Abstract
Energy levels and oscillator strengths (transition probabilities) have been calculated for transitions among 46 fine-structure levels of the (1s(2)) 2s(2) 2p(2), 2s2p(3),2p(4), 2s(2)2p3s, 2s(2) 2p3p and 2s(2)2p3d configurations of C-like K XIV, Sc XVI, Ti XVII, V XVIII, Cr XIX and Mn XX using the GRASP code. Configuration interaction and relativistic effects have been included while generating the wavefunctions. Calculated values of energy levels agree within 3% with the experimentally compiled results, and the length and velocity forms of oscillator strengths agree within 20% for a majority of allowed transitions.
Original language | English |
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Pages (from-to) | 377-383 |
Number of pages | 7 |
Journal | Astronomy and Astrophysics |
Volume | 401 |
Issue number | 1 |
Publication status | Published - Apr 2003 |
ASJC Scopus subject areas
- Space and Planetary Science