Oil dispersal modelling: reanalysis of the Rena oil spill using open-source modelling tools     

HFE Jones  MTS Poot  JC Mullarney  WP de Lange 《新西兰海洋与淡水研究杂志》2016,50(1):10-27

ABSTRACT

Oil spill forecast modelling is typically used immediately after a spill to predict oil dispersal and promote mobilisation of more effective response operations. The aim of this work was to map oil dispersal after the grounding of the MV Rena on Astrolabe Reef and to verify the results against observations. Model predictions were broadly consistent with observed distribution of oil contamination. However, some hot spots of oil accumulation, likely due to surf-zone and rip current circulation, were not well represented. Additionally, the model was run with 81 differing wind conditions to show that the events occurring during the grounding represented the typical likely behaviour of an oil spill on Astrolabe Reef. Oil dispersal was highly dependent on prevailing wind patterns; more accurate prediction would require better observations of local wind patterns. However, comparison of predictions with observations indicated that the GNOME model was an effective low-cost approach.  相似文献   

曹妃甸近岸及周边海区碎屑矿物组成特征及其环境意义     

祝贺  衣华鹏  孙志高  孙万龙  孙文广  王伟  王苗苗  任鹏 《海洋科学》2016,40(8):76-83

为探讨曹妃甸近岸及周边海区沉积物碎屑矿物组成特征以及曹妃甸大规模围填海工程对其影响,作者对2013年10月采自曹妃甸及周边海区的表层沉积物样品采用轻重矿物分离的方法进行了鉴定。结果表明:大规模围填海工程在改变曹妃甸岸线形态的同时也改变了其冲淤环境,使得碎屑矿物组分在大规模围填海前后发生一定变化。研究区的沉积物整体以轻矿物为主,平均含量为97.83%,其中曹妃甸近岸平均含量为95.57%;重矿物平均含量为2.17%,其中曹妃甸近岸平均含量为4.43%。研究区的重矿物优势矿物主要有普通角闪石、绿帘石和自生黄铁矿,其中普通角闪石所占比例在曹妃甸近岸达到最高值(36.41%);轻矿物的优势矿物主要有石英、斜长石和风化碎屑,其中石英所占比例也在曹妃甸近岸达到最高值(62.72%)。研究发现,曹妃甸近岸沉积物碎屑矿物相对含量增加而重矿物基本不变,这在一定程度上揭示了大规模人工围填海工程对曹妃甸近岸及周边海区沉积环境的影响。  相似文献   

青海南山地区角孔变质岩地质特征、年代学及其地质意义     

李佐臣  裴先治  李瑞保  裴磊  张永明  王旭斌  刘成军  陈有炘  王盟 《地质通报》2018,37(4):570-588

青海南山达不祖乎山北部一带的角孔变质岩系原划为早中三叠世隆务河组。通过野外实测地质剖面和路线地质调查,查明该套地层单元野外产出状态及岩石组合特征,并对其物质来源和形成时代进行分析,对进一步研究该区晚古生代-早中生代的构造演化具有重要意义。该套变质岩系为一套长石石英岩、石英岩、大理岩和黑云石英片岩组合,由下向上划分为3个岩段,叠置厚度大于3186.3m。根据碎屑锆石年龄分布特征,可大致划分为5个年龄组段,分别为250～304Ma、405～546Ma、649～1077Ma、1402～1620Ma和1861～2990Ma,其中250～304Ma可进一步划分为250～269Ma和289～304Ma两个亚组。综合前人研究资料与区域构造岩浆活动,将青海南山地区角孔变质岩的沉积时代限定为二叠纪,物源主要来自祁连造山带加里东期和晋宁期岩浆弧,柴北缘构造带海西期岩浆弧也提供了部分物质,晚古生代—早中生代经历了陆内裂陷、洋盆拉张及俯冲碰撞的构造演化过程。  相似文献   

