DocumentCode
3499715
Title
Tungsten wire-array dynamics and power variations from 20 mm arrays on the Sandia Z facility
Author
Sinars, D.B. ; Cuneo, M.E. ; Wenger, D.F. ; Bliss, David E. ; Mazarakis, Michael G. ; Rogowski, S. ; Sarkisov, G.S. ; Waisman, E.
Author_Institution
Sandia Nat. Lab., Albuquerque, NM, USA
fYear
2004
fDate
1-1 July 2004
Firstpage
110
Abstract
Summary form only given. The radiation source for Z-pinch-driven hohlraum, inertial confinement fusion (ICF) tests on the 20 MA Z facility is a single (or nested) 20 mm diameter tungsten wire array. Full-scale ICF designs call for these arrays to be driven by currents of about 60 MA. To ensure that the scaling requirements of these loads are well understood, we conducted an extensive set of experiments to characterize the performance of these arrays. These tests used a comprehensive set of diagnostics developed for this purpose, including monochromatic 1865 eV and 6151 eV crystal backlighters, 527 nm optical shadowgraphy diagnostics, and various X-ray self-emission diagnostics. During these experiments, the wire array diameter (20 mm), height (10 mm), and wire number (300) were kept constant, but the mass of the array was varied (by altering the initial wire diameters) to obtain substantially different implosion times. Statistics were obtained at total masses of 1.14 mg, 2.5 mg, and 6.0 mg (65 ns, 81 ns, and 100 ns implosion times, respectively), resulting in average peak powers of about 100 TW, 120 TW, and 95 TW, respectively. The higher powers obtained using lower masses are notable because the peak currents achieved were lower due to the shorter implosion times (12.7 MA, 16.3 MA, and 17.3 MA, respectively.) Radiography and shadowgraphy measurements of these arrays show that they retain core/corona structure until 55-60% of the total implosion time. Once the core/corona structure disappears, the arrays appear nominally shell-like and the bulk of the mass starts to move radially inward. Radiography measurements at the same absolute time during the implosion suggest that the ablation dynamics of each array are identical up until the start of the array motion. We present the experimental results and hypotheses for these trends.
Keywords
Z pinch; explosions; plasma diagnostics; plasma inertial confinement; radiography; tungsten; 1.14 mg; 10 mm; 100 TW; 100 ns; 12.5 MA; 120 TW; 16.3 MA; 17.3 MA; 2.5 mg; 20 MA; 20 mm; 527 nm; 6.0 mg; 60 MA; 65 ns; 81 ns; 95 TW; ICF test; Sandia Z pinch hohlraum; W; X-ray self-emission diagnostics; ablation dynamics; core structure; corona structure; implosion times; inertial confinement fusion test; monochromatic crystal backlighters; nested tungsten wire array dynamics; optical shadowgraphy diagnostics; plasma diagnostics; power variations; radiation source; radiography; statistics; Automatic testing; Corona; Current measurement; Inertial confinement; Motion measurement; Radiography; Statistics; Time measurement; Tungsten; Wire;
fLanguage
English
Publisher
ieee
Conference_Titel
Plasma Science, 2004. ICOPS 2004. IEEE Conference Record - Abstracts. The 31st IEEE International Conference on
Conference_Location
Baltimore, MD, USA
ISSN
0730-9244
Print_ISBN
0-7803-8334-6
Type
conf
DOI
10.1109/PLASMA.2004.1339603
Filename
1339603
Link To Document