2D particle-in-cell simulations reveal that weakly magnetized quasi-parallel shocks transition from Bell-dominated (inefficient electron acceleration) to Weibel-dominated (efficient electron acceleration) regimes at an Alfvénic Mach number of ~100.
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Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
Large-scale statistical study finds quasi-perpendicular interplanetary shocks enhance perpendicular proton temperatures downstream, deviate from CGL predictions, and are regulated by instabilities.
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Dependence of Particle Acceleration Efficiency on Shock Velocity in Weakly Magnetized Electron-Ion Shocks
2D particle-in-cell simulations reveal that weakly magnetized quasi-parallel shocks transition from Bell-dominated (inefficient electron acceleration) to Weibel-dominated (efficient electron acceleration) regimes at an Alfvénic Mach number of ~100.
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Energetic particle-mediated interplanetary shocks observed by Solar Orbiter
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
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Proton Temperature Anisotropy Across Interplanetary Shocks: A Statistical Analysis with WIND observations
Large-scale statistical study finds quasi-perpendicular interplanetary shocks enhance perpendicular proton temperatures downstream, deviate from CGL predictions, and are regulated by instabilities.