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- W3202362021 abstract "Interplanetary Coronal Mass Ejection (ICME) shocks are known to accelerate particles and contribute significantly to Solar Energetic Particle (SEP) events. We have performed Magnetohydrodynamic-Particle in Cell (MHD-PIC) simulations of ICME shocks to understand the acceleration mechanism. These shocks vary in Alfv'enic Mach numbers as well as in magnetic field orientations (parallel & quasi-perpendicular). We find that Diffusive Shock Acceleration (DSA) plays a significant role in accelerating particles in a parallel ICME shock. In contrast, Shock Drift Acceleration (SDA) plays a pivotal role in a quasi-perpendicular shock. High-Mach shocks are seen to accelerate particles more efficiently. Our simulations suggest that background turbulence and local particle velocity distribution around the shock can indirectly hint at the acceleration mechanism. Our results also point towards a few possible textit{in situ} observations that could validate our understanding of the topic." @default.
- W3202362021 created "2021-10-11" @default.
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- W3202362021 date "2021-12-01" @default.
- W3202362021 modified "2023-09-27" @default.
- W3202362021 title "Acceleration of Solar Energetic Particles by the Shock of Interplanetary Coronal Mass Ejection" @default.
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- W3202362021 doi "https://doi.org/10.3847/1538-4357/ac2c7a" @default.
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