Analysis of time-resolved argon line spectra from OMEGA direct-drive implosions.
We discuss the observation and data analysis of argon K-shell line spectra from argon-doped deuterium-filled OMEGA direct-drive implosion cores based on data recorded with two streaked crystal spectrometers. The targets were 870 microm in diameter, 27 microm wall thickness plastic shells filled with 20 atm of deuterium gas, and a tracer amount of argon for diagnostic purposes. The argon K-shell line spectrum is primarily emitted at the collapse of the implosion and its analysis provides a spectroscopic diagnostic of the core implosion conditions. The observed spectra includes the He alpha, Ly alpha, He beta, He gamma, Ly beta, and Ly gamma line emissions and their associated He- and Li-like satellites thus covering a broad photon energy range from 3100 to 4200 eV with a spectral resolution power of approximately 500. The data analysis relies on detailed atomic and spectral models that take into account nonequilibrium collisional-radiative atomic kinetics, Stark-broadened line shapes, and radiation transport calculations.
Florido
R
R
Department of Physics, University of Nevada, Reno, Nevada 89557, USA.
Nagayama
T
T
Mancini
R C
RC
Tommasini
R
R
Delettrez
J A
JA
Regan
S P
SP
Smalyuk
V A
VA
Rodríguez
R
R
Gil
J M
JM