Progress towards steady state on NSTX

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dc.contributor.authorGates, DAko
dc.contributor.authorKessel, Cko
dc.contributor.authorMenard, Jko
dc.contributor.authorTaylor, Gko
dc.contributor.authorWilson, JRko
dc.contributor.authorBell, MGko
dc.contributor.authorBell, REko
dc.contributor.authorBernabei, Sko
dc.contributor.authorBialek, Jko
dc.contributor.authorBiewer, Tko
dc.contributor.authorBlanchard, Wko
dc.contributor.authorBoedo, Jko
dc.contributor.authorBush, Cko
dc.contributor.authorCarter, MDko
dc.contributor.authorChoe, Wonhoko
dc.contributor.authorCrocker, Nko
dc.contributor.authorDarrow, DSko
dc.contributor.authorDavis, Wko
dc.contributor.authorDelgado-Aparicio, Lko
dc.contributor.authorDiem, Sko
dc.contributor.authorFerron, Jko
dc.contributor.authorField, Ako
dc.contributor.authorFoley, Jko
dc.contributor.authorFredrickson, EDko
dc.contributor.authorGibney, Tko
dc.contributor.authorHarvey, Rko
dc.contributor.authorHatcher, REko
dc.contributor.authorHeidbrink, Wko
dc.contributor.authorHill, Kko
dc.contributor.authorHosea, JCko
dc.contributor.authorJarboe, TRko
dc.contributor.authorJohnson, DWko
dc.contributor.authorKaita, Rko
dc.contributor.authorKaye, Sko
dc.contributor.authorKubota, Sko
dc.contributor.authorKugel, HWko
dc.contributor.authorLawson, Jko
dc.contributor.authorLeBlanc, BPko
dc.contributor.authorLee, KCko
dc.contributor.authorLevinton, Fko
dc.contributor.authorMaingi, Rko
dc.contributor.authorManickam, Jko
dc.contributor.authorMaqueda, Rko
dc.contributor.authorMarsala, Rko
dc.contributor.authorMastrovito, Dko
dc.contributor.authorMau, TKko
dc.contributor.authorMedley, SSko
dc.contributor.authorMeyer, Hko
dc.contributor.authorMikkelsen, DRko
dc.contributor.authorMueller, Dko
dc.contributor.authorMunsat, Tko
dc.contributor.authorNelson, BAko
dc.contributor.authorNeumeyer, Cko
dc.contributor.authorNishino, Nko
dc.contributor.authorOno, Mko
dc.contributor.authorPark, Hko
dc.contributor.authorPark, Wko
dc.contributor.authorPaul, Sko
dc.contributor.authorPeebles, Tko
dc.contributor.authorPeng, Mko
dc.contributor.authorPhillips, Cko
dc.contributor.authorPigarov, Ako
dc.contributor.authorPinsker, Rko
dc.contributor.authorRam, Ako
dc.contributor.authorRamakrishnan, Sko
dc.contributor.authorRaman, Rko
dc.contributor.authorRasmussen, Dko
dc.contributor.authorRedi, Mko
dc.contributor.authorRensink, Mko
dc.contributor.authorRewoldt, Gko
dc.contributor.authorRobinson, Jko
dc.contributor.authorRoney, Pko
dc.contributor.authorRoquemore, Lko
dc.contributor.authorRuskov, Eko
dc.contributor.authorRyan, Pko
dc.contributor.authorSabbagh, SAko
dc.contributor.authorSchneider, Hko
dc.contributor.authorSkinner, CHko
dc.contributor.authorSmith, DRko
dc.contributor.authorSontag, Ako
dc.contributor.authorSoukhanovskii, Vko
dc.contributor.authorStevenson, Tko
dc.contributor.authorStotler, Dko
dc.contributor.authorStratton, Bko
dc.contributor.authorStutman, Dko
dc.contributor.authorSwain, Dko
dc.contributor.authorSynakowski, Eko
dc.contributor.authorTakase, Yko
dc.contributor.authorTritz, Kko
dc.contributor.authorvon Halle, Ako
dc.contributor.authorWade, Mko
dc.contributor.authorWhite, Rko
dc.contributor.authorWilgen, Jko
dc.contributor.authorWilliams, Mko
dc.contributor.authorZhu, Wko
dc.contributor.authorZweben, SJko
dc.contributor.authorAkers, Rko
dc.contributor.authorBeiersdorfer, Pko
dc.contributor.authorBetti, Rko
dc.contributor.authorBigelow, Tko
