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Use of wiener filtration in wavelet domain in ensemble pulsar time algorithm
Zhong Chong-Xia; Yang Ting-Gao
2007
发表期刊ACTA PHYSICA SINICA
ISSN1000-3290
卷号56期号:10页码:6157-6163
摘要Pulsars rotate extremely stably, they can be used as time standard. However, pulsar time defined by single pulsar is influenced by several noise resources. To weaken these influences to get a more stable time scale, one can take ensemble analysis to obtain the ensemble pulsar time. Since different pulsars have different rotation frequency, and the noise source have different influence on different frequency of each pulsars we can apply wavelet analysis to integrate the pulsar time, and this algorithm can take consideration of the long-term and short-term stability of pulsar time. On the other hand, the pulsar timing residuals are caused by reference atomic clock and pulsar itself, so we can apply Wiener filtration analysis,to distinguish the two parts, and then calculate the ensemble pulsar time with the residuals after removing the error of reference atomic clock. Based on both of the two algorithms, a new algorithm of Wiener filtration in wavelet domain has been presented, which combines the merits of wavelet analysis and Wiener filtration and can remove the noise influence to pulsar time more effectively. Experimental results prove that Wiener filtration in wavelet domain can reduce noise influence of pulsar timing residuals effectively.
部门归属守时理论与方法研究室
关键词Ensemble Pulsar Time Wavelet Analysis Wiener Filtration Wiener
收录类别SCI
语种英语
WOS记录号WOS:000250313000102
引用统计
文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/4752
专题守时理论与方法研究室
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Zhong Chong-Xia,Yang Ting-Gao. Use of wiener filtration in wavelet domain in ensemble pulsar time algorithm[J]. ACTA PHYSICA SINICA,2007,56(10):6157-6163.
APA Zhong Chong-Xia,&Yang Ting-Gao.(2007).Use of wiener filtration in wavelet domain in ensemble pulsar time algorithm.ACTA PHYSICA SINICA,56(10),6157-6163.
MLA Zhong Chong-Xia,et al."Use of wiener filtration in wavelet domain in ensemble pulsar time algorithm".ACTA PHYSICA SINICA 56.10(2007):6157-6163.
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