AbstractIn this paper, we provide simulated intensities for Solar-B EIS to aid in the scientific planning for Solar-B. These simulations are obtained with the latest atomic data and EIS response functions. We also report on our progress in reviewing and benchmarking atomic data for the Fe coronal ions, that are of particular importance for spectral and instrument calibration purposes. We highlight the most prominent lines that can be used for plasma diagnostics.
Spectral diagnostic capabilities of Solar-B EIS
Advances in Space Research ; 36 , 8 ; 1503-1511
2005-03-24
9 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Spectral diagnostic capabilities of Solar-B EIS
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