{"title":"Characteristics of the chandler wobble","authors":"Wu Shou-Xian, Wang Shu-he, Hua Ying-min","doi":"10.1016/0146-6364(80)90043-2","DOIUrl":null,"url":null,"abstract":"<div><p>We carried out a spectral analysis (by FFT and periodograms) on a homogenized set of data of coordinates of the Earth's pole in the period 1900–1969.9, and found the Chandler wobble to have 4 peaks at periods of 1.142, 1.169, 1.199 and 1.230 years. The two main peaks at 1.169 and 1.199 years have equal amplitudes (TABLE 4 and Fig. 1). According to Fedrov and Yatskiv's (1964) interpretation of sudden phase changes, our data would give a natural period of 1.184 years, but the observed asymmetry between the two secondary peaks is a difficulty for this interpretation. The observed multiplicity of peaks can also be explained by the theory of amplitude modulation, if we suppose there is a modulating oscillation with a period around 48 years. In this case, the natural period of the Chandler wobble would be 1.199 years; but this interpretation also has some difficulties.</p></div>","PeriodicalId":100241,"journal":{"name":"Chinese Astronomy","volume":"4 2","pages":"Pages 127-135"},"PeriodicalIF":0.0000,"publicationDate":"1980-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://sci-hub-pdf.com/10.1016/0146-6364(80)90043-2","citationCount":"1","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Chinese Astronomy","FirstCategoryId":"1085","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/0146636480900432","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 1
Abstract
We carried out a spectral analysis (by FFT and periodograms) on a homogenized set of data of coordinates of the Earth's pole in the period 1900–1969.9, and found the Chandler wobble to have 4 peaks at periods of 1.142, 1.169, 1.199 and 1.230 years. The two main peaks at 1.169 and 1.199 years have equal amplitudes (TABLE 4 and Fig. 1). According to Fedrov and Yatskiv's (1964) interpretation of sudden phase changes, our data would give a natural period of 1.184 years, but the observed asymmetry between the two secondary peaks is a difficulty for this interpretation. The observed multiplicity of peaks can also be explained by the theory of amplitude modulation, if we suppose there is a modulating oscillation with a period around 48 years. In this case, the natural period of the Chandler wobble would be 1.199 years; but this interpretation also has some difficulties.