First PIC simulations capture the whistler heat-flux instability and show its saturation by reduced electron drifts and induced temperature anisotropies.
P., Neagu, E., Skoug, R
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Particle-in-cell simulations of the whistler heat-flux instability in the solar wind conditions
First PIC simulations capture the whistler heat-flux instability and show its saturation by reduced electron drifts and induced temperature anisotropies.