Estimation of stagnation performance metrics in magnetized liner inertial fusion experiments using Bayesian data assimilation

Author:

Knapp P. F.1ORCID,Glinsky M. E.1ORCID,Schaeuble M. A.1ORCID,Jennings C. A.1,Evans M.2,Gunning J.3,Awe T. J.1,Chandler G. A.1,Geissel M.1,Gomez M. R.1ORCID,Hahn K. D.4ORCID,Hansen S. B.1,Harding E. C.1,Harvey-Thompson A. J.1ORCID,Humane S.5ORCID,Klein B. T.1ORCID,Mangan M.1,Nagayama T.1,Porwitzky A. J.1ORCID,Ruiz D. E.1ORCID,Schmit P. F.1ORCID,Slutz S. A.1ORCID,Smith I. C.1,Weis M. R.1ORCID,Yager-Elorriaga D. A.1ORCID,Ampleford D. J.1ORCID,Beckwith K.1ORCID,Mattsson T. R.1,Peterson K. J.1ORCID,Sinars D. B.1ORCID

Affiliation:

1. Sandia National Laboratories, Albuquerque, New Mexico 87185, USA

2. University of Rochester Department of Physics and Astronomy, Rochester, New York 14627, USA

3. CSIRO Energy, Clayton, Victoria 3168, Australia

4. Lawrence Livermore National Laboratories, Livermore, California 94550, USA

5. Department of Nuclear Engineering and Radiological Sciences, University of Michigan, Ann Arbor, Michigan 48109, USA

Abstract

We present a new analysis methodology that allows for the self-consistent integration of multiple diagnostics including nuclear measurements, x-ray imaging, and x-ray power detectors to determine the primary stagnation parameters, such as temperature, pressure, stagnation volume, and mix fraction in magnetized liner inertial fusion (MagLIF) experiments. The analysis uses a simplified model of the stagnation plasma in conjunction with a Bayesian inference framework to determine the most probable configuration that describes the experimental observations while simultaneously revealing the principal uncertainties in the analysis. We validate the approach by using a range of tests including analytic and three-dimensional MHD models. An ensemble of MagLIF experiments is analyzed, and the generalized Lawson criterion χ is estimated for all experiments.

Funder

U.S. Department of Energy

Publisher

AIP Publishing

Subject

Condensed Matter Physics

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