Laboratory Experiments in the Collisionless Kinetic Regime of Magnetic Reconnection
POSTER
Abstract
The Terrestrial Reconnection EXperiment (TREX)[1] at the Wisconsin Plasma Physics Laboratory (WiPPL)[2] can reliably reach the collisionless kinetic reconnection regime by driving a magnetic field via a cylindrical coil geometry. The most resent upgrade to the TREX configuration is the Drive Cylinder, which creates asymmetric reconnection that generates a ~2m long current layer with a normalized system size of L/di ≈ 13. Compared to the previous TREX systems, the lower inductance of the Drive Cylinder has increased the reconnection rate from Erec ≈ 100V/m to 900V/m. With these improved parameters, the Drive Cylinder produces reconnection events with Lundquist numbers up to S ≈ 105. These upgrades reduce the effects of collisionality in the experiment, such that electron pressure anisotropy is expected to develop unimpeded. By operating in this regime with a highly reproducible plasma, the Drive Cylinder aims to investigate plasma dynamics in the electron diffusion region similar to spacecraft data observed in the Earth's magnetosphere.
[1] Experimental Demonstration of the Collisionless Plasmoid Instability below the Ion Kinetic Scale during Magnetic Reconnection J.Olson et al, Phys. Rev. Lett., 116, 255001 (2016)
[2] The Wisconsin Plasma Astrophysics Laboratory C. B. Forest et al., J Plasma Physics, 81, Oct 2015.
[1] Experimental Demonstration of the Collisionless Plasmoid Instability below the Ion Kinetic Scale during Magnetic Reconnection J.Olson et al, Phys. Rev. Lett., 116, 255001 (2016)
[2] The Wisconsin Plasma Astrophysics Laboratory C. B. Forest et al., J Plasma Physics, 81, Oct 2015.
*This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Fusion Energy Sciences under Award Number DE-SC0018266.This material is based upon work supported by the U.S. Department of Energy, Office of Science, Office of Sciences, under Award Number DE-SC0020989.The material is based upon work supported by NASA under award No. 80NSSC22K0556.
Presenters
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Paul Gradney
- University of Wisconsin- Madison