Infrared spectral evolution of carbon stars

We collected almost all Highly Processed Data Products(HPDP)of ISO SWS01 spectra for the Galactic visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich proto-planetary nebulae(PPNs).Those infrared spectra are primarily analyzed and discussed.It is shown that either spectral shapes/peaks,or main molecular/dust features are evidenced to change in the sequence of visual carbon stars,infrared carbon stars,extreme carbon stars and carbon-rich PPNs.Statistically,in this sequence,continua are gradually changed from blue to red and locations of spectral peaks of continua are also gradually changed from short wavelengths to long wavelengths.In addition,in this sequence,intensifies of main molecular/dust features are also gradually changed from prominent in the short wavelengths to prominent in the long wavelengths.Furthermore,from 2MASS and IRAS photometric data,the sequence is also proved.Results in this paper strongly support the previous suggestion for the evolution sequence of carbon-rich objects in our Galaxy,that is the sequence of visual carbon stars→infrared carbon stars→extreme carbon stars→carbon-rich PPNs.     

Scientific Objectives of China-Russia Joint Mars Exploration Program YH-1

Compared with other planets, Mars is a planet most similar with the earth and most possible to find the extraterrestrial life on it, and therefore especially concerned about by human beings. In recent years, some countries have launched Mars probes and announced their manned Mars exploration programs. China has become the fifth country in the world to launch independently artificial satellites, and the third country able to carry out an independent manned space program. However, China is just at the beginning of deep space explorations. In 2007, China and Russia signed an agreement on a joint Mars exploration program by sending a Chinese micro-satellite Yinghuo-1 (YH-1) to the Mars orbit. Once YH-1 enters its orbit, it will carry out its own exploration, as well as the joint exploration with the Russian Phobos-Grunt probe. This paper summarizes the scientific background and objectives of YH-1 and describes briefly its payloads for realizing these scientific objectives. In addition, the main exploration tasks of YH-1 and a preliminary prospect on its exploration results are also given.     

湘赣边界鹿井铀矿床流体包裹体及成矿机制

位于南岭成矿带南西部的鹿井矿床是华南热液型铀矿的典型代表.为查明其成矿流体来源、性质与演化以及成矿机制,开展了不同成矿阶段石英、萤石及方解石中流体包裹体的显微测温和不同阶段石英的氢?氧同位素分析.矿床地质特征表明成矿过程可划分为(I)粗晶石英+黄铁矿±绿泥石±绢云母、(II)沥青铀矿+硫化物+绿泥石+绢云母+暗灰色微晶...     

降雨量与闽西北地区地质灾害关系初探

通过对闽西北某地区2010年"6.13"特大强降雨下产生地质灾害的频数及程度分析对比,探讨降雨量与形成地质灾害的影响。分析结果表明,降雨的强度和时间对地质灾害的形成有重要的影响,对以后地质灾害预报预警有一定的指导意义。     

水平定向钻进铺管孔／管直径比设计取值方法

孔／管直径比是水平定向钻进铺管工程的重要基础设计参数,其取值大小直接关系到工程的成败、效率、安全和铺设后的管道运行安全。采用力学分析方法建立的回拖阻力数值模型及开发的专用软件,可以方便快捷地对孔管直径比取值进行精确的量化评价,并能够较好地解决工程设计中的一些复杂的数值计算问题,具有良好的推广应用前景。     

玄武质岩石的单颗粒锆石U-Pb年龄谱

报道了托云、东浮山、羊角、雪花山和山旺5处新生代玄武岩的SHRIMP锆石U-Pb测年结果。位于西南天山造山带的托云新生代玄武岩的14个测点年龄值十分发散,最大值与最小值分别为857.1和203.4Ma,它们与其余4件玄武岩样品49个SHRIMP锆石测点年龄一同构筑了涵盖各个地质时期几乎贯穿整个地质时间的复杂年龄谱。位于华北克拉通中部区域南太行山造山带的东浮山、羊角和雪花山新生代玄武岩3件样品累计36个锆石测点形成的锆石年龄谱相对简单,其中35个测点的年龄集中在1719.9～2641.6Ma,唯一的古生代年龄(311.3Ma)出现在雪花山玄武岩7.1测点。位于华北克拉通东部裂谷带内山旺玄武岩6件样品27个测点的单颗粒锆石年龄构筑的锆石年龄谱形成3个集中时间段,分别为新太古代—古元古代(2595.4～1852.2Ma)、古生代(385.8～271.1Ma)和中生代(109.4Ma)。3个年龄谱中大部分单颗粒锆石U-Pb年龄均能在各自所处区域内发现与之对应的岩浆-热事件,部分单颗粒锆石年龄可能暗示所在区域至今未发现的岩浆热事件,托云、东浮山-羊角-雪花山、山旺新生代玄武岩的复杂单颗粒锆石年龄谱再造了各自所处区域的地质演化史。3个锆石年龄谱的复杂程度与各自区域地表出露岩浆岩的规模和期次复杂程度相关,天山造山带内岩浆岩发育,托云玄武岩锆石年龄普最复杂,记录了天山造山带的演化,而华北克拉通中部区域南太行山造山带地表零星出露岩浆岩,东浮山-羊角-雪花山玄武岩的锆石年龄普最简单。处于后期遭受破坏改造的华北克拉通东部裂谷带内的山旺玄武岩的单颗粒锆石年龄谱,其复杂程度明显低于托云玄武岩的年龄谱,而又高于东浮山-羊角-雪花山玄武岩的年龄谱。鉴于玄武质岩浆同化混染围岩过程中能量消耗和地球化学印记以及玄武质岩浆上升的耗时限制,认为托云、东浮山、羊角、雪花山和山旺新生代玄武岩中具有复杂年龄信息的锆石捕掳晶不是玄武质岩浆在快速上升过程中从围岩中捕获的,而是在岩石圈拆沉过程中进入软流圈地幔中,随着具原生岩浆性质的玄武质岩浆喷发到达地表。     

