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Accretionary wedge

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pressure (source terms) and those that limit flow (permeability and drainage path length). Sediment permeability and incoming sediment thickness are the most important factors, whereas fault permeability and the partitioning of sediment have a small effect. In one such study, it was found that as sediment permeability is increased, pore pressure decreases from near-lithostatic to hydrostatic values and allows stable taper angles to increase from ~2.5° to 8°–12.5°. With increased sediment thickness (from 100–8,000 m (330–26,250 ft)), increased pore pressure drives a decrease in stable taper angle from 8.4°–12.5° to <2.5–5°. In general, low-permeability and thick incoming sediment sustain high pore pressures consistent with shallowly tapered geometry, whereas high-permeability and thin incoming sediment should result in steep geometry. Active margins characterized by a significant proportion of fine-grained sediment within the incoming section, such as northern
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overpressured fluid. Dilatant fracturing will create escape routes, so the fluid pressure is likely to be buffered at the value required for the transition between shear and oblique tensile (dilatant) fracture, which is slightly in excess of the load pressure if the maximum compression is nearly horizontal. This in turn buffers the strength of the wedge at the cohesive strength, which is not pressure-dependent, and will not vary greatly throughout the wedge. Near the wedge front the strength is likely to be that of the cohesion on existing thrust faults in the wedge. The shear resistance on the base of the wedge will also be fairly constant and related to the cohesive strength of the weak sediment layer that acts as the basal detachment. These assumptions allow the application of a simple plastic continuum model, which successfully predicts the observed gently convex taper of accretionary wedges.
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margin of North America. This process formed a stacking sequence in which the structurally highest rocks (on the east) are the oldest, and in which each major thrust wedge to the west becomes younger. Within each of the terrane blocks, however, the rocks become younger upsection, but the sequence may be repeated multiple times by thrust faults.
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basement, where imaged, appears to diverge from the sedimentary package, dipping under the wedge while the overlying sediments are often lifted up against it. Backthrusting may be favored where relief is high between the crest of the wedge and the surface of the forearc basin because the relief must be supported by
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of accretionary wedges dip back toward the arc, and that accreted material is emplaced below such backstops, is contradicted by observations from many active forearcs that indicate (1) backthrusting is common, (2) forearc basins are nearly ubiquitous associates of accretionary wedges, and (3) forearc
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in Italy are largely an accretionary wedge formed as a consequence of subduction. This region is tectonically and geologically complex, involving both subduction of the Adria micro-plate beneath the Apennines from east to west, continental collision between the Eurasia and Africa plates building the
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range in age from about 200 million to 80 million years old. The Franciscan Complex is composed of a complex amalgamation of semi-coherent blocks, called tectonostratigraphic terranes, that were episodically scraped from the subducting oceanic plate, thrust eastward, and shingled against the western
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of the South China Sea slope. The existence of the South China Sea slope also leads the strike of impinging folds with NNW-trend to turn more sharply to a NE-strike, parallel to strike of the South China Sea slope. Analysis shows that the pre-orogenic mechanical/crustal heterogeneities and seafloor
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margin, suggesting that pre-orogenic sediment thickness is the major control on the geometry of frontal structures. The preexisting South China Sea slope that lies obliquely in front of the advancing accretionary wedge has impeded the advancing of frontal folds resulting in a successive termination
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is dominated by two major lithologic units, the Valdez Group (Late Cretaceous) and the Orca Group (Paleocene and Eocene). The Valdez Group is part of a 2,200-km-long by 100-km-wide belt of Mesozoic accretionary complex rocks called the Chugach terrane. This terrane extends along the Alaska coastal
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and trench rollback of the Ionian basin under Eurasia, causing the opening of the Liguro-Provençal and Tyrrhenian back-arc basins and the formation of the Calabrian accretionary wedge. The Calabrian accretionary wedge is a partially submerged accretionary complex located in the Ionian offshore and
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as critically tapered wedges of sediment demonstrate that pore pressure controls their taper angle by modifying basal and internal shear strength. Results from some studies show that pore pressure in accretionary wedges can be viewed as a dynamically maintained response to factors which drive pore
188:, are transported toward the subduction zone and accreted to the continental margin. Since the Late Devonian and Early Carboniferous periods, some 360 million years ago, subduction beneath the western margin of North America has resulted in several collisions with terranes, each producing a 388:
Rapid tectonic loading of wet sediment in accretionary wedges is likely to cause the fluid pressure to rise until it is sufficient to cause dilatant fracturing. Dewatering of sediment that has been underthrust and accreted beneath the wedge can produce a large steady supply of such highly
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The topographic expression of the accretionary wedge forms a lip, which may dam basins of accumulated materials that, otherwise, would be transported into the trench from the overriding plate. Accretionary wedges are the home of
329:, are preserved on land. They provide a valuable natural laboratory for studying the composition and character of the oceanic crust and the mechanisms of their emplacement and preservation on land. A classic example is the 1043:
Nemcok, M., Coward, M. P., Sercombe, W. J. and Klecker, R. A., 1999: Structure of the West Carpathian Accretionary Wedge: Insights from Cross Section Construction and Sandbox Validation. Phys. Chem. Earth (A), 24, 8, pp.
