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1.
Basic types of stratification in small eolian dunes   总被引：5，自引：0，他引：5  
The thinnest recognizable strata in modern eolian dune sands can be grouped into six classes. They are herein named planebed laminae, rippleform laminae, ripple-foreset crosslaminae, climbing translatent strata, grainfall laminae, and sandflow cross-strata. Planebed laminae are formed by tractional deposition on smooth surfaces at high wind velocities. They are very rare in the deposits studied. Grainfall laminae are also formed on smooth surfaces, largely by grainfall deposition in zones of flow separation. They are much more common than planebed laminae, which they closely resemble. Eolian climbing-ripple structures are composed primarily of climbing trans-latent strata, each of which is the depositional product of a single climbing ripple. Climbing translatent strata that formed at relatively high or supercritical angles of ripple climb are typically accompanied by rippleform laminae, which are wavy layers parallel to the rippled depositional surfaces. Ripple-foreset crosslaminae, which are incomplete rippleform laminae produced when the angle of ripple climb is relatively low or subcritical, are rarely visible in eolian sands. Sandflow cross-strata are formed by the avalanching of noncohesive sand on dune slipfaces. Their form varies with slipface height and with other factors.  相似文献   

2.
《Sedimentology》2018,65(4):993-1042
Reconstruction of the palaeoenvironmental context of Martian sedimentary rocks is central to studies of ancient Martian habitability and regional palaeoclimate history. This paper reports the analysis of a distinct aeolian deposit preserved in Gale crater, Mars, and evaluates its palaeomorphology, the processes responsible for its deposition, and its implications for Gale crater geological history and regional palaeoclimate. Whilst exploring the sedimentary succession cropping out on the northern flank of Aeolis Mons, Gale crater, the Mars Science Laboratory rover Curiosity encountered a decametre‐thick sandstone succession, named the Stimson formation, unconformably overlying lacustrine deposits of the Murray formation. The sandstone contains sand grains characterized by high roundness and sphericity, and cross‐bedding on the order of 1 m in thickness, separated by sub‐horizontal bounding surfaces traceable for tens of metres across outcrops. The cross‐beds are composed of uniform thickness cross‐laminations interpreted as wind‐ripple strata. Cross‐sets are separated by sub‐horizontal bounding surfaces traceable for tens of metres across outcrops that are interpreted as dune migration surfaces. Grain characteristics and presence of wind‐ripple strata indicate deposition of the Stimson formation by aeolian processes. The absence of features characteristic of damp or wet aeolian sediment accumulation indicate deposition in a dry aeolian system. Reconstruction of the palaeogeomorphology suggests that the Stimson dune field was composed largely of simple sinuous crescentic dunes with a height of ca 10 m, and wavelengths of ca 150 m, with local development of complex dunes. Analysis of cross‐strata dip azimuths indicates that the general dune migration direction and hence net sediment transport was towards the north‐east. The juxtaposition of a dry aeolian system unconformably above the lacustrine Murray formation represents starkly contrasting palaeoenvironmental and palaeoclimatic conditions. Stratigraphic relationships indicate that this transition records a significant break in time, with the Stimson formation being deposited after the Murray formation and stratigraphically higher Mount Sharp group rocks had been buried, lithified and subsequently eroded.  相似文献   

3.
A Late Precambrian fluvial sandstone sequence in northern Norway is dominated by large-scale cross-sets that show either lenticular or tabular geometries in the streamwise sections. The lenticular sets interdigitate and in places show nearly symmetrical formsets. The tabular sets are in places solitary, but are mainly grouped in cosets. In both cross-set types, the cross-strata range from concave-up to sigmoidal in shape, with the latter variety comprising subhorizontal to gently inclined topset strata (with parting lineation) that merge uninterruptedly downflow into the steeper (10–2°) foresets. Within the cross-sets the geometry and dip azimuths of the foresets are conspicuously consistent, although the concave-up and sigmoidal strata commonly alternate downcurrent. The cross-strata characteristics suggest flood stage deposition from relatively high velocity steady currents heavily laden with suspended sand. Both cross-set types are interpreted as representing bedforms generated by flow in the dune to upper-stage plane-bed transition. The lenticular cross-sets probably represent periodic dunes, but it is far less clear whether the long bedforms represented by the tabular sets should be classified as dunes, or rather as solitary to quasi-periodic bars.  相似文献   

