Power enhancement by increasing the initial array radius and wire number of tungsten Z pinches

被引:133
作者
Deeney, C
Nash, TJ
Spielman, RB
Seaman, JF
Chandler, GC
Struve, KW
Porter, JL
Stygar, WA
McGurn, JS
Jobe, DO
Gilliland, TL
Torres, JA
Vargas, MF
Ruggles, LE
Breeze, S
Mock, RC
Douglas, MR
Fehl, DL
McDaniel, DH
Matzen, MK
Peterson, DL
Matuska, W
Roderick, NF
MacFarlane, JJ
机构
[1] LOS ALAMOS NATL LAB,LOS ALAMOS,NM 87545
[2] UNIV WISCONSIN,FUS TECHNOL INST,MADISON,WI 53706
来源
PHYSICAL REVIEW E | 1997年 / 56卷 / 05期
关键词
D O I
10.1103/PhysRevE.56.5945
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
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 +/- 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 addition, 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-diam wires, a 4-ns pulse width with a peak power of 75 +/- 10 TW 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 100-200 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 perturbation. These calculations also indicate that the radiated energy is accounted for by the total work done on the plasma by the magnetic field.
引用
收藏
页码:5945 / 5958
页数:14
相关论文
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