Magnetohydrodynamic Turbulence in the Plasmoid-mediated Regime

Comisso, L.; Huang, Y. -M.; Lingam, M.; Hirvijoki, E.; Bhattacharjee, A.

doi:10.3847/1538-4357/aaac83

Title: Magnetohydrodynamic Turbulence in the Plasmoid-mediated Regime

Journal Article · Fri Feb 16 00:00:00 EST 2018 · The Astrophysical Journal (Online)

DOI:https://doi.org/10.3847/1538-4357/aaac83· OSTI ID:1425071

^[1];

^[2]; Hirvijoki, E. ^[3]; Bhattacharjee, A. ^[1]

Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States); Princeton Univ., NJ (United States)
Harvard Univ., Cambridge, MA (United States); Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
Princeton Plasma Physics Lab. (PPPL), Princeton, NJ (United States)

Magnetohydrodynamic turbulence and magnetic reconnection are ubiquitous in astrophysical environments. In most situations these processes do not occur in isolation but interact with each other. This renders a comprehensive theory of these processes highly challenging. Here we propose a theory of magnetohydrodynamic turbulence driven at a large scale that self-consistently accounts for the mutual interplay with magnetic reconnection occurring at smaller scales. Magnetic reconnection produces plasmoids (flux ropes) that grow from turbulence-generated noise and eventually disrupt the sheet-like structures in which they are born. The disruption of these structures leads to a modification of the turbulent energy cascade, which in turn exerts a feedback effect on the plasmoid formation via the turbulence-generated noise. The energy spectrum in this plasmoid-mediated range steepens relative to the standard inertial range and does not follow a simple power law. As a result of the complex interplay between turbulence and reconnection, we also find that the length scale that marks the beginning of the plasmoid-mediated range and the dissipation length scale do not obey true power laws. The transitional magnetic Reynolds number above which the plasmoid formation becomes statistically significant enough to affect the turbulent cascade is fairly modest, implying that plasmoids are expected to modify the turbulent path to dissipation in many astrophysical systems

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Research Organization:: Princeton Plasma Physics Laboratory (PPPL), Princeton, NJ (United States)

Sponsoring Organization:: USDOE

Grant/Contract Number:: AC02-09-CH11466

OSTI ID:: 1425071

Journal Information:: The Astrophysical Journal (Online), Vol. 854, Issue 2; ISSN 1538-4357

Publisher:: Institute of Physics (IOP)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 38 works

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3D turbulent reconnection: Theory, tests, and astrophysical implications Lazarian, Alex; Eyink, Gregory L.; Jafari, Amir Physics of Plasmas, Vol. 27, Issue 1 https://doi.org/10.1063/1.5110603	journal	January 2020
The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A* Chael, Andrew; Rowan, Michael; Narayan, Ramesh Monthly Notices of the Royal Astronomical Society, Vol. 478, Issue 4 https://doi.org/10.1093/mnras/sty1261	journal	June 2018
Stochastic Reconnection for Large Magnetic Prandtl Numbers Jafari, Amir; Vishniac, Ethan T.; Kowal, Grzegorz The Astrophysical Journal, Vol. 860, Issue 1 https://doi.org/10.3847/1538-4357/aac517	journal	June 2018
Large-scale Compression Acceleration during Magnetic Reconnection in a Low- β Plasma Li, Xiaocan; Guo, Fan; Li, Hui The Astrophysical Journal, Vol. 866, Issue 1 https://doi.org/10.3847/1538-4357/aae07b	journal	October 2018
The Interplay of Magnetically Dominated Turbulence and Magnetic Reconnection in Producing Nonthermal Particles Comisso, Luca; Sironi, Lorenzo The Astrophysical Journal, Vol. 886, Issue 2 https://doi.org/10.3847/1538-4357/ab4c33	journal	November 2019
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