Dual‐frequency bistatic radar experiments were conducted with Mars Express at a rate of one to two per month during 2005. Each observation provided power measurements of orthogonally polarized surface echoes at one specular point; the ratio of these components yielded values of the dielectric constant in the range 2.0 < ɛ < 4.0. Doppler sorting of X‐band (wavelength λ = 3.6 cm) echoes was used to achieve one‐dimensional surface resolutions of about 20 km. Although much weaker, simultaneous S‐band (13‐cm) echoes yielded dielectric constants that are 10–50% higher than 3.6 cm echoes, consistent with deeper surface penetration.
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Simpson et al. (2006) studied this question.
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