海拉尔盆地火山碎屑岩的成岩作用

对来自海拉尔盆地40口井的白垩系火山碎屑岩样品显微镜观察与分析显示,火山碎屑岩的成岩作用具有特殊性,表现在熔结作用、脱玻化与重结晶作用、粘土矿物形成与转变和交代作用等方面。熔结作用可以区分出熔浆/熔岩熔结、浆屑熔结和热灰熔结三种类型。脱玻化与重结晶作用常常是交织在一起,流纹质玻璃物质经脱玻化,并进一步重结晶,常具有特殊的结构,呈现一种复杂的硅质胶结样式。粘土矿物形成与转变在成岩作用早期就开始了,如蒙脱石化。一些特征性矿物如浊沸石、绿泥石的出现也不代表变质作用的开始,而是特定成岩环境的产物。碳酸盐的交代-胶结和溶解在火山碎屑岩中普遍发育,使得原岩面貌发生了严重的改变。成岩作用的特征揭示海拉尔盆地火山碎屑岩的成分和结构演变,这在测井岩性解释和孔隙度预测上具有意义。     

煤层气井监控系统建设方案及其应用

在煤层气开发信息化建设的基础上,对煤层气井监控系统建设方案进行了全面总结。本方案结合韩城地区煤层气开发,研究形成了一套煤层气排采制度;提出了直井、水平井定量化排采与自动调控的主要技术参数和相关工艺流程。另外,在充分调研分析现有相关技术的基础上,研发出煤层气排采生产自动控制技术,包括远程排采信息采集技术、信息传输与通信技术、定量化分析方法、自动调控技术、配套软件和调控规范等。应用结果表明,煤层气井监控系统建设方案可满足国内煤层气井排采的需求。     

极干旱地区土壤与大气水分的相互影响

基于建立在莫高窟窟顶的密闭拱棚,通过监测棚内凝结水量和空气温湿度,对极干旱地区典型极干旱气候条件下土壤与大气水分的相互影响进行综合分析。棚内凝结水量和空气温湿度的监测结果表明,在热动力作用下存在地下水分向大气输送的过程,其原因主要是在温度作用下土壤结合水分的分解蒸发与土壤盐分的吸湿吸附的交替作用。这也是形成所谓“土壤凝结水分”与“土壤水分呼吸”的根源。当温度升高时,土壤结合水分分解蒸发“呼出”水分,当温度降低时土壤盐分吸湿吸附,“吸入”大气水分,形成土壤与大气不对称水分交流。称质量实验表明：土壤水分的变化与空气温度的变化完全对应;有深层水分支持的土壤吸收大气水分的能力相对较差。极干旱地区土壤与大气水分的相互影响研究结果能为莫高窟珍贵文物的保护提供参考。     

江淮地区梅雨的新定义及其气候特征

用Cressman客观分析方法得到我国1954～2005年0.5°×0.5°的逐日降水格点资料,并定义了一个新的江淮地区的 “广义梅雨评定标准”,研究了包括长江中下游地区和淮河流域地区的整个江淮地区（28°N～34°N,110°E～122°E）梅雨期降水的气候特征。结果表明:江淮梅雨有显著的年际和年代际变化特征,主要存在2～3年、6～8年、 12～15年和18～20年的周期变化,2～3年的显著周期主要集中在20世纪70年代末以后。江淮地区梅雨在1965年前后、70年代末～80年代初和90年代初发生了三次显著的气候跃变。最后,从季风气流的水汽输送和副热带高压及阻塞高压的稳定维持三个方面讨论了江淮梅雨丰梅年和弱梅年时大气环流的异常特征。     

一种提高大高差短基线精度的方法

提出采用半参数模型解算大高差短基线,削弱残余对流层误差的影响。算例表明,与常规最小二乘法相比,采用半参数模型处理基线能很好地分离GPS残余对流层误差,提高基线解算精度。     

Evidence for high‐temperature fractionation of lithium isotopes during differentiation of the Moon

