International audienceIn order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we determined Stark widths and shifts due to electron, proton and ionized helium impacts for nine lines (4191.0, 4259.4, 5912.1, 6043.2, 6045.0, 6752.9, 7503.9, 7514.6, 7724.2 Å), using jK coupling and semiclassical perturbation theory. The obtained results will enter the STARK-B database, which is a part of the Virtual Atomic and Molecular Data Center
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...
In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of ...
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 ...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
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....
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
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...
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 provide Stark broadening data in X-ray and far UV wavelength regio...
In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of ...
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 ...
In order to complete data on Stark broadening parameters for Ar I line in the visible spectrum, we d...
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....
Stark broadening parameters, full width at half maximum of spectral line and shift, have been calcul...
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...
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 provide Stark broadening data in X-ray and far UV wavelength regio...
In order to complete Stark broadening data for Ne I spectral lines which are needed for analysis of ...