瑞利波法检验客运专线湿陷性黄土地基处理效果

黄土地基具有明显的湿陷性,试验采用3种方法(柱锤冲扩桩、挤密桩、强夯)进行处理.测试得到地基在3种方案处理前后的瞬态瑞利波频散曲线,比较处理前后的瑞利波波速分布图,反演分析地基剪切波速度,得到黄土地基处理后的波速变化特性.结果表明,经3种方案处理后的黄土地基弹性波波速均得到了提高,波速增大幅度从大到小分别为柱锤冲扩桩、挤密桩和强夯,与静力触探法对比结果较为一致,表明瞬态瑞利波测试方法能大面积无损测试地基处理效果.     

超声提取-固相萃取小柱净化-气相色谱法测定土壤中14种有机氯农药

对土壤中14种有机氯农药的超声提取技术和磺化、固相萃取小柱两种净化方法进行系统研究。结果表明,超声提取节省提取时间,提高分析效率;磺化法和固相萃取小柱法都有净化作用,但磺化法使样品中的艾氏剂、狄氏剂和异狄氏剂全部损失;固相萃取小柱净化当丙酮-正己烷淋洗液体积比为1∶9、淋洗液收集8 mL时回收率>90%,干扰最小。方法检出限为0.63~2.59μg/kg,精密度(RSD,n=7)为1.17%~14.66%,基体加标平均回收率为82.78%~106.94%。方法用于生态地球化学调查评价批量土壤样品的实际分析,检测结果满足评价工作需要。     

长江三角洲南翼晚更新世——全新世沉积物地球物理研究

利用蕴涵着丰富的地球物理信息的波速测试成果 ,对长江三角洲南翼晚更新世—全新世沉积物作沉积过程及其沉积环境讨论     

跑马岗组时代涉及的若干重大问题

湖北当阳新店—跑马岗剖面的跑马岗组跨白垩系与古近系 ,所含轮藻、介形类化石的丰富程度极为罕见。跑马岗组的时代问题与白垩系 -古近系界线及其陆相辅助层型的建立、印度德干玄武岩沉积夹层的时代、印度与亚洲大陆联合的时代和白垩系 -古近系界线事件起因假说等数个重大地学问题 ,以及江汉盆地深层油气资源评价密切相关 ,值得重视 ,尽早搞清     

正交矩阵的若干性质

通过对正交矩阵的深入研究，得到正交矩阵的一系列常用性质。     

川西上三叠统须家河组超致密砂岩储层评价

川西须家河组超致密砂岩中发育多种储层类型,天然气产出能力各异。针对须家河组超致密砂岩整体孔渗关系差,以孔隙度为基础、单定量孔渗关系模型评价精度低的特点,以微观孔隙结构与储集物性关系深入分析为基础,建立了以渗透率为基础,利用与多种储集类型相配置的孔渗多定量关系模型,分别确定了不同储集类型的不同下限,提高了超致密砂岩储层的评价水平。     

东昆仑西段黑山构造蛇绿岩带特征

通过对黑山构造蛇绿岩中基性火山岩、基-超基性岩的岩石组合及其岩石学、岩石化学、微量元素、稀土元素等特征研究认为:黑山构造蛇绿岩带是祁漫塔格结合带重要物质组分,是在加里东晚期板块俯冲-碰撞过程中逐渐演化形成的,区域上与那棱格勒构造带相连,是柴达木陆块与东昆北陆块的分界断裂。通过同位素地质年龄研究认为该蛇绿岩形成于南华—奥陶纪,构造就位于志留纪—早中泥盆世。对东昆仑构造演化提供了重要新资料。指出黑山构造蛇绿岩以北的祁漫塔格地区(柴达木陆块)发育与岩浆岩、变质岩有关的铜、钨、钛、铁等与热液、区域变质有关的内生矿产;以南的库木库里盆地发育砂砾岩型铜矿、砂金、石膏和石盐等外生矿产。     

