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Can the Time-Spectral Method GWRM Advance Fusion Transport Modelling?
KTH, School of Electrical Engineering and Computer Science (EECS), Fusion Plasma Physics.ORCID iD: 0000-0003-0160-4060
KTH, School of Electrical Engineering and Computer Science (EECS), Fusion Plasma Physics.ORCID iD: 0000-0001-6379-1880
2017 (English)In: 59th Annual Meeting of the APS Division of Plasma Physics, 2017Conference paper, Oral presentation with published abstract (Refereed)
Abstract [en]

Transport phenomena in fusion plasma pose a daunting task for both real-time experiments and numerical modelling. The transport is driven by micro-instabilities caused by a host of unstable modes, for example ion temperature gradient and trapped electron modes. These modes can be modelled using fluid or gyrokinetic equations. However, the equations are characterised by high degrees of freedom and high temporal and spatial numerical requirements. Thus, a time-spectral method GWRM has been developed in order to efficiently solve these multiple time scale equations. The GWRM assumes a multivariate Chebyshev expansion ansatz in time, space, and parameter domain. Advantages are that time constraining CFL criteria no longer apply and that the solution accurately averages over small time-scale dynamics. For benchmarking, a two-fluid 2D drift wave turbulence model has been solved in order to study toroidal ion temperature gradient growth rates and nonlinear behaviour.

Place, publisher, year, edition, pages
2017.
National Category
Natural Sciences
Research subject
Physics
Identifiers
URN: urn:nbn:se:kth:diva-240838OAI: oai:DiVA.org:kth-240838DiVA, id: diva2:1274976
Conference
59th Annual Meeting of the APS Division of Plasma Physics, Milwaukee, Wisconsin, USA, 23 October – 27 October 2017
Note

QC 20190121

Available from: 2019-01-04 Created: 2019-01-04 Last updated: 2019-01-21Bibliographically approved

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