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 YO6: Magneto-Inertial Fusion
9:30 AM–12:06 PM,
Friday, November 9, 2018
OCC
Room: B115-116
Chair: Kyle Peterson, Sandia National Laboratories
Abstract ID: BAPS.2018.DPP.YO6.6
Abstract: YO6.00006 : Long lived Taylor states in SSX for magneto-inertial fusion*
10:30 AM–10:42 AM
Presenter:
Michael R Brown
(Swarthmore College)
Authors:
Michael R Brown
(Swarthmore College)
Manjit Kaur
(Swarthmore College)
Katie Gelber
(Swarthmore College)
David A Schaffner
(Bryn Mawr College)
Our recent focus has been on increasing the magnetic lifetime of compressed Taylor state plasmas at SSX $[1]$ primarily by focussing attention on the electron temperature. We have installed a new tungsten coated copper flux conserver to reduce sputtering and provide a clean plasma facing surface. We estimate $T_e$ with a vacuum ultraviolet spectrometer measurement of the ratio of the $C_{III}~97.7~nm$ to $C_{IV}~155~nm$ line intensities $[2]$. A preliminary measurement has $T_e \sim 10~eV$. We bake and glow discharge clean the vacuum surface to remove adsorbed contaminants. Our current measured parameters include velocity ($40~km/s$), density ($0.5 \times 10^{16}~cm^{-3}$), proton temperature ($20~eV$), and magnetic field ($0.4~T$) of relaxed helical Taylor states in the new flux conserver.
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\noindent
$[1]$ T. Gray \textit{et. al.}, Phys. Rev. Lett. 110, 085002 (2013).
\newline
$[2]$ V. Chaplin \textit{et. al.}, Phys. Plasmas 16, 042505 (2009).
*Work supported by DOE ARPA-E ALPHA program.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.YO6.6
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