渤海湾表层沉积物元素地球化学分布特征与影响因素     

张连杰  朱龙海  张盼  赵博  王鹏 《海洋科学》2019,43(6):78-87

对取自渤海湾的307个表层沉积物进行了元素测试和粒度分析。渤海湾表层沉积物的常微量元素呈现4种组合:富集于粗粒沉积区的SiO_2、Na_2O亲碎屑元素组合;富集于细粒沉积区的以Al_2O_3和重金属元素为代表的亲黏土元素组合;与缺氧环境有关的MnO、V、TOC元素组合和与河流输入有关的陆源CaO、TiO_2元素组合。粒度粗细主导了渤海湾元素含量分布的整体格局;海域河流物源供应不同较大影响了渤海湾南部(富Na_2O、CaO和SiO_2)和北部(富Ba和P_2O_5)在元素含量上的差异;高流速潮流对海底的冲刷再分配导致曹妃甸南侧Sr、Ca元素的条带状富集异常;有机质在细粒沉积区的富集导致缺氧环境的形成和K_2O、Mn、V、自生黄铁矿的海洋自生化学沉积;人类活动导致以Pb为代表的重金属污染在河流入海口、港口及沿岸海域的元素分布异常;曹妃甸沙坝内侧的泻湖(海洋钙质生物沉积)与沙坝外侧水下岸坡(陆源碎屑沉积)的截然不同的物源,导致了独特地貌沉积环境下元素分布的局部差异。  相似文献   

Risk evaluation of dam-break environmental impacts based on the set pair analysis and cloud model     

Ge  Wei  Li  Zongkun  Li  Wei  Wu  Meimei  Li  Juanjuan  Pan  Yipeng 《Natural Hazards》2020,104(2):1641-1653

Natural Hazards - Many dams have been constructed around the world. Compared with the potential losses of life and economy, the environmental impacts caused by dam breach were less analyzed. As a...  相似文献   

自然海岸资源价值核算方法研究与应用          下载免费PDF全文

闫吉顺  张盼  黄小露  王鹏  方海超 《海洋开发与管理》2019,36(5):26-31

文章通过构建自然海岸资源价值核算指标体系,确定了评估因子量化标准,建立了自然海岸基本价值核算系数计算模型、服务价值核算系数计算模型、综合核算系数计算模型和基准价值计算模型。在此基础上,构建了自然海岸资源价值核算模型,并应用其模型对大连市大陆自然海岸资源价值进行核算。最终得出大连市大陆自然海岸资源总价值约为2 409亿元。  相似文献   

祁连山北部基岩河道宽度对构造和岩性的响应     

李琼  秦冰雪  潘保田 《第四纪研究》2020,(1):132-147

活动造山带基岩河流地貌研究,目前已成为构造地貌学研究的前沿和热点。河道宽度形态的调整变化是基岩河流响应构造、岩性和气候等扰动的重要方式之一。通过研究祁连山北部地区6个重点流域基岩河道的宽度形态发现:河道宽度总体上呈现出东西向和南北向的变化特征,河道向下游增宽的速率,东段地区显著高于中段地区,低山带显著高于高山带;对比河道宽度的变化特征与构造抬升速率及岩性抗蚀性的变化,可以推断:在祁连山北部地区,基岩河道宽度响应构造抬升和岩性抗蚀性的变化进行了系统地调整,构造抬升控制了流域河道宽度变化的总体趋势,而岩性抗蚀性变化则导致了流域内部局部河段河道宽度的大幅波动。在祁连山北部地区开展的基岩河道宽度形态研究,为利用基岩河道形态研究造山带的构造变形奠定了基础,对于探索构造抬升背景下地貌的发育过程具有十分重要的意义。  相似文献   

