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38
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-
33646649906
-
-
note
-
We acknowledge that others have used reshock and reverberating shock techniques (see, for example, Refs. 31-34,36). However, in this context, these studies represent the use of these techniques to attempt to discern the limiting shock compression in this high pressure regime.
-
-
-
-
41
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33646660262
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-
note
-
In previous publications (Refs. 8,9) we compared our experimental results with an earlier, incomplete revision of the Sesame 72 model, referred therein as the Sesame model (also known as the Sesame 98 or Kerley 98 model). The current revision, referred to as the Kerley 03 model, consists of several improvements over the earlier revision. At the request of the author of these models (G.I. Kerley), we have done away with the earlier revision of the Sesame 72 model in favor of the more recent revision.
-
-
-
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43
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33646646442
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unpublished
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M.D. Knudson, D.L. Hanson, J.E. Bailey, C.A. Hall, J.R. Asay, and C. Deeney (unpublished).
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Knudson, M.D.1
Hanson, D.L.2
Bailey, J.E.3
Hall, C.A.4
Asay, J.R.5
Deeney, C.6
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44
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0142057572
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M.D. Knudson, R.W. Lemke, D.B. Hayes, C.A. Hall, C. Deeney, and J.R. Asay, J. Appl. Phys. 94, 4420 (2003).
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Asay, J.R.6
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45
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0037393641
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R.W. Lemke, M.D. Knudson, C.A. Hall, T.A. Haill, P.M. Desjarlais, J.R. Asay, and T.A. Mehlhorn, Phys. Plasmas 10, 1092 (2003).
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Lemke, R.W.1
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Asay, J.R.6
Mehlhorn, T.A.7
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46
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0037620356
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R.W. Lemke, M.D. Knudson, A.C. Robinson, T.A. Haill, K.W. Struve, J.R. Asay, and T.A. Mehlhorn, Phys. Plasmas 10, 1867 (2003).
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Lemke, R.W.1
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Robinson, A.C.3
Haill, T.A.4
Struve, K.W.5
Asay, J.R.6
Mehlhorn, T.A.7
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47
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0242351874
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edited by M.D. Furnish, L.C. Chhabildas, and R.S. Hixson (AIP Press, New York)
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D.L. Hanson, J.R. Asay, C.A. Hall, M.D. Knudson, J.E. Bailey, K.J. Fleming, R.R. Johnston, B.F. Clark, M.A. Bernard, W.W. Anderson, G. Hassall, and S.D. Rothman, in Shock Compression of Condensed Matter-1999, edited by M.D. Furnish, L.C. Chhabildas, and R.S. Hixson (AIP Press, New York, 2000), p. 1175; D.L. Hanson, R.R. Johnston, M.D. Knudson, J.R. Asay, C.A. Hall, J.E. Bailey, and R.J. Hickman, in Shock Compression of Condensed Matter-2001, edited by M.D. Furnish, N.N. Thadani, and Y. Horie (AIP Press, New York, 2002), p. 1141.
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Shock Compression of Condensed Matter-1999
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Hanson, D.L.1
Asay, J.R.2
Hall, C.A.3
Knudson, M.D.4
Bailey, J.E.5
Fleming, K.J.6
Johnston, R.R.7
Clark, B.F.8
Bernard, M.A.9
Anderson, W.W.10
Hassall, G.11
Rothman, S.D.12
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48
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77955672630
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edited by M.D. Furnish, N.N. Thadani, and Y. Horie (AIP Press, New York)
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D.L. Hanson, J.R. Asay, C.A. Hall, M.D. Knudson, J.E. Bailey, K.J. Fleming, R.R. Johnston, B.F. Clark, M.A. Bernard, W.W. Anderson, G. Hassall, and S.D. Rothman, in Shock Compression of Condensed Matter-1999, edited by M.D. Furnish, L.C. Chhabildas, and R.S. Hixson (AIP Press, New York, 2000), p. 1175; D.L. Hanson, R.R. Johnston, M.D. Knudson, J.R. Asay, C.A. Hall, J.E. Bailey, and R.J. Hickman, in Shock Compression of Condensed Matter-2001, edited by M.D. Furnish, N.N. Thadani, and Y. Horie (AIP Press, New York, 2002), p. 1141.
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Johnston, R.R.2
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Hickman, R.J.7
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49
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Y.S. Touloukian, R.K. Kirby, R.E. Taylor, P.D. Desai, Thermal Expansion-Metallic Elements and Alloys, Vol. 12 of Thermophysical Properties of Matter (IFI/Plenum, New York, 1975), pp. 2, 77.
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IFI/Plenum, New York
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Y.S. Touloukian, R.K. Kirby, R.E. Taylor, and TY.R. Lee, Thermal Expansion-Nonmetallic Solids, Vol. 13 of Thermophysical Properties of Matter (IFI/Plenum, New York, 1977), pp. 176, 350.
