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Desert pavement

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182: 43: 210: 31: 113:, dust and other fine-grained material by the wind and intermittent rain, leaving the larger fragments behind. The larger fragments are shaken into place through the forces of rain, running water, wind, gravity, creep, thermal expansion and contraction, wetting and drying, frost heaving, animal traffic, and the Earth's constant 169:
in the lava flows, building up with exposure time. The helium-3 dates show that the lava stones in the desert pavement at Cima Dome have all been at the surface the same amount of time as the solid lava flows right next to them. He wrote in a July 1995 article in
201:. Desert varnish is a thin coating (patina) of clays, iron, and manganese on the surface of sun-baked boulders. Micro-organisms may also play a role in their formation. Desert varnish is also prevalent in the Mojave desert and Great Basin geomorphic province. 129:
A second theory supposes that desert pavements form from the shrink/swell properties of the clay underneath the pavement; when precipitation is absorbed by clay it causes it to expand, and when it dries it cracks along planes of weakness. Over time, this
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flows are covered by younger soil layers, with desert pavement on top of them, made of rubble from the same lava. The soil has been built up, not blown away, yet the stones remain on top. There are no stones in the soil, not even gravel.
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vibrations. The removal of small particles by wind does not continue indefinitely, because once the pavement forms, it acts as a barrier to resist further erosion. The small particles collect underneath the pavement surface, forming a
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For the geologist, this discovery means that some desert pavements preserve a long history of dust deposition beneath them. The dust is a record of ancient climate, just as it is on the deep sea floor and in the world's ice caps.
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Processes of vesicular horizon development and desert pavement formation on basalt flows of the Cima Volcanic Field and alluvial fans of the Avawatz Mountains Piedmont, Mojave Desert, California
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that he concluded, "stone pavements are born at the surface." While the stones remain on the surface due to heave, deposition of windblown dust must build up the soil beneath that pavement.
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action transports small pebbles to the surface, where they stay through lack of precipitation that would otherwise destroy the pavement by transport of the
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McFadden, L.D., Wells, S.G. and Jercinovich, M.J. 1987. "Influences of aeolian and pedogenic processes on the origin and evolution of desert pavements",
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Several theories have been proposed for the formation of desert pavements. A common theory suggests that they form through the gradual removal of
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The influence of long-term landscape stability on flood hydrology and geomorphic evolution of valley floor in the northeastern Badin of Jordan
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The role and significance of the Gobi desert pavement in controlling sand movement on the cliff top near the Dunhuang Magao Grottoes
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Researchers can determine how many years a stone has been exposed on the ground. Wells used a method based on cosmogenic
495: 376: 368: 433: 193:, a dark brown, sometimes shiny coating that contains clay minerals. In the US a famous example can be found on 437: 407:"Cosmogenic He surface-exposure dating of stone pavements: Implications for landscape evolution in deserts" 595: 232: 342: 17: 473:
East, J.J. 1889. "On the geological structures and physical features of Central Australia",
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A newer theory of pavement formation comes from studies of places such as Cima Dome, in the
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Stony deserts may be known by different names according to the region. Examples include:
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of California, by Stephen Wells and his coworkers. At Cima Dome, geologically recent
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Estimating the fine soil fraction of desert pavements using ground penetrating radar
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ynamical processes on desert pavements and the healing of surficial disturbance
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Transactions and Proceedings and Report of the Royal Society of South Australia
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Dorn, R. I. and T. M. Oberlander, 1981, "Microbial Origin of Desert Varnish,"
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bombardment at the ground surface. Helium-3 is retained inside grains of
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Geologists debate the mechanics of pavement formation and their age.
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surface covered with closely packed, interlocking angular or rounded
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Desert pavement evolution: An example of the role of sheetflood
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Qu Jianjun, Huang Ning, Dong Guangrong and Zhang Weimin. 2001.
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10.1130/0091-7613(1995)023<0613:CHSEDO>2.3.CO;2