内蒙古西乌旗罕乌拉地区下二叠统寿山沟组碎屑锆石LA-ICP-MS U-Pb年龄及其地质意义   总被引：2，自引：2，他引：0  

张晓飞  王必任  张华川  周毅  冯俊岭  曹军  滕超  刘俊来 《地质通报》2018,37(5):863-880

中亚造山带南缘二叠纪的构造背景一直存在争议。以内蒙古西乌旗罕乌拉地区发育的寿山沟组为研究对象,开展了野外地质、岩石学、碎屑锆石LA-ICP-MS U-Pb年龄研究。2个样品锆石阴极发光图像和Th/U值指示,锆石为岩浆成因锆石。103颗碎屑锆石年龄测试结果显示,年龄信息可划分为5组:285~328Ma,峰期年龄302Ma;338~361Ma;455~490Ma;757Ma;1278Ma、2380Ma。最年轻的年龄为285Ma,结合侵入其中的花岗岩同位素年龄,指示西乌旗罕乌拉地区寿山沟组沉积时限介于285~280Ma之间,主体沉积时代应为早二叠世Sakmarian期—Artinskian期。寿山沟组碎屑锆石反映出近源、快速沉积的特点,沉积物源中含有较多的火山碎屑物,可能代表弧后盆地沉积,为早二叠世古亚洲洋闭合前洋壳俯冲消减作用的沉积响应。结合区域资料,寿山沟组碎屑锆石的年龄对应于东北地区的变质基底及其后的构造岩浆事件,物源区物质主要来自于苏尼特左旗—锡林浩特—西乌旗一带早石炭世末—晚石炭世岩浆弧及贺根山—东乌旗一带,并进一步限制了华北与西伯利亚两大板块的缝合线应位于寿山沟组发育地区的南部,即索伦缝合带,拼合时代最可能为晚二叠世—早三叠世。  相似文献   

Occurrence and Chemical Compositions of Amphiboles in Altered Dioritic Rocks of Laiwu Skarn‐Type Iron Deposit in West Shandong Area,China     

《Resource Geology》2018,68(4):425-445

The Laiwu Fe deposit is the largest skarn‐type deposit in West Shandong in China, with an estimated reserve of 290 Mt of iron ore. Here, we investigate the occurrence and chemical composition of amphiboles in altered dioritic rocks of this deposit. Three generations of amphibole group minerals were identified in these rocks. The first type (Type 1) is a hornblende with a generally euhedral crystal shape, 150–500 μm in size, and dominantly occurs in the host monzonite. The second type (Type 2) of hornblende occurs as fine grains (<100 μm) or concentric rims, less than 50 μm in thickness, around the Type 1 hornblende. The third type (Type 3) of amphibole is anhedral actinolite occurring along the boundary or the cracks of the Type 1 or 2 hornblende grains. The Type 1 hornblende has higher FeO (12.5–15.6 wt.%) and lower MgO contents (11.2–14.6 wt.%) than the Type 2 hornblende, which has an FeO content ranging from 8.8 to 10.5 wt.% and MgO content ranging from 14.2 to 17.1 wt.%. The Type 3 actinolite shows the lowest FeO (4.6–6.4 wt.%) and highest MgO (19.8–21.2 wt.%) contents. We infer that the Type 2 hornblende formed from Fe‐rich hydrothermal fluids released during rapid upwelling of the crystallizing magma. The fluids were relatively reduced and enriched in Fe. The Type 3 actinolite formed by coupled dissolution and reprecipitation, and its formation is one of the features denoting Fe‐enrichment events. Our study of these types of amphibole provides insights into the ore formation process.  相似文献   

Isotope stratigraphy and U-Pb dating of detrital zircons from the Vendian-Cambrian deposits of the North Muya block     

I.A. Vishnevskaya  E.F. Letnikova  N.A. Kanygina  A.I. Proshenkin  N.G. Soloshenko  E.V. Vetrov  V.Yu. Kiseleva 《Russian Geology and Geophysics》2018,59(11):1433-1449

U-Pb dating of detrital zircons from the sandstones of the Mamakan Formation has been made. Geochemical and isotope parameters of the carbonate deposits of the Yanguda Formation in the Vendian-Cambrian cover of the North Muya continental block have been estimated. It has been established that only the Neoproterozoic (630-915 Ma) rocks of the North Muya block were the provenances of terrigenous material. In the least altered carbonate rocks of the Yanguda Formation, the ⁸⁷Sr/⁸⁶Sr ratio is within 0.70814-0.70879 and δ¹³C varies from -0.4 to + 1.9‰. Comparison of the evaluated isotope parameters with those of carbonate rocks of typical Vendian-Cambrian sections shows that the carbonate deposits of the Yanguda Formation accumulated in the Early Cambrian, about 520 Ma. Sedimentation of the Mamakan and Yanguda Formations took place in the local sedimentary basin in the Vendian-Early Cambrian, in the absence of tectonic activity within the North Muya block. Detrital material that formed during the destruction of the rocks of the Siberian Platform basement and cover was not supplied into the basin.  相似文献   

