Characteristics of the Stark broadened and overlapping 447.1 nm He I spectral line and its forbidden 447.0 nm components have been measured at electron densities between $4.4 \times 10^{22}$ m-3 and $8.2 \times 10^{22}$ m-3 and electron temperatures between 18 000 K and 33 000 K in plasmas created in five various discharge conditions using the low pressure pulsed arc as an optically thin plasma source operated in helium-nitrogen-oxygen gas mixture. Good agreement was found among our measured line characteristics and their existing calculated values, based on the quasistatic approximation. Possible influence of the singly ionized oxygen impurity atoms (O II) on the intensity values of the dip between allowed and forbidden components was foun...
Context. We studied the Stark broadening of the He I 492.2 nm line, which is sometimes use...
The Stark widths of seventeen N II and ten N III spectral lines, emitted by plasmas with free electr...
Stark widths (W) and shifts (d) of 5 prominent triply ionized oxygen (O IV) spectral lines in 3 mult...
Stark broadening parameters (widths and shifts) of two He I isolated spectral lines are measured in...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm $\...
On the basis of the precisely recorded 706.52 nm He I line shape we have obtained the basic plasma p...
Stark width (W) and shift (d) of the neutral helium (He I) 381.96 nm spectral line in the high lyi...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
This work reports information on the pressure broadened profiles of the HeII Pα, Pβ and P$_\gamma$ ...
Electron densities in an atmospheric helium arc plasma have been measured with the Stark broadening ...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm sp...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Context. We studied the Stark broadening of the He I 492.2 nm line, which is sometimes use...
The Stark widths of seventeen N II and ten N III spectral lines, emitted by plasmas with free electr...
Stark widths (W) and shifts (d) of 5 prominent triply ionized oxygen (O IV) spectral lines in 3 mult...
Stark broadening parameters (widths and shifts) of two He I isolated spectral lines are measured in...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm $\...
On the basis of the precisely recorded 706.52 nm He I line shape we have obtained the basic plasma p...
Stark width (W) and shift (d) of the neutral helium (He I) 381.96 nm spectral line in the high lyi...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
Context. The Stark broadening of the spectral lines of the wavelengths 501.6, 667.8, 728.1, 388.9, 5...
This work reports information on the pressure broadened profiles of the HeII Pα, Pβ and P$_\gamma$ ...
Electron densities in an atmospheric helium arc plasma have been measured with the Stark broadening ...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Characteristics of the astrophysical important Stark broadened 447.15 nm, 587.56 nm and 667.82 nm sp...
Context. Stark broadening of the 447.1 line of neutral helium in a weakly coupled plasma has been st...
Context. We studied the Stark broadening of the He I 492.2 nm line, which is sometimes use...
The Stark widths of seventeen N II and ten N III spectral lines, emitted by plasmas with free electr...
Stark widths (W) and shifts (d) of 5 prominent triply ionized oxygen (O IV) spectral lines in 3 mult...