This study focuses on The Chilean Orographic and Mesoscale Precipitation Study (ChOMPS) which collected data from three vertically profiling Micro-Rain-Radars (MRRs), two Parsivel disdrometers and three meteorological stations, for three locations along a zonal transect at ~36ºS: a coastal site (Concepción, 50m MSL), a central valley site (Chillán, 138m), and a mountain site (Las Trancas, 1235m), from May through October 2016 corresponding to austral winter. ChOMPS provided data unique until now, allowing for the study of mesoscale precipitation processes in the Chilean Andes.
Using MRR data, we objectively classify non-convective rainfall periods as associated with either ice-initiated rain or warm rain microphysical regimes based on the presence or absence of a well-defined melting layer. We calculate statistics to compare between both regimes and transect locations, including: rainfall amount associated with each regime, drop-size distribution, strength of orographic enhancement and frequency of each regime. For ice-initiated periods, we calculate spatial variations in height of the melting layer. These result can be compared with studies in the western coast of the United States, due the similarity between the Sierra Nevada and the Andes topography and location.