Effects of ion dynamics and opacity on stark-broadened argon line profiles

Physical Review E - Statistical Physics, Plasmas, Fluids, and Related Interdisciplinary Topics

Volumn 53, Issue 1, 1996, Pages 1042-1050

  Haynes, D A ^a   Garber, D T ^a   Hooper, C F ^a   Mancini, R C ^b   Lee, Y T ^c   Bradley, D K ^d   Delettrez, J ^d   Epstein, R ^d   Jaanimagi, P A ^d  

^a University of Florida ^*  (United States)

^b UNIVERSITY OF NEVADA   (United States)

^c LAWRENCE LIVERMORE NATIONAL LABORATORY   (United States)

^d UNIVERSITY OF ROCHESTER   (United States)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0000469223     PISSN: 1063651X     EISSN: None     Source Type: Journal    
DOI: 10.1103/PhysRevE.53.1042     Document Type: Article

References (22)

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12. Only the imaginary part of M( Δ ω ), that part leading to electron broadening is included in our calculation. Although shifts due to the radiator-plasma electron interaction have received considerable theoretical attention [see, e.g., H. R. Griem , Phys. Rev. A 41, 5600 (1990);
13. M. Koenig , Phys. Rev. A 38, 2089 (1988);
14. J. Cooper in Radiative Properties of Hot Dense Matter, edited by J. Davis (World Scientific, Singapore, 1985)], we have found no compelling experimental evidence in our data of overall shifts due to this interaction, nor of additional modification of the line shape due to differential shifting of individual components. Thus we have not yet included this part of the radiator-plasma electron interaction in our calculations.
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