1970
DOI: 10.1103/physreva.1.221
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Stark Broadening of Singly Ionized Nitrogen Lines

Abstract: Profiles of nine lines of singly ionized nitrogen have been measured in a dense (Ne= 1.9 && 10 cm ) high-temperature (22 800 'K) plasma produced behind the reflected shock wave in a T tube. Measurements were carried out that verified the fact that the plasma was homogeneous in both the radial and the axial directions and that the plasma was optically thin at the various wavelengths where the profiles were measured. The half-widths of the measured profiles show large discrepancies with earlier reported measurem… Show more

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Cited by 21 publications
(3 citation statements)
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“…During the spark phase, the electron number density N e is determined by modeling the experimental spectra of N + extracted at each radial position from Abel-inverted images. Among the line broadening sources (natural, pressure, Stark, Doppler, instrumental K), Stark broadening due to electron collisions [23,24] appears in our case to be predominant. With our set-up, the contribution of Doppler and pressure to N + lines broadening is negligible compared with the instrumental function (0.1 nm width).…”
Section: Electron Density and Temperature Measurements During The Spa...mentioning
confidence: 54%
“…During the spark phase, the electron number density N e is determined by modeling the experimental spectra of N + extracted at each radial position from Abel-inverted images. Among the line broadening sources (natural, pressure, Stark, Doppler, instrumental K), Stark broadening due to electron collisions [23,24] appears in our case to be predominant. With our set-up, the contribution of Doppler and pressure to N + lines broadening is negligible compared with the instrumental function (0.1 nm width).…”
Section: Electron Density and Temperature Measurements During The Spa...mentioning
confidence: 54%
“…[14] 2s 2 2p( 2 P o )3p-2s 2 2p( 2 P o )3d [9] 39, 3 (12) [15] 32 (12) [16] When comparing Stark widths from this work with previous experimental data, we should restrict ourselves to experiments with similar plasma parameters to those used here, for instance, those from [5,6,8,10,11,16] and the agreement is in general good, especially perhaps with that of Djeniže et al [16]. Concerning data taken under very different plasma conditions, this good agreement extends to all experiments developed at similar temperatures to ours [7,15] and systematically lower values are found in experiments with much higher T e values [12,17], which may be explained according to the predicted and observed (see figure 5) decreasing trend of the Stark width with increasing temperature.…”
Section: Table 1 Summary Of the Plasma Conditions Concerning The Expe...mentioning
confidence: 99%
“…According to reviews [1][2][3], there are a number of important experimental works [4][5][6][7][8][9][10][11][12] and some theoretical ones [13,14] in the literature dealing with the Stark parameters of N II lines. Although several new results have been published subsequently [15][16][17], there still remain some discrepancies to be clarified and the number of lines for which there are available data is small in comparison with the complete visible N II spectrum, especially for 2s 2 2p( 2 P o )3p-2s 2 2p( 2 P o )3d, 2s 2 2p( 2 P o )3d-2s 2 2p( 2 P o 1/2 )4f and 2s2p 2 ( 4 P)3s-2s2p 2 ( 4 P)3p transition arrays.…”
Section: Introductionmentioning
confidence: 99%