High clouds in the tropics have been difficult to reproduce in global climate models (GCMs) because of their complex microphysics and radiative properties (e.g., Del Genio, 2012;Stephens, 2005). Proper representation of the properties of tropical cirrus, especially cloud amount and hydrometeor distribution, is a key issue for improving GCMs (e.g., Inoue et al., 2010;Stephens, 2005;Zelinka et al., 2012). GCMs generally have a low spatial resolution, which is unable to explicitly represent convection and the subsequent tropical cloud life cycle. Diverse convective and ice microphysical parameterizations lead to large differences between GCMs in the ice cloud population (Del Genio, 2012). This is the second of two papers comparing the formation and properties of tropical cirrus in relation to deep convection in several high-resolution global storm-resolving models (GSRMs). Nugent et al. (2022) (hereafter Part I) focuses on deep convection and its role as a source of ice and vapor for cirrus formation. Here, we compare the simulated ice cloud populations with satellite observations, interpreting them in terms of an aggregate cirrus life cycle.As noted in Part I, GSRMs are attractive for modeling tropical cirrus. Unlike conventional climate models with horizontal grid spacings of 25-200 km, GSRMs have sub-5 km grid spacing that enables them to explicitly simulate deep convection and its detrainment of ice into the upper troposphere and better represent the mesoscale