Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session GP12: Poster Session III:
Low Temperature Plasmas
Fundamental Plasma Physics I: computation, boundaries
Fundamental Plasma Physics II: dusty, diagnostics
MFE Measurement and Diagnostics Techniques, Technology, and Edge and Pedestal Physics
9:30 AM - 12:30 PM
Tuesday, October 8, 2024
Hyatt Regency
Room: Grand Hall West
Abstract: GP12.00043 : Kinetic spectral simulations with local-implicit global-explicit approach*
Presenter:
Oleksandr Chapurin
(Los Alamos National Laboratory)
Authors:
Oleksandr Chapurin
(Los Alamos National Laboratory)
Oleksandr Koshkarov
(Los Alamos National Laboratory)
Gian Luca Delzanno
(Los Alamos National Laboratory (LANL))
Cale Harnish
(Los Alamos National Laboratory)
Alexander A Hrabski
(Los Alamos National Laboratory)
Salomon Janhunen
(Los Alamos National Laboratory)
Ryan T Wollaeger
(Los Alamos National Laboratory)
Zach Jibben
(Los Alamos National Laboratory)
Peter T Brady
(Los Alamos National Laboratory)
Daniel Livescu
(LANL)
retain drastic time scale separation which is common for plasma and fluid applications.
Thus, for GD problems, the BGK operator introduces a stiff collisional term, while for the VA system, the stiff parts are the particle acceleration term and current source in Ampere's equation.
The purpose of this presentation is to show speed-up by stepping over fast scale dynamics. This procedure ensures locality in physical space for the implicit part, making it particularly efficient where standard physical space domain decomposition is used.
The local property makes the parallel implementation and its preconditioning significantly easier than for a
fully implicit methods which require global nonlinear iterations.
Both GD and VA systems use a spectral expansion in velocity space that leverages Hermite basis, and finite differences for spatial discretization.
To illustrate the method, we present a Sedov problem, where an initial pressure gradient leads to shock-wave formation and its propagation with IMEX time stepping exceeds the explicit time step by ∼104 times yet recovers the correct dynamics accurately. For plasma applications, the evolution of a large magnetohydrodynamics scale ion-acoustic wave can be evolved with IMEX time stepping of over ∼800 the fastest scale of the problem, which is the electron plasma period.
*This work was supported by the Laboratory Directed Research and Development Program of Los Alamos National Laboratory under project number 20220104DR. Los Alamos National Laboratory is operated by Triad National Security,LLC, for the National Nuclear Security Administration ofU.S. Department of Energy (Contract No. 89233218CNA000001).Computational resources for the simulations were provided by the Los Alamos National Laboratory Institutional Computing Program.
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