Limits on inference of Mars small-scale topography from MOLA data

[i] The surface roughness of Mars at scales from ~ 1-200 m is of interest for lander hazard and radar-sounder clutter analysis, but MOLA data are the only current source of global topographic information. We use synthetic fractal profiles to determine the uncertainties associated with deriving self-affine statistics irom detrended segments of MOLA tracks. The mean Hurst exponent derived from such segments is an underestimate of the true value, H, for H > 0.5, and an overestimate for H < 0.5. Values of H from independent samples along a profile are distributed about this biased mean value. The magnitudes of the bias and variance in H increase for shorter segments. Terrestrial topography data show that extrapolation of roughness statistics to smaller scales based on self-affine relationships is uncertain. Roughness at the 1 -15 m scales may be poorly correlated with topography at >100-m scales. We suggest that any extrapolation be regarded as a lower bound on the true terrain statistics.