Astronomy and Astrophysics – Astrophysics
Scientific paper
Mar 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...447.1165a&link_type=abstract
Astronomy and Astrophysics, Volume 447, Issue 3, March I 2006, pp.1165-1174
Astronomy and Astrophysics
Astrophysics
28
Atomic Data, Atomic Processes
Scientific paper
Dielectronic recombination (DR) rate coefficients for 22 sodium-like ions, between Mg+ and Xe43+, forming magnesium-like ions have been calculated as part of the assembly of a level-resolved DR database necessary for modelling dynamic finite-density plasmas, within the generalized collisional-radiative framework. Calculations have been performed from both ground and metastable initial states, in both LS- and intermediate coupling, allowing for Δ n=0 and Δ n=1 core-excitations from ground and metastable levels. Partial and total DR coefficients have been calculated for Mg+ to Zn19+, as well as Kr25+, Mo31+, and Xe43+. Results for a selection of ions from the sequence are discussed in the paper and compared with existing theoretical and experimental results. A full set of results can be accessed from the Atomic Data and Analysis Structure (ADAS) database or from the Oak Ridge Controlled Fusion Atomic Data Center (http://www-cfadc.phy.ornl.gov/data_and_codes).
Altun Zikri
Badnell Nigel R.
Loch S. D.
Pindzola M. S.
Yumak A.
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