“…In the ISM, ices are adsorbed to carbonaceous or silicate dust grains with a highly irregular morphology containing steps, pores, cracks, and terraces (Dulieu et al, 2013;van Dishoeck 2014). This highly irregular morphology is thought to aid in the formation of astrochemical species through surface-catalyzed processes (Mendoza et al, 2004;Potapov et al, 2019;Suhasaria and Mennella 2021). In laboratory investigations of the chemistry occurring within interstellar ices, however, ices are usually deposited onto flat surfaces used for transmission or reflection spectroscopy (e.g., gold, zinc selenide, magnesium fluoride, etc.).…”