In order to simplify the storage of these data we examine the possibility of
fitting them, both as functions of energy and of ion charge number Z. We
then carry out thermal averaging and fit the resulting effective collision
strengths as functions of temperature T and Z. The
basis for carrying out each of these processes was set out in detail by
Burgess & Tully (1992) (hereafter referred to as B&T) and we use their
notation. B&T also described the interactive program OMEUPS and used it to
obtain such isoelectronic fits for the 2s-2p transition in all the
Li-like ions of charge 1 to 23, and for the 21S-21P transition
in all the Be-like ions of charge 2 to 10.
Our present purpose is to extend the treatment in three ways:
First, we fit the ZSF data for the non-optically allowed transitions 2s-3s, 2s-4s, 2s-5s, 2s-3d, 2s-4d and 2s-5d. To help achieve this, we calculate the Born high energy limit points following the procedure described by Burgess et al. (1997).
Secondly, we incorporate some of the relativistic corrections required for larger values of Z than those treated in B&T.
Finally, we illustrate the use of types of fit other than the 5-point cubic spline adopted as standard in the previous work and in current plasma modelling computer programs.
We use a recent version of the interactive program, renamed OmeUpZ, designed to handle these extensions. Details will be given elsewhere (Burgess 2001).
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