385:, have steep taper angles. Observations from active margins also indicate a strong trend of decreasing taper angle (from >15° to <4°) with increased sediment thickness (from <1 to 7 km). 961:
Jones, D.L., Siberling, N.J., Coney, P.J., and Monger, J.W.H., 1987, Lithotectonic terrane map of Alaska (west of the 141st meridian): U.S. Geological Survey Miscellaneous Field Studies Map MF 1847-A.
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Tsang, Man-Yin; Bowden, Stephen A.; Wang, Zhibin; Mohammed, Abdalla; Tonai, Satoshi; Muirhead, David; Yang, Kiho; Yamamoto, Yuzuru; Kamiya, Nana; Okutsu, Natsumi; Hirose, Takehiro (February 1, 2020).
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Saffer, D. M., and B. A. Bekins (2006), An evaluation of factors influencing pore pressure in accretionary complexes: Implications for taper angle and wedge mechanics, J. Geophys. Res., 111, B04101,
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are not equivalent to tectonic plates, but rather are associated with tectonic plates and accrete as a result of tectonic collision. Materials incorporated in accretionary wedges include:
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Schrader, F.C., 1900, A reconnaissance of a part of Prince William Sound and the Copper River District, Alaska, in 1898: U.S. Geological 20th Anniversary Report, pt. 7, p. 341–423.
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Fruehn, J., R. von Huene, and M. Fisher (1999), Accretion in the wake of terrane collision: The Neogene accretionary wedge off Kenai Peninsula, Alaska, Tectonics, 18(2), 263–277.
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Period, roughly 170 million years ago, in an extensional regime within either a back-arc or a forearc basin. It was later accreted to the continental margin of Laurasia.
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Backthrusting of the rear of the accretionary wedge, arcward over the rocks of the forearc basin, is a common aspect of accretionary tectonics. An older assumption that
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Material exposed in the forearc ridge may include fragments of oceanic crust or high pressure metamorphic rocks thrust from deeper in the subduction zone.
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Pelayo, A., and D. Wiens (1992), Tsunami Earthquakes: Slow Thrust-Faulting Events in the Accretionary Wedge, J. Geophys. Res., 97(B11), 15321–15337.
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event. The piecemeal addition of these accreted terranes has added an average of 600 km (370 mi) in width along the western margin of the
1018: 554:. This wedge incorporates sediment eroded from the continental margin and marine sediments carried into the subduction zone on the Pacific plate. 452:. In recent years, this is the site of attention for studying the temperature of subseafloor life and underground hot fluids in subducting zones. 340:
Longitudinal sedimentary tapering of pre-orogenic sediments correlates strongly with curvature of the submarine frontal accretionary belt in the
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A Seismic Sequence from Northern Apennines (Italy) Provides New Insight on the Role of Fluids in the Active Tectonics of Accretionary Wedges.
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of California, which is one of the most extensive ophiolite terranes in North America. This oceanic crust likely formed during the middle
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In accretionary wedges, seismicity activating superimposed thrusts may drive methane and oil upraising from the upper crust.
