Martian discrete auroras are spatially confined regions of photon emission caused by the precipitation of suprathermal (>∼5 eV) electrons into Mars' nightside upper atmosphere. Electron impact causes electronic excitations of atoms and molecules, whose decay releases ultraviolet and visible photons. Discrete aurorae were discovered by the SPICAM UV spectrometer (Bertaux et al., 2005) onboard Mars Express (MEx) and were characterized by small spatial scales, a tendency to form in regions of strong vertical crustal magnetic fields, and an association with sheath and magnetotail electrons that have been energized (