Spectral line shapes and intensities are used for obtaining information on the various regions of magnetic fusion devices. Emission from low principal quantum numbers of hydrogen isotopes is analyzed for understanding the complex recycling mechanism. Lines emitted from high principal quantum numbers of hydrogen and helium are dominated by Stark effect, allowing an electronic density diagnostic in the divertor. Intensities of lines emitted by impurities are fitted for a better knowledge of ion transport in the confined plasma
International audienceModeling the Stark broadening of spectral lines in plasmas is a complex proble...
International audienceHydrogen line radiation can be trapped in some spatial regions within magnetic...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm sp...
Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in diff...
19th International Conference on Atomic Processes in Plasmas (APiP), Campus Les Cordeliers, Paris, F...
Spectral line broadening manifests itself in the study of high density inertial confinement fusion (...
International audienceStark profiles of high-members (n≥7) of the helium triplet diffuse series 1s2p...
Modeling of the spectral line and continuum radiation emitted by hydrogen isotopes in peripheral reg...
Producción CientíficaLine-shape analysis is one of the most important tools for diagnostics of both ...
International audienceA very fast method for calculating line shapes in the presence of an external ...
A parametrised spectral line profile model is formulated to investigate the diagnostic scope for rec...
There is presented an overview of the latest advances in the analytical theory of Stark broadening o...
Context. We studied the Stark broadening of the He I 492.2 nm line, which is sometimes use...
Spatially resolved measurements of deuterium Balmer and Paschen line emission have been performed in...
The shape of atomic spectral lines in plasmas contains information on the plasma parameters, and can...
International audienceModeling the Stark broadening of spectral lines in plasmas is a complex proble...
International audienceHydrogen line radiation can be trapped in some spatial regions within magnetic...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm sp...
Spectral lines, widths, and shapes are powerful tools for emitting/absorbing gas diagnostics in diff...
19th International Conference on Atomic Processes in Plasmas (APiP), Campus Les Cordeliers, Paris, F...
Spectral line broadening manifests itself in the study of high density inertial confinement fusion (...
International audienceStark profiles of high-members (n≥7) of the helium triplet diffuse series 1s2p...
Modeling of the spectral line and continuum radiation emitted by hydrogen isotopes in peripheral reg...
Producción CientíficaLine-shape analysis is one of the most important tools for diagnostics of both ...
International audienceA very fast method for calculating line shapes in the presence of an external ...
A parametrised spectral line profile model is formulated to investigate the diagnostic scope for rec...
There is presented an overview of the latest advances in the analytical theory of Stark broadening o...
Context. We studied the Stark broadening of the He I 492.2 nm line, which is sometimes use...
Spatially resolved measurements of deuterium Balmer and Paschen line emission have been performed in...
The shape of atomic spectral lines in plasmas contains information on the plasma parameters, and can...
International audienceModeling the Stark broadening of spectral lines in plasmas is a complex proble...
International audienceHydrogen line radiation can be trapped in some spatial regions within magnetic...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm sp...