求解带容量约束车辆路径问题的离散布谷鸟算法     

向明尚  张强 《东北石油大学学报》2021,45(1):95-101

提出一种离散布谷鸟算法(DCA)求解带容量约束的车辆路径问题(Capacitated Vehicle Routing Problem).该算法采用轮盘赌机制增强初始解选择的随机性,对基本布谷鸟算法的莱维飞行操作中,使用2—opt法和exchange法进行位置更新;在寄生巢位置更新中,使用shift法和reverse法增强最优解的局部开发能力.选取augerat标准数据集测试算法,并比较BA、ACO、SA及PSO算法结果.实验结果表明:离散布谷鸟算法能够有效解决带容量约束车辆路径问题,有较强的寻优能力,求解质量优于其他4种对比算法.  相似文献   

基于转录组测序的方斑东风螺单核苷酸多态性位点挖掘及功能注释     

王菁  刘付柏  许尤厚  黄宝松  王忠良 《广东海洋大学学报》2021,(1)

【目次】了解方斑东风螺中响应LPS刺激的SNP位点及SNP所在基因SNP-Unigenes的功能。【方法】使用SOAPsnp软件分析不同时间条件下转录组数据中的SNP位点,使用GO、COG和KEGG数据库进行功能注释。【结果】转录组数据中共挖掘到673 782个SNP位点,分布在110 869条SNP-unigenes序列上。SNP类型分析表明,转换位点发生的频率远高于颠换位点,且6种单碱基变异类型中以A/G转换发生概率最大。有5866条SNP-unigenes富集到298个KEGG子集中,其中以"内吞作用"子集中富集的SNP-Unigenes最多,共富集182条。  相似文献   

山东新汶煤田太原组底部徐家庄灰岩的微体古生物组合及时代探讨          下载免费PDF全文

宋香锁  江泳  陈军  陈诚  刘凤臣 《山东国土资源》2021,37(1)

通过对山东新汶煤田太原组底部徐家庄灰岩发育的有孔虫动物群和牙形石动物群的分析,鉴定出虫筳类有孔虫化石6属14种,非虫筳有孔虫7属16种,牙形石6属10种,建立一个有孔虫组合:Fusulinella-Fusulina组合;一个牙形石组合:Idiognathodusmagnificus-Streptognathodusparvus组合,通过与华北地区的生物群对比分析,太原组底部徐家庄灰岩中的生物群时代为晚石炭世中晚期。  相似文献   

地震沉积学在河流-浅水三角洲沉积相研究中的应用: 以渤海海域蓬莱A构造区馆陶组为例          下载免费PDF全文

付鑫  杜晓峰  官大勇  李瑾  李晓辉 《地质科技通报》2021,40(3):96-108

庙西南凸起蓬莱A构造区馆陶组有良好油气发现,但储层厚度多小于5 m,难以被精确识别刻画。以薄层砂体为研究对象,综合地震、测井、钻井岩心、古生物等基础资料,明确研究区馆陶组沉积时期受北东向物源供给沉积,发育河流-浅水三角洲相。基于90°相位化处理确定砂体地震响应特征;分频解释处理判断相对等时地震同相轴,构建馆陶组高频层序地层格架（三级层序SQ1-3）,优选60Hz地震数据体进行地层切片划分;地层切片高精度沉积学解释揭示研究区馆陶组SQ1层序至SQ3层序依次发育河流-席状化浅水三角洲-朵叶状浅水三角洲-水下河道型浅水三角洲。其中SQ1层序中河道砂体以及SQ2-3层序中浅水三角洲前缘砂体皆为有利储层。此次研究丰富发展了渤海海域河流-浅水三角洲相中地震沉积学在砂体预测中的研究成果。   相似文献   

