arXiv · 2004.14653
Instability in a magnetised collisional plasma driven by a heat flow or a current
Abstract
We solve the linearised Vlasov-Fokker-Planck (VFP) equation to show that heat flow or an electrical current in a magnetized collisional plasma is unstable to the growth of a circularly polarised transverse perturbation to a zeroth order uniform magnetic field. The Braginskii (1965) transport equations exhibit the same instability in the appropriate limit. This is relevant to laser-produced plasmas, inertial fusion energy (IFE) and to dense cold interstellar plasmas.
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Anthony Bell, Robert Kingham, Henry Watkins, James Matthews. 2020-04-30. Instability in a magnetised collisional plasma driven by a heat flow or a current. https://doi.org/10.1088/1361-6587/ab8e1b
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