Chandler wobble period and Q derived by wavelet transform

被引:2
作者
Liao, DC [1 ]
Zhou, YH
机构
[1] Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
[2] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
来源
CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS | 2004年 / 4卷 / 03期
关键词
polar motion; Chandler wobble; wavelet transform; instantaneous period;
D O I
10.1088/1009-9271/4/3/247
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We apply complex Morlet wavelet transform to three polar motion data series, and derive quasi-instantaneous periods of the Chandler and annual wobble by differencing the wavelet transform results versus the scale factor, and then find their zero points. The results show that the mean periods of the Chandler (annual) wobble are 430.71 +/- 1.07 (365.24 +/- 0.11) and 432.71 +/- 0.42 (365.23 +/- 0.18) mean solar days for the data sets of 1900-2001 and 1940-2001, respectively. The maximum relative variation of the quasi-instantaneous period to the mean of the Chandler wobble is less than 1.5% during 1900-2001 (3%-5% during 1920-1940), and that of the annual wobble is less than 1.6% during 1900-2001. Quasi-instantaneous and mean values of Q are also derived by using the energy density-period profile of the Chandler wobble. An asymptotic value of Q = 36.7 is obtained by fitting polynomial of exponential of sigma(-2) to the relationship between Q and sigma during 1940-2001.
引用
收藏
页码:247 / 257
页数:11
相关论文
共 50 条
[31]   On the double-peak spectrum of the Chandler wobble [J].
J.Y. Guo ;
H. Greiner-Mai ;
L. Ballani ;
H. Jochmann ;
C.K. Shum .
Journal of Geodesy, 2005, 78 :654-659
[32]   A stochastic excitation model for the study of the Chandler wobble [J].
Huang, SY ;
Liao, XH ;
Zhu, YL .
CHINESE ASTRONOMY AND ASTROPHYSICS, 2002, 26 (01) :49-56
[33]   Anomalies of the Chandler Wobble in 2010s [J].
L. V. Zotov ;
N. S. Sidorenkov ;
Ch. Bizouard .
Moscow University Physics Bulletin, 2022, 77 :555-563
[34]   Modern observations of the effect of earthquakes on the Chandler wobble [J].
Smylie, D. E. ;
Henderson, Gary A. ;
Zuberi, Midhat .
JOURNAL OF GEODYNAMICS, 2015, 83 :85-91
[35]   Can we explain the post-2015 absence of the Chandler wobble? [J].
Yamaguchi, Ryuji ;
Furuya, Masato .
EARTH PLANETS AND SPACE, 2024, 76 (01)
[36]   Chandler Wobble and Free Core Nutation: Theory and Features [J].
Na, Sung-Ho ;
Roh, Kyoung-Min ;
Cho, Tungho ;
Yoo, Sung-Moon ;
Choi, Byungkyu ;
Yoon, Hasu .
JOURNAL OF ASTRONOMY AND SPACE SCIENCES, 2019, 36 (01) :11-20
[37]   Did the 1977 Sumba earthquake excite the Chandler wobble? [J].
Alfonsi, L ;
Piersanti, A ;
Spada, G .
EARTH AND PLANETARY SCIENCE LETTERS, 1997, 153 (3-4) :287-292
[38]   Effect of the stratified ocean of the core upon the Chandler wobble [J].
Braginsky, SI .
PHYSICS OF THE EARTH AND PLANETARY INTERIORS, 2000, 118 (3-4) :195-203
[39]   Chandler wobble excitation by catastrophic flooding of the Black Sea [J].
Spada, G ;
Alfonsi, L ;
Boschi, E .
ANNALI DI GEOFISICA, 1999, 42 (04) :749-754
[40]   Amplitude and phase variations of Earth's Chandler wobble under continual excitation [J].
Chao, Benjamin F. ;
Chung, Wei-Yung .
JOURNAL OF GEODYNAMICS, 2012, 62 :35-39