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。     

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)     

平湖油气田主断裂西部烃源评价及油源对比

平湖油气田主力含油气区位于平湖主断裂以东区域,油源主要来源于东部生烃凹陷的半封闭海湾暗色泥岩和煤层.公司于2011年11月在主断裂西部钻了一口探井XY井,目的是为探测主断裂西部含油气情况,扩大油气储量.结果钻遇油气层12m,测试获日产气14.66×104m3,日产油107.8 m3,取得了一定突破.为进一步评价西部含油气规模,钻后进行了油源对比研究,认为西部的油气主要是东部运移聚集的结果,西部源岩也有一定贡献.西部有形成一定规模油气藏的潜力.     

四川中坝气田雷口坡组成藏条件及油气主控因素

通过对四川盆地西北部中坝气田中三叠统雷口坡组气藏已发现油气与有利沉积相带、局部构造、等关系的分析,结合试采试油资料与储层厚度、物性与录井显示关系的统计分析,总结认为油气成藏发育了多套烃源岩,具有良好的储集条件和保存条件。通过对各个构造运动阶段雷口坡气藏被改造与再形成的分析,提出油气主控因素是后期构造运动的影响,主要经历了印支期、燕山期和喜山期构造运动的改造形成的古圈闭,油气藏受到破坏然后再形成的整个过程。该主识对中坝气田未来的勘探开发具有指导意义。     

陕北延安“7.3暴雨”诱发地质灾害主要类型与特征

2013年7月3日以来,陕西延安地区百年不遇的持续性强降雨,引发了大量的崩塌、滑坡、泥流地质灾害,造成严重的财产损失和人员伤亡。通过野外实地调查,对本次持续性强降雨诱发大范围地质灾害的主要类型和特征进行了较为系统的研究。研究表明,本次持续性强降雨引发的地质灾害共计8 000余处,灾害类型主要有崩塌、滑坡和泥流,分别以小规模黄土崩塌、浅表层黄土滑坡、坡面型黄土泥流为主,以及上述灾种链生转化形成的沟谷型泥流。在持续降雨条件下,多灾种转化而成的复合型灾害是造成人员伤亡和财产损失的主要类型。     

Accumulation and risk assessment of heavy metals in dust in main living areas of Guiyang City,Southwest China

Guiyang is a famous tourist city located in southwestern China. In this study, dust from eleven residential areas, seven city squares, and nine schools was collected to measure the heavy metal levels and evaluate its risk. At each sampling site, 4-5 sub-samples were taken as a bulk sample. All samples were air-dried, ground, passed through a 0.105 mm nylon sieve, digested with HNO3-HC104 to determine the concentrations of Cd, Cu, Ni, Pb and Zn by ICP-MS, and digested with 1：1 aqua regia to determine As by AFS. The results show that the concentrations of As, Cd, Cu, Ni, Pb and Zn in dust of Guiyang City follow normal distribution with means of 16.1, 1.54, 138, 47.7, 129 and 479 mg/kg, respectively. Levels of As, Cd, Cu, Ni, Pb and Zn exceed the background level of soil in Guizhou Province by 33%, 96%, 100%, 78%, 96%, and 100%, respectively. Cd, Cu, Pb and Zn are heavily accumu- lated in dust of living areas with accumulation factors of 4.10, 5.12, 4.12 and 5.51, respectively. City square pos- sesses the highest geometric means of As, Cd, Cu, Pb, and Zn. The risks of heavy metal exposure to teenagers are not obvious and in an order ofAs〉Pb〉Cu〉Ni〉Zn （Cd）.     

1993年7月湖北咸宁4.1级地震序列的活动特征

1993年 7月底至 8月中旬在咸宁发生的ML4 .1震群是一比较典型的有感震群 ,通过多种测震手段对该震群进行分析和处理 ,得到下列认识和结果 :1、该震群是一个非前兆震群。 2、此震群是一个主震型震群 ,地震主要发生在两个阶段 ,每个阶段均出现密集 -平静过程。 3、该震群可能与NE向潜山断裂的活动有关。 4、对咸宁震群的各种测震学参数计算表明 ,有一些参数在湖北省比较适用 (如b ,η ,U ,K ,ρ等 ) ,而有些则不适合 (如h ,F 等 )。     

基于GIS技术的莱州湾东岸河流分形研究

应用地理信息系统(GIS)技术提取了莱州湾东岸河流信息,在此基础上运用计盒方法对莱州湾东岸的黄水河和王河水系进行了分形分析,获得了两水系的主河道河长分维数和河网分维数,并以此探讨了分维数与流域地貌和地质构造之间的相互关系。分形分析为研究区流域地貌学与水文学研究提供了一种新的研究途经。     

川东北元坝西部须家河组二段优质储层展布特征研究

川东北元坝地区须家河组二段致密砂岩气资源潜力巨大,但储量探明率低、测试效果差异大,主要原因之一是致密砂岩储层非均质性强、优质储层分布规律不清。本文充分利用测录井、岩心及相关分析化验等资料,在分砂组刻画沉积微相展布的基础上,开展了须二段沉积演化过程、储层特征及其分布研究。结果表明：（1）元坝西部须二段经历了辫状河三角洲-滨浅湖-辫状河三角洲演化过程,沉积控制了砂体规模、粒度和矿物成分的空间变化;（2）须二段砂岩类型多样,整体致密,为低孔、低渗储层;储层物性与砂岩粒度,长石、石英和方解石胶结物含量等因素密切相关,这些因素主要受沉积和后期成岩作用控制;（3）须二段发育块状中粒长石岩屑砂岩和交错层理中粒石英砂岩两类有利岩石相,前者自西北向东南逐渐减薄、呈条带状展布,后者呈不连续土豆状,主体分布于西南部地区。