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1.
The sedimentary infill history of the Madeira Abyssal Plain (MAP) is established from correlation of ODP Leg 157 drillsites (Sites 950–952) with an almost regular grid of 7000 km of intermediate-resolution seismic reflection profiles covering the central part of the abyssal plain. The most conspicuous seismic reflectors bounding the seismostratigraphic units have been identified and mapped. Correlation between seismic and borehole data using synthetic seismograms allows the lithological attribution and dating of the reflectors and seismostratigraphic units. Lateral mapping and correlation of seismic units also allows both the volumes and rates of accumulation of sediments within each seismostratigraphic unit and equivalent time periods of deposition to be determined. These calculations have been corrected for the effect of compaction, calculated at around 40% at the base of the drillholes. Three main turbidite types have been identified at the drillsites and their emplacement frequency has been calculated for each site and time period. Our results show that Cretaceous oceanic crust was draped with red pelagic clays, and the fracture-zone valleys were completely infilled and levelled in a geologically rather short time, probably during the latest Oligocene and Early Miocene, by organic-rich turbidites derived from the NW African continental margin. At 16 Ma, the topography was levelled enough to allow large turbidity current flows to cover the entire plain. During the Middle and Late Miocene (16–5.9 Ma), organic-rich turbidites were emplaced on the abyssal plain at a low rate of accumulation (12 m/my). In the uppermost Miocene–Early Pliocene (5.9–3.6 Ma), turbidite emplacement increased markedly in both frequency and accumulation rate (e.g., 26 m/my for organic-rich turbidites). During this time, period emplacement of volcanic-rich turbidites also increased in volume and frequency, a trend that continued into the Pliocene. Increased volcanic-rich turbidite emplacement correlates well with increased volcanic activity on the Canary Islands, and increased organic-rich turbidite emplacement may correlate with periods of erosion on the NW African continental margin. These erosional periods may be related to global cooling and falling sea level, intensification of bottom-water currents, and enhanced upwelling on the margin. 相似文献
2.
Seismic reflection profiles from the equatorial Atlantic off Africa between 12°N and 1°N reveal remarkably widespread deformation of oceanic sediments in an area lacking teleseismic activity. Uplift of abyssal plain sequences has occurred along the eastern extensions of large-offset fracture zones on the Mid-Atlantic Ridge. Between the major transforms pervasive deformation is imaged in the sedimentary column. Diapirism and faulting may have been associated with extensive fluid migration and sediment mobilization. The deformation occurred during the late Cenozoic and was probably related to reactivation of Cretaceous transforms. 相似文献
3.
A corridor 315 km wide centered along the southeast projection of the Atlantis fracture zone between 21°W and 29°W was investigated with seismic reflection, bathymetric, gravity, and magnetic profiles. Six sub-parallel, sediment-filled troughs in acoustic basement trend about 106° across the abyssal hills and lower continental rise off northwest Africa. Where the southernmost structural lineations cross the abyssal plain, they are interrupted by a ridge trending 080° surmounted by volcanic peaks.The structural lineations become less distinct landward of the western margin of the abyssal plain coincident with a decrease in topographic relief on acoustic basement and increasing sediment thickness. This transition is coincident with a reduction in the amplitude of gravity and magnetic anomalies. 相似文献
4.
莱州湾南岸平原浅埋古河道带研究 总被引：11，自引：1，他引：10
菜州湾海岸平原在埋深６０ｍ内的浅埋古河道带,可分弥河、潍河和白浪河３个系统,它们大都呈掌状、放射状分布,并与其所属诉冲洪积扇范围相吻合,该区古河道的形成和发育是新构造运动和古气候环境演变的结果。自晚更新世晚期以来,该区有６期古河道发育,其中玉木早冰期古河道和玉木主冰期古河道的砂体沉积粒度粗、连通性好、分布广,即是富水性强、水质好的淡水含水层,又是该区海（咸）水入侵的主要通道,控制在线积粒度粗、连通 相似文献
5.
