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Adaptive Global Magnetohydrodynamic Simulations

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Space and Astrophysical Plasma Simulation

Abstract

This chapter briefly summarizes global MHD codes that are presently used in geospace modeling with particular attention to their availability for community use through the Community Coordinated Modeling Center (CCMC). It describes the underlining methodologies of modern codes using the University of Michigan’s Space Weather Modeling Framework (SWMF) and the Block-Adaptive Tree Solar-Wind Roe-Type Upwind Scheme (BATS-R-US) multi-physics code. We also describe the new MHD with embedded PIC (MHD-EPIC) code, the latest development in adaptive physics approach.

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Acknowledgements

This work was supported by the NSF Strategic Capabilities grant AGS-1322543, by the NASA Heliophysics Strategic Capabilities grant 80NSSC19K0373, and by the NASA Magnetospheric Multi-Scale mission contract 80NSSC19K0564.

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  1. Department of Climate and Space Sciences and Engineering, University of Michigan, Ann Arbor, MI, USA

    Tamas I. Gombosi, Yuxi Chen, Zhenguang Huang, Ward B. Manchester, Igor Sokolov, Gabor Toth & Bart van der Holst

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Gombosi, T.I. et al. (2023). Adaptive Global Magnetohydrodynamic Simulations. In: BĂĽchner, J. (eds) Space and Astrophysical Plasma Simulation. Springer, Cham. https://doi.org/10.1007/978-3-031-11870-8_7

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