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...
| Váldodahkkit: | , |
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| Eará dahkkit: | |
| Materiálatiipa: | Artihkal |
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American Astronomical Society
2018
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| Liŋkkat: | http://hdl.handle.net/1721.1/117010 https://orcid.org/0000-0001-9755-6563 |