Temperature evolution during magnetic reconnection has been spectroscopically measured for various ion species in a toroidal magnetized plasma. Measurements are made predominantly in the direction parallel to the equilibrium magnetic field. It is found that the increase in parallel ion temperature during magnetic reconnection events increases with the charge-to-mass ratio of the ion species. This trend can be understood if the heating mechanism is anisotropic, favoring heating in the perpendicular degree of freedom, with collisional relaxation of multiple ion species. The charge-to-mass ratio trend for the parallel temperature derives from collisional isotropization. This result emphasizes that collisional isotropization and energy transfer must be carefully modeled when analyzing ion heating measurements and comparing to theoretical predictions.
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May 2013
Research Article|
May 14 2013
Charge-to-mass-ratio-dependent ion heating during magnetic reconnection in the MST RFPa)
S. T. A. Kumar;
S. T. A. Kumar
b)
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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A. F. Almagri;
A. F. Almagri
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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D. Craig;
D. Craig
3
Wheaton College
, Wheaton, Illinois 60187, USA
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D. J. Den Hartog;
D. J. Den Hartog
c)
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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M. D. Nornberg;
M. D. Nornberg
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center 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
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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P. W. Terry
P. W. Terry
1Department of Physics,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
2Center for Magnetic Self-Organization in Laboratory and Astrophysical Plasmas,
University of Wisconsin-Madison
, Madison, Wisconsin 53706, USA
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b)
Electronic mail: stkumar@wisc.edu
c)
Invited speaker.
a)
Paper BI2 2, Bull. Am. Phys. Soc. 57, 22 (2012).
Phys. Plasmas 20, 056501 (2013)
Article history
Received:
December 21 2012
Accepted:
March 26 2013
Citation
S. T. A. Kumar, A. F. Almagri, D. Craig, D. J. Den Hartog, M. D. Nornberg, J. S. Sarff, P. W. Terry; Charge-to-mass-ratio-dependent ion heating during magnetic reconnection in the MST RFP. Phys. Plasmas 1 May 2013; 20 (5): 056501. https://doi.org/10.1063/1.4804958
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