Visualization of Shock Front Deformities in Fusion Ablator Materials Using Streaked Optical Pyrometry

POSTER

Abstract

Because of the abundance of fuel materials and promising energy yield, nuclear fusion may be the answer to the world's growing energy demands. Inertial Confinement Fusion (ICF) is one of the most promising options for nuclear fusion energy. As shock waves pass through ICF target capsule ablators, voids and other imperfections cause instabilities in the shock front leading to reduced energy gains. Studying shock-bubble (SB) interactions gives insights into how defects in ICF target capsules affect ICF reactions. In this study, we investigated how an ICF ablator-like material with voids between 20-40 μm reacted under laser driven shock. We detected an optical emission on our Velocity Interferometer System for Any Reflector (VISAR) streak camera and deduced that it was thermal emission resulting from the shock wave heating the ablator. We further found that the shock wave was accelerated through the void (by jetting as the void collapsed) leading to an inhomogeneous shock front. We hope that this will lead to a better understanding of hydrodynamic instabilities that reduce ICF energy gain.

*Acknowledgements: We acknowledge for funding from the Office of Science, Fusion Energy Sciences, under Award No. DE-SC 0024882: IFE-STAR issued as SLAC FWP 101126 through the IFE RISE Hub partnership. We also thank D. S. Montgomery, K. Kurzer-Ogul, A. F. T. Leong, P. M. Kozlowsk for support and useful conversations. Use of the Linac Coherent Light Source (LCLS), SLAC National Accelerator Laboratory, is supported by the U.S. Department of Energy, Office of Science, Office of Basic Energy Sciences under Contract No. DE-AC02-76SF00515. AEG, SP, RS, DH acknowledge funding support from DOE ECA-Gleason 2019. Part of this work was performed at the Stanford Nano Shared Facilities (SNSF), supported by the National Science Foundation under award ECCS-2026822. JKS,HA, and KKO acknowledge funding support from US NNSA under Grant Nos. DE-NA0003914 and DE-NA0004134. Partial support from grants NSF PHY-2020249, DE-SC0020229, and DE-SC0019329 is also acknowledged.

Presenters

  • Scott Curtis

    • Brigham Young University

Authors

  • Scott Curtis

    • Brigham Young University
  • Richard Lunt Sandberg

    • Brigham Young University
  • Arianna E Gleason

    • SLAC National Accelerator Laboratory
  • Silvia Pandolfi

    • Sorbonne Universite
  • Daniel Steven Hodge

    • Brigham Young University (BYU)