邹平火山岩盆地铜多金属成矿对构造岩浆事件的响应

通过邹平火山岩盆地不同岩石类型岩石化学特征的对比分析:认为火山活动总的趋势是由弱到强,爆发指数为38—68—92;火山岩3个亚组SI值均<40,表明母岩浆可能是由幔源岩浆经分异演化或同化而形成的;侵入岩σ介于2.39～4.99,属钙碱性-碱性岩系;DI为65.15～88.98,岩浆分异演化程度相对较高;A/NKC为0.96～1.02,岩石为弱过铝质。该区岩浆岩属壳幔型中性岩—壳幔型和铝质地壳过渡区中酸性岩—酸性岩的岩浆岩区。铜多金属对构造-岩浆事件的响应可描述为:长期继承性活动的区域性构造和振荡性的岩浆侵入活动,致使富碱质岩浆热液与已结晶的二长质岩石在地球化学界面发生交代蚀变,并进行了物质交换。     

雁荡山破火山口构造特征及成岩物质来源

雁荡山破火山口构造以其独特的火山地貌形态，完美的环状断裂和环状圈层分布的岩相，环形展市的航磁异常和地球化学异常，显示出一个地质─地球物理、地球化学、岩相─构造配置较完整的典型破火山口模式，依壳、幔二元混合模拟计算．火山岩和侵入岩源区物质组成为UC56.2DM43．8和UC56．4DM43．6，两者来自相似源区．源区处于地壳下部。     

新疆金山沟巴塔玛依内山组火山岩及地球化学特征

早石炭世巴塔玛依内山组为一套陆相火山岩,下部以基性熔岩为主,上部以中酸性、酸性火山碎屑岩为主.岩石地球化学研究表明,区内火山岩呈高铝玄武岩-安山岩-英安岩-流纹岩钙碱性系列的演化趋势.从基性岩到酸性岩稀土模式相似,但铕负异常愈加明显.火山活动与金银矿成矿关系密切,玄武岩类、火山碎屑岩类Au、Ag、As含量较高,可能是成矿物源.     

地壳中的应力场及一些诱震因素

把地球考虑为在径向上由ｎ层具有不同物理—力学性质的物质所组成的球体，由此出发，推导了计算地壳中由地球自重、匀速自转、天体引力、地球自转速度变化所产生的位移场和应力场的公式。对由地壳和地幔以下物质所组成的二层体情形进行了详细推演，数值计算表明：作为诱震因素，天体引力特别是月亮对地球的引力似乎比地球自转速度变化所起的作用更大     

Recognition and Significance of Volcanic Rocks of the Anda Depression of the Songliao Basin in Jurassic-Cretaceous

A series of volcanic rocks were developed in the deep part of Anda faulting depression. The reflection of therocks are mainly stratiform and hummocky. Three kinds of volcanic facies, e.g. explosion facies, effusion facies andsub-volcanic facies,were recognized by different reflecting characteristics in the seismic profile. The volcanic rocks areformed during three episodes of volcanic activities from Shahezi Formation to Yingcheng Formation. The volcanismshave relation to the formation of Songliao Basin and regional tectonics of northeastern China. Some of the volcanic rocksare good oil and gas reservoirs.     

FRAME DESIGN OF REMOTE SENSING MONITORING FOR VOLCANIC ACTIVITIES IN CHANGBAI MOUNTAINS

Volcanic eruption is one of the most serious geological disasters, however, a host of facts have proven that the Changbai Mountains volcano is a modem dormant one and has ever erupted disastrously. With the rapid development of remote sensing technology, space monitoring of volcanic activities has already become possible, particularly in the application of thermal infrared remote sensing. The paper, through the detailed analysis of geothermal anomaly factors such as heat radiation, heat conduction and convection, depicts the monitoring principles by which volcano activities would be monitored efficiently and effectively. Reasons for abrupt geothermal anomaly are mainly analyzed, and transmission mechanism of geothermal anomaly in the volcanic regions is explained. Also, a variety of noises disturbing the transmission of normal geothermal anomaly are presented. Finally, some clues are given based on discussing thermal infrared remote sensing monitoring mechanism toward the volcanic areas.     

中国及邻区地震的天文潮汐触发特征研究——附加潮汐应力对发震断层的作用模式及其应用

本文在潮汐应力、构造应力、地震断层和岩石破裂滑动理论的基础上 ,建立了潮汐应力对地震断层作用的力学模式 ,该模式将潮汐应力与地震应力作用相结合 ,描述了沿地震主压应力和地震主张应力方向的附加潮汐应力对发震断层的力学作用方式 ,从而切入潮汐应力触发地震的物理机制 ,认为潮汐对地震的触发作用在实质上归结为潮汐应力对地震断层的促滑作用 ,这种促滑作用分增压型和减压型。在此模式基础上 ,对中国大陆及邻区的不同类型地震的潮汐触发性进行了研究 ,内容包括 :计算了中国及邻区一千多个地震震源处沿主压应力P轴和主张应力T轴方向的附加潮汐应力分量 ,分析了这些量对发震断层的作用方式 ,按纬度区域统计了受到潮汐应力促滑作用的发震断层类型以及它们与潮汐应力作用方式的关系 ,得到了如下结论 :受到潮汐应力促滑作用的发震断层的比例随区域纬度增加有减小趋势 ,其中 ,走滑型断层的比例在低纬区较大 ,而倾滑斜型断层的比例在中高纬度区较大 ;对整个统计区域而言 ,受增压型潮汐应力促滑作用的发震断层数比例大于受减压型潮汐应力促滑作用的发震断层 ;对不同的纬度区域 ,不同的潮汐应力作用方式与之促滑的发震断层类型也有不同的分布特征。最后 ,本文将中国及邻区受到潮汐触发作用的地震按构造应力     

