This study explores how ACC’s impact on the mesoscale environment around future supercells will influence supercell frequency, storm scale characteristics, behavior, and dynamical processes through examination of output from two 13 year dynamically downscaled convective resolving simulations following the Pseudo Global Warming methodology. One simulation is governed by ‘modern’ climate conditions, while the second contains ‘future’ conditions at the end of the 21st century following the high end RCP8.5 scenario (‘business as usual’) emission projection. Uniquely, each individual model-resolved supercell was identified and tracked throughout its lifetime in both datasets, providing a modern and future supercell ‘climatology’. Corresponding climatological attributes and mesoscale environmental data were collected for each supercell in these datasets, as well as a variety of supercell characteristics, including supercell lifetime and intensity. A series of statistical tests were conducted to compare the distributions of these characteristics and the local inflow environments of the modern and future supercells. Initial results suggest future supercells are seen more frequently in March-April with little change in May-June, in line with previous research. A strong eastward shift in occurrence of springtime supercells is also identified, but this is not collocated with strongest increases in severe weather parameters; a change in initiation mechanism is hypothesized to cause this shift. Thus, this research will identify how ACC will cascade down to the convective scale, thus providing a more explicit picture into the sensible impacts of climate change.