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Stark Width Regularities within Beryllium Spectral Series

Published online by Cambridge University Press:  02 January 2013

I. P. Dojčinović ,
I. Tapalaga  and
J. Purić
I. P. Dojčinović
Affiliation:
University of Belgrade, Faculty of Physics, PO Box 44, 11000 Belgrade, Serbia
I. Tapalaga*
Affiliation:
University of Belgrade, Faculty of Physics, PO Box 44, 11000 Belgrade, Serbia
J. Purić
Affiliation:
University of Belgrade, Faculty of Physics, PO Box 44, 11000 Belgrade, Serbia
*
BCorresponding author. Email: irinelko@gmail.com
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Abstract

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The dependences of Stark width on the upper-level ionization potential within different series of the neutral beryllium spectral lines have been studied. The dependences previously observed for electron impact contribution to the Stark widths were also obtained for the proton impact contribution. The emphasis is on the fine structure influence on the studied Stark parameter dependences. The influence of temperature on the dependences of Stark width parameters has been demonstrated. The relations found can be used in both cases for prediction of new Stark broadening data, thus avoiding much more complicated procedures.

Keywords

atomic dataline: profilesopacityplasmasradiative transfer
Type
Research Article
Information
Publications of the Astronomical Society of Australia , Volume 28 , Issue 4 , 2011 , pp. 281 - 289
Copyright
Copyright © Astronomical Society of Australia 2011

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