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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3 Pith papers cite this work, alongside 182 external citations. Polarity classification is still indexing.
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representative citing papers
Four Solar Orbiter interplanetary shocks show energetic particle pressure dominating upstream, indicating particle-mediated modification of collisionless shocks.
Numerical modeling of corrugated versus smooth CME-driven shocks indicates that wave-like features produce irregular shock-normal-angle distributions that predispose the shocks to varied particle-acceleration regimes.
citing papers explorer
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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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Corrugated Features in Coronal-mass-ejections-driven Shocks: A Discussion on the Predisposition to Particle Acceleration
Numerical modeling of corrugated versus smooth CME-driven shocks indicates that wave-like features produce irregular shock-normal-angle distributions that predispose the shocks to varied particle-acceleration regimes.