Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in different astrophysical objects (from the solar system to the most distant objects in the universe—quasars). On the other hand, experimental and theoretical investigations of laboratory plasma have been applied in spectroscopic astrophysical research, especially in research on atomic data needed for line shape calculations. Data on spectral lines and their profiles are also important for diagnostics, analysis, and the modelling of fusion plasma, laser-produced plasma, laser design and development, and various plasmas in industry and technology, like light sources based on plasmas or the welding and piercing of metals by laser-produced plasma. The...
In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the ex...
International audienceNew Stark broadening parameters of interest for the astrophysical, laboratory ...
International audienceUsing a semi-classical approach, we have calculated electron-, proton-, and io...
articles are available on line http://www.mdpi.com/journal/atoms/special_issues/SpectralLineShapesIn...
Producción CientíficaLine-shape analysis is one of the most important tools for diagnostics of both ...
International audienceThe spectrum emitted by a star is determined by the conditions where the photo...
There is presented an overview of the latest advances in the analytical theory of Stark broadening o...
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space ...
Spectral line shapes and intensities are used for obtaining information on the various regions of ma...
Experimental and theoretical studies of Stark broadening of spectral lines in plasmas are the corner...
We have developed computer programs to compare the relative importance of Stark and Doppler broadeni...
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space ...
The spectra emitted by a pulsed-arc discharge have been photographed with a medium resolution spectr...
Spectral line broadening manifests itself in the study of high density inertial confinement fusion (...
A new approach to evaluation of asymmetry parameters of Stark-broadened isolated spectral lines is p...
In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the ex...
International audienceNew Stark broadening parameters of interest for the astrophysical, laboratory ...
International audienceUsing a semi-classical approach, we have calculated electron-, proton-, and io...
articles are available on line http://www.mdpi.com/journal/atoms/special_issues/SpectralLineShapesIn...
Producción CientíficaLine-shape analysis is one of the most important tools for diagnostics of both ...
International audienceThe spectrum emitted by a star is determined by the conditions where the photo...
There is presented an overview of the latest advances in the analytical theory of Stark broadening o...
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space ...
Spectral line shapes and intensities are used for obtaining information on the various regions of ma...
Experimental and theoretical studies of Stark broadening of spectral lines in plasmas are the corner...
We have developed computer programs to compare the relative importance of Stark and Doppler broadeni...
Line-shape analysis is one of the most important tools for diagnostics of both laboratory and space ...
The spectra emitted by a pulsed-arc discharge have been photographed with a medium resolution spectr...
Spectral line broadening manifests itself in the study of high density inertial confinement fusion (...
A new approach to evaluation of asymmetry parameters of Stark-broadened isolated spectral lines is p...
In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the ex...
International audienceNew Stark broadening parameters of interest for the astrophysical, laboratory ...
International audienceUsing a semi-classical approach, we have calculated electron-, proton-, and io...