Particle transport in hybrid PIC shock simulations: A comparison of diagnostics

Abstract

Recent in-situ and remote observations suggest that the transport regime associated with shock accelerated particles may be anomalous i.e., the Mean Square Displacement (MSD) of such particles scales non-linearly with time. We use self-consistent, hybrid PIC plasma simulations to simulate a quasi-parallel shock with parameters compatible with heliospheric shocks, and gain insights about the particle transport in such a system. For suprathermal particles interacting with the shock we compute the MSD separately in the upstream and downstream regions. Tracking suprathermal particles for sufficiently long times up and/or downstream of the shock poses problems in particle plasma simulations, such as statistically poor particle ensembles and trajectory fragments of variable length in time. Therefore, we introduce the use of time-averaged mean square displacement (TAMSD), which is based on single particle trajectories, as an additional technique to address the transport regime for the upstream and downstream regions. MSD and TAMSD are in agreement for the upstream energetic particle population, and both give a strong indication of superdiffusive transport, consistent with interplanetary shock observations. MSD and TAMSD are also in reasonable agreement downstream, where indications of anomalous transport are also found. TAMSD shows evidence of heterogeneity in the diffusion properties of the downstream particle population, ranging from subdiffusive behaviour of particles trapped in the strong magnetic field fluctuations generated at the shock, to superdiffusive behaviour of particles transmitted and moving away from the shock.

Solar Energetic Particles

“…Particle-in cell (PIC) simulations show these variations (e.g. Trotta et al 2020) and small-scale variations have been observed in interplanetary shocks by the Cluster spacecraft (e.g. ).…”

Phase space transport in the interaction between shocks and plasma turbulence

“…For instance, shock-reflected particles may show superdiffusive behavior (e.g., ref. 53), and coherent structures present in the up-/downstream of the shock provide excellent traps (or accelerators) for energetic particles (40).…”

Hydrogen Abundances and Shock Waves

“…Particle-in cell (PIC) simulations show these variations (e.g. Trotta et al 2020) and small-scale variations have been observed in interplanetary shocks by the Cluster spacecraft (e.g. Kajdič et al 2019).…”