We are undertaking to develop a set of computational capabilities which will facilitate the access, manipulation, and understanding of atomic data in calculations of x-ray spectral modeling. In this present limited description we will emphasize the objectives for this work, the design philosophy, and aspects of the atomic database, as a more complete description of this work is available. The project is referred to as the Plasma Spectroscopy Initiative; the computing environment is called PSI, or the ``PSI shell`` since the primary interface resembles a UNIX shell window. The working group consists of researchers in the fields of x-ray plasma spectroscopy, atomic physics, plasma diagnostics, line shape theory, astrophysics, and computer sci...
Plasma emission models used in X-ray astronomy need to simulate X-ray spectra from at least thirteen...
We summarize progress that has been made on the determination of atomic data pertinent to the fusion...
CHIANTI provides a database of atomic energy levels, wavelengths, radiative transition probabilities...
The design and analysis of plasma spectroscopy experiments can be significantly complicated by relat...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
Our research program is designed to carry out state-of-the-art atomic physics calculations crucial t...
Trends and focii of interest in atomic modelling and data are identified in connection with recent o...
We describe the atomic database of the xstar spectral modeling code, summarizing the systematic upgr...
The advancement in the acquisition of spectral data from meteors, as well as the capability to analy...
This publication contains written versions of most of the invited talks presented at the workshop on...
This book is a data book for atomic and plasma physicists. Numerical data are given for atoms, atomi...
We describe recent work at NIST to develop and maintain databases for spectra, transition probabilit...
Hot astrophysical plasma is ubiquitous in the Universe, from comets in our Solar system to the large...
International audienceA method is presented to interpret spectroscopic measurements to obtain a diag...
Plasma emission models used in X-ray astronomy need to simulate X-ray spectra from at least thirteen...
We summarize progress that has been made on the determination of atomic data pertinent to the fusion...
CHIANTI provides a database of atomic energy levels, wavelengths, radiative transition probabilities...
The design and analysis of plasma spectroscopy experiments can be significantly complicated by relat...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
CHIANTI is an atomic database and software package for modeling emission lines and continua from hot...
Our research program is designed to carry out state-of-the-art atomic physics calculations crucial t...
Trends and focii of interest in atomic modelling and data are identified in connection with recent o...
We describe the atomic database of the xstar spectral modeling code, summarizing the systematic upgr...
The advancement in the acquisition of spectral data from meteors, as well as the capability to analy...
This publication contains written versions of most of the invited talks presented at the workshop on...
This book is a data book for atomic and plasma physicists. Numerical data are given for atoms, atomi...
We describe recent work at NIST to develop and maintain databases for spectra, transition probabilit...
Hot astrophysical plasma is ubiquitous in the Universe, from comets in our Solar system to the large...
International audienceA method is presented to interpret spectroscopic measurements to obtain a diag...
Plasma emission models used in X-ray astronomy need to simulate X-ray spectra from at least thirteen...
We summarize progress that has been made on the determination of atomic data pertinent to the fusion...
CHIANTI provides a database of atomic energy levels, wavelengths, radiative transition probabilities...