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Supporting Autonomous Navigation with Flash Lidar Images in Proximity to Small Celestial Bodies

机译:支持与小型天体邻近的激光雷达激光雷达自主导航

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摘要

Spacecraft navigation in proximity to small celestial bodies, such as asteroids and comets, is challenging due to their complex dynamical environment and the lag in communications from Earth to the spacecraft. Increasing autonomous spacecraft navigation reduces the burden of ground-based planning and modeling, and enables insightful mission profiles. The state-of-the-art of relative spacecraft navigation uses optical images, requires an iterative procedure, and currently must be performed on the ground. A flash lidar instrument instantaneously returns a 3D elevation map of its target and shows promise for advancing autonomous spacecraft navigation. Using this instrument as a relative measurement source for navigation performed similarly or better than landmark-based navigation from optical images. The model-based approach used to compute the onboard flash lidar images eliminated the correlation procedures required of landmark-based approaches, and reduced the computational load. An extended Kalman filter (EKF), an unscented Kalman filter (UKF), and an iterative least-squares (LS) filter were investigated in this analysis. The iterative LS filter iterated the estimation state at each observation time, produced smaller errors than the EKF and UKF, and did not encounter filter saturation. The image properties of the flash lidar measurements allowed for pointing to be estimated. The UKF and LS filters were robust to initial position errors as long as an overlap occurred between the observed and computed flash lidar images. When introducing shape modeling errors, the filters did not diverge, and the majority of the state errors were captured with a sequential consider covariance analysis. Using the image properties of the flash lidar images, and assuming inertial spacecraft pointing knowledge, the filter was initialized through pre-processing algorithms and the iterative LS algorithm. Optimally reducing the number of altimetry measurements processed by maximizing their information contribution increased the computational efficiency and combated filter saturation without sacrificing accuracy.
机译:由于小行星和彗星等复杂的动态环境以及从地球到航天器的通信滞后,使航天器在诸如小行星和彗星之类的小天体附近航行非常具有挑战性。越来越多的自主航天器导航减轻了地面计划和建模的负担,并实现了洞察力强的任务概况。相对航天器导航的最新技术使用光学图像,需要迭代过程,并且当前必须在地面上执行。闪光灯激光雷达仪器会立即返回其目标的3D高程图,并显示出推进自主航天器导航的希望。使用该仪器作为导航的相对测量源,与从光学图像进行基于地标的导航相比,其性能类似或更好。用于计算机载闪光灯激光雷达图像的基于模型的方法消除了基于界标的方法所需的相关过程,并减少了计算量。在此分析中,研究了扩展卡尔曼滤波器(EKF),无味卡尔曼滤波器(UKF)和迭代最小二乘(LS)滤波器。迭代LS滤波器在每个观察时间迭代估计状态,产生的误差小于EKF和UKF,并且没有遇到滤波器饱和。闪光激光雷达测量的图像属性允许估计指向。 UKF和LS滤波器对于初始位置误差具有鲁棒性,只要在观察到的和计算出的闪光激光雷达图像之间出现重叠即可。引入形状建模误差时,滤波器不会发散,并且大多数状态误差是通过顺序考虑协方差分析而捕获的。利用闪光灯激光雷达图像的图像属性,并假设惯性航天器指向知识,可通过预处理算法和迭代LS算法初始化滤波器。通过最大程度地减少信息量贡献来最佳地减少其处理次数,可以提高计算效率,并在不牺牲精度的情况下降低了滤波器的饱和度。

著录项

  • 作者

    Dietrich, Ann B.;

  • 作者单位

    University of Colorado at Boulder.;

  • 授予单位 University of Colorado at Boulder.;
  • 学科 Aerospace engineering.
  • 学位 Ph.D.
  • 年度 2017
  • 页码 250 p.
  • 总页数 250
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类
  • 关键词

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