Origin of abundant moonmilk deposits in a subsurface granitic environment     

《Sedimentology》2018,65(5):1482-1503

Subsurface granitic environments are scarce and poorly investigated. A multi‐disciplinary approach was used to characterize the abundant moonmilk deposits and associated microbial communities coating the granite walls of the 16th Century Paranhos spring water tunnel in Porto city (north‐west Portugal). It is possible that this study is the first record of moonmilk in an urban subsurface granitic environment. The morphology and texture, mineralogical composition, stable isotope composition and microbial diversity of moonmilk deposits have been studied to infer the processes of moonmilk formation. These whitish secondary mineral deposits are composed of very fine needle‐fibre calcite crystals with different morphologies and density. Calcified filaments of fungal hyphae or bacteria were distinguished by field emission scanning electron microscopy. Stable isotope analysis revealed a meteoric origin of the needle‐fibre calcite, with an important contribution of atmospheric CO ₂, soil respiration and from weathering of Ca‐bearing minerals. The DNA ‐based analyses revealed the presence of micro‐organisms related to urban contamination, including Actinobacteria, mainly represented by Pseudonocardia hispaniensis , Thaumarchaeota and Ascomycota, dominated by Cladosporium . This microbial composition is consistent with groundwater pollution and contamination sources of the overlying urban area, including garages, petrol stations and wastewater pipeline leakage, showing that the Paranhos tunnel is greatly perturbed by anthropogenic activities. Whether the identified micro‐organisms are involved in the formation of the needle‐fibre calcite or not is difficult to demonstrate, but this study evidenced both abiotic and biogenic genesis for the calcite moonmilk in this subsurface granitic environment.  相似文献   

川北地区寒武系筇竹寺组钙质结核裂缝充填物特征及指示意义   总被引：1，自引：0，他引：1  

冯明友  郑江  刘田  刘小洪  张家强  梅文华  孙霓源  龙涛 《地质论评》2018,64(3):711-722

川北地区寒武系筇竹寺组钙质结核泥页岩中早成岩期钙质结核较发育,结核裂缝中见多期次矿物充填。为揭示钙质结核裂缝形成机理,本次结合岩石学特征及地球化学特征等开展系统研究。川北筇竹寺组钙质结核裂缝中见三~四期矿物充填。第一期微晶方解石表面较脏,阴极发光暗淡,δ13C_(PDB)、δ18O_(PDB)平均值分别为-4.26‰及-7.69‰;第二期为细—中晶粒状方解石充填,阴极发光为橘黄色,流体包裹体均一温度为平均值为86.4℃,δ13C_(PDB)、δ18O_(PDB)平均值分别为-3.15‰及-7.41‰;第三期为粗晶方解石充填阴极发光暗淡,流体包裹体均一温度平均值为96.6℃,δ~(13)C_(_(PDB))、δ~(18)O_(_(PDB))平均值分别为-1.73‰及-10.28‰;第四期为重晶石充填。结合区域构造史—热演化史分析表明,钙质结核裂缝中四期充填物分别指示早期脱水、烃源岩早成熟期生烃、加里东构造运动抬升释压及深埋藏期硫酸盐热还原作用事件。  相似文献   

Paleogene stratigraphy of Kutch,India: an update about progress in foraminiferal biostratigraphy     

Pratul Kumar Saraswati  Sonal Khanolkar  Santanu Banerjee 《Geodinamica Acta》2018,30(1):100-118

The Paleogene sections of Kutch are the reference for the regional chronostratigraphic units of India. The ages of these dominantly shallow marine carbonates are mainly based on larger benthic foraminifera (LBF). The taxonomic revisions of the LBF and the progressively refined shallow benthic zonations (SBZ) have necessitated the present study on updating the stratigraphy of the area. The sedimentation in Kutch commenced with the deposition of volcaniclastics in terrestrial environments in the Paleocene. The marine transgression in SBZ 5/6 deposited finer clastics and carbonates, designated as Naredi Formation, in early Eocene. There is no evidence of marine Paleocene in Kutch. A major hiatus spanning SBZ 12 to SBZ 16 was followed by the development of a carbonate platform and deposition of Harudi Formation – Fulra Limestone during the Bartonian, SBZ 17. The hiatus corresponds to a widespread stratigraphic break in Pakistan and India to Australia, referred as the ‘Lutetian Gap.’ The Maniyara Fort Formation is assigned to SBZ 22 B and SBZ 23, and its age is revised to Chattian. Climate played a major role in building up of the Paleogene stratigraphic succession of Kutch, the carbonates formed during the warming intervals and the stratigraphic gaps were in the intervening cooling periods.  相似文献   

柴达木盆地鱼卡地区中侏罗统石门沟组砂岩碎屑组分特征及其物源构造环境分析     

王涛  刘招君  孙平昌  白悦悦  宋朔 《世界地质》2018,37(1):154-161

利用砂岩碎屑骨架成分统计和碎屑颗粒结构特征分析,研究柴达木盆地北缘鱼卡地区中侏罗统石门沟组碎屑岩的源岩类型及其构造环境。石门沟组砂岩成分成熟度中等、结构成熟度较低,具有近源物源的特点。砂岩碎屑骨架成分统计结果表明石门沟组的物源区构造背景属于再旋回造山带。结合柴达木盆地北缘中侏罗统古地理特征,确认鱼卡地区石门沟组物源区为祁连山造山带。砂岩碎屑组分可能来自于南祁连山上石炭世宗务隆山群火山岩和达肯达坂山群变质岩。  相似文献