Confirmation of the topology of the Wendelstein 7-X magnetic field to better than 1:100,000

dc.contributor.authorHoury, M
dc.contributor.authorPedersen, Thomas Sunn
dc.contributor.authorOtte, Matthias
dc.contributor.authorLazerson, Samuel A.
dc.contributor.authorHelander, Per
dc.contributor.authorBozhenkov, Sergey A.
dc.contributor.authorBiedermann, Christoph
dc.contributor.authorKlinger, Thomas
dc.contributor.authorWolf, Robert
dc.contributor.authorBosch, Hans Stephan
dc.contributor.authorBlackwell, Boyd
dc.contributor.authorWright, Adelle
dc.date.accessioned2018-11-29T22:56:28Z
dc.date.available2018-11-29T22:56:28Z
dc.date.issued2016
dc.date.updated2018-11-29T08:12:34Z
dc.description.abstractFusion energy research has in the past 40 years focused primarily on the tokamak concept, but recent advances in plasma theory and computational power have led to renewed interest in stellarators. The largest and most sophisticated stellarator in the world, Wendelstein 7-X (W7-X), has just started operation, with the aim to show that the earlier weaknesses of this concept have been addressed successfully, and that the intrinsic advantages of the concept persist, also at plasma parameters approaching those of a future fusion power plant. Here we show the first physics results, obtained before plasma operation: that the carefully tailored topology of nested magnetic surfaces needed for good confinement is realized, and that the measured deviations are smaller than one part in 100,000. This is a significant step forward in stellarator research, since it shows that the complicated and delicate magnetic topology can be created and verified with the required accuracy
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2041-1723
dc.identifier.urihttp://hdl.handle.net/1885/153531
dc.publisherMacmillan Publishers Ltd
dc.sourceNature Communications
dc.titleConfirmation of the topology of the Wendelstein 7-X magnetic field to better than 1:100,000
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage13493
local.bibliographicCitation.startpage13493
local.contributor.affiliationHoury, M, CEA-Saclay
local.contributor.affiliationPedersen, Thomas Sunn, Max Planck Institut fur Plasmaphysik
local.contributor.affiliationOtte, Matthias, Max Planck Institute for Plasma Physics
local.contributor.affiliationLazerson, Samuel A., Princeton Plasma Physics Laboratory
local.contributor.affiliationHelander, Per, Max Planck Institut fur Plasmaphysik
local.contributor.affiliationBozhenkov, Sergey A., Max Planck Institut fur Plasmaphysik
local.contributor.affiliationBiedermann, Christoph, Max Planck Institut fur Plasmaphysik
local.contributor.affiliationKlinger, Thomas, Max Planck Institute of Physics
local.contributor.affiliationWolf, Robert, Max Planck Institut fuer Plasmaphysik
local.contributor.affiliationBosch, Hans Stephan, Max Planck Institut fur Plasmaphysik
local.contributor.affiliationBlackwell, Boyd, College of Science, ANU
local.contributor.affiliationWright, Adelle, College of Science, ANU
local.contributor.authoruidBlackwell, Boyd, u8508956
local.contributor.authoruidWright, Adelle, u5018015
local.description.notesImported from ARIES
local.identifier.absfor020204 - Plasma Physics; Fusion Plasmas; Electrical Discharges
local.identifier.ariespublicationa383154xPUB5109
local.identifier.citationvolume7
local.identifier.doi10.1038/ncomms13493
local.identifier.scopusID2-s2.0-84999106918
local.identifier.thomsonID000388809900001
local.type.statusPublished Version

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