Energy levels and oscillator strengths (transition probabilities) have been
calculated for the fine-structure transitions among the levels of the (1s(
2)) 2s(2)2p(2), 2s2p(3), 2p(4), 2s(2)2p3s, 2s(2)2p3p, and 2s(2)2p3d configu
rations of C-like F IV, Na VI, Al VIII, P X, Cl XII, and Ar XIII using the
CIV3 program. The extensive configuration interaction and relativistic effe
cts have been included while generating the wavefunctions. Calculated value
s of energy levels generally agree within 5% with the experimentally compil
ed results, and the length and velocity forms of oscillator strengths agree
within 20% for a majority of allowed transitions.