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Titlebook: Earthquake Displacement Fields and the Rotation of the Earth; A NATO Advanced Stud L. Mansinha,D. E. Smylie,A. E. Beck Book 1970 Springer S

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发表于 2025-3-21 19:42:21 | 显示全部楼层 |阅读模式
书目名称Earthquake Displacement Fields and the Rotation of the Earth
副标题A NATO Advanced Stud
编辑L. Mansinha,D. E. Smylie,A. E. Beck
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Earthquake Displacement Fields and the Rotation of the Earth; A NATO Advanced Stud L. Mansinha,D. E. Smylie,A. E. Beck Book 1970 Springer S
描述The seeds of this conference were sown with the publication by Press, in 1965, of a paper in which he suggested that the displacement field due to a major earthquake may extend over much greater distances than had been thought possible before. Later on, Mansinha and Smylie pointed out that if Press was correct then, since the redistri­ bution of significant quantities of mass was involved, the inertia tensor of the earth would be altered and thus cause the earth to wobble; this revived the idea that earth­ quakes might be the long sought source for maintaining the Chandler Wobble. They argued that since earthquakes are sudden events it should be worthwhile trying to determine if there was any correlation between sudden changes in the Chandler term of the pole path and major earthquakes. Furthermore, since displacements occur both before and after an earthquake it might be possible to obtain a few days warning of a major earthquake by making instantaneous observations of the pole path. Analysis of the data indicated some correlation but, as often happens in science in general and in geophysics in particular, the results were not conclusive because of imperfect theory and the need fo
出版日期Book 1970
关键词Libration; interferometry; solar; solar activity
版次1
doihttps://doi.org/10.1007/978-94-010-3308-4
isbn_softcover978-94-010-3310-7
isbn_ebook978-94-010-3308-4Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 1970
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发表于 2025-3-21 23:58:28 | 显示全部楼层
https://doi.org/10.1007/978-94-010-3308-4Libration; interferometry; solar; solar activity
发表于 2025-3-22 03:36:45 | 显示全部楼层
978-94-010-3310-7Springer Science+Business Media Dordrecht 1970
发表于 2025-3-22 07:51:14 | 显示全部楼层
https://doi.org/10.1007/978-3-030-93027-1 faults are used to obtain empirical relationships between fault dimensions and earthquake magnitude. It is shown that only large earthquakes contribute significantly to the displacement fields at large distances from a fault zone. The mechanics of fault slippage, and some of the problems of the ela
发表于 2025-3-22 08:49:45 | 显示全部楼层
Paul Bratley,Bennett L. Fox,Linus E. Schragee to finite dip-slip and strike-slip faults. The theory is applied to strain observations from the Alaska earthquake of March 28, 1964. It is shown that the theoretical values are within an order of magnitude of the observed values and are of the correct sign..The method can be extended to derive th
发表于 2025-3-22 16:44:56 | 显示全部楼层
https://doi.org/10.1007/978-3-642-71402-3he collaboration of more than 50 stations in 24 countries — Algeria, Argentina, Australia, Belgium, Brazil, Canada, Chile, China, Czechoslovakia, Equador, Finland, France, Germany, Italy, Japan, Poland, Rumania, South Africa, Spain, Switzerland, UK, USA, USSR and Yugoslavia.
发表于 2025-3-22 19:52:11 | 显示全部楼层
The Business Case for Sustainability,e observations (80 instruments); precautions are taken to keep an homogeneous system in spite of the changes in the list of the participating observatories. Recent results are presented. The accuracy on . and . is 0″.01; on UT1, 0..001 (standard errors).
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发表于 2025-3-23 04:16:22 | 显示全部楼层
Holly Hassel,Christie Launius,Susan Rensingot occur in speed but do in acceleration, about every 4 years. The motion of the mean pole consists of a progressive component of 10 cm/yr plus a 24-year oscillation. A deviation for 1966.0 is noted. No correlation is found between earthquakes and changes in rotational speed or acceleration.
发表于 2025-3-23 06:53:24 | 显示全部楼层
John Marks MA, MD, FRCP, FRCPathlar changes in mean latitudes of the cooperative stations on + 39°8′ irrespective of the effect by the secular drift of the mean pole. Local drifts of — 0″.00156/year for Mizusawa and of + 0″.00105/year for Ukiah were derived from the analyses of the notable increases in the residual latitudes of th
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