The use of Bayesian inversion to resolve plasma equilibrium
| dc.contributor.author | Hole, M. J. | |
| dc.contributor.author | von Nessi, G. | |
| dc.contributor.author | Pretty, D. | |
| dc.contributor.author | Howard, J. | |
| dc.contributor.author | Blackwell, B. | |
| dc.contributor.author | Svensson, J. | |
| dc.contributor.author | Appel, L. C. | |
| dc.date.accessioned | 2015-12-09T00:48:43Z | |
| dc.date.available | 2015-12-09T00:48:43Z | |
| dc.date.issued | 2010-10-27 | |
| dc.date.updated | 2016-02-24T11:22:27Z | |
| dc.description.abstract | Recently, bayesian probability theory has been used at a number of experiments to fold uncertainties and interdependencies in the diagnostic data and forward models, together with prior knowledge of the state of the plasma, to increase accuracy of inferred physics variables. A new probabilistic framework, MINERVA, based on bayesian graphical models, has been used at JET and W7-AS to yield predictions of internal magnetic structure. A feature of the framework is the bayesian inversion for poloidal magnetic flux without the need for an explicit equilibrium assumption. Building on this, we discuss results from a new project to develop bayesian inversion tools that aim to (1) distinguish between competing equilibrium theories, which capture different physics, using the MAST spherical tokamak, and (2) test the predictions of MHD theory, particularly mode structure, using the H-1 Heliac. Specifically, we report on correction of the motional Stark effect, pickup coils, flux-loop constrained bayesian inferred equilibrium for varying toroidal flux. | |
| dc.description.sponsorship | This work was jointly funded by the Australian Government through International Science Linkages Grant No. CG130047, the Australian National University, the United Kingdom Engineering and Physical Sciences Research Council, and by the European Communities under the contract of Association between EURATOM and CCFE. | en_AU |
| dc.identifier.issn | 0034-6748 | en_AU |
| dc.identifier.uri | http://hdl.handle.net/1885/38441 | |
| dc.publisher | American Institute of Physics (AIP) | |
| dc.rights | http://www.sherpa.ac.uk/romeo/issn/0034-6748..."Publishers version/PDF may be used on author's personal website, institutional website or institutional repository" from SHERPA/RoMEO site (as at 9/12/15). Copyright 2010 American Institute of Physics. This article may be downloaded for personal use only. Any other use requires prior permission of the author and the American Institute of Physics. The following article appeared in Review of Scientific Instruments and may be found at https://doi.org/10.1063/1.3491044 | |
| dc.source | Review of Scientific Instruments | |
| dc.subject | Keywords: Bayesian; Bayesian graphical models; Bayesian inversion; Bayesian probability theory; Equilibrium theory; Forward models; Mode structure; Motional stark effects; New projects; Pick-up coils; Plasma equilibria; Prior knowledge; Probabilistic framework; Sph | |
| dc.title | The use of Bayesian inversion to resolve plasma equilibrium | |
| dc.type | Journal article | |
| local.bibliographicCitation.issue | 10 | en_AU |
| local.bibliographicCitation.startpage | 10E127 | en_AU |
| local.contributor.affiliation | Hole, Matthew, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National University | en_AU |
| local.contributor.affiliation | Von Nessi, Gregory, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National University | en_AU |
| local.contributor.affiliation | Pretty, David, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National University | en_AU |
| local.contributor.affiliation | Howard, John, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National University | en_AU |
| local.contributor.affiliation | Blackwell, Boyd, College of Physical and Mathematical Sciences, CPMS Research School of Physics and Engineering, Plasma Research Laboratory, The Australian National University | en_AU |
| local.contributor.affiliation | Svensson, Jakob, Max Planck Institute for Plasma Physics, Germany | en_AU |
| local.contributor.affiliation | Appel, Lynton C, UKAEA Fusion, United Kingdom | en_AU |
| local.contributor.authoruid | u4219046 | en_AU |
| local.description.notes | Imported from ARIES | en_AU |
| local.identifier.absfor | 020204 | en_AU |
| local.identifier.absseo | 850599 | en_AU |
| local.identifier.ariespublication | u4735977xPUB51 | en_AU |
| local.identifier.citationvolume | 81 | en_AU |
| local.identifier.doi | 10.1063/1.3491044 | en_AU |
| local.identifier.essn | 1089-7623 | en_AU |
| local.identifier.scopusID | 2-s2.0-78149456443 | |
| local.identifier.thomsonID | 000283754000186 | |
| local.publisher.url | https://www.aip.org/ | en_AU |
| local.type.status | Published Version | en_AU |
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