4.
Aeolian granule ripple deposits, Namibia   总被引：1，自引：0，他引：1  
Granule ripples are a common feature of most dunefields, yet they have seldom been recognized in ancient deposits. Although granule ripples are common in erosional settings, such as windward slopes of dunes, or scour surfaces in interdunes, they nevertheless migrate laterally and leave distinctive deposits that can be recognized in ancient rocks. These deposits have characteristics of ‘type B’sand sheet deposits, including: ‘poured-in’texture; curving ripple trough; tangential, coarse-grained foresets; irregular silty layers; well-sorted coarse and fine layers (either horizontal or within foresets); and fine layers in ripple troughs. Wind tunnel experiments suggest that under low-velocity wind conditions, granule ripples grow to a significant degree as parasites dependent on saltation of fine sand grains whose impact moves the larger grains of the granule ripple. Although the depositional surface of granule ripples is commonly coated with a layer of coarse grains, this is in most places only a few grains thick. Underlying deposits commonly have a poorly sorted, or ‘poured-in’texture. This texture results from an admixture of fine grains that fall among the spaces between the larger grains during deposition.  相似文献   

5.
The type, scale, and relative abundance of sedimentary structures in four kinds of dunes at White Sands National Monument, New Mexico, were determined by examination of vertical sections on walls of trenches cut through the dunes both in a windward direction and at right angles to this direction. Analysis of cross-stratification in all dunes examined indicated certain common features: sets of cross-strata mostly are medium- to large-scale; nearly all laminae dip downwind at high angles (not uncommonly at 30°-34°); most bounding surfaces between sets of cross-strata are nearly horizontal on the upwind side, but have progressively steeper dips to lee, downwind; and individual sets of cross-strata tend to be thinner and the laminae flatter near the top than at the bottom of a dune in vertical section. Sparse but distinctive structural features that are characteristic of the four types of dunes are varieties of contorted bedding, rare ripple laminae, and either local scour-and-fill bedding, or festoon bedding. Other structures, apparently limited to either one or two types of dunes, are the concave-downward foresets in some parabolic dunes; the low-angle reverse dips of upwind strata on high transverse dunes; and the almost horizontal laminae which represent apparent dip in sections normal to wind direction in dome-shaped and transverse dunes. Describing cross-stratification in terms of three dimensions, dune structure at White Sands consists dominantly of the tabular planar sets, with units thickest near the dune base, thinner above. To a lesser extent the sets are of simple (non-erosion) tabular form and relatively uncommonly, of the trough type. Wedge planar forms are scarce. The planar forms characteristically are of two classes in nearly equal proportions: those in which bounding surfaces are virtually horizontal and those in which they dip at moderate to high degree. A brief comparison is made between the structures of dunes that are characteristic of one effective wind direction, as at White Sands, and certain others formed by winds of two or more directions. Seif dunes of Libya, reversing dunes of the San Luis Valley, Colorado, and star dunes in Saudi Arabia are discussed as examples of complex dunes formed by multi-directional winds.  相似文献   

6.
Xie  Liangfu  Ge  Ying  Zhang  Jiaqi  Tan  Shunli  Wang  Bo  Yan  Echuan  Qin  Yongjun  Wang  Jianhu  Shi  Chen  Yu  Guangming 《Natural Hazards》2021,106(3):1879-1894

This paper presents the analyses of toppling response of layered reverse-dip slopes under the influence of geometric factors of slope angle, strata thickness and dip. The toppling response of reverse-dip slopes under different geometric factors is obtained by using the discrete element code UDEC. Then, a prediction model for toppling deformation is developed by utilizing support vector machine and the toppling-prone combinations of these geometric factors are determined from a total of 120 samples of reverse-dip slopes. The study has shown that the geometric model is a quarter of a spheroid with a slope angle of 80°, a strata dip of 80°, and a strata thickness of 0.19 m as the center. The length of the long equatorial radius of the spheroid is 31° (strata dip axial), that of the short equatorial radius is 21° (slope angle axial), and the polar radius is 0.075 m (strata thickness axial). And the ratio of long equatorial radius, short equatorial radius, and polar radius is 2.48:1.68:1.00.

