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Title: Trends in radiation production from dynamic-hohlraums driven by single and nested wire arrays

Journal Article · · Physics of Plasmas
DOI:https://doi.org/10.1063/1.1587708· OSTI ID:889411
 [1];  [1];  [1];  [2]
  1. Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
  2. Los Alamos National Lab. (LANL), Los Alamos, NM (United States)

The axial radiation developed primarily from the interior of an imploding dynamic hohlraum (DH) target within a Z pinch using a single array with a large number of tungsten wires is compared with that generated using a standard [Phys. Plasmas 9, 3573 (2002)] nested (outer plus inner) array on Z. These measurements indicate that a single-array with a mass (2.5 mg) near that of the combined mass of the nested-array maximizes the DH axial power. At this mass, the DH utilizing the standard nested array generates (23±15)%(23±15)% more axial power than that of a single array. Measurements over a range of single-array masses (2–6 mg) show a decrease in radiation power for masses above 3.5 mg. Two-dimensional radiation magnetohydrodynamic simulations, which have successfully described radial emission from targetless implosions for both single and nested-array configurations [Phys. Plasmas 6, 2178 (1999)], but, do not follow the observed trends well. Furthermore, this lack of tracking implies that current 2D models, which take into account the development of the magnetic Rayleigh–Taylor (RT) instability in the r–zr–z plane, require improvements in order to provide a self-consistent description of the implosion dynamics and radiation production for DH experiments.

Research Organization:
Sandia National Lab. (SNL-NM), Albuquerque, NM (United States)
Sponsoring Organization:
USDOE
DOE Contract Number:
AC04-94AL85000
OSTI ID:
889411
Report Number(s):
SAND2003-0131J; PHPAEN; TRN: US0604397
Journal Information:
Physics of Plasmas, Vol. 10, Issue 8; ISSN 1070-664X
Publisher:
American Institute of Physics (AIP)
Country of Publication:
United States
Language:
English

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