Urban Heat Island

What Is an Urban Heat Island?

On warm summer days, the air in urban areas can be 6-8°F hotter than its surrounding areas. Scientists call these cities “urban heat islands.” Link to: High Temperatures

What Are Problems with the “Heat Island Effect?”

The higher temperatures in urban heat islands increases air conditioning and raises pollution levels. Link to: Air Quality and Energy Use

What Causes an Urban Heat Island?

Causes of the “heat island effect” include dark surfaces–that absorb more heat from the sun–and less vegetation that would provide shade and cool the air. Link to: Cool Roofs, Cool Pavements, and Vegetation

What Does the Heat Island Group Do?

The Heat Island Group’s research is very diverse and encompasses many areas. For an overview of our projects (updated in 1999), link to: Learn > Overview. For a review of our research (up to 1998), link to: Learn > 1998 Review.

The Heat Island Group also researches new cooling roofing materials. Link to: “Measurements and Database for Cool Roofing Materials”

How Can We Reduce the Heat Island Effect?

The Heat Island Group supports the development of cooler roofing and pavement materials as well as urban planting programs (see links above). The Heat Island Group also develops guideline standards to mitigate the heat island effect through regional and local building design codes. Link to: Learn > “Wholesale Technology Transfer: Standards”

What Would Be the Benefits of These Mitigation Measures?

As well as reduce the temperature, these measures would conserve energy and improve air quality. Link to: “Estimating Energy Saving Potentials of Heat Island Mitigation Measures” and Learn > “Meteorological and Air-Quality Modeling”

In addition, cooler pavements would also be more durable and may also be useful at nighttime. link to: “Benefits of Cooler Pavements”

What’s an Example of a Heat Island?

Los Angeles is a very severe heat island. The Heat Island Group has studied Los Angeles and its surrounding South Coast Air Basin extensively. Link to: Learn > L.A. Island

source:http://heatisland.lbl.gov

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Greenbelts and Rural-Urban Fringe

Greenbelts

Greenbelts were established to prevent the continued growth of many of the largest cities of England and Scotland.

They are rings of heavily protected open land circling an urban area. They aim to protect the surrounding countryside from development, and in some cases stop two large cities from merging. Planning permission is not usually granted for schemes on green belt land, although there is often great pressure to allow some proposals through.

The M25 is built through much of London’s greenbelt. One of the main problems of the greenbelts is that they have led to people commuting further into work.

The Rural-Urban Fringe

 

The Rural-Urban fringe is the name given to the land at the edge of an urban area, where there is often a huge mixture of land uses.

Often science parks, business parks and industrial estates locate in the rural-urban fringe as the land is cheaper, there is room for expansion and they are closer to transport links to allow export and import of goods.

Motorways and by-passes, such as the M25 and the Newbury by-pass have been built on the rural-urban fringe, much to the disgust of environmental groups who feel that the area should be kept as green as possible.

Recreational land-uses such as golf courses and leisure parks have been established in the rural-urban fringe.

Housing has also encroached into the rural-urban fringe, and small villages have grown as more people move out of the cities and commute to work.

Out-of-town shopping centres also find that the space available, good transport connections and cheap land encourage them to establish in the rural-urban fringe.

Farming still occurs in the rural-urban fringe, although the farmers often come under great pressure to sell their land for development. A farmer will make far more money from a sale if there is already planning permission for building to occur on the land.

Source:http://www.s-cool.co.uk

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Landforms of Glaciation

Glaciers have played an important role in the shaping of landscapes in the middle and high latitudes and in alpine environments. Their ability to erode soil and rock, transport sediment, and deposit sediment is extraordinary. During the last glacial period more than 50 million square kilometers of land surface were geomorphically influenced by the presence of glaciers.

