Recent values of the measured spectral lines Stark widths (since 1988) for neutral and ionized argon atoms, have been compared to the values previously predicted by us. These were found from the established regularities of the Stark widths along the argon isonuclear sequence for 4s-4p and 4s'-4p' types of transitions. Using new experimental Stark width values we have established trends for 4p-4d, 4p'-4d' and 4p-5s type of transitions which enables predictions of the Stark width values for the Ar III and Ar VIII spectral lines, that have not been calculated or measured before, but are of a considerable astrophysical interest
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
Rare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broade...
The existence of the Stark width dependence on the upper-level ionization potential of the quantu...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the ex...
Measured Stark widths and shifts of the neutral argon spectral lines in 4s–4p and 4s–4pV transitions...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Aims. The aim of this work is to analyse experimental Stark halfwidths behaviour for the $(^3$P)ns–$...
International audienceA critical review of the available experimental data on Stark widths and shift...
On the basis of the observed satisfactory agreement between recent experimental and calculated Stark...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
Rare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broade...
The existence of the Stark width dependence on the upper-level ionization potential of the quantu...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
The Stark widths and shifts of 18 triply ionized argon (Ar IV) spectral lines have been measured at ...
In order to find reliable Stark width data, needed in plasma spectroscopy comparision between the ex...
Measured Stark widths and shifts of the neutral argon spectral lines in 4s–4p and 4s–4pV transitions...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Aims. The aim of this work is to analyse experimental Stark halfwidths behaviour for the $(^3$P)ns–$...
International audienceA critical review of the available experimental data on Stark widths and shift...
On the basis of the observed satisfactory agreement between recent experimental and calculated Stark...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
Dependencies enabling one to estimate the Stark widths of spectral lines due to s-p and p-s transiti...
International audienceIn order to complete data on Stark broadening parameters for Ar I line in the ...
Rare Earth Elements are important for stellar atmosphere analysis but the corresponding Stark broade...