Top/bottom asymmetry measured in axial radiation exiting dynamic-hohlraum X-ray source on Z

T.W.L. Sanford1, R.C. Mock1, G.A. Chandler1,2, R.J. Leeper3, R.W. Lemke1,2, T.A. Mehlhorn3, T.J. Nash4, G.S. Sarkisov, E.M. Waisman5,1, R.E. Chrien6, G.C. Idzorek6, D.L. Peterson6, R.G. Watt6, J.P. Chittenden7, M.G. Haines7, S.V. Lebedev7, D. Mosher8
1Sandia National Laboratories, Albuquerque, NM, USA
2Sandia National Laboratories, Albuquerque, NM, US
3Sandia Nat. Labs., Albuquerque, NM, USA
4Sandia National Laboratories, Albuquerque NM, USA
5Alameda Applied Sciences Corporation, San Diego, CA, USA
6Los Alamos National Laboratory, Los Alamos, NM, USA
7Imperial College, Blackett Laboratories, London, UK
8Pulsed Power Physics Branch, Naval Research Laboratory, Inc., Washington D.C., DC, USA

Tóm tắt

Summary form only given, as follows. A radiation source has been developed on the 20-MA Z facility that produces a high-power x-ray pulse, generated in the positive z direction primarily from the interior of a collapsing dynamic hohlraum The hohlraum is created from a solid cylindrical CH/sub 2/ target centered within an imploding tungsten wire-array z-pinch. This pulse, which exits a 4.5 mm/sup 2/ REH (radiation exit hole) centered above the target, begins /spl sim/5 ns prior to stagnation (as defined by radial-radiation power). The 5-ns interval leading to stagnation represents the duration the imploding tungsten plasma acts as a hohlraum, trapping radiation developed within its interior. The trapped radiation exiting the top hole is remarkably reproducible, having a risetime of 2.5/spl plusmn/0.2 ns, a pulsewidth of 4.6/spl plusmn/0.5 ns, and reaches a maximum intensity of 9.7/spl plusmn/1.8 TW (assuming Lambertian emission) 1.4/spl plusmn/0.3 ns prior to stagnation. This radiation pulse is useful for performing radiation-transport experiments in excess of 200 eV. By adding an identical REH at the bottom of the hohlraum, the radiation generated in the negative z direction through a bottom REH offers the possibility of doubling the utility of the hohlraum as a source of high-temperature radiation. Because of the up/down symmetry of the load about the mid-plane of the z-axis (aside from the power feed), a radiation pulse similar to that exiting the top-REH (anode) is expected from the bottom REH (cathode).

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