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101.
Crustal density structure in the Spanish Central System derived from gravity data analysis (Central Spain) 总被引：2，自引：0，他引：2
Shallow and deep sources generate a gravity low in the central Iberian Peninsula. Long-wavelength shallow sources are two continental sedimentary basins, the Duero and the Tajo Basins, separated by a narrow mountainous chain called the Spanish Central System. To investigate the crustal density structure, a multitaper spectral analysis of gravity data was applied. To minimise biases due to misleading shallow and deep anomaly sources of similar wavelength, first an estimation of gravity anomaly due to Cenozoic sedimentary infill was made. Power spectral analysis indicates two crustal discontinuities at mean depths of 31.1 ± 3.6 and 11.6 ± 0.2 km, respectively. Comparisons with seismic data reveal that the shallow density discontinuity is related to the upper crust lower limit and the deeper source corresponds to the Moho discontinuity. A 3D-depth model for the Moho was obtained by inverse modelling of regional gravity anomalies in the Fourier domain. The Moho depth varies between a mean depth of 31 km and 34 km. Maximum depth is located in a NW–SE trough. Gravity modelling points to lateral density variations in the upper crust. The Central System structure is described as a crustal block uplifted by NE–SW reverse faults. The formation of the system involves displacement along an intracrustal detachment in the middle crust. This detachment would split into several high-angle reverse faults verging both NW and SE. The direction of transport is northwards, the detachment probably being rooted at the Moho. 相似文献
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Dynamite shots of the crustal-scale refraction seismic project ALP 2002 were recorded by an array of 40 seismological three-component stations on the TRANSALP profile. These observations provide a direct link between the two deep seismic projects. We report preliminary results obtained from these data. In a first approach, we verified the TRANSALP refraction seismic velocity model computing travel times for several shots and comparing them to the new observations. The results generally confirm this model. Significant first-break travel time differences in and near the Tauern Window are explained by anisotropy. Large-scale features of the model, particularly the Moho structure, seem to be continuous towards the east. Travel time residuals of wide-angle reflections indicate a slight eastward dip component of the Adriatic Moho. 相似文献
104.
在青藏高原,利用远震波形及演所得的Moho界面深度,其横向变化很大．在班公缝合带附近,Moho界面出现10余公里的错断．羌塘块体的Moho界面向北倾斜,而柴达木和巴颜喀拉的Moho界面向南倾斜．利用近震Pn的走时验证远震波形反演所得的Moho界面深度,两者的结果十分吻合．综合近来地球物理观测的结果。我们得到喜马拉雅─祁连山的地壳构造图,它贯穿印度─欧亚的碰撞带和中生代的陆─陆碰撞带．特提斯喜马拉雅和拉萨块体的地壳是由多个双向冲断层所组成,它们可以解释为在不同时期中,印度次大陆曾经数次向拉萨块体地壳挤入,而且羌塘块体的地壳也向拉萨块体的地壳挤入．测量冲断层的水平长度,可以定量估算自50Ma陆─陆碰撞以来,印度次大陆和羌塘块体向特提斯喜马拉雅和拉萨块体地壳挤入的长度． 相似文献
105.
青藏高原重力场特征和地壳构造 总被引：3，自引：0，他引：3
本文利用布格重力异常图,结合其它地质和地球物理资料,探讨了青藏高原区域重力场和剩余重力场特征及所反映的地壳构造。 相似文献
106.
以１∶５０万比例尺,实测了新疆阿尔干－青海老茫崖重力剖面。研究了该剖面及其邻区为主的青藏高原西北边缘重力场特征;划分了３个地质构造单元及８条较大断裂;计算并分析了Ａｉｒｙ重力均衡异常及莫霍界面深度。 相似文献
107.
According to the theory of isostasy, the Earth has a tendency to deform its surface in order to reach an equilibrium state. The land-uplift phenomenon in the area of the Fennoscandian Shield is thought to be a process of this kind. The geoid, as an equipotential surface of the Earth's gravity field, contains information on how much the Earth's surface departs from the equilibrium state. In order to study the isostatic process through geoidal undulations, the structural effects of the crust on the geoid have to be investigated.
The structure of the crust of the Fennoscandian Shield has been extensively explored by means of deep seismic sounding (DSS). The data obtained from DSS are used to construct a 3-D seismic-velocity structure model of the area's crust. The velocity model is converted to a 3-D density model using the empirical relationship that holds between seismic velocities and crustal mass densities. Structural effects are then estimated from the 3-D density model.
The structural effects computed from the crustal model show that the mass deficiency of the crust in Fennoscandia has caused a geoidal depression twice as deep as that observed from the gravimetric geoid. It proves again that the crust has been isostatically compensated by the upper mantle. In other words, an anomalously high-density upper mantle must exist beneath Fennoscandia. 相似文献
The structure of the crust of the Fennoscandian Shield has been extensively explored by means of deep seismic sounding (DSS). The data obtained from DSS are used to construct a 3-D seismic-velocity structure model of the area's crust. The velocity model is converted to a 3-D density model using the empirical relationship that holds between seismic velocities and crustal mass densities. Structural effects are then estimated from the 3-D density model.
The structural effects computed from the crustal model show that the mass deficiency of the crust in Fennoscandia has caused a geoidal depression twice as deep as that observed from the gravimetric geoid. It proves again that the crust has been isostatically compensated by the upper mantle. In other words, an anomalously high-density upper mantle must exist beneath Fennoscandia. 相似文献
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