Fig. C.1


Download original image

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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.