Abstract:The poles of Mars are cold traps for Martian atmospheric volatiles. The layered structures of polar deposits are thought to represent a record of Martian climatic history. In this paper, the propagation of electromagnetic waves in the polar caps is considered. Kirchhoff approximation and geometrical optics method are adopted to simulate the radar echo from Martian gently undulating surface and subsurface. The radar is modulated with linear frequency-modulated signals. Location information of the Martian surfac… Show more
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