Measurements of collective fuel velocities in deuterium-tritium exploding pusher and cryogenically layered deuterium-tritium implosions on the NIF

Journal Article · Mon Apr 15 00:00:00 EDT 2013 · Physics of Plasmas

DOI:https://doi.org/10.1063/1.4802810· OSTI ID:22130458

Gatu Johnson, M.; Casey, D. T.; Frenje, J. A.; Li, C. -K.; Seguin, F. H.; Petrasso, R. D. ^[1]; Ashabranner, R.; Bionta, R.; LePape, S.; McKernan, M.; Mackinnon, A. ^[2]; Kilkenny, J. D. ^[3]; Knauer, J.; Sangster, T. C. ^[4]

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1. Massachusetts Institute of Technology Plasma Science and Fusion Center, Cambridge, Massachusetts 02139 (United States)
2. Lawrence Livermore National Laboratory, Livermore, California 94550 (United States)
3. General Atomics, San Diego, California 92186 (United States)
4. Laboratory for Laser Energetics, University of Rochester, Rochester, New York 14623 (United States)

For the first time, quantitative measurements of collective fuel velocities in Inertial Confinement Fusion implosions at the National Ignition Facility are reported. Velocities along the line-of-sight (LOS) of the Magnetic Recoil neutron Spectrometer (MRS), positioned close to the equator (73 Degree-Sign -324 Degree-Sign ), were inferred from the measured mean energy of the deuterium-tritium (DT)-primary neutron peak. Substantial mean energy shifts up to 113 {+-} 16 keV were observed in DT gas-filled exploding-pusher implosions, driven in a polar-direct drive configuration, which corresponds to bulk fuel velocities up to 210 {+-} 30 km/s. In contrast, only marginal bulk fuel velocities along the MRS LOS were observed in cryogenically layered DT implosions. Integrated analysis of data from a large number of cryogenically layered implosions has recently identified a deficit in achieved hot-spot energy of {approx}3 kJ for these implosions [C. Cerjan et al., Phys. Plasmas (2013)]. One hypothesis that could explain this missing energy is a collective, directional fuel velocity of {approx}190 km/s. As only marginal bulk fuel velocities are observed in the MRS data, this might indicate that turbulent or radial flows would be a likely explanation for the missing energy. However, a directional velocity close to perpendicular to the MRS LOS cannot be ruled out.

• OSTI ID: 22130458
• Journal Information: Physics of Plasmas, Vol. 20, Issue 4; Other Information: (c) 2013 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 1070-664X
• Country of Publication: United States
• Language: English

Related Subjects

70 PLASMA PHYSICS AND FUSION TECHNOLOGY
ANGULAR VELOCITY
DATA ANALYSIS
DEUTERIUM
EXPLOSIONS
HOT SPOTS
IMPLOSIONS
INERTIAL CONFINEMENT
KEV RANGE 10-100
NEUTRON SPECTROMETERS
NEUTRONS
PLASMA DIAGNOSTICS
THERMONUCLEAR FUELS
TRITIUM
TURBULENCE