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Contrasting physics in wire array z pinch sources of 1-20 keV emission on the Z facility.

Authors :
Ampleford, D. J.
Jones, B.
Jennings, C. A.
Hansen, S. B.
Cuneo, M. E.
Harvey-Thompson, A. J.
Rochau, G. A.
Coverdale, C. A.
Laspe, A. R.
Flanagan, T. M.
Moore, N. W.
Sinars, D. B.
Lamppa, D. C.
Harding, E. C.
Thornhill, J. W.
Giuliani, J. L.
Chong, Y.-K.
Apruzese, J. P.
Velikovich, A. L.
Dasgupta, A.
Source :
Physics of Plasmas; May2014, Vol. 21 Issue 5, p056708-1-056708-10, 10p
Publication Year :
2014

Abstract

Imploding wire arrays on the 20 MA Z generator have recently provided some of the most powerful and energetic laboratory sources of multi-keV photons, including ~375 kJ of Al K-shell emission (hν ~1-2 keV), ~80 kJ of stainless steel K-shell emission (hν ~5-9 keV) and a kJ-level of Mo K-shell emission (hν ~17 keV). While the global implosion dynamics of these different wire arrays are very similar, the physical process that dominates the emission from these x-ray sources fall into three broad categories. Al wire arrays produce a column of plasma with densities up to ~3 × 10<superscript>21</superscript> ions/cm<superscript>3</superscript>, where opacity inhibits the escape of K-shell photons. Significant structure from instabilities can reduce the density and increase the surface area, therefore increase the K-shell emission. In contrast, stainless steel wire arrays operate in a regime where achieving a high pinch temperature (achieved by thermalizing a high implosion kinetic energy) is critical and, while opacity is present, it has less impact on the pinch emissivity. At higher photon energies, line emission associated with inner shell ionization due to energetic electrons becomes important. [ABSTRACT FROM AUTHOR]

Details

Language :
English
ISSN :
1070664X
Volume :
21
Issue :
5
Database :
Complementary Index
Journal :
Physics of Plasmas
Publication Type :
Academic Journal
Accession number :
96355128
Full Text :
https://doi.org/10.1063/1.4876621