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On the Stark Broadening of Be II Spectral Lines

Author

Listed:
  • Milan S. Dimitrijević

    (Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia
    Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-92190 Meudon, France)

  • Magdalena Christova

    (Department of Applied Physics, Technical University–Sofia, 1000 Sofia, Bulgaria)

  • Sylvie Sahal-Bréchot

    (Sorbonne Université, Observatoire de Paris, Université PSL, CNRS, LERMA, F-92190 Meudon, France)

Abstract

Calculated Stark broadening parameters of singly ionized beryllium spectral lines have been reported. Three spectral series have been studied within semiclassical perturbation theory. The plasma conditions cover temperatures from 2500 to 50,000 K and perturber densities 10 11 cm −3 and 10 13 cm −3 . The influence of the temperature and the role of the perturbers (electrons, protons and He + ions) on the Stark width and shift have been discussed. Results could be useful for plasma diagnostics in astrophysics, laboratory, and industrial plasmas.

Suggested Citation

  • Milan S. Dimitrijević & Magdalena Christova & Sylvie Sahal-Bréchot, 2020. "On the Stark Broadening of Be II Spectral Lines," Data, MDPI, vol. 5(4), pages 1-7, November.
    • Handle: RePEc:gam:jdataj:v:5:y:2020:i:4:p:106-:d:449365
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