Analysis of time-resolved argon line spectra from OMEGA direct-drive implosions
- Department of Physics, University of Nevada, Reno, Nevada 89557 (United States)
- Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
- Laboratory for Laser Energetics, University of Rochester, New York 14623 (United States)
- Departamento de Fisica, Universidad de Las Palmas de Gran Canaria, 35017 Las Palmas de Gran Canaria (Spain)
We discuss the observation and data analysis of argon K-shell line spectra from argon-doped deuterium-filled OMEGA direct-drive implosion cores based on data recorded with two streaked crystal spectrometers. The targets were 870 {mu}m in diameter, 27 {mu}m wall thickness plastic shells filled with 20 atm of deuterium gas, and a tracer amount of argon for diagnostic purposes. The argon K-shell line spectrum is primarily emitted at the collapse of the implosion and its analysis provides a spectroscopic diagnostic of the core implosion conditions. The observed spectra includes the He{alpha}, Ly{alpha}, He{beta}, He{gamma}, Ly{beta}, and Ly{gamma} line emissions and their associated He- and Li-like satellites thus covering a broad photon energy range from 3100 to 4200 eV with a spectral resolution power of approximately 500. The data analysis relies on detailed atomic and spectral models that take into account nonequilibrium collisional-radiative atomic kinetics, Stark-broadened line shapes, and radiation transport calculations.
- OSTI ID:
- 21266475
- Journal Information:
- Review of Scientific Instruments, Vol. 79, Issue 10; Other Information: DOI: 10.1063/1.2965779; (c) 2008 American Institute of Physics; Country of input: International Atomic Energy Agency (IAEA); ISSN 0034-6748
- Country of Publication:
- United States
- Language:
- English
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Related Subjects
70 PLASMA PHYSICS AND FUSION TECHNOLOGY
ARGON
DATA ANALYSIS
DEUTERIUM
DOPED MATERIALS
EMISSION
EV RANGE
IMPLOSIONS
INERTIAL CONFINEMENT
K SHELL
PHOTONS
PLASMA DIAGNOSTICS
PLASTICS
RADIANT HEAT TRANSFER
SPECTROMETERS
THICKNESS
TIME RESOLUTION
X-RAY SPECTRA