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dc.contributor.authorCziegler, I.
dc.contributor.authorTynan, G. R.
dc.contributor.authorHubbard, Amanda E
dc.contributor.authorHughes Jr, Jerry
dc.contributor.authorTerry, James L
dc.date.accessioned2017-03-17T13:59:58Z
dc.date.available2017-03-17T13:59:58Z
dc.date.issued2017-03
dc.date.submitted2016-11
dc.identifier.issn0031-9007
dc.identifier.issn1079-7114
dc.identifier.urihttp://hdl.handle.net/1721.1/107458
dc.description.abstractA comprehensive study of fully frequency-resolved nonlinear kinetic energy transfer has been performed for the first time in a diverted tokamak, providing new insight into the parametric dependences of edge turbulence transitions. Measurements using gas puff imaging in the turbulent L-mode state illuminate the source of the long known but as yet unexplained “favorable-unfavorable” geometric asymmetry of the power threshold for transition to the turbulence-suppressed H mode. Results from the recently discovered I mode point to a competition between zonal flow (ZF) and geodesic-acoustic modes (GAM) for turbulent energy, while showing new evidence that the I-to-H transition is still dominated by ZFs. The availability of nonlinear drive for the GAM against net heat flux through the edge corresponds very well to empirical scalings found experimentally for accessing the I mode.en_US
dc.description.sponsorshipUnited States. Dept. of Energy. Office of Science (Awards DE-SC-0008689 and DE-FC02- 99ER54512)en_US
dc.publisherAmerican Physical Societyen_US
dc.relation.isversionofhttp://dx.doi.org/10.1103/PhysRevLett.118.105003en_US
dc.rightsArticle is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use.en_US
dc.sourceAmerican Physical Societyen_US
dc.titleTurbulence Nonlinearities Shed Light on Geometric Asymmetry in Tokamak Confinement Transitionsen_US
dc.typeArticleen_US
dc.identifier.citationCziegler, I. et al. “Turbulence Nonlinearities Shed Light on Geometric Asymmetry in Tokamak Confinement Transitions.” Physical Review Letters 118.10 (2017): n. pag. © 2017 American Physical Societyen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Centeren_US
dc.contributor.mitauthorHubbard, Amanda E
dc.contributor.mitauthorHughes Jr, Jerry
dc.contributor.mitauthorTerry, James L
dc.relation.journalPhysical Review Lettersen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dc.date.updated2017-03-09T23:00:03Z
dc.language.rfc3066en
dc.rights.holderAmerican Physical Society
dspace.orderedauthorsCziegler, I.; Hubbard, A. E.; Hughes, J. W.; Terry, J. L.; Tynan, G. R.en_US
dspace.embargo.termsNen_US
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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