Spectral analysis techniques have been applied to data sets of gravity and topography selected across fracture zones with large offset in the Equatorial and Central Atlantic Ocean and processed independently for each fracture zone. Three simple compensation models, two in local isostatic equilibrium (Airy I and II) and one in regional equilibrium (Plate model) have been tested. It is found that the free-air anomalies are primarily controlled by the topography and its isostatic response. For short wavelengths, admittance can be explained either by the effect of uncompensated sea floor topography with high density basement or by the effect of uncompensated sea floor topography with normal oceanic basement density but accompanied by a crust of constant thickness. For intermediate wavelengths, admittance for the Romanche fracture zone agrees best with a local isostatic model in which compensation is achieved by a less dense material in the upper mantle. No such evidence exists for the Vema and Chain fracture zones for which topography could just as well be regionally supported by an elastic plate 3 to 10 km thick. For longer wavelengths, the admittances computed for the three fracture zones are compatible with a thermal compensation of the topography. 相似文献
6.
Jacques Wannesson Monique Pelras Bernard Petitperrin Martine Perret Jacques Segoufin 《Marine and Petroleum Geology》1985,2(3):192-200
In 1982, a geophysical survey of the Antarctic margin, including multichannel seismic, gravity, magnetic and bathymetric surveying, was carried out off Adélie Coast-Wilkes Land and in the eastern Ross Sea. Of the 5000 km of lines recorded, 3000 km were in the Adélie Coast area. Lines ATC 101–102, approximately following meridian 138°E, show the first complete transect of the Adélie Coast margin from the Southeast Indian abyssal plain at DSDP Site 269 to the continental shelf. These lines reveal a thick sedimentary series divided into three main acoustic units by two major unconformities considered to be Upper Eocene (42 Ma) and late Oligocene (25 Ma). Oceanic or continental basement can be traced under the whole area, and the ocean-continent boundary clearly lies beneath the lower continental slope. A deep, high-amplitude, low-frequency horizon, extending under the oceanic basement for over 300 km of line, is considered to be the Moho. Our interpretation supports a recent revision be Cande and Mutter proposing an early Upper Cretaceous opening between Australia and East Antarctica. 相似文献
7.
Seismic reflection profiles from the northern end of Juan de Fuca Ridge reveal three axial valleys having a basement relief of as much as 2 sec (two-way travel time). A thick sequence, presumably of turbidites, mainly less than 0.7 m.y. old, covers much of the area. The oldest turbidites form the upper part of the fill of a possible Tertiary trench between the ridge and North America. The second turbidite unit extends beyond the trench and once formed an abyssal plain over most of northern Juan de Fuca Ridge and the area west to Explorer Ridge. Following formation of the plain, vertical movements began that broadly uplifted the crest of Juan de Fuca Ridge, block-faulted its northern end, produced faulting along Sovanco Fracture Zone, and upwarped the basement north of the ridge. Younger turbidites have filled the lowlands created by the vertical movements. The present sea floor topography and seismic activity show evidence of continued movements. 相似文献
8.
Abstract It is clear from morphology alone that distinctly different dynamic and sedimentary processes can be expected to be associated with the Greater Antilles Outer Ridge relative to those of the adjacent Nares Abyssal Plain. This difference is further substantiated by seismic reflection data which show the ridge to be a very large prism of acoustically transparent sediment in contrast to the stratified deposits of the abyssal plain. An examination of the geotechnical properties of the near‐surface (0 to 2.4m) deposits of the two areas also reveals distinct differences in their sedimentological characteristics. The outer ridge sediments, of more or less homogenous clay‐size material, display much higher water contents, porosities, sensitivities, plasticity, and organic carbon contents in contrast to the abyssal plain deposits which are much less homogenous owing to the presence of turbidite sequences. The turbidites themselves are uniquely contrasted to the other abyssal plain sediments by their higher silt content, wet bulk density, shear strength, and sensitivity. 相似文献
9.
南海西北部晚第四纪典型地震相—沉积相特征 总被引：1，自引：0，他引：1
南海西北部地形变化大,水深由近岸几十米变化至深海盆区的3 500m,跨越了陆架、陆坡、深海盆、岛礁等地貌单元。南海西北部也是深水油气的重要勘探地区。利用高分辨率单道地震资料,采用地震相分析方法,对研究区晚第四纪典型地震相—沉积相分布特征开展深入分析。研究区内的主要地震相包括：①席状、亚平行、强振幅、低连续、中频地震相;②披盖状、波状、中振幅、中—低连续、中低频地震相;③披盖状、平行—亚平行、中—弱振幅、中连续、中—低频地震相;④披盖状、平行、强振幅、高连续、中—高频地震相;⑤席状、平行、中—弱振幅、高连续、中—低频地震相;⑥披盖状、波状、弱振幅、低连续、低频地震相;⑦前积相;⑧下切充填地震相;⑨杂乱地震相;⑩条带状、波状、中—弱振幅、中—低连续、低频地震相;瑏瑡披盖状、平行、强振幅、高频、高连续地震相共11种。对地震相—沉积相及其分布特征的分析结果认为,区内晚第四纪主要发育有三角洲相、河道相、滨浅海相、浅海相、半深海相、深海相、滑塌相、斜坡相、浊流相、生物礁相等沉积相,其分布主要受海底地形地貌、构造运动等多种因素所控制。 相似文献
10.
