Modelling of periodic wave transformation in the inner surf zone

In this paper, we analyse the ability of the nonlinear shallow-water (NSW) equations to predict wave distortion and energy dissipation of periodic broken waves in the inner surf zone. This analysis is based on the weak-solution theory for conservative equations. We derive a new one-way model, which applies to the transformation of non-reflective periodic broken waves on gently sloping beaches. This model can be useful to develop breaking-wave parameterizations (in particular broken-wave celerity expression) in both time-averaged wave models and time-dependent Boussinesq-type models. We also derive a new wave set-up equation which provides a simple and explicit relation between wave set-up and energy dissipation. Finally, we compare numerical simulations of both, the NSW model and the simplified one-way model, with spilling wave breaking experiments and we find a good agreement.     

盆地岩石圈结构与油气成藏及分布

本文综述了大陆岩石圈研究现状和克拉通盆地、裂谷盆地和前陆盆地的岩石圈结构特征,指出在古裂谷、褶皱带或区域性深断裂等陆壳构造薄弱带上发育起来的多期叠合盆地,具有很好的含油气前景。大型含油气盆地往往存在地幔上隆、地壳减薄和地壳内低速层,盆地基底沉降与盖层沉积厚度较大。适度的后期构造活动改造和岩浆活动有利于沉积盆地内油气生成与保存。     

四川盆地：周缘活动主控下形成的叠合盆地

四川盆地位于扬子板块西缘和青藏高原东缘,地震勘探资料等揭示盆地前寒武纪基底保存完整的古俯冲带和地堑-地垒结构,说明盆地基底后期构造活动非常稳定;显生宙以来经历晚震旦世-石炭纪、二叠纪-中三叠世两幕克拉通边缘强拉张-强挤压,而克拉通内弱拉张-弱挤压的构造演化过程,体现出盆地内部稳定性结构沉积演化特征。克拉通内弱拉张初期以海相碳酸盐岩大面积稳定沉积（即震旦系灯影组和二叠系栖霞-茅口组）和随后的风化壳岩溶作用（即桐湾期、东吴期等不整合面）为特征,弱拉张期以拉张槽（如：绵阳-长宁拉张槽和开江-梁平拉张槽等）的形成为典型特征;弱挤压则以古隆起（如：加里东期乐山-龙女寺古隆起、印支期泸州古隆起等）的发育为典型特征。四川盆地晚三叠世后的前陆盆地演化阶段受控于其周缘造山带逆冲推覆构造活动,是现今地貌和构造盆地的主要建造期,形成了四川盆地周缘突变（线型）和渐变（弥散型）两种盆山结构。盆地西边界（龙门山）和北边界（米仓山-大巴山）即是线型突变边界,也是扬子地块（板块）的边界,边界几何形状和扬子板块刚性特征对盆山系统结构-构造特征等有较大的控制作用;四川盆地的东边界（齐岳山-大娄山）和西南边界（大凉山）即是渐变弥散型边界,同时也是板（陆）块内部的边界,它们受控于邻区（盆外）的构造变形和盆内沉积盖层中滑脱层的分布特征。受控于盆地（克拉通）周缘活动,四川盆地垂向上前寒武纪基底与盖层、盖层内早期和晚期构造具解耦特征。基底与盖层构造的解耦有利于盆地内部前寒武纪基底结构构造的保存和盖层内大型隆-坳结构的形成演化;盖层内早期和晚期构造的解耦有利于早期构造免遭后期破环,对深层油气藏的保存意义重大。总之,四川盆地可能是具独特形成过程和特征的叠合盆地新类型,其突出特征表现为周缘活动、内部稳定及早期和晚期构造解耦。     

A survey of numerical methods for stochastic differential equations

The development of numerical methods for stochastic differential equations has intensified over the past decade. The earliest methods were usually heuristic adaptations of deterministic methods, but were found to have limited accuracy regardless of the order of the original scheme. A stochastic counterpart of the Taylor formula now provides a framework for the systematic investigation of numerical methods for stochastic differential equations. It suggests numerical schemes, which involve multiple stochastic integrals, of higher order of convergence. We shall survey the literature on these and on the earlier schemes in this paper. Our discussion will focus on diffusion processes, but we shall also indicate the extensions needed to handle processes with jump components. In particular, we shall classify the schemes according to strong or weak convergence criteria, depending on whether the approximation of the sample paths or of the probability distribution is of main interest.     

Study on Statistical Features About Weak Earthquake Activity Before Moderately Strong Earthquakes in the Middle Northern Part of the Qinghai-Xizang （Tibet） Block

In regards to the earthquakes recording M ≥ 5.0 that occurred in middle northern part of the Qinghai-Xizang （Tibet） Block from 1970 - 2003, in this study we describe the temporal and spatial centralization features of the weak earthquakes and the enhancement and anomalous quiescence of their seismic activity before main shocks through 4 parameters, which are basically not correlated： earthquake time centralization degree parameter Ct, earthquake space centralization degree parameter Cd, η value and weak earthquake frequency and so on. On the basis of calculation results, it has been seen that before earthquakes with M ≥ 5.0 took place in the middle northern part of the Qinghal-Xizang （Tibet） Block, the frequency of weak earthquakes often shows ascent and drop, their strength shows an obvious enhancement and the centralization distribution with time and space is evident.     

