Issue 
A&A
Volume 494, Number 2, February I 2009



Page(s)  729  737  
Section  Atomic, molecular, and nuclear data  
DOI  https://doi.org/10.1051/00046361:200809788  
Published online  11 December 2008 
BreitPauli Rmatrix calculation of finestructure effective collision strengths for the electron impact excitation of Mg V^{}
C. E. Hudson  C. A. Ramsbottom  P. H. Norrington  M. P. Scott
School of Mathematics and Physics, The Queens University of Belfast, Belfast BT7 1NN, Northern Ireland, UK
Received 17 March 2008 / Accepted 13 November 2008
Abstract
Context. Electronimpact excitation collision strengths are required for the analysis and interpretation of stellar observations.
Aims. This calculation aims to provide effective collision strengths for the Mg V ion for a larger number of transitions and for a greater temperature range than previously available, using collision strength data that include contributions from resonances.
Methods. A 19state BreitPauli Rmatrix calculation was performed. The target states are represented by configuration interaction wavefunctions and consist of the 19 lowest LS states, having configurations 2s^{2}2p^{4}, 2s2p^{5}, 2p^{6}, 2s^{2}2p^{3}3s, and 2s^{2}2p^{3}3p. These target states give rise to 37 finestructure levels and 666 possible transitions. The effective collision strengths were calculated by averaging the electron collision strengths over a Maxwellian distribution of electron velocities.
Results. The nonzero effective collision strengths for transitions between the finestructure levels are given for electron temperatures ()
in the range
.
Data for transitions among the 5 finestructure levels arising from the 2s^{2}2p^{4} ground state configurations, seen in the UV range, are discussed in the paper, along with transitions in the EUV range  transitions from the ground state ^{3}P levels to 2s2p^{5} ^{3}P
levels. The 2s^{2}2p^{4} ^{1}D2s2p^{5} ^{1}P transition is also noted. Data for the remaining transitions are available at the CDS.
Key words: atomic processes  line: formation  methods: analytical
1 Introduction
Recently, highionisation forbidden lines from Mg V were found in Hubble Space Telescope STIS ultraviolet spectra of the symbiotic star AG Draconis (Young et al. 2006). Here, Young et al. use the density and temperature sensitive pair of lines 2s^{2}2p^{4} ^{3}P_{1}2s^{2}2p^{4} ^{1}S_{0} and 2s^{2}2p^{4} ^{3}P_{2}2s^{2}2p^{4} ^{1}D_{2} (occurring at 1324 and 2782 Å in the UV range, respectively) as a diagnostic. In the EUV range, the 2s^{2}2p^{4} ^{1}D_{2}2s2p^{5} ^{1}P emission line at 276.58 Å has been observed using the EIS instrument onboard Hinode (Young et al. 2007a). Young et al. (2007b) note that this line gives valuable temperature information.
Observational data such as these require atomic data in the form of effective collision strengths for analysis and interpretation. Two previous closecoupling calculations have been carried out but were limited to data for a handful of transitions. The work of Mendoza & Zeippen (1987) was a sixstate calculation with LScoupled collision strengths calculated using the IMPACT (Crees et al. 1978) code. The LScoupled reactance matrices were adapted to intermediate coupling by algebraic transformations neglecting relativistic effects and finestructure energy splittings using the JAJOM (Saraph 1972,1978) program. This calculation determined effective collision strengths for the 3 finestructure transitions within the ground state 2p^{4} ^{3}P_{J} levels and for the 3 LS transitions between the 2p^{4} ^{3}P, ^{1}D and ^{1}P levels. The Rmatrix calculation of Butler & Zeippen (1994) was also a sixstate calculation carried out in LScoupling with the Kmatrices being transformed, and here values are given for the 10 finestructure transitions arising from the 2p^{4} ^{3}P_{J}, ^{1}D and ^{1}S levels. However, neither of these calculations gives data for the EUV lines, in particular the line at 276 Å observed by Hinode.
