Magnetic reconnection near a stagnation point.

Details Magnetic reconnection near a stagnation point. Magnetic reconnection near a stagnation point.

Jan 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.285...51h&link_type=abstract

Reconnection in Space Plasma; proceedings of an international workshop, held September 5-9, 1988, in Potsdam, GDR. ESA SP-285 (V

Astronomy and Astrophysics

Astrophysics

Magnetohydrodynamics: Dissipative Processes

Scientific paper

Starting from an exact solution of the dissipative MHD equations for a magnetic neutral layer with intrinsic stagnation point flow a normal magnetic field component is introduced as a perturbation. The resulting set of coupled ordinary differential equations is solved numerically and the behaviour of the perturbed quantities with distance from the neutral layer is presented and discussed.

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