Bulletin of the American Physical Society
63rd Annual Meeting of the APS Division of Plasma Physics
Volume 66, Number 13
Monday–Friday, November 8–12, 2021; Pittsburgh, PA
Session UP11: Poster Session VIII:
Fundamental Plasma Physics - Analytical and Computational Techniques; Magnetic Reconnection; Antimatter Heliospheric, Magnetospheric, and Ionospheric Plasma Phenomena and Their Scaled Laboratory Experiments
MFE - DIII-D Tokamak II, ITER, HBT-EP, and Other Tokamaks
2:00 PM - 5:00 PM
Thursday, November 11, 2021
Room: Hall A
Abstract: UP11.00071 : Reconnection Drive Cylinder for the Terrestrial Reconnection Experiment*
Presenter:
Paul Gradney
Authors:
Paul Gradney
Jan Egedal
(University of Wisconsin - Madison)
Cary B Forest
(University of Wisconsin - Madison)
Samuel Greess
(University of Wisconsin - Madison)
Alexander Millet-Ayala
(University of Wisconsin - Madison)
Joseph R Olson
(University of Wisconsin - Madison)
Cameron Kuchta
(University of Wisconsin - Madison)
John P Wallace
(University of Wisconsin - Madison)
Mike Clark
(University of Wisconsin - Madison)
Collaborations:
TREX, WiPPL
The Terrestrial Reconnection EXperiment (TREX) at Wisconsin Plasma Physics Laboratory (WiPPL) [1] aims to explore the kinetic regime by driving an induced electric field through a cylindrical coil geometry. The enhanced drive will reduce the effective collisionality of the experiment, such that electron pressure anisotropy can develop unimpeded by Coulomb collisions providing a more accurate model of Earth’s magnetospheric plasma dynamics. The drive cylinder is composed of aluminum and Teflon, has a radius of 60cm, and is surrounded by 13 copper coils. Compared to TREX’s previous four drive coil configuration [2], we estimate that the drive cylinder reconnection current layer will be 70% longer, increase the absolute reconnection rate tenfold (up to Erec ? 1kV/m), and reduce the collision frequency by a factor of four. These effects will allow us to reliably access the regime of kinetic reconnection where electron pressure anisotropy is known to strongly impact the reconnection dynamics.
[1] C. B. Forest et al., “The Wisconsin Plasma Astrophysics Laboratory,” Journal of Plasma Physics, vol. 81, Oct 2015.
[2] J. Olson et al., “Experimental demonstration of the collisionless plasmoid instability below the ion kinetic scale during magnetic reconnection,” Phys. Rev. Lett., vol. 116, Jun 2016.
*DOE funds DE-SC0019153, DE-SC0013032, DE-SC0018266, and DE-SC0010463, NASA fund 80NSSC18K1231
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