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Distortions of Rectangular Pulse with Linear Frequency Modulation during Trans-Ionospheric Sounding of the Martian Surface

机译:火星表面跨电离层探测过程中带有线性调频的矩形脉冲的畸变

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摘要

Specific features of propagation of a wideband rectangular pulse along the route spacecraft-Martian surface-spacecraft caused by the influence of the planetary ionosphere are considered as applied to the problem of radio pulse sounding of the subsurface Martian soil from the Mars-Express satellite. The night Martian ionosphere considerably reduces the energy of the pulse, but does not lead to degradation of its envelope or uncertainty function. When sounding a two-layer surface, the influence of the ionosphere is also manifested in limitation from below of the thickness of the upper layer accessible for measurement, which is more essential than when sounding with the use of a wideband Gaussian pulse. It is demonstrated that the surface sounding is possible through the dayside planet ionosphere at the parameters of operating pulse of the MARSIS radar.
机译:由行星电离层的影响引起的宽带矩形脉冲沿路径航天器-火星表面航天器的传播的特定特征被认为适用于火星快车卫星从火星表面探测无线电脉冲的问题。夜晚的火星电离层显着降低了脉冲能量,但并未导致其包络或不确定性函数降低。当探测两层表面时,电离层的影响还表现为从可测量的上层厚度的下方受到限制,这比使用宽带高斯脉冲探测时更重要。结果表明,在MARSIS雷达的工作脉冲参数下,可以通过日间行星电离层进行表面探测。

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