Issue |
A&A
Volume 572, December 2014
|
|
---|---|---|
Article Number | A115 | |
Number of page(s) | 10 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361/201424849 | |
Published online | 05 December 2014 |
R-matrix electron-impact excitation data for the Mg-like iso-electronic sequence⋆
1 Department of Physics, University of Strathclyde. Glasgow G4 0NG, UK
e-mail: luis.fernandez-menchero@strath.ac.uk
2 Department of Applied Mathematics and Theoretical Physics, University of Cambridge, Cambridge CB3 0WA, UK
Received: 22 August 2014
Accepted: 18 September 2014
Aims. Emission lines from ions in the Mg-like iso-electronic sequence can be used as reliable diagnostics of temperature and density of astrophysical and fusion plasmas over a wide range of parameters. Data in the literature are quite lacking, there are no calculations for many of the ions in the sequence.
Methods. We have carried-out intermediate coupling frame transformation R-matrix calculations which include a total of 283 fine-structure levels in both the configuration interaction target and close-coupling collision expansions. These arise from the configurations 1s2 2s2 2p6 3 {s,p,d} nl with n = 4,5, and for l = 0−4.
Results. We obtain ordinary collision strengths and Maxwell-averaged effective collision strengths for the electron-impact excitation of all the ions of the Mg-like sequence, from Al+ to Zn18 +. We compare our results with those from previous R-matrix and distorted waves calculations, where available, for some benchmark ions. We find good agreement with the results of previous calculations for the transitions n = 3−3. We also find good agreement for the most intense transitions n = 3−4. These transitions are important for populating the upper levels of the main diagnostic lines.
Key words: atomic data / techniques: spectroscopic
These data are made available in the APAP archive via http://www.apap-network.org, CHIANTI via http://www.chiantidatabase.org and open-ADAS via http://open.adas.ac.uk
© ESO, 2014
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