Fig. 3: Dune length (blue-to-yellow circles) and large-ripple wavelength (light purple1 and dark green circles36) decreases with increasing atmospheric density.
From: A distinct ripple-formation regime on Mars revealed by the morphometrics of barchan dunes

Ripple data follows a previously derived scaling relationships for drag ripples5; best-fit power law to an updated global compilation of dark-toned large-ripple wavelength has an exponent of −0.63 (green dashed line)35. The width of the hydrodynamic anomaly (gray shade) was calculated for a 125 μm grain size7 and assuming that wind shear velocity is at the transport threshold49 (Methods), using the model of ref. 12. The statistical significance of the regression slope was computed using a Wald Test, and errorbars (narrower than line width) indicate a 95% confidence interval. Each dot in the figure represents the 2nd percentile dune length in equal-area bins (60 km2).