侏罗纪洋壳为现存最古老的海洋地壳, 残留在地球表面上很少, 目前对于侏罗纪洋壳的断裂特征和构造变形了解很少。本文利用高分辨率的反射地震剖面精细解释了位于西太平洋的侏罗纪洋壳基底、沉积地层和断裂结构, 发现在研究区存在基底断层、沉积断层和垮塌断层三种类型的断裂构造, 并对其走向、倾角、断距等几何参数与变形特征进行了推测和定量研究。研究还发现, 基底断层是洋壳受到板块伸展拉张而产生的, 在后期海底沉积过程中持续发育并错断上覆沉积物, 在海底形成明显的断层陡坎。沉积断层是沉积地层自身重力作用的产物,受到沉积地层岩石性质的控制。垮塌断层是岩浆侵出或者侵入形成海山, 导致洋壳及其上覆沉积局部抬升并向两侧推移, 引起先存的基底断层和沉积断层重新错动产生的。研究区内切断洋壳基底和上覆沉积的活动断层的推测走向大体符合侏罗纪洋壳基底面起伏、重力异常骤变界面以及地磁异常条带等的走向, 表明这些断裂从侏罗纪洋中脊的海底扩张中演变而来, 并且持续活动至今。这些发育在古老洋壳上的断层能够长时间让水进入岩石圈并进入俯冲带及地球内部, 从而促进地球水循环。尽管目前尚未发现这些断裂产生大地震, 但这些断层可能随着板块俯冲而演变成俯冲带地震大断裂, 今后研究应该关注这类断层在靠近海沟之前的演化规律和潜在地震风险。 相似文献
11.
The External Calabrian Arc is located off the convex side of the Calabro-Peloritanian Arc in the northern Ionian Sea. A systematic reflection seismic survey indicates that it is made of different structural elements whose characters seem consistent with an active accretionary margin. The main structures are the Crotone-Spartivento slope (comparable to an inner trench slope) and the intermediate depressions (comparable to a trench area). Internal to these elements, the Crotone-Spartivento basin may represent a fore-arc basin. This partly outcrops in Calabria and its structure suggests that the accretionary margin developed at least since middle-upper Miocene.Subduction processes do not affect a true oceanic crust, because of the great thickness of sediments covering the whole eastern Mediterranean. Hence some peculiar features occur in the system. as the cobblestone topography, or are lacking, as a typical and continuous trench zone.In the areas with cobblestone topography we distinguish a Calabrian Ridge sensu stricto from a Calabrian Ridge sensu lato. The former is a N-S trending swell, external to the supposed trench zone, interpreted as a sedimentary outer-arc ridge produced by rather surficial tectonic accumulation of sediments further chaoticized by gravitative mechanisms. The Ridge s.l. is a very wide area with low relief and little or no seismic penetration. Tectonization seems gentler than in the Ridge s.s. and structural axes seem to possess different orientations. These areas are interpreted as due to a widespread surficial chaoticization above presumed decollement layers occurring within the sedimentary column of the Ionian bathyal plain.The pattern of deformations of the Calabrian Ridge seems consistent with the Calabro-Peloritanian Arc actively overriding the eastern Mediterranean, with a resultant direction of movement essentially towards the East. 相似文献
12.
Chun-Feng Li Zuyi Zhou Jiabiao Li Bing Chen Jianhua Geng 《Marine Geophysical Researches》2008,29(4):223-238
We made a systematic investigation on major structures and tectonic units in the South China Sea basin based on a large magnetic
and seismic data set. For enhanced magnetic data interpretation, we carried out various data reduction procedures, including
upward continuation, reduction to the pole, 3D analytic signal and power spectrum analyses, and magnetic depth estimation.
