Radiative Properties of Hot Dense Matter, SANTA BARBARA, CA, NOV, 1992International audienceFor hot and dense plasma studies both fundamental or diagnosis oriented, one needs to solve concurrently several problems coming from different fields. Our contribution to such studies has been to develop a fast computer code capable of providing spectral profiles for the radiation emitted by multiply charged ions imbedded in hot and dense non-equilibrium plasmas. The results of this numerical method have been carefully compared to those generated by a simulation code based on a molecular dynamic simulation of the stochastic microfield. This paper provides information about some new aspects of the line mixing model used to account for the ion dynamic...
This book is devoted to the calculation of hot-plasma properties which generally requires a huge num...
We discuss the line shapes for the 1s-2p, 1s-3p and (ls)/sup 2/ - 1s2p, (1s)/sup 2/ - 1s3p absorptio...
International audienceA very fast method to account for charged particle dynamics effects in calcula...
International audienceA model is developed that permits the calculation of the radiation emitted by ...
International audienceA model aimed at describing the electronic structure of hot dense plasmas is p...
International audienceA method for calculating the redistribution of resonance radiation in hot, den...
Abstract: The effect of spectral line broadening under influence of ion microfield (Stark ...
International audienceA method is presented to interpret spectroscopic measurements to obtain a diag...
In recent experiments uniform plasmas have been generated at high densities and low temperatures, (t...
Meeting on Radiative Properties of Hot Dense Matter III, LAWRENCE LIVERMORE NATL LAB, LIVERMORE, CAL...
We present a Stark-Zeeman spectral line shape model and the associated numerical code, PPPB, designe...
We have developed computer programs to compare the relative importance of Stark and Doppler broadeni...
The ionization and radiation dynamics of dense magnetohydrodynamic plasmas has been modeled in a fas...
The scope for developing the present numerical method was to perform parametric studies for optimiza...
Motivation for the study of hot, dense ($\sim$solid density) plasmas has historically been in connec...
This book is devoted to the calculation of hot-plasma properties which generally requires a huge num...
We discuss the line shapes for the 1s-2p, 1s-3p and (ls)/sup 2/ - 1s2p, (1s)/sup 2/ - 1s3p absorptio...
International audienceA very fast method to account for charged particle dynamics effects in calcula...
International audienceA model is developed that permits the calculation of the radiation emitted by ...
International audienceA model aimed at describing the electronic structure of hot dense plasmas is p...
International audienceA method for calculating the redistribution of resonance radiation in hot, den...
Abstract: The effect of spectral line broadening under influence of ion microfield (Stark ...
International audienceA method is presented to interpret spectroscopic measurements to obtain a diag...
In recent experiments uniform plasmas have been generated at high densities and low temperatures, (t...
Meeting on Radiative Properties of Hot Dense Matter III, LAWRENCE LIVERMORE NATL LAB, LIVERMORE, CAL...
We present a Stark-Zeeman spectral line shape model and the associated numerical code, PPPB, designe...
We have developed computer programs to compare the relative importance of Stark and Doppler broadeni...
The ionization and radiation dynamics of dense magnetohydrodynamic plasmas has been modeled in a fas...
The scope for developing the present numerical method was to perform parametric studies for optimiza...
Motivation for the study of hot, dense ($\sim$solid density) plasmas has historically been in connec...
This book is devoted to the calculation of hot-plasma properties which generally requires a huge num...
We discuss the line shapes for the 1s-2p, 1s-3p and (ls)/sup 2/ - 1s2p, (1s)/sup 2/ - 1s3p absorptio...
International audienceA very fast method to account for charged particle dynamics effects in calcula...