Stark broadening parameters, full width at half maximum of spectral line and shift, have been calculated for 3 spectral lines of Ar VII, for broadening by electron, proton, and He III impacts. For calculations, the semiclassical perturbation approach in the impact approximation has been used. The results are provided for temperatures from 20 000 K to 500 000 K and for an electron density of 1017 cm-3. Obtained results will be included in the STARK-B database which is also included in Virtual atomic and molecular data center (VAMDC)
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact l...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
We present in this paper the results of a theoretical study of electron impact broadening for severa...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
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 ...
Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line wid...
Electron-, proton-, and ionized helium-impact broadening parameter tables for In II spectral lines, ...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact l...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
Using the semi-classical perturbation approach in the impact approximation, full width at half maxim...
We present in this paper the results of a theoretical study of electron impact broadening for severa...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
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 ...
Using a semiclassical approach, we have calculated electron−, proton−, and He III−impact line wid...
Electron-, proton-, and ionized helium-impact broadening parameter tables for In II spectral lines, ...
Stark broadening theory is currently operated for calculating widths and shifts of spectral lines th...
Using a semiclassical approach, we have calculated electron-, proton-, and ionized helium-impact l...
International audienceIn order to provide Stark broadening data in X-ray and far UV wavelength regio...