Ultra-high-β WHFI saturates with δB∼B0 and regulates parallel heat flux by advection at the whistler phase velocity, giving q∥/qfs≈4.7βe−1 (2D3V) or ≈0.3βe−1/2 (1D3V).
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Collisionless whistler heat-flux instability in ultra-high-$\beta$ plasmas
Ultra-high-β WHFI saturates with δB∼B0 and regulates parallel heat flux by advection at the whistler phase velocity, giving q∥/qfs≈4.7βe−1 (2D3V) or ≈0.3βe−1/2 (1D3V).