Inference of mix in direct-drive implosions on OMEGA

被引:49
作者
Radha, PB
Delettrez, J
Epstein, R
Glebov, VY
Keck, R
McCrory, RL
McKenty, P
Meyerhofer, DD
Marshall, F
Regan, SP
Roberts, S
Sangster, TC
Seka, W
Skupsky, S
Smalyuk, V
Sorce, C
Stoeckl, C
Soures, J
Town, RPJ
Yaakobi, B
Frenje, J
Li, CK
Petrasso, R
Seguin, F
Fletcher, K
Padalino, S
Freeman, C
Izumi, N
Lerche, R
Phillips, TW
机构
[1] Univ Rochester, Laser Energet Lab, Dept Engn Mech, Rochester, NY 14623 USA
[2] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA
[3] MIT, Ctr Plasma Fus, Cambridge, MA 02139 USA
[4] SUNY Coll Geneseo, Geneseo, NY 14454 USA
[5] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
关键词
D O I
10.1063/1.1459452
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
Direct-drive implosions on the OMEGA laser [T. R. Boehly, D. L. Brown, R. S. Craxton , Opt. Commun. 133, 495 (1997)] have been diagnosed using a wide range of techniques based on neutrons, charged particles, and x rays. These implosions use full single-beam smoothing (distributed phase plates, 1-THz-bandwidth smoothing by spectral dispersion and polarization smoothing). The beam-to-beam power imbalance is less than or equal to5%. Fuel areal densities close to those in one-dimensional (1-D) simulations are inferred for implosions with calculated convergence ratios similar to15. The experimental neutron yields are similar to35% of 1-D yields. The complementary nature of the experimental observables is exploited to infer fuel shell mix in these implosions. Data suggest that this mix occurs at relatively small scales. Analysis of the experimental observables results in a picture of the core and mix region indicating that nearly 70% of the compressed fuel areal density is unmixed, and about 20% of the compressed shell areal density is in the mixed region. Comparisons of this model with inferred core conditions from argon-doped implosions are also presented. (C) 2002 American Institute of Physics.
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收藏
页码:2208 / 2213
页数:6
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