Contributors to chromium isotope variation of meteorites

We report the results of a comprehensive, high precision survey of the Cr isotopic compositions of primitive chondrites, along with some differentiated meteorites. To ensure complete dissolution of our samples, they were first fused with lithium borate-tetraborate at 1050-1000 °C. Relative to the NIST Cr standard SRM 3112a, carbonaceous chondrites exhibit excesses in ⁵⁴Cr/⁵²Cr from 0.4 to 1.6ε (1ε = 1 part in 10,000), and ordinary chondrites display a common ⁵⁴Cr/⁵²Cr deficit of ∼0.4ε. Analyses of acid-digestion residues of chondrites show that carbonaceous and ordinary chondrites share a common ⁵⁴Cr-enriched carrier, which is characterized by a large excess in ⁵⁴Cr/⁵²Cr (up to 200ε) associated with a very small deficit in ⁵³Cr/⁵²Cr (<2ε). We did not find ⁵⁴Cr anomalies in either bulk enstatite chondrites or in leachates of their acid-digestion residues. This either requires that the enstatite chondrite parent bodies did not incorporate the ⁵⁴Cr anomaly carrier phase during their accretion, or the phase was destroyed by parent body metamorphism. Chromium in the terrestrial rocks and lunar samples analyzed here show no deviation from the NIST SRM 3112a Cr standard. The eucrite and Martian meteorites studied exhibit small deficits in ⁵⁴Cr/⁵²Cr. The ⁵⁴Cr/⁵²Cr variations among different meteorite classes suggest that there was a spatial and/or temporal heterogeneity in the distribution of a ⁵⁴Cr-rich component in the inner Solar System.We confirm the correlated excesses in ⁵⁴Cr/⁵²Cr and ⁵³Cr/⁵²Cr for bulk carbonaceous chondrites, but the new data yield a steeper slope (∼6.6) than that reported in Shukolyukov and Lugmair (2006). The correlated excesses may affect the use of the Mn-Cr chronometer in carbonaceous chondrites. We could not confirm the bulk carbonaceous chondrite Mn-Cr isochron reported by Shukolyukov and Lugmair (2006) and Moynier et al. (2007), mostly because we find much smaller total variations in ε⁵³Cr (∼0.2). All bulk chondrites have small ε⁵³Cr excesses (up to 0.3) relative to the Earth, most likely reflecting the sub-chondritic Mn/Cr ratio of the Earth. The ε⁵³Cr variations in chondrites do seem to grossly correlate with Mn/Cr and yield an initial Solar System ⁵³Mn/⁵⁵Mn value of 5.4(±2.4) × 10⁻⁶, corresponding to an absolute age of 4566.4 (±2.2) Ma.Nuclear interactions with cosmic rays result in coupled excesses in ε⁵⁴Cr and ε⁵³Cr with a ∼4:1 ratio in phases with high Fe/Cr. These are most dramatically demonstrated in the iron meteorite Carbo, showing excesses in ε⁵⁴Cr of up to 140ε. These new results show that the Mn-Cr chronometer should be used with caution in samples/minerals with high Fe/Cr and long cosmic ray exposure ages.     

利用功率谱直接求埋深的影响因素

功率谱方法在磁数据处理方面的应用比较广泛。采用近似公式直接求出地质体的上下底埋深。在此近似方法中,会出现一些影响结果的因素。主要对地质体的水平尺寸和厚度的影响做了一些研究,并得出相应的结论。     

星际A型CH_3CH－H_2含超精细能级的碰撞跃迁速率系数的理论计算

本文作者利用ＩＯＳ近似模型，计算了星际分子云条件下Ａ型ＣＨ３ＣＮ－Ｈ２含超精细能级的碰撞跃迁速率系数。温度范围是２０Ｋ－１４０Ｋ。为研究分子云与恒星形成区的物理、化学性质提供了有用的基础分子数据。