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Simulation-based Assessment of Polarimetric L-band Synthetic Aperture Radar for Shallow Ice Detection on Mars

  • Authors: Ivan Mishev, Étienne Boulais, Isaac B. Smith, Catherine Neish, Michael Daly

Ivan Mishev et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 11.

Case 12: 5 m LVF regolith, 5 m HVF ice. From left to right: diagram of scenario showing subsurface profile. Stokes S1 radargram displaying total return power in dB, with range-averaged response overlaid as a black line. CPR radargram, with range-averaged response overlaid as a black line. Degree of polarization (m) plotted against apparent depth, with background shading denoting regolith, ice, and basalt units. The m-χ decomposition plotted against apparent depth. The m-χ decomposition radargram. Dashed vertical lines in S1 and m-χ plots at −123 dB indicate the NE-Γ noise floor (SNR = 0 dB). Orange, blue, and brown horizontal lines denote interfaces of regolith, ice, and basalt, respectively.

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