南海成因及其演化模式探讨

尽管南海已进行深入的调查与研究,提出多种成因模型,包括挤出模型、弧后扩张模型、古南海俯冲拖曳模型等,但因其所处构造位置特殊,周边构造环境经历了复杂的改造,所有成因模式均未能得到广泛的认可。本文从三大板块相互作用入手,结合南海实测数据,提出南海形成的弧后扩张—左旋剪切模型。认为南海是古南海往北俯冲的弧后盆地,菲律宾海板块往北漂移形成的大规模左旋走滑是南海扩张的触发因素。印度—欧亚碰撞产生中南半岛挤出主要影响西南海盆扩张方向,使得扩张轴从近东西向转为北东向。南海及邻区晚中生代以来的演化可以分为以下阶段：1）早白垩世开始澳大利亚板块往北漂移,新特提斯洋往北俯冲消亡,导致弧后扩张,形成古南海;2）晚白垩世末—始新世,古南海往北俯冲,导致弧后拉张形成陆缘裂谷;3）早渐新世,受菲律宾海板块西缘大型左旋走滑影响,在原有裂谷的基础上从东往西海底扩张,形成南海;4）渐新世末,受俯冲后撤的影响,扩张中心往南跃迁,同时受西缘断裂左旋活动的影响,扩张轴从近东西西逐步转为北东向;5）早中新世晚期,南沙地块—北巴拉望地块与卡加延脊碰撞,南海扩张停止。     

西南印度洋脊中段Indomed-Gallieni洋中脊岩浆-构造动力模式

利用西南印度洋脊中段Indomed-Gallieni洋段49-51°E区段全覆盖高分辨率多波束水深地形资料,应用构造地貌学分析方法,结合区域地形及其他地球物理等资料,在分段分析49-51°E区段岩浆-构造动力学模式的基础上,进一步探讨了约10 Ma以来Indomed-Gallieni洋段的演化史.28、29洋段目前岩浆供应不足,在轴部不对称深断层的控制之下不对称扩张,属于超慢速扩张洋脊较常见的演化方式.轴部火山建造主要向北翼增生,发育与火山脊相关的火山地貌;南翼构造拉张作用强烈,地貌上可观察到大量断块,拆离断层可能大量存在.而27洋段水深浅、火山密集、轴部缺失裂谷,超慢速扩张下却具有较高的岩浆通量.Indomed-Gallieni洋段地形高地建造于一次岩浆增强事件,但应该不是因为Crozet热点的影响.27洋段为目前仍受该岩浆增强事件影响的唯一区段,但其强度和规模也在逐渐减小;包括28、29洋段在内的Indomed-Gallieni段其他部分,已重新恢复到岩浆供应不足的正常超慢速扩张洋脊演化模式.28、29洋段和27洋段岩浆供应均存在岩浆通量由多至少的周期,周期内岩浆供应较多时期轴部建脊,减少时期轴部火山建造裂离.但27洋段由于仍受岩浆增强事件的影响,与28、29洋段表现形式不同,主要表现为火山建造裂离方式、岩浆供应周期长短以及构造活动强烈程度的不同.     

The magmatic activity mechanism of the fossil spreading center in the Southwest sub-basin,South China Sea

Petrogeochemical data indicate that after the end of seafloor spreading,residual magmatic activity still exists in the deep basin of the South China Sea.By using different viscous structure models beneath the fossil spreading center of the Southwest sub-basin we simulated the amount of melt produced,the length of the melting period,and the thermal evolution process in terms of geothermics and the buoyant decompression melting mechanism.We compared the results of our model with observed heat flow,seismic,and petrogeochemistry data.The results show that depletion buoyancy induced by buoyant decompression melting plays an important role in the melting process,while retention buoyancy,thermal buoyancy,and viscous shear force have only a weak influence on the melting process.From the length of the melting period,we determined that for the three viscous structures models the magmatic activity lasted about 5,12,and 15 Ma.Under the effect of buoyant depression melting,local high-temperature areas will develop under the basin,which can explain the low-velocity layer detected by seismic exploration in the middle and upper lithosphere of the Southwest sub-basin.We also simulated the possible lithology distribution beneath the fossil spreading center with the physical conditions of different viscous structure,different temperature structure,and different melting fraction,which provided a greater understanding of the rock petrogeochemical data of the deep sea basin in the South China Sea.     

