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121.
Piled embankments, which offer many advantages, are increasingly popular in construction of high-speed railways in China. Although the performance of piled embankment under static loading is well-known, the behavior under the dynamic train load of a high-speed railway is not yet understood. In light of this, a heavily instrumented piled embankment model was set up, and a model test was carried out, in which a servo-hydraulic actuator outputting M-shaped waves was adopted to simulate the process of a running train. Earth pressure, settlement, strain in the geogrid and pile and excess pore water pressure were measured. The results show that the soil arching height under the dynamic train load of a high-speed railway is shorter than under static loading. The growth trend for accumulated settlement slowed down after long-term vibration although there was still a tendency for it to increase. Accumulated geogrid strain has an increasing tendency after long-term vibration. The closer the embankment edge, the greater the geogrid strain over the subsoil. Strains in the pile were smaller under dynamic train loads, and their distribution was different from that under static loading. At the same elevation, excess pore water pressure under the track slab was greater than that under the embankment shoulder. 相似文献
122.
This paper describes synthetically the seismic activity, deep and shallow structures and rock dynamic features in and near Chaoyang—Yixian region. It is supposed that there is a low velocity layer in middle crust and the three-layered crustal velocities are all lower than that in both sides of the region. There exists uplifts of upper mantle and asthenosphere-low resistance layer. It is also studied the composition of matter of three-layered crust, low velocity layer, upper mantle and asthenosphere. In the end the direct relations between the deep and shallow structure, composition and the seismic activity and new activities of faults in this region are discussed. 相似文献
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In this work,we studied the variable stars in the open cluster NGC 1912 based on the photometric observations and Gaia DR2 data.More than 3600 CCD frames in B,V,R filters were reduced,and we obtained the light curves that span about 63 hours.By analyzing these light curves,we detected 24 variable stars,including 16 periodic variable stars,seven eclipsing binaries and one star whose type is unclear.Among these 24 variable stars,11 are newly discovered,which are classified as sixγDoradus stars,oneδScuti star,three detached binaries and one contact binary.We also confirmed 13 previously known variable stars.Based on cluster members identified by Cantat-Gaudin et al.(2018),we inferred cluster memberships for these detected variable stars.Using Gaia DR2 data,we plotted a new color-magnitude diagram for NGC1912,and showed the nature of variable cluster members in kinematical properties and heliocentric distance.Among the 24 variable stars,seven variables are probable cluster members,which show homogeneity in kinematic characters and space position with the established cluster members.Four of the seven variable cluster members are the previously discovered stars,consisting of twoγDor stars and twoδSct stars.The remaining three variable cluster members,which are allγDor stars,are firstly detected in this work.The main physical parameters of these variable cluster members estimated from the color-magnitude diagram are log(age/yr)=8.75,[Fe/H]=-0.1,m-M=10.03 mag,and E(B-V)=0.307. 相似文献
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受全球气候变化和人类活动影响,青藏高原上的土地沙漠化正呈现加速发展态势。沙漠化产生的风沙堆积势必改变地表辐射和能量平衡状况,对较为敏感和脆弱的多年冻土环境造成影响,并可能影响青藏铁路路基的稳定性。因此,研究积沙对多年冻土的影响对于高原沙害防治、多年冻土保护和道路工程建设都具有重要的理论及现实意义。目前,前人已在青藏高原地表能量平衡研究方面取得了一些成果,并开始关注积沙对冻土温度影响问题。然而,由于已有观测资料的连续性、同步性和可比性等局限,对积沙地表辐射和能量平衡方面的研究还比较薄弱,积沙对冻土温度过程影响的研究结果尚不一致,而积沙对路基影响的问题也亟待开展研究。为此,本文提出了加强定位观测、开展室内低温实验以及数值模拟等建议,以期对今后的深入研究起到抛砖引玉作用。 相似文献
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Jianping Huang Elizabeth Vanacore Fenglin Niu Alan Levander 《Earth and Planetary Science Letters》2010,289(1-2):105-111
We analyzed receiver-function data recorded by a temporary broadband array deployed as part of the BOLIVAR project and the permanent seismic network of Venezuela to study the mantle transition zone structure beneath the Caribbean-South American plate boundary and Venezuela. Significant topography on both the 410-km and the 660-km discontinuities was clearly imaged in the CCP (common-conversion-point) stacked images. Beneath the southeastern Caribbean, the 410-km is featured by a narrow (~ 200 km EW) ~ 25-km uplift extending in the NS direction around 63° west, while the 660-km is depressed by ~ 20 km in a narrow region slightly west to the uplift, a scenario that is more consistent with westward descent of the oceanic South American plate rather than a break-off of NNW dipping proto-Caribbean oceanic lithosphere along the El Pilar Fault. We also found a thick transition zone beneath the Falcon region in northwestern Venezuela, possibly associated with the subducted Nazca plate. A flat 410-km was observed beneath the Guayana shield, suggesting that the shield has a stable and moderately deep keel, which has little effect on the underlying transition zone structure. 相似文献
130.
论太行山构造岩浆带的岩浆来源及其成因 总被引:8,自引:0,他引:8
本文以太行山构造岩浆带及其东西两侧断陷盆地的地质特征及深部探测资料为依据,探讨远离俯冲板内构造岩浆带中岩浆的成因、来源及侵位机制。提出了韧性流变-岩浆隆起模式。认为在区域构造应力场和地幔位势差、密度差的控制下?隆升的造山带剥蚀物向两侧断陷盆地搬运,而中下地壳则沿深部向山根缓倾的韧性拆离带迁移到造山带的深部,并在拆离剪切作用及流体的参与下形成深熔岩浆,这种深熔岩浆,在沿陡倾剪切带上侵过程中,不断与中 相似文献