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1.T. R. Boehly et al., Fusion Eng. Des. 44, 35 (1999);
1.R. Spielman et al., Plasma Phys. Controlled Fusion 42, B157 (2000);
1.E. I. Moses, Fusion Sci. Technol. 43, 420 (2003).
2.K. M. Campbell, F. A. Weber, E. L. Dewald et al., Rev. Sci. Instrum. 75, 3768 (2004).
3.R. R. Peterson et al., Phys. Plasmas 13, 056901 (2006).
4.R. E. Marshak, Phys. Fluids 1, 24 (1958).
5.J. H. Hammer and M. D. Rosen, Phys. Plasmas 10, 1829 (2003);
5.Y. B. Zel’dovich and Y. P. Razier, Physics of Shock Waves and High Temperature Hydrodynamic Phenomena (Academic, New York, 1966);
5.D. Mihalas and B. Weibel-Mihalas, Foundations of Radiation Hydrodynamics (Dover, Mineola, NY, 1999);
5.J. F. Hansen, et al., Phys. Plasmas 13, 022105 (2006);
5.R. P. Drake, High-Energy-Density Physics: Fundamentals, Inertial Fusion, and Experimental Astrophysics (Springer, Berlin, 2006).
6.R. B. Spielman et al., Proceedings of the 11th IEEE International Pulsed Power Conference, 1997 (unpublished), p.709.
7.T. W. L. Sanford et al., Phys. Plasmas 9, 3573 (2002).
8.D. Sinars et al., Rev. Sci. Instrum. 75, 3672 (2004);
8.G. R. Bennett et al., Rev. Sci. Instrum. 72, 657 (2001).
9.G. C. Idzorek, T. E. Tierney, and R. G. Watt, Proceedings of the Pulsed Power Plasma Science Conference, 2007 (unpublished), p. 49;
9.T. E. Lockard, G. C. Idzorek, T. E. Tierney, and R. G. Watt, Rev. Sci. Instrum. (to be published).
10.G. B. Zimmermann and W. L. Kruer, Comments Plasma Phys. Controlled Fusion 2, 51 (1975).
11.H. E. Tierney et al., Phys. Plasmas (to be published).
12.G. A. Rochau et al., Plasma Phys. Controlled Fusion 49, B591 (2007);
12.G. A. Rochau et al., Phys. Rev. Lett. 100, 125004 (2008).

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The distance radiation waves that supersonically propagate in optically thick, diffusive media are energy sensitive. A blast wave can form in a material when the initially diffusive, supersonic radiation wave becomes transonic. Under specific conditions, the blast wave is visible with radiography as a density perturbation. [Peterson et al. , Phys. Plasmas13, 056901 (2006)] showed that the time-integrated drive energy can be measured using blast wave positions with uncertainties less than 10% at the Z Facility. In some cases, direct measurements of energy loss through diagnostic holes are not possible with bolometric and x-ray radiometric diagnostics. Thus, radiography of high compression blast waves can serve as a complementary technique that provides time-integrated energy loss through apertures. In this paper, we use blast waves to characterize the energy emerging through a 2.4 mm aperture and show experimental results in comparison to simulations.


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