Mars is prone to atmospheric turbulence. Its thin, nearly cloudless atmosphere and low surface thermal inertia entail strong near-surface unstable temperature gradients, resulting in convective turbulencecells, plumes, vortices-at daytime in the planetary boundary layer (PBL;Larsen et al., 2002;Petrosyan et al., 2011;Tillman et al., 1994). This induces a wealth of daytime high-frequency variations in the atmospheric pressure, wind and temperature measured by landers and rovers (Martínez et al., 2017 for a review). Conversely, nighttime conditions in Mars' PBL are highly stable because of strong radiative cooling efficiently inhibiting convection. Nevertheless, in the night, shear-driven weak turbulence may exist on Mars (e.g., Pla-García et al., 2020;Savijärvi, 1999) and, intriguingly, vortex-induced pressure drops have been observed in Gale Crater by Curiosity (Ordonez-Etxeberria et al., 2018.