Astronomy and Astrophysics – Astrophysics
Scientific paper
Apr 1999
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..136..385e&link_type=abstract
Astronomy and Astrophysics Supplement, v.136, p.385-394
Astronomy and Astrophysics
Astrophysics
16
Atomic And Molecular Data, Sun: Corona
Scientific paper
As part of the IRON Project, electron impact excitation effective collision strengths are computed for the ion Fe xvi familiar in solar spectra. A Breit-Pauli R-matrix calculation is performed with a 12-level (n<= 4) target representation. The calculation for this relatively simple ion is approached as a test case where we can analyze in detail most of the effects that contribute to the accuracy of the collision strengths: the energy mesh, relativistic corrections, the asymptotic multipole potentials and contributions from high partial waves. By comparing with two recent independent calculations, an accuracy rating of 10% is assigned to the present effective collision strengths in the electron-temperature range of 10(5<=) T/{K}<= 10(7) .
Eissner Werner
Galavis M. E.
Mendoza Carolina
Zeippen Claude J.
No associations
LandOfFree
Atomic data from the IRON Project. XXXIV. Electron impact excitation of Fe XVI does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Atomic data from the IRON Project. XXXIV. Electron impact excitation of Fe XVI, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Atomic data from the IRON Project. XXXIV. Electron impact excitation of Fe XVI will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1428607