Flexible Kinetic Coupling Model with FLEKS for Simulating Ganymede's Magnetosphere
Abstract
To capture the local kinetic processes within fluid simulations, we couple the MHD model BATS-R-US to the recently developed implicit kinetic particle-in-cell (PIC) model Flexible Exascale Kinetic Simulator (FLEKS). This new model allows the users to set flexible PIC regions based on geometric and physical criteria, and is more efficient in doing large scale parallelized simulations. The coupled model is applied to the magnetosphere simulation of Ganymede, with the high-resolution PIC region covering the entire magnetopause and tail current sheet. The prolific outputs of electrons and ions from kinetic simulation shed light on the reconnection driven physics across the entire magnetosphere that are not available in the simplified fluid description.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2020
- Bibcode:
- 2020AGUFMSM0540015Z
- Keywords:
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- 6025 Interactions with solar wind plasma and fields;
- PLANETARY SCIENCES: COMETS AND SMALL BODIES;
- 5706 Aurorae;
- PLANETARY SCIENCES: FLUID PLANETS;
- 5729 Ionospheres;
- PLANETARY SCIENCES: FLUID PLANETS;
- 5737 Magnetospheres;
- PLANETARY SCIENCES: FLUID PLANETS