This is a summary of predicted emission line intensities along solar radial direction listed in Landi et al. 2016.
The list of lines used in UCoMP (Upgraded CoMP).
We use CHIANTI version 8.0.2 to do the calculation. The calculation and plotting was made in May, 2018.
The results served as an informal reference for the science discussion of building the big solar coronagraph in China.
You can download the full PDF file here.
For the codes I used to calculate and plot the intensity variation radially, please check my GitHub repo.