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Synthetic spectra (green) compared to observation (black) taken by Hinode/EIS at 12 November 2007 12:32:02 UT of the Northern coronal hole during the Carrington Rotation 2063 (from Szente et al., 2019). Line profiles of Fe XI 201.734 Å, Fe XIII 201.121 Å and 202.044 Å are closely predicted in intensity, width and Doppler-shift; while there is no line in the CHIANTI database between 201.5 and 201.6 Å, which explains the missing peak in the model’s result.
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