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When galaxies collide, stars are born. But many such close encounters also result in the formation of clusters with many of the characteristics of ancient globular clusters. Richard de Grijs argues the case that this process represents continuing formation of globular clusters in a hierarchical scheme of galaxy formation. 相似文献
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Ulrich Klein 《地球物理与天体物理流体动力学》2013,107(1-3):27-34
Abstract The observational facts about magnetic fields in galactic halos are reviewed. The existence, origin and significance of poloidal field components are described. Observational evidence that magnetic fields channel winds from active galactic centres is discussed. Field strengths adduced from the radio polarizations of edge-on galaxies are given. Priorities for future research are suggested. 相似文献
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层间隔震技术评述 总被引:32,自引:5,他引:32
祁皑 《地震工程与工程振动》2004,24(6):114-120
层间隔震结构是隔震技术的新发展,它将隔震层设置在建筑物某层柱子和楼板之间进行结构的地震反应控制。层间隔震结构在减震机理、振动特性以及设计方法等诸多方面有别于基础隔震结构和屋盖隔震结构。本文对层间隔震结构的适用范围、优点以及其在实际工程中的应用情况进行了综述,最后,指出了层问隔震结构需要进一步研究的问题。现有的研究成果和工程应用情况表明,层间隔震结构具有明确的减震效果,施工方便,是一种具有发展前途的减震体系。 相似文献
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G.J. Barnes 《Geophysical Prospecting》2019,67(6):1620-1625
In airborne gravity gradiometry, the Gravity Module Assembly is an optional gravimeter unit that is mounted on the same stabilized platform as the Full Tensor Gradiometer. Direct measurements of the gravity field are needed from this device to constrain the long wavelengths when gradient data are integrated mathematically to form high-resolution gravity fields. The Gravity Module Assembly is, however, capable of providing independent gravity data with a specification approaching that expected from a dedicated airborne gravity system. Presented here is an error analysis of data from this instrument collected alongside the Full Tensor Gradiometer during an airborne survey. By having both gradiometry and gravity datasets, comparisons of the information content in these two types of measurement are made. 相似文献
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多元素能谱测井通过全能谱分析方法求取单个地层元素的产额,进而求取元素重量百分含量和矿物百分含量,为识别复杂油气藏岩石类型和矿物类型、建立复杂油气藏新的测井解释模型及应用正确评价方法开辟了新的途径,为地质问题和工程问题的解决提供了新的手段,全能谱分析方法研究是当前国内核辐射测井研究热点之一.本文表分析多元素能谱测井的重要... 相似文献
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Yvonne Battiau-Queney 《地球表面变化过程与地形》1984,9(3):229-252
The classical explanation of the development of the Welsh landscape by the effects of a pulsed ‘eustatic’ uplift during the Cenozoic times is challenged by new data on the geology and geomorphology of Wales and the adjacent regions. The post-Caledonian surface developed over most of Wales in the upper Westphalian plays a major role in landform development. Since its emergence before mid-Cretaceous times, the Welsh Massif has suffered a long subaerial evolution which favoured a powerful chemical weathering. In Anglesey and St. David's Land, residual hills were formed by a process of differential weathering, and downwearing in saprolites. The Millstone Grit quartzites have been deeply weathered and dolines or flat-bottomed basins have been developed. From Cretaceous to Miocene times, a morphotectonic equilibrium has existed between uplift and denudation, so that, in the major part of Wales, the original planation surface was constantly maintained by lowering on itself and in some places it is possible to prove that no more than a few dozen metres of rock thickness disappeared during that period. Several main escarpments were produced by the warping of the planation surface along sharp flexures, during Neogene times. The Cenozoic vertical movements were controlled by the Caledonian or pre-Caledonian tectonic pattern which has divided the continental crust into major structural units. Welsh tectonic development is related to the opening of the North Atlantic, associated stresses reactivating ancient lines of weakness in the heterogeneous lower crust or upper mantle. 相似文献
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Landscapes subject to constant forcing tend to evolve toward equilibrium states in which individual landforms have similar characteristics. Yet, even in landscapes at or near equilibrium, there can be significant variability among individual landforms. Furthermore, sites subject to similar processes and conditions can have different mean landform characteristics. This variability is often ascribed to on‐going transient evolution, or to heterogeneity in processes, material properties, forcing, or boundary conditions. Three surprising outcomes of landform evolution models suggest, however, that such variability could arise in equilibrium landscapes without any heterogeneity in the physical processes shaping the