排序方式： 共有3条查询结果，搜索用时 15 毫秒
1
1.
利用哈佛大学GCMT数据中心和前人积累的历史地震资料(1962～2016年MW 4.0地震)以及Crust2.0地壳结构统计分析了喜马拉雅地区、天山地区的地壳区域构造与地震活动间的相关性。此外,利用GFZ地学研究中心提供的静态卫星重力模型GGM03S/EGM2008和地形模型Topo计算了2个地区的各类重力异常场,同时还模拟了不同地壳弹性参数下的重力异常场,结果表明喜马拉雅地区重力异常场在水平、垂直方向的梯度特征远大于天山地区的异常特征,且喜马拉雅地区的有效弹性板厚度T_e(6～15km)小于天山地区的有效弹性板厚度T_e(20～30km)。最后,利用喜马拉雅地区与天山地区的GPS震间三维形变场约束了断层运动模型,结果显示两者主前缘断裂的断层闭锁深度及应力积累状态存在较大的差异。因此认为,造成青藏高原及邻区的边界地壳区域地震活动性差异的动力学因素,与地壳有效弹性板厚度、孕震断层参数及区域应力积累状态等密切相关。 相似文献
2.
Effect of local variations of vertical and horizontal stresses on the Cenozoic structuring of the mid-Norwegian shelf 总被引：1，自引：1，他引：0
I. Grunnaleite W. Fjeldskaar J. Wilson J.I. Faleide J. Zweigel 《Tectonophysics》2009,470(3-4):267-283
The mid-Norwegian margin has a complex history and has experienced several phases of changing horizontal and vertical stresses on regional and local scale during the Cenozoic time. In addition to regional stresses related to the opening of the North Atlantic (i.e. ridge push), local variations in stress history may be important for development, distribution and reactivation of structures in the Vøring area in Cenozoic time. Presence and stability of flexural hinge zones between areas of relative uplift and subsidence have played an important role for focusing shallow horizontal stresses within the basins. Emplacement of lower crustal bodies during break-up will, whatever the nature of these bodies, have substantial isostatic effects, and modelling show that this could cause many hundred meters of temporal uplift above the lower crustal bodies, locally exceeding 1300 m of surface uplift. Effects of intra plate stress (IPS) are modelled along three 2D transects across the Vøring Basin. Modelling shows that IPS may have given substantial vertical motions in certain areas of the mid-Norwegian shelf, both with extensional IPS at the time of break-up, and later with compressive IPS during Tertiary time. The modelling assumes a strongly reduced effective elastic thickness (EET) due to lithospheric heating at break-up and later increasing EET as the lithosphere cooled towards present time. Our modelling takes into account the tectonic and isostatic effects of loading faulting and lithospheric thinning throughout the geological history, including several phases of extension prior to the Cenozoic compression. This approach emphasizes the importance of the deformation history of the lithosphere compared to other studies that only take into account the effects of Cenozoic processes of compression and loading on the sedimentary units. We do not state that isostatic uplift or intra plate stress are the most important causes for Cenozoic uplift and compressional deformation in this area, but point to the fact that these factors locally may have played an important role in focusing deformation caused by an interplay of different mechanisms. 相似文献
3.
EET 96008是一块发现于南极Elephant地区的玄武岩质角砾岩月球陨石。本文对该陨石的矿物岩石学特征进行了详细的观察和描述。EET 96008具有典型的碎屑结构,其角砾浑圆度低,角砾大小一般为0.1-2mm,它主要由角砾（50.2vol%）和基质（49.8vol%）组成,该陨石角砾类型多样：（1）晶屑：主要为辉石、橄榄石、长石以及石英;（2）岩屑：主要为变粒岩岩屑、基性岩岩屑、苏长岩质斜长岩岩屑;（3）玻屑：主要为斜长岩质。基质和角砾在颗粒上是连续过渡的,基质主要是由粒度小于0.1mm的矿物碎屑和玻屑组成。该陨石辉石类型多样,成分变化大Fs18.0-58.0Wo3.9-45.2En3.5-79.1,出溶现象普遍,出溶条纹达到1μm宽;橄榄石中Fa值主要分为两个区域,Fa50-70以及Fa80-95,铁含量较高,平均Fa71.8;长石成分以钙长石为主（An84.9-97.9）,部分斜长石已熔长石化。该陨石与QUE 94281同为月球玄武岩质角砾岩,在结构及矿物组成上具有类似性,但是在岩屑类型及橄榄石矿物成分上存在着明显不同,为非成对陨石,且源区可能不同。EET 96008具有三个典型的冲击暗化区域,有大量的玻璃质以及冲击熔融囊的产生,冲击程度达到S5以上。该陨石在冲击作用下,富铁辉石分解产生钙铁辉石-铁橄榄石-石英,该现象为了解月球表面冲击历史提供了重要的科学依据。 相似文献
1