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Atoms 2014, 2(3), 357-377; doi:10.3390/atoms2030357

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.
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)
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Abstract

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
This is an open access article distributed under the Creative Commons Attribution License (CC BY 3.0).

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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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