中国大陆动力学研究内涵与轨迹的思考   总被引：4，自引：0，他引：4       下载免费PDF全文

滕吉文  皮娇龙  杨辉  刘少华 《地球物理学报》2012,55(3):851-862

大陆动力学已成为21世纪地球科学研究中的热点和中坚,在它面对当今资源、能源、灾害和环境等社会与经济快速发展需求日益增长的同时,是机遇,却也是挑战.因此厘定其研究的内涵和导向是十分重要的.基于多年的研究实践和探索,本文将对以下五个方面进行讨论:1)大陆动力学研究的内涵与界定;2)大陆动力学研究的导向和轨迹;3)大陆动力学研究中地球物理反演结果和解释中的矛盾;4)强化发展学科交叉以构成交叉科学;5)对2011年大陆动力学委员会学术活动的思考.  相似文献   

钢结构高温响应影响因素的研究     

江雪玲  魏德敏 《地震学刊》2012,(1):111-116

根据考虑几何和材料非线性及温度沿杆件截面高度线性分布等因素对钢结构常温和高温响应影响的基本方程,用自行编制的计算程序对单层双跨钢框架进行结构非线性温度响应研究,分析了弯曲应变、屈强比、梁柱刚度比、初始弹性模量等因素对结构响应的影响,并研究了温度步长、保护层厚度对结构耐火时间的影响。由计算结果发现,弯曲应变、初始弹性模量、梁柱线刚度比对梁跨中挠度及边柱柱顶水平位移影响较大,而对柱顶竖向位移影响不明显;当结构有防火保护层时,时间步长对结构耐火时间的影响不大,而保护层厚度对结构耐火时间的影响较明显。  相似文献   

汶川地震形成位移场的空间分布     

白玉柱  周庆  徐锡伟  徐杰  周本刚 《地球物理学进展》2012,27(1):29-37

采用Yoshimitsu Okada及Steketee的断裂位错模型和汶川地震现有成果,通过坐标转换和合成矢量的方法将断裂位错模型用于映秀—北川断裂、灌县—安县断裂和北川—青川断裂组成的断裂系统的错动研究中,理论上计算龙门山近断裂地区的水平位移场(包括沿走向和垂直走向方向)和垂直位移场从震源到地表的分布.模型参数源于现有的研究成果和野外实地考察,计算得到的地表位移场与先前研究成果,包括GPS实测数据,具有的近似性表明了模型的正确性.但GPS只能测定地表水平和垂直变形,对于地下变形情况及其分布却无法描述;目前对于地下变形的研究主要基于对大量仪器记录的地震资料进行反演或通过野外观测进行推测;但是反演多集中于空间较大范围,这样虽可阐述断裂运动引起的大范围位移趋势,而对于震源附近空间介质位移的描述却略显粗糙;同时,野外观测误差较大.本文通过理论模型计算汶川地震中近断裂区域(距断裂50km)内的位移及分布.由计算发现在近断裂区域内垂直位移场和垂直走向方向位移场变化趋势一样,幅值都是从震源到地表逐渐减小;沿断裂走向方向的水平位移场从震源到地表逐渐变大,同时计算还表明位移场的变化在断裂上盘比下盘剧烈,余震分布主要集中于断裂上盘,这说明余震分布和位移剧烈程度存在某种相关性.  相似文献   

晚第四纪中国北方沙地风沙沉积的Zr/Rb比值特征及意义     

周亚利  鹿化煜  弋双文  王先彦 《中国沙漠》2013,33(6):1661-1669

Zr/Rb比值因不受后期成壤作用影响,在黄土高原黄土堆积中可作为较好的冬季风气候替代性指标。与黄土沉积相比,中国北方沙地的气候变化研究相对较弱,能够敏感反映沙地气候变化的替代性指标仍处于探索阶段。本文选取东亚季风控制区的毛乌素沙地、浑善达克沙地和科尔沁沙地11个典型的风成沉积序列,对Zr/Rb比值及其意义进行了研究。通过全岩样品Zr、Rb元素含量、Zr/Rb比值与平均粒径和>63 μm的粗颗粒百分含量对比分析,发现在毛乌素沙地,Zr/Rb比值与粗颗粒百分含量和平均粒径成正相关关系,与黄土高原的变化趋势相似,可作为冬季风强度的替代性指标。而在浑善达克沙地和科尔沁沙地,虽然Rb含量在砂质古土壤层中随着细颗粒物质的增加而增大,与毛乌素沙地的变化相同;但是,Zr含量也表现出增加趋势,导致Zr/Rb比值变化趋势与毛乌素沙地相反。其主要原因可能是沙地所处的构造地貌单元不同,物源区存在差异。因此,Zr/Rb比值作为冬季风的替代性指标在不同沙地应用需要慎重分析。  相似文献   

河流附近非水平初始面潜水渗流分析     

曹彭强  束龙仓  鲁程鹏 《吉林大学学报(地球科学版)》2014,44(1):295

考虑初始面非水平条件,建立河流边界控制下的半无限含水层渗流模型,提出非水平初始面及其相关参数（a、t_N）的简易计算方法,并探讨模型的适用条件。分析表明,该法适用于观测数据较少、地下水水位变幅相对于潜水含水层厚度较小、且观测孔距河岸较近条件下河流附近潜水含水层渗流计算。结合实例,采用查表法和配线法求解模型。计算结果表明:参数a和t_N的计算值不同,水位计算误差在0.02 m以内,较原公式精度有明显提高。新模型为初始面非水平条件下的潜水渗流计算提供一种简易方法。  相似文献   

