Astronomy and Astrophysics – Astrophysics
Scientific paper
Jan 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26as..141..285s&link_type=abstract
Astronomy and Astrophysics Supplement, v.141, p.285-296
Astronomy and Astrophysics
Astrophysics
25
Sun: Corona, Atomic Data, Uv Radiation
Scientific paper
We calculate collision strengths and thermally averaged collision strengths for electron excitation between the forty energetically lowest levels of Fe13+. The scattering calculation is more complete than any previous work on this ion and significant differences are found in the excitation rates for many of the extreme ultra-violet (EUV) transitions, compared to earlier work. A detailed comparison is made between predicted line intensity ratios and those observed in solar coronal spectra which shows that several outstanding discrepancies are resolved by the new atomic data.
Mason Harris E.
Storey Peter J.
Young Paul R.
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