Article ID Journal Published Year Pages File Type
1781309 Planetary and Space Science 2013 8 Pages PDF
Abstract

•Same-beam VLBI observations are the first simulated for the Chang'E-3.•The LRV's position to the LM is estimated by LS, EKF and AEKF.•The best accuracy is obtained with 1.86 m, 0.33 m and 0.09 m in X, Y and Z-axis with AEKF.

The real-time and high precision positioning of the lunar rover vehicle is an important step for lunar exploration and science. SBI (same-beam interferometry) is the differential very long baseline interferometry (VLBI) technology, which can be used in lunar exploration with its high precision and stability. In this paper, the relative positioning model of the lunar rover vehicle (LRV) to lunar module (LM) based on the SBI and extended kalman filtering (EKF) is developed and presented. Using the current Chinese VLBI network and the planed Chang'E-3, SBI observation data with an attainable precision of picoseconds and a sample interval of 4 s are simulated. The LRV's relative position to the LM is then estimated by the least squares adjustment, EKF and an adaptive EKF, respectively. Results show that the Adaptive EKF performs the best real-time solutions with the accuracy of 1.86 m in X direction, 0.33 m in Y direction and 0.09 m in Z direction, which can provide a good reference for real-time positioning of planed Chang'E-3 rover.

Related Topics
Physical Sciences and Engineering Earth and Planetary Sciences Geophysics
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