运用STOMP数值模拟器进行多空介质中尿素水解以及方解石沉淀数值模拟

遍布于美国能源部所辖野外场地的地下放射性核素和痕量金属污染对美国能源部的长期监管职能提出了最严峻的挑战。目前较有前景的一个原地固化污染物方法是利用尿素酶催化尿素水解,进而推动方解石沉淀及与之共同沉淀。运用STOMP数值模拟器实施一系列反应性溶质数值模拟来研究系统中水流、运移、反应与反应导致的介质性质变化之间的紧密的非线性耦合,并在研究中系统性增加反应系统的复杂度和物理-化学的非均质性以考察模拟效果。通过调整反应速率表达式中尿素酶浓度和沉淀反应常数,对尿素水解和方解石沉淀速率进行了敏感度分析。结果显示:尿素水解速率是矿物沉淀总量的决定性因素,沉淀物的空间分布既取决于水解速率也取决于沉淀速率;在一维水流柱6个空隙体积的时间段模拟中,观察到了5%的最大空隙度减少;当二维模拟中考虑一个低渗透性包裹体时,被改变的流场重新对生成的沉淀组成物进行了分布,形成了扭曲的反应锋面。模拟结果也显示沉淀在低渗透性区域边界上形成,这说明位于这个区域里面的污染物可能被囊裹而从流线中被隔离起来。     

强烈气洗作用导致原油成分变化的定量计算:以库车坳陷天然气藏为例

库车坳陷以产天然气为主,同时产出少量原油和凝析油,油气充注不同步,普遍具有"油早气晚"的特点,晚期大量天然气的侵入,必然对早期聚集的油藏发生改造作用。对气藏中原油成分变化的定量计算和讨论,可为天然气的注入强度定量评价提供直接证据。未遭受气洗的原油,正构烷烃摩尔浓度的对数与相应的碳数呈线性关系,而气洗作用可使轻组分的正构烷烃最先溶解于干气中,并随着天然气继续向前运移,原始油藏中的轻组分正构烷烃大大减少。以此为理论基础,建立了正构烷烃损失的定量计算模型。结果表明克拉2构造原油正构烷烃损失程度最高,平均可达70%左右,大北构造带原油正构烷烃损失程度差异较大,与该地区断块发育有关。气洗作用导致原油正构烷烃减少,而金刚烷、多环芳烃等在天然气中溶解度较低的化合物得以浓缩富集,相对含量大大增加。轻芳烃含量也会随之而增加,原油芳香度增加,石蜡度降低。在模拟实验基础上对气洗程度进行了定量评价,初步估算表明,克拉2构造原油遭受的气洗作用最强,是其他构造带的2～5倍。     

Some Fundamental Issues in Dynamic Compression and Tension Tests of Rocks Using Split Hopkinson Pressure Bar

Accurate characterizations of rock strengths under higher loading rates are crucial in many rock engineering applications. The split Hopkinson pressure bar (SHPB) system has been used to quantify the dynamic compressive strength of rocks using the short cylindrical specimen and the dynamic tensile strength of rocks using the Brazilian disc (BD) specimen. However, SHPB is a standard tool that is suitable for metal testing; there are some fundamental issues that need to be carefully visited in applying SHPB to rock dynamic tests. This paper addresses several such critical issues, including the choice of slenderness ratio of the compressive specimen, the effect of friction between the sample and bars on the measured results of compressive strength, the necessity of dynamic force balance on the dynamic BD test, and the validity of using the standard BD equation in the data reduction. We show that with proper experimental designs that address these issues, the dynamic compressive strength and dynamic tensile strength of rocks measured using SHPB are valid and reliable.