Results 11 to 20 of about 2,894,075 (299)

Electron-Only Reconnection in Plasma Turbulence

open access: yesFrontiers in Physics, 2020
Hybrid-Vlasov–Maxwell simulations of magnetized plasma turbulence including non-linear electron-inertia effects in a generalized Ohm's law are presented.
Francesco Califano   +7 more
doaj   +2 more sources

Dependence of Kinetic Plasma Turbulence on Plasma β [PDF]

open access: yesThe Astrophysical Journal Letters, 2018
Abstract We study the effects of plasma β (the ratio of plasma pressure to magnetic pressure) on the evolution of kinetic plasma turbulence using fully kinetic particle-in-cell simulations of decaying turbulence. We find that the plasma β systematically affects spectra, measures of intermittency, decay rates of turbulence fluctuations ...
Tulasi N. Parashar   +2 more
openaire   +4 more sources

The GBS code for the self-consistent simulation of plasma turbulence and kinetic neutral dynamics in the tokamak boundary [PDF]

open access: yesJournal of Computational Physics, 2021
A new version of GBS (Ricci et al. Plasma Phys. Control. Fusion 54, 124047, 2012; Halpern et al. J. Comput. Phys. 315, 388-408, 2016; Paruta et al. Phys. Plasmas 25, 112301, 2018) is described.
M. Giacomin   +9 more
semanticscholar   +1 more source

Ion and Electron Acceleration in Fully Kinetic Plasma Turbulence [PDF]

open access: yesAstrophysical Journal Letters, 2022
Turbulence is often invoked to explain the origin of nonthermal particles in space and astrophysical plasmas. By means of 3D fully kinetic particle-in-cell simulations, we demonstrate that turbulence in low-β plasmas (β is the ratio of plasma pressure to
L. Comisso, L. Sironi
semanticscholar   +1 more source

Ion-scale Transition of Plasma Turbulence: Pressure–Strain Effect [PDF]

open access: yesAstrophysical Journal, 2022
We investigate properties of solar-wind-like plasma turbulence using direct numerical simulations. We analyze the transition from large, magnetohydrodynamic (MHD) scales to the ion characteristic ones using two-dimensional hybrid (fluid electrons and ...
P. Hellinger   +6 more
semanticscholar   +1 more source

Evidence for electron Landau damping in space plasma turbulence. [PDF]

open access: yesNat Commun, 2019
How turbulent energy is dissipated in weakly collisional space and astrophysical plasmas is a major open question. Here, we present the application of a field-particle correlation technique to directly measure the transfer of energy between the turbulent
Chen CHK, Klein KG, Howes GG.
europepmc   +3 more sources

Identification of Active Magnetic Reconnection Using Magnetic Flux Transport in Plasma Turbulence [PDF]

open access: yesAstrophysical Journal Letters, 2021
Magnetic reconnection has been suggested to play an important role in the dynamics and energetics of plasma turbulence by spacecraft observations, simulations, and theory over the past two decades, and recently, by magnetosheath observations of MMS.
T. Li, Yi‐Hsin Liu, Y. Qi
semanticscholar   +1 more source

Thermal disequilibration of ions and electrons by collisionless plasma turbulence. [PDF]

open access: yesProc Natl Acad Sci U S A, 2019
Significance Large-scale astrophysical processes inject energy into turbulent motions and electromagnetic fields, which carry this energy to small scales and eventually thermalize it. How this energy is partitioned between ions and electrons is important
Kawazura Y, Barnes M, Schekochihin AA.
europepmc   +3 more sources

Relativistic Particle Transport and Acceleration in Structured Plasma Turbulence [PDF]

open access: yesAstrophysical Journal, 2021
We discuss the phenomenon of energization of relativistic charged particles in three-dimensional incompressible MHD turbulence and the diffusive properties of the motion of the same particles.
O. Pezzi, P. Blasi, W. Matthaeus
semanticscholar   +1 more source

Data-driven model discovery for plasma turbulence modelling

open access: yesJournal of Plasma Physics, 2022
An important problem in nuclear fusion plasmas is the prediction and control of turbulence which drives the cross-field transport, thus leading to energy loss from the system and deteriorating confinement.
I. Abramovic, E. Alves, M. Greenwald
semanticscholar   +1 more source

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