Inertial-range reconnection in a magnetohydrodynamic simulation of a solar wind event showing the magnetic cloud isosurface in yellow, and turbulent magnetic field lines wandering in and out.

From the article:

Inertial-Range Reconnection in Magnetohydrodynamic Turbulence and in the Solar Wind
Cristian C. Lalescu, Yi-Kang Shi, Gregory L. Eyink, Theodore D. Drivas, Ethan T. Vishniac, and Alexander Lazarian
Phys. Rev. Lett. 115, 025001 (2015)

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