1988
DOI: 10.1109/27.3858
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The type and extent of non-LTE in argon arcs at 0.1-10 bar

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Cited by 17 publications
(5 citation statements)
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“…The major source of error in the absolute-intensity method is the uncertainty in the transition probability used. It has been found by Eddy and Sedghinasab [23] that the same corrections to transition probabilities do not make a significant change in the temperature but would make larger changes in the species' densities because of the exponential effects. An overall extent of departures from LTE is indicated by these figures.…”
Section: Resultsmentioning
confidence: 84%
“…The major source of error in the absolute-intensity method is the uncertainty in the transition probability used. It has been found by Eddy and Sedghinasab [23] that the same corrections to transition probabilities do not make a significant change in the temperature but would make larger changes in the species' densities because of the exponential effects. An overall extent of departures from LTE is indicated by these figures.…”
Section: Resultsmentioning
confidence: 84%
“…On the other hand, some workers have provided spectroscopic evidence for departures from LTE near the cathode of similar arcs [4][5][6]. Moreover, it has been suggested that the departure from LTE in argon arcs is extensive up to a pressure of 3 [7] or even 5 atm [8]. In hydrogen the critical number density for complete LTE at 20 000 K has been given as 2 × 10 24 m −3 [9].…”
Section: Introductionmentioning
confidence: 99%
“…Modelling high pressure arcs, and in particular their temperature distribution, is useful for the development of high power light sources, arc-jet thrusters, and arc welding processes [1][2][3]. In two extreme cases, theoretical modelling is relatively simple: (1) If the arc plasma is transparent to its own thermal radiation, energy loss may be described in terms of a 'sink', by including a radiation term in the energy balance equation [4][5][6]. (2) If the plasma column is completely opaque to its own thermal radiation, the radiation is in local thermodynamic equilibrium and radiative heat conductivity can be determined from well-known expressions for the radiation intensity and density [4,7].…”
Section: Introductionmentioning
confidence: 99%