Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session CP11: Poster Session II: Basic Plasma Physics; Boundary, PMI, Proto-MPEX; International Tokamaks; Turbulence and Transport; Other Configurations; Z-pinch, Dense Plasma Focus and MagLIF (2:00pm-5:00pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.CP11.13
Abstract: CP11.00013 : Turbulent Fluctuations in a Flux-Rope Plasma at the Big Red Ball*
Presenter:
Emma M. Suen-Lewis
(University of Wisconsin Madison, Swarthmore College)
Authors:
Emma M. Suen-Lewis
(University of Wisconsin Madison, Swarthmore College)
Cary B. Forest
(University of Wisconsin Madison)
Michael R Brown
(Swarthmore College)
Douglass Endrizzi
(University of Wisconsin Madison)
Karsten J McCollam
(University of Wisconsin Madison)
David A Schaffner
(Bryn Mawr College)
Jason M Milhone
(University of Wisconsin Madison)
Ethan E Peterson
(University of Wisconsin Madison)
Mark D Nornberg
(University of Wisconsin Madison)
Observations of flux rope plasmas in the spherical BRB device at WiPPL are used to study turbulence and magnetic relaxation in plasma with beta between 0.25-1, flow speeds of approximately 20 km/s, and dB/B of approximately 12%. The flux ropes are generated via three plasma guns electrically biased relative to an anode on the opposite pole of the sphere, creating a current across the device. Magnetic fields can be applied externally in either a solenoid or mirror geometry. We use zero-time-lag correlations of co-located density and parallel magnetic field measurements in order to study the character of MHD wave fluctuations in the plasma. Excitations are also observed in the ion-cyclotron range, pointing to possible ion heating from turbulent dissipation. We intend to measure ion temperature at various beta values in order to test predictions for ion heating to scale with beta [1] and are able to vary beta between 0.1 and 10 for these purposes. These measurements were taken along with similar density-magnetic field correlations at SSX.
[1] Kunz, M. W., et al. “Astrophysical Gyrokinetics: Turbulence in Pressure-Anisotropic Plasmas at Ion Scales and Beyond.” Journal of Plasma Physics, vol. 84, no. 2, 2018, p. 715840201.
*This work is supported by the US DOE and the NSF.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.CP11.13
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