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The Wisconsin Plasma Astrophysics Laboratory

  • C. B. Forest (a1), K. Flanagan (a1), M. Brookhart (a1), M. Clark (a1), C. M. Cooper (a1), V. Désangles (a2), J. Egedal (a1), D. Endrizzi (a1), I. V. Khalzov (a3), H. Li (a4), M. Miesch (a5), J. Milhone (a1), M. Nornberg (a1), J. Olson (a1), E. Peterson (a1), F. Roesler (a1), A. Schekochihin (a6) (a7), O. Schmitz (a1), R. Siller (a1), A. Spitkovsky (a8), A. Stemo (a1), J. Wallace (a1), D. Weisberg (a1) and E. Zweibel (a1)...

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 $10~\text{m}^{3}$ , fully ionized, magnetic-field-free plasma in a spherical geometry. Plasma parameters of $T_{e}\approx 5$ to $20~\text{eV}$ and $n_{e}\approx 10^{11}$ to $5\times 10^{12}~\text{cm}^{-3}$ 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.

Copyright

Corresponding author

Email address for correspondence: cbforest@wisc.edu

References

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The Wisconsin Plasma Astrophysics Laboratory

  • C. B. Forest (a1), K. Flanagan (a1), M. Brookhart (a1), M. Clark (a1), C. M. Cooper (a1), V. Désangles (a2), J. Egedal (a1), D. Endrizzi (a1), I. V. Khalzov (a3), H. Li (a4), M. Miesch (a5), J. Milhone (a1), M. Nornberg (a1), J. Olson (a1), E. Peterson (a1), F. Roesler (a1), A. Schekochihin (a6) (a7), O. Schmitz (a1), R. Siller (a1), A. Spitkovsky (a8), A. Stemo (a1), J. Wallace (a1), D. Weisberg (a1) and E. Zweibel (a1)...

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