Current Sheet Formation in Force-Free Magnetic Fields

  • Gregory Vekstein
  • Eric R. Priest


Abstract. The evolution of coronal magnetic fields in response to slow photospheric footpoint motions does not in general produce smooth a force-free eguilibrium. The presence of separatrix lines results in current sheet formation even under an infinitesimal shearing deformation of a 2-D magnetic field. When a separatrix without neutral points is present a regular perturbation approach is valid and preserves the magnetic field geometry. In the case of a neutral X-point perturbation the scheme fails and a geometry with cusped triple points is formed. In general these current sheets could create coronal heating, but when new flux emerges into a highly sheared field it could also trigger a solar flare.


Current Sheet Solar Phys Solar Flare Solar Corona Magnetic Configuration 
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Copyright information

© Springer-Verlag Berlin Heidelberg 1991

Authors and Affiliations

  • Gregory Vekstein
    • 1
  • Eric R. Priest
    • 2
  1. 1.Institute of Nuclear PhysicsNovosibirsk, 90USSR
  2. 2.Mathematical Sciences DepartmentThe UniversitySt.AndrewsScotland

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