Bulletin of the American Physical Society
65th Annual Meeting of the APS Division of Plasma Physics
Monday–Friday, October 30–November 3 2023; Denver, Colorado
Session UI10: Rosenbluth Awardee and Processes in Extreme Plasmas
2:00 PM–4:30 PM,
Thursday, November 2, 2023
Room: Governor's Square 17
Chair: Vikram Dharodi, Auburn University
Abstract: UI10.00003 : Finding the Best Uses of Imposed Magnetic Fields to Improve Indirect Drive Inertial Confinement Fusion*
3:00 PM–3:30 PM
Presenter:
David J Strozzi
(Lawrence Livermore Natl Lab)
Authors:
David J Strozzi
(Lawrence Livermore Natl Lab)
Blagoje Z Djordjevic
(Lawrence Livermore Natl Lab)
Chris A Walsh
(Lawrence Livermore National Laboratory)
Bruce A Hammel
(Lawrence Livermore Natl Lab)
John D Moody
(Lawrence Livermore National Laboratory)
Hong Sio
(Lawrence Livermore National Laboratory)
Bradley B Pollock
(Lawrence Livermore Natl Lab)
George B Zimmerman
(Lawrence Livermore National Laboratory)
Jeremy P Chittenden
(Imperial College London)
Besides traditional axial seed fields, we are also considering non-axial fields. Azimuthal fields with closed field lines have long been deemed ideal, since there is no direction for unmagnetized heat flow out of the hotspot. Modeling bears this out, unless electrons are so hot that they do not equilibrate with ions. We consider ways to impose azimuthal field other than running a current through the capsule, such as the “Omega coil” [Hohenberger et al., PoP 2012]. A mirror field, or a mostly axial one which increases at the capsule poles, is modeled to outperform an axial one, since the imploded field lines are less orthogonal to the shell boundary at the equator.
A separate potential benefit of magnetization is reduced hydro instability and mix [C. Walsh, PRE 2022]. We are exploring this in modeling and NIF shots with the dual crystal backlit imager (dual CBI) diagnostic scheduled for summer 2023.
*Work performed under auspices of US Dept. of Energy by LLNL under Contract DE-AC52-07NA27344 and LDRD project 23-ERD-025.
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