314: 231: 524:. The Orca Group is part of an accretionary complex of Paleogene age called the Prince William terrane that extends across 1116: 630: 550:. During the Neogene the terrane's western part was subducted after which a sediment wedge accreted along the northeast 1754: 1074: 798:
Platt, J. (1990), Thrust Mechanics in Highly Overpressured Accretionary Wedges, J. Geophys. Res., 95(B6), 9025–9034.
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is a current (in modern use) or former accretionary wedge. Accretionary complexes are typically made up of a mix of
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have resulted from rupture through the sedimentary rock along the basal decollement of an accretionary wedge.
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are formed with the youngest most outboard structures progressively uplifting the older more inboard thrusts.
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Minelli, L. and C. Faccenna (2010), Evolution of the Calabrian accretionary wedge (central Mediterranean),
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Silver, E., and D. Reed (1988), Backthrusting in Accretionary Wedges, J. Geophys. Res., 93(B4), 3116–3126.
731: 613: 577: 562: 378: 267:, intensely deformed packages of rocks that lack coherent internal layering and coherent internal order. 1698: 1502: 1391: 1261: 1241: 1141: 1111: 558: 382: 330: 297:. Once the wedge reaches a critical taper, it will maintain that geometry and grow only into a larger 1675: 1559: 1276: 1231: 931: 864: 743: 525: 497: 445: 432: 361: 270:
The internal structure of an accretionary wedge is similar to that found in a thin-skinned foreland
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Piggy-back basins, which are small basins located in surface depression on the accretionary prism.
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Alpine mountain belt further to the north and the opening of the Tyrrhenian basin to the west.
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located in Washington State. The mountains began to form about 35 million years ago when the
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The small sections of oceanic crust that are thrust over the overriding plate are said to be
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The sediments accreted onto the non-subducting tectonic plate at a convergent plate boundary
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Pelagic sediments – typically immediately overlying oceanic crust of the subducting plate
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morphology exert strong controls on the thrust-belt development in the incipient Taiwan
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The shape of the wedge is determined by how readily the wedge will fail along its basal
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Lin, Andrew T.; Liu, Char-Shine; Lin, Che-Chuan; et al. (December 5, 2008).
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Material transported into the trench by gravity sliding and debris flow from the
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Ocean-floor basalts – typically seamounts scraped off the subducting plate
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Davis, George H. Structural Geology of Rocks and Regions. (1996). pp583.
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thin-skinned zone of Carpathian thrustbelt, which is thrust over the
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Calderoni, Giovanna et al. Earth and Planetary Science Letters.
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Calabrian Accretionary Wedge in the Central Mediterranean – The
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Adjacent continental masses located along strike (such as
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laterally bounded by the Apulia and Malta escarpments.
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Volume 281, Issues 1-2, April 30, 2009, pages 99–109.
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Archived from 994:"Geology of the Golden Gate Headlands" 120:Materials within an accretionary wedge 116:is made up of accretionary complexes. 7: 232:adding citations to reliable sources 1332:List of tectonic plate interactions 25: 124:Accretionary wedges and accreted 1750: 1749: 208: 78:formed on the overriding plate. 1060:United States Geological Survey 1019:"Magnitude 6.3 - CENTRAL ITALY" 878:10.1016/j.marpetgeo.2019.104080 467:BahĂ­a Mansa Metamorphic Complex 219:needs additional citations for 679:. Britannica. January 22, 2014 176:such as linear island chains, 1: 532:area, underlying much of the 360:Mechanical models that treat 138:Trench sediments – typically 857:Marine and Petroleum Geology 756:10.1016/j.margeo.2008.10.002 631:Subduction zone metamorphism 172:Elevated regions within the 145:Oceanic, volcanic island arc 838:10.14379/iodp.proc.370.2017 442:Nankai accretionary complex 345:of folds against and along 108:. For example, most of the 1792: 448:is subducting beneath the 274:belt. A series of thrusts 1745: 1417:Thick-skinned deformation 476:tectonics of the central 142:that may be derived from: 89:of terrestrial material, 64:convergent plate boundary 1422:Thin-skinned deformation 1198:Stereographic projection 1188:Orthographic projection 1171:Measurement conventions 1117:LamĂ©'s stress ellipsoid 999:. National Park Service 542:accretionary wedge off 509:Chugach National Forest 465:between 38°S and 43°S ( 417:Currently active wedges 614:East European Platform 578:Carpathian Flysch Belt 457:Exhumed ancient wedges 435:is subducting beneath 408:along the backthrust. 362:accretionary complexes 318: 37: 1699:Paleostress inversion 1392:Strike-slip tectonics 1262:Extensional tectonics 1242:Continental collision 1112:Deformation mechanism 657:on September 16, 2016 528:westward through the 507:– The geology of the 331:Coast Range ophiolite 312: 35: 1277:Fold and thrust belt 919:10.1029/2009TC002562 787:10.1029/2005JB003990 559:Franciscan Formation 526:Prince William Sound 503:Kodiak Shelf in the 498:North American Plate 446:Philippine Sea Plate 433:South American Plate 313:Accretionary wedge ( 228:improve this article 162:ridge (olistostrome) 83:accretionary complex 1709:Section restoration 1585:Rock microstructure 1247:Convergent boundary 1147:Strain partitioning 1132:Overburden pressure 1122:Mohr–Coulomb theory 932:"Olympic Mountains" 869:2020MarPG.11204080T 748:2008MGeol.255..186L 522:southwestern Alaska 480:are related to the 463:Chilean Coast Range 423:Mediterranean Ridge 291:pore fluid pressure 110:geological basement 1686:Kinematic analysis 1342:Mountain formation 1257:Divergent boundary 1222:Accretionary wedge 1098:Structural geology 992:Elder, William P. 494:Juan de Fuca Plate 319: 46:accretionary prism 42:accretionary wedge 38: 18:Accretionary prism 1763: 1762: 1694:3D fold evolution 1580:Pressure solution 1575:Oblique foliation 1455:Exfoliation joint 1445:Columnar jointing 1105:Underlying theory 1025:on April 14, 2010 709:"Plate Tectonics" 677:"Deep-sea Trench" 534:continental shelf 490:Olympic Mountains 260: 259: 252: 190:mountain-building 182:crustal fragments 16:(Redirected from 1783: 1753: 1752: 1498:Detachment fault 1493:Cataclastic rock 1427:Thrust tectonics 1397:Structural basin 1372:Pull-apart basin 1312:Horst and graben 1091: 1084: 1077: 1068: 1045: 1041: 1035: 1034: 1032: 1030: 1015: 1009: 1008: 1006: 1004: 998: 989: 983: 980: 974: 968: 962: 959: 953: 950: 944: 943: 941: 939: 928: 922: 907: 901: 900: 890: 880: 848: 842: 841: 823: 817: 814: 808: 805: 799: 796: 790: 779: 773: 766: 760: 759: 742:(3–4): 186–203. 727: 721: 720: 718: 716: 704: 698: 695: 689: 688: 686: 684: 673: 667: 666: 664: 662: 653:. 