In the 2D standard flare model, magnetic reconnection takes place at a null point between anti-parallel coplanar field lines. Magnetic reconnection refers to the topological reconfiguration of magnetic field, which is responsible for solar flares. Yang 1ġ School of Astronomy and Space Science, Nanjing University, Nanjing 210093, ChinaĢ Department of Physics, Montana State University, Bozeman, MT 59717, USA
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