Although the Antarctic Ice Sheet (AIS) contribution to sea level rise is heavily influenced by ocean-driven mass loss (e.g., Edwards et al., 2019;Seroussi et al., 2020), the effects of sub-decadal to decadal precipitation variation on surface mass balance (SMB) dominate the overall mass balance variability of East Antarctica (IMBIE, 2018). A detailed understanding of SMB variability is therefore crucial to assess the future contribution of Antarctica to sea level rise (Seroussi et al., 2020). Uncertainties in future SMB changes contribute substantially to uncertainties in the projected Antarctic contribution to sea level rise, which varies between −7.8 and 43 cm sea level equivalent by 2100 under Representative Concentration Pathway (RCP) 8.5 scenario (Edwards et al., 2019(Edwards et al., , 2021Seroussi et al., 2020). Estimates of regional scale SMB distribution and trends remain difficult to obtain as high-resolution data remain very scarce (e.g., Favier et al., 2017;Lenaerts et al., 2019). The strong variability of Antarctic SMB, both in time and space, further complicates this effort. Precipitation over most regions of Antarctica is controlled by a few high precipitation events (Turner et al., 2019). This characteristic has to be understood and correctly represented in models for accurate projections.The strongly baroclinic Southern Ocean exhibits a high rate of cyclogenesis, and the southern Indian Ocean sector exhibits the highest frequency and strongest zone of cyclogenesis of the southern mid-latitudes (Simmonds et al., 2003). Yet, only a few of these cyclones actually reach the Antarctic coastline, and even fewer generate high precipitation events (