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We limit the discussion to NIF relevant plasmas in which the acoustic waves involved in SBS are strongly damped; other materials produce higher SBS reflectivities
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We limit the discussion to NIF relevant plasmas in which the acoustic waves involved in SBS are strongly damped; other materials produce higher SBS reflectivities.
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R. K. Kirkwood, B. J. MacGowan, D. S. Montgomery, B. B. Afeyan, W. L. Kruer, J. D. Moody, K. G. Estabrook, C. A. Back, S. H. Glenzer, M. A. Blain, E. A. Williams, R. L. Berger, and B. F. Lasinski, Phys. Rev. Lett. 77, 2706 (1996); J. C. Fernandez, J. A. Cobble, B. H. Failor, D. F. DuBois, D. S. Montgomery, H. A. Rose, H. X. Vu, B. H. Wilde, M. D. Wilke, and R. E. Chrien, ibid. 77, 2706 (1996).
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11744257704
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If the wave is spatially localized, the linear Landau damping is properly done by Fourier transform where the wavenumber dependence of the damping can be accounted for. Such a spatial localization may have an important effect on the Langmuir wave damping as discussed recently by A. Simon and R. Short, Bull. Am. Phys. Soc. 42, 1882 (1997).
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34
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-
85034276177
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-
The arbitrariness of the choice of coefficients can be removed by analysis of simulations that include the microscopic wave-wave and wave-particle interactions
-
The arbitrariness of the choice of coefficients can be removed by analysis of simulations that include the microscopic wave-wave and wave-particle interactions.
-
-
-
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37
-
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6244275101
-
-
The appropriate distribution of intensities will depend on the particular physical problem, e.g., whether the depth of plasma is less or greater than a speckle length or whether the instability is absolutely unstable in a few localized hotspots. Specific models have been published: H. A. Rose and D. F. Dubois, Phys. Rev. Lett. 72, 2883 (1994); and V. T. Tikhonchuk, S. Hüller, and Ph. Mounaix, Phys. Plasmas 4, 4369 (1997).
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Rose, H.A.1
Dubois, D.F.2
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38
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0031380560
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The appropriate distribution of intensities will depend on the particular physical problem, e.g., whether the depth of plasma is less or greater than a speckle length or whether the instability is absolutely unstable in a few localized hotspots. Specific models have been published: H. A. Rose and D. F. Dubois, Phys. Rev. Lett. 72, 2883 (1994); and V. T. Tikhonchuk, S. Hüller, and Ph. Mounaix, Phys. Plasmas 4, 4369 (1997).
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Tikhonchuk, V.T.1
Hüller, S.2
Mounaix, Ph.3
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40
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85034283956
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First measurement of near forward scattering from a smoothed laser in a large ICF plasma
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J. D. Moody, B. J. MacGowan, B. B. Afeyan, S. H. Glenzer, D. E. Hinkel, R. K. Kirkwood, W. L. Kruer, D. S. Montgomery, A. J. Schmitt, E. A. Williams, and G. F. Stone, "First measurement of near forward scattering from a smoothed laser in a large ICF plasma," submitted to Phys. Rev. Lett.
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Phys. Rev. Lett.
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Moody, J.D.1
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Williams, E.A.10
Stone, G.F.11
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42
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11144324854
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Three-dimensional nonlinear hydrodynamics code to study laser-plasma interactions
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See AIP Document No. PAPS PHPAEN-5-007812 for 5 pages of article by C. H. Still, R. L. Berger, A. B. Langdon, and E. A. Williams, "Three-dimensional nonlinear hydrodynamics code to study laser-plasma interactions," ICF Quarterly Report 6, p. 138, July-September 1996 UCRL-LR-105821-96-4. Order by PAPS number in the journal reference from American Institute of Physics, Physics Auxiliary Publication Service, 500 Sunnyside Boulevard, Woodbury, New York 11797-2999. Fax: 516-576-2223, electronic mail: paps@aip.org. The price is $1.50 for each microfiche (98 pages) or $5.00 for photocopies of up to 30 pages, and $0.15 for each additional page over 30 pages. Airmail additional. Make checks payable to the American Institute of Physics.
