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Diagnosing implosions at the national ignition facility with X-ray spectroscopy.

Authors :
Regan, S. P.
Epstein, R.
Hammel, B. A.
Suter, L. J.
Ralph, J.
Scott, H.
Barrios, M. A.
Bradley, D. K.
Callahan, D. A.
Collins, G. W.
Dixit, S. N.
Edwards, M. J.
Farley, D. R.
Glenzer, S. H.
Golovkin, I. E.
Haan, S. W.
Hamza, A.
Hicks, D. G.
Izumi, N.
Kilkenny, J. D.
Source :
AIP Conference Proceedings; 5/25/2012, Vol. 1438 Issue 1, p49-54, 6p, 1 Diagram, 4 Graphs
Publication Year :
2012

Abstract

X-ray spectroscopy is used at the National Ignition Facility (NIF) to diagnose plasma conditions in the hot spot and the compressed shell of ignition-scale inertial confinement fusion (ICF) implosions. Ignition of an ICF target depends on the formation of a central hot spot with sufficient temperature and areal density. The concentric spherical layers of current NIF ignition targets consist of a plastic ablator surrounding a thin shell of cryogenic thermonuclear fuel (i.e., hydrogen isotopes), with fuel vapor filling the interior volume. A fraction of the ablator has a Ge dopant to minimize preheat of the ablator closest to the DT ice caused by Au M-band emission from the hohlraum x-ray drive. This paper concentrates on three spectral features of the implosion: Ge Heα emission, Ge Kα emission, and the Ge K edge. Hydrodynamic instabilities seeded by highmode (50 < ℓ < 200) ablator-surface perturbations on ignition-scale targets can cause mixing of Ge-doped ablator into the interior of the shell at the end of the acceleration phase. As the shell decelerates, it compresses the fuel vapor, forming a hot spot. K-shell line emission from the ionized Ge that has penetrated into the hot spot provides an experimental signature of hot-spot mix. The amount of hot-spot mix mass is estimated from the brightness and spectral line shape of the Ge Heα and satellite emission using a detailed atomic physics code. X-ray continuum from the hot spot is attenuated by the compressed shell, and the photoexcitation causes the shell to fluoresce in Ge Kα emission. The contrast at the Ge K edge and the brightness of Ge Kα emission are used to diagnose the shell areal density. The highlighted spectral features are presented. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
0094243X
Volume :
1438
Issue :
1
Database :
Complementary Index
Journal :
AIP Conference Proceedings
Publication Type :
Conference
Accession number :
76143185
Full Text :
https://doi.org/10.1063/1.4707854