松辽盆地钱家店铀矿含铀岩系层序地层结构对铀成矿的约束          下载免费PDF全文

曹民强 《地质科技通报》2021,40(4):131-142

弄清楚砂岩型铀矿含铀岩系地层结构及其对铀成矿的制约作用,是准确认识铀成矿规律和成矿作用的基础。综合地震、测井、岩心及分析测试资料,对松辽盆地西南部钱家店铀矿床含铀岩系——姚家组层序地层结构进行了研究,在此基础上,探讨了地层结构与铀成矿的关系。研究发现,钱家店地区姚家组为一个完整的三级层序,姚家组底界面为区域不整合界面,底部主要发育泥砾岩、含泥砾砂岩等,姚家组顶界为平行不整合,顶部发育一套紫红色夹灰色泥岩,在姚家组内部识别出了初始湖泛面和最大湖泛面,将其划分为低位体系域、湖泊扩展体系域和高位体系域。低位体系域分布范围较小,厚度平均约40 m,呈北东狭长型分布;湖泊扩展体系域和高位体系域地层连续超覆,分布范围向西南扩展至八仙筒-开鲁一带,总体仍为北东走向,地层平均厚度在研究区分别约为85 m和75 m。层序地层结构对研究区姚家组铀成矿具有约束作用,垂向上,由下至上不同小层序组铀矿化逐渐减弱;平面上,不同体系域铀矿化分布特征不同,低位体系域铀矿化主要发育在钱Ⅳ块-钱Ⅴ一带,呈北东走向条带状分布,矿体呈似板状、透镜状;湖泊扩展体系域铀矿化在钱Ⅱ-钱Ⅳ-钱Ⅴ一带呈不规则弧形分布,矿体呈"似卷状",为典型的层间氧化带型铀矿化;高位体系域铀矿化主要发育在钱Ⅲ块以及南部零星分布,推测向南具有进一步找矿空间。研究结果可为研究区找矿提供依据,并为铀成矿模式及成矿过程研究提供基础。   相似文献   

北部湾盆地福山凹陷流沙港组致密油成藏条件及主控因素          下载免费PDF全文

秦秋寒  雷栋  宋效文  苏俊青  任桂媛  刘德生  马庆林  卢政环  郭浩  廖飞燕  时阳 《地质科技通报》2021,40(4):1-10

查明北部湾盆地福山凹陷流沙港组致密油成藏条件并分析其控制因素,对于进一步明确致密油分布、厘定有利探区具有重要的指导意义。基于地震、录井、测井、岩心及分析化验等资料的综合分析,对北部湾盆地福山凹陷流沙港组有效烃源岩、有利储层、源储匹配关系等进行了研究。结果表明,流沙港组在最大湖泛期于皇桐和白莲两次凹内形成优质烃源岩,具有有机质丰度高、热演化程度适中的特点,提供了致密油形成的物质基础;受多物源供给影响,致密砂岩深入两次凹内,具有源储叠置、分布广泛的特点,溶蚀孔隙与构造裂缝发育,有利于致密油的近源运移与富集;主要烃源岩进入生油高峰期时凹陷构造已基本定型,无大型断裂发育,相对稳定的构造条件有利于致密油形成和保存。因此,福山凹陷流沙港组具备致密油成藏的有利条件,致密油纵向上主要分布在流一下亚段和流二段,平面上主要分布在皇桐次凹和白莲次凹,其形成和分布主要受控于优质烃源岩展布、富溶蚀孔隙"甜点"储层分布及有利的源-储叠置组合。   相似文献   

