Prediction of Apparent Equivalent Thickness Using the Spontaneous Potential Method and Its Application to Oilfield Development

The upper spontaneous potential produced by oil and gas accumulation is of a stable potential field, and its intensity is directly proportional to the content of the source and inversely proportional to the radius apart from the source. Theoretical research and practical results show that anomalies of spontaneous potential can indicate oil-bearing sandstone bodies and locate the areas of oil and gas accumulation. In oil areas which have fewer reservoir beds, the petroleum reservoir thickness can be predicted by determining the linear relationship between potential intensity and apparent equivalent thickness. In the Weixing （卫星） oilfield, which is devoid of sufficient reservoir beds, its apparent equivalent thickness can be predicted by the linear equation h= -0.19x＋0.74. On the basis of geological research, we use the spontaneous potential method to predict the equivalent thickness, helping in the selection of the most appropriate drill sites to enhance the probability of successful well boring so as to serve the next round development of the oilfield.     

内蒙乌拉山金矿控矿条件及成矿作用

乌拉山金矿是华北地台北缘中西部地区近年来探明的有一定远景的金矿床。该矿床受大桦背岩体、韧性剪切带、脆性断裂构造和乌拉山群变质岩系等多种条件所控制，矿体呈脉状产出，成矿具有多期多阶段性，成矿时代较华北地台东缘金矿床早，为晚华力西期，其类型为中深成脉状金矿床     

敦密断裂带盆地群油页岩特征及成矿差异分析

古近纪敦密断裂带上分布一系列的含油页岩盆地群。根据盆地间构造-沉积充填、岩石组合和油页岩赋存特征,初步确认盆地群中油页岩沉积于湖盆鼎盛阶段,均形成于古近系始新统路特阶。盆地群间油页岩矿床特征存在明显的差别,由西南向东北,油页岩厚度逐渐变小,其沉积环境由深湖到半深湖,再到湖沼,而有机质来源则由湖泊生物为主,到湖泊生物和陆源有机质双向来源,过渡为以陆源高等植物为主。结合含油页岩层系形成于同一时期和相似的古气候背景下,盆地沉降和沉积充填作用是影响油页岩矿床差异的关键因素。长期处于欠补偿环境,可容纳空间大的湖盆利于巨厚油页岩的形成,随着可容纳空间的减少、陆源碎屑供给的增多,油页岩厚度减薄,分布也变得相对局限。深湖和湖沼成因油页岩品质较好,半深湖油页岩品质较差。     

西南印度洋中脊表层沉积物非碳酸盐组分的粒度特征及其地质意义

The carbonate-free fraction of 20 surface sediments collected from the ultraslow-spreading Southwest Indian Ridge(SWIR) was studied by grain size analysis and mineralogical analysis with X-ray powder diffraction(XRD),stereo microscopy and scanning electron microscopy(SEM). The characteristics of the carbonate-free fraction of the sediments were obtained, and related influential factors were discussed. The results show that the mean grain size of this fraction is in 1.96Φ–8.19Φ, with poorly sorting and unimodal, bimodal or irregular bimodal distribution patterns. Four grain size end members of the fraction are derived with the End Member Model method. The finest end member EM1 shows a significant contribution of terrigenous materials of the aeolian input and sediment carried by the bottom current. End member EM2 with medium size mainly reflects sediment of a siliceous bioclast origin. EM3 and EM4 are interpreted as representing the coarser volcanic materials related to bedrock weathering or volcanic activities. Multi-provenance is the dominant factor controlling the grain size pattern of the carbonate-free fraction of the sediments in that area. In addition, sediment transport processes such as the bottom current and wind are the minor factors that influence the grain size distribution of the carbonate-free fraction sediments.     

