X-ray pulsar-based autonomous navigation based on asynchronous observation ST-REKF

Author(s):  
Sun Jian ◽  
Guo Xiliang ◽  
Guo Pengbin ◽  
Li Bin
Keyword(s):  
Author(s):  
Po-Ting Chen ◽  
Jason L. Speyer ◽  
David S. Bayard ◽  
Walid A. Majid

2017 ◽  
Vol 2017 ◽  
pp. 1-5 ◽  
Author(s):  
Hao Liang ◽  
Yafeng Zhan

The detection of the X-ray pulsar signal is important for the autonomous navigation system using X-ray pulsars. In the condition of short observation time and limited number of photons for detection, the noise does not obey the Gaussian distribution. This fact has been little considered extant. In this paper, the model of the X-ray pulsar signal is rebuilt as the nonhomogeneous Poisson distribution and, in the condition of a fixed false alarm rate, a fast detection algorithm based on maximizing the detection probability is proposed. Simulation results show the effectiveness of the proposed detection algorithm.


2012 ◽  
Vol 36 (1) ◽  
pp. 97-106 ◽  
Author(s):  
Chong-Xia Zhong ◽  
Li Zhang ◽  
Feng Nian ◽  
Jun Yang

2013 ◽  
Vol 51 (5) ◽  
pp. 849-857 ◽  
Author(s):  
Erhu Wei ◽  
Shuanggen Jin ◽  
Qi Zhang ◽  
Jingnan Liu ◽  
Xuechuan Li ◽  
...  
Keyword(s):  

2017 ◽  
Vol 70 (4) ◽  
pp. 719-734 ◽  
Author(s):  
Jiandong Liu ◽  
Erhu Wei ◽  
Shuanggen Jin

The precise autonomous navigation for deep space exploration by combination of multi-source observation data is a key issue for probe control and scientific applications. In this paper, the performance of an integrated Optical Celestial Navigation (OCN) and X-ray Pulsars Autonomous Navigation (XNAV) system is investigated for the orbit of Mars Pathfinder. Firstly, OCN and XNAV single systems are realised by an Unscented Kalman Filter (UKF). Secondly, the integrated system is simulated with a Federated Kalman Filter (FKF), which can do the information fusion of the two subsystems of UKF and inherits the advantages of each subsystem. Thirdly, the performance of our system is evaluated by analysing the relationship between observation errors and navigation accuracy. The results of the simulation experiments show that the biases between the nominal and our calculated orbit are within 5 km in all three axes under complex error conditions. This accuracy is also better than current ground-based techniques.


2012 ◽  
Vol 29 ◽  
pp. 4369-4373 ◽  
Author(s):  
Jian Du ◽  
Bao-jun Fei ◽  
Ying Liu ◽  
Yu Xiao
Keyword(s):  

2017 ◽  
Vol 40 (9) ◽  
pp. 2237-2249 ◽  
Author(s):  
Po-Ting Chen ◽  
Jason L. Speyer ◽  
David S. Bayard ◽  
Walid A. Majid

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