“…Moreover, the discontinuity almost disappears for the high 40% iron content. These transitions contrast with those on Earth, for which both the reduced iron content and the higher pressure gradient result in sharp discontinuities, with a typical width of < 10 km (e.g., Tibi and Wiens, 2005). Reflections from mantle discontinuities on Mars might be less impulsive than reflections on Earth, and as a result, they might only be observable only at LPs, when the seismic wavelength is much greater than the width of the discontinuity, or below frequencies of 0.05-0.1 Hz.…”