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487: 483: 479: 478:Mediterranean 475: 471: 468: 464: 461: 460: 456: 451: 447: 443: 440: 438: 434: 430: 427: 424: 421: 420: 416: 411: 409: 407: 402: 397: 395: 390: 386: 384: 380: 376: 372: 368: 363: 358: 355: 353: 352:arc-continent 348: 343: 338: 336: 332: 328: 324: 316: 311: 304: 302: 300: 296: 292: 288: 283: 281: 277: 273: 268: 266: 254: 251: 243: 233: 229: 223: 222: 217:This section 215: 211: 206: 205: 199: 197: 195: 191: 187: 183: 179: 175: 167: 164: 161: 157: 154: 150: 147: 144: 141: 137: 134: 131: 130: 129: 127: 119: 117: 115: 111: 107: 104: 100: 96: 92: 88: 84: 79: 77: 73: 72:oceanic crust 69: 65: 61: 58: 55:onto the non- 54: 51: 47: 43: 34: 30: 19: 1523:Thrust fault 1221: 1212:Large-scale 1183:Inclinometer 1157:Stress field 1059: 1039: 1027:. Retrieved 1023:the original 1013: 1001:. Retrieved 987: 978: 966: 957: 948: 936:. Retrieved 934:. Britannica 926: 910: 905: 860: 856: 846: 828: 821: 812: 803: 794: 777: 769: 764: 739: 735: 725: 713:. Retrieved 711:. Britannica 702: 693: 681:. Retrieved 671: 659:. Retrieved 655:the original 645: 536:to the west 518:Sanak Island 406:shear stress 398: 391: 387: 369:and eastern 359: 356: 339: 320: 305:Significance 284: 278:towards the 269: 261: 246: 237: 226:Please help 221:verification 218: 180:, and small 178:ocean ridges 174:ocean basins 171: 123: 82: 80: 45: 41: 39: 29: 1704:Paleostress 1590:Slickenside 1565:Crenulation 1518:Fault trace 1513:Fault scarp 1503:Disturbance 1488:Cataclasite 1377:Rift valley 1297:Half-graben 1267:Fault block 1252:DĂ©collement 1029:January 14, 1003:January 14, 938:January 14, 715:January 14, 683:January 14, 287:decollement 240:August 2021 196:continent. 103:hemipelagic 95:ocean floor 76:island arcs 48:forms from 1776:Subduction 1732:Pure shear 1719:Shear zone 1676:Competence 1560:Compaction 1437:Fracturing 1232:Autochthon 1227:Allochthon 888:2164/13157 863:: 104080. 661:August 12, 637:References 602:Cretaceous 600:represent 482:subduction 450:Amur Plate 327:ophiolites 140:turbidites 87:turbidites 57:subducting 1668:Boudinage 1648:Monocline 1643:Homocline 1623:Anticline 1605:Tectonite 1595:Stylolite 1570:Fissility 1547:lineation 1543:Foliation 1407:Syneclise 1352:Obduction 1322:Inversion 1214:tectonics 911:Tectonics 897:0264-8172 571:Apennines 401:backstops 106:sediments 93:from the 50:sediments 1770:Category 1755:Category 1727:Mylonite 1658:Vergence 1653:Syncline 1555:Cleavage 1480:Faulting 625:See also 586:Slovakia 563:Bay Area 412:Examples 375:Cascadia 367:Antilles 335:Jurassic 323:obducted 200:Geometry 186:terranes 153:Barbados 126:terranes 53:accreted 1628:Chevron 1615:Folding 1460:Fissure 1412:Terrane 1357:Orogeny 1337:MĂ©lange 1272:Fenster 1162:Tension 1044:659-665 865:Bibcode 744:Bibcode 606:Neogene 598:Romania 594:Ukraine 582:Bohemia 540:Neogene 474:Neogene 276:verging 265:mĂ©lange 160:forearc 99:pelagic 91:basalts 1402:Suture 1387:Saddle 1327:Klippe 1292:Graben 1152:Stress 1142:Strain 895:  590:Poland 514:Alaska 444:- the 431:- the 383:Mexico 381:, and 371:Nankai 347:strike 280:trench 272:thrust 97:, and 1737:Shear 1465:Joint 1347:Nappe 1307:Horst 1302:Horse 997:(PDF) 379:Chile 114:Japan 62:at a 1638:Dome 1545:and 1470:Vein 1450:Dike 1382:Rift 1193:Rake 1031:2016 1005:2016 940:2016 893:ISSN 717:2016 685:2016 663:2016 612:and 596:and 569:The 557:The 488:The 315:USGS 101:and 68:slab 915:doi 883:hdl 873:doi 861:112 834:doi 783:doi 752:doi 740:255 604:to 580:in 520:in 516:to 230:by 112:of 81:An 70:of 44:or 40:An 1772:: 891:. 881:. 871:. 859:. 855:. 750:. 738:. 734:. 592:, 588:, 584:, 469:). 377:, 301:. 155:). 1090:e 1083:t 1076:v 1062:) 1033:. 1007:. 942:. 921:. 917:: 899:. 885:: 875:: 867:: 840:. 836:: 789:. 785:: 758:. 754:: 746:: 719:. 687:. 665:. 620:. 500:. 253:) 247:( 242:) 238:( 224:. 20:)

Index

Accretionary prism

sediments
accreted
subducting
tectonic plate
convergent plate boundary
slab
oceanic crust
island arcs
turbidites
basalts
ocean floor
pelagic
hemipelagic
sediments
geological basement
Japan
terranes
turbidites
Barbados
forearc
ocean basins
ocean ridges
crustal fragments
terranes
mountain-building
North American

verification

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