软岩的强度—变形—时间之间关系的试验分析

对软岩和有不连续面的软岩试样进行一系列固结不排水三轴压缩和蠕变试验,测定并分析了它们在正常固结和超固结状态下的应变软化性状、蠕变特性和残余强度的变化规律。探讨了软岩中存在的不连续面对应力－应变关系、残余强度特性和蠕变应变速率的影响。     

南宁市引种金花茶的气候分析与评价

依据原种金花茶的生态特性及引种试验结果,通过分析南宁市的气候条件得出,南宁市适宜种植金花茶的结论     

Errors prediction for vector-to-raster conversion based on map load and cell size

Vector-to-raster conversion is a process accompanied with errors.The errors are classified into predicted errors before rasterization and actual errors after that.Accurate prediction of the errors is beneficial to developing reasonable rasterization technical schemes and to making products of high quality.Analyzing and establishing a quantitative relationship between the error and its affecting factors is the key to error prediction.In this study,land cover data of China at a scale of 1:250 000 were taken as an example for analyzing the relationship between rasterization errors and the density of arc length(DA),the density of polygon(DP) and the size of grid cells(SG).Significant correlations were found between the errors and DA,DP and SG.The correlation coefficient(R2) of a model established based on samples collected in a small region(Beijing) reaches 0.95,and the value of R2 is equal to 0.91 while the model was validated with samples from the whole nation.On the other hand,the R2 of a model established based on nationwide samples reaches 0.96,and R2 is equal to 0.91 while it was validated with the samples in Beijing.These models depict well the relationships between rasterization errors and their affecting factors(DA,DP and SG).The analyzing method established in this study can be applied to effectively predicting rasterization errors in other cases as well.     

GIS-based Mineral Prospectivity Mapping of Seafloor Massive Sulfide on Ultraslow-spreading Ridges: A Case Study of Southwest Indian Ridge 48.7°–50.5° E

With the depletion of mineral resources on land, seafloor massive sulfide deposits have the potential to become as important for exploration, development and mining as those on land. However, it is difficult to investigate the ocean environment where seafloor massive sulfide deposits are located. Thus, improving prospecting efficiency by reducing the exploration search space through mineral prospectivity mapping (MPM) is desirable. MPM has been used in the exploration for seafloor deposits on regional scales, e.g., the Mid-Atlantic Ridge and Arctic Ridge. However, studies of MPM on ultraslow-spreading ridges on segment scales to aid exploration for seafloor massive sulfide have not been carried out to date. Here, data of water depth, geology and hydrothermal plume anomalies were analyzed and the weights-of-evidence method was used to study the metallogenic regularity and to predict the potential area for seafloor massive sulfide exploration in 48.7°–50.5° E segments on the ultraslow spreading Southwest Indian Ridge. Based on spatial analysis, 11 predictive maps were selected to establish a mineral potential model. Weight values indicate that the location of seafloor massive sulfide deposits is correlated mainly with mode-E faults and oceanic crust thickness in the study area, which correspond with documented ore-controlling factors on other studied ultraslow-spreading ridges. In addition, the detachment fault and ridge axis, which reflect the deep hydrothermal circulation channel and magmatic activities, also play an important role. Based on the posterior probability values, 3 level A, 2 level B and 2 level C areas were identified as targets for further study. The MPM results were helpful for narrowing the search space and have implications for investigating and evaluating seafloor massive sulfide resources in the study area and on other ultraslow-spreading ridges.

     

More than two hundred and fifty thousand spectroscopic binary or variable star candidates discovered by LAMOST

About 786.4 thousand stars were observed by LAMOST twice or more during the first stage of its spectroscopic survey. The radial velocity differences for about 256 thousand targets are larger than10 km s^-1 and they are possible spectroscopic binary or variable candidates(SBVCs). It is shown that most SBVCs are slightly metal poorer than the Sun. There are two peaks in the temperature distribution of SBVCs around 5760 K and 4870 K, while there are three peaks in the distribution of the gravitational acceleration at 2.461, 4.171 and 4.621 cm s^-2. The locations of SBVCs on the [Fe/H]-T, [Fe/H]-log g, log g-T and H-R diagrams are investigated. It is found that the detected SBVCs could be classified into four groups. The first group has higher log g～4.621 and lower T ～ 4870 K which are mainly cool red dwarf binaries. The second group of SBVCs has logg around 4.171 cm s^-2 that includes binaries and pulsating stars such as δSet and γ Dor variables. The gravitational accelerations of the third group of SBVCs are higher and some of them are below the zero-age main sequence. They may be contact binaries in which the primary components are losing energy to the secondaries in the common envelopes and are at a special stellar evolutionary stage.The last group is composed of giants or supergiants with log g around 2.461 cm s^-2 that may be evolved pulsating stars. One target(C134624.29+333921.2) is confirmed as an eclipsing binary with a period of 0.65 days. A preliminary analysis suggests that it is a detached binary with a mass ratio of 0.46. The primary fills its critical Roche lobe by about 89%, indicating that mass transfer will occur between the two components.     