西藏甲玛铜多金属矿床磁黄铁矿标型矿物学特征及其地质意义   总被引：2，自引：0，他引：2  

杨阳  唐菊兴  吴纯能  林彬  唐攀  张泽斌  何亮  祁婧  李怡萱 《矿床地质》2020,39(2):337-350

甲玛矿床位于冈底斯成矿带东段,是西藏地区最大的铜多金属矿床之一。磁黄铁矿是甲玛矿床最常见的金属矿物之一,其标型特征不仅反映其自身形成环境,对其形成机制和矿床成因也具有指示意义。文章选取产于不同岩性中的磁黄铁矿矿石样品,利用矿相学、X射线衍射和电子探针分析等手段对磁黄铁矿的形态、成分和结构进行了分析研究。研究表明,甲玛矿床的磁黄铁矿主要分布在距离岩体中心较远的矿区远端矽卡岩和角岩中。磁黄铁矿的晶胞参数和粉晶X射线衍射曲线显示矽卡岩中的磁黄铁矿主要为高温六方磁黄铁矿,角岩中的磁黄铁矿为高温六方磁黄铁矿和低温单斜磁黄铁矿的交生体,但主要以低温单斜磁黄铁矿为主。通过对矽卡岩和角岩中的磁黄铁矿进行电子探针测试,结果显示:矽卡岩中的磁黄铁矿中w(Fe)为60.09%～60.71%,平均为60.38%,w(S)为38.18%～38.69%,平均38.35%,化学分子式为Fe_8S_9～Fe_(10)S_(11);角岩中的磁黄铁矿中w(Fe)为59.05%～59.57%,平均为59.10%,w(S)为39.28%～39.95%,平均39.59%,化学分子式为Fe_5S_6～Fe_7S_8。根据以上矿物学特征,笔者进一步探讨了该矿床磁黄铁矿的沉淀机制:炽热的岩浆热液上涌,与碳酸盐岩地层和碎屑岩地层接触发生相互作用,并有大气水的加入,使得成矿流体在角岩中先快速降温,形成高温六方磁黄铁矿和低温单斜磁黄铁矿的交生体。同时,大量的含矿热液形成,并充填于有利的成矿空间(主要为层间破碎带)沉淀成矿,形成矽卡岩矿体,然后流体在矽卡岩矿段中经历缓慢降温,形成高温六方磁黄铁矿。结合矿床地质特征和相关元素地球化学特征,认为甲玛矿床类型为斑岩-矽卡岩型。  相似文献   

准噶尔盆地西北缘及玛湖凹陷沉积储集层研究进展^*          下载免费PDF全文

张昌民  尹太举  唐勇  郭旭光  赵康  潘进  陈美玲 《古地理学报》2020,22(1):129-146

准噶尔盆地西北缘玛湖凹陷中心区10×10⁸ t级砾岩大油区的发现,带动了该区沉积储集层研究的不断深入。作者梳理了准噶尔盆地西北缘及玛湖凹陷的沉积储集层研究现状和进展,认为准噶尔盆地西北缘及玛湖凹陷的沉积储集层研究的进展主要表现为: (1)提出了新的砂砾岩储集层岩石相和岩石学分析方法;(2)探索形成了新的沉积储集层地球物理测井和地震描述技术;(3)针对不同层系,在沉积物源、沉积相、沉积环境、沉积体系和沉积模式等方面取得大量新认识,建立了大型退覆式浅水缓坡扇三角洲沉积模式,指导油气勘探不断获得新突破;(4)在成岩作用理论指导下,所发现的储集层埋藏深度不断增加。研究表明,玛湖凹陷的沉积体系具有继承性: 从二叠纪到新近纪,发育了火山—碎屑岩沉积体系、细粒—蒸发盐沉积体系以及粗粒冲积扇、扇三角洲、辫状河三角洲等沉积体系,气候、构造和湖平面变化控制了沉积体系的形成和演化。沉积储集层研究为玛湖砾岩大油田的发现提供了有力的理论支持。未来应当加强针对古老层系和深部地层的沉积储集层研究工作,重视新理论新技术在西北缘和玛湖沉积储集层研究中的应用,已经形成的理论技术需要在勘探实践中接受进一步检验和完善。  相似文献   

Habitability analyses of aquatic bacteria     

Md. Nurul Haider  Masahiko Nishimura  Minoru Ijichi  Ching-chia Yang  Wataru Iwasaki  Kazuhiro Kogure 《Journal of Oceanography》2018,74(2):197-207