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Lee, T.Y.R.4
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51
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33646637298
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note
-
For example, the linear correction (L2-L1)/L1 for Cu at 20 K is -0.324 (±0.010)% or -2.6 (±0.1) μm for an 800 μm thick reference spacer. The largest thermal expansion correction for any material was that for aluminum, -0.415 (±0.01)% at 20 K.
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52
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33646659102
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note
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The initial flyer thickness was nominally 800 μm. The ∼300 μm thickness refers to portion of the flyer at impact that remained unaffected by magnetic diffusion.
-
-
-
-
54
-
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33646648788
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-
note
-
2 interface, appear to exhibit dissimilar rise times. This is a result of the different time resolutions for each of the diagnostics. In this case (Z824S), the time resolutions of the diagnostics were ∼1-2, ∼1, and ∼0.5 ns for the VISAR, FOSBO, and self-emission, respectively.
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-
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56
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2042502376
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Greg Dunham, J.E. Bailey, A. Carlson, P. Lake, and M.D. Knudson, Rev. Sci. Instrum. 75, 928 (2004).
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Dunham, G.1
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59
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0022962937
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unpublished
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G.I. Kerley, Int. J. Impact Eng. 5, 441 (1987); G.I. Kerley (unpublished).
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Kerley, G.I.1
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61
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33646641864
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note
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The flyer plate experiences further quasi-isentropic compression and release, but since that process is reversible we only need consider the release from the shocked state. Also, the density, temperature, and particle velocity of the flyer at impact are not constants. Since the shock forms at the foot of the pulse and grows with distance, the density is lower and the temperature is higher towards the impact side of the flyer plate. However, given that we are only concerned with approximately 200-300 μm of the impact side of the flyer and the low rate of shock growth, the magnitude of the gradients are not significant, and can be ignored.
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62
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33646665413
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note
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1, on average,
-
-
-
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63
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33646664470
-
-
note
-
2 in addition to the reflected laser light. A portion of this self-emission signal was transmitted through the band-pass filter used in the FOSBO diagnostic, thus providing a measure of the self-emission in accordance with that obtained by the spectroscopy diagnostic.
-
-
-
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64
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33646669960
-
-
note
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2 (∼1-2 eV), and much greater than the shocked sapphire temperature (few tenths of an eV).
-
-
-
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66
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33646658272
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note
-
The first and second shock in the anvil (sapphire or a-quartz) were at pressure levels of ∼300-400 GPa and ∼600-800 GPa, respectively, corresponding the shock temperatures of ∼0.5-0.75 eV and ∼1-2 eV, respectively. The observed increase in emission corresponded to the resulting temperature increase as the second shock overtook the first shock.
-
-
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67
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33646649357
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note
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3.
-
-
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68
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0000992588
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B.L. Glushak, A.P. Zharkov, M.V. Zhernokletov, V.Ya. Ternovoi, A.S. Filimonov, and V.E. Fortov, Zh. Eksp. Teor. Fiz. 96, 1301 (1989) [Sov. Phys. JETP 69, 739 (1989)].
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Glushak, B.L.1
Zharkov, A.P.2
Zhernokletov, M.V.3
Ternovoi, V.Ya.4
Filimonov, A.S.5
Fortov, V.E.6
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69
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0001363083
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B.L. Glushak, A.P. Zharkov, M.V. Zhernokletov, V.Ya. Ternovoi, A.S. Filimonov, and V.E. Fortov, Zh. Eksp. Teor. Fiz. 96, 1301 (1989) [Sov. Phys. JETP 69, 739 (1989)].
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70
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33646642580
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note
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3).
-
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72
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B. Militzer, D.M. Ceperley, J.D. Kress, J.D. Johnson, L.A. Collins, and S. Mazevet, Phys. Rev. Lett. 87, 275502 (2001).
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73
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private communication
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M.P. Desjarlais (private communication).
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Desjarlais, M.P.1
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0006770881
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edited by S.C. Schmidt, J.W. Shaner, G.A. Samara, and M. Ross (AIP Press, New York)
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N.C. Holmes, in High-Pressure Science and Technology-1993, edited by S.C. Schmidt, J.W. Shaner, G.A. Samara, and M. Ross (AIP Press, New York, 1994), p. 153.
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Holmes, N.C.1
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77
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33646661352
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note
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The power varies as a function of wavelength; at 400 and 600 nm the power is approximately 1.9 and 1.5, respectively.
-
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83
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0042887438
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D.M. Hicks, P.M. Celliers, G.W. Collins, J.H. Eggert, and S.J. Moon, Phys. Rev. Lett. 91, 035502 (2003).
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84
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2142701318
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