鲁西邹平盆地中生代火山岩的演化:对地幔源区的约束

邹平盆地中生代火山岩可分为三个亚组：中、下亚组具有相似的岩石组合,岩性主要为玄武岩-粗面玄武岩-玄武质粗面安山岩-粗面安山岩;上亚组岩性主要为粗面安山岩。火山岩由早期基性向晚期中偏碱性方向演化,与正常岩浆房酸度增高的岩浆分异趋势相同。具有Rb、Ba、Sr等大离子亲石元素（LILE）和轻稀土元素（LREE）富集,Nb、Ta、Ti等高场强元素（HFSE）相对亏损,类似于岛弧火山岩的地球化学特征。Nb／La、Hf／Sm比值随MgO的降低而升高或基本不变,说明高场强元素亏损是岩浆的原始特征。各亚组火山岩相似的稀土配分模式和微量元素蛛网图,表明它们具有共同的岩浆源区和密切的成因联系,分离结晶起了关键性作用。La／Nb、La／Ta、Ba／Nb比值较高,说明成岩物质可能主要来自岩石圈地幔。拆沉的大陆中、下地壳部分熔融形成的熔体与古生代岩石圈地幔（亏损的地幔橄榄岩）的相互作用是岩石圈地幔富集的重要方式,随之该富集地幔在陆内岩石圈伸展和区域热异常的双重作用下发生减压部分熔融而形成具有岛弧特征的邹平盆地火山岩。     

两种随机地下水位动态预测模型在吉林西部的应用与对比

时间序列模型和人工神经网络模型是两种常见的地下水资源模拟预测模型,为了对比二者的优缺点,本文对比分析了两者的建模过程及其模拟精度.选择吉林省西部干旱半干旱区为研究区,该区地下水资源在过去10年问由于长期超采而导致地下水位持续下降.相比ANN模型,时间序列模型建模过程更为简单,计算效率更高."后验差"检验结果表明两种模型均能很好的模拟地下水位变化规律,但改进ANN具有更高的拟舍精度.同时,两种模型预报结果均显示研究区如继续按过去的开发模式开采地下水,地下水位还将持续下降,且下降速率逐步增大.     

杭州泗岭铝质A型花岗岩的发现及其构造意义

初步研究表明,以往被认为是典型的S型花岗岩或改造-重熔型花岗岩的泗岭岩体应为铝质A型花岗岩。该岩体高硅、碱、钾而明显贫钙、镁;高(K2O Na2O)/CaO值(平均16.79)和AKI指数(平均0.92);FeO*/MgO比值大(平均13.95),高于M型、S型和I型花岗岩,而与世界A型花岗岩平均值(13.4)相近;岩石为弱碱性、准铝-弱过铝质,富含稀土元素、HFSE元素,高Rb、F和Nb,反映其具A型花岗岩的成分特征。泗岭岩体氧同位素δ18O为 8‰～ 9‰,反映岩浆主要起源于下地壳。该岩体侵位于拉张的构造环境,是晚白垩世早期一次重要的构造-岩浆热事件,同时也反映了区域性孝丰—三门湾大断裂与学川—湖州大断裂在晚白垩世早期处于拉伸阶段。     

深层裂缝性储层防漏堵漏实验评价研究

深层裂缝性气藏具有异常高压、高产等特点,钻井完井过程中易出现又喷又漏等复杂事故,因此需做好“防漏为主、堵漏为辅”的防漏堵漏措施。通过全尺寸堵漏装置进行了高压静态、动态模拟堵漏实验,优选配方组合,并系统评价了防漏、堵漏配方的封堵能力、承压能力以及酸溶性,评价研究出的防漏堵漏配方,具有酸溶率高、堵塞强度高、返排效果好等特点,为防漏、堵漏方案现场实施提供依据。     

地下管线内损伤电视检测系统的研制

介绍了地下管线内损伤电视检测系统的基本结构、工作原理、主要技术参数及其现场试验情况。     

阿尔金南缘构造带西段辉绿岩墙群的地球化学特征及构造环境

对阿尔金南缘构造带西段辉绿岩墙群的岩石学和地球化学的详细研究表明,该区辉绿岩墙群为拉斑系列岩石,其主量元素以中等TiO2(1.19%～1.59%)、高MgO(5.51%～7.88%)、贫K2O(0.04%～0.84%)和P2O5(0.10%～0.20%)、Na2OK2O为特征;高场强元素(HFSE)丰度特征显示其为E-MORB型或过渡型玄武岩质岩石;稀土元素总量相对较高,轻重稀土元素分馏不显著[(La/Yb)N=1.93～3.61,LREE/HREE=3.01～4.10],在球粒陨石标准化配分模式图上呈略富集型.结合玄武岩构造环境判别图解综合分析推测,它们可能形成于一种裂谷向MORB环境过渡的构造环境,即初始小洋盆构造环境.     

Cyclotron amplification of geomagnetic micropulsations Pc1 in the magnetosphere

A numerical analysis of cyclotron instabilities is carried out by computing the dispersion relation for a three component cold plasma-beam system. Rates of growth and damping for various values of the stream density are calculated from the dispersion relation. The rates of growth and damping increase monotonically as the number density of the proton stream increases. It is found that the frequencies at the rates of maximum growth and the damping decrease slightly to lower frequencies and a sharp peak at these frequencies becomes blunt. The minimum e-folding times of an ion cyclotron wave for (a) σ_s = 10⁻⁴, σ_i = 10⁻² and (b) σ_s = 10⁻¹, σ_i = 10⁻² are about 3·84 and 0·16 sec respectively in the vicinity of the equatorial plane at 6 Re, where σ_s and σ_i are the ratios of the beam density N_s and the helium ion (H₆⁺) density N_i to the total positive ions in the plasma-beam system.     

Variations in exospheric density at heights near 1100km, derived from satellite orbits

In an earlier paper, values of exospheric density were obtained from the orbit of Echo 2 for the years 1964–1965. The results indicated a semi-annual variation in density by a factor of between 2 and 3, considerably larger than predicted by existing atmospheric models.

These studies have now been extended to the beginning of 1967, using both Echo 2 and Calsphere 1, to show how the density is responding to increasing solar activity. Variations in density during 1964 have been analysed in more detail. The long-term variation associated with the solar cycle and the short-term variations associated with magnetic and solar disturbances agree with the variations expected on the basis of current models. The semi-annual variation is persisting to higher levels of solar activity, and although its amplitude is diminishing the factor of variation was still 1.6 in 1966.