We present numerical simulations from the code GALAXY, frequently employed to model the distribution of excitation and ionization, and the spectral emission from laboratory plasma experiments. In particular, preliminary calculations relevant to the Lawrence Livermore National Laboratory photoionization collaboration are presented, along with results which compare GALAXY with results from the astrophysical code CLOUDY.
|Name||ASP Conference Series|
|Publisher||Astronomical Society of the Pacific|
|Conference||Spectroscopic challenges of photoionized plasmas|
|Period||1/01/01 → …|