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physics.plasm-ph2026
PIC simulations of nonrelativistic high-Mach-number oblique shocks propagating in a turbulent medium
Karol Fulat, Eloise Moore, Mahmoud Alawashra +4
Collisionless shocks are common in astrophysical systems and stand as sites of particle acceleration. While particles at perpendicular shocks may not return to the upstream region,…
physics.plasm-ph2023★ 11 cited
Pre-acceleration in the Electron Foreshock II: Oblique Whistler Waves
Paul J. Morris, Artem Bohdan, Martin S. Weidl +3
Thermal electrons have gyroradii many orders of magnitude smaller than the finite width of a shock, thus need to be pre-accelerated before they can cross it and be accelerated by d…