Explicit sufficient stability criteria and a Hall MHD energy principle for XMHD equilibria with flow, derived from energy-Casimir, dynamically accessible, and Lagrangian methods.
F ′ = G′ = 0, it is clear that Q > 0 implies δ2HC > 0
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Energy-Casimir, dynamically accessible, and Lagrangian stability of extended magnetohydrodynamic equilibria
Explicit sufficient stability criteria and a Hall MHD energy principle for XMHD equilibria with flow, derived from energy-Casimir, dynamically accessible, and Lagrangian methods.