Abstract
We present spectral line wavelengths, identifications, and intensities in the 171-211 and 245-291 A ranges from five solar plasma regions recorded by the Extreme-Ultraviolet Imaging Spectrometer (EIS) on Hinode. The recorded data were emitted from a quiet region, two active areas on the solar disk, a limb region, and a region 20'' above the limb. The line list contains 500 lines of which 55% were identified with previously known transitions. Although the EIS spectral coverage is limited to two ranges approximately 40 A wide, the identified lines belong to a total of 56 ions from 15 elements.
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