TY - GEN
T1 - A method to calibrate the on-board timing based on pulsar observation
AU - Lan, Sheng Chang
AU - Zhang, Xu
AU - Pan, Rui
AU - Li, Jiong Hui
PY - 2011
Y1 - 2011
N2 - Considering the on-board clock stability, the paper presents a method of timing calibration strategy based on the observation of pulsars, a natural celestial source, in order to improve the timing accuracy. A calibration model is established and the error factors are considered based on the characteristic of pulsars' stable and periodical signals, and the pulsar timing residuals are caused by reference normal clock and pulsar itself, and the two influences are not correlative. Firstly, filters such as wavelet and HHT are implementing to data handling and error analysis, and then the paper investigated and developed a multiple-pulsar-observation method. Judging from the signals transmitted from different pulsars, the onboard timing residuals are determined by credibility weight of different pulsars' observation different components. Finally this paper comes to the conclusion via simulations. The method allows separating the error from a single pulsar timing errors and the on-board time can be obtained by filtering the observation residuals of pulsars observed, extracting the filtering result of different pulsars, and then choosing the weight according to the stability of timing result denoted with timing variance.
AB - Considering the on-board clock stability, the paper presents a method of timing calibration strategy based on the observation of pulsars, a natural celestial source, in order to improve the timing accuracy. A calibration model is established and the error factors are considered based on the characteristic of pulsars' stable and periodical signals, and the pulsar timing residuals are caused by reference normal clock and pulsar itself, and the two influences are not correlative. Firstly, filters such as wavelet and HHT are implementing to data handling and error analysis, and then the paper investigated and developed a multiple-pulsar-observation method. Judging from the signals transmitted from different pulsars, the onboard timing residuals are determined by credibility weight of different pulsars' observation different components. Finally this paper comes to the conclusion via simulations. The method allows separating the error from a single pulsar timing errors and the on-board time can be obtained by filtering the observation residuals of pulsars observed, extracting the filtering result of different pulsars, and then choosing the weight according to the stability of timing result denoted with timing variance.
KW - distribution weight
KW - fusion
KW - on-board timing
KW - pulsars
KW - residual local filtering
UR - https://www.scopus.com/pages/publications/80052205681
U2 - 10.1109/ICIEA.2011.5975968
DO - 10.1109/ICIEA.2011.5975968
M3 - 会议稿件
AN - SCOPUS:80052205681
SN - 9781424487554
T3 - Proceedings of the 2011 6th IEEE Conference on Industrial Electronics and Applications, ICIEA 2011
SP - 2265
EP - 2269
BT - Proceedings of the 2011 6th IEEE Conference on Industrial Electronics and Applications, ICIEA 2011
T2 - 2011 6th IEEE Conference on Industrial Electronics and Applications, ICIEA 2011
Y2 - 21 June 2011 through 23 June 2011
ER -