基于天基雷达的地球自转建模

S. Pillai, B. Himed, K. Li
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引用次数: 7

摘要

天基雷达(SBR)由于自身的运动特性,对地球上任何一点的杂波回波产生多普勒频率分量,该多普勒频率分量是SBR -地球几何形状的函数。地球绕地轴自转的影响也增加了多普勒频率的额外分量。地球自转对多普勒的总体影响被证明是两个校正因子,即螃蟹角影响方位角,螃蟹星等缩放杂波斑块的多普勒星等。有趣的是,这两个量只取决于SBR轨道的倾角和纬度,而不取决于感兴趣的杂波斑块的位置。此外,螃蟹角对赤道以上的极轨道上的SBR影响最大。另一方面,在赤道轨道上的SBR的蟹状星等是最大的。本文给出了这些结果的详细推导。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Modeling of Earth's rotation for space based radar
Space-based radars (SBR) by virtue of their motion generate a Doppler frequency component to the clutter return from any point on the Earth as a function of the SBR - Earth geometry. The effect of Earth's rotation around its own axis also adds an additional component to this Doppler frequency. The overall effect of the Earth's rotation on the Doppler turns out to be two correction factors in terms of a crab angle affecting the azimuth angle, and a crab magnitude scaling the Doppler magnitude of the clutter patch. Interestingly, both these quantities depend only on the SBR orbit inclination and its latitude and not on the location of the clutter patch of interest. Further the crab angle has maximum effect for an SBR on a polar orbit that is above the equator. The crab magnitude on the other hand peaks for an SBR on an equatorial orbit. A detailed derivation of these results is presented in this paper.
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