Physical model assessment of the energy confinement time scaling in stellarators

dc.contributor.authorDinklage, Andreas
dc.contributor.authorMaassberg, Henning
dc.contributor.authorPreuss, Roland
dc.contributor.authorYamada, Hiroshi
dc.contributor.authorAscasibar, E
dc.contributor.authorBeidler, C
dc.contributor.authorFunaba, Hisamichi
dc.contributor.authorHarris, Jeffrey
dc.contributor.authorKus, A
dc.contributor.authorMurakami, S
dc.contributor.authorSano, F
dc.contributor.authorStroth, U
dc.contributor.authorSuzuki, Y
dc.date.accessioned2015-12-10T22:55:22Z
dc.date.issued2007
dc.date.updated2015-12-10T07:49:35Z
dc.description.abstractThe International Stellarator Confinement Database (ISCDB) is a joint effort of the helical device community. It is publicly available at http://www.ipp.mpg.de/ISS and http://iscdb.nifs.ac.jp. The validity of physics models is investigated employing ISCDB data. Bayesian model comparison shows differences in the confinement scaling of data subgroups. Theory-based assessment of pure neoclassical transport regimes, however, indicates scalability which is supported by experimental results in specific W7-AS scenarios. Therefore, neoclassical simulations are employed for predictive purposes in W7-X, accounting for effects due to power deposition, plasma profiles and the ambipolar radial electric field. Neoclassical case studies for W7-X are presented as examples for the neoclassical predictions to be considered as an upper limit of plasma performance.
dc.identifier.issn0029-5515
dc.identifier.urihttp://hdl.handle.net/1885/60081
dc.publisherIOP Publishing
dc.sourceNuclear Fusion
dc.subjectKeywords: Ambipolar radial electric fields; Bayesian model; Energy confinement; Helical devices; Neoclassical transport; Physical model; Plasma performance; Plasma profiles; Power deposition; Time-scaling; Upper limits; Bayesian networks; Electric fields; Magnetohy
dc.titlePhysical model assessment of the energy confinement time scaling in stellarators
dc.typeJournal article
local.bibliographicCitation.lastpage1273
local.bibliographicCitation.startpage1265
local.contributor.affiliationDinklage, Andreas, Max Planck Institute for Plasma Physics
local.contributor.affiliationMaassberg, Henning, Max Planck Institute for Plasma Physics
local.contributor.affiliationPreuss, Roland, Max Planck Institute for Plasma Physics
local.contributor.affiliationYamada, Hiroshi, National Institute for Fusion Science
local.contributor.affiliationAscasibar, E, EURATOM
local.contributor.affiliationBeidler, C, Max Planck Institute for Plasma Physics
local.contributor.affiliationFunaba, Hisamichi, National Institute for Fusion Science
local.contributor.affiliationHarris, Jeffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationKus, A, Max Planck Institute for Plasma Physics
local.contributor.affiliationMurakami, S, Kyoto University
local.contributor.affiliationSano, F, Kyoto University
local.contributor.affiliationStroth, U, University of Stuttgart
local.contributor.affiliationSuzuki, Y, National Institute for Fusion Science
local.contributor.authoruidHarris, Jeffrey, u9702287
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020203 - Particle Physics
local.identifier.ariespublicationu4167262xPUB521
local.identifier.citationvolume47
local.identifier.doi10.1088/0029-5515/47/9/025
local.identifier.scopusID2-s2.0-42449101307
local.type.statusPublished Version

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