论文标题
使用光学成像,脉冲星进行时间跟踪和/或辐射跟踪的深空导航进行比较
Comparison of Deep Space Navigation Using Optical Imaging, Pulsar Time-of-Arrival Tracking, and/or Radiometric Tracking
论文作者
论文摘要
NASA在太空原子时钟和PULSAR X射线导航中开发的太空导航技术的最新进展以及使用光学成像在自主导航中取得的过去成功,这使您需要使用光学,放射线仪和基于PULSAR的衡量标准,使得需要使用普通的假设和技术集合。这篇评论文章以两种不同的方式研究了这些导航数据类型。首先,提出了简化的深空轨道确定问题,该问题捕获了动力学和几何形状的关键特征,然后每个数据类型的特征是其为轨道求解的能力。比较数据类型并使用半分析方法与精确技术的几何稀释进行对比。结果为每种数据类型的强度提供了有用的参数见解。在本文的第二部分中,研究了对火星巡航,进近和进入导航问题的高保真,蒙特卡洛模拟。结果发现的结果是第一部分的半分析结果,并说明了特定问题,例如每种数据类型对解决方案准确性的定量影响及其支持向行星自主传递的能力。
Recent advances with space navigation technologies developed by NASA in space-based atomic clocks and pulsar X-ray navigation combined with past successes in autonomous navigation using optical imaging, brings to the forefront the need to compare space navigation using optical, radiometric, and pulsar-based measurements using a common set of assumptions and techniques. This review article examines these navigation data types in two different ways. First, a simplified deep space orbit determination problem is posed that captures key features of the dynamics and geometry, and then each data type is characterized for its ability to solve for the orbit. The data types are compared and contrasted using a semi-analytical approach with geometric dilution of precision techniques. The results provide useful parametric insights into the strengths of each data type. In the second part of the paper, a high-fidelity, Monte Carlo simulation of a Mars cruise, approach, and entry navigation problem is studied. The results found complement the semi-analytic results in the first part, and illustrate specific issues such as each data type's quantitative impact on solution accuracy and their ability to support autonomous delivery to a planet.