Comparison of high frequency variations of the atmosphere and the polar motion
文献类型:期刊论文
作者 | Wang, BW; Gu, ZN; Jin, WJ |
刊名 | CHINESE ASTRONOMY AND ASTROPHYSICS
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出版日期 | 2002 |
卷号 | 26期号:1页码:88-96 |
关键词 | excitation function atmospheric angular momentum high-frequency oscillation |
英文摘要 | The inferred excitation function X-m derived from EOP(IERS 97C04) polar motion series and the series X-p and X-ib(p) of the atmospheric angular momentum (AAM) provided by NCEP/NCAR for 1988-1999 are used to assess the contribution of AAM to the polar motion. Power spectra and complex wavelet analysis show that there are high peaks and similar structures in X-m and X-p, and their cross correlation coefficient is 0.75 (retrograde) and 0.60 (prograde). The peaks in X-ib(p) are lower. The phase of X-p is about one day ahead of X-m. The indications are that atmosphere variation is the main source of excitation of polar motion in the high-frequency range, and particularly so for the retrograde motion, while there may be other sources. |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | EARTHS |
收录类别 | SCI |
语种 | 英语 |
WOS记录号 | WOS:000174388500011 |
源URL | [http://119.78.226.72/handle/331011/28678] ![]() |
专题 | 上海天文台_星系宇宙学重点实验室 |
作者单位 | Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, BW,Gu, ZN,Jin, WJ. Comparison of high frequency variations of the atmosphere and the polar motion[J]. CHINESE ASTRONOMY AND ASTROPHYSICS,2002,26(1):88-96. |
APA | Wang, BW,Gu, ZN,&Jin, WJ.(2002).Comparison of high frequency variations of the atmosphere and the polar motion.CHINESE ASTRONOMY AND ASTROPHYSICS,26(1),88-96. |
MLA | Wang, BW,et al."Comparison of high frequency variations of the atmosphere and the polar motion".CHINESE ASTRONOMY AND ASTROPHYSICS 26.1(2002):88-96. |
入库方式: OAI收割
来源:上海天文台
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