Self-adaptive Event-Driven Simulations of Multi-Scale Plasma Systems

dc.contributor.authorOmelchenko, Y.
dc.contributor.authorKarimabadi, H.
dc.contributor.authorGoldstein, Melvyn
dc.contributor.authorUsmanov, A.V.
dc.date.accessioned2023-11-13T19:52:34Z
dc.date.available2023-11-13T19:52:34Z
dc.date.issued2006
dc.descriptionASP Conference Series, 2006en_US
dc.description.abstractMulti-scale systems pose a formidable computational challenge. Explicit time stepping suffers from the global CFL restriction. Efficient application of adaptive mesh refinement (AMR) to systems with irregular dynamics (e.g. turbulence, reactive systems, particle acceleration etc.) may be problematic. To address these issues, we developed an alternative approach (Karimabadi et al. 2005; Omelchenko & Karimabadi 2006a,b) to time-stepped integration of physics-based systems: Discrete-Event Simulation (DES). We combine finite difference and particle-in-cell techniques with this new methodology by assuming two caveats: (1) a local time increment, ∆f for a discrete quantity f can be expressed in terms of a physically meaningful increment, ∆f; (2) f is considered to be modified only when its change exceeds ∆f. Event-driven asynchronous time advance makes use of local causality rules. This technique enables flux conserving integration of the solution, removes the curse of global CFL condition, and eliminates unnecessary computation in inactive regions. It can be naturally combined with various mesh refinement techniques. DES results in robust and fast simulation codes, which can be efficiently parallelized when implemented via a Preemptive Event Processing (PEP) technique (Omelchenko & Karimabadi 2006c). We discuss this novel technology in the context of diffusion reaction and computational fluid dynamics (CFD) applications, as well as general model-model (flux) coupling.en_US
dc.description.sponsorshipThis work was supported by NSF ITR program Grant 0529919, and NASA grants NNG05GJ01G and NNG06GE65G. The work of M. Goldstein was supported by NASA Supporting Research and Technology grant in Solar and Heliospheric Physics to the Goddard Space Flight Center. Simulations were partially performed at the San Diego Supercomputer Center, which is supported by the National Science Foundation.en_US
dc.description.urihttps://aspbooks.org/custom/publications/paper/359-0171.htmlen_US
dc.format.extent7 pagesen_US
dc.genreconference papers and proceedingsen_US
dc.genrebook chaptersen_US
dc.identifierdoi:10.13016/m2xhaj-veue
dc.identifier.citationOmelchenko, Y., et al. “Self-Adaptive Event-Driven Simulations of Multi-Scale Plasma Systems.” ASP Conference Series 359 (2006): 171– 177. https://aspbooks.org/custom/publications/paper/359-0171.html.en_US
dc.identifier.urihttp://hdl.handle.net/11603/30742
dc.language.isoen_USen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC Goddard Planetary Heliophysics Institute (GPHI)
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleSelf-adaptive Event-Driven Simulations of Multi-Scale Plasma Systemsen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0002-5317-988Xen_US

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