Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...376..803b&link_type=abstract
Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 376, Aug. 1, 1991, p. 803-808. Research supported by SERC.
Astronomy and Astrophysics
Astrophysics
9
Electron Transitions, Solar Spectra, Ultraviolet Spectra, Atomic Energy Levels, Magnesium, Solar Corona, Atomic Processes
Scientific paper
Using the programs RMATRX and DSTWAV, which are based, respectively, on the close coupling and distorted wave approximations, we compute and compare partial collision strengths for the optically allowed transitions between the 2s22p2 and 2s2p3 configurations of Mg+6. From this investigation we conclude that the differences between the published results of Mason and Bhatia (DSTWAV) and Aggarwal (RMATRX) arise not simply because they used different target wave functions, but also because the method used by Aggarwal for treating the outer region in his close coupling calculation is inadequate for optically allowed transitions.
Burgess Andrew
Mason Harris E.
Tully John A.
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