During the first 379 sols of NASA's Perseverance rover mission on Mars, over 5 km had been driven over the Jezero Crater Floor. The rover had gone from the Octavia E. Butler landing site (OEB), located on the relatively flat terrain of the Máaz Formation, to the distinct rugged exposures of the Séítah Formation. Afterward, the rover drove back again to OEB, largely backtracking its original route. The Radar Imager for Mars' Subsurface Exploration (RIMFAX;Hamran et al., 2020) conducted measurements along the whole traverse, providing an exceptional data set for constraining subsurface parameters over a large geographical area spanning several different regions (Figure 1). Moreover, the close vicinity of the two passes allows for testing replicability of obtained media parameters.The first look into the shallow Martian subsurface disclosed intriguing reflector geometries, which at places can be correlated with outcropping rock formations on the surface (Hamran et al., 2022). Yet, more information is contained in the acquired data, hidden by randomly distributed reflections dominating the radar image. This calls for supplementary analysis of the radar data beyond that of visual inspection.Ground-penetrating radar (GPR) data is strongly affected by the frequency dependent attenuation mechanisms. In general, higher frequency content is attenuated more than lower, so that subsurface reflection spectra will be altered compared to that of the transmitted waveform. The constant-Q factor was originally used to describe similar behavior of seismic waves due to cumulative attenuating effects in the ground (Richards & Aki, 1980), but it has also been found applicable for electromagnetic propagation in natural soil and rocks over the GPR frequency range 0.1-1.0 GHz (Harbi & McMechan, 2012;Turner & Siggins, 1994). For this reason, it can be appropriate to assume a linear frequency dependence for the attenuation in GPR sounding: