Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-12-04T19:40:10.314Z Has data issue: false hasContentIssue false
  • English
  • Français

Calculations and diagnostic applications of Stark-broadened absorption line profiles for the L-shell ions of argon

Published online by Cambridge University Press:  09 March 2009

D. A. Haynes Jr ,
R. C. Mancini  and
C. F. Hooper Jr
D. A. Haynes Jr
Affiliation:
Department of Physics, University of Florida, Gainesville, FL 32611
R. C. Mancini
Affiliation:
Department of Physics, University of Florida, Gainesville, FL 32611
C. F. Hooper Jr
Affiliation:
Department of Physics, University of Florida, Gainesville, FL 32611
Get access Rights & Permissions [Opens in a new window]

Abstract

We calculated Stark-broadened absorption line profiles for n = 1 to n = 2 inner-shell transitions in the L-shell ions of Ar for electron number densities between 5 × 1023 cm-3 and 5 × 1024 cm-3 and for temperatures in the range 100–600 eV. These line profiles are used to calculate the frequency-dependent optical depth of hot, dense Ar plasmas. We also investigated the possibility of using Stark-broadened absorption line profiles for diagnostic applications.

Type
Research Article
Information
Laser and Particle Beams , Volume 11 , Issue 1 , March 1993 , pp. 205 - 219
Copyright
Copyright © Cambridge University Press 1993

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

REFERENCES

Abdallah, J. & Clark, R. 1991 J. Appl. Phys. 69, 23.CrossRefGoogle Scholar
Abdallah, J. et al. 1991 Phys. Rev. A 44, 4072.CrossRefGoogle Scholar
Bruneau, J. et al. 1990 Phys. Rev. Lett. 65, 1435.CrossRefGoogle Scholar
Bruneau, J. et al. 1991 Phys. Rev. A 44, R832.CrossRefGoogle Scholar
Chenais-Popovics, C. et al. 1989 Phys. Rev. A. 40, 3194.CrossRefGoogle Scholar
Chen, M.H. & Crasemann, B. 1987 Phys. Rev. A 35, 4579.CrossRefGoogle Scholar
Coldwell, R. & Bamford, G. 1991 The Theory and Operation of Spectral Analysis Using ROBFIT (American Institute of Physics, New York).Google Scholar
Cowan, R.D. 1981 The Theory of Atomic Structure and Spectra (University of California Press, Berkeley, CA).CrossRefGoogle Scholar
Davidson, S.J. et al. 1988 Appl. Phys. Lett. 52, 847.CrossRefGoogle Scholar
Foster, J.M. et al. 1991 Phys. Rev. Lett. 67, 3255.CrossRefGoogle Scholar
Griem, H. 1974 Spectral Line Broadening by Plasmas (Academic Press, New York).Google Scholar
Hauer, A. et al. 1986 Phys. Rev. A 34, 411.CrossRefGoogle Scholar
Kilcrease, D. 1991 Ph.D. thesis (University of Florida, Gainesville, FL).Google Scholar
Lee, Y.T. 1987 J. Quant. Spectrosc. Radial. Transfer 38, 131.CrossRefGoogle Scholar
Mancini, R.C. et al. 1991a In Radiative Properties of Hot Dense Matter, Goldstein, W., Hooper, C., Gauthier, J., Seely, J., and Lee, R., eds. (World Scientific, Singapore) pp. 82–90.Google Scholar
Mancini, R. et al. 1991b Comp. Phys. Comm. 63, 314.CrossRefGoogle Scholar
Perry, T.S. et al. 1991 Phys. Rev. Lett. 67, 3784.CrossRefGoogle Scholar
Woltz, L. & Hooper, C. 1988 Phys. Rev. A 38, 4766.CrossRefGoogle Scholar
Yaakobi, B. et al. 1980 Opt. Commun. 34, 213.CrossRefGoogle Scholar