Results 1 to 10 of about 6,104 (166)

Direct Evidence of Magnetic Reconnection Onset via the Tearing Instability

open access: yesFrontiers in Astronomy and Space Sciences, 2022
Magnetic reconnection is a sporadic process responsible for energy release in space and laboratory plasmas. It is believed that the tearing mode instability may be responsible for the onset of reconnection in the magnetotail.
Mayur R. Bakrania   +7 more
doaj   +3 more sources

Numerical studies on electron magnetohydrodynamics tearing mode instability

open access: yesAIP Advances, 2021
The 2D electron-magnetohydrodynamics (EMHD) dominant tearing mode in an electron-skin-depth-scale current sheet (ECS) is further studied. The resistive diffusion is proved to be insignificant at the scale.
Wenping Guo, Jiaqi Wang, Dongjian Liu
doaj   +1 more source

Tubular Pinch and Tearing Instability [PDF]

open access: yesThe Physics of Fluids, 1969
Theoretical considerations and previous experimental findings with fast tubular (cylindrical sheet) pinch discharges are reviewed briefly. More recent work with magnetic probes, as well as streak and Kerr cell photography, corroborates that the sheet-current configuration can be sufficiently stable to survive a fair number of pinch oscillations.
Anderson, Oscar A., Kunkel, Wulf B.
openaire   +2 more sources

The onset distribution of rotating tearing modes and its consequences on the stability of high-confinement-mode plasmas in DIII-D

open access: yesNuclear Fusion, 2023
Analysis of a multi-scenario database of over 13 000 DIII-D H-mode discharges shows that the $m,n = 2,1$ magnetic islands are dominantly pressure gradient driven, stochastically triggered non-linear instabilities at all edge safety factor ( $q_\text{95}$
L. Bardóczi, N.J. Richner, N.C. Logan
doaj   +1 more source

Tearing Instability and Current-Sheet Disruption in the Turbulent Dynamo

open access: yesPhysical Review X, 2022
Turbulence in a conducting plasma can amplify seed magnetic fields in what is known as the turbulent, or small-scale, dynamo. The associated growth rate and emergent magnetic-field geometry depend sensitively on the material properties of the plasma, in ...
Alisa K. Galishnikova   +2 more
doaj   +1 more source

Investigation of Tearing Modes on the Spherical Tokamak Globus-M2 Using the Doppler Backscattering Method

open access: yesApplied Sciences, 2023
In this study, we observed magnetohydrodynamic (MHD) activity of the spherical tokamak Globus-M2 which led to a deterioration in plasma confinement, such as a transition from the H-mode to L-mode, or even disruption.
Alexander Yashin   +9 more
doaj   +1 more source

Resistive instabilities in toroidal anisotropic plasmas

open access: yesAIP Advances, 2023
Resistive singular layer equations are developed by applying the magnetohydrodynamic (MHD) model to toroidal anisotropic plasmas. This work extends the previous ideal MHD theory [Shi et al. Phys. Plasmas 23, 082121 (2016)] to the resistive case.
Tonghui Shi, B. Shen, B. Wan
doaj   +1 more source

A fundamental understanding of the unstable eigenmodes of double tearing instabilities in a shear slab geometry

open access: yesAIP Advances, 2020
Two types of unstable eigenmodes of resistive tearing instabilities, namely, symmetric and anti-symmetric modes, in a double current sheet configuration are analyzed by means of both an eigenvalue solver and initial value simulation.
L. Wei, F. Yu, H. J. Ren, Z. X. Wang
doaj   +1 more source

Gyrokinetic simulations of the tearing instability [PDF]

open access: yesPhysics of Plasmas, 2011
Linear gyrokinetic simulations covering the collisional–collisionless transitional regime of the tearing instability are performed. It is shown that the growth rate scaling with collisionality agrees well with that predicted by a two-fluid theory for a low plasma beta case in which ion kinetic dynamics are negligible.
Numata, R.   +5 more
openaire   +2 more sources

Effects of compressibility and guiding field on the Kelvin–Helmholtz instability in weakly reversed magnetic shear configurations

open access: yesAIP Advances, 2022
The effects of compressibility and guiding field on the Kelvin–Helmholtz (KH) instability in a double resonant surface system are numerically investigated by using a compressible magnetohydrodynamics model.
Z. Li   +7 more
doaj   +1 more source

Home - About - Disclaimer - Privacy