Glacial Erosion

Two major erosional processes occur at the base of a glacier. First, at the base of a glacier, large amounts of loose rock and sediment are incorporated into the moving glacial ice by partial melting and refreezing. The second process of erosion involves the abrasive action of the held rock and sediment held by the ice on the surface underneath the glacier. This abrasive process is known as scouring. Scouring creates a variety of features. The most conspicuous feature of scouring is striations. Striations appear as scratches of various size on rock surfaces. In some cases, abrasion can polish the surface of some rock types smooth. This geomorphic feature is known as glacial polish. The abrasive action of scouring also produces a fine clay-sized sediment that is often transported away from the glacier by meltwater. As a result of this process, glacial meltwater can have a light, cloudy appearance, and is called glacial milk.

Glacial striations, Lac Blanchet, Canada. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

The second major erosional process that occurs at the base of a glacier is plucking. Plucking is the process of particle detachment by moving glacial ice. In this process, basal ice freezes in rock surface cracks. As the main body of the glacial ice moves material around the ice in the cracks is pulled and plucked out. The intensity of the plucking process is greatest on the lee-side of rock mounds. When combined with glacial abrasion, the action of plucking on rock mounds produces a unique asymmetrical feature known as roche moutonnee. Roche moutonnee are smooth on the side of ice advancement and steep and jagged on the opposite side.

Glaciers generally flow over the land surface along a path of least resistance. The flow of an alpine glacier into a valley, causes the glacier to rapidly advance producing a swollen tongue of ice at the glacier’s snout, known as a lobe. As the lobe movesdown the valley it often encounters the lobes of other glaciers from connecting valleys. The glacier grows in size with addition of the flow of connected sub-valleys. The following image illustrates one of these networks of connectedalpineglaciers .

Merging alpine glaciers viewed from above (Source: NASA).

A number of distinct erosional features can be observed in mountainous regions that have experienced the effects of glaciation. Much of this erosion is exerted on the bottoms and sides of alpine valleys that guide the flow of glaciers. This erosion causes the bottom and the sides of any glaciated valley to become both wider and deeper over time. Glacial erosion also results in a change in the valley’s cross-sectional shape. Glacial valleys tend to have a pronounced U-shape that contrasts sharply with V-shape valleys created by stream erosion. Small adjoining feeder valleys entering a large valley in a glaciated mountainous region tend to have their floors elevated some distance above the level of the main valley’s floor. Geomorphologist call this landform a hanging valley. Hanging valleys develop because of two reasons: 1) larger, more massive glaciers create greater erosion and subsequently a deeper valley, and 2) some valleys have seen more glacier ice pass through them which also results in more erosion and a deeper valley. Many hanging valleys are also the sites of sensational waterfalls.

Some of the other features associated with glacier erosion in alpine regions are cirques, horns, and arêtes . Cirques are the bowl shaped depressions found at the head of glacial valleys. For most alpine glaciers, cirques are the areas in the alpine valleys where snow first accumulated and was modified into glacial ice. The glaciers that occupy cirques are called cirque glaciers. Horns are pyramidal peaks that form when several cirques chisel a mountain from three or more sides. The most famous horn is the Matterhorn found in the Swiss Alps. Arêtes are the narrow serrated ridges found in glaciated alpine areas. Arêtes form when two opposing cirques back erode a mountain ridge.

Features associated with alpine glaciation.

Talusand otherfoot-slope deposits are also common in a glaciated valley. Because of the enhancement of freeze-thaw processes bedrock in alpine areas is weathered by the growth of ice crystals. This type of weathering shatters the bedrock into sharp angular fragments that accumulate at the bottom of rock slopes as talus. Much of the debris carried by an alpine glacier comes from valley sides where talus accumulates.

The erosional landforms produced by continental glaciers are usually less obvious than those created by alpine glaciers. Like alpine glaciers, the movement of continental glaciers followed topographic trends found in the landscape. Continental ice sheets were very thick, between 1000 to 3000 meters. The mass of these glaciers covered all but the highest features and had extremely strong erosive power. Much of the Canadian Shield shows the effects of abrasion and gouging which created glacial polish and striations on bedrock surfaces. In some areas, continental ice sheets produced huge U-shaped valleys from previously V-shaped stream valleys. In other areas, erosion by the continental ice sheets scooped out large shallow basins, many of which exist today as lakes. Many of the lakes on the Canadian Shield, including those of the Great Lakes, were created by glacial erosion.

