POWER ENHANCEMENT BY INCREASING THE INITIAL ARRAY RADIUS AND WIRE NUMBER OF TUNGSTEN Z-PINCH

Citation
C. Deeney et al., POWER ENHANCEMENT BY INCREASING THE INITIAL ARRAY RADIUS AND WIRE NUMBER OF TUNGSTEN Z-PINCH, Physical review. E, Statistical physics, plasmas, fluids, and related interdisciplinary topics, 56(5), 1997, pp. 5945-5958
Citations number
39
Categorie Soggetti
Physycs, Mathematical","Phsycs, Fluid & Plasmas
ISSN journal
1063651X
Volume
56
Issue
5
Year of publication
1997
Part
B
Pages
5945 - 5958
Database
ISI
SICI code
1063-651X(1997)56:5<5945:PEBITI>2.0.ZU;2-M
Abstract
Tungsten wire array implosions on the 7- to 8-MA Saturn generator have been optimized using wire number and array diameter variations to pro duce 75 +/- 10 TW of x rays with total energy outputs of 450 +/- 50 kJ . By increasing the number of wires in a 12.5-mm-diam array from 24 to 70 and simultaneously decreasing the individual wire diameter from 13 to 7.5 mu m, the total radiated power increased from 20 +/- 3 to 40 /- 6 TW and the x-ray pulse width decreased from 18 to 8.5 ns. In addi tion, a diameter scan at an implosion time of 50 +/- 5 ns showed that the pulse width has a strong dependence on collapse velocity and wire thickness. For the largest diameter load of 17.5 mm with 120 5-mu m-di am wires, a 4-ns pulse width with a peak power of 75 +/- 10 TW was. ac hieved: four times power gain over the 20-TW electrical power generate d by the pulsed power system. Time-resolved pinhole photography confir ms that the power enhancement with increased wire number is associated with the plasma achieving a tighter compression and better axial unif ormity. For the higher-velocity implosions, we infer from two-dimensio nal radiation-magnetohydrodynamic calculations that the plasma becomes hotter and hence radiates at a higher brightness temperature. Zero-an d two-dimensional load models coupled with a detailed circuit model ha ve shown expected radial kinetic energies in the range of 100-200 kJ. The total radiated energy of > 400 kJ in a 4-20-ns FWHM pulse exceeds the total kinetic energy by more than a factor of 2. Two-dimensional, three-temperature simulations reproduce the observed trends in powers and pulse widths by using a variable initial random density perturbati on. These calculations also indicate that the radiated energy is accou nted for by the total work done on the plasma by the magnetic field.