Photoionised plasmas are common in astrophysical environments and new high resolution spectra from such sources have been recorded in recent years by the Chandra and XMM-Newton satellites. These provide a wealth of spectroscopic information and have motivated recent efforts aimed at obtaining a detailed understanding of the atomic-kinetic and radiative characteristics of photoionised plasmas. The Z-pinch facility at the Sandia National Laboratories is the most powerful terrestrial source of X-rays and provides an opportunity to produce photoionised plasmas in a well characterised radiation environment. We present modelling work and experimental design considerations for a forthcoming experiment at Sandia in which X-rays from a collapsing Z-...
We describe laboratory experiments to generate x-ray photoionized plasmas of relevance to accretion-...
In this paper we report the experimental implementation of a theoretically proposed technique for cr...
Many of the fundamental questions in astrophysics can be addressed using spectroscopic observations ...
c Springer-Verlag Abstract Photoionised plasmas are common in astro-physical environments and new h...
We report on an initial spectroscopic study of low-density, x-ray photoionized neon with x-ray spect...
Photoionized plasmas are a special class of plasma common in astrophysical environments, such as x-r...
Present-day Z-pinch experiments generate similar to2 x 10(21) erg/s peak power, similar to6 ns full-...
Due to the lack of spaceships with intergalactic capability, now and in the foreseeable future, we m...
We have extensively modeled a neon photoionization experiment on the Z machine at Sandia National La...
Presented in this thesis are numerical simulations from the code GALAXY, frequently employed to mode...
We present numerical simulations from the code GALAXY, frequently employed to model the distribution...
We report on a theoretical study on atomic kinetics modeling of a photoionized neon plasma at condit...
In order to provide benchmark data for models used to interpret X-ray astronomy data from newly-laun...
We present some recent highlights and prospects for the study of hot astrophysical plasmas. Hot plas...
Implementation of a novel experimental approach using a bright source of narrowband x-ray emission h...
We describe laboratory experiments to generate x-ray photoionized plasmas of relevance to accretion-...
In this paper we report the experimental implementation of a theoretically proposed technique for cr...
Many of the fundamental questions in astrophysics can be addressed using spectroscopic observations ...
c Springer-Verlag Abstract Photoionised plasmas are common in astro-physical environments and new h...
We report on an initial spectroscopic study of low-density, x-ray photoionized neon with x-ray spect...
Photoionized plasmas are a special class of plasma common in astrophysical environments, such as x-r...
Present-day Z-pinch experiments generate similar to2 x 10(21) erg/s peak power, similar to6 ns full-...
Due to the lack of spaceships with intergalactic capability, now and in the foreseeable future, we m...
We have extensively modeled a neon photoionization experiment on the Z machine at Sandia National La...
Presented in this thesis are numerical simulations from the code GALAXY, frequently employed to mode...
We present numerical simulations from the code GALAXY, frequently employed to model the distribution...
We report on a theoretical study on atomic kinetics modeling of a photoionized neon plasma at condit...
In order to provide benchmark data for models used to interpret X-ray astronomy data from newly-laun...
We present some recent highlights and prospects for the study of hot astrophysical plasmas. Hot plas...
Implementation of a novel experimental approach using a bright source of narrowband x-ray emission h...
We describe laboratory experiments to generate x-ray photoionized plasmas of relevance to accretion-...
In this paper we report the experimental implementation of a theoretically proposed technique for cr...
Many of the fundamental questions in astrophysics can be addressed using spectroscopic observations ...