Glacial Deposition

A large part of the surface of a glacier is covered with a coating of sediment and rock debris. This is especially prevalent near the snout of the glacier, where most of the ice has been lost to ablation and sediment is left behind. Sediment is added to glacial ice in two ways. Large quantities of sediment are picked up by abrasion and plucking at the base of the ice. In alpine areas, sediment is added to the surface of the glacier from the valley walls through various types of mass movement. Much of the debris that is added to the ice of the glacier is eventually delivered to the snout because of the continual forward flow of glacial ice. From the snout this material can be placed directly from the ice or it can be deposited through the action of flowing meltwater. Geomorphologists call the later deposits glaciofluvialdeposits. The technical term used to describe material deposited by the ice is called till or moraine. All glacial deposits are by and large known as glacial drift.

Till is a heterogeneous combination of unstratified sediments ranging in size from large boulders to minute particles of clay. When till is deposited along the edge of a glacier it tends to form irregular hills and mounds known as moraines. A terminal moraine is a deposit that mark, the farthest advance of a glacier. Moraine deposits created during halts in the retreat of the glacier are called recessionalmoraines. The debris that falls from valley side slopes can be concentrated in a narrow belt and cause a deposit known as a lateral moraine . When two glaciers flow together, two lateral moraines can merge to form an interior belt of debris, called a medial moraine . A till plain is a large, relatively flat plain of till that forms when a sheet of ice becomes detached from the main body of the glacier and melts in place. Sometimes the sediments in a till plain can contain large boulders. If these boulders are transported a great distance from their place of origin, they are called erratics.

Lateral moraines along the sides of the Salmon Glacier, British Columbia, Canada (Photo © Trudy Kavanagh).

Medial moraine down the center of the Salmon Glacier, British Columbia, Canada (Photo © Trudy Kavanagh).

Glacial erratic near Point Lake, Northwest Territories. Glacial erratics are large pieces of rock that have been transported away from their source areas by moving glacial ice sheets. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

Glaciofluvial deposits are generally quite stratified and less sorted in terms of particle size. Outwash deposits are formed when sand is eroded, transported, and deposited by meltwater streams from the glacier’s snout and nearby till deposits to areas in front of the glacier. Outwash plain develops when there are a great number of meltwater streams depositing material ahead of the glacier .

Glacier snout and outwash plain, Bylot Island, Canada. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

Glaciofluvial deposits are also associated with the melting of stagnant ice at the front of the glacier. Where sediment rich water flows into a crevasse or depression in the ice, a conical-shaped pile of sand and gravel, known as a kame, can form (Figure 10af-8). Many kames are often found on or at the edge of moraines.

Kame, La Bluff, Ile de la Grande Entree, Canada. This kame was deposited during the main stage of the last glaciation when the Laurentide ice sheet filled the Gulf of St. lawrence. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

Glaciers can also contain sinuous flows of meltwater that occur in ice tunnels at the base of the ice. The beds of these sub-surface glacial streams are composed of layers of sand and gravel. When the ice melts from around the meltwater tunnels, the beds of sand and gravel are deposited on the Earth’s surface as long twisting ridges known as eskers (Figure 10af-9).

Esker near Lac du Sauvage, Northwest Territories. The slightly curving thin ridge in the centers of this photo is the esker. The flat region in the foreground to the left of the esker was formed by glacial outwash. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

Another feature of continental glaciation are hill shaped deposits of till known as drumlins . Drumlins often occur in large numbers across areas of New York and Wisconsin, USA and Ontario, Canada. The streamline shape of these glacial features resembles a extended teaspoon laying bowl down. The gently sloping tapered end of the drumlin points in the general direction the glacier traveled. Drumlins also come in a variety of dimensions. Lengths can range from 100 to 5000 meters and heights can sometimes exceed 200 meters. A couple theories exist to explain their formation. The most excepted theory suggests they form when saturated ground sediments oozes up into hollows at the base of an advancing glacier. The sediment is then stretched out and molded into a streamline form as the ice moves forward.

