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Spectral-Kinetic Coupling and Effect of Microfield Rotation on Stark Broadening in Plasmas
Open AccessArticle

On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach

1
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia
2
Laboratoire d'Etude du Rayonnement et de la Matière en Astrophysique, Observatoire de Paris, UMR CNRS 8112, UPMC, 5 Place Jules Janssen, 92195 Meudon Cedex, France
*
Author to whom correspondence should be addressed.
Atoms 2014, 2(3), 357-377; https://doi.org/10.3390/atoms2030357
Received: 5 May 2014 / Revised: 20 June 2014 / Accepted: 16 July 2014 / Published: 7 August 2014
(This article belongs to the Special Issue Spectral Line Shapes in Plasmas)
The significance of Stark broadening data for problems in astrophysics, physics, as well as for technological plasmas is discussed and applications of Stark broadening parameters calculated using a semiclassical perturbation method are analyzed. View Full-Text
Keywords: Stark broadening; isolated lines; impact approximation Stark broadening; isolated lines; impact approximation
MDPI and ACS Style

Dimitrijević, M.S.; Sahal-Bréchot, S. On the Application of Stark Broadening Data Determined with a Semiclassical Perturbation Approach. Atoms 2014, 2, 357-377.

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