PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.
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Observed CR pitch-angle diffusion matches quasi-slab fast-mode turbulence predictions shaped by damping, but not Alfvénic turbulence, evidencing fast-mode dominance and constraining LISM to low beta ≈0.1 with δB/B0 ≈0.5.
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PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
PIC simulations of oblique shocks in turbulent plasma show that pre-existing 15% compressive turbulence produces a shorter hotter foreshock and more numerous higher-energy non-thermal electrons.