We report the development of techniques to diagnose plasmas produced by x-r
ay photoionization of thin foils placed near the Z-pinch on the Sandia Z Ma
chine. The development of 100+ TW x-ray sources enables access to novel pla
sma regimes, such as the photoionization equilibrium. To diagnose these pla
smas one must simultaneously characterize both the foil and the driving pin
ch. The desired photoionized plasma equilibrium is only reached transiently
for a 2-ns window, placing stringent requirements on diagnostic synchroniz
ation. We have adapted existing Sandia diagnostics and fielded an additiona
l gated three-crystal Johann spectrometer with dual lines of sight to meet
these requirements. We present sample data from experiments using 1-cm, 180
-eV tungsten pinches to photoionize foils made of 200 Angstrom Fe and 300 A
ngstrom NaF co-mixed and sandwiched between 1000 Angstrom layers of Lexan (
C16H14O3), and discuss the application of this work to benchmarking astroph
ysical models. (C) 2001 American Institute of Physics.