Kinetic Modeling of Magnetospheres
Stefano Markidis, Vyacheslav Olshevsky, Gabor Toth, Yuxi Chen, Ivy, Peng, Giovanni Lapenta, Tamas Gombosi

TL;DR
This paper reviews advanced kinetic modeling techniques for simulating plasma dynamics in magnetospheres, highlighting numerical methods and their application to particle acceleration in Ganymede's magnetic reconnection.
Contribution
It introduces novel numerical approaches for large-scale kinetic simulations and demonstrates their application to Ganymede's magnetospheric phenomena.
Findings
Effective parameter scaling enables large-scale simulations
Implicit Particle-in-Cell schemes improve stability
Fluid-kinetic coupling enhances modeling accuracy
Abstract
This paper presents the state of the art of kinetic modeling techniques for simulating plasma kinetic dynamics in magnetospheres. We describe the critical numerical techniques for enabling large-scale kinetic simulations of magnetospheres: parameter scaling, implicit Particle-in-Cell schemes, and fluid-kinetic coupling. We show an application of these techniques to study particle acceleration and heating in asymmetric magnetic reconnection in the Ganymede magnetosphere.
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Gas Dynamics and Kinetic Theory
