supported by the National Natural Science Foundation of China(Nos.61172138 and 61401340);the Natural Science Basic Research Plan in Shaanxi Province of China(No.2013JQ8040);the Research Fund for the Doctoral Program of Higher Education of China(No.20130203120004);the Open Research Fund of the Academy of Satellite Application(No.2014_CXJJ-DH_12);the Xi’an Science and Technology Plan(No.CXY1350(4));the Fundamental Research Funds for the Central Universities(Nos.201413B,201412B,and JB141303);the Open Fund of Key Laboratory of Precision Navigation and Timing Technology,National Time Service Center,CAS(Nos.2014PNTT01,2014PNTT07,and 2014PNTT08)
Weak L1 signal acquisition in a high dynamic environment primarily faces a challenge: the integration peak is neg- atively influenced by the possible bit sign reversal every 20 ms and the frequency error. The block a...
Project supported by the National Natural Science Foundation of China(Grant Nos.61172138 and 61401340);the Research Fund for the Doctoral Program of Higher Education of China(Grant No.20130203120004);the Fundamental Research Funds for the Central Universities,China(Grant Nos.201413B,201412B,and JB141303)
To improve the link efficiency and decrease the payloads in space explorations, a novel simultaneous communication and ranging method based on x-ray communication(XCOM) is proposed in this paper. A delicate signal s...
Project supported by the National Natural Science Foundation of China(Grant Nos.61172138 and 61401340);the Open Research Fund of the Academy of Satellite Application,China(Grant No.2014 CXJJ-DH 12);the Fundamental Research Funds for the Central Universities,China(Grant Nos.JB141303 and201413B);the Natural Science Basic Research Plan in Shaanxi Province,China(Grant No.2013JQ8040);the Research Fund for the Doctoral Program of Higher Education of China(Grant No.20130203120004);the Xi’an Science and Technology Plan,China(Grant.No CXY1350(4))
The log-polar transform (LPT) is introduced into the star identification because of its rotation invariance. An improved autonomous star identification algorithm is proposed in this paper to avoid the circular shift...
supported by the National Natural Science Foundation of China(Grant Nos.61172138 and 61401340);the Natural Science Basic Research Plan in Shaanxi Province of China(Grant No.2013JQ8040);the Research Fund for the Doctoral Program of Higher Education of China(Grant No.20130203120004);the Open Research Fund of the Academy of Satellite Application,China(Grant No.2014 CXJJ-DH 12);the Xi’an Science and Technology Plan,China(Grant No.CXY1350(4));the Fundamental Research Funds for the Central Universities,China(Grant Nos.201413B,201412B,and JB141303);the Open Fund of Key Laboratory of Precision Navigation and Timing Technology,National Time Service Center,Chinese Academy of Sciences(Grant Nos.2014PNTT01,2014PNTT07,and 2014PNTT08)
Range measurement has found multiple applications in deep space missions. With more and further deep space ex- ploration activities happening now and in the future, the requirement for range measurement has risen. In ...
Project supported by the National Natural Science Foundation of China(No.61172138);the Fundamental Research Funds for the Central Universities(Nos.K5051302015 and K5051302040);the Natural Science Basic Research Plan in Shaanxi Province of China(No.2013JQ8040);the Research Fund for the Doctoral Program of Higher Education of China(No.20130203120004)
X-ray pulsar navigation(XPNAV) is an attractive method for autonomous navigation of deep space in the future. Currently, techniques for estimating the phase of X-ray pulsar radiation involve the maximization of the ge...