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991.
Observations of Titan obtained by the Cassini Visual and Infrared Mapping Spectrometer (VIMS) have revealed Selk crater, a geologically young, bright-rimmed, impact crater located ∼800 km north-northwest of the Huygens landing site. The crater rim-crest diameter is ∼90 km; its floor diameter is ∼60 km. A central pit/peak, 20-30 km in diameter, is seen; the ratio of the size of this feature to the crater diameter is consistent with similarly sized craters on Ganymede and Callisto, all of which are dome craters. The VIMS data, unfortunately, are not of sufficient resolution to detect such a dome. The inner rim of Selk crater is fluted, probably by eolian erosion, while the outer flank and presumed ejecta blanket appear dissected by drainages (particularly to the east), likely the result of fluvial erosion. Terracing is observed on the northern and western walls of Selk crater within a 10-15 km wide terrace zone identified in VIMS data; the terrace zone is bright in SAR data, consistent with it being a rough surface. The terrace zone is slightly wider than those observed on Ganymede and Callisto and may reflect differences in thermal structure and/or composition of the lithosphere. The polygonal appearance of the crater likely results from two preexisting planes of weakness (oriented at azimuths of 21° and 122° east of north). A unit of generally bright terrain that exhibits similar infrared-color variation and contrast to Selk crater extends east-southeast from the crater several hundred kilometers. We informally refer to this terrain as the Selk “bench.” Both Selk and the bench are surrounded by the infrared-dark Belet dune field. Hypotheses for the genesis of the optically bright terrain of the bench include: wind shadowing in the lee of Selk crater preventing the encroachment of dunes, impact-induced cryovolcanism, flow of a fluidized-ejecta blanket (similar to the bright crater outflows observed on Venus), and erosion of a streamlined upland formed in the lee of Selk crater by fluid flow. Vestigial circular outlines in this feature just east of Selk’s ejecta blanket suggest that this might be a remnant of an ancient, cratered crust. Evidently the southern margin of the feature has sufficient relief to prevent the encroachment of dunes from the Belet dune field. We conclude that this feature either represents a relatively high-viscosity, fluidized-ejecta flow (a class intermediate to ejecta blankets and long venusian-style ejecta flows) or a streamlined upland remnant that formed downstream from the crater by erosive fluid flow from the west-northwest.  相似文献   
992.
通过对当地暴雨特征、地层岩性、地质构造、泥石流固体物质源及形成的踏勘,针对该泥石流具有危险度高,流量大的特点,执行全面规划、重点治理的设计思路,采取了防护、生物工程相结合的综合防治措施。拦挡工程为有效发挥工程泻洪、拦渣、调节、固床、稳坡和控制固体物质补给量,预防沟道下切及沟壑发展,减少泥石流对下游村庄危害,起到了积极作用;生物工程的主要作用是稳固堤前砂土、减缓水石流流速、减小水石流对护堤的直接冲蚀和破坏、保障堤内居民生命财产安全和耕地的正常使用,增大植被覆盖率,绿化环境等。  相似文献   
993.
拉萨地块北部广泛分布着白垩纪火山岩。本文及已有年代学研究表明,这些火山岩主要形成于早白垩世中期(140~110Ma)和晚白垩世早期(100~80Ma)两个阶段。早白垩世中期火山岩主要为则弄群和多尼组地层中的火山岩夹层,岩性组合包括玄武岩、玄武安山岩、安山岩、英安岩和流纹岩,主体为高钾钙碱和钾玄质系列,具有初始87Sr/86Sr比值(0.7068~0.7102)较高、εNd(t)(-9.3~-1.5)较低和δ18OV-SMOW(7.2‰~9.8‰)较高等同位素组成特征,源区为受消减沉积物和/或蚀变玄武质洋壳的含水流体/熔体交代的富集岩石圈地幔楔。晚白垩世早期火山岩零星分布在拉萨地块北部和羌塘地块南部,岩石类型以玄武岩、玄武安山岩、安山岩为主,有少量的酸性火山岩(英安岩),主体为典型的钙碱性系列组合(低钾拉斑+中钾钙碱),具有较高的Mg(Mg#可高达59)和相容元素Cr(162×10-6)、V(216×10-6)和Ni(80×10-6)含量以及更为原始的Sr-Nd同位素组成,(87Sr/86Sr)t=0.7041~0.7048,εNd(t)=0.9~2.2,指示源区可能为受到上涌软流圈地幔熔体二次交代的交代富集岩石圈地幔,本文将其命名为尼玛火山岩。综合以上白垩纪火山岩和拉萨地块南部叶巴组、桑日群和林子宗群火山岩的时空分布特征,认为中生代至早第三纪冈底斯岛弧的演化发生了两次大的空间迁移:中生代早侏罗世以来由南向北变新,从最南部的叶巴组(早侏罗世,193~174Ma)和桑日群火山岩(J3—K1),到北部的则弄群和多尼组火山岩(早白垩世中期,140~110Ma),最后到最北部的尼玛火山岩(晚白垩世早期,100~80Ma);早第三纪由北向南跃迁回南部,从北部的尼玛火山岩迁移到南部的林子宗群火山岩(70~40Ma)。冈底斯岛弧火山岩的时空分布特征和成分演化规律,揭示了新特提斯洋板块的俯冲历史,即早期新特提斯洋壳由南向北低角度俯冲,然后再高角度反向旋转,直至最后发生拆沉。  相似文献   
994.