叠加褶皱研究进展综述   总被引：1，自引：0，他引：1  

陈龙  施炜 《地质力学学报》2014,20(4):455-468

叠加褶皱作为地壳构造变形中一种常见的地质现象, 对于确定多期变形和构造运动期次, 探讨构造演化历史以及内外生矿床的空间分布、形成与变形特征均有重要研究意义。在回顾叠加褶皱研究历史与近年来取得的主要进展基础上, 系统地总结了叠加褶皱几何学与运动学特征, 指出叠加褶皱主要有纵弯褶皱作用、横弯褶皱作用及剪切褶皱作用3种成因机制。在此基础上, 选取典型的叠加褶皱, 剖析了其构造样式及形成机制, 并探讨了叠加褶皱研究的难点与可行研究方法。   相似文献   

Multiridge Euler deconvolution   总被引：1，自引：0，他引：1  

Giovanni Florio  Maurizio Fedi 《Geophysical Prospecting》2014,62(2):333-351

Potential field interpretation can be carried out using multiscale methods. This class of methods analyses a multiscale data set, which is built by upward continuation of the original data to a number of altitudes conveniently chosen. Euler deconvolution can be cast into this multiscale environment by analysing data along ridges of potential fields, e.g., at those points along lines across scales where the field or its horizontal or vertical derivative respectively is zero. Previous work has shown that Euler equations are notably simplified along any of these ridges. Since a given anomaly may generate one or more ridges we describe in this paper how Euler deconvolution may be used to jointly invert data along all of them, so performing a multiridge Euler deconvolution. The method enjoys the stable and high‐resolution properties of multiscale methods, due to the composite upward continuation/vertical differentiation filter used. Such a physically‐based field transformation can have a positive effect on reducing both high‐wavenumber noise and interference or regional field effects. Multiridge Euler deconvolution can also be applied to the modulus of an analytic signal, gravity/magnetic gradient tensor components or Hilbert transform components. The advantages of using multiridge Euler deconvolution compared to single ridge Euler deconvolution include improved solution clustering, increased number of solutions, improvement of accuracy of the results obtainable from some types of ridges and greater ease in the selection of ridges to invert. The multiscale approach is particularly well suited to deal with non‐ideal sources. In these cases, our strategy is to find the optimal combination of upward continuation altitude range and data differentiation order, such that the field could be sensed as approximately homogeneous and then characterized by a structural index close to an integer value. This allows us to estimate depths related to the top or the centre of the structure.  相似文献   

Discovery of magnetic fields in three He variable Bp stars with He and Si spots     

M. Briquet  S. Hubrig  M. Schller  P. De Cat 《Astronomische Nachrichten》2007,328(1):41-45

It is essential for the understanding of stellar structure models of high mass stars to explain why constant stars, nonpulsating chemically peculiar hot Bp stars and pulsating stars co‐exist in the slowly pulsating B stars and β Cephei instability strips. We have conducted a search for magnetic fields in the four Bp stars HD55522, HD105382, HD131120, and HD138769 which previously have been wrongly identified as slowly pulsating B stars. A recent study of these stars using the Doppler Imaging technique revealed that the elements He and Si are inhomogeneously distributed on the stellar surface, causing the periodic variability. Using FORS 1 in spectropolarimetric mode at the VLT, we have acquired circular polarisation spectra to test the presence of a magnetic field in these stars. A variable magnetic field is clearly detected in HD55522 and HD105382, but no evidence for the existence of a magnetic field was found in HD131120. The presence of a magnetic field in HD138769 is suggested by one measurement at 3σ level. We discuss the occurrence of magnetic B stars among the confirmed pulsating B stars and find strong magnetic fields of order kG and oscillations to be mutually exclusive. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Evidence for interchange reconnection between a coronal hole and an adjacent emerging flux region     

D. Baker  L. van Driel‐Gesztelyi  G.D.R. Attrill 《Astronomische Nachrichten》2007,328(8):773-776

Coronal holes are regions of dominantly monopolar magnetic field on the Sun where the field is considered to be ‘open’ towards interplanetary space. Magnetic bipoles emerging in proximity to a coronal hole boundary naturally interact with this surrounding open magnetic field. In the case of oppositely aligned polarities between the active region and the coronal hole, we expect interchange reconnection to take place, driven by the coronal expansion of the emerging bipole as well as occasional eruptive events. Using SOHO/EIT and SOHO/MDI data, we present observational evidence of such interchange reconnection by studying AR 10869 which emerged close to a coronal hole. We find closed loops forming between the active region and the coronal hole leading to the retreat of the hole. At the same time, on the far side of the active region, we see dimming of the corona which we interpret as a signature of field line ‘opening’ there, as a consequence of a topological displacement of the ‘open’ field lines of the coronal hole. (© 2007 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)  相似文献   

Liquefaction-induced deformation of earthen embankments on non-homogeneous soil deposits under sequential ground motions     

《Soil Dynamics and Earthquake Engineering》2014

Damage of embankments during earthquakes is widely attributed to the liquefaction of foundation soil. Previous studies have investigated the dynamic response of embankments by mainly considering uniform sand foundation and a single earthquake event. However, the foundation of an embankment consists of many sublayers of soil from liquefiable sand to relatively impermeable layer, and during earthquakes a mainshock may trigger numerous aftershocks within a short time which may have the potential to cause additional damage to soil structures. Accordingly, the investigation of liquefaction-induced deformation of earthen embankments on various liquefiable foundation conditions under mainshock–aftershock sequential ground motions is carried out by a series of dynamic centrifuge tests in this study. The liquefiable foundation includes uniform sand profile, continuous layered soil profile, and non-homogeneous soil profiles. Effects of various foundation conditions on embankment deformations are compared and analyzed. From the test results, it is found that the embankment resting on non-homogeneous soil deposits suffer more damage compared to the uniform sand foundation of same relative density. The test results also suggest that the sequential ground motions have a significant effect on the accumulated deformation of embankment.  相似文献