The more recent work of Bhatia et al. (2006) calculated collision strengths in the Distorted Wave approximation. In this calculation 44 LS states were employed which gives rise to 86 jlevels and a total of 3655 transitions. However, the Distorted Wave approximation does not take into account contributions from the resonances, and so the collision strengths are less accurate. Therefore, these authors have used the results of Butler & Zeippen (1994) for the transitions within the ground configuration to complement their data. However, Butler & Zeippen (1994) only provide data for temperatures up to 10^{5} K and so in their paper Bhatia et al. (2006) call for a new closecoupling calculation to provide values for the 10^{5}10^{6} K range, since Mg V lines are formed in plasmas at these temperatures.
Therefore to provide accurate collisional data for this ion we have carried out a sophisticated BreitPauli Rmatrix calculation. Such calculations are carried out in intermediate coupling and hence using a transformation such as JAJOM is no longer required and the collision strengths become more accurate in the resonance region. This calculation was performed with 19 LS target states (including levels up to 2s^{2}2p^{3}(^{2}D)3p ^{3}P) which give rise to 37 jlevels, and a total of 666 possible finestructure transitions. The effective collision strengths have been determined for electron temperatures in the range . We present some of these values in this paper, with the remainder being tabulated at the CDS website.
2 Calculation details
Configuration interaction wavefunctions for the 19 LS target states used in this calculation were constructed using the CIV3 code of Hibbert (1975). Each targetstate wavefunction
is represented by a linear combination of singleconfiguration functions ,
each of which has the same total
symmetry as the targetstate
The in (1) are constructed from a set of oneelectron orbitals. The represent the coupling of the angular momenta associated with these oneelectron spin orbitals to form the total L and S. The mixing coefficients a_{i} are determined by the CIV3 code and are eigenvector components of the Hamiltonian matrix having particular LS symmetry. The Hamiltonian matrix elements are defined as
(2) 
where H denotes the Hamiltonian operator. The oneelectron orbitals used to construct the each consist of a radial function, a spherical harmonic and a spin function:
(3) 
These orbitals are chosen to be analytic, with the radial part being expressed as a sum of Slatertype orbitals:
(4) 
In this expression, for each orbital, the powers of r (I_{jnl}) are kept fixed and the coefficients c_{jnl} and exponents are treated as variational parameters which are optimised by the CIV3 code. For this calculation the 19 LS states included as the target states are: 2s^{2}2p^{4} ^{3}P, ^{1}D, ^{1}S; 2s2p^{5} ^{3}P, ^{1}P; 2p^{6} ^{1}S; 2s^{2}2p^{3}3s ^{5}S, ^{3}S, ^{3}D, ^{1}D, ^{3}P, ^{1}P and 2s^{2}2p^{3}3p ^{5}P, ^{3}P , ^{1}P, ^{3}D, ^{3}F, ^{1}F.
In describing these target states () we employed eight oneelectron orbitals, including five real orbitals  1s, 2s, 2p, 3s, 3p and to these we added three pseudoorbitals  a orbital which corrects for the differing orbital in the 2s2p^{5} and 2s^{2}2p^{3}nl configurations; a orbital which corrects for the 2p orbital differing from the 2s2p^{5} configuration; and a orbital which allows for coupling between 2s2p^{5}2s^{2}2p^{3}nd. The states used in the orbital optimisations are given in Table 1, and the resulting orbital parameters are shown in Table 2.
Table 1: Orbital optimisations.
Table 2: Orbital parameters (c, I, ) of the radial wavefunctions.
Table 3: Distribution of configurations for each symmetry in the two versions of the calculation.
The orbitals from Table 2 were used to build a set of singleconfiguration functions (), which were generated by a two electron replacement on the 1s^{2}2s^{2}2p^{4} basis configuration, with the 1s shell being kept closed, and allowing at most only one of the pseudoorbitals to be occupied. Using the 14 symmetries involved in the target state set, this generation leads to a total of 1044 configurations. A larger set of configurations was also employed for comparison at this stage, but due to memory constraints within the collision calculation only the smaller set was retained for the remainder of the calculation. This larger set utilised the same orbitals and the configurations were generated in the same manner but the restriction of only allowing one pseudoorbital to be occupied was removed. This leads to 1350 configurations being produced. The distribution of configurations between the 14 symmetries is shown in Table 3.