topography. First, homogeneous systems subjected to constant forcing can generate a heterogeneous distribution of equilibrium landforms. Second, even simple non‐linear systems can have multiple stable equilibrium states. Third, evolving landscapes can exhibit path dependence and hysteresis. We show how these three mechanisms can produce variability in landforms that arises from the characteristics of the initial topographic surface rather than from heterogeneity in geomorphic processes. Numerical experiments on the formation of low‐order fluvial valleys and transportational cyclic steps in erodible streambeds illustrate why it is important to consider the influence of initial conditions when comparing models with natural topography, estimating the uncertainty of model predictions, and studying how landscapes respond to disturbances. Copyright © 2011 John Wiley & Sons, Ltd. 相似文献
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中国地震工程地质学之发展 总被引:2,自引:0,他引:2
综述了中国地震工程地质学(亦称为地震岩土工程学)在过去50年中的发展,历史地震年表、中国地震目录、中国地震区划图和新中国地震烈有等是本学科发展初期的里程碑。在进一步的发展中,逐步形成了两个学科分支:区域地震危险性评定(SHA)和场地抗震性能评价。1966~1976年的一系列强烈地震发生后,SHA和地震小区划的方法有了迅速改进,更深刻地认识了局部地条件对地震中强地震动和场地失效的影响。若干“地硅工程 相似文献
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《Astronomy& Geophysics》2008,49(2):2.38-2.38
A series of public lectures at Burlington House on topics of broad interest has got off to a good start – and there's more to come this year, so tell your friends! 相似文献
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《Astronomy& Geophysics》2009,50(5):5.12-5.19
Simon P Driver, Peder Norberg, Ivan K Baldry, Steven P Bamford, Andrew M Hopkins, Jochen Liske, Jon Loveday, John A Peacock and the GAMA Survey Team (Galaxy and Mass Assembly) review progress on the latest large galaxy redshift survey now underway on the 3.9 m Anglo-Australian Telescope. 相似文献
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The evolution of bubble size distributions in volcanic eruptions 总被引:1,自引:0,他引:1
J.D. Blower J.P. Keating H.M. Mader J.C. Phillips 《Journal of Volcanology and Geothermal Research》2003,120(1-2):1-23
We review observations of bubble size distributions (BSDs) generated during explosive volcanic eruptions and laboratory explosions, as inferred from vesicle size distributions found in the end products. Unimodal, polymodal, exponential and power law BSDs are common, even in the absence of coalescence, and both power law and exponential distributions have been generated in the same eruption. To date theoretical models have proposed incompatible mechanisms for producing the various distributions. We here present a unifying mechanism. Data from our laboratory analogue experiments suggest that power law distributions are associated with highly non-equilibrium degassing. A numerical model is developed in which bubbles nucleate repeatedly and grow in the spaces between those of previous generations, where, in a non-equilibrium degassing scenario, the volatile concentration remains high. This process causes the BSD to evolve from unimodal, through exponential, into a power law. The exponent of the power law is a measure of the number of nucleation events, or the duration of the nucleation period compared with the timescale of bubble growth. The mathematical inevitability of the evolution from unimodal (Poissonian) to power law is discussed. The findings may resolve the apparent contradiction between the equilibrium degassing conduit flow models and the non-equilibrium degassing conditions derived from bubble growth models of explosive volcanic eruptions. The process of ongoing nucleation is the mechanism whereby the volcanic system maintains near-equilibrium in the case of rapid depressurisation and slow volatile diffusion. 相似文献
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Integrating migration velocity analysis and full waveform inversion can help reduce the high non‐linearity of the classic full waveform inversion objective function. The combination of inverting for the long and short wavelength components of the velocity model using a dual objective function that is sensitive to both components is still very expensive and have produced mixed results. We develop an approach that includes both components integrated to complement each other. We specifically utilize the image to generate reflections in our synthetic data only when the velocity model is not capable of producing such reflections. As a result, we get the migration velocity analysis working when we need it, and we mitigate its influence when the velocity model produces accurate reflections (possibly first for the low frequencies). This is achieved using a novel objective function that includes both objectives. Applications to a layered model and the Marmousi model demonstrate the main features of the approach. 相似文献
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