Fig. 3
Flux rope formation at three times during interchange reconnection near the solar surface. (a)–(c) Out-of-planeelectron current Jez with overlying magnetic field lines. Along the horizontal line in (c), in (d) the magnetic field components, Bx, By, Bz and B in red, green, blue and black, respectively, in (e) the corresponding ion velocities and in (f) the electron and ion temperatures.
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