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  1. 131 地震研究所
  2. 東京大学地震研究所彙報
  3. 57
  4. 1
  1. 0 資料タイプ別
  2. 30 紀要・部局刊行物
  3. 東京大学地震研究所彙報
  4. 57
  5. 1

The Variable Period Hypothesis and Q of the Chandler Wobble Reexamined

https://doi.org/10.15083/0000032997
https://doi.org/10.15083/0000032997
e1f9b96c-f9dd-4343-b484-d65cfee4ea32
名前 / ファイル ライセンス アクション
ji0571001.pdf ji0571001.pdf (2.8 MB)
Item type 紀要論文 / Departmental Bulletin Paper(1)
公開日 2008-05-30
タイトル
タイトル The Variable Period Hypothesis and Q of the Chandler Wobble Reexamined
言語 en
言語
言語 eng
資源タイプ
資源 http://purl.org/coar/resource_type/c_6501
タイプ departmental bulletin paper
ID登録
ID登録 10.15083/0000032997
ID登録タイプ JaLC
その他のタイトル
その他のタイトル チャンドラー極運動の周波数変調仮説の検定とそのQに関する研究
著者 Okubo, Shuhei

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Okubo, Shuhei

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著者別名
識別子Scheme WEKO
識別子 128650
姓名 大久保, 修平
著者所属
著者所属 東京大学理学部
抄録
内容記述タイプ Abstract
内容記述 The Chandler wobble is one of the elastic-gravitational normal modes of the Earth. The eigenperiod is about 435 sidereal days, larger than the other modes by a factor 104, which gives the Chandler wobble an exotic status in the group of normal modes. The quality factor of the Chandler wobble, Qw, plays a critically important role in discussing the mantle rheology since the frequency dependence of the mantle Q is affected more seriously by the low frequency Chandler Qw than by the other seismic Q's. A problem should be resolved in advance so as to estimate Qw safely from the spectral analysis of the polar motion. Namely, significance of the variable Chandler period hypothesis. We test the hypothesis in two ways. First, we reexamine throughly the observational grounds of the hypothesis by applying the same scheme as employed by the proponents of the hypothesis to synthetic polar motion of a constant Chandler period. It is revealed that most of the evidence for the hypothesis is not definitive and it is also explained by the invariant Chandler period model as well. Next, we trace the time variation of the spectral structure of the Chandler wobble. For this purpose, we extend the high-resolution Instantaneous Frequency Analysis to be applicable to a complex-valued time series. Applying the technique to IPMS and BIH polar motion data, we find that the result favors the time-invariant Chandler period model. After confirming that there is no observational difficulty in the time-invariant Chandler period model, we estimate Qw by critically applying Maximum Entropy Spectral Analysis (MESA) to ILS and IPMS data. It is found that Qw lies in the range of 50≦Qw≦100 and Graber's result of Qw=600 is due to the erroneous choice of the length of the prediction error filter. Finally, we discuss the effect of the mantle anelasticity upon the period and Q of the Chandler wobble. We calculate the complex Love number k for the realistic Q models by Rayleigh's principle and relate it to Qw. The ratio of Qw to lower mantle Qm is found to be about 1.5 and it is shown to be consistent with the energy budget arguments. If the Chandler wobble energy is totally dissipated in the mantle, Qm should be frequency-dependent to account for the observed Qw of 50~100. If the frequency dependence of Qm is the power law, the power exponent is found to be 0.1~0.2. Anelasticity of the mantle is shown to lengthen the theoretical Chandler period by 7~11 days due to physical dispersion. Adding 29.8 days of ocean effect to the theoretical period of oceanless Earth yields 438~443 sidereal days as the Chandlerian period, in excellent agreement with the observed one.
抄録
内容記述タイプ Abstract
内容記述 チャンドラー極運動は地球のelastic-gravitationalな自由振動の一つのモードであり,瞬間自転軸が形状軸のまわりを反時計回りに回転する極運動である.その周期は約435日であり,他の地震学的なモードの周期よりも104倍以上も長いという特徴がある.したがって,そのQ値はマントルの非弾性的性質,とりわけ周波数依存性を議論する上できわめて重要となる.また地球科学の諸分野(地震学,海洋学,気象学,地球電磁気学)とチャンドラー極運動の関りの上でもQを確定することは大切になってくる.
書誌情報 東京大學地震研究所彙報 = Bulletin of the Earthquake Research Institute, University of Tokyo

巻 57, 号 1, p. 1-47, 発行日 1982-07-16
ISSN
収録物識別子タイプ ISSN
収録物識別子 00408972
書誌レコードID
収録物識別子タイプ NCID
収録物識別子 AN00162258
フォーマット
内容記述タイプ Other
内容記述 application/pdf
日本十進分類法
主題Scheme NDC
主題 453
出版者
出版者 東京大学地震研究所
出版者別名
Earthquake Research Institute, University of Tokyo
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