dc.date.accessioned2013-03-07T21:56:49Z-
dc.date.available2013-03-07T21:56:49Z-
dc.date.created2012-02-06-
dc.date.created2012-02-06-
dc.date.issued2006-03-
dc.identifier.citationNUCLEAR FUSION, v.46, pp.S22 - S28-
dc.identifier.issn0029-5515-
dc.identifier.urihttp://hdl.handle.net/10203/91476-
dc.description.abstractIn order to reduce recirculating power fraction to acceptable levels, the spherical torus concept relies on the simultaneous achievement of high toroidal beta and high bootstrap fraction in steady state. In the last year, as a result of plasma control system improvements, the achievable plasma elongation on NSTX has been raised from kappa similar to 2.1 to kappa similar to 2.6-approximately a 25% increase. This increase in elongation has led to a substantial increase in the toroidal beta for long pulse discharges. The increase in beta associated with an increase in plasma current at nearly fixed poloidal beta, which enables higher beta(1), with nearly constant bootstrap fraction. As a result, for the first time in a spherical torus, a discharge with a plasma current of I MA has been sustained for 1 s (0.8 s current flat-top). Data are presented from NSTX correlating the increase in performance with increased plasma shaping capability. In addition to improved shaping, H-modes induced during the current ramp phase of the plasma discharge have been used to reduce flux consumption and to delay the onset of MHD instabilities. Based on these results, a modelled integrated scenario, which has 100% non-inductive current drive with very high toroidal, will also be discussed. The NSTX poloidal field coils are currently being modified to produce the plasma shape which is required for this scenario, which requires high triangularity (delta similar to 0.8) at elevated elongation (kappa similar to 2.5). The other main requirement of steady state on NSTX is the ability to drive a fraction of the total plasma current with RF waves. The results of high harmonic fast wave heating and current drive studies as well as electron Bernstein wave emission studies will be presented.-
dc.languageEnglish-
dc.publisherINT ATOMIC ENERGY AGENCY-
dc.subjectSPHERICAL-TORUS-EXPERIMENT-
dc.subjectELECTRON BERNSTEIN WAVES-
dc.subjectHARMONIC FAST-WAVE-
dc.subjectHIGH-BETA-
dc.subjectPLASMAS-
dc.subjectEXPLORATION-
dc.subjectTRANSPORT-
dc.subjectTOKAMAKS-
dc.subjectMODE-
dc.titleProgress towards steady state on NSTX-
dc.typeArticle-
dc.identifier.wosid000236682000005-
dc.identifier.scopusid2-s2.0-31444443397-
dc.type.rimsART-
dc.citation.volume46-
dc.citation.beginningpageS22-
dc.citation.endingpageS28-
dc.citation.publicationnameNUCLEAR FUSION-
dc.contributor.localauthorChoe, Wonho-
dc.contributor.nonIdAuthorGates, DA-
dc.contributor.nonIdAuthorKessel, C-
dc.contributor.nonIdAuthorMenard, J-
dc.contributor.nonIdAuthorTaylor, G-
dc.contributor.nonIdAuthorWilson, JR-
dc.contributor.nonIdAuthorBell, MG-
dc.contributor.nonIdAuthorBell, RE-
dc.contributor.nonIdAuthorBernabei, S-
dc.contributor.nonIdAuthorBialek, J-
dc.contributor.nonIdAuthorBiewer, T-
dc.contributor.nonIdAuthorBlanchard, W-
dc.contributor.nonIdAuthorBoedo, J-
dc.contributor.nonIdAuthorBush, C-
dc.contributor.nonIdAuthorCarter, MD-
dc.contributor.nonIdAuthorCrocker, N-
dc.contributor.nonIdAuthorDarrow, DS-
dc.contributor.nonIdAuthorDavis, W-
dc.contributor.nonIdAuthorDelgado-Aparicio, L-
dc.contributor.nonIdAuthorDiem, S-