南海张裂过程及其对晚中生代以来东南亚构造的启示——IODP建议书735-Full介绍

南海的形成揭示了大陆边缘张裂和盆地形成的复杂模式,尽管已经进行了广泛研究,但是关于基底岩石和深海盆沉积层的精确年代数据还很缺乏,这使得对南海张裂年代的估计存在很大的误差,对张裂机制和历史的各种假设没有得到验证.同时只有对南海的张裂过程有了精确地分析与刻画,才能更好地理解西太平洋边缘海盆地的形成以及它们在印支块体受印度-欧亚板块碰撞而向东南挤出、青藏高原隆升中可能起到的作用.2009年正式提交的国际综合大洋钻探计划(IODP)建议书735-Full建议在南海深海盆内的4个站位上实施钻探.这4个站位分布在南海盆地4个不同的次级构造单元上(南海东北部、西北次海盆、东部次海盆和西南次海盆),这样的站位设计会确保完成本建议书的整体研究目标,即揭示南海的张裂历史和它对晚中生代以来东南亚构造的启示.位于南海盆地最东北部的站位有助于确定该区域地壳的属性和验证古南海是否存在,位于西北次海盆的站住可能会提供南海的最早张裂年代,另外2个分别位于东部次海盆和西南次海盆的站位将重点确定2个次海盆的绝对年龄、基底矿物成分与磁化率以及2个次海盆的相对张裂次序.这些站位的水深大约在2 910～4 400 m,钻探深度预计到海底以下大约700～2 200 m,总的钻透深度为5 959 m,其中5 359 m穿透沉积层,另外600 m或400 m钻入基底.所有这些站位的位置是由已有的地球物理观测数据所确定,目前计划收集更多的地质与地球物理数据以满足IODP对井位调查数据的要求.     

Parametric analysis of single pile response in laterally spreading ground

Extensive damage to pile-supported structures has been witnessed in several recent earthquakes (Chi-Chi, 1999; Kobe, 1995, etc.), as a result of liquefaction-induced lateral spreading of slightly sloping ground or free-face topographic irregularities. This paper presents a parametric analysis of the basic pile and soil parameters, as well as the pile-soil interaction mechanisms affecting the response of single piles subjected to such lateral spreading, based on numerical simulation with the nonlinear P-y method. In parallel, a set of design charts and analytical relations is established, for approximate computation of maximum pile deflections and bending moments, using a “theory guided” multi-variable statistical analysis of the numerical predictions. Three different combinations (design cases) of pile head constraints and soil conditions were considered, which are commonly encountered in practice. The overall accuracy of the proposed analytical relations is evaluated against experimental results from seven centrifuge and five large shaking table experiments.     

综合定点前兆异常推测地震危险区域的一种途径

1998年张北6.2级地震前,山西、河北及其附近地区出现的定点形变、流体前兆异常,具有随时间推移从震区外围大范围区域向震区附近迁移、集中的趋势特性.通过构建异常信号传播函数,借助网格搜索—拟牛顿最小二乘法反演汇聚区域即推测可能的地震危险区,所得汇聚区域边缘距实际震中仅25 ～51 km、汇聚时刻与发震时刻仅差数天,且震前中短期阶段汇聚速度加快.     

中日规范中关于液化和侧向扩流场地桥梁桩基抗震设计考虑之比较

评述了我国液化场地和侧向扩流场地桥梁桩基抗震设计规范。总结了中日两国液化场地和侧向扩流场地桥梁桩基的抗震设计方法与技术细节,阐述了日本规范中液化场地和侧向扩流场地桥梁桩基抗震设计中的液化地基土反力折减系数的确定方法,以及土体液化侧向扩流对桩作用力的计算模式。指出我国规范中在液化和侧向扩流场地桩的抗震分析方法、不同土层分界处桩的抗震措施、桩的竖向承载力及桩的屈曲稳定性分析等方面存在的主要问题,据此给出了亟待改进的初步建议。这对我国桥梁工程的抗震安全性具有重要意义,可供我国工程技术人员参考借鉴。     

强震作用下松散海床地基的动力响应

海上和沿海区域砂性土地基在强震作用下需同时考虑液化、震陷以及流滑效应。选用杨朝晖叠套屈服面模型,提出了获取计算参数的简化方法,用OpenSees验证了该模型模拟液化的能力;开发了OpenSees与ANSYS的接口,对处于强震地区、地基土为松散砂性土的印尼某进水明渠堤坝进行了非线性有限元动力计算,判断了场地的液化情况,预测了堤坝及地基的震陷量和侧向流滑,计算结果对该类地基的加固处理具有一定的指导意义     

砂-黏土双层地基极限承载力的数值研究

在实际工程中,常见天然的或通过人工换填形成的上部砂土、下部黏土的层状地基,目前关于这种双层地基极限承载力和破坏机制研究还不够深入。通过有限差分法建立双层地基数值模型,分析基底粗糙程度、砂土剪胀角和超载对地基破坏模式及极限承载力的影响,并根据有限差分法计算结果对强度加权平均法、应力扩散法和冲剪破坏法等现有实用计算方法的估算正确性进行评价。研究结果表明,基底粗糙程度对极限承载力的影响随着砂土内摩擦角的增大而减小;当剪胀角较小时,剪胀角变化对承载力的影响更为明显;当下层黏土强度较小时,超载的作用更明显。强度加权平均法由于低估破坏面影响深度导致砂土层权重较大,计算结果偏大;应力扩散法忽略了砂土剪切强度,在砂土层较厚时出现低估;冲剪破坏法由于可较为精确地计算砂土破坏面上抗剪强度和被动土压力,是3种实用方法中计算最准确的,当砂土厚度和黏土强度较大时,建议按太沙基经验公式对下卧黏土进行局部剪切破坏修正后确定极限承载力。     

Geodynamic evolution of a forearc rift in the southernmost Mariana Arc

The southernmost Mariana forearc stretched to accommodate opening of the Mariana Trough backarc basin in late Neogene time, erupting basalts at 3.7–2.7 Ma that are now exposed in the Southeast Mariana Forearc Rift (SEMFR). Today, SEMFR is a broad zone of extension that formed on hydrated, forearc lithosphere and overlies the shallow subducting slab (slab depth ≤ 30–50 km). It comprises NW–SE trending subparallel deeps, 3–16 km wide, that can be traced ≥ ∼30 km from the trench almost to the backarc spreading center, the Malaguana‐Gadao Ridge (MGR). While forearcs are usually underlain by serpentinized harzburgites too cold to melt, SEMFR crust is mostly composed of Pliocene, low‐K basaltic to basaltic andesite lavas that are compositionally similar to arc lavas and backarc basin (BAB) lavas, and thus defines a forearc region that recently witnessed abundant igneous activity in the form of seafloor spreading. SEMFR igneous rocks have low Na₈, Ti₈, and Fe₈, consistent with extensive melting, at ∼23 ± 6.6 km depth and 1239 ± 40°C, by adiabatic decompression of depleted asthenospheric mantle metasomatized by slab‐derived fluids. Stretching of pre‐existing forearc lithosphere allowed BAB‐like mantle to flow along the SEMFR and melt, forming new oceanic crust. Melts interacted with pre‐existing forearc lithosphere during ascent. The SEMFR is no longer magmatically active and post‐magmatic tectonic activity dominates the rift.