  相似文献   

7.
Aeolian dune interactions provide the dynamics for field‐scale pattern emergence and evolution within a set of boundary conditions. Although morphologies for a spectrum of dune interactions are recognized, associated stratigraphic architectures are unknown and have probably been misidentified in the rock record. A unique data set for the White Sands Dune Field in New Mexico (USA) allowed for a detailed analysis in which the morphological evolution of defect and bedform repulsion interactions is chronicled over a decadal time‐series of images and coupled with the resulting stratigraphic architecture, documented from cross‐strata exposed in interdune areas and ground‐penetrating radar imaging of dune interiors. Defect and bedform repulsions represent a class of interactions in which the faster‐migrating dune termination or defect (defect repulsion), or pair of defects (bedform repulsion), collides with the target dune downwind. Results document that during the collision, the defect(s) of the impactor dune recombine(s) with a segment of the target dune, and the redundant target dune segment is ejected as a parabolic‐shaped ejecta dune. The ejecta dune assumes a more barchanoid shape as it migrates downwind. The interaction architecture consists of lateral truncation of the target set by an interaction bounding surface. Defect cross‐strata tangentially approach the surface in plan‐view, and downlap onto the surface in cross‐section. The orientation of the defect cross‐strata is at an acute angle to the trend of the interaction surface. Orientations of the defect cross‐strata, which represent the defect approach angle, and the target dune cross‐strata, which represent the general dune migration direction, diverge at a high angle. Defect cross‐strata typically consist of wind‐ripple laminae, in contrast to the target set that may house grainflow cross‐strata. In the transport direction, the erosional interaction surface curves to become subparallel to subjacent and superjacent cross‐strata where the defect and target unify into a single lee face.  相似文献   

8.
Lacustrine environments are an excellent indicator of continental palaeoclimate. In particular, the sedimentary record of waves in lakes may be used to constrain atmospheric palaeocirculation. Wave ripples have been identified in a Permian lacustrine basin (the Salagou Formation, 260–250 Ma, Lodève Basin) located in the southern French Massif Central, part of the western European Hercynian mountain chain. Wave ripple patterns are interpreted with regards to hydrodynamics and water palaeodepth. It is shown that, in the case of the Salagou Formation, wave ripple orientations were controlled by the direction of the prevailing palaeowind. The Late Permian wind blew from between north and 20° east of north, possibly over several millions of years and certainly throughout the period of deposition of about 2000 m of strata in the Lodève Basin. Permian lacustrine sedimentation is widespread and well preserved on the Earth's surface and so wave ripple data may help constrain numerical modelling of the Earth's past climates, especially with regards to Permian times outside of desert regions.  相似文献   

9.
Mountney  & Howell 《Sedimentology》2000,47(4):825-849
Sets of aeolian cross‐strata within the Cretaceous Etjo Formation of NW Namibia are bounded by a hierarchy of surfaces, the origin of which are ascribed to one of four processes related to aeolian bedform and erg behaviour. The base of the main aeolian succession is characterized by a basin‐wide erosional supersurface that formed in response to a period of aeolian deflation before the onset of the main phase of erg building. Interdune migration surfaces formed by draa migration are planar in sections parallel to the palaeowind and are inclined at up to 5° in an upwind direction (SW). Perpendicular to the palaeowind, interdune surfaces form 500‐m‐wide troughs, signifying crestline sinuosity within the original bedforms. Superimposition surfaces are inclined at 5–10° in a downwind direction and indicate the migration of crescentic oblique dunes over larger, slipfaceless transverse draa. Reactivation surfaces associated with minor changes in dune slipface orientation are distinct from other bounding surface types because overlying cross‐strata lie parallel to them, rather than downlap onto them. Analysis of the geometry of these bounding surfaces, together with the orientation of the cross‐strata within the sets that they bound, has enabled the detailed morphology of the original bedforms to be reconstructed. The maximum preserved thickness of individual aeolian sets varies systematically across the basin, from 52 m in the basin depocentre to only 8 m at the basin margin. The set architecture indicates that this spatial variation is primarily the result of decreased angles of bedform climb at the basin margin, rather than the presence of smaller bedforms. Similarly, a temporal reduction in the angle‐of‐climb, rather than a reduction in bedform size, is considered to be responsible for an upward decrease in preserved set thickness. Reductions in bedform climb angle reflect progressive loss of accommodation space as the accumulating erg filled the basin.  相似文献   

