Energy Levels, Radiative Rates, and Collision Strengths for Transitions in Fe XVII

Details Energy Levels, Radiative Rates, and Collision Strengths for Transitions in Fe XVII Energy Levels, Radiative Rates, and Collision Strengths for Transitions in Fe XVII

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003apjs..144..169a&link_type=abstract

The Astrophysical Journal Supplement Series, Volume 144, Issue 1, pp. 169-210.

Astronomy and Astrophysics

Astronomy

13

Atomic Data, Plasmas

Scientific paper

Energy levels and radiative rates have been calculated for fine-structure transitions among the lowest 89 levels of the (1s2) 2s22p6, 2s22p53l, 2s22p54l, 2s2p63l, and 2s2p64l configurations of Fe XVII, using the GRASP code of Dyall et al. Collision strengths have also been calculated, for transitions among the lowest 55 levels, using the recently developed Dirac atomic R-matrix code (DARC) of Norrington & Grant. The results are compared with those available in the literature, and the accuracy of the data is assessed.

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