Abstract
The large number of high-resolution spectra routinely recorded in the astrophysical and fusion communities leads to the need for an extensive set of accurate baseline atomic data. The advantages of the intermediate-coupling frame transformation R-matrix method make it feasible to provide excitation data along iso-electronic sequences covering a substantial range of astrophysically important ions at the high level of accuracy afforded by the R-matrix method. This is one of the key goals of the UK Atomic Processes for Astrophysical Plasmas (APAP) network.
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