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CLC number: V448.21

On-line Access: 2013-01-31

Received: 2012-06-09

Revision Accepted: 2013-01-01

Crosschecked: 2013-01-04

Cited: 6

Clicked: 7740

Citations:  Bibtex RefMan EndNote GB/T7714

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Journal of Zhejiang University SCIENCE C 2013 Vol.14 No.2 P.133-142


Determination of inter-satellite relative position using X-ray pulsars

Author(s):  Da-jun Feng, Lu-ping Xu, Hua Zhang, Shi-bin Song

Affiliation(s):  School of Electronic Engineering, Xidian University, Xian 710071, China; more

Corresponding email(s):   xd203@yahoo.com.cn

Key Words:  Pulsar navigation, Position determination, Phase cycle ambiguity, Geometric dilution of precision (GDOP)

Da-jun Feng, Lu-ping Xu, Hua Zhang, Shi-bin Song. Determination of inter-satellite relative position using X-ray pulsars[J]. Journal of Zhejiang University Science C, 2013, 14(2): 133-142.

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author="Da-jun Feng, Lu-ping Xu, Hua Zhang, Shi-bin Song",
journal="Journal of Zhejiang University Science C",
publisher="Zhejiang University Press & Springer",

%0 Journal Article
%T Determination of inter-satellite relative position using X-ray pulsars
%A Da-jun Feng
%A Lu-ping Xu
%A Hua Zhang
%A Shi-bin Song
%J Journal of Zhejiang University SCIENCE C
%V 14
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%P 133-142
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%I Zhejiang University Press & Springer
%DOI 10.1631/jzus.C12a0142

T1 - Determination of inter-satellite relative position using X-ray pulsars
A1 - Da-jun Feng
A1 - Lu-ping Xu
A1 - Hua Zhang
A1 - Shi-bin Song
J0 - Journal of Zhejiang University Science C
VL - 14
IS - 2
SP - 133
EP - 142
%@ 1869-1951
Y1 - 2013
PB - Zhejiang University Press & Springer
ER -
DOI - 10.1631/jzus.C12a0142

Pulsars are rapidly rotating neutron stars that generate pulsed electromagnetic radiation. A new method for inter-satellite relative position determination between a global navigation satellite system (GNSS) and spacecraft using X-ray pulsars is proposed in this paper. The geometric model of this method is formulated, and two different resolution algorithms are introduced and analyzed. The phase cycle ambiguity resolution is investigated, and a new strategy is proposed and formulated. Using the direct vector parameters of the pulsar, geometric dilution of precision (GDOP) is studied. It is shown that this method has advantages of simplicity and efficiency, and is able to eliminate the clock errors. The analytical results are verified numerically via computer simulations.

Darkslateblue:Affiliate; Royal Blue:Author; Turquoise:Article


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