NTSC-IR
Wavelet Analysis Algorithm for Synthetic Pulsar Time
Chongxia Zhong; Tinggao Yang
2007
发表期刊Chinese Astronomy and Astrophysics
ISSN0275-1062
卷号31期号:4页码:443
摘要The pulsar time defined by a single pulsar is affected by several noises and in order to weaken their effects and acquire a much more stable time scale we define a synthetic pulsar time from many single pulsar times. Synthesis of the two pulsars, PSR B1855 + 09 and PSR B1937 + 21 is implemented by two methods: the classical weighting algorithm and the wavelet decomposition algorithm. The results are compared. The classical weighting algorithm is unable to take into consideration the different degrees of stability at different frequencies while the wavelet algorithm can, and thereby get better results.
关键词astrometry time method: data analysis
语种英语
文献类型期刊论文
条目标识符http://210.72.145.45/handle/361003/12312
专题中国科学院国家授时中心
作者单位中国科学院国家授时中心
第一作者单位中国科学院国家授时中心
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GB/T 7714
Chongxia Zhong,Tinggao Yang. Wavelet Analysis Algorithm for Synthetic Pulsar Time[J]. Chinese Astronomy and Astrophysics,2007,31(4):443.
APA Chongxia Zhong,&Tinggao Yang.(2007).Wavelet Analysis Algorithm for Synthetic Pulsar Time.Chinese Astronomy and Astrophysics,31(4),443.
MLA Chongxia Zhong,et al."Wavelet Analysis Algorithm for Synthetic Pulsar Time".Chinese Astronomy and Astrophysics 31.4(2007):443.
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