Hi Will,
Thanks for your question. The masterlist contains ions that have the wgfa, scups and elvlc file and so yield emission lines. For computing the ionization balance we store recombination and ionization rates for each ion, including those ions that are missing in the regular database.
So, in the case of ca_3, for example, you’ll see diparams, drparams, easplom, easplups and rrparams files that are for ionization and recombination rates. You don’t see wgfa, scups and elvlc files, though, hence this ion isn’t in the masterlist.
Thanks, Peter
--
You received this message because you are subscribed to the Google Groups "chianti" group.
To unsubscribe from this group and stop receiving emails from it, send an email to
chianti+u...@googlegroups.com.
To view this discussion on the web visit
https://groups.google.com/d/msgid/chianti/a3da2c56-c994-48f2-b2b6-8d79a8849de4n%40googlegroups.com.