Dear all, those of you at the last loop meeting will recall that in many instances I raised the issue that many lines in the EIS spectra are blended/unidentified.
Here is a link to a preprint with a detailed list of lines and identifications:
http://solar.physics.montana.edu/cgi-bin/eprint/index.pl?entry=15559
this paper only deals with coronal lines. It also includes new elemental abundance measurements. Together with
http://adsabs.harvard.edu/abs/2009A%26A...508..501D
where a list of purely `cool' TR lines is given, it provides a fairly complete line list, if one excludes high-density, high-temperature (flare) plasmas, or weak lines.
best,