Wavefunctions () for the 19 Mg V target states are constructed as linear combinations of these singleconfiguration functions () according to Eq. (1). In Table 4 we show the target state energies calculated from these wavefunctions (noted as ``This work:1044'' in the table). The energies calculated for the target states using the larger set of configurations are also noted in Table 4 as ``This work:1350''.
Table 4 compares the calculated LS target state energies in Rydbergs (1 Ryd = 2.17987 J) relative to the 2s^{2}2p^{4} ^{3}P ground state with values from NIST. The NIST database is available at http://www.physics.nist.gov/PhysRefData and the data for this ion is attributed to Artru & Kaufman (1979), Edlen (1964), Fawcett et al. (1974), Guennou et al. (1979), Johannesson et al. (1972) and Soderqvist (1934,1946). From Table 4, we find that using our smaller set of configurations (1044, instead of 1350) gives slightly better energy levels, when compared to the values of NIST.
As an additional check on the quality of the wavefunctions for the target states, we also examine the oscillator strengths produced using the wavefunctions generated. Oscillator strengths for the allowed transitions between the 19 LS target states are given in Table 5. We show values obtained using both our configuration sets  the larger set of 1350 and the smaller set of 1044 which was retained for the scattering calculation. Comparisons are made with Tachiev & Froese Fischer (2002) and we have averaged over the finestructure oscillator strengths of Tachiev & Froese Fischer (2002) to compare with our LS values.
For the transitions noted in Table 5, on the whole, there is not much difference between the values for the larger calculation (1350 configurations) and the smaller calculation (1044 configurations). In both calculations the agreement between the length and velocity forms of the oscillator strengths is quite reasonable, and it is only for the very small oscillator strengths that larger differences are seen. The values from the current work also compare well with those of Tachiev & Froese Fischer (2002). This analysis of the energy levels and oscillator strengths generated using the constructed target state wavefunctions from the smaller calculation leads us to be confident that we have an accurate representation of the target system.
Table 4: Target state energies for our two configuration sets (1350 and 1044) compared to available NIST data.
Table 5: Oscillator strengths for the allowed transitions, in both length and velocity forms (f_{l} and f_{v}) for our two configuration sets (1350 and 1044), compared to Tachiev & Froese Fischer (2002)[T&F].
Table 6: Finestructure energy levels for the current calculation compared to the earlier works of Bhatia et al. (2006), Tachiev & Froese Fischer (2002) [T&F] and Butler & Zeippen (1994) [B&Z], along with the observed values from NIST.
Table 7: Effective Collision Strengths for transitions between the first 5 jlevels of Mg V at selected temperatures^{a}.
Using these wavefunctions for the Mg V target ion, the electronion collision problem was investigated using the BreitPauli Rmatrix method (Scott & Burke 1980), employing the RMATRX1 codes of Berrington et al. (Berrington et al. 1987). The version of the codes used here are the serial version available at http://amdpp.phys.strath.ac.uk/tamoc/code.html. The Rmatrix radius was calculated to be 7.0 atomic units and for each orbital angular momentum, 17 Schmidtorthogonalised continuum orbitals were included, ensuring that a converged collision strength was obtained up to an incident electron energy of 28 Rydbergs (1 Ryd = J).
The (N+1)electron bound configurations, which are included in the expansion of the (N+1)electron collision wavefunction to describe the situation when the scattering electron comes close into the target ion were obtained by systematically adding one electron to the Nelectron configurations used in the description of the target Mg V ion.
The current 19 LS state calculation was carried out for all contributing partial waves with . Within the BreitPauli framework this gives rise to a 37 finestructure level problem for partial waves up to 2J=29 (J=L+S), for both even and odd parity. For optically forbidden transitions, this is sufficient to obtain converged results. However, for optically allowed transitions, additional partial waves or a topup procedure is required. In this case, our calculation was supplemented by a nonexchange calculation for partial waves up to L=40 (in terms of Jvalue this allows access up to 2J=85). The ICFT method (as discussed by Griffin et al. 1998) was then used to generate the intermediatecoupling results and finally topup was used to account for contributions from any higher partial waves (i.e. L>40).
