R-matrix electron-impact excitation data for the Mg-like iso-electronic sequence
Fernández-Menchero, L. and Del Zanna, G. and Badnell, N. R. (2014) R-matrix electron-impact excitation data for the Mg-like iso-electronic sequence. Astronomy and Astrophysics, 572. A115. ISSN 0004-6361 (https://doi.org/10.1051/0004-6361/201424849)
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Abstract
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. 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. 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.
ORCID iDs
Fernández-Menchero, L., Del Zanna, G. and Badnell, N. R. ORCID: https://orcid.org/0000-0001-7418-7996;-
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Item type: Article ID code: 54182 Dates: DateEvent5 December 2014Published18 September 2014AcceptedSubjects: Science > Physics Department: Faculty of Science > Physics Depositing user: Pure Administrator Date deposited: 08 Sep 2015 07:52 Last modified: 11 Nov 2024 11:10 URI: https://strathprints.strath.ac.uk/id/eprint/54182