Issue |
A&A
Volume 511, February 2010
|
|
---|---|---|
Article Number | A78 | |
Number of page(s) | 10 | |
Section | Atomic, molecular, and nuclear data | |
DOI | https://doi.org/10.1051/0004-6361/200912689 | |
Published online | 12 March 2010 |
Atomic data from the IRON project*
LXVII. Electron impact excitation of Fe XIII
1
Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK e-mail: pjs@star.ucl.ac.uk
2
Observatoire de Paris, UMS 2201, CNRS/INSU, 61 avenue de l'Observatoire, 75014 Paris, France
Received:
12
June
2009
Accepted:
14
December
2009
A new R-matrix calculation of rate coefficients for electron collisional excitation of is presented and compared to recent calculations of comparable complexity. At temperatures at which Fe12+ is typically found in the solar corona, the present results, which use the intermediate coupling frame transformation method, show significant differences compared to some earlier work. We use a large configuration interaction calculation with extensive correlation to assess the accuracy of our and earlier workers' scattering targets.
Key words: atomic data / Sun: corona / techniques: spectroscopic
Full Tables 7 and 8 are only available in full in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/511/A78
© ESO, 2010
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