Power enhancement by increasing the initial array radius and wire number of tungsten Z pinches
- Sandia National Laboratory, MS-1194, Albuquerque, New Mexico 87185-1194 (United States)
- Los Alamos National Laboratory, MS B-259, Los Alamos, New Mexico 87545 (United States)
- Fusion Technology Institute, University of Wisconsin, Madison, Wisconsin 53706 (United States)
Tungsten wire array implosions on the 7- to 8-MA Saturn generator have been optimized using wire number and array diameter variations to produce 75{plus_minus}10TW of x rays with total energy outputs of 450{plus_minus}50kJ. 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{plus_minus}3 to 40{plus_minus}6TW and the x-ray pulse width decreased from 18 to 8.5 ns. In addition, a diameter scan at an implosion time of 50{plus_minus}5ns 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-diam wires, a 4-ns pulse width with a peak power of 75{plus_minus}10TW was achieved: four times power gain over the 20-TW electrical power generated by the pulsed power system. Time-resolved pinhole photography confirms that the power enhancement with increased wire number is associated with the plasma achieving a tighter compression and better axial uniformity. For the higher-velocity implosions, we infer from two-dimensional radiation-magnetohydrodynamic calculations that the plasma becomes hotter and hence radiates at a higher brightness temperature. Zero- and two-dimensional load models coupled with a detailed circuit model have shown expected radial kinetic energies in the range of 100{endash}200 kJ. The total radiated energy of {gt}400kJ in a 4{endash}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 perturbation. These calculations also indicate that the radiated energy is accounted for by the total work done on the plasma by the magnetic field. {copyright} {ital 1997} {ital The American Physical Society}
- Research Organization:
- Sandia National Laboratory
- DOE Contract Number:
- AC04-94AL85000
- OSTI ID:
- 544890
- Journal Information:
- Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics, Journal Name: Physical Review. E, Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics Journal Issue: 5 Vol. 56; ISSN PLEEE8; ISSN 1063-651X
- Country of Publication:
- United States
- Language:
- English
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