Bulletin of the American Physical Society
66th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 7–11, 2024; Atlanta, Georgia
Session TP12: Poster Session VII:
Turbulence and transport in fusion plasmas
ITER
MFE Heating and Energetic Particles
Self-organized configuration FRC, RFP, Spheromak
9:30 AM - 12:30 PM
Thursday, October 10, 2024
Hyatt Regency
Room: Grand Hall West
Abstract: TP12.00137 : Status of Diagnostic Campaign for the ECLAIR Magneto-inertial Fusion Experiment at Helicity Space*
Presenter:
Seth Pree
(Helicity Space Corporation)
Authors:
Seth Pree
(Helicity Space Corporation)
Joseph Isaac Samaniego
(Helicity Space Corporation)
Allyson M Sellner
(Helicity Space Corporation)
Setthivoine You
(Helicity Space Corporation)
Yegeon Lim
(Caltech)
Paul Murray Bellan
(Caltech)
Natalija Marin
(University of Maryland, Baltimore County)
Carlos A Romero-Talamas
(University of Maryland, Baltimore County)
Xiyue Shen
(Swarthmore/Cornell)
Michael R Brown
(Swarthmore College)
In collaboration with groups at Caltech, UMBC, and Swarthmore, we are developing and installing a series of plasma diagnostics on ECLAIR to measure plasma temperature, density, velocity, and evolving magnetic fields. The initial diagnostic suite includes time resolved, multichord spectroscopy, 4-chord heterodyne interferometry, B-dot arrays, and Rogowski coils. These diagnostics are placed at key locations along ECLAIR to measure the plasma properties throughout the formation, merger, compression and exhaust sequence [2,3].
The objective is to quantitatively verify that our Helicity Drive concept, for the first time in a single integrated machine, 1) forms magnetized plectonemic jets as in past experiments (SSX, MOCHI), 2) undergoes magnetic reconnection-heating upon jet merging as in past experiments (SSX, UT, MAST), and 3) compresses with the peristaltic magnetic nozzle scheme shown previously at tabletop scale (Caltech).
We present the design and status of each diagnostic along with preliminary data. The goal is to strengthen the physics basis for extrapolating to higher temperature regimes.
**This work is supported in part by DOE INFUSE.
Follow Us |
Engage
Become an APS Member |
My APS
Renew Membership |
Information for |
About APSThe American Physical Society (APS) is a non-profit membership organization working to advance the knowledge of physics. |
© 2024 American Physical Society
| All rights reserved | Terms of Use
| Contact Us
Headquarters
1 Physics Ellipse, College Park, MD 20740-3844
(301) 209-3200
Editorial Office
100 Motor Pkwy, Suite 110, Hauppauge, NY 11788
(631) 591-4000
Office of Public Affairs
529 14th St NW, Suite 1050, Washington, D.C. 20045-2001
(202) 662-8700