10.
浙江省寿昌盆地火山沉积型硼异常特征   总被引：2，自引：0，他引：2  
在对浙江寿昌中生代火山沉积盆地寿昌组 (J3 s)地层进行的硼及相关多元素测试中 ,发现一处厚度大 ,层位稳定的较高含硼异常 ,钾、锂、铷、铯、砷、锑等含量亦高 ,与硼相关性好。经X射线衍射、能谱及电镜扫描等物性测试 ,初步确定存在独立的沉积型钙硼石类矿物 ,这为今后在该区寻找中生代火山沉积型硼矿奠定了良好的工作基础。  相似文献   

11.
本次研究在柴达木盆地旺尕秀地区上侏罗统红水沟组上覆地层中,首次发现了风成沉积。地层主体为一套棕黄色细-中砂岩,由分选、磨圆好的石英砂组成;扫描电镜下可见风成砂特有的碟形撞击坑和新月形撞击坑等特征;层内普遍发育风成大型高角度板状交错层理,层系厚度巨大,风成沙丘前积层特征明显;发育液化作用产生的牵引褶曲、倒转褶曲等常见的风成沙丘同沉积变形构造。根据岩性和沉积构造特征共在地层中识别出4种沉积亚相: 沙丘亚相、丘间亚相、旱谷亚相和沙漠湖亚相,其中沙丘亚相以风成大型交错层理为显著特征,丘间、旱谷和沙漠湖亚相则以水成沉积为主。风成砂沉积的存在丰富了柴达木盆地中生代的沉积类型,为区域地层对比及西北地区晚中生代古气候和古环境研究提供了新的证据和材料。  相似文献   

12.
《Sedimentology》2018,65(6):2034-2054
Grain flows are an integral part of sand dune migration; they are a direct response to the local wind regime and reflect complex interactions between localized over‐steepening of a dune slipface and complex turbulent airflow on the lee slope. Grain flows are primarily responsible for delivering sediment to the base of a dune, thus driving slipface advancement; yet, there are few constraints on their morphological and spatial characteristics or the amount of sediment that is redistributed by these flows. Using a combination of high‐resolution terrestrial laser scanning and video recordings, four distinct grain‐flow types are identified based on morphology and area on a dune slipface. Grain‐flow morphologies range from small, superficial flows to larger flows that affect greater portions of the slipface, moving significant amounts of sediment. Detailed field observations are presented of the dynamics of lee slopes, including measurements of the initiation location, thickness, magnitude and frequency statistics of grain flows, as well as volume estimates of redistributed sediment for each grain flow observed. High‐resolution laser scans enable accurate quantification of bulk sediment transfer from individual grain flows and can be used to study grain flows in a variety of environments. A categorization of grain‐flow morphologies is presented that links styles of flows with wind strength and direction, turbulent airflow, sediment deposition and environment.  相似文献   

13.
This paper reports on mathematical models of rock media processing and on their use in designing open pit coal mines. Spatial mathematical model of rock media was processed on a 25 km2 model site, incorporating 918 borehole logs. The model is capable of providing information concerning the geological structure of every point of the investigated area by plotting geological cross-sections along given lines or by plotting contour lines of the surface or the base for thickness of chosen lithological strata. The computation of one point of a grid involves the following steps: Borehole logs are numericaly coded. The geological structure at an arbitrarily chosen pointP is computed as follows. All borehole logs inside the circle (P; R) are used to compute theZ-coordinate of the ground atP by some interpolation formula chosen from those contained in the program system. Next, we check what stratum occurs topmost at boreholes inside the circle and which is most probable as the top stratumC 1 atP. TheZ-coordinate of theC 1 stratum surface atP is computed. Then what strata occur underC 1 stratum and which of them is the most probable stratumC 2 is determined. The process of computation is repeated until a sequence of strataC i atP andZ i coordinates of their surfaces is ascertained. The interpolation formulas included in the system are proper linear combination of PAF (polynomial approximations formulas, linear or quadratic and weighted) and WAF (weighted average formulas). Among the various interpolation formulas, some proved more useful for tectonic fault lines, others for ordinary sedimentary surfaces.  相似文献   

