The Wisconsin Plasma Astrophysics Laboratory
arXiv:1506.07195 · doi:10.1017/S0022377815000975
Abstract
The Wisconsin Plasma Astrophysics Laboratory (WiPAL) is a flexible user facility designed to study a range of astrophysically relevant plasma processes as well as novel geometries that mimic astrophysical systems. A multi-cusp magnetic bucket constructed from strong samarium cobalt permanent magnets now confines a 10 m, fully ionized, magnetic-field free plasma in a spherical geometry. Plasma parameters of to eV and to cm provide an ideal testbed for a range of astrophysical experiments including self-exciting dynamos, collisionless magnetic reconnection, jet stability, stellar winds, and more. This article describes the capabilities of WiPAL along with several experiments, in both operating and planning stages, that illustrate the range of possibilities for future users.
21 pages, 12 figures, 2 tables
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Cited by in corpus (28)
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- Magnetic reconnection in the era of exascale computing and multiscale experiments
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- The structure of a perturbed magnetic reconnection electron diffusion region
- Amplitude limits and nonlinear damping of shear-Alfvén waves in high-beta low-collisionality plasmas
- Weakly magnetized, Hall dominated plasma Couette flow
- Magnetized Plasma Target for Plasma-Jet-Driven Magneto-Inertial Fusion
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- Formation of Transient High- Plasmas in a Magnetized, Weakly Collisional Regime
- Experimental observation of drift wave turbulence in an inhomogeneous six-pole cusp magnetic field of MPD
- Ion heating and flow driven by an Instability found in Plasma Couette Flow
- Plasma Flow Generation and Particle Acceleration from Expanding Magnetic Bubbles