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- W2066265129 abstract "The ion contribution to the Stark broadening, as described by a suitably defined asymmetry function ${A}_{L}$, was investigated from the asymmetry behavior of the vacuum-uv spectral lines of N I at 119.955 nm ($^{4}Pensuremath{rightarrow}^{4}S^{0}$), 141.194 nm ($^{2}Densuremath{rightarrow}^{2}P^{0}$), 149.467 nm ($^{2}Pensuremath{rightarrow}^{2}D^{0}$), and 174.273 nm ($^{2}Pensuremath{rightarrow}^{2}P^{0}$). The line radiation, which was emitted under controlled optical depths, was generated in a dense equilibrium plasma (wall-stabilized arc; electron number density $4.0ifmmodetimeselsetexttimesfi{}{10}^{22} {mathrm{m}}^{ensuremath{-}3}ensuremath{le}{n}_{e}ensuremath{le}3.7ifmmodetimeselsetexttimesfi{}{10}^{23} {mathrm{m}}^{ensuremath{-}3}$; temperature $11000ensuremath{le}Tensuremath{le}15000$ K). Deviations between experimental asymmetry functions of this study and those calculated from recently published data by Griem, have been found for the wings of N I 119.955 nm (normalized wavelength distance from the line center $frac{ensuremath{Delta}ensuremath{lambda}}{ensuremath{Delta}{ensuremath{lambda}}_{frac{1}{2}}}ensuremath{ge}1$; ${A}_{L}^{mathrm{Griem}}ensuremath{-}{A}_{L}^{mathrm{this}mathrm{study}}ensuremath{le}0.1$). For N I 141.194, N I 149.467, and N I 174.273 nm, the asymmetry functions based on line profiles calculated by Griem are in agreement with the asymmetry functions of this study within the given uncertainties. In addition, Stark-width and Stark-shift parameters were experimentally determined for the N I spectrum between 118 and 180 nm. The Stark-width parameters calculated by Griem and by Wilson and Nicolet agreed with the data of this study within ifmmodepmelsetextpmfi{} 20%. Only for N I 131.054 and N I 132.663 nm did the Stark-width parameters calculated by Wilson and Nicolet deviate from the corresponding values of this study by approximately + 31%. The calculated Stark-shift parameters of Wilson and Nicolet, however, were considerably higher than the corresponding data of this study (maximum deviation + 78%), whereas the Stark-shift parameters calculated by Griem showed smaller deviations from the data of this study (maximum deviation + 49%)." @default.
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- W2066265129 date "1980-09-01" @default.
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- W2066265129 title "Experimental ion contribution to the Stark broadening of neutral-nitrogen spectral lines in the vacuum uv" @default.
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- W2066265129 doi "https://doi.org/10.1103/physreva.22.1034" @default.
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