1996
DOI: 10.1016/s0921-4526(96)00364-x
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On dense hydrogen and noble gases plasma spectra

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1996
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Cited by 7 publications
(7 citation statements)
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“…First of all, the extreme density lowers the ionization energy threshold and thus 'erases' the upper energy levels of atoms. This results in the absence of the H β and H γ lines, for example, along with an increase in continuum radiation [20,25]. These effects can only occur in non-ideal plasmas and can clearly be observed on our spectra, as mentioned earlier.…”
Section: Non-ideality Of the Plasmasupporting
confidence: 72%
See 1 more Smart Citation
“…First of all, the extreme density lowers the ionization energy threshold and thus 'erases' the upper energy levels of atoms. This results in the absence of the H β and H γ lines, for example, along with an increase in continuum radiation [20,25]. These effects can only occur in non-ideal plasmas and can clearly be observed on our spectra, as mentioned earlier.…”
Section: Non-ideality Of the Plasmasupporting
confidence: 72%
“…We hardly distinguish on figure 7(c) the H α line, two oxygen lines and two copper lines. Such extreme densities destroy the upper energy levels of the atoms, and the free-bound radiation becomes more important than line radiation [24,25]. As discussed in section 3.3, this is spectroscopic evidence that the plasma created during the earliest time of an EDM discharge is a non-ideal plasma.…”
Section: Time-integrated Emission Spectramentioning
confidence: 93%
“…This results in absence of the H ␤ and H ␥ lines, for example, along with an increase in continuum radiation [11,15]. These effects can only occur in non-ideal plasma and can clearly be observed on our spectra as said previously.…”
Section: Non-ideality Of the Plasmasupporting
confidence: 64%
“…5(c) the H ␣ line, two oxygen lines and two copper lines. Such extreme densities destroy the upper energy levels of the atoms, and the free-bound radiation becomes more important than line radiation [15]. As discussed in Section 3.3, this is spectroscopic evidence that the plasma created during the earliest time of an EDM discharge is a non-ideal plasma.…”
Section: Time-integrated Emission Spectramentioning
confidence: 94%
“…Specially, the present results can play useful role to improve our understanding about the evolution of stellar environments. We believe that our present results will encourage further studies in the experiments with the non‐ideal helium plasmas produced in flashlamps [44], helium atmospheric pressure plasma jet [45], penning plasma discharge [46], and so forth.…”
Section: Discussionmentioning
confidence: 83%