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Still, C.H.1
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44
-
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85034274742
-
-
For multiple species plasmas, the light ions are primarily responsible for the damping and thus also for the emission. Thus the source will be proportional to the light ion temperature
-
For multiple species plasmas, the light ions are primarily responsible for the damping and thus also for the emission. Thus the source will be proportional to the light ion temperature.
-
-
-
-
46
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0021477513
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W. Seka, E. A. Williams, R. S. Craxton, L. M. Goldman, R. W. Short, and K. Tanaka, Phys. Fluids 27, 2181 (1984).
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47
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85034310055
-
-
Estimates are given on p. 1089 in Ref. 37
-
Estimates are given on p. 1089 in Ref. 37.
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51
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0000050776
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E. Epperlein, Phys. Rev. Lett. 65, 2145 (1990); Phys. Fluids B 1, 3082 (1991).
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53
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85034308728
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-
note
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0.
-
-
-
-
54
-
-
85034281444
-
-
note
-
Other shapes such as Gaussians, a finite sum of sinusoids such as given by Eq. (34) in Sec. III b but with constant phases, or the (diffraction-limited) field at the focus of a cylindrical lens. An advantage of 33 over a Gausian is that the lateral dimensions for a Gaussian must be quite large to avoid short wavelength noise arising from not adequately resolved transverse wavelengths. We did not experiment with other shapes but expect similar results with the proper normalizations.
-
-
-
-
55
-
-
85034296742
-
-
note
-
The strong damping limit is appropriate (in a homogeneous plasma at least) provided the absolute threshold is not exceeded. Near the focus, the absolute intensity is exceeded for SRS and a steady-state spatial gain rate will be restored only by pump depletion or gradient stabilization.
-
-
-
-
56
-
-
85034283587
-
-
Observed at the position of the incident light focussing lens, the near-field in our terminology, the reflected light will be broader in angle than the incident light
-
Observed at the position of the incident light focussing lens, the near-field in our terminology, the reflected light will be broader in angle than the incident light.
-
-
-
-
57
-
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0003713090
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Nonlinear wave-wave interaction
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edited by T. M. O'Neil and D. L. Book Benjamin, Amsterdam
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58
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85034283969
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private communication
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0000428919
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R. K. Kirkwood, C. A. Back, M. A. Blain, D. E. Desenne, A. G. Dulieu, S. H. Glenzer, B. J. MacGowan, D. S. Montgomery, and J. D. Moody, Rev. Sci. Instrum. 68, 636 (1997).
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MacGowan, B.J.7
Montgomery, D.S.8
Moody, J.D.9
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62
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85034284740
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The reflectivity might be much larger if the noise level exceeded the thermal level assumed in these simulations
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The reflectivity might be much larger if the noise level exceeded the thermal level assumed in these simulations.
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B. J. MacGowan, R. L. Berger, B. B. Afeyan, C. A. Back, M. A. Blain, B. Canaud, B. I. Cohen, D. E. Desenne, K. G. Estabrook, S. H. Glenzer, D. E. Hinkel, R. K. Kirkwood, W. L. Kruer, A. B. Langdon, B. F. Lasinski, D. S. Montgomery, J. D. Moody, C. Rouseaux, C. H. Still, and E. A. Williams, "Laser scattering in large-scale-length plasmas relevant to National Ignition Facility hohlraums," 1996 IAEA Conference, Montreal, Canada (International Atomic Energy Agency, Vienna, 1997).
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Cohen, B.I.7
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Estabrook, K.G.9
Glenzer, S.H.10
Hinkel, D.E.11
Kirkwood, R.K.12
Kruer, W.L.13
Langdon, A.B.14
Lasinski, B.F.15
Montgomery, D.S.16
Moody, J.D.17
Rouseaux, C.18
Still, C.H.19
Williams, E.A.20
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