轮南油田原油中三甲基苯基类异戊烯化合物的检出及其意义

轮南油田不同时代储层原油中检出了丰富的三甲基苯基类异戊二烯化合物.该类化合物被普遍认为是来自于高盐度和强还原水体沉积环境中绿硫菌体内的类胡萝卜素的特征性生物标志化合物.该类化合物的检出对轮南油田烃源岩研究具有重要的指示意义,暗示了具有分层水体或高盐度的强还原环境下发育的优势烃源岩,对该区烃类的主力生烃贡献不容忽视.基于C15- 3,4,5-三甲基苯基类异戊二烯异构体在轮南油田原油中的分布规律,及C15-3,4,5/C13-2,3,6比值与Pr/Ph,Ga/C31H和Ts/Tm等常规地球化学参数的对比,说明具有生源意义、能够指示沉积相特征的三甲基苯基类异戊二烯化合物分布,在一定程度上也受烃类热演化程度的影响.     

An X-Ray Study of Lobe-Dominated Radio-Loud Quasars with XMM-Newton

We report on our results of X-ray spectral analysis for a sample of radio-loud quasars covering a wide range of the radio core-dominance parameter, R, from core-dominated to lobe-dominated objects, using data obtained mostly with the XMM-Newton Observatory. We find that the spectral shape of the underlying power-law continuum is flat even for the lobe-dominated objects (average photon index ～ 1.5), indistinguishable from that of core-dominated quasars. For lobe-dominated objects, contribution of X-rays from the jets is expected to be very small based on previous unification schemes, more than one order of magnitude lower than the observed X-ray luminosities. Assuming that radio-loud quasars follow the same X-ray-UV/optical luminosity relation for the disk-corona emission as found for radio-quiet quasars, we estimate the X-ray flux contributed by the disk-corona component from the optical/UV continuum. We find that neither the luminosity, nor the spectral shape, of the disk-corona X-ray emission can account for the bulk of the observed X-ray properties. Thus in lobe-dominated quasars, either the disk-corona X-ray emission is much enhanced in strength and flatter in spectral shape (photon index～1.5) compared to normal radio-quiet quasars, or their jet X-ray emission is much enhanced compared to their weak radio core-jet emission. If the latter is the case, our result may imply that the jet emission in X-rays is less Doppler beamed than that in the radio. As a demonstrating example, we test this hypothesis by using a specific model in which the X-ray jet has a larger opening angle than the radio jet.     

High Spatial Resolution X-Ray Spectroscopy of Cas A with Chandra

We present high spatial resolution X-ray spectroscopy of the supernova remnant Cassiopeia A with the Chandra observations. The X-ray emitting region of this remnant was divided into 38 × 34 pixels of 10″× 10″ each. Spectra of 960 pixels were created and fitted with an absorbed two component non-equilibrium ionization model. From the results of the spectral analysis we obtained maps of absorbing column density, temperatures, ionization ages, and the abundances of Ne, Mg, Si, S, Ca and Fe. The Si, S and possibly Ca abundance maps show obvious jet structures, while Fe does not follow the jet but seems to be distributed perpendicular to it. The abundances of Si, S and Ca show tight correlations between one another over a range of about two dex. This suggests that they are ejecta from explosive Oburning and incomplete Si-buming. Meanwhile, the Ne abundance is well correlated with that of Mg, indicating them to be the ashes of explosive C/Ne burning. The Fe abundance is positively correlated with that of Si when the latter is lower than 3 times the solar value, and is negatively correlated when higher. We suggest that such a two phase correlation is due to the different ways in which Fe was synthesized.     

射电选和X射线选BL Lacertae天体的射电性质

收集了射电选和X射线选BL Lac天体的射电数据(包括核和延展光度), 并计算了它们的核主导系数R.研究显示: 射电选BL Lac(RBLs)天体的总射电光度是X射线选BL Lac(XBLs)天体的2个量级.详细分析得到这种差别主要是来自于核光度的差别因为延展光度差别只有1个量级.研究RBLs和XBLs的核(延展元)光度与核主导系数之间的关系, 发现延展元光度与核主导系数负相关, 而核(总)光度几乎与核主导系数没有相关.     

