Collisionless Reconnection in Magnetohydrodynamic and Kinetic Turbulence
It has recently been proposed that the inertial interval in magnetohydrodynamic (MHD) turbulence is terminated at small scales not by a Kolmogorov-like dissipation region, but rather by a new sub-inertial interval mediated by tearing instability. However, many astrophysical plasmas are nearly collis...
Main Authors: | , |
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Other Authors: | , |
Format: | Article |
Language: | English |
Published: |
American Astronomical Society,
2018-07-19T17:51:45Z.
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Subjects: | |
Online Access: | Get fulltext |