Collision strengths for electron excitation of highly ionized, complex atoms
- 1 May 1971
- journal article
- Published by IOP Publishing in Journal of Physics B: Atomic and Molecular Physics
- Vol. 4 (5) , 697-705
- https://doi.org/10.1088/0022-3700/4/5/012
Abstract
Using atomic structure and atomic collision programs developed, respectively, by Eissner and Nussbaumer (1969, 1970) and Eissner (1970), collision strengths have been computed for transitions, produced by electron impact, between terms of the following configurations of the following ions: N V, Si XII: 1s22s, 2p, 3s, 3p, 3d; Fe XIII: 3s2 3p2, 3s 3p3, 3s2 3p 3d; Fe XIV: 3s2 3p, 3s 3p2, 3s2 3d; Fe XV: 3s2, 3s 3p, 3p2, 3s 3d; Fe XVII: 2p6, 2p5 3s, 3p, 3d. The calculations are in a configuration interaction representation and in LS coupling. The collision problem is solved by the distorted wave approximation and the results obtained are found to be in good agreement with the results of close coupling calculations, where such a comparison can be made.Keywords
This publication has 16 references indexed in Scilit:
- Laboratory measurements of excitation coefficients for five transitions in nitrogen VJournal of Physics B: Atomic and Molecular Physics, 1970
- Excitation of semi-forbidden 2s21S-2s2p3P lines observed in quasars and nebulaeJournal of Physics B: Atomic and Molecular Physics, 1970
- The excitation of the forbidden coronal linesSolar Physics, 1969
- A programme for calculating atomic structuresJournal of Physics B: Atomic and Molecular Physics, 1969
- Emission of FeXV in coronal conditionsSolar Physics, 1968
- The X-Ray Emission Spectrum of a Solar Active RegionThe Astrophysical Journal, 1968
- Excitation of forbidden lines: Calculations for the 2p3, 2p4, 3p2and 3p4isoelectronic sequencesProceedings of the Physical Society, 1967
- The excitation of Fe XVII by electron impactsSolar Physics, 1967
- The Abundance of Iron in the Solar CoronaMonthly Notices of the Royal Astronomical Society, 1966
- Excitation of N V by electron impactProceedings of the Physical Society, 1966