We want to determine where specific energy transfer processes can occur in the space around Mars, because they can act to channel solar wind energy into the atmosphere. To do this, we use data from MAVEN (NASA 2014) and cross-validated our results with previous case studies. We focused on two parameters: magnetic field strength and ion density. Using a binning method, we grouped data by location in the Martian environment. This allowed us to analyze where certain energy transfer processes may be favored. Preliminary results highlight regions around Mars where these processes are likely to occur. These maps provide new insight into how such interactions may impact the atmosphere of Mars and help build a statistical foundation for further analysis of energy transfer.