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AEOLIAN LANDSCAPES 299


























              Plate 12.1 Lag deposits lying on a stone pavement, Dhakla, Western Desert, Egypt.
              (Photograph by Tony Waltham Geophotos)



              names – desert pavements in the USA, gibber plains in  by deflation (Figure 12.2; Plate 12.2). In size, they range
              Australia, gobi in Central Asia, and hammada, reg,or  from a few metres wide and only centimetres deep, to
              serir in the Arab world. Hammada is rocky desert, in  kilometres across and tens of metres deep. The largest
              which the lag consists of coarse, mechanically weath-  known pan, which was discovered in eastern Australia, is
              ered regolith. Serir is pebbly desert with a lag of rounded  45 km wide. Pans are prominently developed in southern
              gravel and coarse sand produced by deflation of alluvial  Africa, on the High Plains of the USA, in the Argentinian
              deposits.                                 pampas, Manchuria, western and southern Australia, the
                                                        west Siberian steppes, and Kazakhstan (Goudie 1999).
                                                        They sometimes have clay dunes or lunette dunes
                                                        formed on their leeside that are composed of sandy, silty,
              Deflation hollows and pans
                                                        clayey, and salty material from the pan floor. The pres-
              Deflation can scour out large or small depressions called  ence of a lunette is a sure sign that a pan has suffered
              deflation hollows or blowouts. Blowouts are the com-  deflation. The evolution of pans is a matter of debate
              monest landforms produced by wind erosion. They are  (Box 12.1).
              most common in weak, unconsolidated sediments. In  Deflation appears to have played a starring role in
              size, they range from less than a metre deep and a few  scooping out great erosional basins, such as the large
              metres across, through enclosed basins a few metres deep  oasis depressions in the Libyan Desert. However, such
              and hundreds of metres across (pans), to very large fea-  large basins are almost certain to have had a complex
              tures more than 100 m deep and over 100 km across.  evolution involving processes additional to deflation,
              They are no deeper than the water table, which may be  including tectonic subsidence. The deepest of such
              several hundred metres below the ground surface, and  basins is the Qattara Depression in northern Egypt,
              may attain diameters of kilometres.       which is cut into Pliocene sediments. At its lowest
                Pans are closed depressions that are common in many  point, the Qattara Depression lies 134 m below sea
              dryland areas and that seem to be at least partly formed  level.
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