Double Current Sheet Instabilities and the Transition to Turbulence.
Abstract
The double tearing instability has often been studied as a proxy for the m=1 kink mode in cylindrical plasma. In this paper we describe the results of 3D simulations of an initially periodic double current sheet described by Harris equilibria with a guide field in two cases: 1) zero net helicity and an average magnetic field and 2) a well defined helicity (force free but non constant alpha). We study and contrast the de-stabilization and transition to turbulence for these two cases: we describe spectra, cascades, and possible application to heliospheric phenomena, in particular CME evolution and relaxation. The research leading to these results has received fund- ing from the European Union's Seventh Framework Pro- gramme (FP7/2007-2013) under grant agreement No. 339032
- Publication:
-
AGU Fall Meeting Abstracts
- Pub Date:
- December 2016
- Bibcode:
- 2016AGUFMSH41A2528P
- Keywords:
-
- 2149 MHD waves and turbulence;
- INTERPLANETARY PHYSICSDE: 2164 Solar wind plasma;
- INTERPLANETARY PHYSICSDE: 7827 Kinetic and MHD theory;
- SPACE PLASMA PHYSICSDE: 7863 Turbulence;
- SPACE PLASMA PHYSICS