Magnetic data suggest that the South China Sea basin can be divided into five magnetic zones, each with a unique magnetic
pattern. Zone A corresponds roughly to the area between Taiwan Island and a relict transform fault, zone B is roughly a circular
feature between the relict transform fault and the northwest sub-basin, and zones C, D, and E are the northwest sub-basin,
the east sub-basin, and the southwest sub-basin, respectively. This complexity in basement magnetization suggests that the
South China Sea evolved from multiple stages of opening under different tectonic settings. Magnetic reduction also fosters
improved interpretation on continental margin structures, such as Mesozoic and Cenozoic sedimentary basins and the offshore
south China magnetic anomaly. We also present, for the first time, interpretations of three new 2D reflection seismic traverses,
which are of ~2,000 km in total length and across all five magnetic zones. Integration of magnetic and seismic data enables
us to gain a better 3D mapping on the basin structures. It is shown that the transition from the southwest sub-basin to the
east sub-basin is characterized by a major ridge formed probably along a pre-existing fracture zone, and by a group of primarily
west-dipping faults forming an exact magnetic boundary between zones D and E. The northwest sub-basin has the deepest basement
among the three main sub-basins (i.e., the northwest sub-basin, the southwest sub-basin, and the east sub-basin). Our seismic
data also reveal a strongly faulted continent–ocean transition zone of about 100 km wide, which may become wider and dominated
with magmatism or transit to an oceanic crust further to the northeast. 相似文献
13.
渤海莱州湾南岸平原浅埋古河道带及其与海(咸)水入侵关系研究 总被引：2，自引：0，他引：2
根据2100余个钻孔资料,并结合大比例尺地形图、航片、卫片判读分析,以及野外实地考察和沉积物样品的粒度分析、岩相分析、14C测年,研究了莱州湾南岸平原浅埋古河道带的分布规律、埋藏和沉积特征、古河道的分期断代以及与海(咸)水入侵关系。该区在埋深60m内的浅埋古河道带,可分成弥河、潍河和白浪河3个系统,它们大都呈掌状、放射状分布,并与其所属河流的冲洪积扇范围相吻合。该区古河道的形成和发育与古气候和海平面变化密切相关。自晚更新世晚期以来,该区有4期古河道发育,其中玉木旱冰期古河道和玉术主冰期古河道的砂层沉积粒度粗、连通性好、分布广,既是富水性强、水质好的淡水含水层,又是该区海(咸)水入侵的主要通道。控制在浅埋古河道带超采地下淡水,并在丰水季节利用其进行地下水回灌,是治理该区海(咸)水入侵灾害的重要措施之一。 相似文献
14.
K. Solli B. Kuvaas Y. Kristoffersen G. Leitchenkov J. Guseva V. Gandjukhin 《Marine Geophysical Researches》2007,28(1):43-57
Multichannel seismic data from the eastern parts of the Riiser-Larsen Sea have been analyzed with a sequence stratigraphic
approach. The data set covers a wide bathymetric range from the lower continental slope to the abyssal plain. Four different
sequences (termed RLS-A to RLS-D, from deepest to shallowest) are recognized within the sedimentary section. The RLS-A sequence
encompasses the inferred pre-glacial part of the deposits. Initial phases of ice sheet arrival at the eastern Riiser-Larsen
Sea margin resulted in the deposition of multiple debris flow units and/or slumps on the upper part of the continental rise
(RLS-B). The nature and distribution of these deposits indicate sediment supply from a line or a multi-point source. The subsequent
stage of downslope sediment transport activity was dominated by turbidity currents, depositing mainly as distal turbidite
sheets on the lower rise/abyssal plain (RLS-C). We attribute this to margin progradation and/or a more focussed sediment delivery
to the continental shelf edge. As the accommodation space on the lower rise/abyssal plain declined and the base level was
raised, the turbidite channels started to backstep and develop large channel–levee complexes on the upper parts of the continental
rise (RLS-D). The deposition of various drift deposits on the lower rise/abyssal plain and along the western margin of the
Gunnerus Ridge indicates that the RLS-D sequence is also associated with increased activity of contour currents. The drift
deposits overlie a distinct regional unconformity which is considered to reflect a major paleoceanographic event, probably
related to a Middle Miocene intensification of the Antarctic Circumpolar Current. 相似文献
15.
