Abstract
Magnetic neutral sheets in weakly ionized interstellar gas are rapidly annihilated by ohmic diffusion. In this paper we extend the model to a sheared magnetic configuration, and show that the magnetic pressure associated with even a small nonzero field drastically reduces the reconnection rate of the reversing component.
Cite
CITATION STYLE
APA
Heitsch, F., & Zweibel, E. G. (2003). Suppression of Fast Reconnection by Magnetic Shear. The Astrophysical Journal, 590(1), 291–295. https://doi.org/10.1086/375009
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