Drumlin field in northwestern Manitoba. These features are made of till and are formed at the base of a glacial ice sheet. The long axis of this feature aligns with the direction of glacial movement. (Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

When glaciers are rapidly retreating, numerous blocks of ice can become detached from the main body of the glacier. If glacial drift is then placed around the ice, a depression on the surface called a kettle holecan be created when the ice melts . Kettle holes are commonly found on moraine and outwash plain deposits. Large kettle holes that reach below the water table can form into lakes. The photograph below shows some kettle lakes in glaciofluvial outwash complex located in the Northwestern District of Mackenzie, Northwest Territories . Some kettle holes develop into wetlands such as bogs, swamps, and marshes.

Kettle Lakes, Northwest Territory, Canada.

(Source: Natural Resources Canada – Terrain Sciences Division – Canadian Landscapes).

source:http://www.physicalgeography.net

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Lessons from St. Helens:Science of Prediction of Volcanoes

Giant plume of black smoke pours out of volcano. When earthquakes started jolting Mount St. Helens in March, 1980, little infrastructure was available to monitor the mountain or warn of an eruption. As the quakes continued, scientists scavenged seismographs and surveying equipment to take the mountain’s pulse. Their agenda combined science (What is going on inside the volcano?) and public service (When and how should we warn residents and touristo-gawkers?)

The real thing: During the 1980 eruption, Mount St. Helens spewed superheated ash, rock and gas. Photo: USGS

After a couple of months of nerve-wracking foreplay, St. Helens exploded on May 18. Fifty-seven people died, mainly because the eruption started with a rare but phenomenally powerful sideways blast. Crusty old Harry Truman, who had become a media hero by refusing to leave his compound at Spirit Lake, died under a gigantic landslide.

St. Helens taught scientists a great deal about how volcanoes work — or at least, how that particular volcano works, says Steve Malone, who watched the events from a seismology lab at the University of Washington, where he now heads the Pacific Northwest Seismograph Network.

The experience, he says, was “like a baptism of fire” that “got us a huge leg up” on the difficult problem of predicting eruptions.

Volcanoes give four major categories of information that can serve as a basis for predictions:

Geologic history: What has this volcano done in the past? How regular and frequent were the eruptions, and what did they do?

Land deformation: Rising magma changes the surface in and near the crater. Broad deformation indicates that the magma is deep, while more focused deformation signifies shallow magma, and perhaps an eruption in the near future.

Gas emissions: Rising magma releases gases like carbon dioxide and sulfur dioxide. The timing and intensity of these gases hints at the magma’s location.

Earthquakes: Rising magma must bust through rock, and the resulting quakes may be the best single indication of magma movement.

Each of these factors became the subject of intense scrutiny as St. Helens rocked and rolled in spring, 1980. Just two years before, a U.S. Geological Survey report had predicted that the volcano might erupt before 2000. “It was a long-range forecast based on the geological record” of fairly regular eruptions, says Dan Dzurisin, a volcanologist with the Cascades Volcano Observatory.

...of green vegetation turning to barren rock-scape, and back to green.1973, 1983 and 2000: The time machine at Mount St. Helens. These satellite pix show the area before and after the 1980 eruption, and after 20 years of ecological healing. 284KB Movie: Landsat, NASA

Although there were plenty of warnings, there were no eruption forecasts as such in 1980, Dzurisin says. “Clearly we issued statements anticipating eruptive activity, but the exact timing was difficult to forecast. Even in hindsight, on May 18, 1980, there was nothing we were measuring that could have offered any short-term warning that it would start that morning.”