裂缝型储层预测技术优选——以塔北地区奥陶系为例

塔北地区奥陶系碳酸盐岩裂缝型储层的地震反射特征总体表现为弱振幅,常用技术难以预测。通过预测技术优选发现相关分量P1属性能够较好地预测这类储层。应用该属性分别对塔北英买2井区奥陶系一间房组、轮古7井区奥陶系鹰山组以及轮古东地区奥陶系良里塔格组的弱振幅反射的裂缝型储层进行了预测,结果与实钻有较高的吻合率。     

Weak stability boundary trajectories for the deployment of lunar spacecraft constellations

Suitable lunar constellation coverage can be obtained by separating the satellites in inclinations and node angles. It is shown in the paper that a relevant saving of velocity variation ΔV can be achieved using weak stability boundary trajectories. The weakly stable dynamics of such transfers allows the separation of the satellites from the nominal orbit to the required orbit planes with a small amount of ΔV. This paper also shows that only one different set of orbital parameters at Moon can be reached with the same ΔV manoeuvre starting from a nominal trajectory and ending at a fixed periselenium altitude. In fact, such a feature is proved to be common to other simpler dynamical systems, such as the two- and three-body problems.     

坝基软弱结构面工程特性的动态研究方法与应用

水电工程具有规模大、施工快、地质缺陷不易揭露等特点,特别是对于水电工程的安全运营至关重要的深层抗滑稳定性问题.基于上述原因,本文以金沙江观音岩水电站为例,借助坝基开挖,总结出工程地质条件软弱结构面展布特征动态评价软弱结构面参数动态取值坝基稳定性评价这一套坝基软弱结构面动态评价方法,并以软弱结构面展布特征与参数动态研究为核心,建立起合理的坝基深层抗滑稳定性评价方法.实践表明,该套方法能合理地评价重力坝抗滑稳定性问题,保证水电工程的安全运营.     

Acoustic-Gravity Waves from Bolide Sources

We have developed a new approach to modeling the acoustic-gravity wave (AGW) radiation from bolide sources. This first effort involves entry modeling of bolide sources that have available satellite data through procedures developed in ReVelle (Earth Moon Planets 95, 441–476, 2004a; in: A. Milani, G. Valsecchi, D. Vokrouhlicky (eds) NEO Fireball Diversity: Energetics-based Entry Modeling and Analysis Techniques, Near-earth Objects: Our Celestial Neighbors (IAU S236), 2007b). Results from the entry modeling are directly coupled to AGW production through line source blast wave theory for the initial wave amplitude and period at (at 10 blast wave radii and perpendicular to the trajectory). The second effort involves the prediction of the formation and or dominance of the propagation of the atmospheric Lamb, edge-wave composite mode in a viscous fluid (Pierce, J. Acoust. Soc. Amer. 35, 1798–1807, 1963) as a function of the source energy, horizontal range and source altitude using the Lamb wave frequency that was deduced directly during the entry modeling and that is used as a surrogate for the source energy. We have also determined that Lamb wave production by bolides at close range decreases dramatically as either the source energy decreases or the source altitude increases. Finally using procedures in Gill (Atmospheric-Ocean Dynamics, 1982) and in Tolstoy (Wave Propagation, 1973), we have analyzed two simple dispersion relationships and have calculated the expected dispersion for the Lamb edge-wave mode and for the excited, propagating internal acoustic waves. Finally, we have used the above formalism to fully evaluate these techniques for four large bolides, namely: the Tunguska bolide of June 30, 1908; the Revelstoke bolide of March 31, 1965; the Crete bolide of June 6, 2002 and the Antarctic bolide of September 3, 2004. Due to page limitations, we will only present results in detail for the Revelstoke bolide.     

The study on the interannual variation and the mechanism of the south china sea monsoon

l.Intr0ductionTheonset0ftheSouthChinaSea(SCS)monsoonisasignofthecomingoftheAsianmonsoon.Inaverage,theonsetoftheSCSmonsoonisinthemiddleofMay,butitsstrengthandtheonsetdatediffergreatlyfromoneyeartoanother.TheanomaliesoftheSCSmon-soonhighlydePendonnotonIytheprecipitationinSCS,butalsotheanomaliesofthecircu-lationintheworld.WhyisthemonsoononsetearliestinSCS?Whatisthemechanismoftheonsetanditsvariation?Thisisascientificproblemthatisinterestedinbymeteorologistsbothathomeandabroad.TaoandChen…