山东省泰安市大汶口盆地岩盐矿地质特征及开发意义

大汶口盆地岩盐矿均为第四系所覆盖,钻孔揭露,除第四系外,主要为古近系官庄群大汶口组。大汶口盆地主要是由南留断裂所控制。岩盐矿是大汶口盆地盐类矿床的主体,矿层多而集中,厚度大而变化小,品位高而稳定。矿层延展面积约45km3,其平面形态为一个椭圆形,在空间上整个含盐段似一个向北缓倾的大透镜体。矿石自然类型有3种,即块状岩盐（灰白盐）、含杂质岩盐（杂色盐）和脉状岩盐,其中以块状岩盐为主,含杂质岩盐次之,脉状岩盐不具有工业意义。该矿床地质条件好、埋藏深度适宜,外部建设条件好,该矿床具备大规模开发的条件,矿业开发可促进当地的经济发展.当地政府有关部门已在着手工作,推动该岩盐矿规模开发进程。     

Nonstationary dynamic control of seismic activity of platform regions by mid-ocean ridges

The plot of temporal variation in the seismic activity level in the central and eastern North American platform (NAP) is shown to be similar to that for the Mid-Atlantic Ridge (MAR). This fact was previously noted for Fennoscandia [Skordas et al., 1991]. The characteristic features of the MAR plot recur approximately every three years for Fennoscandia and every four to eight years for the NAP. These data indicate that the mid-ocean ridge largely controls the seismic activity of the adjacent platforms. The control is provided by the ridge push force. As a result of variations in this force due to the nonstationary process of dike intrusion in the axial zone of the ridge, disturbances of the stationary stress-strain state of the lithosphere migrate from the ridge. Using the Elsasser model, the observed time shift can be used for estimating the viscosity of the asthenosphere, amounting to 10¹⁷ Pa s with an accuracy of ±30% in the case considered. The disturbance amplitudes decaying away from the ridge are high enough to change the seismic activity of the adjacent platforms.     

The territory of Georgia and surrounding countries in the Upper Cretaceous: paleomagnetic data

Paleomagnetic researches of the Upper Cretaceous rocks, collected from 24 cross-sections (530 samples) of Georgia have shown that only nine samples are suitable for the paleotectonic problem to be solved. The method of thermomagnetic cleaning was used for the paleomagnetic directions of these rocks to be determined. Magnetic-mineralogical data and the tests of paleomagnetic accuracy have proved the ancient age of the stable part of the natural remnant magnetization (NRM) that is close to the initial one. The study results have demonstrated that the position of the areas studied in the Upper Cretaceous time was located 11°–18° southward from their modern latitudinal position; the distance between structures of the Great Caucasus and Trans-Caucasus was 10°–14°. The wide variations of the paleoinclinations are connected with the local turns of tectonic blocks     

Radial velocities of the components of multiple star systems of Trapezium type. I

Translated fromAstrofizika, Vol. 36, No. 2, pp. 273–275, April–June 1993.     

Neutron stars in the multidimensional einstein theory of gravitation

The radius, mass, total number of baryons, and other parameters of static, spherically symmetric, superdense stars are calculated. A model with one Ricci-flat inner space of arbitrary dimensionality and the approximation p₁=?0.5ε + ap for additional components of the energy — momentum tensor are used (ε and ρ are the total energy density and the pressure of the stellar matter and a is a fitting parameter). In the case of white dwarfs, the results of the multidimensional theory do not depend on the dimensionality D of space-time for ?10 ? a ? 10 and coincide with the analogous data of the general theory of relativity (GTR). For neutron stars there is a dependence on D and a. For D>4, in particular, the greatest mass M_max of a neutron star as a function of a has a maximum at 3<a(D) ? 4, which exceeds the greatest mass M _max ⁰ =2.14 M_⊙ in the GTR. A comparison of theoretical results with observational data determines the allowable values of a. Data for PSR 1913 + 16 lead to 0.2 ≤ a ≤ 9.2 in the case of D=26, while the results of [P. C. Joss and S. A. Rappaport, Annu. Rev. Astron. Astrophys.,22, 537 (1984)] lead to the stricter limits 1 ≤ a ≤ 7.4.     

The gravitation theory in bimetric formulation

The gravitation theory is considered in bimetric formulation with a Lagrangian of the most common type and quadratic with respect to the derivativesg _ik/l of the metric tensor. Restrictions on the dimensionless parameters of the theory are found, basing on the comparison with the Newtonian theory and the analysis of corresponding observational data in the vicinity of the solar system. Propagation of the weak gravitation waves is investigated in the outside gravitational field.     

