The Origin of the Element Eu in Extremely Metal-poor Halo Stars

The fast neutron capture process (the r-process) occurs in the neutron-rich circumstance. However its concrete physical environment is not very clear. With recent progress in observations, many extremely metal-poor halo stars have been discovered. They have two characteristics: one is the overabundance of fast neutron elements with the relative abundance consistent with that of the sun; the other is that fast neutron element contents in stars at the same metal abundance have a very large dispersion. This provides a particular way to study the origin of the r-process. Simulation was used to study the galaxy's evolution process and the resulting dispersion of fast neutron nuclide contents in stars. The model of galaxy evolution obtained in this way not only contains spontaneous star formation in the gas region, but also includes the star formation excited by the supernova explosion. It is shown from our results that the supernovae at the low mass end should be the place producing the fast neutron nuclides. In addition, it is also shown that the non-uniformity of the galaxy evolution caused by the supernova explosion is not enough to explain the observed dispersion of fast neutron element contents in halo stars. This problem should be further studied.     

A Study on the Light Curves of GRBs

It is generally believed that the complexity and variability of the light curves of gamma-ray bursts (GRBs) are caused by the internal shocks, which would occur when a rapid shell catches up a slower one and collides with it. The electrons in the shock layer are heated by the shocks and radiate via the mechanisms of synchrotron radiation and inverse Compton scattering. Based on relativistic kinematics, a relation between the photon number of the emission from the rapidly moving shock layer and the number of the photons received by an observer is derived. Then, employing the angular spreading of the internal shock emission, the curve equation and profile of a single pulse are obtained, and the shape is typically in the shape of a fast rise and exponential decline. Furthermore, by using the model of the successive collisions of multiple shells under the condition of reasonable parameters, the observed light curves are fitted with a rather good effect. Therefore, by this means, more different types of light curves of GRBs can be explained.     

云南剑川金河岩体中地幔流体交代特征及其成矿意义

云南剑川金河岩体中的硅化霓辉正长斑岩含有较多的镁铁-超镁铁质深源岩石包体.岩相学研究表明,伴随交代蚀变,其主岩和各类包体岩石中普遍发育沿矿物粒间和矿物晶体裂隙或解离纹贯入或穿插的呈网状和细脉浸染状分布的黑色不透明物质.对该物质进行了电子探针及扫描电镜和能谱分析,发现其组成以微晶硅酸盐矿物为主,含少量微晶石英,尤其是含有微晶地幔标型矿物--含钛磁铁矿(或镜铁矿)和含铬自然铁;后两者与硅酸盐矿物构成超显微熔离结构交生.研究认为,这种物质组成和特征,是具超临界和熔浆性质的地幔流体的微观表现,其活动所引发的交代蚀变表现为硅化、钠化及深源包体中的暗色矿物由辉石→角闪石→黑云母的退变序列.这一地幔流体作用微观踪迹的揭示,对于分析和论证滇西地区新生代多金属成矿的深部地质作用规律具有重要的理论和现实意义.     

准噶尔盆地天然气成藏体系和成藏过程分析

准噶尔盆地目前已发现的天然气以中—小型的中浅层晚期次生气藏为主。研究表明,以区域盖层上三叠统白碱滩组泥岩为界可划分为下部近源原生天然气成藏体系和上部远源次生天然气成藏体系,前者一般具有异常高压的特征,后者则具有正常的压力系统。通过对盆地东部地区、腹部地区、西北缘地区、莫索湾凸起天然气成藏过程的解剖获得了比较一致的认识,即上部次生天然气是在下部原生天然气的改造和调整的基础上形成的,下部天然气成藏体系的原生大—中型天然气藏是未来准噶尔盆地天然气的勘探方向。值得注意的是南缘冲断带的上部成藏体系既有源自侏罗系煤系烃源岩的原生天然气聚集,又伴随有次生天然气藏的形成。     

贵州后槽铝土矿古岩溶地貌控矿作用及找矿意义

后槽铝土矿区位于黔中遵义铝土矿带中部,受NE向岩溶盆地控制,发育众多形态各异的中、小型的溶洼、溶坑和溶沟,在这些溶蚀洼地中,沉积了下石炭统九架炉组含铝岩系.文章通过对后槽地区354个钻探工程揭露的含铝岩系厚度、矿体厚度及化学成分的系统统计分析,研究了该区岩溶古地貌特征及其控矿作用,并进行找矿靶区预测.研究结果表明,后槽...     

同构造沉积分析反演逆冲构造变形过程--燕山东段凌源南部中生代逆冲构造变形过程研究

介绍了同构造沉积分析的基本概念、研究思路、主要研究方法及其在区域构造变形过程研究中的重要作用。基于对辽西凌源南部区域构造变形、晚侏罗世土城子组同构造沉积粗碎屑沉积物成分变化规律的研究 ,获得如下主要认识 :( 1)同构造沉积始于髫髻山组火山活动之后 ;沉积物成分变化及古水动力特征表明 ,同构造沉积物源区主体位于盆地西侧褶皱隆起区 ,而不是来自南东方向的大型逆冲断层上盘的前渊沉积 ;而且显示了正常层序的物源区倾斜岩层的剥蚀和揭顶过程 ;当时的剥蚀作用已达中元古界蓟县系雾迷山组上部。 ( 2 )分布于郭家店盆地和邓杖子盆地之间的中元古界长城系地层“残片” ,与其东侧北票组间为向SEE逆冲的断层接触 ,而西侧与土城子组 (原邓杖子组 )之间为不整合接触 ;在老虎沟东南长城系地层“残片”不复存在的区域 ,土城子组不整合于北票组之上。该“残片”很可能是髫髻山组火山活动之前指向SEE的逆冲构造变形形成的飞来峰构造的残余部分。( 3 )凌源南部中生代逆冲构造变形可以区分为 :早侏罗世北票组之前 (印支期 )由北向南的逆冲作用、北票组之后髫髻山组之前向SEE的冲断推覆、髫髻山组之后的逆冲褶皱变形与同构造沉积作用以及九佛堂组之后局部的逆冲作用。指向SEE的主要逆冲作用以及伴生褶皱变形     