Habitability is defined as an ability of an organism to inhabit different environments. Habitability of organisms, however, cannot be inferred from analyses such as a whole genome or community structures. A recently developed database, the MetaMetaDB, gives us information from what kind of environments one particular 16S rRNA sequence data has ever been obtained, and thus enables us to infer the habitability of the bacterium in question. In order to check the applicability of this database to study the habitability of aquatic bacteria, samples collected at two Naka River stations, one estuarine station from Naka River Estuary, two coastal stations at Oarai in Ibaraki Prefecture, Japan and one station in the Kuroshio Current of the western North Pacific were examined. The phylotypes were tracked against the MetaMetaDB and it was reasonably found that the low-salinity stations were dominated by sequences with “freshwater and groundwater”, “human” and “wastewater” habitat identities, while the high-salinity stations were dominated by those with a “marine” identity. The phylotypes of low-salinity stations with a particular habitat identity were absent or rare in the high-salinity stations and vice versa. The MetaMetaDB also showed that sequences of Cyanobacteria or related phylogenetic groups may be present in the human gut, as well as the probable distribution of the relatives (ancestors/descendants/siblings) of some bacteria. These overall findings proved that the MetaMetaDB is useful as a new tool to infer microbial habitability and it gives us new information on the possible origin and ecology of microorganisms in the environments.  相似文献   

Tide-related Changes in mRNA Abundance of Aromatases and Estrogen Receptors in the Ovary and Brain of the Threespot Wrasse <Emphasis Type="Italic">Halichoeres trimaculatus</Emphasis>     

Dae-Ju Oh  Sung-Pyo Hur  Selma Bouchekioua  Yuki Takeuchi  Shingo Udagawa  Neelakanteswar Aluru  Yong-Ju Park  Ji-Gweon Park  Se-Jae Kim  Thomas W. Moon  Mathilakath M. Vijayan  Akihiro Takemura 《Ocean Science Journal》2018,53(2):239-249

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Dark energy cosmological models with cosmic string     

T. Vinutha  V. U. M. Rao  Bekele Getaneh  Molla Mengesha 《Astrophysics and Space Science》2018,363(9):188

In this paper we have studied the anisotropic Kantowski-Sachs, locally rotationally symmetric (LRS) Bianchi type-I and LRS Bianchi type-III geometries filled with dark energy and one dimensional cosmic string in the Saez-Ballester theory of gravitation. To get physically valid solution we take hybrid expansion law of the average scale factor which is a product of power and exponential type of functions that results in time dependent deceleration parameter (\(q\)). The equation of state parameter of dark energy (\(\omega _{\mathit{de}}\)) has been discussed and we have observed that for the three models it crosses the phantom divide line (\(\omega _{\mathit{de}} = -1\)) and shows quintom like behavior. The density of dark energy (\(\rho _{\mathit{de}}\)) is an increasing function of redshift and remains positive throughout the evolution of the universe for the three models. Moreover in Kantowski-Sachs and LRS Bianchi type-I geometries the dark energy density dominates the string tension density (\(\lambda \)) and proper density (\(\rho \)) throughout the evolution of the universe. The physical and geometrical aspects of the statefinder parameters (\(r,s\)), squared speed of sound (\(v_{s}^{2} \)) and \(\omega _{\mathit{de}}\)–\(\omega ^{\prime }_{\mathit{de}}\) plane are also discussed.  相似文献   

An on Orbit Determination of Point Spread Functions for the <Emphasis Type="Italic">Interface Region Imaging Spectrograph</Emphasis>     

Hans Courrier  Charles Kankelborg  Bart De Pontieu  Jean-Pierre Wülser 《Solar physics》2018,293(9):125

Using the 2016 Mercury transit of the Sun, we characterize on orbit spatial point spread functions (PSFs) for the Near- (NUV) and Far- (FUV) Ultra-Violet spectrograph channels of NASA’s Interface Region Imaging Spectrograph (IRIS). A semi-blind Richardson–Lucy deconvolution method is used to estimate PSFs for each channel. Corresponding estimates of Modulation Transfer Functions (MTFs) indicate resolution of 2.47 cycles/arcsec in the NUV channel near 2796 Å and 2.55 cycles/arcsec near 2814 Å. In the short (\({\approx}\,1336~\mathring{\mathrm{A}}\)) and long (\({\approx}\,1394~\mathring{\mathrm{A}}\)) wavelength FUV channels, our MTFs show pixel-limited resolution (3.0 cycles/arcsec). The PSF estimates perform well under deconvolution, removing or significantly reducing instrument artifacts in the Mercury transit spectra. The usefulness of the PSFs is demonstrated in a case study of an isolated explosive event. PSF estimates and deconvolution routines are provided through a SolarSoft module.  相似文献