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dc.contributor.authorHolland, C.
dc.contributor.authorCandy, J.
dc.contributor.authorTheiler, C.
dc.contributor.authorWhite, Anne E.
dc.contributor.authorHoward, Nathaniel Thomas
dc.contributor.authorCreely, Alexander James
dc.contributor.authorChilenski, Mark Alan
dc.contributor.authorHubbard, Amanda E
dc.contributor.authorHughes Jr, Jerry
dc.contributor.authorSierchio, Jennifer M.
dc.contributor.authorSung, Choongki
dc.contributor.authorWalk Jr, John R
dc.contributor.authorWhyte, Dennis G
dc.contributor.authorMikkelsen, David
dc.contributor.authorEdlund, Eric Matthias
dc.contributor.authorKung, Chun C
dc.contributor.authorPetty, Clinton C.
dc.contributor.authorReinke, Matthew Logan
dc.contributor.authorTheiler, Christian
dc.contributor.authorGreenwald, Martin J.
dc.contributor.authorMarmar, Earl S.
dc.contributor.authorRice, John E.
dc.date.accessioned2017-05-09T17:58:42Z
dc.date.available2017-05-09T17:58:42Z
dc.date.issued2015-05
dc.date.submitted2014-12
dc.identifier.issn1070-664X
dc.identifier.issn1089-7674
dc.identifier.urihttp://hdl.handle.net/1721.1/108785
dc.description.abstractFor the first time, nonlinear gyrokinetic simulations of I-mode plasmas are performed and compared with experiment. I-mode is a high confinement regime, featuring energy confinement similar to H-mode, but without enhanced particle and impurity particle confinement [D. G. Whyte et al., Nucl. Fusion 50, 105005 (2010)]. As a consequence of the separation between heat and particle transport, I-mode exhibits several favorable characteristics compared to H-mode. The nonlinear gyrokinetic code GYRO [J. Candy and R. E. Waltz, J Comput. Phys. 186, 545 (2003)] is used to explore the effects of E × B shear and profile stiffness in I-mode and compare with L-mode. The nonlinear GYRO simulations show that I-mode core ion temperature and electron temperature profiles are more stiff than L-mode core plasmas. Scans of the input E × B shear in GYRO simulations show that E × B shearing of turbulence is a stronger effect in the core of I-mode than L-mode. The nonlinear simulations match the observed reductions in long wavelength density fluctuation levels across the L-I transition but underestimate the reduction of long wavelength electron temperature fluctuation levels. The comparisons between experiment and gyrokinetic simulations for I-mode suggest that increased E × B shearing of turbulence combined with increased profile stiffness are responsible for the reductions in core turbulence observed in the experiment, and that I-mode resembles H-mode plasmas more than L-mode plasmas with regards to marginal stability and temperature profile stiffness.en_US
dc.description.sponsorshipUnited States. Department of Energy (Contract No. DE-FC02-99ER54512-CMOD)en_US
dc.description.sponsorshipUnited States. Department of Energy. Office of Science (Contract No. DE-AC02- 05CH11231)en_US
dc.language.isoen_US
dc.publisherAmerican Institute of Physics (AIP)en_US
dc.relation.isversionofhttp://dx.doi.org/10.1063/1.4921150en_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.sourceProf. Whyte via Chris Sherratten_US
dc.titleNonlinear gyrokinetic simulations of the I-mode high confinement regime and comparisons with experimenta)en_US
dc.typeArticleen_US
dc.identifier.citationWhite, A. E., N. T. Howard, A. J. Creely, M. A. Chilenski, M. Greenwald, A. E. Hubbard, J. W. Hughes, et al. “Nonlinear Gyrokinetic Simulations of the I-Mode High Confinement Regime and Comparisons with Experimenta).” Physics of Plasmas 22, no. 5 (May 2015):en_US
dc.contributor.departmentLincoln Laboratoryen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Mathematicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Nuclear Science and Engineeringen_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMassachusetts Institute of Technology. Plasma Science and Fusion Centeren_US
dc.contributor.approverWhyte, Dennisen_US
dc.contributor.mitauthorWhite, Anne E.
dc.contributor.mitauthorHoward, Nathaniel Thomas
dc.contributor.mitauthorCreely, Alexander James
dc.contributor.mitauthorChilenski, Mark Alan
dc.contributor.mitauthorGreenwald, Martin J
dc.contributor.mitauthorHubbard, Amanda E
dc.contributor.mitauthorHughes Jr, Jerry
dc.contributor.mitauthorMarmar, Earl S
dc.contributor.mitauthorRice, John E
dc.contributor.mitauthorSierchio, Jennifer M.
dc.contributor.mitauthorSung, Choongki
dc.contributor.mitauthorWalk Jr, John R
dc.contributor.mitauthorWhyte, Dennis G
dc.contributor.mitauthorMikkelsen, David
dc.contributor.mitauthorEdlund, Eric Matthias
dc.contributor.mitauthorKung, Chun C
dc.contributor.mitauthorPetty, Clinton C.
dc.contributor.mitauthorReinke, Matthew Logan
dc.contributor.mitauthorTheiler, Christian
dc.relation.journalPhysics of Plasmasen_US
dc.eprint.versionFinal published versionen_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsWhite, A. E.; Howard, N. T.; Creely, A. J.; Chilenski, M. A.; Greenwald, M.; Hubbard, A. E.; Hughes, J. W.; Marmar, E.; Rice, J. E.; Sierchio, J. M.; Sung, C.; Walk, J. R.; Whyte, D. G.; Mikkelsen, D. R.; Edlund, E. M.; Kung, C.; Holland, C.; Candy, J.; Petty, C. C.; Reinke, M. L.; Theiler, C.en_US
dspace.embargo.termsNen_US
dc.identifier.orcidhttps://orcid.org/0000-0003-2951-9749
dc.identifier.orcidhttps://orcid.org/0000-0002-0026-6939
dc.identifier.orcidhttps://orcid.org/0000-0002-4464-150X
dc.identifier.orcidhttps://orcid.org/0000-0002-3616-8484
dc.identifier.orcidhttps://orcid.org/0000-0002-4438-729X
dc.identifier.orcidhttps://orcid.org/0000-0002-5283-0546
dc.identifier.orcidhttps://orcid.org/0000-0001-8319-5971
dc.identifier.orcidhttps://orcid.org/0000-0001-7700-848X
dc.identifier.orcidhttps://orcid.org/0000-0001-8324-4227
dc.identifier.orcidhttps://orcid.org/0000-0002-9001-5606
mit.licensePUBLISHER_POLICYen_US
mit.metadata.statusComplete


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