Diagnosing and controlling mix in National Ignition Facility implosion experiments
Creators
- 1. Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
- 2. University of Rochester, Laboratory for Laser Energetics, Rochester, New York 14623 (United States)
- 3. Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States)
- 4. Sandia National Laboratories, Albuquerque, New Mexico 87185 (United States)
Description
High mode number instability growth of ''isolated defects'' on the surfaces of National Ignition Facility [Moses et al., Phys. Plasmas 16, 041006 (2009)] capsules can be large enough for the perturbation to penetrate the imploding shell, and produce a jet of ablator material that enters the hot-spot. Since internal regions of the CH ablator are doped with Ge, mixing of this material into the hot-spot results in a clear signature of Ge K-shell emission. Evidence of jets entering the hot-spot has been recorded in x-ray images and spectra, consistent with simulation predictions [Hammel et al., High Energy Density Phys. 6, 171 (2010)]. Ignition targets have been designed to minimize instability growth, and capsule fabrication improvements are underway to reduce ''isolated defects.'' An experimental strategy has been developed where the final requirements for ignition targets can be adjusted through direct measurements of mix and experimental tuning.
Additional details
Identifiers
- DOI
- 10.1063/1.3567520;
Publishing Information
- Journal Title
- Physics of Plasmas
- Journal Volume
- 18
- Journal Issue
- 5
- Journal Page Range
- p. 056310-056310.13
- ISSN
- 1070-664X
- CODEN
- PHPAEN
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 43016905
- Subject category
- S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
- Descriptors DEI
- CONTROL; IMPLOSIONS; PLASMA INSTABILITY; PLASMA SIMULATION; US NATIONAL IGNITION FACILITY; X-RAY SPECTRA
- Descriptors DEC
- INSTABILITY; SIMULATION; SPECTRA
Optional Information
- Notes
- (c) 2011 American Institute of Physics