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Wells S.G.; McFadden L.D.; Poths J.; Olinger C.T. (1995).
311: – Desert landscape with mostly rock instead of sand 305: – Broad area of desert covered with wind-swept sand 293: – Orange-to-black rock coating in arid environments 249:
is also used to describe ecological communities, such as
521:. Doctoral thesis, University of California, Riverside. 545:
Meadows, D.G., Young, M.H. and McDonald, E.V. 2006.
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Geology Underfoot: In Death Valley and Owens Valley
46:Desert pavement showing wind scour on the cobbles; 38:on the pebbles; gibber plains of central Australia 526:The history and nature of wind erosion in deserts 490:, Presses universitaires de France, Paris, 1982. 98:collects on the exposed surface rocks over time. 587: 535:, fifth edition. Freeman and Company. 458–460. 398: 189:Desert pavement surfaces are often coated with 514:. Doctoral thesis, University of Nevada, Reno. 556:. Journal of Arid Environments 48(3):357-371. 566:Williams, S.H. and Zimbelman, J.R. 1994. 570:. The Journal of Geology 102(2):243-248. 264:, a vast stony desert plain is known as 208: 180: 41: 29: 563:. The Lapidary Journal 33(7):1648-1650. 335: 274:, which refers to a sandy desert area. 14: 588: 287: – Processes due to wind activity 227:Gibbers: Covering extensive areas in 362: 317: – Particle transport by fluids 549:. Vadose Zone Journal 5(2):720-730. 538:Haff, P.K. and Werner, B.T. 1996. D 24: 542:. Quaternary Research 45(1):38-46. 25: 617: 574: 561:Deflation armor (desert pavement) 369:Mountain Press Publishing Company 343:"Hamada, Reg, Serir, Gibber, Saï" 138:or excessive vegetative growth. 581:Desert Processes Working Group 480: 467: 454: 385: 356: 204: 13: 1: 504: 488:Géographie des régions arides 213:The desert known as Reg de l' 255:Gibber Transition Shrublands 238:are desert pavements called 104: 27:Type of desert earth surface 7: 277: 268:. This is in contrast with 10: 622: 345:. Springer Reference. 2013 251:Gibber Chenopod Shrublands 531:Grotzinger, et al. 2007. 233:Tirari-Sturt stony desert 185:Desert pavement evolution 90:size. They typically top 328: 34:Desert pavement showing 74:(in central Asia) is a 363:Sharp, Robert (1997). 221: 186: 51: 50:of southern California 39: 517:Anderson, K.C. 1999. 510:Al-Qudah, K.A. 2003. 367:. Missoula, Montana: 242:after the pebbles or 231:such as parts of the 212: 184: 66:(in eastern Sahara), 62:(in western Sahara), 45: 33: 486:Jean Dresch et al., 371:. pp. 119–130. 559:Rieman, H.M. 1979. 533:Understanding Earth 524:Goudie, A.S. 2008. 426:1995Geo....23..613W 315:Saltation (geology) 126:(designated "Av"). 70:(in Australia), or 297:Eduction (geology) 222: 187: 52: 40: 596:Aeolian landforms 285:Aeolian processes 157:, which forms by 16:(Redirected from 613: 498: 484: 478: 471: 465: 458: 452: 451: 449: 448: 442: 436:. Archived from 411: 402: 396: 389: 383: 382: 360: 354: 353: 351: 350: 339: 197:in southeastern 21: 621: 620: 616: 615: 614: 612: 611: 610: 586: 585: 577: 507: 502: 501: 485: 481: 472: 468: 459: 455: 446: 444: 440: 409: 403: 399: 390: 386: 379: 361: 357: 348: 346: 341: 340: 336: 331: 326: 280: 207: 107: 56:desert pavement 28: 23: 22: 15: 12: 11: 5: 619: 609: 608: 603: 598: 584: 583: 576: 575:External links 573: 572: 571: 564: 557: 550: 543: 536: 529: 522: 515: 506: 503: 500: 499: 479: 466: 453: 420:(7): 613–616. 397: 395:15(6):504-508. 384: 377: 355: 333: 332: 330: 327: 325: 324: 318: 312: 306: 300: 294: 291:Desert varnish 288: 281: 279: 276: 206: 203: 195:Newspaper Rock 191:desert varnish 106: 103: 96:Desert varnish 58:, also called 36:desert varnish 26: 9: 6: 4: 3: 2: 618: 607: 604: 602: 599: 597: 594: 593: 591: 582: 579: 578: 569: 565: 562: 558: 555: 551: 548: 544: 541: 537: 534: 530: 527: 523: 520: 516: 513: 509: 508: 497: 496:2-13-037457-3 493: 489: 483: 476: 470: 464:213:1245-1247 463: 457: 443:on 2016-10-06 439: 435: 431: 427: 423: 419: 415: 408: 401: 394: 388: 380: 378:9780878423620 374: 370: 366: 359: 344: 338: 334: 322: 319: 316: 313: 310: 307: 304: 301: 298: 295: 292: 289: 286: 283: 282: 275: 273: 272: 267: 263: 258: 256: 252: 248: 245: 241: 240:Gibber Plains 237: 234: 230: 225: 220: 216: 211: 202: 200: 196: 192: 183: 179: 175: 173: 168: 164: 160: 156: 151: 148: 144: 143:Mojave Desert 139: 137: 133: 127: 125: 121: 116: 112: 102: 99: 97: 93: 92:alluvial fans 89: 85: 82:fragments of 81: 77: 73: 69: 65: 61: 57: 49: 48:Mojave Desert 44: 37: 32: 19: 567: 560: 553: 546: 539: 532: 525: 518: 511: 487: 482: 474: 469: 461: 456: 445:. Retrieved 438:the original 417: 413: 400: 392: 387: 364: 358: 347:. Retrieved 337: 269: 265: 262:North Africa 259: 254: 250: 246: 243: 239: 226: 223: 188: 176: 171: 152: 140: 128: 124:soil horizon 115:microseismic 108: 100: 71: 67: 63: 59: 55: 53: 205:Local names 590:Categories 505:References 447:2016-02-23 349:2013-05-23 219:Mauritania 159:cosmic ray 132:geomorphic 606:Sediments 477:12:31-53. 321:Ventifact 236:ecoregion 229:Australia 120:vesicular 105:Formation 278:See also 244:gibbers. 172:Geology, 167:pyroxene 155:helium-3 601:Deserts 462:Science 422:Bibcode 414:Geology 393:Geology 163:olivine 494:  375:  309:Hamada 247:Gibber 136:clasts 88:cobble 84:pebble 76:desert 68:gibber 18:Gibber 441:(PDF) 410:(PDF) 329:Notes 215:Adrar 64:serir 492:ISBN 373:ISBN 199:Utah 165:and 147:lava 111:sand 86:and 80:rock 430:doi 303:Erg 271:erg 266:reg 260:In 253:or 217:in 72:saï 60:reg 592:: 428:. 418:23 416:. 412:. 257:. 122:A 94:. 54:A 450:. 432:: 424:: 381:. 352:. 20:)

Index

Gibber

desert varnish

Mojave Desert
desert
rock
pebble
cobble
alluvial fans
Desert varnish
sand
microseismic
vesicular
soil horizon
geomorphic
clasts
Mojave Desert
lava
helium-3
cosmic ray
olivine
pyroxene

desert varnish
Newspaper Rock
Utah

Adrar
Mauritania

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