Orbital evolution of a planet with tidal dissipation in a restricted three-body system

The angle between planetary spin and the normal direction of an orbital plane is supposed to reveal a range of information about the associated planetary formation and evolution. Since the orbit's eccentricity and inclination oscillate periodically in a hierarchical triple body and tidal friction makes the spin parallel to the normal orientation of the orbital plane with a short timescale in an isolated binary system, we focus on the comprehensive effect of third body perturbation and tidal mechanism on the angle. Firstly, we extend the Hut tidal model(1981) to the general spatial case, adopting the equilibrium tide and weak friction hypothesis with constant delay time, which is suitable for arbitrary eccentricity and any angle ? between the planetary spin and normal orientation of the orbital plane. Furthermore, under the constraint of angular momentum conservation, the equations of orbital and ratational motion are given. Secondly, considering the coupled effects of tidal dissipation and third body perturbation, and adopting the quadrupole approximation as the third body perturbation effect, a comprehensive model is established by this work. Finally, we find that the ultimate evolution depends on the timescales of the third body and tidal friction. When the timescale of the third body is much shorter than that of tidal friction, the angle ? will oscillate for a long time,even over the whole evolution; when the timescale of the third body is observably larger than that of the tidal friction, the system may enter stable states, with the angle ? decaying to zero ultimately, and some cases may have a stable inclination beyond the critical value of Lidov-Kozai resonance. In addition, these dynamical evolutions depend on the initial values of the orbital elements and may aid in understanding the characteristics of the orbits of exoplanets.     

由卫星云图获取云层分布等值线图

大气中云的分布状况是气象预报的重要依据。本文探讨了利用卫星云图对云的分布作定量分析的可能性。并提出了一种通过红外云图获取云顶高度等值线的快速算法,最后给出了一些实验结果。     

从第二次土地调查看上海市地籍管理

本文分析了上海市第二次土地调查中地籍调查的技术方法,结合上海市地籍管理现状,根据实际工作需要,提出改进和完善地籍管理的几点思考。     

新疆北部镁铁-超镁铁质岩的PGE成矿问题

铂族元素(PGE)矿化主要与镁铁-超镁铁杂岩有关,成矿类型主要为岩浆型矿床,这类PGE矿床的形成主要依赖两个条件:一是岩浆中富含PGE;二是具备PGE从岩浆中分离和富集的机制,主要是在岩浆演化过程中硫达到饱和。新疆北部镁铁-超镁铁质杂岩发育,并产有喀拉通克、黄山、黄山东、图拉尔根4个大型铜镍矿床和香山、土墩、葫芦、白石泉等中、小型铜镍矿,以及香山西、尾亚等中型钒钛磁铁矿矿床,但迄今尚未发现成型的PGE矿床。文中通过对PGE矿床的形成机制与镁铁-超镁铁杂岩源区特征研究,探讨了北疆地区PGE矿床的成矿问题。综合分析认为,新疆北部后碰撞镁铁-超镁铁质岩的岩石类型为经过了分离结晶形成的铁质岩石系列,是PGE矿床的有利容矿岩石;矿床的Sr、Nd、Pb、O、Os和S同位素和含矿岩石地球化学特征表明,铜镍硫化物矿床含矿岩浆在岩浆演化和成矿过程中有地壳物质加入并可导致硫化物熔离作用,说明在成矿机制上也存在形成岩浆型PGE矿化的条件。新疆北部PGE矿化微弱的原因可能在于该区广泛发育的亏损型地幔源(具正的εNd值特征),这一亏损型地幔可能部分源于洋壳熔融,与产于后碰撞造山带环境、发育于"洋壳"或"不成熟"陆壳基底之上有关,由此决定了原始岩浆为贫PGE的源区,因此不利于PGE的富集成矿。     

鄂尔多斯盆地天环坳陷迁移演化与坳陷西翼油气成藏

鄂尔多斯盆地是我国陆上最重要的含油气盆地之一,本文以鄂尔多斯盆地西缘为研究对象,以地震反射资料为基础,主要采用地震剖面层拉平与平衡剖面恢复等技术手段,对天环坳陷形成与迁移演化历史进行了动态分析。研究结果表明:1)天环坳陷最早形成于晚侏罗世,后期由于受燕山晚期及喜马拉雅山期构造运动影响,坳陷核部逐渐向东迁移至现今位置,前后累计迁移距离约30 km;2)当坳陷核部向东迁移至有效烃源岩范围附近时,原先已形成的油气藏发生重新调整,油气向坳陷西翼高部位运移、聚集,从而形成了次生构造油气藏。