The Discovery of Retene in Precambrian and Lower Paleozoic Marine Formations     

姜乃煌  诸长鼎等 《中国地球化学学报》1995,14(1):41-51

Microscopic and SEM observations of thin sections and kerogens and GC-MS analyses of aromatic fractions in sediment extracts and pyrolysis products of kerogens provide strong evidence suggesting that in the Lower Yangtze Valley area the Sinian and Lower Paleozoic carbonate formations of marine facies received no higher plant input,but there was produced abundant retene during diagenesis and abietic acid substances are still its precursors.  相似文献   

Expert system for earthquake prediction on personal computer (ESEP/PC)     

Kunyuan Zhuang  Wei Wang  Bingshu Huang  Shihua Xia 《地震学报(英文版)》1992,5(4):883-886

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Uncertainty in sewer sediment deposit modelling: Detailed vs simplified modelling approaches     

《Physics and Chemistry of the Earth》2012

The paper presents the results of a study in which the uncertainty levels associated with a detailed and a simplified/parsimonious sewer sediment modelling approach have been compared. The detailed approach used an Infoworks CS sewer network model combined with a user developed sediment transport code and the simplified approach used a conceptual sewer flow and quality model. The two approaches have been applied to a single case study sewer network and the simulation results compared. The case study was selected as moderate storm events had occurred during a 2 year rainfall and sewer flow monitoring period. Flooding had been observed and this was thought to be caused by significant solids accumulation in the sewer network. As a result sediment deposit measurements were carried out over a 6 month period. Model simulations were made of this period and predictions obtained of sediment deposit location and depth. The uncertainty analysis of both modelling approaches was carried out using Monte Carlo based computational methods. This was a limitation for the detailed approach with regards to computational time. Use of the simplified model was not constrained by this issue and so a more conventional assessment of the uncertainty was possible. The simplified approach, due to its structure, only provided a temporal estimate of uncertainty at the final section of the catchment. The detailed approach enabled an assessment of uncertainty at an individual pipe scale but only at the end of the simulation period. A comparison of the uncertainty estimations from both methods at the final section of the catchment and the end of the simulation period indicated comparable values of predicted uncertainty. Therefore a complementary use of both approaches would allow reasonably comparable estimations of levels of uncertainty at both a spatial and temporal scale. The use of such modelling approaches may provide a useful decision-making tool for sewer system management.  相似文献   

2013年1月安徽持续性霾天气成因分析   总被引：10，自引：3，他引：7  

石春娥  邓学良  杨元建  吴必文  孟燕军 《气候与环境研究》2014,19(2):227-236

2013年1月安徽霾天气具有范围广、持续时间长、能见度低等特点。利用合肥、安庆、阜阳2009~2013年1月地面常规资料、高分辨率探空资料,结合轨迹分析和聚类分析,讨论了2013年1月安徽霾天气频发的原因。结果表明:低风速、高湿度不能解释2013年1月霾天气增多、增强的现象。大气层结稳定、接地逆温偏多、偏厚,可部分解释这次霾天气增多现象。边界层中上部输送条件的变化也不能解释2013年1月霾天气增多现象,但近地层输送条件的变化能较好地解释2013年1月霾天气增多现象,如偏东北来向的轨迹组对应着最低的能见度,且2013年1月各地最低能见度对应的轨迹组所占比例(或与次低能见度的轨迹组所占比例之和)在历年中最高。因此,大气层结稳定、近地层偏东北来向气团较多是2013年1月安徽各地能见度偏低、霾天气偏多的主要原因。  相似文献   

利用磁场空间特征对井中磁三分量的有效解释及前景瞻望     

战双庆  刘冬节 《安徽地质》2009,19(3):190-193

目前三分量解释一般采用矢量图解释,由于仪器不能定向,此种方法解释会出现错误结论,本文采用磁异常场垂直分量及水平分量的空间分布特来对磁异常进行解释,能有效地解决井底及井旁磁性体的体赋存情况,在见矿时能确定磁性矿体的主体方向及产状。  相似文献   

一种地电观测的配套软件(DDPT)   总被引：1，自引：0，他引：1  

李治华  汪贵章 《地震地磁观测与研究》2005,26(5):130-131

引言 合肥地震台的地电观测,使用ZD8B数字地电仪实现了自动测量和PC计算机数据采集。但还有许多经常用到的计算结果（如日均值、五日均值、月均值、均方差及其许多图件等）需要我们利用计算机进行计算或绘制,以代替目前的手工操作。另外,地震台的地电观测结果需要抄写记录本和录入月报表,由于原始记录纸带的资料排列格式与报表、记录本的排列格式差别很大,抄录时费工费时又容易出错。为了减少台站工作人员的工作量,降低错情率,便于计算机进行数据格式处理和编写月报表,我们利用Visual BASIC开发工具,自主研制了一套更符合我们实际情况的地电观测配套软件（DDPT）。该软件适用于Windows95／98系统的操作平台,界面友好,操作简便,在合肥台使用已取得良好的效果,并已通过安徽省地震局有关部门验收。  相似文献   

蒙城地震台地电阻率数字化与模拟观测资料的对比分析   总被引：1，自引：0，他引：1  

薛志明  胡连芝  李伟  汪继林  李雪华 《华北地震科学》2005,23(4):31-35

通过对蒙城地震台地电阻率数字化和模拟的标定资料、地电阻率观测数据、资料的年周期变化、以及数、模观测系统的系统差别等几个方面进行对比分析,为蒙城台多年的模拟与数字化资料综合使用以及数字化仪器替代模拟仪器观测提供依据.  相似文献   

