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MHD equilibrium of a low-shear helical axis Heliotron

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dc.contributor.authorSuzuki, Y
dc.contributor.authorNakamura, Yuji
dc.contributor.authorKondo, Katsumi
dc.contributor.authorHayashi, Takaya
dc.contributor.authorLloyd, Sally
dc.contributor.authorGardner, Henry James
dc.date.accessioned2015-12-13T22:37:39Z
dc.date.available2015-12-13T22:37:39Z
dc.date.issued2003
dc.date.updated2015-12-11T09:37:35Z
dc.description.abstractThe HINT code is a three-dimensional MHD equilibrium calculation code which does not assume nested flux surfaces. This code has been applied to the study of helical system plasma and it has reproduced the phenomenon of magnetic islands in finite pressure
dc.identifier.issn0741-3335
dc.identifier.urihttp://hdl.handle.net/1885/77190
dc.publisherInstitute of Physics Publishing
dc.sourcePlasma Physics and Controlled Fusion
dc.subjectKeywords: Computer simulation; Magnetic field effects; Magnetic flux; Magnetohydrodynamics; Phase equilibria; Pressure effects; Shear flow; Shear helical axis Heliotron; Stellarator; Plasmas
dc.titleMHD equilibrium of a low-shear helical axis Heliotron
dc.typeJournal article
local.bibliographicCitation.issue6
local.bibliographicCitation.lastpage981
local.bibliographicCitation.startpage971
local.contributor.affiliationSuzuki, Y, National Institute for Fusion Science
local.contributor.affiliationNakamura, Yuji, Kyoto University
local.contributor.affiliationKondo, Katsumi, Kyoto University
local.contributor.affiliationHayashi, Takaya, National Institute for Fusion Science
local.contributor.affiliationLloyd, Sally, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationGardner, Henry James, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidLloyd, Sally, u3813553
local.contributor.authoruidGardner, Henry James, u8914398
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor010501 - Algebraic Structures in Mathematical Physics
local.identifier.ariespublicationMigratedxPub6083
local.identifier.citationvolume45
local.identifier.doi10.1088/0741-3335/45/6/310
local.identifier.scopusID2-s2.0-0038141198
local.type.statusPublished Version

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