Recent success on the Saturn [C. Deeney , Phys. Rev. E 56, 5945 (1997)] and
Z [R. B. Spielman , Phys. Plasmas 5, 2105 (1998)] accelerators at Sandia N
ational Laboratories have demonstrated the ability to scale Z-pinch paramet
ers to increasingly larger current pulsed power facilities. Next generation
machines will require even larger currents (> 20 MA), placing further dema
nds on pulsed power technology. To this end, experiments have been carried
out on Saturn operating in a long pulse mode, investigating the potential o
f lower voltages and longer implosion times while still maintaining pinch f
idelity. High wire number, 25 mm diam tungsten arrays were imploded with im
plosion times ranging from 130 to 240 ns. The results were comparable to th
ose observed in the Saturn short pulse mode, with rise times on the order o
f 4.5-6.5 ns. Experimental data will be presented, along with two-dimension
al radiation magnetohydrodynamic simulations used to explain and reproduce
the experiment. (C) 2000 American Institute of Physics. [S1070- 664X(00)043
07-X].