New Early Cretaceous paleomagnetic results from Qilian orogenic belt and its tectonic implications

Lower Cretaceous red sedimentary rocks from the depositional basin of East Qilian fold belt have been collected for a paleomagnetic study. Stepwise thermal demagnetization reveals two or three components of magnetization from dark red sandstones. Low-temperature magnetic component is consistent with the present Earth Field direction in geographic coordinates. High-temperature magnetic components are mainly carried by hematite. The mean pole of 19 sites for high-temperature magnetic components after tilt-correction is λ=62.2°N, φ=193.4°E, A95=3.2°, and it passes fold tests at 99% confidence level and reversal tests at 95% confidence level. The paleopole is insignificantly different from that of Halim et al. (1998) from the same sampling area at the 95% confidence level. Compared with paleomagnetic results for North China, South China, and Eurasia, our results suggest that no significant relative latitudinal displacement has taken place between Lanzhou region and these blocks since Cretaceous time. Remarkably, the pole of Lanzhou shows a 20° clockwise rotation with respect to those of North China, South China, and Eurasia. Geological information indicates that the crustal shortening in the western part of Qilian is greater than that in eastern part. In this case, the clockwise rotation of sampling area was related to India/Eurasia collision, and this collision resulted in a left-lateral strike-slip motion of the Altun fault in north Tibetan Plateau after the Cretaceous.     

面向地震应急的山区人口百米格网分布——以麟游县为例

破坏性地震发生后,山区易发生滑坡、泥石流等地质灾害。精细化人口空间分布数据能够有效提升灾情评判精度,为应急救援决策提供参考依据。本文以陕西省麟游县为例,利用"天地图"高分辨率遥感影像解译大比例尺居民地数据,结合人口、行政区划等数据,利用GIS（地理信息系统）技术制作100 m×100 m格网人口分布数据。通过与陕西省地震局现有人口空间数据进行对比,发现百米格网人口分布数据可明显提升山区次生灾害影响人口计算结果的可靠性。     

CIMISS中气象观测资料处理入库效率优化方法

气象资料种类多、海量、格式多样复杂,造成综合气象信息共享系统(CIMISS)巨大的处理压力。以高空L波段数据作为个例,进行详细的分析,在数据库表设计上,通过"键-要素"的拆分方式减少数据库冗余,建立合理的索引和分区提高数据表访问效率。在处理流程方面,通过简约化流程减少系统间消息交互和IO,从而优化系统的存储效率。同时简约流程中对比PRO*C和OCI两种入库方式,PRO*C简单高效便于开发,而OCI功能全面但相对复杂,通过比较两种入库方式的效率,系统采用PRO*C方式。高空L波段数据实际运行效果表明,平均28s完成一份数据的处理。对比高空探测数据的处理,简约流程比原流程入库更快。     

The global joule heat production rate and the AE index

The accuracy of the AE index as a measure of the joule heat production rate is examined for a typical substorm event on 18 March 1978 by estimating the global joule heat production rate, as a function of time, using data obtained from the IMS six meridian chains. In spite of the fact that the AE index had had an initial slow growth which was followed by a rapid growth, the joule heat production rate attained a high level during the slow growth and thus their variations were considerably different from those of the AE index. Therefore, although the AE index is statistically linearly related to the global joule heat production rate, one should be cautious in assuming that details of time variations of the AE index during individual events represent those of the joule heat production rate.     

轴对称稳恒磁场的一种解法

本文依据稳恒磁场中的高斯定理和安培环路定理，用迭代法推导出对称轴上的磁感应强度与空间任意一点磁感应强度的关系式，从而可得出轴对称稳恒磁场的无电流分布空间的解式。     

利用自回归模型检测地球极移重力效应

同时采用4个台站的国际超导重力仪长期连续重力观测资料和国际地球自转服务中心提供的同步地球自转参数，研究了极移引起的地球重力场变化特征。利用自回归模型估计了各序列的功率谱密度和积谱密度，结果表明极移导致的重力效应的主要能量集中在Chandler摆动和周年项附近，叠积后实际重力观测与极移重力信号理论值之间的差异分别为0．4％和3．9％，说明超导重力仪可有效监测极移导致的重力变化。