14.
滇西昌宁-孟连带南段组沉积特征及成因分析   总被引：2，自引：0，他引：2       下载免费PDF全文
南段组是一套厚度巨大的砂岩与泥岩的互层沉积,沉积构造主要是块状层理、水平层理和少量的小型滑动变形构造、小型斜层理和粒序层理以及浪成波痕。砂岩粒度概率累积曲线显示牵引流与重力流的过渡特征,砂岩的C-M图显示重力流沉积特征。砂岩成分成熟度高(石英>90%),结构成熟度中等(杂质为0-16%),有时出现沉积石英岩。砂岩和泥岩的地球化学特征表明是被动大陆边缘背景下的沉积。在南段组中新发现的Chondrites sp.,Scalarituba sp.,Phanolites sp.3种遗迹化石和一些原地埋藏的浅海底栖双壳类化石等,则代表了一个深陆棚沉积环境。以上特征表明南段组是一套浪控三角洲前缘斜坡-深陆棚环境的近源片泛性(非扇模式)重力流和正常陆棚的复合沉积,并非深海复理石建造。  相似文献   

15.
红土山盆地为大面积玄武岩覆盖区,其地球物理特征表现为中、强磁性、高密度。常规重、磁、电等地球物理方法很难取得较好的效果,故开展新方法、新技术以填补长白山玄武岩覆盖区及周边找矿空白,通过电磁勘探可获得研究区内地层电性结构,推断出新生代军舰山组玄武岩,中生代上统石人组和下统义和组沉积岩厚度变化规律、产状特征,及基岩起伏和构造分布情况,为该区成煤靶区的寻找提供了新的物探资料。  相似文献   

16.
本文以黄河边上现代不对称波痕的形成为例,结合民和盆地下白垩统第8岩组沉积环境进行类比分析,一改过去传统的"浅水"认识,而把它定为三角洲平原相沉积。因而不对称波痕不能作为某一种沉积环境,它可以广泛生成于不同的环境。因此应更多强调综合分析、类比分析、层序基本单元和体系域分析,使盆地岩石地层单位的古环境解释建立在可靠的理性基础上。  相似文献   

17.
金湖凹陷西斜坡阜二段湖相碳酸盐岩沉积模式研究   总被引：3，自引：0，他引：3  
前人对金湖凹陷西斜坡地区阜宁组阜二段湖相碳酸盐岩地层的成因认识不统一,因而本次研究以该层碳酸盐岩沉积相为重点,通过对研究区碳酸盐岩的成分组成、虫管保存程度、地层厚度分布规律、泥晶灰岩等的研究,提出研究区发育一套碳酸盐岩坪沉积体系。碳酸盐岩坪是一套静水环境下的泥晶灰岩和生物碎屑灰岩为主体的沉积体系,包含碳酸盐岩席、碳酸盐...  相似文献   

18.
A kinematic model for the structure of lee-side deposits   总被引：2，自引：0，他引：2  
A kinematic model for the structure of the lee-side deposit of a dune-like bedform, Gilbert-type delta, or similar step is developed, based on the assumptions that initial deposition is entirely by grainfall, that the rate of deposition decreases as a power function of distance downflow from the brink of the slipface, and that the resulting steepening of the slipface is periodically interrupted by avalanching. The parameters used in the model are: (1) the deposition rate at a given distance from the brink, (2) the exponent in the equation relating the deposition rate to distance from the brink, (3) the bedform migration rate, (4) the bedform height, (5) the avalanche speed, (6) the angle of initial yield, and (7) the residual angle after avalanching. From these parameters can be calculated structural characteristics such as the proportions of bottomset and foreset deposits, the proportions of avalanche and grainfall deposits in the foreset deposit, and the spacing of avalanche-grainfall couplets. The model correctly predicts the trends of changing avalanche activity and changing structural character with changes in flow character, grain size, and bedform height in both air and water. Moreover, the model correctly predicts certain consistent structural differences between aeolian and subaqueous lee-side deposits. Quantitative evaluation of the model requires more accurate data on the values of the input parameters than are presently available.  相似文献   