赣南新林屋—均村地区低磁性隐伏岩体的识别:来自重磁场的证据          下载免费PDF全文

朱将波  汪启年  张健  葛诚 《华东地质》2019,(2):108-113

通过在赣南新林屋—均村地区开展1∶5万高精度磁法测量工作,结合1∶20万重力测量数据,以岩石物性为基础,分析该区重磁异常并圈定隐伏花岗岩体。新林屋—均村地区低磁性、低密度的花岗岩侵入至具有磁性的前寒武纪变质岩中,形成磁低重低的异常特征;推断新林屋—均村地区存在1个呈NW向展布的隐伏花岗岩体,该隐伏花岗岩体浅部受SN—NE向弧状断裂控制,深部受NW向断裂控制,浅部分布范围较深部更广。这些信息为该区进一步找矿提供了基础地球物理资料,也为同类地区寻找隐伏花岗岩体提供参考。  相似文献   

Wave dynamics of super cloud clusters over the tropical region     

《Dynamics of Atmospheres and Oceans》2001,33(2):79-94

A wave dynamics for the super cloud clusters associated with the tropical intraseasonal oscillation is constructed. Under the present framework, the basic state of super cloud clusters is considered to be a large-scale convergence of the zonal wind. This convergence is created by a nonlinear diabatic Kelvin wave front, which moves eastward slowly without change of shape. When interacting with free equatorial waves with n=−1, 0, 1 and 2, this basic flow will suppress those waves which move eastward except for free Kelvin waves, and permit westward propagating modes such as the mixed Rossby-gravity wave, the inertio-gravity waves with n=1 and 2 to appear in the large-scale convergent region. Among these waves, only fast modes, that is, inertio-gravity waves with n=1 and 2 are regarded to be responsible for the presence of cloud clusters which move westward within a super cloud cluster, while the multiplicity of the occurrences of super cloud clusters, which move eastward within the large-scale convergent region, is due to the superposition of free Kelvin wave upon these inertio-gravity waves.  相似文献   

Palaeohydrodynamics of fluids in the Brent Group (Oseberg Field,Norwegian North Sea) from chemical and isotopic compositions of formation waters     

《Applied Geochemistry》2001,16(6):609-632

Generally, the history of past sub-surface fluid movements is difficult to reconstruct. However, the composition of oil-field waters characterizes the origins and mixing processes that allow such a reconstruction. We have investigated present-day formation waters from Brent Group sedimentary rocks of the Oseberg Field in order to assess both their geochemical variations, and their origin(s). Water samples (sampled at the separator) produced from immediately above the oil–water contact and from the aquifer (water-saturated zone below the oil–water contact) were taken from 11 wells across the field. In addition, 3 trace water samples were extracted from oil produced from higher up in the oil column. The water samples were analysed for their chemical components and isotopic compositions. Conservative tracers such as Cl, Br, δD, and δ¹⁸O were used to evaluate the origin of the waters. All formation waters can be characterised as Na–Cl-brines. The separator samples are of aquifer origin, indicating that aquifer water, drawn up by the pressure reduction near the well, is produced from the lower few tens of metres of the oil-zone. By defining plausible endmembers, the waters can be described as mixtures of seawater (60–90%), meteoric water (10–30%), evaporated seawater (primary brines) (3–5%), and possibly waters which have dissolved evaporites (secondary brines). Alternatively, using multidimensional scaling, the waters can be described as mixtures of only 3 endmembers without presupposing their compositions. In fact, they are seawater, very dilute brine, and a secondary brine (confirming the power of this approach). Meteoric water was introduced into the reservoir during the end-Brent and early-Cretaceous periods of emergence and erosion, and partially replaced the marine pore fluids. Lateral chemical variations across the Oseberg Field are extremely small. The waters from closer to the erosion surfaces show slightly stronger meteoric water isotopic signatures. The primary and secondary brines are believed to come from Permian and Triassic evaporitic rocks in the deeply buried Viking Graben to the west, and to have been modified by water–rock interactions along their migration path. These primary basinal brines have not been detected in the oil–zone waters, suggesting that the brines entered the reservoir after the main phase of oil-migration. There are indications that these external fluids were introduced into the reservoir along faults. Present-day aquifer waters are mixtures of waters from different origins and hardly vary at a field-scale. They are different in composition to the water trapped in the present oil-zone. One of the oil-zone samples is a very dilute brine. It is thought to represent a simple mixture of seawater and meteoric water. Due to oil-emplacement, this geochemical signature was preserved in the waters trapped within the oil-zone. Another oil-zone water shows a very similar chemical signature to the aquifer waters, but the chlorine isotopic signature is similar to that of the dilute oil-zone water. This water is interpreted to represent a palaeo-aquifer water. That is, it was within the aquifer zone in the past, but was trapped by subsequent emplacement of more oil. These vertical differences can be explained by two features: (i) emergence of the Brent Group sedimentary rocks in the Early Cretaceous allowed ingress of meteoric water; (ii) subsequent rapid burial of Viking Graben rocks caused migration of petroleum and aqueous fluids into the adjacent, less deeply buried Oseberg Field.  相似文献