湘中涟源凹陷下石炭统天鹅坪组页岩气成藏条件及主控因素          下载免费PDF全文

田巍  陈孝红  李旭兵  岳勇  李海  刘安 《地质科技通报》2021,40(5):54-63

下石炭统天鹅坪组页岩是湘中地区页岩气勘探的新层系。基于野外地质调查、页岩气钻井的样品采集和分析测试等对湘中涟源凹陷石炭系天鹅坪组泥页岩的发育特征、有机地球化学特征、储层特征和含气性等页岩气成藏地质条件进行了分析。结果表明:涟源凹陷石炭系天鹅坪组有机质丰度较高,w（TOC）分布在0.78%~2.84%之间,有机质类型以Ⅱ₁型为主,有机质成熟度R_o分布在1.48%~2.09%之间,处于高成熟演化阶段;泥页岩矿物成分以石英和黏土矿物为主,黏土矿物主要由伊蒙混层、伊利石和绿泥石组成;泥页岩有机质孔较发育,孔隙度平均为1.97%,渗透率平均为0.847×10-3 μm2,但大多小于0.1×10-3 μm2;湘新地4井天鹅坪组泥页岩含气量分布在1.64~4.29 m3/t,平均2.69 m3/t（不含残余气）。结合区域构造-沉积演化背景的分析表明,涟源凹陷下石炭统天鹅坪组页岩气成藏条件的主控因素为沉积环境、构造保存条件,其中深水陆棚相是页岩气有利相带,复杂构造背景下由对冲式构造样式形成的向斜对页岩气保存条件最为有利,是研究区页岩气勘探的"甜点区"。研究成果可以为该区后续油气勘探提供参考。   相似文献   

Transient accelerating scalar models with exponential potentials     

Wen-Ping Cui  Yang Zhang  Zheng-Wen Fu 《天文和天体物理学研究(英文版)》2013,(6):629-634

We study a known class of scalar dark energy models in which the potential has an exponential term and the current accelerating era is transient. We find that, although a decelerating era will return in the future, when extrapolating the model back to earlier stages (z ■ 4), scalar dark energy becomes dominant over matter. So these models do not have the desired tracking behavior, and the predicted transient period of acceleration cannot be adopted into the standard scenario of the Big Bang cosmology. When couplings between the scalar field and matter are introduced, the models still have the same problem; only the time when deceleration returns will be varied. To achieve re-deceleration, one has to turn to alternative models that are consistent with the standard Big Bang scenario.  相似文献   

Solar flare forecasting based on sequential sunspot data     

Rong Li  Jie Zhu 《天文和天体物理学研究(英文版)》2013,(9):1118-1126

It is widely believed that the evolution of solar active regions leads to solar flares. However, information about the evolution of solar active regions is not employed in most existing solar flare forecasting models. In the current work, a shortterm solar flare forecasting model is proposed, in which sequential sunspot data, including three days of information about evolution from active regions, are taken as one of the basic predictors. The sunspot area, the McIntosh classification, the magnetic classification and the radio flux are extracted and converted to a numerical format that is suitable for the current forecasting model. Based on these parameters, the sliding-window method is used to form the sequential data by adding three days of information about evolution. Then, multi-layer perceptron and learning vector quantization are employed to predict the flare level within 48 h. Experimental results indicate that the performance of the proposed flare forecasting model works better than previous models.  相似文献   

Do protostellar fountains shape the regional core mass function?     

Jin-Zeng Li  Claudio Carlos Mallamaci  Ricardo César Podest  Eloy Actis Vicente  Ya-Fang Huang  Ana Maria Pacheco 《天文和天体物理学研究(英文版)》2013,(6):719-728

The emerging massive binary system associated with AFGL 961 signifies the latest generation of massive star and cluster formation in the Rosette Molecular Complex. We present the detection of a compact cluster of dusty cores toward the AFGL 961 region based on continuum imaging at 1.3 mm by the Submillimeter Array. The binary components of AFGL 961 are associated with the most intensive millimeter emission cores or envelopes, confirming that they are indeed in an early stage of evolution. The other massive cores, however, are found to congregate in the close vicinity of the central high-mass protostellar binary. They have no apparent infrared counterparts and are, in particular, well aligned transverse to the bipolar molecular outflows originating from AFGL 961. This provides evidence for a likely triggered origin of the massive cores. All 40 individual cores with masses ranging between 0.6 and 15 M⊙ were detected above a 3 σ level of 3.6 mJy beam-1 (or0.4 M⊙ ), based on which we derive a total core mass of 107 M⊙ in the AFGL 961 region. As compared to the stellar initial mass function, a shallow slope of 1.8 is, however, derived from the best fit to the mass spectrum of the millimeter cores with a prestellar and/or protostellar origin. The flatter core mass distribution in the AFGL 961 region is attributed here to dynamic perturbations from the massive molecular outflows that originated from the massive protostellar binary, which may have altered the otherwise more quiescent conditions of core or star formation, enhanced the formation of more massive cores and, as a result, influenced the core mass distribution in its close vicinity.  相似文献