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Titlebook: Geodynamics of Lithosphere & Earth’s Mantle; Seismic Anisotropy a Jaroslava Plomerová,Robert C. Liebermann,Vladislav Conference proceedings

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發(fā)表于 2025-3-21 16:07:10 | 只看該作者 |倒序瀏覽 |閱讀模式
書目名稱Geodynamics of Lithosphere & Earth’s Mantle
副標(biāo)題Seismic Anisotropy a
編輯Jaroslava Plomerová,Robert C. Liebermann,Vladislav
視頻videohttp://file.papertrans.cn/384/383125/383125.mp4
叢書名稱Pageoph Topical Volumes
圖書封面Titlebook: Geodynamics of Lithosphere & Earth’s Mantle; Seismic Anisotropy a Jaroslava Plomerová,Robert C. Liebermann,Vladislav Conference proceedings
描述Plate tectonics has significantly broadened our view of the dynamics of continental evolution, involving both the processes currently active at the surface and those extending deep into the interior of the Earth. Seismic anisotropy provides some of the most diagnostic evidence for mapping past and present deformation of the entire crustmantle system. This volume contains papers presented originally at an international workshop at the Chateau of Trest in the Czech Republic in 1996. This workshop brought together geophysicists and geologists who work in the field of observational and theoretical seismology, mineral and rock physics, gravity studies and geodynamic modelling. Topics include large-scale anisotropy of the Earth‘s mantle, mantle heterogeneity vs. anisotropy 3-D velocity and density structures and inferences on mantle dynamics, mineral and rock physics studies, and mathematical aspects of complex wave propagation.
出版日期Conference proceedings 1998
關(guān)鍵詞Deformation; Seismic Anisotropy; evolution; geodynamics; geology; geophysics; lithosphere; mineral; modellin
版次1
doihttps://doi.org/10.1007/978-3-0348-8777-9
isbn_softcover978-3-0348-9770-9
isbn_ebook978-3-0348-8777-9Series ISSN 2504-3625 Series E-ISSN 2504-3633
issn_series 2504-3625
copyrightSpringer Basel AG 1998
The information of publication is updating

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發(fā)表于 2025-3-21 23:18:40 | 只看該作者
,Die Geburtshilfe und Gyn?kologie,nly in boundary layers of convective mantle..We review in this paper, the seismic data sets which provide insight into the location at depth of large-scale anisotropy from the .-layer up to the lithosphere. In addition to the well-documented seismic anisotropy in the lithosphere and asthenosphere, t
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地板
發(fā)表于 2025-3-22 04:58:57 | 只看該作者
https://doi.org/10.1007/978-3-662-06665-2ude of the delay time of the upper layer, the lower layer must lie within the asthenosphere. At other stations splitting parameters are consistent with an anisotropic one-layer model for the upper mantle. Stations near the Bohemian Massif show fast directions near EW. Throughout NE Germany the direc
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發(fā)表于 2025-3-22 11:29:35 | 只看該作者
Meerwassertrinkkur und Mineralstoffwechsel,for adjacent stations, our results show a large scatter of the individual splitting parameters for the set of events used. The magnitude of the splitting time suggests that the deformation extends below the lithosphere and that the thickness of the anisotropic structure is at least 100–200 km..For s
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發(fā)表于 2025-3-22 13:42:11 | 只看該作者
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發(fā)表于 2025-3-22 18:45:17 | 只看該作者
https://doi.org/10.1007/978-3-663-02187-2t polarization direction we determine is quite parallel to the opening of the Ross Sea, an active rift system, but also to the Absolute Plate Motion direction. Therefore, we assume that the identified anisotropy may be induced by the extension, activated by plate motion and is still related to it.
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發(fā)表于 2025-3-23 01:41:26 | 只看該作者
https://doi.org/10.1007/978-3-642-94325-6iding plate extension. However, fast directions beneath the Japan Sea, western Honshu, and Sakhalin Island are highly oblique to subducting plate motion and parallel to present or past overriding plate shearing. Models of back-arc mantle flow that are driven by viscous coupling to local plate motion
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發(fā)表于 2025-3-23 08:44:15 | 只看該作者
Das ?Bild der Bilder?: Dürers , (1514)f the depth and geometry of the Moho through the receiver function technique is in progress. Tomographic results from the northernmost 1994 and the central 1995 teleseismic experiments confirm that a high-velocity anomaly (HVA) does exist in the upper 200–250 km and is confined to the northern Apenn
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