1975
DOI: 10.1070/qe1975v005n06abeh011298
|View full text |Cite
|
Sign up to set email alerts
|

Determination of plasma density from spectra of heliumlike ions

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
1
1
1
1

Citation Types

1
28
0

Year Published

1978
1978
2008
2008

Publication Types

Select...
5
3
1

Relationship

0
9

Authors

Journals

citations
Cited by 86 publications
(29 citation statements)
references
References 0 publications
1
28
0
Order By: Relevance
“…comm. !, Vinogradov et al 1975!,~2! a code based on relativistic many-body perturbation theory combined with complex rotation by Lindroth MBL; Tokman et al, 2002!, and~3!…”
Section: Atomic Datamentioning
confidence: 99%
“…comm. !, Vinogradov et al 1975!,~2! a code based on relativistic many-body perturbation theory combined with complex rotation by Lindroth MBL; Tokman et al, 2002!, and~3!…”
Section: Atomic Datamentioning
confidence: 99%
“…In order to provide an approximate description of the density dependence of the Kα radiative-emission spectra, we have introduced a hierarchy of simple statistical models [1] for the distribution of the population of the initial ions among the various low-lying fine-structure states. The additional collisional transitions among the autoionizing states, which can lead to strong density variations in dense laserproduced plasmas [16][17][18], have not been taken into account in our present Kα spectral simulations. The simple statistical models have been introduced in order to provide a convenient treatment for the multitude of the fine-structure components that must be taken into account.…”
Section: Fementioning
confidence: 98%
“…The spectral intensity of the radiative emission from the autoionizing states can then become a strong function of the electron density [16,17].…”
Section: Spectral Simulations For Kα α α α Emissionmentioning
confidence: 99%
“…Plasma parameters can be determined by the characteristic lines j, k, w, and y 16,17 . The electron temperature, T e , can be determined by the ratio (j+k)/w (the dielectric satellite lines to the resonance line) and the electron density, N e , can be determined by the ratio w/y (the resonance line to the recombination line) 11,12 .…”
Section: Analysis Of Recorded Spectramentioning
confidence: 99%