| タイトル | Calculation of Atomic Data for NASA Missions |
| 本文（外部サイト） | http://hdl.handle.net/2060/20060052444 |
| 著者（英） | Dumitriu, I.; Manson, S. T.; Korista, K. T.; Nikolic, D.; Hasoglu, M. F.; Badnell, N. R.; Savin, D. W.; Fu, J.; Gorczyca, T. W. |
| 著者所属（英） | University of Western Michigan |
| 発行日 | 2006-08-01 |
| 言語 | eng |
| 内容記述 | The interpretation of cosmic spectra relies on a vast sea of atomic data which are not readily obtainable from analytic expressions or simple calculations. Rather, their evaluation typically requires state-of-the-art atomic physics calculations, with the inclusion of weaker effects (spin-orbit and configuration interactions, relaxation, Auger broadening, etc.), to achieve the level of accuracy needed for use by astrophysicists. Our NASA-supported research program is focused on calculating data for three important atomic processes, 1) dielectronic recombination (DR), 2) inner-shell photoabsorption, and 3) fluorescence and Auger decay of inner-shell vacancy states. Some additional details and examples of our recent findings are given. |
| NASA分類 | Astrophysics |
| 権利 | Copyright, Distribution as joint owner in the copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/565061 |
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