CLC number: V44; TP872
On-line Access: 2024-08-27
Received: 2023-10-17
Revision Accepted: 2024-05-08
Crosschecked: 2016-05-14
Cited: 0
Clicked: 6356
Rong Jiao, Lu-ping Xu, Hua Zhang, Cong Li. Orbit determination using incremental phase and TDOA of X-ray pulsar[J]. Frontiers of Information Technology & Electronic Engineering, 2016, 17(6): 543-552.
@article{title="Orbit determination using incremental phase and TDOA of X-ray pulsar",
author="Rong Jiao, Lu-ping Xu, Hua Zhang, Cong Li",
journal="Frontiers of Information Technology & Electronic Engineering",
volume="17",
number="6",
pages="543-552",
year="2016",
publisher="Zhejiang University Press & Springer",
doi="10.1631/FITEE.1500365"
}
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%T Orbit determination using incremental phase and TDOA of X-ray pulsar
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%A Hua Zhang
%A Cong Li
%J Frontiers of Information Technology & Electronic Engineering
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%N 6
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%I Zhejiang University Press & Springer
%DOI 10.1631/FITEE.1500365
TY - JOUR
T1 - Orbit determination using incremental phase and TDOA of X-ray pulsar
A1 - Rong Jiao
A1 - Lu-ping Xu
A1 - Hua Zhang
A1 - Cong Li
J0 - Frontiers of Information Technology & Electronic Engineering
VL - 17
IS - 6
SP - 543
EP - 552
%@ 2095-9184
Y1 - 2016
PB - Zhejiang University Press & Springer
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DOI - 10.1631/FITEE.1500365
Abstract: X-ray pulsars offer stable, periodic X-ray pulse sequences that can be used in spacecraft positioning systems. A method using X-ray pulsars to determine the initial orbit of a satellite is presented in this paper. This method suggests only one detector to be equipped on the satellite and assumes that the detector observes three pulsars in turn. To improve the performance, the use of incremental phase in one observation duration is proposed, and the incremental phase is combined with the time difference of arrival (TDOA). Then, a weighted least squares (WLS) algorithm is formulated to calculate the initial orbit. Numerical simulations are performed to assess the proposed orbit determination method.
This paper presented an initial orbit determination algorithm which uses one detector to observe one single X-ray pulsar at one instant. In addition, an incremental phase measurement is adopted and combined with the Time Difference of Arrival to improve the precision.
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