I am a first-year Ph.D. student, and I have obtained the best-fit parameters from 1D CLOUDY modeling. I want to use these parameters to generate the 3D ionization structure of the nova ejecta to visualize the spatial distribution of elements at different epochs, similar to the approach described in this paper: https://ui.adsabs.harvard.edu/abs/2019A%26A...622A.126P/abstract.
I have few questions: