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克拉通岩石圈地幔的形成与破坏:大洋板块俯冲的贡献

克拉通是地球上最古老的大陆地块.克拉通之所以能够长期稳定存在,主要是因为它具有巨厚、刚性的岩石圈地幔.古老克拉通岩石圈地幔具有高度难熔(富Mg、贫Fe)的特点,其密度较下伏软流圈小,能够"漂浮"在软流圈之上而长期存在.古老克拉通岩石圈地幔是在地球早期壳幔分异之后形成的,其形成可能与大洋板块的俯冲作用密切相关.典型的克拉...     

板块俯冲带岩浆作用过程的研究

综合分析了板块俯冲带岩浆活动的物质来源、岩浆上涌直至喷出的地球化学过程以及与这些过程相对应的时间尺度等研究的进展,指出了目前研究中存在的主要问题,并建议我国在该领域开展相关的研究中应:1)首先利用独有的地理优势,以处于弧后扩张作用早期的冲绳海槽为研究对象,开展相关的调查与研究;2)积极引进先进的技术手段;3)通过加强国际合作,积极参与国际合作项目,拓展研究领域.     

再论纬向正常密度假说与内波假说的比较

本文对“纬向正常密度假说”和“内波假说”再次进行了讨论,进一步比较了二者的联系和区别.根据岩石圈板块概念和地幔对流假说的基本观点、以及“纬向正常密度假说”和“板块运动重力机制”的基本观点,提出了“软流圈板块”概念.     

星地碰撞的板块构造效应

板块构造是一种全球大地构造理论.它以洋底扩张、洋壳边缘俯冲及转换断层为主要构造活动形式,配以地幔对流为原动力,建立一套颇具魅力的板块构造机制理论,被受到广泛认同.但也存在一些重要问题,主要是其地幔对流理念难以令人信服和对海陆格局变迁问题没提出明确的动力机制.在阐明造成板块构造理论这两方面困难问题的主要理由之后,介绍了星地碰撞事件的存在状况及其动力作用,着重论述了大规模星地碰撞的动力作用强大,对全球地质构造活动都有重要影响,板块构造也难以避免;星地碰撞的强烈冲击作用,有能力造成洋底开裂或使大陆裂解.据此设想,可用"星地撞击成缝,减压诱发岩浆上侵"的模式,取代与地球内部层圈结构相抵触的"地幔对流"模式来解释洋底扩张;并以星地碰撞发生地点的随机变化性作为大规模海陆格局变迁的主控原因.如此,则可有助于上述板块构造理论中存在的两大难题的解决.     

环境温度对板式橡胶支座摩擦滑移性能的影响分析

采用有限元模拟的方式,对板式橡胶支座摩擦滑移特性进行分析,并与常温试验中获得的支座摩擦滑移滞回曲线、等效黏滞阻尼比等进行了对比.在获得可靠模型的基础上,分析环境温度对板式橡胶支座摩擦滑移特性的影响,研究了温度与支座摩擦滑移耗能、等效黏滞阻尼比和滑动起始距离的关系.结果表明:(1)板式橡胶支座的有限元模型可以较好地实现支...     

In situ stress field of eastern Australia

New in situ data based on hydraulic fracturing and overcoring have been compiled for eastern Australia, increasing from 23 to 110 the number of in situ stress analyses available for the area between and including the Bowen and Sydney Basins. The Bowen Basin displays a consistent north‐northeast maximum horizontal stress (σ_H) orientation over some 500 km. Stress orientations in the Sydney Basin are more variable than in the Bowen Basin, with areas of the Sydney Basin exhibiting north‐northeast, northeast, east‐west and bimodal σ_H orientations. Most new data indicate that the overburden stress (σ_V) is the minimum principal stress in both the Bowen and Sydney Basins. The Sydney Basin is relatively seismically active, whereas the Bowen Basin is relatively aseismic. Despite the fact that in situ stress measurements sample the stress field at shallower depth than the seismogenic zone, there is a correlation between the stress measurements and seismicity in the two areas. Mohr‐Coulomb analysis of the propensity for failure in the Sydney Basin suggests 41% of the new in situ stress data are indicative of failure, as opposed to 13% in the Bowen Basin. The multiple pre‐existing structural grains in the Sydney Basin further emphasise the difference between propensity for failure in the two areas. Previous modelling of intraplate stresses due to plate boundary forces has been less successful at predicting stress orientations in eastern than in western and central Australia. Nonetheless, stress orientation in the Bowen Basin is consistent with that predicted by modelling of stresses due to plate boundary forces. Variable stress orientations in the Sydney Basin suggest that more local sources of stress, such as those associated with the continental margin and with local structure, significantly influence stress orientation. The effect of local sources of stress may be relatively pronounced because stresses due to plate boundary forces result in low horizontal stress anisotropy in the Sydney Basin.     

辽宁省金矿集中区及其与构造样式的关系

本文将辽宁省金矿划分四种类型,十个主要金矿集中区。这些集中区均受华北地台东西向基底构造活动带及中生代太平洋板块俯冲影响、所产生的北西向构造挤压带和北东向构造—岩浆岩带的复合作用控制。它们分别处于太不洋成矿带的内带(辽东)和外带(辽西)。并以郯庐断裂为轴线,构成了两大“U”字形,类似共轭曲线展布的构造样式。根据深部地球物理资料,综合分析了控制金矿集中区构造样式的形成机制。区内脉状金矿大都分布在深断裂(深度大于五公里断裂)带附近。