Structure of the basins of the White Sea rift systems 总被引：1，自引：0，他引：1
For the first time, the structure of the sedimentary basins of the Late Proterozoic rift system in the White Sea is characterized based on a set of new marine geological geophysical data such as the results of the common depth point seismic method, gravity and magnetic data, and seismoacoustics. The main tectonic structures in the topography of the heterogeneous basement within the basin of the White Sea are distinguished and described. A structural tectonic scheme of the basement surface is presented. The thicknesses of the sediments are estimated and the stratigraphic confinement of the seismic units recognized is done. 相似文献
16.
G. Jané A. Maestro G. Ercilla J. López-Martínez J.R. De Andrés D. Casas D. González-Aller M. Catalán-Morollón 《Marine and Petroleum Geology》2010
A total of 445 pockmarks were observed on the upper continental slope of the northwest corner of the Iberian Peninsula (the Ortegal Spur area) by swath bathymetric and ultrahigh resolution seismic data. The pockmarks are U-, V- and W-shaped and have terraces or indentations in cross-section, and are dish-shaped (circular to oval) in plan view. They occur on the surface of the seabed and buried within the Plio-Quaternary and Neogene sediments. Four types of pockmarks were identified and mapped on the basis of their plan-view and cross-section morphology: regular, irregular, asymmetric and composite. The concentration of pockmarks is attributed to seepage of fluids migrating up-dip from deeper parts of the sedimentary basin. A linear high-density concentration with a NNW to N, NE and ESE trend of pockmarks is observed above inferred basement faults that do not affect the Quaternary succession. These pockmarks are thus caused by seepage of thermogenic gas and/or other pore fluids from deeper Late Cretaceous units, and their distribution may help to improve our understanding of the fluid system and migration regime in this part of the Galicia continental margin. 相似文献
17.
The 1994 Tasmante swath-mapping and reflection seismic cruise covered 200 000 km2 of sea floor south and west of Tasmania. The survey provided a wealth of morphological, structural and sedimentological information, in an area of critical importance in reconstructing the break-up of East Gondwana.The west Tasmanian margin consists of a non-depositional continental shelf less than 50 km wide and a sedimented continental slope about 100 km wide. The adjacent 20 km of abyssal plain to the west is heavily sedimented, and beyond that is lightly sedimented Eocene oceanic crust formed as Australia and Antarctica separated. The swath data revealed systems of 100 m-deep downslope canyons and large lower-slope fault-blocks, striking 320° and dipping landward. These continental blocks lie adjacent to the continent ocean boundary (COB) and are up to 2500 m high and have 15°–20° scarps.The South Tasman Rise (STR) is bounded to the west by the Tasman Fracture Zone extending south to Antarctica. Adjacent to the STR, the fracture zone is represented by a scarp up to 2000 m high with slopes of 15–20°. The scarp consists of continental faultblocks dipping landward. Beyond the scarp to the west is a string of sheared parallel highs, and beyond that is lightly sedimented Oligocene oceanic crust 4200–4600 m deep with distinct E-W spreading fabric. The eastern margin of the bathymetric STR trends about 320° and is structurally controlled. The depression between it and the continental East Tasman Plateau (ETP) is heavily sedimented; its western part is underlain by thinned continental crust and its central part by oceanic crust of Late Cretaceous to Early Tertiary age. The southern margin of the STR is formed by N-S transform faults and south-dipping normal faults.The STR is cut into two major terrains by a N-S fracture zone at 146°15E. The western terrain is characterised by rotated basement blocks and intervening basins mostly trending 270°–290°. The eastern terrain is characterised by basement blocks and intervening strike-slip basins trending 300°–340°. Recent dredging of basement rocks suggests that the western terrain has Antarctic affinities, whereas the eastern terrain has Tasmanian affinities.Stretching and slow spreading between Australia and Antarctica was in a NW direction from 130–45 Ma, and fast spreading was in a N-S direction thereafter. The western STR terrain was attached to Antarctica during the early movement, and moved down the west coast of Tasmania along a 320° shear zone, forming the landward-dipping continental blocks along the present COB. The eastern terrain either moved with the western terrain, or was welded to it along the 146°15 E fracture zone in the Early Tertiary. At 45 Ma, fast spreading started in a N-S direction, and after some probable movement along the 146°15E fracture zone, the west and east STR terrains were welded together and became part of Australia. 相似文献
18.
