2010
DOI: 10.1088/1742-6596/244/2/022009
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Progress on LMJ targets for ignition

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Cited by 17 publications
(17 citation statements)
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“…The electron temperature is around 0.8 keV close to the value deduced from the experimental SBS spectrum. The simulated SBS spectrum calculated with the linear gain postprocessor Piranah, along the rays of the ray-tracing simulations 25 is illustrated in Figure 4(c). As we can see, we observe an initial redshift (around (7 6 1) Å ) as in the experimental spectrum, but in the linear analysis, we do not see the blue shift component of À4 Å observed in the experiment.…”
Section: B Numerical Simulationsmentioning
confidence: 99%
“…The electron temperature is around 0.8 keV close to the value deduced from the experimental SBS spectrum. The simulated SBS spectrum calculated with the linear gain postprocessor Piranah, along the rays of the ray-tracing simulations 25 is illustrated in Figure 4(c). As we can see, we observe an initial redshift (around (7 6 1) Å ) as in the experimental spectrum, but in the linear analysis, we do not see the blue shift component of À4 Å observed in the experiment.…”
Section: B Numerical Simulationsmentioning
confidence: 99%
“…Moreover, silicon has also been used as a dopant to the ablator material for target designs in inertial confinement fusion (ICF) [5][6][7], as well as for mitigating laser-imprint [8,9] and two-plasmon-decay effects [10] in direct-drive ICF.…”
Section: Introductionmentioning
confidence: 99%
“…At OMEGA scale backscattering losses are not very different in cylinders and rugby hohlraum. At MJ scale LPI in rugby hohlraum is an open question but various mitigation options are available including hohlraum wall shape [2,4]. The energetics benefit of rugby-shaped hohlraum could be useful either to increase the x-ray drive (and so favor higher capsule implosion velocity) for the same laser power, to achieve the same drive at reduced laser power or for high-gain target designs [13].…”
Section: Discussionmentioning
confidence: 99%
“…Point designs for ignition requires radiation temperature at 300 eV level [4,10]. A way to achieve such high radiation temperatures on OMEGA is to work with reduced scale empty hohlraums.…”
Section: Demonstration Of Ignition Radiation Temperatures In Reduced mentioning
confidence: 99%
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