三台油气田中上侏罗统储层非均质性特征   总被引:1,自引:0,他引:1  
储层非均质性是储层评价的重要指标,通过对区内近20口井300多个样品统计分析表明,三台油气田中上侏罗统储层存在较强的非均质性.不同层系存在差异,齐古组储层非均质性较头屯河组要弱.近源沉积、储层稳定性差、岩石成分复杂、矿物成熟度低、分选差、岩石颗粒大小混杂、填隙物含量高、类型多等诸多因素是形成本区储层强非均质性的重要原因.  相似文献   
995.
In the Belledonne massif, the steep Paleozoic Belledonne Middle Fault (BMF) separates micaschists, displaying numerous landslides, from amphibolites. The massif is incised by the lower Romanche river valley. When crossing the BMF, the valley widens into a lozenge-shaped basin recently interpreted as an active pull-apart type structure associated with a major N110 striking Quaternary fault. Multidisciplinary investigations were carried out in the basin to check if this model has implications on the seismic and landslide hazard assessment. This study demonstrated the existence of a N80 sinistral strike slip Séchilienne Fault Zone (SFZ). This fault zone is suspected to offset the BMF by 375 m across the basin. Geophysical experiments revealed that the bedrock depth increases strongly in the basin, up to 350 m. Our study invalidates the active pull-apart origin of the basin and suggests it results from Quaternary glacial and fluvial erosion processes, magnified by the intersection of two inherited structures, the BMF and the SFZ.  相似文献   
996.
Research conducted in the Yamé Valley (Dogon Country, Mali) provides valuable information about the river systems and their Holocene evolution in Sudano-Sahelian West Africa. Past research in the region has relied primarily on marine and lacustrine records. The new results confirm correlation between palaeoclimatic fluctuations recorded in both the river system and in tropical African lakes. They offer a new continental milestone for understanding of the environmental repercussions of Holocene monsoon oscillations. These studies demonstrate the value of river systems as a palaeoenvironmental record and the role of palaeoclimatic and anthropogenic factors in the Holocene dynamics of Sudano-Sahelian hydrosystems.  相似文献   
997.
In EGS projects, fault zones are considered as the structures controlling deep flow at the reservoir scale. Using a large set of petrophysical properties (porosity, density, permeability, thermal conductivity [TC]) measured on cores collected along the EPS-1 borehole, a model of fault zone is proposed to describe them. A fault zone is a complex structure, showing different parts with different kinds of deformations and/or materials that could explain chemical and physical processes observed during fluid-rock interactions. The different parts composing the fault zone are: (1) the fault core or gauge zone; (2) the damage zone; (3) and the protolith. They are usually heterogeneous and show different physical properties. The damage zone is a potential high permeability channel and could become the main pathway for fluids if secondary minerals seal the fault core. Porosity is the lowest within the protolith, between 0.5 and 1%, but can go up to 15% in the fault zone. Permeability ranges from 10?20 m2 in the fresh granite to, at least, 10?15 m2 in the fault core, and TC ranges from 2.5 W K?1m?1 to 3.7 W K?1m?1. Finally, variations in specific surface are set over two orders of magnitude. If the lowest values usually characterize the fresh granite far from fault zones, physical properties could show variations spread over their whole respective ranges within these fault zones.  相似文献   
998.
根据大气降水化学成分和岩溶水化学成分的分析,认识到了陕西镇安、旬阳地区夏秋季岩溶水 H+ 与 H C O-3 含量高,岩溶作用活跃,冬春季的变化相反。根据该区及南桂林等地现代岩溶作用强弱变化规律,提出了补充的岩溶作用的物理化学模式。  相似文献   
999.
The Weddell Sea Embayment (WSE) sector of the Antarctic ice sheet has been suggested as a potential source for a period of rapid sea-level rise – Meltwater Pulse 1a, a 20 m rise in ~500 years. Previous modelling attempts have predicted an extensive grounding line advance in the WSE, to the continental shelf break, leading to a large equivalent sea-level contribution for the sector. A range of recent field evidence suggests that the ice sheet elevation change in the WSE at the Last Glacial Maximum (LGM) is less than previously thought. This paper describes and discusses an ice flow modelling derived reconstruction of the LGM ice sheet in the WSE, constrained by the recent field evidence. The ice flow model reconstructions suggest that an ice sheet consistent with the field evidence does not support grounding line advance to the continental shelf break. A range of modelled ice sheet surfaces are instead produced, with different grounding line locations derived from a novel grounding line advance scheme. The ice sheet reconstructions which best fit the field constraints lead to a range of equivalent eustatic sea-level estimates between approximately 1.4 and 3 m for this sector. This paper describes the modelling procedure in detail, considers the assumptions and limitations associated with the modelling approach, and how the uncertainty may impact on the eustatic sea-level equivalent results for the WSE.  相似文献   
1000.
Most conventional statistical methods aiming at defining geochemical concentration thresholds for separating anomalies from background have limited effectiveness in areas with complex geological settings. This paper uses multifractal analysis to combine the characteristics of geochemical frequency distribution and spatial dispersion in order to map geochemical singularities instead of using conventional statistically derived concentration thresholds. The model, termed radius–areal Productivity (rP) model, employs a stable measure and a scale-increasing method to estimate geochemical singularities spatially on geochemical landscape for delineating potential anomalies. The model is applied to geochemical data of regional stream sediments from the Funin Sheet, Yunnan, China.  相似文献   
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