Effective collision strengths
for electron temperatures
(in K) were obtained by averaging the electron collision strengths
over a Maxwellian distribution of velocities, so that
(5) 
where is the final free electron energy after excitation and k is Boltzmann's constant.
3 Results and discussion
The collision strengths calculated in this work have been evaluated for a fine mesh of incident impact energies, at energy intervals of 0.0008 Rydbergs (0.00005 in zscaled Rydbergs) across the energy range from threshold up to the energy of the last target state considered. This ensured that the autoionising resonances which converge to the target state thresholds were fully delineated.
Those resonances located at energies lower than the highest target threshold, i.e. 2s^{2}2p^{3}(^{2}D)3p ^{3}P at 7.4 Ryd, are physically meaningful; however at higher energies pseudoresonances appear. These arise from the inclusion of pseudoorbitals in the wavefunction expansion (Burke et al. 1981). At higher temperatures the highimpact energy region is much more important and so it is necessary to properly average over the pseudoresonances to prevent distortion of the correct results in the calculation of the effective collision strengths. Thus above the last target state energy, a coarser mesh of energies is used (0.002 in zscaled Rydbergs). Much of the detail is filtered out and any very large pseudoresonances are removed, so that in essence a ``background'' level is retained in this region. This is achieved by a scheme which compares each collision strength point in the high energy/pseudoresonance region with its neighbour on either side, and if it is larger than either neighbour by a certain factor, the collision strength at that point is reset to be the smaller of the two neighbours. In this calculation successively smaller factors were used (e.g. 10% difference, 5%, 1%, 0.1% and 0.01%) until the results converged.
The inclusion of the 19 LS target states leads to 37 Jlevels (see Table 6) and a total of 666 transitions. The finestructure energies obtained for these Jlevels are also shown in Table 6 and are compared to values from Bhatia et al. (2006), NIST and Butler & Zeippen (1994), as well as values from the extensive MCHF+BP calculation of Tachiev & Froese Fischer (2002). Although the list of levels available from NIST is limited, we find that calculation of Tachiev & Froese Fischer (2002) achieves the best agreement with these observed values, the agreement being to within 1%. Of the three other calculations the current work agrees best with Tachiev & Froese Fischer (2002)  all the values are within 4%, with 35 of the 39 levels being within 1% of the Tachiev & Froese Fischer (2002) values. The Bhatia et al. (2006) values are found to differ by up to 8% from those of Tachiev & Froese Fischer (2002) (with 4 values agreeing to within 1% and 27 values agreeing to within 2%). The Butler & Zeippen (1994) values lie within 6% of both the NIST and Tachiev & Froese Fischer (2002) values. Thus since the Tachiev & Froese Fischer (2002) energy levels are so close to the NIST values and since in turn the current work is in such good agreement with the Tachiev & Froese Fischer (2002) values for the 39 levels considered, we are confident that we have achieved a good representation of the target.
In Table 7 we present the effective collision strengths for 10 of these transitions, namely those between the first 5 Jlevels arising from the first 3 LS targets  the 2p^{4} ground configurations. The data are given for a range of electron temperatures [ (K) = 3.07.0, in steps of 0.2 dex] suitable for application in plasma and astronomical diagnostics. These transitions are also plotted in Fig. 1, for the temperature range 6.0, and are compared to the values from Bhatia et al. (2006) and Butler & Zeippen (1994).
We find that our results are generally in good agreement with both the earlier Rmatrix work of Butler & Zeippen (1994) and also the Distorted Wave approximation data of Bhatia et al. (2006), although it should be noted that for all the transitions in Fig. 1, Bhatia et al. (2006) merged their Distorted Wave results with the Rmatrix results of Butler & Zeippen (1994). For the most part however, our results are slightly higher than the other two calculations. Focusing on the pair of lines used as a diagnostic by Young et al. (2006), i.e. 2s^{2}2p^{4} ^{3}P_{1}2s^{2}2p^{4} ^{1}S_{0} and 2s^{2}2p^{4} ^{3}P_{2}2s^{2}2p^{4} ^{1}D_{2} occurring at 1324 and 2782 Å in the UV range, these are transitions 25 and 14 respectively using the current system of labelling (see Table 6). For transition 25, the current calculation is up to 25% higher than the calculation of Bhatia et al. (2006), while for transition 14, we find that for lower temperatures ( ) the current work is up to 10% lower than Bhatia et al. (2006) and for higher temperatures ( ) the current work is up to 12% higher.
