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Premium member Presentation Transcript Classroom presentations to accompany Understanding Earth, 3rd edition : Classroom presentations to accompany Understanding Earth, 3rd edition prepared by Peter Copeland and William Dupré University of Houston Chapter 14 Wind and Deserts Slide 2: Wind and Deserts Stanley Breeden/DRK Deserts : Deserts Deserts are usually thought of as hot and dry, but there are different ways to define a desert: Annual rainfall (<25 cm) Less precipitation than the potential for evaporation Deserts can be cold if there is an extremely small amount of precipitation. Atmospheric Circulation Patterns : Fig. 14.1 Atmospheric Circulation Patterns Erosion and deserts : Erosion and deserts Wind is often thought to be the most important agent of erosion in deserts. However, even in deserts, most of the work of erosion is done by water. Because there is so little water in deserts, erosion is very intermittent. Erosion and deserts : Erosion and deserts Typically, when storms take place in desert regions, dry stream courses fill quickly with water. With little vegetation to hold water, flash floods can be brief, but violent. Erosion and deserts : Erosion and deserts When rainfall is unusually heavy, desert soil may become saturated with water and begin to flow. This is known as a debris flow. Slide 8: Fig. 14.2 Slide 9: Fig. 14.3 Slide 10: Fig. 14.4 Tom Bean Wind Direction Rate of Sand Movement as a Function of Wind Velocity : Fig. 14.5 Rate of Sand Movement as a Function of Wind Velocity Wind : Wind Transportation of material: Because wind is much less dense than water, it can transport only small particles, mainly fine sand and silt (clay is usually too cohesive). Particles move by either saltation (sand) or suspension (dust). Wind : Wind Dust can be transported over great distances. Skiers in the Alps commonly encounter a silty surface on the snow. The silt comes from the Sahara desert in Africa, over 1500 km away. Wind : Wind Wind-borne material can become extremely concentrated in air:in 1 km3, there may be up to 1000 tons of dust. Sand grains carried by wind get a frosted exterior (diagnostic of eolian transport). Dust Storm, 1937 : Dust Storm, 1937 Library of Congress Frosted and Rounded Wind-blown Sand : Fig. 14.6 Frosted and Rounded Wind-blown Sand Walter N. Mack Deflation : Deflation The process of removing all of the small (easily moved) particles. As this process proceeds, only larger rocks are left. This is known as “desert pavement”. Deflation Hollow : Fig. 14.7 Breck P. Kent Deflation Hollow Formation of Desert Pavement : Formation of Desert Pavement Fig. 14.9b Slide 20: Fig. 14.8a David Muench Desert Pavement Ventifact : Ventifact Fig. 14.9 E.R.Degginger Yardangs in Iran : Yardangs in Iran Fig. 14.10 Comstock Linear Dunes in Saudi Arabia : Fig. 14.11 Linear Dunes in Saudi Arabia Prevailing Winds ERIM Slide 24: Fig. 14.12 Coastal Dunes in Peru Loren McIntyre Formation of a Wind-shadow Dune : Formation of a Wind-shadow Dune Fig. 14.13 Dune Migration : Dune Migration Fig. 14.14 Dune Migration and the Formation of Cross Bedding : Fig. 14.15 Dune Migration and the Formation of Cross Bedding Compression of Streamlines over Dune Increases Velocity : Fig. 14.16 Compression of Streamlines over Dune Increases Velocity Types of Dunes : Types of Dunes Fig. 14.17 Pleistocene Loess : Fig. 14.18 Pleistocene Loess E.R.Degginger Loess in China : Loess in China Fig. 14.19 Stephen C. Porter Where deserts are : Where deserts are Tropic of Capricorn, Tropic of Cancer High pressure subsiding air heats loses moisture Center of continent Rain shadow Interaction with ocean currents: e.g., Atacama Desert (Peru and Chile). Air moves from above cold ocean waters to warm land and expands, absorbing moisture. Major Deserts of the World : Major Deserts of the World Fig. 14.20 Desert varnish : Desert varnish Surface coating of Fe and Mn oxides Can be used to date exposure intervals. Slide 35: Fig. 14.21 Petroglyphs in Desert Varnish Peter Kresan Streams and lakes in deserts : Streams and lakes in deserts Often streams in the desert dry up before they reach the sea. Those that don’t dry up are usually fed from a wetter area (e.g., Colorado River). Interior drainages are common in deserts — the two are linked. Examples: Nevada, Tibetan plateau “Dry wash” in Flood : Fig. 14.22a “Dry wash” in Flood Peter Kresan The Day After : Fig. 14.22b The Day After Peter Kresan Slide 39: Fig. 14.23 Playa Lake David Muench Typical Landscape Formed by Desert Weathering : Typical Landscape Formed by Desert Weathering Fig. 14.24 Peter Kresan Playa lakes : Playa lakes Formed in a closed basin. Water accumulates after rain; may last days to months before complete evaporation, leaving a playa, a flat lake bed of clay, silt, and evaporites. Faulting : Faulting Fig. 14.25a Deposition of Alluvial Fans : Deposition of Alluvial Fans Fig. 14.25b Erosional Retreat Forms Pediment : Erosional Retreat Forms Pediment Fig. 14.25c Pediment Expands with Continued Erosion : Pediment Expands with Continued Erosion Fig. 14.25d Evolution of a MesaRivers Breach Resistant Cap : Evolution of a MesaRivers Breach Resistant Cap Fig. 14.26a Evolution of a MesaContinued Erosion : Evolution of a MesaContinued Erosion Fig. 14.26b Evolution of a MesaLong-continued Erosion : Evolution of a MesaLong-continued Erosion Fig. 14.26c You do not have the permission to view this presentation. In order to view it, please contact the author of the presentation.
Erosion and Deserts aSGuest169 Download Post to : URL : Related Presentations : Share Add to Flag Embed Email Send to Blogs and Networks Add to Channel Uploaded from authorPOINT lite Insert YouTube videos in PowerPont slides with aS Desktop Copy embed code: (To copy code, click on the text box) Embed: URL: Thumbnail: WordPress Embed Customize Embed The presentation is successfully added In Your Favorites. Views: 524 Category: Entertainment License: All Rights Reserved Like it (1) Dislike it (0) Added: September 24, 2008 This Presentation is Public Favorites: 0 Presentation Description No description available. Comments Posting comment... Premium member Presentation Transcript Classroom presentations to accompany Understanding Earth, 3rd edition : Classroom presentations to accompany Understanding Earth, 3rd edition prepared by Peter Copeland and William Dupré University of Houston Chapter 14 Wind and Deserts Slide 2: Wind and Deserts Stanley Breeden/DRK Deserts : Deserts Deserts are usually thought of as hot and dry, but there are different ways to define a desert: Annual rainfall (<25 cm) Less precipitation than the potential for evaporation Deserts can be cold if there is an extremely small amount of precipitation. Atmospheric Circulation Patterns : Fig. 14.1 Atmospheric Circulation Patterns Erosion and deserts : Erosion and deserts Wind is often thought to be the most important agent of erosion in deserts. However, even in deserts, most of the work of erosion is done by water. Because there is so little water in deserts, erosion is very intermittent. Erosion and deserts : Erosion and deserts Typically, when storms take place in desert regions, dry stream courses fill quickly with water. With little vegetation to hold water, flash floods can be brief, but violent. Erosion and deserts : Erosion and deserts When rainfall is unusually heavy, desert soil may become saturated with water and begin to flow. This is known as a debris flow. Slide 8: Fig. 14.2 Slide 9: Fig. 14.3 Slide 10: Fig. 14.4 Tom Bean Wind Direction Rate of Sand Movement as a Function of Wind Velocity : Fig. 14.5 Rate of Sand Movement as a Function of Wind