Please use this identifier to cite or link to this item: http://hdl.handle.net/10553/35732
Title: Counter-propagating radiative shock experiments on the Orion laser and the formation of radiative precursors
Authors: Clayson, T.
Suzuki-Vidal, F.
Lebedev, S. V.
Swadling, G.F.
Stehlé, C.
Burdiak, G.
Foster, J.M.
Skidmore, J.
Graham, P.
Gumbrell, E.T.
Patankar, S.
Spindloe, C.
Chaulagain, U.
Kozlova, M.
Larour, J.
Singh, R. L.
Rodriguez, R. 
Gil, J. M. 
Espinosa Vivas, Guadalupe 
Velarde, P.
Danson, C.
UNESCO Clasification: 22 Física
Keywords: Radiative shock
Radiative precursor
Counter propagating shocks
Issue Date: 2017
Journal: High Energy Density Physics 
Abstract: We present results from new experiments to study the dynamics of radiative shocks, reverse shocks and radiative precursors. Laser ablation of a solid piston by the Orion high-power laser at AWE Aldermaston UK was used to drive radiative shocks into a gas cell initially pressurised between 0.1 and 1.0 bar with different noble gases. Shocks propagated at 80 +/- 10 km/s and experienced strong radiative cooling resulting in post-shock compressions of x25 +/- 2. A combination of X-ray backlighting, optical self-emission streak imaging and interferometry (multi-frame and streak imaging) were used to simultaneously study both the shock front and the radiative precursor. These experiments present a new configuration to produce counter-propagating radiative shocks, allowing for the study of reverse shocks and providing a unique platform for numerical validation. In addition, the radiative shocks were able to expand freely into a large gas volume without being confined by the walls of the gas cell. This allows for 3-D effects of the shocks to be studied which, in principle, could lead to a more direct comparison to astrophysical phenomena. By maintaining a constant mass density between different gas fills the shocks evolved with similar hydrodynamics but the radiative precursor was found to extend significantly further in higher atomic number gases (similar to 4 times further in xenon than neon). Finally, 1-D and 2-D radiative-hydrodynamic simulations are presented showing good agreement with the experimental data.
URI: http://hdl.handle.net/10553/35732
ISSN: 1574-1818
DOI: 10.1016/j.hedp.2017.03.002
Source: High Energy Density Physics [ISSN 1574-1818], v. 23, p. 60-72
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