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Tearing Instability in Alfvén and Kinetic‐Alfvén Turbulence
Recently, it has been realized that magnetic plasma turbulence and magnetic field reconnection are inherently related phenomena. Turbulent fluctuations generate regions of sheared magnetic field that become unstable to the tearing instability and reconnection, thus modifying turbulence at the corres...
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Published in: | Journal of geophysical research. Space physics 2020-09, Vol.125 (9), p.n/a |
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Main Authors: | , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Recently, it has been realized that magnetic plasma turbulence and magnetic field reconnection are inherently related phenomena. Turbulent fluctuations generate regions of sheared magnetic field that become unstable to the tearing instability and reconnection, thus modifying turbulence at the corresponding scales. In this contribution, we give a brief review of some recent results on tearing‐mediated magnetic turbulence. We illustrate the main ideas of this rapidly developing field of study by concentrating on two important examples—magnetohydrodynamic Alfvén turbulence and small‐scale kinetic‐Alfvén turbulence. Due to various potential applications of these phenomena in space physics and astrophysics, we specifically try not to overload the text by heavy analytical derivations but rather present a qualitative discussion accessible to a non‐expert in the theories of turbulence and reconnection.
Key Points
Magnetic turbulence and magnetic reconnection are inherently related phenomena
Tearing instability modifies energy cascades in both magnetohydrodynamic and kinetic plasma turbulence
Conservation laws play an important role in governing tearing instability effects in magnetic turbulence |
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ISSN: | 2169-9380 2169-9402 |
DOI: | 10.1029/2020JA028185 |