Add to ORKGInternational audienceIn order to provide Stark broadening data in X-ray and far UV wavelength region, of interest for modelling and analysis of astrophysical plasmas in extreme conditions, we performed calculations of Stark broadened line widths and shifts for Ar XV using the semiclassical perturbation theory
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
The significance of Stark broadening data for problems in astrophysics, physics, as well as for tech...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
International audienceThe significance of Stark broadening data for problems in astrophysics, physic...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
The significance of Stark broadening data for problems in astrophysics, physics, as well as for tech...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
International audienceStark broadening parameters (width and shift) of six Ar I spectral lines: 522....
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
International audienceThe significance of Stark broadening data for problems in astrophysics, physic...
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
The significance of Stark broadening data for problems in astrophysics, physics, as well as for tech...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...