简单剪切——中国活动构造变形主要机制

采用简单剪切对中国活动的构造组合进行解译,提出简单剪切是主要变形机制,着重对简单剪切依据进行了论述,对简单剪切与老构造的关系作了初步讨论,提出需要继续探讨的主要问题。     

找出最主要的控矿因素,建立三因控矿分析思路

通过几个已知金矿区的研究,认为到不同矿区有不同的控矿因素,首先找出最主要的控矿因素,再配合两个深层相关因素,进行矿体定位。     

基于主成分分析的库存管理神经网络模型研究

从影响合理库存的诸多因素中,利用数理统计的思想,找出若干主要指标,通过建立神经网络模型,进行模拟仿真,寻求一种解决问题的有效方法,把库存调整到理想的状态。     

正弦激励下零浮力海洋拖缆动力特性与实验研究

海洋地震拖缆是海洋油气资源勘探中的关键设备,为研究海洋地震拖缆的动力特性及其在不同频率正弦激励干扰下的动力响应,建立了零浮力拖缆的数学模型,设计了一套完整的实验方案,通过弹性测力机构放大张力信号以排除环境干扰,测量了不同拖曳速度与激振频率条件下拖缆首部的张力变化及缆上位移响应情况,初步分析了正弦激励作用下零浮力拖缆的动力学响应。弹性测力机构具有良好的线性度与可重复性,拖缆受到的水阻力与拖曳速度的平方成正比,数值计算与实验结果对比验证了数学模型的正确性,初步分析了正弦激励作用下零浮力拖缆的动力学响应。     

商河县馆陶组热储地热尾水回灌可行性研究

从回灌热储层条件、动力场特征、水化学及库容条件等方面,研究了商河县地热回灌地质条件。结合区内地热资源开发利用现状与回灌工程技术条件,对商河县地热尾水回灌的可行性进行了研究,认为在现有条件下,可逐步推行地热尾水回灌。     

Chemical spots on the surface of the strongly magnetic Herbig Ae star HD 101412

Due to the knowledge of the rotation period and the presence of a rather strong surface magnetic field, the sharp‐lined young Herbig Ae star HD 101412 with a rotation period of 42 d has become one of the most well‐studied targets among the Herbig Ae stars. High‐resolution HARPS polarimetric spectra of HD 101412 were recently obtained on seven different epochs. Our study of the spectral variability over the part of the rotation cycle covered by HARPS observations reveals that the line profiles of the elements Mg, Si, Ca, Ti, Cr, Mn, Fe, and Sr are clearly variable while He exhibits variability that is opposite to the behaviour of the other elements studied. Since classical Ap stars usually show a relationship between the magnetic field geometry and the distribution of element spots, we used in our magnetic field measurements different line samples belonging to the three elements with the most numerous spectral lines, Ti, Cr, and Fe. Over the time interval covered by the available spectra, the longitudinal magnetic field changes sign from negative to positive polarity. The distribution of field values obtained using Ti, Cr, and Fe lines is, however, completely different compared to the magnetic field values determined in previous low‐resolution FORS 2 measurements, where hydrogen Balmer lines are the main contributors to the magnetic field measurements, indicating the presence of concentration of the studied iron‐peak elements in the region of the magnetic equator. Further, we discuss the potential role of contamination by the surrounding warm circumstellar matter in the appearance of Zeeman features obtained using Ti lines. (© 2016 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

Finding the most variable stars in the Orion Belt with the All Sky Automated Survey

We look for high‐amplitude variable young stars in the open clusters and associations of the Orion Belt. We use public data from the ASAS‐3 Photometric V ‐band Catalogue of the All Sky Automated Survey, infrared photometry from the 2MASS and IRAS catalogues, proper motions, and the Aladin sky atlas to obtain a list of the most variable stars in a survey area of side 5° centred on the bright star Alnilam (ε Ori) in the centre of the Orion Belt. We identify 32 highly variable stars, of which 16 had not been reported to vary before. They are mostly variable young stars and candidates (16) and background giants (8), but there are also field cataclysmic variables, contact binaries, and eclipsing binary candidates. Of the young stars, which typically are active Herbig Ae/Be and T Tauri stars with Hα emission and infrared flux excess, we discover four new variables and confirm the variability status of another two. Some of them belong to the well known σ Orionis cluster. Besides, six of the eight giants are new variables, and three are new periodic variables (© 2010 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)     

苏丹穆格莱德盆地福拉凹陷油气成藏特征及勘探启示

福拉凹陷下白垩统Abu Gabra组发育有湖相好—极好烃源岩,但热演化程度低、成藏主控因素不确定,勘探潜力不明。通过地层层序划分、构造分析、沉积相分析,认为张剪性区域构造背景控制福拉凹陷的构造与沉积发育,下白垩统Abu Gabra组发育有一定规模有效生烃凹陷,可形成Abu Gabra组烃源岩层,Abu Gabra组自储自盖,Bentiu组储、Aradeiba组盖及Aradeiba组自储自盖等3套生储盖组合,其中第二套储盖组合为该凹陷不同于六区其他凹陷的良好储盖组合。紧邻生烃凹陷、继承性发育的构造带,如中部滚动背斜—断鼻、南部次凹西缘断鼻、南部断阶带断鼻、北部次凹东缘断鼻等构造带是有利的成藏带。继承性发育的Fula1号滚动背斜、Fula2号断鼻构造具有多套储盖组合,勘探风险低,为有利的勘探目标。这些认识为福拉凹陷油气勘探提供了科学依据,且其研究方法及思路也为新区油气勘探提供良好的借鉴。     

利津县城区地热资源状况及开发前景分析

利津县城区的地热资源主要赋存于新生代新近纪和古近纪碎屑沉积岩中,热储类型为层状孔隙-裂隙型热储,地热资源类型属热传导型。新近纪馆陶组热储层组与古近纪东营组热储层组是主要的热储层。该文在论述利津县地热地质条件的基础上,对地热开发的经济、社会、环境效益及开发利用前景进行了分析,对地热开发中的尾水排放和回灌问题进行了探讨,最后提出了地热资源开发与管理方面的建议。     

四川盆地南部下三叠统飞仙关组一段台内鲕滩的主控因素

四川盆地飞仙关组台缘鲕滩气田的发现,激励了人们重新认识台内鲕滩的发育分布规律及其勘探前景。根据野外露头及钻孔资料的分析,认为四川盆地南部飞仙关组一段的台内鲕滩具有发育向上变浅序列、单滩体厚度一般小于3m、横向连续性较差的特征。着重分析了沉积期古地貌、古水深、海水动荡程度以及古海平面相对升降变化对台内鲕滩的控制作用,并把滩体的发育阶段分为雏滩期(低速建造期)、滩核期(高建造期)及衰亡期3个阶段。结果表明,在缓慢等效的海退过程中,处于高能沉积界面附近的水下古高地有利于台内鲕滩的形成,继承性的泸州古隆起核部是区内有利的滩体发育区,形成的台内滩体具有一定的厚度规模和较大的分布面积。这一认识可为该区飞仙关组台内鲕滩的下一步勘探提供必要的地质支持。