shell implosion experiments in which we trace the time evolution of the electron density
through stagnation. Very high electron densities in the range 2–8× 10 24 cm− 3 are inferred.
We also discuss several novel spectral features, including large Stark broadening of satellite
line emission, optical thicknesses for resonant transitions lower than expected, and the
onset of density-dependent ''blue satellites''on the high-energy wing of the He α line.