skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Energy dynamics and current sheet structure in fluid and kinetic simulations of decaying magnetohydrodynamic turbulence

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.4916492· OSTI ID:1291217
ORCiD logo [1];  [2];  [3];  [3];  [1]
  1. Univ. of Chicago, IL (United States)
  2. Univ. of Wisconsin, Madison, WI (United States)
  3. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

We performed simulations of decaying magnetohydrodynamic (MHD) turbulence with a fluid and a kinetic code. The initial condition is an ensemble of long-wavelength, counter-propagating, shear-Alfvén waves, which interact and rapidly generate strong MHD turbulence. The total energy is conserved and the rate of turbulent energy decay is very similar in both codes, although the fluid code has numerical dissipation, whereas the kinetic code has kinetic dissipation. The inertial range power spectrum index is similar in both the codes. The fluid code shows a perpendicular wavenumber spectral slope of k-1.3⊥k⊥-1.3. The kinetic code shows a spectral slope of k-1.5⊥k⊥-1.5 for smaller simulation domain, and k-1.3⊥k⊥-1.3 for larger domain. We then estimate that collisionless damping mechanisms in the kinetic code can account for the dissipation of the observed nonlinear energy cascade. Current sheets are geometrically characterized. Their lengths and widths are in good agreement between the two codes. The length scales linearly with the driving scale of the turbulence. In the fluid code, their thickness is determined by the grid resolution as there is no explicit diffusivity. In the kinetic code, their thickness is very close to the skin-depth, irrespective of the grid resolution. Finally, this work shows that kinetic codes can reproduce the MHD inertial range dynamics at large scales, while at the same time capturing important kinetic physics at small scales.

Research Organization:
Los Alamos National Laboratory (LANL), Los Alamos, NM (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Fusion Energy Sciences (FES)
Grant/Contract Number:
AC52-06NA25396
OSTI ID:
1291217
Alternate ID(s):
OSTI ID: 1228297
Report Number(s):
LA-UR-15-22879; PHPAEN
Journal Information:
Physics of Plasmas, Vol. 22, Issue 4; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 38 works
Citation information provided by
Web of Science

References (35)

Magnetohydrodynamic Turbulence book August 2009
MHD Turbulence at the Laboratory Scale: Established Ideas and New Challenges journal March 1997
Colloquium: Magnetohydrodynamic turbulence and time scales in astrophysical and space plasmas journal December 2004
Inertial-Range Spectrum of Hydromagnetic Turbulence journal January 1965
Toward a theory of interstellar turbulence. 2: Strong alfvenic turbulence journal January 1995
MHD‐driven Kinetic Dissipation in the Solar Wind and Corona journal July 2000
Turbulent heating in galaxy clusters brightest in X-rays journal October 2014
A model of turbulence in magnetized plasmas: Implications for the dissipation range in the solar wind: DISSIPATION OF THE SOLAR WIND journal May 2008
Astrophysical Gyrokinetics: Kinetic and Fluid Turbulent Cascades in Magnetized Weakly Collisional Plasmas journal May 2009
Kinetic Simulations of Magnetized Turbulence in Astrophysical Plasmas journal February 2008
Spectral features of solar wind turbulent plasma: Spectral features of solar wind turbulent plasma journal December 2009
Test Particle Energization by Current Sheets and Nonuniform Fields in Magnetohydrodynamic Turbulence journal December 2004
On the Spectrum of Magnetohydrodynamic Turbulence journal May 2005
Intermittent Dissipation at Kinetic Scales in Collisionless Plasma Turbulence journal November 2012
Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence journal June 2013
Coherent structures, intermittent turbulence, and dissipation in high-temperature plasmas journal January 2013
Current Sheets and Collisionless Damping in Kinetic Plasma Turbulence journal June 2013
Collisionless Damping at Electron Scales in Solar wind Turbulence journal August 2013
An oscillating Langevin antenna for driving plasma turbulence simulations journal February 2014
PLUTO: A Numerical Code for Computational Astrophysics journal May 2007
Ultrahigh performance three-dimensional electromagnetic relativistic kinetic plasma simulation journal May 2008
Shell-to-shell energy transfer in magnetohydrodynamics. I. Steady state turbulence journal October 2005
Scale Locality of Magnetohydrodynamic Turbulence journal February 2010
On Weak and Strong Magnetohydrodynamic Turbulence journal December 2007
Quantifying energetics and dissipation in magnetohydrodynamic turbulence journal December 2013
Dissipation Wavenumbers for Turbulence in Electron–Positron Plasmas journal August 2009
Energy Dissipation in Magnetohydrodynamic Turbulence: Coherent Structures or “Nanoflares”? journal October 2014
Streaming sausage, kink and tearing instabilities in a current sheet with applications to the Earth's magnetotail journal January 1988
Kinetic theory of the drift kink instability in a current sheet journal December 1998
Decay Laws for Three-Dimensional Magnetohydrodynamic Turbulence journal September 1999
Spectral Scaling laws in Magnetohydrodynamic Turbulence Simulations and in the Solar wind journal October 2011
Dissipation in Compressible Magnetohydrodynamic Turbulence journal November 1998
Compressible Sub-Alfvénic MHD Turbulence in Low- β Plasmas journal May 2002
Magnetic Reconnection in Two-Dimensional Magnetohydrodynamic Turbulence journal March 2009
Energy transfer in Hall-MHD turbulence: cascades, backscatter, and dynamo action journal June 2007

Cited By (20)

Slab magnetised non-relativistic low-beta electron–positron plasmas: collisionless heating, linear waves and reconnecting instabilities journal December 2017
Kinetic Properties of Solar Wind Discontinuities at 1 AU Observed by ARTEMIS journal June 2019
Particle acceleration during magnetic reconnection in a low-beta pair plasma journal May 2016
Driving reconnection in sheared magnetic configurations with forced fluctuations journal February 2018
Study of magnetic reconnection in large-scale magnetic island coalescence via spatially coupled MHD and PIC simulations journal August 2018
3D turbulent reconnection: Theory, tests, and astrophysical implications journal January 2020
Observations of AlfvÉN and slow Waves in the Solar wind near 1 au journal December 2015
Stochastic reacceleration of relativistic electrons by turbulent reconnection: a mechanism for cluster-scale radio emission? journal March 2016
Magnetohydrodynamic Turbulence in the Plasmoid-mediated Regime journal February 2018
Parametric Decay Instability and Dissipation of Low-frequency Alfvén Waves in Low-beta Turbulent Plasmas journal March 2018
Dissipation Scale Lengths of Solar Wind Turbulence journal February 2019
Contextual Predictions for the Parker Solar Probe . I. Critical Surfaces and Regions journal March 2019
Turbulence in Magnetized Pair Plasmas journal October 2018
Stochastic reacceleration of relativistic electrons by turbulent reconnection: a mechanism for cluster-scale radio emission ? text January 2016
Particle Acceleration during Magnetic Reconnection in a Low-beta Pair Plasma text January 2016
Parametric Decay Instability and Dissipation of Low-frequency Alfvén Waves in Low-beta Turbulent Plasmas text January 2017
Magnetohydrodynamic Turbulence in the Plasmoid-Mediated Regime text January 2018
Role of the Plasmoid Instability in Magnetohydrodynamic Turbulence text January 2018
Contextual Predictions for Parker Solar Probe I: Critical Surfaces and Regions text January 2018
3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications text January 2020