Frontal precipitation systems are simulated with a 2D cloud model incl
uding ice-phase microphysics. Despite the use of idealized frontogenet
ic forcing in the simulations, some observed characteristics of fronta
l zones and their associated cloud and precipitation fields are reprod
uced in the simulations. The effects of melting snow on surface fronto
genesis is investigated. It is found that the cooling effects of melti
ng snow significantly accelerate surface frontogenesis in winter storm
environments, especially when the melting layer is close to the surfa
ce. However, the steady-state surface frontal strength in the model is
not sensitive to the melting effects. Finescale thermal and kinematic
perturbations inside the frontal zone near the melting level, quite s
imilar to those recently reported in the literature, are evident in th
e model results. Analysis of the model results suggests that cooling f
rom melting snow may induce these thermal and kinematic perturbations
and may enhance baroclinicity, resulting in accelerating frontogenesis
. These frontogenetic effects should be strongest when the melting lay
er is near the surface, thus explaining the often observed coincidence
of surface fronts with the surface rain-snow boundary in winter storm
s.