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141.
10余年来,通过对鲁东胶北地区太古宙地层的研究,原胶东群中剔除出大量的变质变形深成侵入岩,并从其底部分离出一套呈包体状态残存于花岗质岩石中的紫苏磁铁石英岩、二辉斜长角闪麻粒岩等,据此建立了唐家庄岩群。该岩群为一套经受角闪麻粒岩相高级变质的表壳岩组合,同位素测年数据为2763~2936Ma,与之相伴产出的超基性岩同位素地质年龄值为2693~3150Ma,其特征与鲁西地区沂水岩群相似,说明太古宙时鲁东和鲁西曾是一个统一的克拉通陆核。 相似文献
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峨眉山玄武岩的铂族元素地球化学特征 总被引:38,自引:4,他引:34
采用镍锍试金预处理中子活化分析方法,系统地测定了峨眉山玄武岩的铂族元素含量。14个样品的平均值为:Os=0.39ng/g,Ir=0.0698ng/g,Ru=0.49ng/g,Rh=0.25ng/g,Pt=7.71ng/g,Pd=5.48ng/g。相对于原始上地幔,峨眉山玄武岩的铂族元素分异明显,Os、Ir、Ru、Rh亏损,Pt、Pd富集。(Pt+Pd)/(Os+Ir+Ru)比值(平均13.96)和Pd/Ir比值(平均78.5)显著高于原始上地幔、地幔捕虏体、阿尔卑斯型橄榄岩及科马提岩。铂族元素配分模式为铂钯富集型。以上这些特征表明其原始岩浆为上地幔低程度部分熔融形成的玄武岩浆。 相似文献
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Group velocities of Rayleigh and Love waves along the paths across the Black Sea and partly Asia Minor and the Balkan Peninsula are used to estimate lateral variations of the crustal structure in the region. As a first step, lateral variations of group velocities for periods in the range 10–20 s are determined using a 2D tomography method. Since the paths are oriented predominantly in NE–SW or N–S direction, the resolution is estimated as a function of azimuth. The local dispersion curves are actually averaged over the extended areas stretched in the predominant direction of the paths. The size of the averaging area in the direction of the best resolution is approximately 200 km. As a second step, the local averaged dispersion curves are inverted to vertical sections of S-wave velocities. Since the dispersion curves in the 10–20 s period range are mostly affected by the upper crustal structure, the velocities are estimated to a depth of approximately 25 km. Velocity sections along 43° N latitude are determined separately from Rayleigh and Love wave data. It is shown that the crust under the sea contains a low-velocity sedimentary layer of 2–3 km thickness, localized in the eastern and western deeps, as found earlier from DSS data. Beneath the sedimentary layer, two layers are present with velocity values lying between those of granite and consolidated sediments. Velocities in these layers are slightly lower in the deeps, and the boundaries of the layers are lowered. S-wave velocities obtained from Love wave data are found to be larger than those from Rayleigh wave data, the difference being most pronounced in the basaltic layer. If this difference is attributed to anisotropy, the anisotropy coefficient = (SH - SV)/Smean is reasonable (2–3%) in the upper layers, and exceeds 9% in the basaltic layer. 相似文献
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INTRODUCTIONInhighlyextendedregions(β>1.5-2)suchastheBasinandRangeProvinceandpasivemargins,extensionaltectonicsystemischaract... 相似文献
149.
Different phenomena such as soil consolidation, erosion, and scour beneath an embedded footing supported on piles may lead to loss of contact between soil and the pile cap underside. The importance of this separation on the dynamic stiffness and damping of the foundation is assessed in this work. To this end, a numerical parametric analysis in the frequency domain is performed using a rigorous three‐dimensional elastodynamic boundary element–finite element coupling scheme. Dimensionless plots relating dynamic stiffness functions computed with and without separation effects are presented for different pile–soil configurations. Vertical, horizontal and rocking modes of oscillation are analyzed for a wide range of dimensionless frequencies. It is shown that the importance of separation is negligible for frequencies below those for which dynamic pile group effects start to become apparent. Redistribution of stiffness contributions between piles and footing is also addressed. Copyright © 2009 John Wiley & Sons, Ltd. 相似文献
150.
Taeyoung Lee Melvin Leok N. Harris McClamroch 《Celestial Mechanics and Dynamical Astronomy》2007,98(2):121-144
Equations of motion, referred to as full body models, are developed to describe the dynamics of rigid bodies acting under
their mutual gravitational potential. Continuous equations of motion and discrete equations of motion are derived using Hamilton’s
principle. These equations are expressed in an inertial frame and in relative coordinates. The discrete equations of motion,
referred to as a Lie group variational integrator, provide a geometrically exact and numerically efficient computational method
for simulating full body dynamics in orbital mechanics; they are symplectic and momentum preserving, and they exhibit good
energy behavior for exponentially long time periods. They are also efficient in only requiring a single evaluation of the
gravity forces and moments per time step. The Lie group variational integrator also preserves the group structure without
the use of local charts, reprojection, or constraints. Computational results are given for the dynamics of two rigid dumbbell
bodies acting under their mutual gravity; these computational results demonstrate the superiority of the Lie group variational
integrator compared with integrators that are not symplectic or do not preserve the Lie group structure. 相似文献