The high temperature behaviour for transition 45, i.e. 2s^{2}2p^{4} ^{1}D_{2}2s^{2}2p^{4} ^{1}S_{0}, differs significantly between Bhatia et al. (2006) and the current work, with the Bhatia et al. (2006) values falling off much more sharply than the current values. Since the Bhatia et al. (2006) values for this transition are their Distorted Wave results merged with the Butler & Zeippen (1994) Rmatrix data, it could be that the pure Distorted Wave results give an effective collision strength which is relatively low but when merged with the Butler & Zeippen (1994) Rmatrix data (which was produced in the range ) gives rise to a large enhancement at the upper end of this region near . Beyond this one assumes the sharp drop is because the values connect back to the possibly low pure Distorted Wave results. Certainly when the collision strength from the current calculation is examined and compared to the values presented in Bhatia et al. (2006), the Distorted Wave values are lower than the background level of the Rmatrix results by about 40 per cent at the high energy extremity and so this suggests that the Distorted Wave effective collision strength results should be in the region of about 40 per cent lower than the current work, which does seem to be the case at .
In Figure 2, we plot some transitions which appear in the EUV range. These involve initial levels 1, 2 and 3, and final levels 6, 7 and 8, and occur at 350 Å. Also plotted on the same figure, is transition 49, which is the line recently seen by Hinode, i.e. the 2s^{2}2p^{4} ^{1}D_{2}2s2p^{5} ^{1}P emission line at 276.58 Å. The transitions 1, 2, 36, 7, 8 are from the ground 2s^{2}2p^{4} ^{3}P_{0,1,2} levels to the 2s2p^{5} ^{3}P levels. We find that in all cases, except one (transition 36), the Distorted Wave values are higher than the those of the current Rmatrix calculation.
For the graphs plotted in Fig. 2, where the Distorted wave is larger than the Rmatrix values, we see differences of up to almost 40%. For transition 36, i.e. 2s^{2}2p^{4} ^{3}P_{0}2s2p^{5} ^{3}P , the Rmatrix results are larger by almost a factor of two in the lower temperature region, and the two calculations converge at the upper temperature extremity. For transition 49, i.e. 2s^{2}2p^{4} ^{1}D_{2}2s2p^{5} ^{1}P which is seen by Hinode at 276.58 Å, the Distorted Wave values are larger by 13%.
Figure 1: Effective collision strengths as a function of electron temperature (in Kelvin) for transitions within the ground state configurations (levels 15). Solid line: current Rmatrix calculation, Crosses: Butler & Zeippen (1994) 6state Rmatrix calculation, Dashed line: Bhatia et al. (2006) (Distorted Wave calculation merged with Butler & Zeippen 1994). Transitions marked * have been recently observed in AG Draconis (Young et al. 2006). 

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Figure 2: Effective collision strengths as a function of electron temperature (in Kelvin) for transitions between initial levels 1, 2 and 3 and final levels 6, 7 and 8 and transition 49. Solid line: current Rmatrix calculation, Dashed line: Bhatia et al. (2006, Distorted Wave results). Transition marked * has been recently observed by Hinode (Young et al. 2007a). 

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As a sample of the detail obtained from the current work and an indication of what may cause the differences in the effective collision strengths between the current work and the Distorted wave calculation, Fig. 3 shows collision strengths for three of the transitions given in Fig. 2. These are: transitions 28, 36 and 45 (i.e. 2s^{2}2p^{4} ^{3}P_{1}2s2p^{5} ^{3}P , 2s^{2}2p^{4} ^{3}P_{0}2s2p^{5} ^{3}P and 2s^{2}2p^{4} ^{1}D_{2}2s^{2}2p^{4} ^{1}S_{0}).
