Calculation of the Stark splitting for some levels of xenon

Gorchakov, L. V.; Yancharina, A. M.; Murav'ev, I. I.

doi:10.1007/bf00894687

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4 Line Pro$les1

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1979

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“…Unsold 1955). For our calculations we used the C4 constants of Spiegelhalter (1968), Lesage and Richou (1972), Gorchakov and Yancharina (1972) and Yancharina (1973). Additional C4 constants have been calculated using the relation C40cn*7 within an energy level sequence where n+ is the effective principal quantum number.…”

Section: 4 Line Pro$lesmentioning

confidence: 99%

The contribution of lines to the total emission coefficient of xenon plasmas

Günther¹

1979

J. Phys. D: Appl. Phys.

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The line radiation of xenon plasma at T=10000-14000K and p=(2-40)*105 Pa was calculated using published transition probabilities and broadening constants. Self-absorption proved to be important for many lines and was taken into account by means of a simple model. These results have been used to calculate the total radiation power which has been compared with the results of Kozlov (1974) and with the earlier experiments of Gunther (1973). The best agreement between theory and experiment was achieved on the basis of the Schirmer line factor due to Gunther.

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Section: 4 Line Pro$lesmentioning

confidence: 99%

The contribution of lines to the total emission coefficient of xenon plasmas

Günther¹

1979

J. Phys. D: Appl. Phys.

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show abstract

Calculation of the Stark splitting for some levels of xenon

Cited by 1 publication

References 3 publications

The contribution of lines to the total emission coefficient of xenon plasmas

The contribution of lines to the total emission coefficient of xenon plasmas

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