Genesis of the Xinqiao Gold-Sulfide Orefield, Anhui Province, China

The Xinqiao S-Fe-Cu-Au orefield is located in the Tongling ore cluster in the middle and lower reaches of the Yangtze River in East China. There have been many researches regarding the genesis of the Xinqiao orefield in recent years, showing that it belongs to various types, such as sedimentary-reformed type, stratabound-skarn type, sedimentary submarine rocks-hosted exhalative type. We propose that it was formed in two periods of mineralization base on systematic field observation and Pb and S isotopic analyses in nearly ten years. The first period was formed during a syngenetic sedimentary process, whereas the massive sulphide orebodies are mainly related to the Yanshanian granitic magmatism. Sulfide metallic mineral associations show zoning around a granite intrusion, i.e. magnetite and pyrite→pyrite, chalcopyrite and native gold→pyrite, sphalerite and galena. Gold orebodies occur outside the contact zone of the granite intrusion.     

Solar Type III Bursts and the Generation of Backward Langmuir Wave

It is generally believed that the conversion of Langmuir wave (LW) to electromagnetic wave is the generating mechanism of solar type III bursts. The Langmuir wave can be easily excited by the instability of the electron-beam current, and the interaction of the forward and backward Langmuir waves is considered to be the cause for the second harmonic of a type III burst, but, so far, the dispersion equation and generating mechanism of the backward Langmuir wave have not yet been thoroughly studied. For the equation of two-stream instability with temperature included, an analytical solution is derived. It is found that the dispersion relation of the forward LW strongly depends on the beam-current speed, while that of the backward LW depends only on the thermal velocity, when the other parameters are fixed. These analytical results are partially confirmed by particle-in-cell (PIC) simulations. With the PIC simulation, the generating mechanism of the backward LW is studied, and it is revealed that the backward LW can not be excited directly by the electron-beam current, and that its energy is obtained basically from the scattering of the forward LW. However, the electron-beam current does cause a direct amplification of the second harmonic of the forward LW.     

黑河下游额济纳绿洲现代荒漠化过程及其驱动机制

额济纳绿洲是发育在黑河下游内陆河三角洲上著名的天然绿洲。20世纪50年代以来,额济纳绿洲现代荒漠化过程加剧,绿洲萎缩,生态恶化。绿洲现代荒漠化过程是由水环境恶化过程、土壤干燥化过程、植被退化与生物多样性衰减过程、土地沙漠化过程和土壤盐碱化过程构成的地表动力学过程。导致额济纳绿洲荒漠化的驱动力是区域气候暖干化、强盛的风蚀侵蚀力、上中游过度开发水土资源的人为活动和额济纳绿洲内的“三滥”活动等。荒漠化驱动力的第一主成分与第二主成分的贡献率分别为59．276％和28．083％,反映出绿洲荒漠化驱动因子的多面性和综合性,绿洲内外过度的人为活动是其主导驱动因素。内在、外在驱动力在时间与空间上的耦合性是绿洲荒漠化的区域机制,驱动力因子团的互动-激发作用形成荒漠化的动力机制,驱动力与荒漠化土地间的响应形成正反馈机制,三种作用机制组合成绿洲现代荒漠化过程的复杂的驱动机制。     

疏勒河上游径流组分及其变化特征定量模拟

气候变化背景下,西北干旱区内陆河流域的水文过程发生显著变化,制约着地区经济社会和生态建设的稳定发展。定量分析和评估高寒山区径流的变化,有助于加强西北地区水资源的规划管理,实现水资源的可持续利用,保障区域水安全。选取位于青藏高原东北边缘、祁连山西段的疏勒河上游作为研究区,利用包含冰雪消融模块的寒区水文模型分布式SPHY模型（Spatial Processes inHydrology model）对流域的径流过程进行定量模拟,根据模拟结果分析了疏勒河上游近45 a径流组成及径流与各组分的变化特征。结果表明：（1）率定期日径流和月径流模拟的Nash效率系数分别为0.62和0.86,验证期达到0.79和0.95,模拟的月径流与实测月径流过程基本一致;（2）径流由四部分组成,冰川径流占总径流的年平均比例为30.5%,融雪径流的占比为12.9%,降雨径流的占比为13.5%,基流的占比为43.1%;（3）由于气温升高、降水增多,冰川径流与降雨径流均呈增加的趋势,平均增加幅度分别为4.66×10⁶ m³·a^-1和2.46×10⁶ m³·a^-1,融雪径流呈减少的趋势,平均减少幅度为1.01×10⁶ m³·a^-1;（4）近45 a年径流增加了69.6%,冰川融水对流域径流增加的贡献率达到48%,非冰川区降水增加的贡献率达到52%。