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dc.contributor.author이정표-
dc.date.accessioned2018-04-20T01:05:39Z-
dc.date.available2018-04-20T01:05:39Z-
dc.date.issued2012-04-
dc.identifier.citationPhysics of Plasmas, Vol.19, No.5 [2012], p056113-1 ~ 056113-7en_US
dc.identifier.issn1070-664X-
dc.identifier.urihttp://aip.scitation.org/doi/10.1063/1.3694668-
dc.identifier.urihttps://repository.hanyang.ac.kr/handle/20.500.11754/70181-
dc.description.abstractNew results suggest that changes observed in the intrinsic toroidal rotation influence the internal transport barrier (ITB) formation in the Alcator C-Mod tokamak E. S. Marmar and Alcator C-Mod group, Fusion Sci. Technol. 51, 261 (2007). These arise when the resonance for ion cyclotron range of frequencies (ICRF) minority heating is positioned off-axis at or outside of the plasma half-radius. These ITBs form in a reactor relevant regime, without particle or momentum injection, with Ti ≈ Te, and with monotonic q profiles (qmin ≤ 1). C-Mod H-mode plasmas exhibit strong intrinsic co-current rotation that increases with increasing stored energy without external drive. When the resonance position is moved off-axis, the rotation decreases in the center of the plasma resulting in a radial toroidal rotation profile with a central well which deepens and moves farther off-axis when the ICRF resonance location reaches the plasma half-radius. This profile results in strong E × B shear (>1.5 × 105 rad/s) in the region where the ITB foot is observed. Gyrokinetic analyses indicate that this spontaneous shearing rate is comparable to the linear ion temperature gradient (ITG) growth rate at the ITB location and is sufficient to reduce the turbulent particle and energy transport. New and detailed measurement of the ion temperature demonstrates that the radial profile flattens as the ICRF resonance position moves off axis, decreasing the drive for the ITG the instability as well. These results are the first evidence that intrinsic rotation can affect confinement in ITB plasmas.en_US
dc.description.sponsorshipThe authors are indebted to John Wright, Ted Baker, and Paul Bonoli for providing use of the LOKI computer cluster for use in the simulations and also to Anne White and Martin Greenwald for useful discussions. Access to the GYRO code was provided by Jeff Candy and Ron Waltz of General Atomics. The authors would also like to acknowledge the assistance and support of the C-Mod experimental staff. This work was supported by US-DoE DE-FC02–99ER54512, DE-FG03–96ER5437, and DE-AC02–09CH11466.en_US
dc.language.isoenen_US
dc.publisherAMERICAN INSTITUTE OF PHYSICSen_US
dc.subjectLaboratory proceduresen_US
dc.subjectH modeen_US
dc.subjectInternal transport barrieren_US
dc.subjectAtmospheric physicsen_US
dc.subjectPlasma diagnosticsen_US
dc.subjectGeneral physicsen_US
dc.subjectPlasma gyrokineticsen_US
dc.subjectGeophysicsen_US
dc.subjectIonospheric physicsen_US
dc.subjectOptics and optical physicsen_US
dc.titleProduction of internal transport barriers via self-generated mean flows in Alcator C-Moden_US
dc.typeArticleen_US
dc.relation.no5-
dc.relation.volume19-
dc.identifier.doi10.1063/1.3694668-
dc.relation.page56113-56119-
dc.relation.journalPHYSICS OF PLASMAS-
dc.contributor.googleauthorFiore, C.L.-
dc.contributor.googleauthorErnst, D.R.-
dc.contributor.googleauthorPodpaly, Y.A.-
dc.contributor.googleauthorMikkelsen, D.-
dc.contributor.googleauthorHoward, N.T.-
dc.contributor.googleauthorLee, J.-
dc.contributor.googleauthorReinke, M.L.-
dc.contributor.googleauthorRice, J.E.-
dc.contributor.googleauthorHughes, J.W.-
dc.contributor.googleauthorMa, Y.-
dc.relation.code2012207624-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF ENGINEERING[S]-
dc.sector.departmentDEPARTMENT OF NUCLEAR ENGINEERING-
dc.identifier.pidjungpyo-
dc.identifier.researcherID36476380500-
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COLLEGE OF ENGINEERING[S](공과대학) > NUCLEAR ENGINEERING(원자력공학과) > Articles
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