scispace - formally typeset
Open AccessJournal ArticleDOI

Viscous dissipation in 3D spine reconnection solutions

Reads0
Chats0
TLDR
It is shown that viscous dissipation in spine reconnection models can dominate resistive damping by many orders of magnitude and applies to current sheet “fan” solutions.
Abstract
Aims. We consider the influence of viscous dissipation on “spine” reconnection solutions in coronal plasmas. It is known from 2D and 3D “fan” reconnection studies that viscous losses can be important. We extend these arguments to 3D “spine” reconnection solutions. Methods. Steady 3D spine reconnection models were constructed by time relaxation of the governing visco-resistive MHD equations. Scaling laws were derived that compare the relative importance of viscous and resistive damping. Results. It is shown that viscous dissipation in spine reconnection models can dominate resistive damping by many orders of magnitude. A similar conclusion, but with less severe implications, applies to current sheet “fan” solutions. These findings are not sensitive to whether classical or Braginskii viscosity is employed.

read more

Content maybe subject to copyright    Report

Citations
More filters
Journal ArticleDOI

Extended Magnetohydrodynamic Simulations of Decaying, Homogeneous, Approximately-Isotropic and Incompressible Turbulence

Hideaki Miura
- 11 Mar 2019 - 
TL;DR: In this paper, the effects of the Hall and gyro-viscosity on the energy transfer in the equations of motions of motions were studied by means of direct numerical simulations of freely decaying, homogeneous and approximately isotropic turbulence.
Journal ArticleDOI

The effect of anisotropic viscosity on the nonlinear MHD kink instability

TL;DR: It is shown that the form of viscosity has a significant effect on the nonlinear dynamics of the instability, affecting the behaviour of magnetic relaxation, the formation of secondary instabilities and the Ohmic and viscous heating produced.
Journal ArticleDOI

The Evolution of Quasi-Separatrix Layer in Two Solar Eruptive Events

TL;DR: In this article, the authors used the theory of quasi-separatrix layer (QSL) to calculate the logarithmic distribution of Q-factors at different heights above the solar photosphere with the results of the PF and NLFFF extrapolations, in order to determine the location of QSL.
References
More filters
Book

Magnetic Reconnection: MHD Theory and Applications

TL;DR: Magnetic reconnection is at the core of many dynamic phenomena in the universe, such as solar flares, geomagnetic substorms and tokamak disruptions as discussed by the authors.
Journal ArticleDOI

Three-dimensional kinematic reconnection in the presence of field nulls and closed field lines

TL;DR: In this article, the geometric structures of configurations with a pair of type A and B nulls permit reconnection across the null-null lines; these are the field lines which join the two nulls.
Journal ArticleDOI

Numerical tests of fast reconnection in weakly stochastic magnetic fields

TL;DR: In this paper, the effects of turbulence on magnetic reconnection using three-dimensional direct numerical simulations were studied. And the authors found that the reconnection speed is proportional to the square root of the injected power, as predicted by the model.
Journal ArticleDOI

Magnetic Reconnection at Three-Dimensional Null Points

TL;DR: In this article, the skeleton of an isolated null point in three dimensions consists of a "spine curve" and a "fan surface" and the kinematics of steady reconnection at such a null point are considered, depending on the nature of the imposed boundary conditions on the surface that encloses the null, in particular on a cylindrical surface with its axis along the spine.

Magnetic Reconnection at Three-Dimensional Null Points

TL;DR: In this article, the skeleton of an isolated null point in three dimensions consists of a "spine curve" and a "fan surface" and the kinematics of steady reconnection at such a null point are considered, depending on the nature of the imposed boundary conditions on the surface that encloses the null, in particular on a cylindrical surface with its axis along the spine.
Related Papers (5)