Audun Libak Rolf Mjelde Henk Keers Jan Inge Faleide Yoshio Murai 《Marine Geophysical Researches》2012,33(2):185-207
This paper describes results from a geophysical study in the Vestbakken Volcanic Province, located on the central parts of the western Barents Sea continental margin, and adjacent oceanic crust in the Norwegian-Greenland Sea. The results are derived mainly from interpretation and modeling of multichannel seismic, ocean bottom seismometer and land station data along a regional seismic profile. The resulting model shows oceanic crust in the western parts of the profile. This crust is buried by a thick Cenozoic sedimentary package. Low velocities in the bottom of this package indicate overpressure. The igneous oceanic crust shows an average thickness of 7.2 km with the thinnest crust (5–6 km) in the southwest and the thickest crust (8–9 km) close to the continent-ocean boundary (COB). The thick oceanic crust is probably related to high mantle temperatures formed by brittle weakening and shear heating along a shear system prior to continental breakup. The COB is interpreted in the central parts of the profile where the velocity structure and Bouguer anomalies change significantly. East of the COB Moho depths increase while the vertical velocity gradient decreases. Below the assumed center for Early Eocene volcanic activity the model shows increased velocities in the crust. These increased crustal velocities are interpreted to represent Early Eocene mafic feeder dykes. East of the zone of volcanoes velocities in the crust decrease and sedimentary velocities are observed at depths of more than 10 km. The amount of crustal intrusions is much lower in this area than farther west. East of the Kn?legga Fault crystalline basement velocities are brought close to the seabed. This fault marks the eastern limit of thick Cenozoic and Mesozoic packages on central parts of the western Barents Sea continental margin. 相似文献
19.
The peculiarities of the microseisms spectra shape when recording on the ocean floor in the frequency band of 0.003–20 Hz are examined. The origin of the stable minima in the microseisms spectrum (“transparency windows”) at frequencies of about 0.02–0.1 Hz and 5–15 Hz is analyzed. In these frequency bands, weak earthquake signals are recorded by bottom instruments. The origin of the low-frequency “transparency windows” can be explained by the conditions of the microseisms propagation in the oceanic waveguide (between the bottom and the water’s surface) in the abyssal plain zones. The results of the full-waveform numerical simulation of the seismoacoustic waves propagation in the oceanic environment and on the ocean-continent border are presented, and the experimental data as well. The peculiarities of the microseisms spectra in the band of high-frequency “transparency windows” can be caused by the constructive resonance in the water-saturated layer of bottom sediments. The theoretical foundation and experimental results are given. 相似文献
20.
The Eastern Mediterranean Sea is a remnant of a deep Mesozoic oceanic basin, now almost totally consumed as a result of long-term
plate convergence between Eurasia and Africa. The present-day surface morphology of the Eastern Mediterranean relates both
to the early history of formation of the deep basins and the recent geodynamic interactions between interfering microplates.
Among the most conspicuous morphologic features of the basin is an arc-shape, elongated and wide, bathymetric swell bisecting
the entire basin from the Ionian to Levantine areas, known as the Mediterranean Ridge. During the last decade this tectono-sedimentary
accretionary prism, which results from the Hellenic subduction, has been intensively surveyed by swath mapping, multichannel
seismic profiling and deep dives. We present here, and briefly discuss, the main morphological characteristics of this feature
as derived from swath bathymetric data that considerably help to better assess the lateral and north–south morphostructural
variability of the Mediterranean Ridge. This study reveals that the characteristics and morphostructural variability of the
Mediterranean Ridge are related to: (1) a specific incipient collision geodynamic setting south of Crete, where the African
and Aegean continental margins are nearly in contact, (2) a unique regional kinematics, controlled by frontal convergence
south of Crete (central Mediterranean Ridge) and oblique subduction with opposite sense of shear for the western (Ionian)
and eastern (Levantine) domains of the Mediterranean Ridge, that explain the lateral variations of deformation and (3) particularities
of its sedimentary cover, which includes massive salt layers within the outer Mediterranean Ridge and local salt deposits
within the inner domains, that control the north–south morphostructural variability of the sedimentary wedge. 相似文献