dc.contributor.nonIdAuthorFerron, J-
dc.contributor.nonIdAuthorField, A-
dc.contributor.nonIdAuthorFoley, J-
dc.contributor.nonIdAuthorFredrickson, ED-
dc.contributor.nonIdAuthorGibney, T-
dc.contributor.nonIdAuthorHarvey, R-
dc.contributor.nonIdAuthorHatcher, RE-
dc.contributor.nonIdAuthorHeidbrink, W-
dc.contributor.nonIdAuthorHill, K-
dc.contributor.nonIdAuthorHosea, JC-
dc.contributor.nonIdAuthorJarboe, TR-
dc.contributor.nonIdAuthorJohnson, DW-
dc.contributor.nonIdAuthorKaita, R-
dc.contributor.nonIdAuthorKaye, S-
dc.contributor.nonIdAuthorKubota, S-
dc.contributor.nonIdAuthorKugel, HW-
dc.contributor.nonIdAuthorLawson, J-
dc.contributor.nonIdAuthorLeBlanc, BP-
dc.contributor.nonIdAuthorLee, KC-
dc.contributor.nonIdAuthorLevinton, F-
dc.contributor.nonIdAuthorMaingi, R-
dc.contributor.nonIdAuthorManickam, J-
dc.contributor.nonIdAuthorMaqueda, R-
dc.contributor.nonIdAuthorMarsala, R-
dc.contributor.nonIdAuthorMastrovito, D-
dc.contributor.nonIdAuthorMau, TK-
dc.contributor.nonIdAuthorMedley, SS-
dc.contributor.nonIdAuthorMeyer, H-
dc.contributor.nonIdAuthorMikkelsen, DR-
dc.contributor.nonIdAuthorMueller, D-
dc.contributor.nonIdAuthorMunsat, T-
dc.contributor.nonIdAuthorNelson, BA-
dc.contributor.nonIdAuthorNeumeyer, C-
dc.contributor.nonIdAuthorNishino, N-
dc.contributor.nonIdAuthorOno, M-
dc.contributor.nonIdAuthorPark, H-
dc.contributor.nonIdAuthorPark, W-
dc.contributor.nonIdAuthorPaul, S-
dc.contributor.nonIdAuthorPeebles, T-
dc.contributor.nonIdAuthorPeng, M-
dc.contributor.nonIdAuthorPhillips, C-
dc.contributor.nonIdAuthorPigarov, A-
dc.contributor.nonIdAuthorPinsker, R-
dc.contributor.nonIdAuthorRam, A-
dc.contributor.nonIdAuthorRamakrishnan, S-
dc.contributor.nonIdAuthorRaman, R-
dc.contributor.nonIdAuthorRasmussen, D-
dc.contributor.nonIdAuthorRedi, M-
dc.contributor.nonIdAuthorRensink, M-
dc.contributor.nonIdAuthorRewoldt, G-
dc.contributor.nonIdAuthorRobinson, J-
dc.contributor.nonIdAuthorRoney, P-
dc.contributor.nonIdAuthorRoquemore, L-
dc.contributor.nonIdAuthorRuskov, E-
dc.contributor.nonIdAuthorRyan, P-
dc.contributor.nonIdAuthorSabbagh, SA-
dc.contributor.nonIdAuthorSchneider, H-
dc.contributor.nonIdAuthorSkinner, CH-
dc.contributor.nonIdAuthorSmith, DR-
dc.contributor.nonIdAuthorSontag, A-
dc.contributor.nonIdAuthorSoukhanovskii, V-
dc.contributor.nonIdAuthorStevenson, T-
dc.contributor.nonIdAuthorStotler, D-
dc.contributor.nonIdAuthorStratton, B-
dc.contributor.nonIdAuthorStutman, D-
dc.contributor.nonIdAuthorSwain, D-
dc.contributor.nonIdAuthorSynakowski, E-
dc.contributor.nonIdAuthorTakase, Y-
dc.contributor.nonIdAuthorTritz, K-
dc.contributor.nonIdAuthorvon Halle, A-
dc.contributor.nonIdAuthorWade, M-
dc.contributor.nonIdAuthorWhite, R-
dc.contributor.nonIdAuthorWilgen, J-
dc.contributor.nonIdAuthorWilliams, M-
dc.contributor.nonIdAuthorZhu, W-
dc.contributor.nonIdAuthorZweben, SJ-
dc.contributor.nonIdAuthorAkers, R-
dc.contributor.nonIdAuthorBeiersdorfer, P-
dc.contributor.nonIdAuthorBetti, R-
dc.contributor.nonIdAuthorBigelow, T-
dc.type.journalArticleArticle; Proceedings Paper-
dc.subject.keywordPlusSPHERICAL-TORUS-EXPERIMENT-
dc.subject.keywordPlusELECTRON BERNSTEIN WAVES-
dc.subject.keywordPlusHARMONIC FAST-WAVE-
dc.subject.keywordPlusHIGH-BETA-
dc.subject.keywordPlusPLASMAS-
dc.subject.keywordPlusEXPLORATION-
dc.subject.keywordPlusTRANSPORT-
dc.subject.keywordPlusTOKAMAKS-
dc.subject.keywordPlusMODE-
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