网格GIS及其在数字油田中的应用探讨

数字油田是解决当前油田智能化管理问题的最好途径。该文分析了当前油田建设中所面临的问题,结合油田在勘探开发中的实际需要,特别就当前数字油田建设中所面临的共性问题,在分析现有油田技术及发展需求的基础上,指出了基于中间件的分布式网格GIS技术是解决当前数字油田领域中所存在的问题的最佳方式,并讨论了其实现过程。     

春风油田石炭系火山岩油气层综合判识研究

火山岩油气藏是一种特殊类型油气藏,受岩性、岩相、储集空间类型等因素影响较大。常规测井仅能对储层进行评价,录井仅能对岩性及油气显示进行评价。利用测录井资料无法快速判识油气层现状,制约了现场完井方式及试油方案的及时决策,并影响钻井周期、成本及对区块的潜力评价。通过岩心描述、镜下薄片储集空间及含油性观察,结合测井解释和试油结果,总结了春风油田石炭系火山岩油藏岩石类型及含油性特征;火山岩储集空间类型、影响因素、识别方法及物性有效性;孔隙、裂缝等储集空间有效性电性识别方法;建立了春风油田石炭系油气层综合判识准则。本次研究可快速对该区石炭系完钻探井进行油气层综合判识,指导现场完井方式决策,提高勘探效益。     

低渗透储层地质状况分析及提高采收率的方法研究——评《低渗透油田开发技术》

近年来,我国在低渗透油气田勘探开发中取得重大突破,以塔里木油田和长庆油田为典型代表。低渗透油气藏是指采用常规开发技术无法实现经济有效开发,必须是采用特殊工艺技术开发的的油气藏,不同岩性都可形成低渗储层,以致密砂岩、碳酸盐岩最发育。《低渗透油田开发技术》一书,从地质、钻井、油藏、采油及地面工程等方面,讲述了低渗透油气田地质特征、面临的难题和采取的技术方法,对不同开发技术进行了实例论证,为进一步提高我国低渗透油气藏开发水平提供技术支持。本书专业性、逻辑性和实用性较强,对低渗透油气田开发具重要指导作用。     

基于正演模拟的复合曲流带砂体内部构型解剖研究及应用

Q油田是渤海大型河流相沉积的稠油油田,其北区NmⅣ1主力含油砂体为复合曲流带沉积,经过16年的注水开发,油水关系复杂,平面注水受效不均的问题日益严重,如何优化注釆结构来改善开发效果已成为急需解决的问题。优化现有注釆井网的关键是认识复合曲流带砂体内部不同单河道砂体的切叠关系及展布特征,即对目标砂体开展内部不同单河道的构型单元分布特征研究。首先,依据岩电标定的测井曲线特征、局部发育的薄夹层以及曲流河纵向下切模式,对复合砂体内部不同单河道砂进行划分与对比;然后基于单井沉积微相划分结果,开展井间剖面相对比分析,表明复合砂体内部存在5种不同单河道砂体切叠模式;建立5种正演概念模型,利用地震正演模拟合成地震记录,总结了不同单河道砂体间顶面高程差异、点坝边界、废弃河道等曲流河砂体构型边界的波形特征;利用地震属性提取及多种地质构型方法,综合分析,最终实现了海上大井距条件下复合曲流带砂体内部不同单一曲流河砂体构型边界的精细识别;最后由注采动态资料的响应关系评估不同的切叠模式对注水效果的侧向遮挡程度,并以此为依据,优化现有的注釆井网并取得了非常好的生产效果。     

临南油田夏32断块沙二段下部储层特征及其主控因素

通过岩芯和薄片观察,结合测井资料,对临南油田夏32断块沙二段下部储层发育特征及其主控因素进行了研究。结果表明：该区储层的岩石类型主要为岩屑质长石砂岩和长石质岩屑砂岩,颗粒分选中等,磨圆较差,成分成熟度及结构成熟度中等;储层物性表现为中低孔特低—低渗的特征,且孔隙度和渗透率相关性较好;孔隙类型包括原生粒间孔、粒内溶孔、粒间溶孔和铸模孔。综合储层特征的研究结果认为：夏32断块沙二段下部储层主要受基准面旋回、沉积、成岩以及构造作用的影响;三角洲平原的分支河道砂体物性最好,其次是三角洲前缘的水下分支河道,其他沉积微相储层物性较差;压实作用和胶结作用破坏储层物性,溶蚀作用则可改善储层物性;此外,构造作用所产生的裂隙也有利于改善储层物性,对储层物性起到了积极的建设作用。     

X荧光光谱分析技术在测定安徽月山矿床铁铜矿石中Fe、Cu的应用研究

为建立符合安徽月山矿区的X荧光光谱(XRF)分析方法,针对矿区铁矿、铜矿的特点,用铁、铜矿石的国家标准物质制作系列校准样片,通过粉末压片和玻璃熔融两种制样方法,波长色散X荧光光谱法测定主矿体样品中的Fe、Cu等主量元素,并将测定结果与传统化学方法分析结果进行比较。结果显示,熔片法-XRF的测定结果与化学容量法测定结果一致,试样在850℃灼烧,按40∶1大稀释比熔融制样,解决了样品在高温熔融过程中对铂黄坩埚的腐蚀,适用于月山矿区铁铜矿样品中Fe、Cu的测定。粉末压片法不能克服矿物效应和粒度效应的影响,测定结果与化学容量法结果比对偏差较大,不适用于月山地区铁铜矿中Fe、Cu的测定。