川藏公路然乌-鲁朗段地质灾害影响因素定量分析

川藏公路然乌—鲁朗段工程地质条件极其复杂,导致大型地质灾害频繁发生。为了定量地分析各种影响因素对大型地质灾害的贡献,本文根据信息熵的理论和方法,提出了“地质灾害熵”的概念。通过详细分析川藏公路然乌—鲁朗段大型地质灾害资料,选择平均坡度、断层和节理、岩体结构、松散堆积物、水文地质条件、冰川作用和降雨等7个影响因素,分析它们对研究区某些大型地质灾害的影响程度,计算出了各影响因素的“地质灾害熵”。根据“地质灾害熵”计算得到了各影响因素的权重,在一定程度上解决了地质灾害影响因素的定量分析问题。     

VENTILATION FLOW IN A BAROCLINIC VORTEX RELATED TO TROPICAL CYCLONE MOTION

The tropical cyclone motion is numerically simulated with a quasi-geostrophic baroclinic model.The flow field of a tropical cyclone is decomposed into its axisymmetric and asymmetric components.The relation between the ventilation flow vector and the motion vector of the tropical cyclone is inves-tigated.The results of numerical experiments indicate:(1) There are both large-scale beta gyres andsmall-scale gyres in the asyrnmetric flow field.(2) The interaction between small-scale gyres andlarge-scale beta gyres leads to the oscillation of translation speed and translation direction for the tropi-cal cyclone.(3) There are the large deviations between the ventilation flow vector calculated bymeans of Fiorino and Elsberry's method and the motion vector of tropical cyclone.(4) The ventila-tion flow vector computed using the improved method closely correlates with the motion vector of thetropical cyclone.     

Multi-layer Tectonic Model for Intraplate Deformation and Plastic-Flow Network in the Asian Continental Lithosphere

In a large area of the east—central Asian continent there is a unified seismic network system composed of two families of large—seismic belts that intersect conjugately. Such a seismic network in the middle—upper crust is actually a response to the plastic flow network in the lower lithosphere including the lower crust and lithospheric mantle. The existence of the unified plastic flow system confirms that the driving force for intraplate tectonic deformation results mainly from the compression of the India plate, while the long-range transmission of the force is carried out chiefly by means of plastic flow. The plastic flow network has a control over the intraplate tectonic deformation.     

Geodynamic settings of Mesozoic large-scale mineralization in North China and adjacent areas

Based on the summary of the highly precise datings of the metal deposits and related granitic rocks in North China craton and adjacent areas, such as the molybdenite Re-Os datings,⁴⁰Ar-³⁹Ar datings of mica, K-feldspar and quartz, some Rb-Sr isochrons, and the SHRIMP zircon U-Pb dating and single grain zircon U-Pb dating, we suggest that the large-scale mineralization in North China craton and adjacent areas take place in three periods of 200-160Ma, 140Ma±, and 130-110Ma. Their corresponding geodynamic settings are proposed to be the collision orogenic process, transformation of the tectonic regime, and delamination of the lithosphere, respectively, in light of analyzing the Mesozoic geodynamic evolution in the North China craton.     

青藏高原东缘龙门-锦屏造山带的崛起——大型拆离断层和挤出机制

龙门-锦屏山的东缘发育一系列逆冲断裂和飞来峰构造,逆冲作用使山体向东叠置在四川盆地之上。新的野外调查、显微构造分析和糜棱岩石英组构的EBSD测量表明,在龙门-锦屏山的前震旦纪变质杂岩体西缘(即青藏高原东缘)发育一条近NS向的大型韧性拆离断裂,被20Ma以来形成的NW—SE向鲜水河韧性走滑剪切带[1]左行错位80km。青藏高原东缘韧性拆离断裂中黑云母40Ar-39Ar测年获得112～120Ma的年龄,表明龙门-锦屏山的崛起可能与白垩纪开始的垂向挤出机制密切关联。结合四川前陆盆地的沉积及演化特征,认为晚三叠世时期羌塘/东昆仑/扬子陆块的碰撞形成松潘-甘孜造山带,晚三叠世—侏罗纪在其东南缘形成四川前陆盆地沉积;早白垩世龙门-锦屏山开始抬升,晚白垩世快速崛起,在四川前陆盆地沉积之上叠置白垩纪—第四纪再生前陆盆地的沉积。龙门-锦屏山的崛起与白垩纪以来扬子板块岩石圈对于松潘-甘孜地体的陆内俯冲作用有关,使位于中下地壳的变质基底岩石在挤出机制下隆起。     

煤层气井绳索取心钻进技术的改进

通过大口径绳索取心技术在某煤层气参数井＋生产井施工过程中的应用，介绍了在应用该技术的过程中所遇到的技术难题及解决方案，同时介绍了煤层气参数井绳索取心过程中钻井冲洗液的选用及钻进参数的优选方法。     

Cosmological perturbation theory and the spherical collapse model — III. The velocity divergence field and the Ω dependence

Cosmological perturbation theory (PT) is a useful tool to study the cumulants of the density and velocity fields in the large-scale structure of the Universe. In Papers I and II of this series we saw that the spherical collapse (SC) model provides the exact solution to PT at tree-level and gives a good approximation to the loop corrections (next-to-leading orders), indicating negligible tidal effects. Here, we derive predictions for the (smoothed) cumulants of the velocity divergence field θ ≡ ▽ ⊙  v for an irrotational fluid in the SC model. By comparing these with the exact analytic results of Scoccimarro &38; Frieman, it is shown that, at least for the unsmoothed case, the loop corrections to the cumulants of θ are dominated by tidal effects. However, most of the tidal contribution seems to cancel out when computing the hierarchical ratios, T _J  = 〈θ ^J 〉 / 〈θ²〉  ^{J −1}. We also extend the work presented in Papers I and II to give predictions for the cumulants of the density and velocity divergence fields in non-flat spaces. In particular, we show the equivalence between the spherically symmetric solution to the equations of motion in the SC model (given in terms of the density) and that of the Lagrangian PT approach (given in terms of the displacement field). It is shown that the Ω dependence is very weak for both cosmic fields even at one loop (a 10 per cent effect at most), except for the overall factor f (Ω) that couples to the velocity divergence.     

The non-linear redshift-space power spectrum of galaxies

We study the power spectrum of galaxies in redshift space, with third-order perturbation theory to include corrections that are absent in linear theory. We assume a local bias for the galaxies: i.e., the galaxy density is sampled from some local function of the underlying mass distribution. We find that the effect of the non-linear bias in real space is to introduce two new features: first, there is a contribution to the power which is constant with wavenumber, whose nature we reveal as essentially a shot-noise term. In principle this contribution can mask the primordial power spectrum, and could limit the accuracy with which the latter might be measured on very large scales. Secondly, the effect of second- and third-order bias is to modify the effective bias (defined as the square root of the ratio of galaxy power spectrum to matter power spectrum). The effective bias is almost scale-independent over a wide range of scales. These general conclusions also hold in redshift space. In addition, we have investigated the distortion of the power spectrum by peculiar velocities, which may be used to constrain the density of the Universe. We look at the quadrupole-to-monopole ratio, and find that higher order terms can mimic linear theory bias, but the bias implied is neither the linear bias, nor the effective bias referred to above. We test the theory with biased N -body simulations, and find excellent agreement in both real and redshift space, providing the local biasing is applied on a scale whose fractional rms density fluctuations are < 0.5.