For transition 28, 2s^{2}2p^{4} ^{3}P_{1}2s2p^{5} ^{3}P , we see that in the high energy region, the two calculations achieve the same level, but towards low energy the Distorted Wave values may be higher than the Rmatrix values. This enhancement at lower energies results in the effective collision strength being raised in the low temperature region by almost 25%, but at the high temperature extremity this difference is about 10% corresponding to the better agreement in the high energy region of the collision strength.
For transition 36, 2s^{2}2p^{4} ^{3}P_{0}2s2p^{5} ^{3}P , there is a large resonance near threshold for the collision strength and this greatly enhances the effective collision strength for this transition in Fig. 2. For the remainder of the transitions shown in Fig. 2, the discrepancies observed between the Distorted Wave values and the current Rmatrix calculation can be explained in a fashion similar to the discussion of transition 28, i.e., we find that for these transitions, the collision strength values from the current work have a lower background level than the Distorted Wave calculation, and this in turn produces a lowered effective collision strength.
Transition 45, 2s^{2}2p^{4} ^{1}D_{2}2s^{2}2p^{4} ^{1}S_{0}, has been discussed above, and is given to show that despite good agreement in the behaviour of the high energy backround level of the collision strengths, that the differing behaviour in the effective collision strengths in Fig. 1 is most likely due to the merging of the Distorted Wave results of Bhatia et al. (2006) with the earlier Rmatrix results of Butler & Zeippen (1994).
Figure 3: Collision strengths as a function of incident electron energy in Rydbergs for transitions 28, 36 and 45. Solid line  Current Rmatrix calculation, Circles  Bhatia et al. (2006, Distorted Wave). 

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Table 8, available at CDS, gives the nonzero finestructure effective collision strength data for the 666 transitionsconsidered and contains the following information: Col. 1 lists the transition index noted as ij (initialfinal level) where the levels are given in the accompanying table and correspond to those in Table 6. For example, 25 denotes the transition 2s^{2}2p^{4} ^{3}P_{1}2s^{2}2p^{4} ^{1}S_{0}. The remaining columns list the effective collision strengths for each transition at logarithmic electron temperatures (K) = 3.07.0 in steps of 0.1 dex.
4 Conclusions
In this paper we present effective collision strengths for the electron impact excitation of the Mg V ion. The atomic data are evaluated for the electron temperature range (K) = 3.07.0 and for all transitions among the lowest 19 LS states of Mg V, corresponding to 37 finestructure levels and 666 individual finestructure transitions. Whilst the overall accuracy is difficult to assess, we expect the current data to have an accuracy of 10%.
The effective collision strengths are available at the CDS or alternatively all the collision strength and effective collision strength data over the temperature range (K) = 3.07.0 (in steps of 0.1 dex) are available, by contacting the author or via the website http://www.am.qub.ac.uk/apa/data.
Acknowledgements
This work has been supported by PPARC, under the auspices of a Rolling Grant. C.E.H. wishes to thank E. Landi for assistance in obtaining data from Bhatia et al. (2006).
References
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 Berrington, K. A., Burke, P. G., Butler, K., et al. 1987, J. Phys. B, 20, 6379 [NASA ADS] [CrossRef] (In the text)
 Bhatia, A. K., Landi, E., & Eissner, W. 2006, Atomic Data and Nuclear Data Tables, 92, 105 [NASA ADS] [CrossRef] (In the text)
 Burke, P., Sukamar, C., & Berrington, K. A. 1981, J. Phys. B, 14, 289 [NASA ADS] [CrossRef] (In the text)
 Butler, K., & Zeippen, C. J. 1994, A&ASS, 108, 1 [NASA ADS] (In the text)
