point , 1993 .

[3]  J. Birn,et al.  Three-dimensional magnetotail equilibria by numerical relaxation techniques , 1993 .

[4]  T. Hill,et al.  Limits on plasma anisotropy in a tail-like magnetic field , 1992 .

[5]  E. Priest,et al.  Magnetohydrodynamic equilibria and cusp formation at an X-type neutral line by footpoint shearing , 1992 .

[6]  J. Finn,et al.  Magnetohydrodynamic equilibria in the vicinity of an X‐type neutral line specified by footpoint shear , 1991 .

[7]  J. Drake,et al.  Structure of the dissipation region during magnetic reconnection in collisionless plasma , 1991 .

[8]  J. Birn,et al.  Quantitative study of the nonlinear formation and acceleration of plasmoids in the Earth's magnetotail , 1990 .

[9]  H. Wiechen,et al.  Quasi‐static theory of the Earth's magnetotail, including the far tail , 1988 .

[10]  B. Low,et al.  Spontaneous formation of electric current sheets and the origin of solar flares , 1988 .

[11]  B. Low Electric Current Sheet Formation in a Magnetic Field Induced by Continuous Magnetic Footpoint Displacements , 1987 .

[12]  Dieter Biskamp,et al.  Magnetic Reconnection via Current Sheets , 1986 .

[13]  A. A. van Ballegooijen,et al.  Electric currents in the solar corona and the existence of magnetostatic equilibrium , 1985 .

[14]  W. Zwingmann,et al.  On sheared magnetic field structures containing neutral points , 1985 .

[15]  J. Birn,et al.  On the cause of approximate pressure isotropy in the quiet near-earth plasma sheet , 1985 .

[16]  J. Brackbill,et al.  Nonlinear evolution of the lower‐hybrid drift instability , 1984 .

[17]  W. Zwingmann Self‐consistent magnetotail theory: Equilibrium structures including arbitrary variation along the tail axis , 1983 .

[18]  J. Birn,et al.  Self‐consistent theory of three‐dimensional convection in the geomagnetic tail , 1983 .

[19]  Russell M. Kulsrud,et al.  Forced magnetic reconnection , 1985 .

[20]  N. T. Gladd,et al.  On the role of the lower hybrid drift instability in substorm dynamics , 1981 .

[21]  A. Samain,et al.  Evolution of magnetic islands in tokamaks , 1980 .

[22]  J. Birn Computer studies of the dynamic evolution of the geomagnetic tail , 1980 .

[23]  S. Akasofu Dynamics of the Magnetosphere , 1979 .

[24]  H. Wobig,et al.  Stability of Two-Dimensional Collision-Free Plasmas , 1973 .

[25]  E. Parker Topological dissipation and the small-scale fields in turbulent gases. , 1972 .

[26]  J. T. Stuart On finite amplitude oscillations in laminar mixing layers , 1967, Journal of Fluid Mechanics.

[27]  Willard H. Bennett,et al.  Magnetically self-focussing streams , 1934 .