地球节律的成因

地球节律主要受地球内部能量间歇性的释放所控制。旋转系统有不同于非旋转系统的位能、热能和旋转能的相互转换方式。在重力分异和热对流过程中，地核不仅有巨量热能，而且有巨量的旋转能和放射性蜕变能。这是地球能量释放的内因。天文因素使地球内核周期性地南北振动，使地球轨道、体积，形状、自转速度、公转速度和差异旋转状态周期性地变化。这是地球能量间歇性释放的外因。对作差异旋转的内核而言，万有引力常数Ｇ的变化可以改变太阳辐射量和太阳系体积，影响核幔的角动量交换和地壳地幔容积，造成热幔柱的形成与喷发，控制了核幔边界的能量交换过程。这是天文周期与地质旋回一一对应的原因，也是地球节律产生的根本原因。这使人们可以从天文周期预测地质变动。     

法国中央高原Margeride花岗岩中黑云母岩的起源探讨

法国中央高原Ｍａｒｇｅｒｉｄｅ花岗岩暗色相中包含的Ａｎｃｅ和Ｖａｚｅｉｌｌｅｓ黑云母岩，大小达数十米，分别含有４０％和９０％以上的黑云母及少量的磷灰石、锆石、斜长石或钾长石，且发现有变质岩包体。野外观察可见，黑云母岩与其上覆花岗岩呈逐渐过渡关系，而其下部界限则很分明；它的面状及线状结构与相邻花岗岩的一致。矿物成分显示，各矿物（黑云母、斜长石、磷灰石）的化学成分与相邻花岗岩中相同矿物的相似或相同。由     

鄂西重力地质灾害的研究

综观鄂西地区岩崩、滑坡、坍方和泥石流等地质灾害的成生，笔者认为大宇宙天体运动控制下的内动力和地质基础背景是其成生变形的主要因素，而与大宇宙天体运动有关的各种外动力条件的影响和变化及人类与生物对自然环境的影响和破坏，则是其成生发展的诱发因素。两种变量（即内、外动力）和天体运动的有机组合与变化趋势，使地质灾害成生的类型及其频度、强度、破坏（形变）特征及变形机制不尽相同，变形特征多样。在发生时间和灾害规模上多受天体运动变化规律所制约。据此可对地质灾害的预测、预报进行更深入地研究，并采取相应的防治措施。     

Evolution of the West Andean Escarpment at 18°S (N. Chile) during the last 25 Ma: uplift, erosion and collapse through time

The geological record of the Western Andean Escarpment (WARP) reveals episodes of uplift, erosion, volcanism and sedimentation. The lithological sequence at 18°S comprises a thick pile of Azapa Conglomerates (25–19 Ma), an overlying series of widespread rhyodacitic Oxaya Ignimbrites (up to 900 m thick, ca. 19 Ma), which are in turn covered by a series of mafic andesite shield volcanoes. Between 19 and 12 Ma, the surface of the Oxaya Ignimbrites evolved into a large monocline on the western slope of the Andes. A giant antithetically rotated block (Oxaya Block, 80 km×20 km) formed on this slope at about 10–12 Ma and resulted in an easterly dip and a reversed drainage on the block's surface. Morphology, topography and stratigraphic observations argue for a gravitational cause of this rotation. A “secondary” gravitational collapse (50 km³), extending 25 km to the west occurred on the steep western front of the Oxaya Block. Alluvial and fluvial sediments (11–2.7 Ma) accumulated in a half graben to the east of the tilted block and were later thrust over by the rocks of the escarpment wall, indicating further shortening between 8 and 6 Ma. Flatlying Upper Miocene sediments (<5.5 Ma) and the 2.7 Ma Lauca–Peréz Ignimbrite have not been significantly shortened since 6 Ma, suggesting that recent uplift is at least partly caused by regional tilting of the Western Andean slope.     

Interprétation hydrogéologique de l'aquifère des bassins sud-rifains (Maroc) : apport de la sismique réflexion

The aquifer of the Rharb Basin is constituted by heterogeneous material. The seismic reflexion interpretation carried out in this area, highlighted a permeable device compartmentalized in raised and subsided blocks. Depressions identified in the northern and southernmost zones are characterized by Plio-Quaternary fillings that are favourable to the hydrogeological exploitation. Two mechanisms contribute to structure the Plio-Quaternary aquifer: the Hercynian reactivation in the southernmost part, and the gravitational mechanism of the Pre-Rifean nappe. The groundwater flow and the aquifer thickening are controlled by this reactivation.     

KAGRA引力波探测器中蓝宝石测试镜光学性质研究

低温制冷技术是下一代激光干涉仪引力波探测器的核心技术之一. 日本引力波探测器KAGRA (Kamioka Gravitational Wave Detector)作为该技术的前沿开拓者, 将运行在20K的超低温环境中, 并使用在低温下热噪声较低的单晶蓝宝石晶体作为测试镜. 然而, 高质量大尺寸低吸收率的蓝宝石晶体极难制备. 此外, 由于蓝宝石晶体存在晶格结构不均匀, 很容易导致不必要的双折射效应, 从而影响探测器的目标灵敏度. 基于上述问题, 开发了两套大尺寸光学测量系统, 首次系统研究了KAGRA低温蓝宝石测试镜的光学特性. 首先, 根据探测器对测试镜热噪声的要求, 开发了一套基于光热共光路干涉技术的光学测量系统, 该系统可对测试镜以及测试镜表面涂层的光学吸收进行有效的表征. 其次, 基于光学吸收测量系统, 开发了一套双折射效应测量系统, 该系统可以有效表征测试镜中双折射的均匀性. 目前两套测量系统的搭建与调试已完成, 对蓝宝石测试镜光学吸收的测量灵敏度达到了1.5ppm/cm, 双折射测量系统的空间分辨率小于0.3mm times 0.3mm. 该工作对降低大尺寸低温测试镜双折射效应及提高探测器灵敏度具有重要意义.     

土剪切流变试验仪改进设计

土流变测定仪由土剪切试验仪改制而成,主要由剪切仪机架、剪切盒、垂直荷载杠杆加压系统、水平剪力施加系统等部件组成。水平剪力施加系统采用重力加压,两级变矩传动,传动系中配置了滚动轴承,安装了测力计,保证了试验数据的准确性。该土流变测定仪重量轻,体积小,结构紧凑,操作简便,具有剪切试验和流变试验两用功能。     

Elliptic-type motion in Fock's gravitational field

The elliptic-type motion in the gravitational field found by Fock as exact solution of Einstein's vacuum equations in the case of spherical symmetry (Solution called here Fock's gravitational field) is studied by means of a classic method based on the perturbation theory. Regarding the deviations of the orbit from a Kepleian orbit as perturbations, the first and second order variations of the Keplerian orbital elements over one nodal period as well as those of the nodal period itself are determined.     

The stability of tension stars

By studying the cylindrically symmetric solution for matter in 2+1 space-time dimensions we arrive at stability criteria for such a configuration when the local energy density is proportional to the square of the tension (negative pressure). Our analysis demonstrates that to the post-Newtonian approximation that such a configuration is stable provided it does not shrink below a certain radius. We find our model provides a reason for how stars form from a two-dimensional configuration with both a maximum mass and a minimum radius.