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Title: Turbulent heating due to magnetic reconnection

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4993423· OSTI ID:1497875

Dissipation of plasma turbulent energy is a phenomenon having significant implications for the heating of the solar corona and solar wind. While processes involving linear wave damping, stochastic heating, and reconnection have been postulated as contributors to heating mechanisms, the relative role that they play is not currently understood. In this manuscript, we establish a theoretical framework for applying reconnection heating predictions to turbulent systems. Kinetic particle-in-cell (PIC) simulations are used to study heating due to reconnection, and these results are then adapted to a turbulent medium. First, the factors controlling the heating of plasmas in reconnection exhausts are examined using laminar reconnection simulations; predictions for heating are determined which require only the plasma conditions just upstream of the reconnection diffusion region as input. The laminar predictions are then applied to PIC simulations of turbulence. Key assumptions are: (1) the plasma conditions just upstream of the diffusion region are consistent with Kolmogorov scaling of turbulent fluctuations at the ion inertial scale and (2) the statistics of the numbers of reconnecting x-lines do not vary significantly between the various turbulent simulations. We find that the reconnection theory predicts quite well the scaling of the ratio of ion to electron heating, in which the statistics of the turbulent reconnection sites are expected to roughly cancel. Separate ion and electron heating rates scale differently from the theory, however. This suggests that the statistics of the turbulent reconnection (e.g., number of x-lines, percentage of x-lines reconnecting) is playing an important role in determining the ion and electron heating.

Research Organization:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE
OSTI ID:
1497875
Journal Information:
Physics of Plasmas, Vol. 25, Issue 1; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 24 works
Citation information provided by
Web of Science

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Cited By (14)

The multi-scale nature of the solar wind journal December 2019
Interplay between intermittency and dissipation in collisionless plasma turbulence journal June 2019
ViDA: a Vlasov–DArwin solver for plasma physics at electron scales journal October 2019
Transition from ion-coupled to electron-only reconnection: Basic physics and implications for plasma turbulence journal August 2019
The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A* journal June 2018
Species Entropies in the Kinetic Range of Collisionless Plasma Turbulence: Particle-in-cell Simulations journal May 2018
Electron and Proton Heating in Transrelativistic Guide Field Reconnection journal February 2019
Proton–Proton Collisions in the Turbulent Solar Wind: Hybrid Boltzmann–Maxwell Simulations journal December 2019
Energy Partition between Ion and Electron of Collisionless Magnetic Reconnection journal November 2018
The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A* text January 2018
Interplay between intermittency and dissipation in collisionless plasma turbulence text January 2018
Energy Partition between Ion and Electron of Collisionless Magnetic Reconnection text January 2018
Electron and Proton Heating in Transrelativistic Guide Field Reconnection text January 2019
Proton-proton collisions in the turbulent solar wind: Hybrid Boltzmann-Maxwell simulations text January 2019

Figures / Tables (8)


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