Impurity ion dynamics measured with simultaneously high spatial and temporal resolution reveal classical ion transport in the reversed-field pinch. The boron, carbon, oxygen, and aluminum impurity ion density profiles are obtained in the Madison Symmetric Torus [R. N. Dexter et al., Fusion Technol. 19, 131 (1991)] using a fast, active charge-exchange-recombination-spectroscopy diagnostic. Measurements are made during improved-confinement plasmas obtained using inductive control of tearing instability to mitigate stochastic transport. At the onset of the transition to improved confinement, the impurity ion density profile becomes hollow, with a slow decay in the core region concurrent with an increase in the outer region, implying an outward convection of impurities. Impurity transport from Coulomb collisions in the reversed-field pinch is classical for all collisionality regimes, and analysis shows that the observed hollow profile and outward convection can be explained by the classical temperature screening mechanism. The profile agrees well with classical expectations. Experiments performed with impurity pellet injection provide further evidence for classical impurity ion confinement.
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May 2012
Research Article|
May 18 2012
Classical confinement and outward convection of impurity ions in the MST RFP
S. T. A. Kumar;
S. T. A. Kumar
b)
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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D. J. Den Hartog;
D. J. Den Hartog
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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V. V. Mirnov;
V. V. Mirnov
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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K. J. Caspary;
K. J. Caspary
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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R. M. Magee;
R. M. Magee
3
Department of Physics, West Virginia University
, Morgantown, WV 26506, USA
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D. L. Brower;
D. L. Brower
4
Department of Physics and Astronomy, University of California
, Los Angeles, California 90095, USA
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B. E. Chapman;
B. E. Chapman
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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D. Craig;
D. Craig
5
Physics Department, Wheaton College
, Wheaton, Illinois 60187, USA
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W. X. Ding;
W. X. Ding
4
Department of Physics and Astronomy, University of California
, Los Angeles, California 90095, USA
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S. Eilerman;
S. Eilerman
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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G. Fiksel;
G. Fiksel
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
6
Laboratory for Laser Energetics, University of Rochester
, Rochester, New York, USA
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L. Lin;
L. Lin
4
Department of Physics and Astronomy, University of California
, Los Angeles, California 90095, USA
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M. Nornberg;
M. Nornberg
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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E. Parke;
E. Parke
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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J. A. Reusch;
J. A. Reusch
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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J. S. Sarff
J. S. Sarff
1
Department of Physics, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2
Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas, University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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b)
Invited speaker. Electronic mail: stkumar@wisc.edu.
a)
Paper NI2 4, Bull. Am. Phys. Soc. 56, 183 (2011).
Phys. Plasmas 19, 056121 (2012)
Article history
Received:
December 05 2011
Accepted:
April 13 2012
Citation
S. T. A. Kumar, D. J. Den Hartog, V. V. Mirnov, K. J. Caspary, R. M. Magee, D. L. Brower, B. E. Chapman, D. Craig, W. X. Ding, S. Eilerman, G. Fiksel, L. Lin, M. Nornberg, E. Parke, J. A. Reusch, J. S. Sarff; Classical confinement and outward convection of impurity ions in the MST RFP. Phys. Plasmas 1 May 2012; 19 (5): 056121. https://doi.org/10.1063/1.4718310
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