Stark broadening models for plasma diagnostics
MA Gigosos - Journal of Physics D: Applied Physics, 2014 - iopscience.iop.org
A review of the models used for the calculation of the Stark broadening spectrum for
plasmas is presented. The aim is to provide an overview of the related theories using a …
plasmas is presented. The aim is to provide an overview of the related theories using a …
[图书][B] Introduction to plasma spectroscopy
HJ Kunze - 2009 - books.google.com
Although based on lectures given for graduate students and postgraduates starting in
plasma physics, this concise introduction to the fundamental processes and tools is as well …
plasma physics, this concise introduction to the fundamental processes and tools is as well …
Widths and shifts of isolated lines of neutral and ionized atoms perturbed by collisions with electrons and ions: An outline of the semiclassical perturbation (SCP) …
S Sahal-Bréchot, MS Dimitrijević, N Ben Nessib - Atoms, 2014 - mdpi.com
“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 …
years. The theory can now be considered as mature for many applications, especially for …
The STARK-B database VAMDC node: A repository for spectral line broadening and shifts due to collisions with charged particles
S Sahal-Bréchot, MS Dimitrijević, N Moreau… - Physica …, 2015 - iopscience.iop.org
Accurate spectroscopic diagnostics and modeling require the knowledge of numerous
collisional line profiles. Access to such data via an online database has become …
collisional line profiles. Access to such data via an online database has become …
Quantum Stark widths of Se III–VI lines
Stark broadening for 19 spectral lines of several selenium ions (four Se III lines, eight Se IV
lines, three Se V lines and four Se VI lines) have been calculated using our quantum …
lines, three Se V lines and four Se VI lines) have been calculated using our quantum …
Stark broadening for Br VI and Kr V-VII lines in hot star atmospheres
S Sahal-Bréchot, H Elabidi - Astronomy & Astrophysics, 2021 - aanda.org
Context. This paper provides missing Stark broadening of the Br VI and Kr V-VII lines
recently discovered in the ultraviolet spectrum of the hot white dwarf RE 0503–289 and …
recently discovered in the ultraviolet spectrum of the hot white dwarf RE 0503–289 and …
Sr v–vi line widths in hot white dwarf atmospheres
Missing Stark widths for 37 spectral lines of strontium ions (17 Sr v lines and 20 Sr vi lines)
have been calculated using a quantum-mechanical method. Twenty-three spectral lines of …
have been calculated using a quantum-mechanical method. Twenty-three spectral lines of …
Quantum Stark broadening of 3s–3p spectral lines in Li-like ions; Z-scaling and comparison with semi-classical perturbation theory
H Elabidi, S Sahal-Bréchot, N Ben Nessib - The European Physical …, 2009 - Springer
Quantum mechanical results for the electron impact Stark widths of the 3s–3p transitions in
ten Li-like ions from C IV to P XIII are carried out. The atomic structure is obtained through a …
ten Li-like ions from C IV to P XIII are carried out. The atomic structure is obtained through a …
Stark broadening of Zr iv spectral lines in the atmospheres of chemically peculiar stars
Z Majlinger, Z Simić… - Monthly Notices of the …, 2017 - academic.oup.com
Stark widths for 18 Zr iv spectral lines have been calculated by using the modified semi-
empirical method. The obtained results have been used to investigate the influence of Stark …
empirical method. The obtained results have been used to investigate the influence of Stark …
Electron impact excitation and broadening of Ar X and Ar XIII lines
We calculate in this work quantum Stark broadening, radiative atomic data (energy levels,
radiative decay rates, line strengths, oscillator strengths) and collisional parameters …
radiative decay rates, line strengths, oscillator strengths) and collisional parameters …