All Tables

Table 1: The Hartree-Fock orbital parameters (c, I, $\zeta$ ) of the radial wavefunctions for the 1s, 2s, 3s and 2p orbitals.
Table 2: The optimised c, I and $\zeta$ parameters of the non-Hartree-Fock orbitals.
Table 3: Energy levels in Rydbergs for the 14 LS target states included in the calculation, relative to the S V 2p⁶3s² ¹S $^{\rm e}$ ground state. Values are shown for the experimental data of NIST along with the values obtained from the current calculation, as well as data from the calculations of the Opacity Project (Butler et al. 1992)[OP], Christensen et al.(1986)[C et al.] and Dufton & Kingston (1984)[D&K]. The differences between the observed values of NIST and the data from each of the three calculations are given in parentheses.
Table 4: Oscillator strengths for the allowed transitions between the 14 LS target states included in the current calculation. Values are given for the length and velocity forms of the oscillator strength (f_l and f_v) and are compared, where available, to values from the Opacity Project (Butler et al. 1992)[OP], Gupta & Msezane (2000)[G&M] and Christensen et al. (1986)[C et al.]
Table 5: J-levels.
Table 6: Effective collision strengths for the fine structure transitions from the 3s² ¹S₀ ground state to levels 2-14 of S V, for electron temperatures ranging from $\log_{10} T_{\rm e}({\rm K}) = 4.0$ to 6.0 in steps of 0.2 dex. A superscript indicates the power of 10 with which the number must be multiplied i.e., $a^{-n}=a \times 10^{-n}$ , i and j denote the initial and final levels of the transition (see Table 5).