 Clementi, E., & Roetti, C. 1974, Atomic Data and Nuclear Data Tables, 14, 177 [NASA ADS] [CrossRef]
 Crees, M., Seaton, M. J., & Wilson, P. M. H. 1978, Comput. Phys. Comm., 15, 23 [NASA ADS] [CrossRef] (In the text)
 Edlen, B. 1964, in Encyclopedia of Physics, ed. S. Flugge, 27, 172 (In the text)
 Fawcett, B. C., Galanti, M., & Peacock, J. 1974, J. Phys. B, 7, 1149 [NASA ADS] [CrossRef] (In the text)
 Griffin, D. C., Badnell, N. R., & Pindzola, M. S. 1998, J. Phys. B, 31, 3713 [CrossRef] (In the text)
 Guennou, H., Surreau, A., Carillon, A., & Jamelot, G. 1979, J. Phys. B, 12, 1657 [NASA ADS] [CrossRef] (In the text)
 Hibbert, A. 1975, Comput. Phys. Comm., 9, 141 [CrossRef] (In the text)
 Johannesson, G. A., Lundstrom, T., & Minnhagen, L. 1972, Phys. Scr., 6, 129 [NASA ADS] [CrossRef] (In the text)
 Mendoza, C., & Zeippen, C. J. 1987, MNRAS, 224, 7 [NASA ADS] (In the text)
 Saraph, H. E. 1972, Comput. Phys. Comm., 3, 256 [NASA ADS] [CrossRef]
 Saraph, H. E. 1978, Comput. Phys. Comm., 15, 247 [NASA ADS] [CrossRef]
 Scott, N. S., & Burke, P. G. 1980, J. Phys. B, 13, 4299 [NASA ADS] [CrossRef] (In the text)
 Soderqvist, J. 1934, Nova Acta Regiae Soc. Sci. Ups., Ser. IV, 9, 1
 Soderqvist, J. 1946, Ark. Mat., Astron. Fys., 32, 1
 Tachiev, G. I., & Froese Fischer, C. 2002, A&A, 385, 716 [NASA ADS] [CrossRef] [EDP Sciences] (In the text)
 Young, P. R., Dupree, A. K., Espey, B. R., & Kenyon, S. J. 2006, ApJ, 650, 1091 [NASA ADS] [CrossRef] (In the text)
 Young, P. R., Del Zanna, G., Mason, H. E., et al. 2007a, Publ. Astron. Soc. Japan, 59, S727 [NASA ADS] (In the text)
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Footnotes
 ... Mg V^{}
 Table 8 is only available in electronic form at the CDS via anonymous ftp to cdsarc.ustrasbg.fr (130.79.128.5) or via http://cdsweb.ustrasbg.fr/cgibin/qcat?J/A+A/494/729
All Tables
Table 1: Orbital optimisations.
Table 2: Orbital parameters (c, I, ) of the radial wavefunctions.
Table 3: Distribution of configurations for each symmetry in the two versions of the calculation.
Table 4: Target state energies for our two configuration sets (1350 and 1044) compared to available NIST data.
Table 5: Oscillator strengths for the allowed transitions, in both length and velocity forms (f_{l} and f_{v}) for our two configuration sets (1350 and 1044), compared to Tachiev & Froese Fischer (2002)[T&F].
Table 6: Finestructure energy levels for the current calculation compared to the earlier works of Bhatia et al. (2006), Tachiev & Froese Fischer (2002) [T&F] and Butler & Zeippen (1994) [B&Z], along with the observed values from NIST.
Table 7: Effective Collision Strengths for transitions between the first 5 jlevels of Mg V at selected temperatures^{a}.
All Figures
Figure 1: Effective collision strengths as a function of electron temperature (in Kelvin) for transitions within the ground state configurations (levels 15). Solid line: current Rmatrix calculation, Crosses: Butler & Zeippen (1994) 6state Rmatrix calculation, Dashed line: Bhatia et al. (2006) (Distorted Wave calculation merged with Butler & Zeippen 1994). Transitions marked * have been recently observed in AG Draconis (Young et al. 2006). 

Open with DEXTER  
In the text 
Figure 2: Effective collision strengths as a function of electron temperature (in Kelvin) for transitions between initial levels 1, 2 and 3 and final levels 6, 7 and 8 and transition 49. Solid line: current Rmatrix calculation, Dashed line: Bhatia et al. (2006, Distorted Wave results). Transition marked * has been recently observed by Hinode (Young et al. 2007a). 

Open with DEXTER  
In the text 
Figure 3: Collision strengths as a function of incident electron energy in Rydbergs for transitions 28, 36 and 45. Solid line  Current Rmatrix calculation, Circles  Bhatia et al. (2006, Distorted Wave). 

Open with DEXTER  
In the text 
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