南阿尔金木纳布拉克地区高压泥质麻粒岩的确定及其地质意义

南阿尔金木纳布拉克地区出露一套典型的高压泥质麻粒岩,其峰期特征矿物组合为Grt+ Ky+ Kfs+Qz+Ilm.根据矿物内部一致性热力学数据和Thermocalc3.33程序计算,确定其峰期变质温压条件为T＞850℃和P＞11kbar.结合岩相学研究和P-T视剖面图计算,可识别出该岩石经历了3个阶段的变质演化,构成了一个早期降温降压,后期近等压降温的顺时针型的退变质P-T演化轨迹.该岩石锆石阴极发光图像显示其内部具有明显的核-边结构,核部为残留的原岩碎屑锆石,边部则表现为面状生长的变质锆石的特征.微区原位LA-ICP-MS微量元素分析和锆石U-Pb定年表明,该岩石原岩的形成时代上限值约为579Ma,变质年龄为486±5Ma.该麻粒岩与南阿尔金淡水泉地区的高压麻粒岩具有相似变质演化轨迹和一致的峰期变质年龄,亦与南阿尔金其它超高压岩石的峰期变质年龄一致,表明它们都是南阿尔金陆壳深俯冲作用引发的高压-超高压变质事件的产物,它们共同构成南阿尔金高压-超高压变质带.同时代的UHP榴辉岩和高压麻粒岩共存的现象,可以很好地利用“俯冲隧道模型”来解释,即可能是由于陆壳在深俯冲过程中不同深度不同热状态下发生拆离作用后折返引起的.另外,该麻粒岩的原岩形成时代(约为579Ma),可能为新元古代晚期,与南阿尔金高压-超高压岩石的原岩形成时代基本一致或稍晚,因此不应再作为岩石地层单元划归为“长城系”,而应归属为南阿尔金高压-超高压变质岩带的一部分.     

长牡蛎繁殖周期、生化成分的季节变化与环境因子的关系

为了阐明长牡蛎的繁殖策略,自2004年3月—2005年2月对乳山湾养殖海区的环境因子(水温、盐度、叶绿素a含量)、长牡蛎繁殖周期及其生化成分(糖原、脂肪、蛋白质、RNA/DNA比值)的季节变化进行研究。结果显示,水温在一年中呈现显著变化,夏季水温最高,最高值为29.5℃(8月),冬季水温最低,最低值为1.8℃(1月);盐度在夏季雨水较多的时候略有降低;叶绿素a含量在夏末秋初(8月和9月)和春季(4月)有2个峰值,冬季最低。长牡蛎的繁殖周期分为冬季的休止期和从春季到夏季的繁殖期,在长牡蛎的繁殖期,条件指数逐渐下降到最低值,表明繁殖期长牡蛎生长变慢。在长牡蛎的配子发生过程中软体部蛋白质和脂肪含量略有上升,而糖原含量显著下降,表明长牡蛎配子的发生需要储存的糖原提供能量;RNA/DNA比值在配子发生过程中逐渐升高,显示RNA/DNA比值可以作为一个指标来指示长牡蛎的性成熟。配子发生过程中,长牡蛎的灰分含量逐渐升高,表明长牡蛎通过分解自身的贮能物质提供能量,使体内有机物含量减少,从而导致灰分含量上升。实验结果表明长牡蛎的配子发生类型为保守种。     

Vibration analysis of rectangular Mindlin plates on elastic foundations and vertically in contact with stationary fluid by the Ritz method

In this study Free vibration analysis of vertical rectangular Mindlin plates resting on Pasternak elastic foundation and fully or partially in contact with fluid on their one side is investigated for different combinations of boundary conditions. The plate is assumed to be one of vertical rectangular walls of a container in contact with fluid. In order to analyze the interaction of the Mindlin plate with the elastic foundation and fluid system, three displacement components of the plate are expressed in the Ritz method by adopting a set of static Timoshenko beam functions satisfying geometric boundary conditions in a Cartesian co-ordinate system. The method of separation of variables and the method of Fourier series expansion is used to model fluid and to obtain the exact expression of the motion of fluid in the form of integral equations. The fluid domain is finite in depth and width but infinite in the length direction. To demonstrate the accuracy of the present solution, convergence study is first carried out and then a few comparison studies are carried out with the available data in the literature. Finally, natural frequencies of rectangular plates are presented in tabular and graphical forms for different fluid levels, foundation parameters, aspect ratios, thickness to width ratios and boundary conditions.