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Title: Nonlinear Reconnection in Magnetized Turbulence

Abstract

Recent analytical works on strong magnetized plasma turbulence have hypothesized the existence of a range of scales where the tearing instability may govern the energy cascade. In this paper, we estimate the conditions under which such tearing may give rise to full nonlinear magnetic reconnection in the turbulent eddies. When those conditions are met, a new turbulence regime is accessed where reconnection-driven energy dissipation becomes common, rather than the rare feature that it must be when they are not. We conclude that while such conditions are very stringent for fluid-scale eddies, they are easily met for kinetic-scale eddies; in particular, we suggest that our arguments may help explain recent Magnetospheric Multiscale (MMS) observations of (so-called) electron-only reconnection and of energy dissipation via electron Landau damping in the Earthʼs magnetosheath.

Authors:
;
Publication Date:
DOE Contract Number:  
SC0018266; SC0016215
Research Org.:
Univ. of Wisconsin, Madison, WI (United States); Massachusetts Inst. of Technology (MIT), Cambridge, MA (United States). Plasma Science and Fusion Center
Sponsoring Org.:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Subject:
70 PLASMA PHYSICS AND FUSION TECHNOLOGY; 79 ASTRONOMY AND ASTROPHYSICS
OSTI Identifier:
1884769
DOI:
https://doi.org/10.7910/DVN/LGOKIK

Citation Formats

Loureiro, N. F., and Boldyrev, S. Nonlinear Reconnection in Magnetized Turbulence. United States: N. p., 2021. Web. doi:10.7910/DVN/LGOKIK.
Loureiro, N. F., & Boldyrev, S. Nonlinear Reconnection in Magnetized Turbulence. United States. doi:https://doi.org/10.7910/DVN/LGOKIK
Loureiro, N. F., and Boldyrev, S. 2021. "Nonlinear Reconnection in Magnetized Turbulence". United States. doi:https://doi.org/10.7910/DVN/LGOKIK. https://www.osti.gov/servlets/purl/1884769. Pub date:Sun Jun 27 00:00:00 EDT 2021
@article{osti_1884769,
title = {Nonlinear Reconnection in Magnetized Turbulence},
author = {Loureiro, N. F. and Boldyrev, S.},
abstractNote = {Recent analytical works on strong magnetized plasma turbulence have hypothesized the existence of a range of scales where the tearing instability may govern the energy cascade. In this paper, we estimate the conditions under which such tearing may give rise to full nonlinear magnetic reconnection in the turbulent eddies. When those conditions are met, a new turbulence regime is accessed where reconnection-driven energy dissipation becomes common, rather than the rare feature that it must be when they are not. We conclude that while such conditions are very stringent for fluid-scale eddies, they are easily met for kinetic-scale eddies; in particular, we suggest that our arguments may help explain recent Magnetospheric Multiscale (MMS) observations of (so-called) electron-only reconnection and of energy dissipation via electron Landau damping in the Earthʼs magnetosheath.},
doi = {10.7910/DVN/LGOKIK},
journal = {},
number = ,
volume = ,
place = {United States},
year = {2021},
month = {6}
}

Works referencing / citing this record:

Nonlinear Reconnection in Magnetized Turbulence
journal, February 2020