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Integral field observations of galaxies now produce spatially resolved emission line diagnostic diagrams that can reveal the diverse processes impacting the ISM, and are necessarily dependent on the geometry and distribution of their gas clouds. Simulations of galaxies can now model the diverse geometries of interstellar clouds, which are often different than the simple geometries employed in photoionisation codes like cloudy. Thus, we suggest that the future of emission line modeling willdoi:10.5281/zenodo.1208084 fatcat:46232ohd7nbvljx3lwbtrnmecq