Overview of results from the MST reversed field pinch experiment (Articolo in rivista)

Type
Label
  • Overview of results from the MST reversed field pinch experiment (Articolo in rivista) (literal)
Anno
  • 2013-01-01T00:00:00+01:00 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#doi
  • 10.1088/0029-5515/53/10/104017 (literal)
Alternative label
  • J.S. Sarff; A.F. Almagri; J.K. Anderson; M. Borchardt; D. Carmody; K. Caspary; B.E. Chapman; D.J. Den Hartog; J. Duff; S. Eilerman; A. Falkowski; C.B. Forest; J.A. Goetz; D.J. Holly; J.-H. Kim; J. King; J. Ko; J. Koliner; S. Kumar; J.D. Lee; D. Liu; R. Magee; K.J. McCollam; M. McGarry; V.V. Mirnov; M.D. Nornberg; P.D. Nonn; S.P. Oliva; E. Parke; J.A. Reusch; J.P. Sauppe; A. Seltzman; C.R. Sovinec; H. Stephens; D. Stone; D. Theucks; M. Thomas; J. Triana; P.W. Terry; J. Waksman; W.F. Bergerson; D.L. Brower; W.X. Ding; L. Lin; D.R. Demers; P. Fimognari; J. Titus; F. Auriemma; S. Cappello; P. Franz; P. Innocente; R. Lorenzini; E. Martines; B. Momo; P. Piovesan; M. Puiatti; M. Spolaore; D. Terranova; P. Zanca; V. Belykh; V.I. Davydenko; P. Deichuli; A.A. Ivanov; S. Polosatkin; N.V. Stupishin; D. Spong; D. Craig; R.W. Harvey; M. Cianciosa; J.D. Hanson (2013)
    Overview of results from the MST reversed field pinch experiment
    in Nuclear fusion; International Atomic Energy Agency, Vienna (Austria); IOP PUBLISHING LTD, BRISTOL BS1 6BE (Regno Unito)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • J.S. Sarff; A.F. Almagri; J.K. Anderson; M. Borchardt; D. Carmody; K. Caspary; B.E. Chapman; D.J. Den Hartog; J. Duff; S. Eilerman; A. Falkowski; C.B. Forest; J.A. Goetz; D.J. Holly; J.-H. Kim; J. King; J. Ko; J. Koliner; S. Kumar; J.D. Lee; D. Liu; R. Magee; K.J. McCollam; M. McGarry; V.V. Mirnov; M.D. Nornberg; P.D. Nonn; S.P. Oliva; E. Parke; J.A. Reusch; J.P. Sauppe; A. Seltzman; C.R. Sovinec; H. Stephens; D. Stone; D. Theucks; M. Thomas; J. Triana; P.W. Terry; J. Waksman; W.F. Bergerson; D.L. Brower; W.X. Ding; L. Lin; D.R. Demers; P. Fimognari; J. Titus; F. Auriemma; S. Cappello; P. Franz; P. Innocente; R. Lorenzini; E. Martines; B. Momo; P. Piovesan; M. Puiatti; M. Spolaore; D. Terranova; P. Zanca; V. Belykh; V.I. Davydenko; P. Deichuli; A.A. Ivanov; S. Polosatkin; N.V. Stupishin; D. Spong; D. Craig; R.W. Harvey; M. Cianciosa; J.D. Hanson (literal)
Pagina inizio
  • 104017 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#altreInformazioni
  • Article Number 104017; E-ISSN: 1741-4326. (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#url
  • http://iopscience.iop.org/0029-5515/53/10/104017/ (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 53 (literal)
Rivista
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  • 7 (literal)
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  • 10 (literal)
Note
  • ISI Web of Science (WOS) (literal)
  • Scopu (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1 University of Wisconsin, Madison, Wisconsin, USA and the Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas; / 2 Physics Department, The University of California at Los Angeles, Los Angeles, CA, USA; / 3 Xantho Technologies, LLC, Madison, WI, USA; / 4 Physics Department, Florida A&M University, Tallahassee, FL, USA; / 5 Consorzio RFX, Associazione EURATOM-ENEA sulla Fusione, Padova, Italy; / 6 Budker Institute of Nuclear Physics, Novosibirsk, Russia; / 7 The Oak Ridge National Laboratory, Oak Ridge, TN, USA; / 8 Physics Department, Wheaton College, Wheaton, IL, USA; / 9 CompX, Del Mar, CA, USA; / 10 Physics Department, Auburn University, Auburn, AL, USA. (J.S. Sarff1, A.F. Almagri1, J.K. Anderson1, M. Borchardt1, D. Carmody1, K. Caspary1, B.E. Chapman1, D.J. Den Hartog1, J. Duff1, S. Eilerman1, A. Falkowski1, C.B. Forest1, J.A. Goetz1, D.J. Holly1, J.-H. Kim1, J. King1, J. Ko1, J. Koliner1, S. Kumar1, J.D. Lee1, D. Liu1, R. Magee1, K.J. McCollam1, M. McGarry1, V.V. Mirnov1, M.D. Nornberg1, P.D. Nonn1, S.P. Oliva1, E. Parke1, J.A. Reusch1, J.P. Sauppe1, A. Seltzman1, C.R. Sovinec1, H. Stephens1, D. Stone1, D. Theucks1, M. Thomas1, J. Triana1, P.W. Terry1, J. Waksman1, W.F. Bergerson2, D.L. Brower2, W.X. Ding2, L. Lin2, D.R. Demers3, P. Fimognari3, J. Titus4, F. Auriemma5, S. Cappello5, P. Franz5, P. Innocente5, R. Lorenzini5, E. Martines5, B. Momo5, P. Piovesan5, M. Puiatti5, M. Spolaore5, D. Terranova5, P. Zanca5, V. Belykh6, V.I. Davydenko6, P. Deichuli6, A.A. Ivanov6, S. Polosatkin6, N.V. Stupishin6, D. Spong7, D. Craig8, R.W. Harvey9, M. Cianciosa10 and J.D. Hanson10) (literal)
Titolo
  • Overview of results from the MST reversed field pinch experiment (literal)
Abstract
  • An overview of recent results from the MST programme on physics important for the advancement of the reversed field pinch (RFP) as well as for improved understanding of toroidal magnetic confinement more generally is reported. Evidence for the classical confinement of ions in the RFP is provided by analysis of impurity ions and energetic ions created by 1 MW neutral beam injection (NBI). The first appearance of energetic-particle-driven modes by NBI in a RFP plasma is described. MST plasmas robustly access the quasi-single-helicity state that has commonalities to the stellarator and 'snake' formation in tokamaks. In MST the dominant mode grows to 8% of the axisymmetric field strength, while the remaining modes are reduced. Predictive capability for tearing mode behaviour has been improved through nonlinear, 3D, resistive magnetohydrodynamic computation using the measured resistivity profile and Lundquist number, which reproduces the sawtooth cycle dynamics. Experimental evidence and computational analysis indicates two-fluid effects, e.g., Hall physics and gyro-viscosity, are needed to understand the coupling of parallel momentum transport and current profile relaxation. Large Reynolds and Maxwell stresses, plus separately measured kinetic stress, indicate an intricate momentum balance and a possible origin for MST's intrinsic plasma rotation. Gyrokinetic analysis indicates that micro-tearing modes can be unstable at high beta, with a critical gradient for the electron temperature that is larger than for tokamak plasmas by roughly the aspect ratio. (literal)
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