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951.
Meng Yu Shuang Li Shuquan Wang Xiangyu Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2019,63(2):1085-1099
In this paper, a novel crater-aided inertial navigation approach for autonomous asteroid landing mission is developed. It overcomes the major deficiencies of existing approaches in the literature, which mainly focuses on the case where craters are abundant in the camera field of view. As a result, traditional crater based methods require at least three craters to achieve crater matching, which limits their application in final landing phase where craters are scarce in the camera’s field of view. In contrast, the proposed algorithm enables single crater based crater matching based on a novel 2D-3D crater re-projection model. The re-projection model adopts inertial measurements as a reference, and re-projects the 3D crater model onto descent images to achieve the matching to its counterpart. An asteroid landing simulation toolbox is developed to validate the performance of the proposed approach. Through comparison with the state-of-the-art local image feature and crater based navigation algorithms, the proposed approach is validated to achieve a competitive performance in terms of feature matching and pose estimation accuracy with a much lighter computational cost. 相似文献
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Yi Xie Wei-Tou Ni Peng Dong Tian-Yi Huang 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2009
Deep space laser ranging missions like ASTROD I (Single-Spacecraft Astrodynamical Space Test of Relativity using Optical Devices) and ASTROD, together with astrometry missions like GAIA and LATOR will be able to test relativistic gravity to an unprecedented level of accuracy. More precisely, these missions will enable us to test relativistic gravity to 10-7–10-9 of the size of relativistic (post-Newtonian) effects, and will require second post-Newtonian approximation of relevant theories of gravity. The first post-Newtonian approximation is valid to 10-6 and the second post-Newtonian approximation is valid to 10-12 in terms of post-Newtonian effects in the solar system. The scalar-tensor theory is widely discussed and used in tests of relativistic gravity, especially after the interests in inflation models and in dark energy models. In the Lagrangian, intermediate-range gravity term has a similar form as cosmological term. Here we present the full second post-Newtonian approximation of the scalar-tensor theory including viable examples of intermediate-range gravity. We use Chandrasekhar’s approach to derive the metric coefficients and the equation of the hydrodynamics governing a perfect fluid in the second post-Newtonian approximation in scalar-tensor theory; all terms inclusive of O(c-4) are retained consistently in the equations of motion. 相似文献
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957.
行星表面陨石坑检测与匹配方法 总被引:2,自引:0,他引:2
针对深空探测器光学导航技术的需要,提出了行星表面陨石坑导航路标的提取与匹配方法。陨石坑是行星表面最显著的地形特征,在光照条件下,陨石坑具有清晰的几何轮廓。结合光照方向,通过陨石坑边缘的检测、边缘配对以及形状参数拟合等处理实现陨石坑的提取。对检测出的陨石坑,基于平面二次曲线的几何不变特性,采用投票策略实现与陨石坑数据库的匹配,并设计陨石坑误匹配及失配的校正策略,从而有效地确定陨石坑在目标天体表面的全局位置。最后通过嫦娥一号获得的目表图像验证了所提方法的有效性和可行性。 相似文献
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摘要: 针对用于地外天体着陆视觉导航的路标图像信息存在的计算量大和占用存储空间大等问题,提出一种路标图像的稀疏化表征方法.引入着陆路标图像的尺度估计和尺度变换,采用Harris 算法提取路标特征点,改进了FREAK特征描述子用以稀疏化表征天体路标信息;并针对图像旋转、尺度变化、图像噪声和尺度估计误差4种外界干扰,仿真对比改进算法与原FREAK算法、SURF算法的性能.仿真结果表明:提出的算法大幅减少计算量和特征描述子所占用的存储空间,同时能够正确匹配到更多的路标特征,鲁棒性更好,更适合地外天体着陆任务应用. 相似文献
960.
针对载人登月短期全球访问任务,月面上升过程存在上升舱与返回舱异面交会问题。以减小调面机动燃料消耗为目标,利用三垂线定理给出上升轨道与目标轨道的最小平面夹角(楔角)求解公式,考虑应急返回任务需求,以降低整个任务期间最坏的平面夹角为目标,给出全月面到达着陆轨道与上升轨道倾角求解方法。仿真结果表明,所提方法计算简单,精度高,可为载人登月任务设计和分析提供参考。 相似文献