Deserts and Winds Chapter 19
A typical desert landscape, Sonoran Desert east of Phoenix, Arizona
Distribution and causes of dry lands Dry regions cover 30 percent of Earth’s land surface Two climatic types are commonly recognized Desert or arid Steppe or semiarid
Arid and Semiarid Climates Cover @ 30% of Earth’s Land Surface Arid and Semiarid Climates Cover @ 30% of Earth’s Land Surface. No Other Climate Group Covers So Much Area
Distribution and causes of dry lands Dry regions are characterized by a combination of two important factors Minimal rainfall (typically 5-10 inches annually) High rates of evaporation (evaporation > precipitation)
Deserts are Defined by a Combination of Average Annual Temperature, Average Annual Rainfall, & How the Rainfall is Distributed
Distribution and causes of dry lands Because evaporation is greatly reduced in a cold climate, areas near the earth’s poles can experience relatively little rainfall and still not exhibit desert conditions. Climatologists consider the average annual temperature, the total annual precipitation & when the rain falls in determining desert conditions
Distribution and causes of dry lands Dry lands are concentrated in two regions Subtropics Low-latitude deserts In the vicinities of the Tropics of Cancer and Capricorn Areas of high pressure and sinking air that is compressed and warmed, resulting in little rainfall http://study.com/academy/lesson/subtropical-desert-climate-and-biome.html
Earth’s Wind Circulation Patterns Produce Sinking Air & Little Rain Near the Subtropical High Pressure Belts
Distribution and causes of dry lands Dry lands are concentrated in two regions Middle-latitudes Located in the deep interiors of continents High mountains in the path of the prevailing winds produce a rainshadow desert
Rainshadow deserts form in earth’s mid-latitude regions when high mountains cause air to rise and rain on their windward sides, then sink without raining on the leeward sides
Note the Distribution of Desert & Steppe Climates Note the Distribution of Desert & Steppe Climates. They are Concentrated along the Subtropical Highs and in the Rainshadows of High Mountain Ranges. There are NO Deserts in the Polar Regions
Distribution and causes of dry lands Human activity can hasten the “desertification” of steppe regions, usually as the result of excess water comsumption for grazing or irrigation Areas at particular risk today include the southern Sahara steppe and the Aral Sea
The Aral Sea was replenished primarily by water from the Amu & Syr Rivers. Since 1960, most of their waters have been diverted for irrigation
Blooming, But This Region is Being Destroyed. The Aral Sea is Shrinking Rapidly. It’s Fishing Economy is Gone & Entire Towns Are Disappearing. Other Areas Are Blooming, But This Region is Being Destroyed.
Geologic processes in arid climates Weathering Not as effective as in humid regions Mechanical weathering produces unaltered rock and mineral fragments Some chemical weathering in deserts does produce Clay Thin soils Oxidized minerals
Geologic processes in arid climates Role of water in arid climates Practically all streambeds are dry most of the time Desert streams are classified as ephemeral Carry water only during periods of rainfall Different names are used for desert streams in various region Wash and arroyo (western United States) Wadi (Arabia and North Africa) Despite its scarcity, water is still the major erosive agent in deserts
Desert Streams are Ephemeral – They Rarely Contain Water – But Erosion is Dramatic When “The Rains” Come
Geologic processes in arid climates Role of water in arid climates Desert rainfall Rain often occurs as heavy, localized showers Because desert vegetative cover is sparse, runoff is largely unhindered and flash floods are common Poorly integrated drainage systems and streams lack an extensive system of tributaries Most of the erosion work in a desert is done by running water
Tucson, Arizona, a desert Rains in the Desert Can Be Spectacular and Quite Heavy, But They Cover Small Geographic Areas Tucson, Arizona, a desert Van Horn, Texas, a steppe
Basin and Range: Evolution of a desert landscape Characterized by interior drainage Landscape evolution in the Basin and Range region Uplift of mountains – block faulting Interior drainage into basins produces Alluvial fans Bajadas Playas and Playa lakes
Typical “Block Faulting” (Normal Faulting) Creates Basin and Range Topography in Parts of the Western United States
Most Block Faulted Mountains in the Basin & Range Are Actually Horsts and Grabens. The Mountains Are Faulted on Both Sides and Moved “Up” Relative to the Intervening Valleys
Alluvial Fans Develop Along Horst Mountain Blocks in the Basin and Range Province Where Stream Gradients Change Abruptly from Steep to Flat
Coalescing Alluvial Fans Form Bajadas Along the Horst Block Mountain Fronts in Death Valley, Basin & Range Province
Playas Are Dry Lake Beds that are Common in the Graben Valleys of the Basin & Range. They Often Display Evaporative Salt Crusts Bajada Playa
When Localized Rains Fills the Playa with Water, it Becomes a Playa Lake
Basin and Range: Evolution of a desert landscape Landscape evolution in the Basin and Range region Ongoing erosion of the mountain mass Produces sediment that fills the basin Diminishes local relief Produce isolated erosional remnants called inselbergs
Without Continued Uplift, the Horst Block Mountains are Gradually Eroded. The Resulting Sediment Fills the Graben Valleys, Leaving Only Isolated Inselbergs as Erosional Remnants
An Inselberg (Erosional Mountain Remnant) in the Basin & Range of Southern California
Mount Uluru (Formerly Ayers Rock) is an Inselberg in the Center of the Australian Outback
Wind in the desert Transportation of sediment by wind Differs from that of running water in two ways Wind is less capable of picking up and transporting coarse materials Wind is not confined to channels and can spread sediment over large areas
Wind in the desert Transportation of sediment by wind Mechanisms of transport Bedload Saltation – skipping and bouncing along the surface About 20 to 25 percent of the sand transported in a sandstorm is moved this way Suspended load Silt and clay can be carried by wind for long distances
A Cloud of Saltating Sand Grains (Bed Load) Moves up the Gentle Slope of a Dune During a Time of High Desert Wind Velocity
Silt and Clay (Suspended Load) Transported by Wind During the “Dust Bowl” Days of the 1930’s
Dust from the Sahara Desert is transported by wind toward the Canary Islands. The Sahara is the world’s largest dust source today.