Velocity Wind : Wind Transportation of material: Because wind is much less dense than water, it can transport only small particles, mainly fine sand and silt (clay is usually too cohesive). Particles move by either saltation (sand) or suspension (dust). Wind : Wind Dust can be transported over great distances. Skiers in the Alps commonly encounter a silty surface on the snow. The silt comes from the Sahara desert in Africa, over 1500 km away. Wind : Wind Wind-borne material can become extremely concentrated in air:in 1 km3, there may be up to 1000 tons of dust. Sand grains carried by wind get a frosted exterior (diagnostic of eolian transport). Dust Storm, 1937 : Dust Storm, 1937 Library of Congress Frosted and Rounded Wind-blown Sand : Fig. 14.6 Frosted and Rounded Wind-blown Sand Walter N. Mack Deflation : Deflation The process of removing all of the small (easily moved) particles. As this process proceeds, only larger rocks are left. This is known as “desert pavement”. Deflation Hollow : Fig. 14.7 Breck P. Kent Deflation Hollow Formation of Desert Pavement : Formation of Desert Pavement Fig. 14.9b Slide 20: Fig. 14.8a David Muench Desert Pavement Ventifact : Ventifact Fig. 14.9 E.R.Degginger Yardangs in Iran : Yardangs in Iran Fig. 14.10 Comstock Linear Dunes in Saudi Arabia : Fig. 14.11 Linear Dunes in Saudi Arabia Prevailing Winds ERIM Slide 24: Fig. 14.12 Coastal Dunes in Peru Loren McIntyre Formation of a Wind-shadow Dune : Formation of a Wind-shadow Dune Fig. 14.13 Dune Migration : Dune Migration Fig. 14.14 Dune Migration and the Formation of Cross Bedding : Fig. 14.15 Dune Migration and the Formation of Cross Bedding Compression of Streamlines over Dune Increases Velocity : Fig. 14.16 Compression of Streamlines over Dune Increases Velocity Types of Dunes : Types of Dunes Fig. 14.17 Pleistocene Loess : Fig. 14.18 Pleistocene Loess E.R.Degginger Loess in China : Loess in China Fig. 14.19 Stephen C. Porter Where deserts are : Where deserts are Tropic of Capricorn, Tropic of Cancer High pressure subsiding air heats loses moisture Center of continent Rain shadow Interaction with ocean currents: e.g., Atacama Desert (Peru and Chile). Air moves from above cold ocean waters to warm land and expands, absorbing moisture. Major Deserts of the World : Major Deserts of the World Fig. 14.20 Desert varnish : Desert varnish Surface coating of Fe and Mn oxides Can be used to date exposure intervals. Slide 35: Fig. 14.21 Petroglyphs in Desert Varnish Peter Kresan Streams and lakes in deserts : Streams and lakes in deserts Often streams in the desert dry up before they reach the sea. Those that don’t dry up are usually fed from a wetter area (e.g., Colorado River). Interior drainages are common in deserts — the two are linked. Examples: Nevada, Tibetan plateau “Dry wash” in Flood : Fig. 14.22a “Dry wash” in Flood Peter Kresan The Day After : Fig. 14.22b The Day After Peter Kresan Slide 39: Fig. 14.23 Playa Lake David Muench Typical Landscape Formed by Desert Weathering : Typical Landscape Formed by Desert Weathering Fig. 14.24 Peter Kresan Playa lakes : Playa lakes Formed in a closed basin. Water accumulates after rain; may last days to months before complete evaporation, leaving a playa, a flat lake bed of clay, silt, and evaporites. Faulting : Faulting Fig. 14.25a Deposition of Alluvial Fans : Deposition of Alluvial Fans Fig. 14.25b Erosional Retreat Forms Pediment : Erosional Retreat Forms Pediment Fig. 14.25c Pediment Expands with Continued Erosion : Pediment Expands with Continued Erosion Fig. 14.25d Evolution of a MesaRivers Breach Resistant Cap : Evolution of a MesaRivers Breach Resistant Cap Fig. 14.26a Evolution of a MesaContinued Erosion : Evolution of a MesaContinued Erosion Fig. 14.26b Evolution of a MesaLong-continued Erosion : Evolution of a MesaLong-continued Erosion Fig. 14.26c