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 BP12: Poster Session I:
DIII-D and Conventional Tokamaks 1
HBT-EP and TCV
Space Plasmas
ICF1: Analytical and Computational Techniques; Machine learning and data science techniques in inertially confined plasmas; Z-pinch, X-pinch, exploding wire plasma, and dense plasma focus; Compression and burn; Magneto-inertial fusion
High Energy Density Physics
9:30 AM - 12:30 PM
Monday, October 7, 2024
Hyatt Regency
Room: Grand Hall West
Abstract: BP12.00124 : An overview of recent results from the PUFFIN group at MIT*
Presenter:
Jack D Hare
(MIT PSFC)
Authors:
Jack D Hare
(MIT PSFC)
Katherine Chandler
(Sandia National Laboratories)
Rishabh Datta
(MIT PSFC)
Samuel Engebretson
(MIT PSFC)
Emily R Neill
(MIT PSFC)
Thomas Varnish
(MIT PSFC)
Collaboration:
The MARZ (Magnetic Reconnection on Z) Collaboration
Oblique shock experiments on COBRA, which using an exploding wire array to drive magnetized plasma flows to interact with an angled, insulating wedge. The shock opening angles are measured using shadowgraphy, enabling the plasma adiabatic index to be measured.
Radiatively cooled reconnection experiments on Z, where we observe the formation and collapse of a reconnection layer using a suite of X-ray diagnostics which reveal the existence of bright hotpots within the layer which correspond to plasmoids in our 3D MHD simulations. We also observe the structure and evolution of the reconnection layer using laser shadowgraphy.
Guide field reconnection on MAIZE, using tilted wire arrays which embed an out-of-plane magnetic field in the reconnection layer. We observe a rotation of the outflows from the reconnection layer on global scales (>10 d_i) indicative of the interplay between the Hall field created by two-fluid effects and the guide field.
The status of the new PUFFIN facility at MIT, a new 1 MA peak current, 1.5 us rise time pulsed-power generator, which is designed to drive plasmas in a quasi-steady-state suitable for studying the growth of instabilities and the development of magnetised turbulence.
*This work is supported by the NSF through PHY2108050, PHY2339326, and PHY2213898. This work was supported in part by the NNSA Stewardship Science Academic Programs under DOE Cooperative Agreement DE-NA0004148. Experimental time on the Z facility was provided through the Z Fundamental Science Program.
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