2D Stationary Reconnection Solutions in the Vicinity of a Magnetic Null Point and a Stagnation Point

Physics

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Scientific paper

The classical reconnection solutions propose an X-type inflow of the plasma into the X-point structure of the magnetic field. We analyse systematically the implications of the different magnetic field structures of a field which depends linearly on the spatial coordinates. The linear dependence is valid if the Jacobian matrix of the magnetic field does not vanish at the null point. We solve the complete set of the resistive MHD equations for the case that the stagnation point has only a small offset to the magnetic null point. We assume also that the Jacobian of the velocity field does not vanish. This leads to the question which topological and geometrical type of the flow corresponds to which type of magnetic field structure.

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