Spectral diagnostic capabilities of Solar-B EIS

In 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.