“Stark broadening” theory and calculations have been extensively developed for about 50
years. The theory can now be considered as mature for many applications, especially for …

With the development of astronomical observations from space, spectral lines of trace
elements can now be observed in stellar spectra with good resolution, and atomic data for …

Stark broadening theory is currently operated for calculating widths and shifts of spectral
lines that are needed for spectroscopic diagnostics and modeling in astrophysics, laboratory …

Energy levels, electric dipole transition probabilities and oscillator strengths in five times
ionized silicon have been calculated in intermediate coupling. The present calculations …

We have calculated the energy levels, oscillator strengths, and transition probabilities for
eight carbon-like ions (Na vi, Mg vii, Al viii, Si ix, P x, S xi, Cl xii and Ar xiii) using the Hartree …

Stark-broadening parameters have been calculated for 114 spectral lines of triply charged
lead ion (Pb iv) using semiclassical perturbation approach in the impact approximation. The …

New Stark broadening parameters of interest for the astrophysical, laboratory and
technological plasma modelling, investigations and analysis for nine resonant Cr ii …

Stark broadening theories and calculations have been extensively developed for about 50
years. The theory can now be considered as mature for many applications, especially for …

Atomic physics in plasmas has been an essential tool for many years. Accurate
spectroscopic diagnostics and modeling require the knowledge of numerous collisional line …

Published data concerning Stark widths for spectral lines originating from 3s-3p transition
arrays of multiply charged ions of different elements are used to demonstrate their …