P. S. Barklem, S. D. Anstee, B. J. O'Mara, PASA, 15 (3), 336
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Conclusions
A program enabling easy interpolation of previously published line broadening data has been demonstrated by application to two lines in the solar spectrum. The source code for this program is available from the World Wide Web. The code is only applicable to lines originating from neutral atoms. We are currently investigating the application of the theory to lines originating from atoms in ionised states.
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