Arid Zone Geomorphology 2011
DOI: 10.1002/9780470710777.ch9
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Pavements and Stone Mantles

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Cited by 13 publications
(7 citation statements)
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References 81 publications
(215 reference statements)
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“…There is a spectrum of grain sizes that characterizes the coarse-grained surfaces in arid deserts [Laity, 2011]. In many cases, desert pavements consist of very coarse sediment that are beyond the realm of wind transport [Haff and Werner, 1996].…”
Section: Discussionmentioning
confidence: 99%
“…There is a spectrum of grain sizes that characterizes the coarse-grained surfaces in arid deserts [Laity, 2011]. In many cases, desert pavements consist of very coarse sediment that are beyond the realm of wind transport [Haff and Werner, 1996].…”
Section: Discussionmentioning
confidence: 99%
“…At L0106/0130, the quadrants with the highest artifact counts were found on subdued topography covered by fine-grained, artifactbearing sediments allowing the formation of lag deposits through winnowing of fine material by wind and water (as well as sporadic high-energy surface sheet flow during rainstorms), by exposing artifacts and other clasts, but with insufficient energy to move them into areas of net sedimentation where they could be buried. Such deposits sometimes referred to as deflationary desert pavements (Laity, 2011), are familiar to those working in Paleolithic archaeology in the arid zone (e.g., Hill, 2000;Jones et al, 2011;Knight & Zerboni, 2018 (Pedley, 1990) and algae aid removal of carbon dioxide from solution to encourage carbonate precipitation (Ford & Pedley, 1996), whereas flowing water encourages turbulent carbon dioxide degassing, again encouraging carbonate precipitation (Ford & Pedley, 1996). Drivers behind periods of tufa formation in this now semiarid to arid basin were climatic, corresponding to periods of increased rainfall and reduced evapotranspiration as documented elsewhere in Saudi…”
Section: Surface Variability and Artifact Distribution In The Wadi mentioning
confidence: 99%
“…In a functional sense, the actual parent material for the developing soil is not the basalt bedrock of the flow, but rather, the aeolian sediments added to the surface and incorporated into the vesicular A horizon directly beneath the stone pavement. A considerable amount of additional evidence supporting the accretionary model of pavement development based on investigations of other types of geological surfaces (e.g., cobbly to bouldery alluvial fan deposits) has appeared over the last two decades; Laity [60] and McFadden [61] provide comprehensive summaries of this body of work. Although there are geological settings where selective erosion (aeolian or fluvial) of fine materials may first be required to generate a lag of coarser clasts on the surface (e.g., see later section on Quartz pavements of the Knersvlakte), even in those situations, once such a surface lag is created, the dust-trapping effect of the surface clasts contributes to the accumulation of aeolian sediments and development of an underlying accretionary mantle beneath a stone pavement.…”
Section: Stone Pavementsmentioning
confidence: 99%
“…Behind the knife is the uppermost portion of a sequence of reddened Bt horizons; the colour is 7.5 YR 6/4. Stone pavements and their associated, underlying clast-free vesicular A horizons derived largely from the accretion of aeolian sediments occur on diverse substrates, including fan deposits and terraces of coarse gravelly to stony alluvium and pediments in arid regions throughout the world [60,[68][69][70][71][72]. Soils with the same kinds of clast-free vesicular A horizons beneath pavements have been described for arid regions of South Africa [15,73], and Ellis [74] mapped their overall geographic distribution in western South Africa.…”
Section: Stone Pavementsmentioning
confidence: 99%