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A first model of stable magnetic configuration in stellar radiation zones
2010
Proceedings of the International Astronomical Union
AbstractWe test the stability of a magnetic equilibrium configuration using numerical simulations and semi-analytical tools. The tested configuration is, as described by Duez & Mathis (2010), the lowest energy state for a given helicity in a stellar radiation zone. We show using 3D magneto-hydrodynamic (MHD) simulations that the present configuration is stable with respect to all submitted perturbations, that would lead to the development of kink-type instabilities in the case of purely
doi:10.1017/s1743921311007514
fatcat:jqpvwkkmjjguvfp2uucsjmque4