内蒙额尔古纳在矿带中生代火山岩浆活动与金属成矿的关系

在岩石学和微量元素地球化学研究的基础上,通过对不同类型矿床的成矿岩体及围岩条件的分析,探讨了中生代火山岩浆活动与金属成矿的关系。认为晚侏罗世火山岩浆活动为成矿提供了有利的围岩的构造空间;早白垩世岩浆活动提供了成矿岩体及热力学条件,该期次火山岩浆的侵入并作用于不同的围岩、形成了由斑岩型Ｃｕ、Ｍｏ矿,浅成熟液型Ａｇ、Ｐｂ、Ｚｎ矿等组成的一系列矿床组合。     

Oxygen isotope fractionation in mantle minerals

The increment method is adopted to calculate oxygen isotope fractionation factors for mantle minerals, particularly for the polymorphic phases of MgSiO₃ and Mg₂SiO₄. The results predict the following sequence of¹⁸O-enrichment:pyroxene (Mg, Fe, Ca)₂Si₂O₆>olivine (Mg, Fe)₂SiO₄ > spinel (Mg, Fe)₂SiO₄> ilmenite (Mg, Fe, Ca) SiO₃>perovskite (Mg, Fe, Ca) SiO₃. The calculated fractionations for the calcite-perovskite (CaTiO₃) System are in excellent agreement with the experimental calibrations. If there would be complete isotopic equilibration in the mantle, the spinel-structured silicates in the transition zone are predicted to be enriched in¹⁸O relative to the perovskite-structured silicates in the lower mantle but depleted in¹⁸O relative to olivines and pyroxenes in the upper mantle. The oxygen isotope layering of the mantle might result from differences in the chemical composition and crystal structure of mineral phases at different mantle depths. Assuming isotopic equilibrium on a whole earth scale, the chemical structure of the Earth’s interior can be described by the following sequence of¹⁸O-enrichment:upper crust>lower crust>upper mantle>transition zone>lower mantle>core. Project supported by the National Natural Science Foundation of China and the Chinese Academy of Sciences.     

Solar internal rotation rate and the latitudinal variation of the tachocline

A new set of accurately measured frequencies of solar oscillations is used to infer the rotation rate inside the Sun, as a function of radial distance as well as latitude. We have adopted a regularized least-squares technique with iterative refinement for both 1.5D inversion, using the splitting coefficients, and 2D inversion using individual m splittings. The inferred rotation rate agrees well with earlier estimates showing a shear layer just below the surface and another one around the base of the convection zone. The tachocline or the transition layer where the rotation rate changes from differential rotation in the convection zone to an almost latitudinally independent rotation rate in the radiative interior is studied in detail. No compelling evidence for any latitudinal variation in the position and width of the tachocline is found, although it appears that the tachocline probably shifts to a slightly larger radial distance at higher latitudes and possibly also becomes thicker. However, these variations are within the estimated errors and more accurate data would be needed to make a definitive statement about latitudinal variations.     

OPserver: interactive online computations of opacities and radiative accelerations

Codes to compute mean opacities and radiative accelerations for arbitrary chemical mixtures using the Opacity Project recently revised data have been restructured in a client–server architecture and transcribed as a subroutine library. This implementation increases efficiency in stellar modelling where element stratification due to diffusion processes is depth dependent, and thus requires repeated fast opacity re-estimates. Three user modes are provided to fit different computing environments, namely, a web browser, a local workstation and a distributed grid.     

强台风下导管架平台倒塌全过程数值仿真

针对强台风引起的平台倒塌问题,综合隐式有限元与显式动力有限元算法,建立导管架平台结构倒塌全过程仿真流程;提出基于重现期的Pushover分析方法,充分考虑平台侧向环境载荷分布的变化以及可能的甲板上浪载荷因素,使得确定的倒塌环境载荷更加真实;采用APDL编制平台隐式与显式有限元模型转化程序,有效解决波浪载荷计算与精确施加的难题;在此基础上,应用LS-DYNA实现导管架平台在强台风载荷下的倒塌全过程仿真,动态再现平台结构倒塌过程中的构件破坏失效及内力分布,深入揭示平台结构的倒塌机理。研究成果可为导管架平台结构抗台风设计及理论研究提供参考。     

Interpretation of Mars southern highlands high amplitude magnetic field with total gradient and fractal source modeling: New insights into the magnetic mystery of Mars

Using model studies, the total gradient (TG) of the Z-component magnetic field is shown to be a useful quantity for delineating sources of satellite-altitude magnetic anomalies; this field is used to constrain the location and lateral boundaries of sources of high amplitude magnetic anomalies of southern highlands of Mars. The TG field suggests two parallel linear and oppositely magnetized sources of 1000 and 1800 km length separated by 1000 km of region of intervening non-parallel sources. The simplest interpretation of the long, linear features is that they are zones of multitudinous crustal scale dikes formed in separate episodes of rifting, and not features associated with the mechanism of seafloor spreading. Forward modeling with uniformly magnetized sources suggests that magnetizations of the order of 10-50 A/m (40 km thickness) over ∼100 km width in the case of the southern source and of 12.5-27.5 A/m (40 km thickness) and ∼200 km width for the northern source are necessary to explain the Z-component amplitudes and features of the TG field. If the crustal magnetization on Mars were to be distributed fractally as on Earth, magnetizations matching the largest amplitude features on Mars may be spatially correlated from a 50-100 km distance range (β ∼ 3) to approaching nearly uniform magnetization (β ∼ 5) values. To keep magnetization intensity as small as possible, the higher end of β values are preferred, whereas, small amplitude anomaly features could be generated from sources with β ∼ 3. Many of the Mars anomaly features could be coalescence effects similar to the coalescence of anomaly features observed on http://icarus.cornell.edu/information/keywords.html.Earth.     

On the interaction of internal gravity waves with a magnetic field – I. Artificial wave forcing

We present results from numerical simulations of the interaction of internal gravity waves (IGW) with a magnetic field. In accordance with the dispersion relation governing IGW in the presence of magnetism and rotation, when the IGW frequency is approximately that of the Alfvén frequency, strong reflection of the wave occurs. Such strong reflection markedly changes the angular momentum transport properties of the waves. In these simple models a strong, time-independent shear layer develops, in contrast to the oscillating shear layer that develops in the purely hydrodynamic case.     

不同洞口位置节能砌块隐形密框复合墙体恢复力模型研究

为研究洞口位置对节能砌块隐形密框复合墙体滞回特性的影响,对6个采用低周反复加载方式的1/2缩尺试件的试验现象及数据进行分析。基于试验结果和现有恢复力模型理论,对试验数据进行拟合分析,利用退化四折线模型和回归方法,建立节能砌块隐形密框复合墙体的四折线恢复力模型。试验结果表明:当洞口位于墙体中间时,试件滞回环愈加丰满,试件初始刚度有所增加,承载力衰减速率减小,卸载刚度退化速率变慢。通过对骨架曲线特征参数的计算,并和试验骨架曲线对比,两者吻合较好,表明该恢复力模型可以较好的反映出不同洞口位置对其滞回特性的影响,可为节能砌块隐形密框复合墙体的弹塑性分析及工程应用提供参考。     

矿山土地复垦方案中对开采塌陷区预测方法的探讨

通过对土地复垦方案采用的几种方法的比较及分析,选择导水裂隙带最大高度与移动角组合判别法的方法,圈定出矿山因开采易导致地表塌陷的区域,为矿山土地复垦方案中主要拟破坏土地的确定提供方便、实用的方法。