土的弹塑性应力——应变模型理论(续)

四、弹塑性应力应变模型十几年来学者们建议采用的应力～应变数学模型有许多种.在弹性模型方面最常使用的模型有两种.第一种是以E(杨氏模量)及v(泊桑比)两种弹性常数表达的称E～v弹性模型.第二种是以K(体积变形模量)及G(剪切模量)两个弹性常数表达的称K～G弹性模型.这两种弹性模型将在本章中介绍.     

Theory of Elastoplastic Stress-Strain Model for Soil

This paper first introduces the currently adopted stress-strain symbols，some specific terms and their definitions，the commonly used stress-strain testing methods and the formulations for test results。Then，the incremental elastoplastic theories upen which mathematical models are finally given。     

一种硼酸盐的新矿物─—袁复礼石

袁复礼石是一种Ｍｇ、Ｆｅ￣（３＋）、Ａｌ和Ｔｉ的硼酸盐新矿物，发现于辽宁省宽甸县砖庙硼矿区。该矿物黑色，近不透明，金刚光泽一半金属光泽。反射色亮灰，内反射深红褐色。非均质性弱，偏光色红褐。晶体呈细柱状，０．１×０．２×１ｍｍ。晶体化学式为：空间群：Ｈ＝５－６，ＶＨＮ＿（５０）＝８４３ｋｇ／ｍｍ￣２。｛１００｝解理完全。红外光谱吸收谱带为：１３８７，１２１０，１０２４，９５１，７３３，６００，５１０和４０８ｃｍ￣（－１）。穆斯堡尔谱证明，以三价铁为主，二价铁较少。Ｆｅ￣（３＋）占据Ｍ（１）晶位，Ｆｅ￣（２＋）占据Ｍ（１）和Ｍ（２）晶位。袁复礼石为硼钛镁石的富Ｆｅ￣（３＋）类似物。     

非接触极化曲线视反应电位差区分矿体矿物成分及确定其边界的实验研究

本文用非接触极化曲线视反应电位差区分矿体矿物成分和确定矿体边界的基本原理，着重阐述矿物非接触极化曲线视反应电位差特征的实验研究方法和结果，并指出非接触极化曲线视反应电位差区分矿体矿物成分和确定矿体边界是有可能的。     

石墨炉原子吸收光谱法测定地质样品中微量银

样品经盐酸-硝酸分解处理,以硫酸铵为基体改进剂,石墨炉原子吸收光谱法测定地质样品中微量的银.结果表明该方法简便、快速、准确,相对标准偏差（RSD,n=6）为1.89％～6.70％,加标回收率为94％～106％.     

AHDEB油田白垩系油藏油气充注期次的流体包裹体证据

伊拉克AHDEB油田油藏成藏规律对油田后期开发具有重要意义, 与埋藏史相结合的流体包裹体研究是揭示油藏油气成藏期次和时间的有效手段.利用伊拉克AHDEB油田白垩系油藏储层样品对流体包裹体特征进行了分析, 并且通过流体包裹体的显微观察、荧光颜色、单一包裹体的红外光谱和均一温度测定, 结合地质背景对该油田的油充注期次进行了研究.研究表明, 油包裹体以发绿色和黄绿色荧光为主, 少数发浅黄色和黄褐色荧光.油包裹体的显微傅立叶红外光谱测定结果计算的CH_2a/CH_3a、X_inc、X_std可划分油的成熟度, 表明存在两种成熟度的油.最后, 根据均一温度测定结果, 结合埋藏史和热史, 认为该油田可能存在4期油充注成藏相关的流体活动: 第1成藏期发生在95.0~96.5Ma, 相当于晚白垩世早期; 第2成藏期为71.0~78.5Ma, 相当于晚白垩世晚期, 第1期和第2期烃源岩排烃规模小, 产生中-重质油, 后期遭受氧化而形成沥青; 第3成藏期发生在14.0~15.0Ma, 相当于中中新世, 处于生排烃高峰期, 为主要成藏期; 第4期发生在10.0Ma左右, 与第3期为多幕连续充注.      

A Preliminary Study on Dust Grains in the Stratosphere

Collected by means of a high-altitude scientific balloon and a self-made automatic sample collector,a total of 276 dust grains were selected for the study of shape,grain size and optical property.Some of the grains were examined by X-ray diffraction and electrom microprobe techniques,The stratospheric dust grains can be classified as 6 types:cosmic dusts,cosmic dusts(?),microtektite,natural pollutants,artificial pollutants and the unknown substances.The different types of dust grains have different characters and distinguishing symbols.Widespread in the space of the solar system,cosmic dusts are the initial substances of the solar system and ,to some degree,have recorded a great wealth of information on the early history of the solar system.So they have become one of the important objects in the field of cosmochemistry at present time,Since the 1960‘s,scholars of many countries have collected cosmic dusts both in the space near the earth(using rock ets,space probes and space shuttles)and in the stratosphere (using high-altitude balloons or U-2air planes).According to the shape(the scanning electron microimage),element composition(the energy-dispersive X-ray spectrum)and optical properties of dust grains,the substances in the stratosphere can be classified as 5 types:cosmic dusts,alumina spheroids,terrestrial artificial pollutants,terrestrial natural pollutants and unknown substances(CDPET,1982).     

Experimental Study of Failure Zone in Soil and Rock Blast

In this paper, according to in situ experimental data of sonic, seismic, hole television, acceleration, velocity and visual investigaton after explosion, we consulted laboratory experimental results. Study in soil and rock blasr destroy effect and zone. By comparing with blast destroy zone of rock mass, vartical tunnel, parallal tunnel.     

安康双龙桥碱性辉长杂岩中磷灰石和榍石的矿物成分研究

X射线衍射分析和化学成分研究表明,磷灰石为氟磷灰石,榍石成分中存在着的主要类质同象替代是(Fe~(3+)、Al)+(F,OH)~-=Ti~(4+)+O~(2-)。磷灰石和榍石是碱性辉长岩的REE、Ba、Zr等微量元素的主要载体;它们是在较高氧逸度的条件下结晶的。磷灰石的Sr同位素特征说明形成双龙桥碱性辉长杂岩的物质来源于上地幔。     

REE Geochemistry in the Weathered Crust of Granites, Longnan Area,Jiangxi Province

Warm and humid climate and gentle hilly topography have provided favourable conditions for the devel-opment of the weathering crust of the granite intrusions in the Longnan area, Jiangxi Province. REE is mostlyconcentrated in an adsorption state in clay in the wholly weathered zone. The rare-earth minerals enriched inthe parent rocks provided the source material for the REE enrichment. Exchangeable REE accounts for48-86%. Extraction experiments and stable isotopic study of clay minerals suggest that the downward infiltra-tion of meteoric water and increasing gradient of pH values have played an important role in the enrichment ofREE during the progressive weathering. Slight fractionation of individual REE can not change their distribu-tion patterns in the profiles. which are inherited from the parent rocks.