2008
DOI: 10.1016/j.ijimpeng.2008.07.075
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Analysis of Z-pinch shock wave experiments on meteorite and planetary materials

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Cited by 8 publications
(14 citation statements)
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“…As an alternative to shock experiments, high-pressure Brillouin scattering, which provides a measurement of the bulk mod-ulus, in conjunction with X-ray diffraction measurements of volume, can be integrated to provide an EOS, but a correction must be made to transfer from an adiabatic to an isothermal path [3]. New approaches such as quasi-adiabatic Z-pinch based experiments [4,5] also hold future promise for a primary scale. There have been attempts to refine the ruby scale [6], and new calibrations have also been suggested [3].…”
mentioning
confidence: 99%
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“…As an alternative to shock experiments, high-pressure Brillouin scattering, which provides a measurement of the bulk mod-ulus, in conjunction with X-ray diffraction measurements of volume, can be integrated to provide an EOS, but a correction must be made to transfer from an adiabatic to an isothermal path [3]. New approaches such as quasi-adiabatic Z-pinch based experiments [4,5] also hold future promise for a primary scale. There have been attempts to refine the ruby scale [6], and new calibrations have also been suggested [3].…”
mentioning
confidence: 99%
“…where P 300K is the room-temperature contribution, fit to the Vinet form. The phonon contribution is written in an aug- mented Debye model, (5) in which the Debye temperature, θ, is a function of both V and T (Table I(b)). The Debye free energy per two-atom cell, excluding the zero-point term, is given by…”
mentioning
confidence: 99%
“…This is a continuation of earlier work [1,2] describing high energy density (HED) experiments measuring soft X-ray coupling to a variety of materials on the Sandia National Laboratories (SNL) Z-pinch facility, expanding the suite of materials and adding simulations. The overall motivation is to experimentally determine the impulses imparted by a known warm (~250 eV) Xray pulse onto representative solid astrophysical materials (iron meteorites, chondritic meteorites) and analogue materials (dunite, aluminum, iron and silicon), for purposes of NEO mitigation and understanding astrophysical impulses imparted by certain stellar events on nearby objects.…”
Section: Introductionmentioning
confidence: 75%
“…The experimental configuration in Figure 1 [2] uses samples ~1 mm thick, backed by transparent [100] LiF crystals that allow in-material optical access to VISAR diagnostics. Without such a window, experience has shown that VISAR velocimetry would not be successful for many of these samples.…”
Section: Experimental Methodsmentioning
confidence: 99%
“…Other common minerals are schriebersite ( (Fe,Ni) 3 P), troilite (iron sulfite) nodules mixed with graphite, graphite nodules, and cohenite (iron carbide). Acoustic P and S wave velocity profiles for Odessa indicate wave propagation speeds corresponding to different material phases 2 . The Fe-Ni meteorite Hugoniot response is dominated by a single crystal kamacite phase with bulk octahedral properties.…”
Section: Appendix 1 Detailed Petrographic Descriptions Of Samplesmentioning
confidence: 99%