Astronomy and Astrophysics – Astrophysics
Scientific paper
May 1996
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...309..677s&link_type=abstract
Astronomy and Astrophysics, v.309, p.677-682
Astronomy and Astrophysics
Astrophysics
28
Atomic Data, Sun: Corona
Scientific paper
We calculate collision strengths and collision rates for electron excitation of the ^2^P^o^_1/2_-^2^P^o^_3/2_ ground term fine-structure transition in Fe xiv, the coronal green line at 5303A. The collision strength for the green line is found to be strongly enhanced by resonances for the first 4 Rydberg above the excitation threshold, and as a result the collision rates are found to be significantly larger than other recently published results, even at coronal temperatures. The calculations are carried out using the R-matrix formulation of the close-coupling approximation.
Mason Harris E.
Saraph Hannelore E.
Storey Peter J.
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