After the cataclysmic eruption, however, it was easy to find research funding on St. Helens, and the ensuing scientific activity paid off during a series of minor eruptions. “We began to see a pattern repeated … with increased seismicity and deformation of the crater floor,” Dzurisin says. “In most cases, a new lava lobe would extrude onto the surface. From December, 1980, to October, 1986, we successfully predicted each dome-building eruption, at least 18 of them, as far as three weeks in advance, although sometimes it was just hours in advance.” Domes are mounds of lava that form, usually inside the existing crater.

Using seismology only, scientists also predicted four of five explosive eruptions in the summer of 1980, Malone adds.

St. Helens made history, and not just for the giant landslide, says Dzurisin. “For the first time, were willing to step up to the plate and predict the style and timing of eruption events. It’s fair to say this was a watershed, and since then, it has become more common to make specific forecasts.”

Man fiddles with machine mounted on tripod, mountain in background.
Sept. 30, 2004: U.S. Geological Survey scientist Dan Dzurisin collects information from a Global Positioning System station on the east flank of St. Helens. Since intense earthquakes started Sept. 23, more than a dozen GPS stations have measured surface deformation. Photo: Michael Poland, USGS.

Predictive perspicacity
St. Helens offered two types of lessons, says Dzurisin. “There are two aspects to an eruption forecast. One is pattern recognition. If you see the same thing happening repeatedly, you are in a position to forecast the next occurrence. To a large extent, that’s what we used for the dome-building forecasts at Mount St. Helens.”

A second aspect is understanding what’s going on inside an active volcano. “If we understand the processes, even if the pattern changes, we should be in a position to understand why they might have changed, and still provide some form of forecast,” Dzurisin adds. Although achieving such an understanding is “much more difficult,” it’s also potentially more helpful, since it might apply to other volcanoes.

Since 1980, the biggest advances in forecasting have come from seismology, says Dzurisin, who was at the Hawaii Volcano Observatory before St. Helens. “At HVO, we counted the number of quakes per day. …Now, instead of saying, we had 250 quakes yesterday and 324 today, we say” that groundwater or magma seems to be moving inside the volcano, based on the size and shape of traces on the seismograph.

Graph showing jumps in seismic activity of Mount St. Helens. Oct. 6, 2004: Traces of seismic activity at Mount St. Helens. These little squiggles read the heart of the volcano. Courtesy Pacific Northwest Seismograph Network

A successful prediction
In 1991, the lessons of Mount St. Helens were tested in the Philippines, after the ground began shaking around Mount Pinatubo, a short mountain but productive volcano. A collaboration of U.S. and Filipino volcanologists watched, waited, and eventually made an accurate forecast. “There was no question that the learning curve took a huge jump at St. Helens, and they succeeded at Pinatubo, it was a dramatically successful forecast,” says Malone, who adds that he was not involved in Pinatubo.

The Philippine government evacuated tens of thousands of residents, saving massive casualties during the largest eruption of the 20th century. Although gigantic mud flows and ash deposits lead to the closing of two major US military bases, few lives were lost.

Helen’s present
No evacuation warnings have been issued around Mount St. Helens, where, as we write, in October, 2004, magma has risen to a few hundred meters below the surface, and a lava dome is forming in the crater. “The fact that the deformation is very localized tells us that the immediate cause is very shallow,” Dzurisin said.

White and gray clouds of smoke escape from mountainOct. 1, 2004: A small eruption of Mount St. Helens; the first in more than a decade — followed a week of earthquakes beneath the volcano and deformation of the lava dome. This eruption sent a steam and minor ash plume to about 10,000 feet above sea level. Photo: USGS

It’s unlikely that the surface lava flow is being driven by a monster flow deep under the volcano, Dzurisin adds. “If there was a large body of magma pressurizing it,” says Dzurisin, “it would definitely cause ground movement on the outer flank, but we are not seeing that.”

The mountain’s shape is also reassuring, courtesy of the 1980 eruption, Dzurisin adds. “There has been a change in the edifice itself. It was decapitated, so there is no potential for a large landslide, or the large, lateral, directed eruption. That’s off the table.

source:http://whyfiles.org

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