19.
Climbing‐ripple cross‐lamination is most commonly deposited by turbidity currents when suspended load fallout and bedload transport occur contemporaneously. The angle of ripple climb reflects the ratio of suspended load fallout and bedload sedimentation rates, allowing for the calculation of the flow properties and durations of turbidity currents. Three areas exhibiting thick (>50 m) sections of deep‐water climbing‐ripple cross‐lamination deposits are the focus of this study: (i) the Miocene upper Mount Messenger Formation in the Taranaki Basin, New Zealand; (ii) the Permian Skoorsteenberg Formation in the Tanqua depocentre of the Karoo Basin, South Africa; and (iii) the lower Pleistocene Magnolia Field in the Titan Basin, Gulf of Mexico. Facies distributions and local contextual information indicate that climbing‐ripple cross‐lamination in each area was deposited in an ‘off‐axis’ setting where flows were expanding due to loss of confinement or a decrease in slope gradient. The resultant reduction in flow thickness, Reynolds number, shear stress and capacity promoted suspension fallout and thus climbing‐ripple cross‐lamination formation. Climbing‐ripple cross‐lamination in the New Zealand study area was deposited both outside of and within channels at an inferred break in slope, where flows were decelerating and expanding. In the South Africa study area, climbing‐ripple cross‐lamination was deposited due to a loss of flow confinement. In the Magnolia study area, an abrupt decrease in gradient near a basin sill caused flow deceleration and climbing‐ripple cross‐lamination deposition in off‐axis settings. Sedimentation rate and accumulation time were calculated for 44 climbing‐ripple cross‐lamination sedimentation units from the three areas using TDURE, a mathematical model developed by Baas et al. (2000) . For Tc divisions and Tbc beds averaging 26 cm and 37 cm thick, respectively, average climbing‐ripple cross‐lamination and whole bed sedimentation rates were 0·15 mm sec?1 and 0·26 mm sec?1 and average accumulation times were 27 min and 35 min, respectively. In some instances, distinct stratigraphic trends of sedimentation rate give insight into the evolution of the depositional environment. Climbing‐ripple cross‐lamination in the three study areas is developed in very fine‐grained to fine‐grained sand, suggesting a grain size dependence on turbidite climbing‐ripple cross‐lamination formation. Indeed, the calculated sedimentation rates correlate well with the rate of sedimentation due to hindered settling of very fine‐grained and fine‐grained sand–water suspensions at concentrations of up to 20% and 2·5%, respectively. For coarser grains, hindered settling rates at all concentrations are much too high to form climbing‐ripple cross‐lamination, resulting in the formation of massive/structureless S3 or Ta divisions.  相似文献   

20.
位于印度板块北缘和雅鲁藏布江结合带之间的珠穆朗玛峰北坡地区，属于喜马拉雅造山带，是特提斯洋的重要组成部分。自奥陶纪至古近纪约5亿年期间发育一套基本连续的海相沉积，厚度达14 km，是研究特提斯洋形成演化的最佳地区。作者在对该区显生宙地层主干剖面和辅助剖面详细观察研究以及区域地质调查填图的基础上，将珠穆朗玛峰北坡地区显生宙沉积地层划分为海相、海陆过渡相和陆相3个沉积相组、15个沉积相和若干个沉积亚相。作者通过对该区沉积盆地的地层系统、沉积相、沉积特征的系统研究，将珠穆朗玛峰北坡地区显生宙沉积演化划分为6个阶段:1)奥陶纪-泥盆纪为稳定陆表海演化阶段；2)石炭纪-二叠纪为大陆裂谷盆地演化阶段；3)三叠纪-侏罗纪为被动大陆边缘盆地演化阶段；4)早中白垩世为前陆早期复理石盆地演化阶段；5)晚白垩世-古新世为前陆晚期磨拉石盆地演化阶段；6)古近纪-第四纪为造山隆升断陷盆地形成演化阶段。研究结果表明，珠穆朗玛峰北坡地区显生宙沉积盆地经历了由陆表海盆地-大陆裂谷盆地-被动大陆边缘盆地-前陆盆地-断陷盆地的演化过程。  相似文献   

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