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Mars rover navigation using pseudolite transceiver arrays: Network-based ranging and extended self-calibration algorithm.

机译:使用伪卫星收发器阵列的火星探测器导航:基于网络的测距和扩展的自校准算法。

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摘要

A Self-Calibrating Pseudolite Array (SCPA) is a self-deployable GPS pseudolite-based local-area navigation system that can be used on future robotic and manned planetary explorations. By utilizing bidirectional pseudolite transceivers, the SCPA can provide common global positioning to multiple agents working in a local designated area of a remote planet, including all the benefits of satellite-based carrier-phase differential GPS, such as drift-free, centimeter-level, and three-dimensional positioning, without requiring a satellite constellation above the remote planet.; Previous work has demonstrated that changing the relative array geometry by moving a roving transceiver unit enables the SCPA to self-calibrate both the array locations and the rover trajectory to centimeter-level accuracy. This self-calibration capability has overcome the difficulty of autonomous robotic deployment of the pseudolite-based navigation system on remote planets, eliminating the need for accurate a priori position information or precise placement of the array.; However, early field trials raised the issue of robustness due to pseudolite signal dropouts caused by multi-path fading, cycle slips, or losing line-of-sight. In order to complete the self-calibration process successfully, the SCPA was required to maintain all the signal locks over the entire calibration maneuver; the lack of necessary ranging measurements due to any signal dropout requires the process to start over.; This dissertation solves this robustness issue by two new methods: network-based ranging and an extended self-calibration algorithm. The combination of the two algorithms yields a dual-fault-tolerant system, tolerating at least any two simultaneous dropouts intermittently during the calibration process while still operating in the minimum one-mobile three-stationary transceiver configuration with single-frequency pseudolite signals. The resulting improved robustness has been demonstrated in field trials using the K9 Mars rover platform operated in the Marscape at NASA Ames Research Center. The experimental results validate that the new algorithms can reliably complete the self-calibration process while experiencing severe signal dropouts, yet still achieve centimeter-level calibration performance.
机译:自校准伪卫星阵列(SCPA)是一种基于GPS可伪卫星的可自部署的局域导航系统,可用于未来的机器人和有人驾驶的行星探测。通过使用双向伪卫星收发器,SCPA可以为在偏远星球本地指定区域工作的多个代理提供通用的全球定位,包括基于卫星的载波相位差分GPS的所有优势,例如无漂移,厘米级,以及三维定位,而无需偏远星球上方的卫星星座。先前的工作表明,通过移动粗纱收发器单元来改变相对阵列的几何形状,可使SCPA对阵列位置和流动站轨迹进行自校准,以达到厘米级的精度。这种自校准能力克服了伪卫星导航系统在远程星球上自动机器人部署的困难,从而无需精确的先验位置信息或阵列的精确位置。但是,早期的现场试验提出了由于多路径衰落,周期滑移或视线丢失而导致伪卫星信号丢失的鲁棒性问题。为了成功完成自校准过程,SCPA被要求在整个校准过程中保持所有信号锁定。由于任何信号丢失而导致缺乏必要的测距测量,因此需要重新开始该过程。本文通过两种新方法解决了鲁棒性问题:基于网络的测距和扩展的自校准算法。两种算法的结合产生了一个双容错系统,在校准过程中间歇地至少容忍了至少两个同时丢失,同时仍在单频伪卫星信号的最小单机三站收发器配置中运行。使用在NASA Ames研究中心的Marscape中运行的K9火星漫游者平台进行的现场试验已证明了由此带来的更高的耐用性。实验结果证明,新算法可以可靠地完成自校准过程,同时遇到严重的信号丢失,但仍可以实现厘米级的校准性能。

著录项

  • 作者

    Matsuoka, Masayoshi.;

  • 作者单位

    Stanford University.;

  • 授予单位 Stanford University.;
  • 学科 Engineering Aerospace.
  • 学位 Ph.D.
  • 年度 2005
  • 页码 117 p.
  • 总页数 117
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 航空、航天技术的研究与探索;
  • 关键词

  • 入库时间 2022-08-17 11:42:02

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