Wind in the desert Wind erosion Wind is a relatively insignificant erosional agent with most erosion in a desert performed by intermittent running water Mechanisms of wind erosion Deflation Lifting of loose material Deflation produces blowouts (shallow depressions) and desert pavement (a surface of coarse pebbles and cobbles)
Formation of a Blowout (A) Area Prior to Deflation (B) Shallow Depression After Deflation Has Removed Fine-Grained, Loose Material
Soil Mound Below The Bush Shows the Land Surface Prior to Blowout Formation
Formation of Desert Pavement Formation of Desert Pavement! If Undisturbed, the Concentrated Layer of Coarse Pebbles Will Prevent Further Erosion, But The Layer is Thin & Easily Disrupted
Undistrubed Desert Pavement
Wind in the desert Wind erosion Mechanisms of wind erosion Abrasion Produces ventifacts (stones with flat faces) and yardangs (wind sculpted ridges) Limited in vertical extent
Ventifacts – Rocks That Are Polished and Shaped by Sandblasting
Wind in the desert Wind deposits Significant depositional landforms are created by wind in some regions Two types of wind deposits Dunes Mounds or ridges of sand Often asymmetrically shaped Windward slope is gently inclined and the leeward slope is called the slip face
Dunes Have an Asymmetrical Shape, with a Gently Sloping Windward Side and a Steeply Dipping Leeward Side (the Slip Face)
The Slip Face is Aptly Named The Slip Face is Aptly Named. Because Grains are at or near the Angle of Repose, they readily Slide Down the Slip Face
Dune Deposits Are Characterized by their Dramatic Cross-Bedding, Which is Produced When Wind Directions Shift
Wind in the desert Wind deposits Two types of wind deposits Dunes Slow migration of dunes occurs in the direction of wind movement Several types of sand dunes are formed, including barchan, transverse, longitudinal, parabolic and star dunes
Dunes Display Various Shapes & Sizes, Controlled by a Combination of Wind Direction & Velocity, Abundance of Sand & Amount of Vegetation
Barchan Dunes – Crescent-Shaped with Tips Pointing Downwind Barchan Dunes – Crescent-Shaped with Tips Pointing Downwind. Form When Sand Supply is Limited & Ground is Flat, Hard & Largely Free of Vegetation Wind Direction
Barchanoid Dunes – Transverse Dunes with Scallops Barchanoid Dunes – Transverse Dunes with Scallops. White Sands National Monument Wind Direction Transverse Dunes – Long Ridges Separated by Troughs. Form When Sand Supply is Abundant, Winds Are Steady & Vegetation is Sparse
Longitudinal Dunes – Long Sand Ridges Somewhat Parallel to the Prevailing Wind. Form When Sand Supply is Moderate & Wind Direction Variable, But Out of the Same Quadrant Parabolic Dunes – Crescent Shaped with Tips Pointing Upwind. Form along Coastlines Where There is a Strong Onshore Wind, Abundant Sand & Vegetation to Stabilize the Dune
Star Dunes – Dunes that Create Isolated Hills of Sand that Display Complex Shapes. Form When Wind Directions Are Variable. Largely Confined to the Sahara & Arabian Deserts
Wind in the desert Wind deposits Two types of wind deposits Loess Blankets of windblown silt Two primary silt sources are deserts and glacial outwash deposits Extensive deposits occur in China and the central United States
Loess Bluff @ 9 feet high along the Mississippi River Loess Bluff @ 9 feet high along the Mississippi River. The Source of the Silt is Glacial Outwash