ε_（Nd）－La／Nb、Ba／Nb、Nb／Th图对地幔不均一性研究的意义──岛弧火山岩分类及EMII端元的分解

本文提出一组εＮｄ－Ｌａ／Ｎｂ、εＮｄ－Ｂａ／Ｎｂ和εＮｄ－Ｎｂ／Ｔｈ图。在这些图中岛弧火山岩呈三角形分布，从而将其源区的三个主要端元（ＭＯＲＢ型亏损地幔、俯冲洋壳析出流体、陆源沉积物）同时显示在一张图上。据此，岛弧火山岩可根据其源区特征划分成两类：二端元型（无陆源沉积物）和三端元型。此外，ＥＭＩＩ型幔源岩石在这些图中也被分成两类：与岛弧火山岩类似的，具有高Ｌａ／Ｎｂ、Ｂａ／Ｎｂ和低Ｎｂ／Ｔｈ的大陆溢流玄武岩和某些橄榄岩包体；具有低Ｌａ／Ｎｂ、Ｂａ／Ｎｂ和高Ｎｂ／Ｔｈ的萨莫德型海岛玄武岩。它们对应的ＥＭＩＩ富集地幔端元也可分为两种：ＥＭＩＩＭ，由俯冲洋壳析出流体交代楔型地幔而成；ＥＭＩＩＳＲ，与陆源沉积物再循环进入对流上地幔有关。     

Volcanic hazard assessment incorporating expert knowledge: Application to the yucca mountain region, Nevada, USA

Multiple-expert hazard/risk assessments have considerable precedent, particularly in the Yucca Mountain site characterization studies. A certain amount of expert knowledge is needed to interpret the geological data used in a probabilistic data analysis. As may be the situation in science, experts disagree on crucial points. Consequently, lack of consensus in some studies is a sure outcome. In this paper, we present a Bayesian approach to statistical modeling in volcanic hazard assessment for the Yucca Mountain site. Specifically, we show that the expert opinion on the site disruption parameterp is incorporated into the prior distribution, π(p), based on geological information that is available. Moreover, π(p) can combine all available geological information motivated by conflicting but realistic arguments (e.g., simulation, cluster analysis, structural control, ..., etc.). The incorporated uncertainties about the probability of repository disruptionp eventually will be averaged out by taking the expectation over π(p). We use the following priors in the analysis: (1) priors selected for mathematical convenience: Beta (r,s) for (r,s) = (2, 2), (3, 3), (5, 5), (2, 1),(2, 8), (8, 2), and (1, 1);and (2) three priors motivated by expert knowledge. Sensitivity analysis is performed for each prior distribution. Our study concludes that estimated values of hazard based on the priors selected for mathematical simplicity are uniformly higher than those obtained based on the priors motivated by expert knowledge. And, the model using the prior, Beta (8, 2), yields the highest hazard (=2.97 × 10^-2 . The minimum hazard is produced by the “three-expert prior” (i.e., values of p are equally likely for p = 10^-3, 10^-2,and 10^-1 . The estimate of the hazard is 1.39 × 10^-3, which is only about one order of magnitude smaller than the maximum value. The term, “hazard, ” is defined as the probability of at least one disruption of a repository at the Yucca Mountain site by basaltic volcanism for the next 10,000 years.     

2个二次触发型太阳耀斑的射电时间轮廓及其日冕磁结构

利用国家天文台(北京和昆明)的射电频谱仪(频段为0.65~7.6 GHz)和相关的NoRH/17GHz射电以及TRACE/171 EUV和Yohkoh/SXT的观测资料,分析了2001/04/10和10/19的2个共生精细时间结构的稀有事件,这2个事件的射电爆发时间轮廓和观测特征相似,通过这2个事件的微波(17GHz)偏振观测资料的比较,发现这2个射电爆发均由包含多重(4极)磁结构的复杂活动区引起,特别指出这2个耀斑最后都导致了耀斑后相的分米波射电爆发(第二次触发耀斑),这可能是后环引起的射电爆发。它们都分别对应于双极磁位形,表明这两次触发耀斑是由相似的耀斑模型产生。2个分米波爆发可能是相似(homologous)耀斑的射电表现,可以推测这两次耀斑的驱动器可能皆是磁流浮现或对消(因为源区有新的单或双极出现或消失),而它们的触发器皆是由双极反向Y型位形(具有一个双极拱的单磁流系统)的磁重联,耀斑后环的演化是导致耀斑后相分米波射电爆发的必要条件。我们认为,这双带耀斑对应的宽带射电爆发辐射机制是回旋同步加速辐射过程,而耀斑后相的窄带分米波爆发的辐射机制是等离子体辐射过程。