Escarpment - Wikipedia, the free encyclopedia
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In geomorphology, an escarpment is a transition zone between different physiogeographic provinces that involves a sharp, steep elevation differential, characterized by a cliff or steep slope. Usuall...
en.wikipedia.org/wiki/Escarpment
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Title:; Morphologic dating of scarps formed by repeated slip events along the San Andreas Fault, Carrizo Plain, California ... Morphologic dating of fault scarps determines late Cenozoic fault activity by comparing observed topographic profiles with those determined using a calibrated hillslope development model.
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adsabs.harvard.edu/abs/1998JGR...10310141A
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Scarps formed by normal faulting in the West Yellowstone Basin are much more difficult to date than are terrace scarps, because of the possible complexity of their initial morphology.
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bulletin.geoscienceworld.org/cgi/content/abstract/95/12...
bulletin.geoscienceworld.org/cgi/content/abstract/95/12/1413
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and 3) that a barrier island core separated the two scarps formed during the same Pleistocene highstand. A modern analog is Hilton Head Island. It contains two Pleistocene barrier-island cores separated by successively lower scarps formed during successively lower highstands.
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gsa.confex.com/gsa/2006SE/finalprogram/abstract_102019....
gsa.confex.com/gsa/2006SE/finalprogram/abstract_102019.htm
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These 15 scarps may have all formed in one earthquake, with rupture propagation from depth to the near-surface aided by clay gouge along the detachment. The detachment is abandoned in the footwall east of the scarps.
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geology.geoscienceworld.org/cgi/content/abstract/27/3/2...
geology.geoscienceworld.org/cgi/content/abstract/27/3/247
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This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a series of curving scarps formed by erosion and sublimation of carbon dioxide from the south polar cap. This area is located near 86.3°S, 51.2°W. The image is illuminated by sunlight from the upper left;
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www.msss.com/mars_images/moc/2003/07/31/index.html
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The pattern of degradation observed on some scarps formed by normal, range-front faulting of alluvial fan surfaces may be accurately modeled, and, when properly calibrated, these models provide a means for determining the ages of some scarps (morphologic dating).
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www.nap.edu/openbook.php?record_id=624&page=181
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The scarps, of which several are known from the Mariner images, probably formed when the planet's interior cooled and shrank long ago, much as wrinkles form on the skin of an old shrunken apple. If we can apply to Mercury the cratering age estimates we use for the Moon, the scarps probably formed about 4 billion years ago.
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dev.prenhall.com/divisions/esm/app/chaissonat3/CHAISSON...
dev.prenhall.com/divisions/esm/app/chaissonat3/CHAISSON/AT308/HTML/AT30806.HTM
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Strictly speaking, the term ‘fault scarp’ refers to the scarp formed along the intersection of a fault plane with the Earth's surface and should only be used in the case of a fault that reaches ground level. ... Erosional scarps result from vertical incision...
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www.encyclopedia.com/doc/1O112-faultscarp.html
www.encyclopedia.com/doc/1O112-faultscarp.html
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