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Mars advanced radar for subsurface and ionosphere sounding (MARSIS): Subsurface performances evaluation

机译:火星用于地下和电离层探测的先进雷达(MARSIS):地下性能评估

摘要

According to the Mars Express mission, the MARSIS primary scientific objectives are to map the distribution of water. both liquid and solid, in the upper portions of the crust of Mars. Three secondary objectives are also defined subsurface geologic probing, surface characterization, and ionosphere sounding. In order to obtain the primary objectives the Radar Sounder design was based on the kelwater interface and Dry/ice interface scenario: defining the material composition of the first layers and porosity and the pore filling materials. Concerning the surface, we have characterized the geometric structure in terms of a large-scale morphology, on which a small-scale geometric structure, due to rocks, is superimposed, taking into account also that recently the structure of the planets surface was described by means of fractals and in particular the new MARS surface models obtained by processing of the MOLA data. According to these models, this paper provides a description of the operational planning approach and expected performances of MARSIS.
机译:根据火星快车的任务,MARSIS的主要科学目标是绘制水的分布图。在火星地壳的上部都有液体和固体。还定义了三个次要目标,即地下地质探测,表面表征和电离层探测。为了获得主要目标,Radar Sounder设计基于kelwater界面和Dry / ice界面方案:定义第一层的材料组成,孔隙率和孔隙填充材料。关于表面,我们已经用大范围的形态学表征了几何结构,并在其上叠加了由于岩石引起的小规模的几何结构,同时考虑到最近对行星表面的结构进行了描述:分形的手段,特别是通过处理MOLA数据获得的新的MARS表面模型。根据这些模型,本文描述了MARSIS的作战计划方法和预期性能。

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