Lithium isotope and abundance data are reported for Apollo 15 and 17 mare basalts and the LaPaz low‐Ti mare basalt meteorites, along with lithium isotope data for carbonaceous, ordinary, and enstatite chondrites, and chondrules from the Allende CV3 meteorite. Apollo 15 low‐Ti mare basalts have lower Li contents and lower δ⁷Li (3.8 ± 1.2‰; all uncertainties are 2 standard deviations) than Apollo 17 high‐Ti mare basalts (δ⁷Li = 5.2 ± 1.2‰), with evolved LaPaz mare basalts having high Li contents, but similar low δ⁷Li (3.7 ± 0.5‰) to Apollo 15 mare basalts. In low‐Ti mare basalt 15555, the highest concentrations of Li occur in late‐stage tridymite (>20 ppm) and plagioclase (11 ± 3 ppm), with olivine (6.1 ± 3.8 ppm), pyroxene (4.2 ± 1.6 ppm), and ilmenite (0.8 ± 0.7 ppm) having lower Li concentrations. Values of δ⁷Li in low‐ and high‐Ti mare basalt sources broadly correlate negatively with ¹⁸O/¹⁶O and positively with ⁵⁶Fe/⁵⁴Fe (low‐Ti: δ⁷Li ≤4‰; δ⁵⁶Fe ≤0.04‰; δ¹⁸O ≥5.7‰; high‐Ti: δ⁷Li >6‰; δ⁵⁶Fe >0.18‰; δ¹⁸O <5.4‰). Lithium does not appear to have acted as a volatile element during planetary formation, with subequal Li contents in mare basalts compared with terrestrial, martian, or vestan basaltic rocks. Observed Li isotopic fractionations in mare basalts can potentially be explained through large‐degree, high‐temperature igneous differentiation of their source regions. Progressive magma ocean crystallization led to enrichment in Li and δ⁷Li in late‐stage liquids, probably as a consequence of preferential retention of ⁷Li and Li in the melt relative to crystallizing solids. Lithium isotopic fractionation has not been observed during extensive differentiation in terrestrial magmatic systems and may only be recognizable during extensive planetary magmatic differentiation under volatile‐poor conditions, as expected for the lunar magma ocean. Our new analyses of chondrites show that they have δ⁷Li ranging between ?2.5‰ and 4‰. The higher δ⁷Li in planetary basalts than in the compilation of chondrites (2.1 ± 1.3‰) demonstrates that differentiated planetary basalts are, on average, isotopically heavier than most chondrites.     

Direct constraint on cosmic neutrino mass using observational Hubble parameter data

In order to explore the properties of cosmic neutrinos, i.e. sum of the neutrino mass(∑m_ν) and the effective number of neutrino species(N_(eff)), which affects the Hubble expansion rate H(z)and the power of observational Hubble parameter data(OHD) in constraining cosmological parameters under the ΛCDM model, we utilize OHD to constrain the properties of cosmic neutrinos and apply an accurate H(z) function with mνand Neff. First, we simulate new OHD beyond the existing 43 OHD. According to the predictions of measurements of H_0(the current H(z) value), baryon acoustic oscillations(BAO) peaks, Sandage-Loeb(SL) test and cosmic microwave background(CMB), we assume observational accuracy up to 2% and redshift 0 z ≤5. With simulated H(z) data obtained from the fiducial model, we constrain the parameters including mνand Neff. When all parameters are set free, mν 0.196 eV(95%) and N_(eff)= 2.984 ± 0.826(68%) are obtained, and when fixing Neff as the standard baseline 3.046, we attain ∑m_ν 0.240 eV(95%). These constrained results are much tighter than the ones obtained by the current OHD, which makes the prospect of OHD in constraining cosmological parameters more promising as its accuracy and quantity grow.     

扬子地块新元古代裂谷盆地莲沱组沉积分异及其物源分析

扬子地块莲沱组及相当地层单元的划分和对比,一直是我国南华系(即Cryogenian)研究关键难题之一.新元古代裂谷盆地开启早期,构造-沉积分异作用,同裂谷相变很大,使得盆地边缘区地层序列不完整.过分依赖岩石地层单元对比,历存分歧,典型的就是关于莲沱组与板溪群地层对比、时代归属以及莲沱组的沉积环境问题.本文通过对扬子地块...     

辽西建昌盆地义县组上部英安岩的40Ar/39Ar年龄及其地质意义

建昌盆地义县组可分为两部分：下部以巨厚的沉积层为主,自下而上称为要路沟层、罗家沟层,局部地区沉积层之下有中基性火山岩;上部（罗家沟层之上）为酸性、中酸性火山岩系夹沉积层.罗家沟层与义县-北票地区尖山沟（砖城子）层可进行生物地层学对比.对义县组上部的一件英安岩样品进行40Ar/39Ar年代学研究,获得年龄为120 Ma,应与义县地区义县组顶部火山岩（金刚山层之上）对比.建昌地区义县组顶、底均可与义县地区大致对比.     

云南地区房屋建筑的震害矩阵

自1992年4月23日云南孟连西中缅交界6.7、6.9级地震始,地震部门对云南地区的破坏性地震进行了现场灾害调查和经济损失评估。1992~2003年,云南地区共发生50次破坏性地震,积累了丰富的震害资料。本文根据云南地区的主要建筑结构,统计分析了50次地震不同烈度区的破坏比、损失比和震害指数,给出了房屋建筑的震害矩阵。