{"id":71,"date":"2014-06-21T03:34:23","date_gmt":"2014-06-21T03:34:23","guid":{"rendered":"https:\/\/courses.candelalearning.com\/env131fmusu14\/?post_type=chapter&#038;p=71"},"modified":"2017-11-07T16:33:34","modified_gmt":"2017-11-07T16:33:34","slug":"glaciers","status":"publish","type":"chapter","link":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/chapter\/glaciers\/","title":{"raw":"Glaciers","rendered":"Glaciers"},"content":{"raw":"A\u00a0<b>glacier<\/b>\u00a0(<small>US<\/small>\u00a0\/\u02c8\u0261le\u026a\u0283\u0259r\/\u00a0or\u00a0<small>UK<\/small>\u00a0\/\u02c8\u0261l\u00e6si\u0259\/) is a persistent body of dense ice that is constantly moving under its own weight; it forms where the accumulation of snow exceeds its ablation (melting and sublimation) over many years, often centuries. Glaciers slowly deform and flow due to stresses induced by their weight, creating crevasses, seracs, and other distinguishing features. They also abrade rock and debris from their substrate to create landforms such as cirques and moraines. Glaciers form only on land and are distinct from the much thinner sea ice and lake ice that form on the surface of bodies of water.\r\n\r\n<a style=\"line-height: 1.5em;\" href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Baltoro_glacier_from_air.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Baltoro_glacier_from_air.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div id=\"mw-content-text\" dir=\"ltr\" lang=\"en\">\r\n<div>\r\n<div>\r\n<div>\r\n\r\nThe Baltoro Glacier in the Karakoram, Baltistan, Northern Pakistan. At 62 kilometres (39\u00a0mi) in length, it is one of the longest alpine glaciers on earth.\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Perito_Moreno_Glacier_Patagonia_Argentina_Luca_Galuzzi_2005.JPG\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Perito_Moreno_Glacier_Patagonia_Argentina_Luca_Galuzzi_2005.JPG\" alt=\"\" width=\"220\" height=\"147\" \/><\/a>\r\n<div>\r\n\r\nIce calving from the terminus of the Perito Moreno Glacier in western Patagonia, Argentina\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Grosser_Aletschgletscher_3178.JPG\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Grosser_Aletschgletscher_3178.JPG\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nThe Aletsch Glacier, the largest glacier of the Alps, in Switzerland\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Quelccaya_Glacier.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Quelccaya_Glacier.jpg\" alt=\"\" width=\"220\" height=\"147\" \/><\/a>\r\n<div>\r\n\r\nThe Quelccaya Ice Cap is the largest glaciated area in the tropics, in Peru\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<span style=\"line-height: 1.5em;\">On Earth, 99% of glacial ice is contained within vast ice sheets in the polar regions, but glaciers may be found in mountain ranges on every continent except Australia, and on a few high-latitude oceanic islands. Between 35\u00b0N and 35\u00b0S, glaciers occur only in the Himalayas, Andes, Rocky Mountains, a few high mountains in East Africa, Mexico, New Guinea and on Zard Kuh in Iran.<\/span><sup id=\"cite_ref-Post_2000_1-0\" style=\"line-height: 1.5em;\"><a href=\"#cite_note-Post_2000-1\">[1]<\/a><\/sup>\r\n\r\nGlacial ice is the largest reservoir of freshwater on Earth.<sup id=\"cite_ref-IMS_2-0\"><a href=\"#cite_note-IMS-2\">[2]<\/a><\/sup>\u00a0Many glaciers from temperate, alpine and seasonal polar climates store water as ice during the colder seasons and release it later in the form of meltwater as warmer summer temperatures cause the glacier to melt, creating a water source that is especially important for plants, animals and human uses when other sources may be scant. Within high altitude and Antarctic environments, the seasonal temperature difference is often not sufficient to release meltwater.\r\n\r\nBecause glacial mass is affected by long-term climate changes, e.g., precipitation, mean temperature, and cloud cover, glacial mass changes are considered among the most sensitive indicators of climate change and are a major source of variations in sea level.\r\n\r\n&nbsp;\r\n<h2>Etymology and related terms<\/h2>\r\nThe word\u00a0<i>glacier<\/i>\u00a0comes from French. It is derived from the Vulgar Latin\u00a0<i>glacia<\/i>\u00a0and ultimately from Latin\u00a0<i>glacies<\/i>\u00a0meaning \"ice\".<sup id=\"cite_ref-3\"><a href=\"#cite_note-3\">[3]<\/a><\/sup>\u00a0The processes and features caused by glaciers and related to them are referred to as\u00a0<b>glacial<\/b>. The process of glacier establishment, growth and flow is called\u00a0<b>glaciation<\/b>. The corresponding area of study is called glaciology. Glaciers are important components of the global cryosphere.\r\n<h2>Types<\/h2>\r\n<div>Main article: Glacier morphology<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacier_mouth.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacier_mouth.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nMouth of the Schlatenkees Glacier near Innergschl\u00f6\u00df, Austria\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nGlaciers are categorized by their morphology, thermal characteristics, and behavior.\u00a0<i>Alpine glaciers,<\/i>\u00a0also known as\u00a0<i>mountain glaciers<\/i>or\u00a0<i>cirque glaciers<\/i>, form on the crests and slopes of mountains. An alpine glacier that fills a valley is sometimes called a\u00a0<i>valley glacier<\/i>. A large body of glacial ice astride a mountain, mountain range, or volcano is termed an ice cap or ice field.<sup id=\"cite_ref-4\"><a href=\"#cite_note-4\">[4]<\/a><\/sup>\u00a0Ice caps have an area less than 50,000\u00a0km\u00b2 (20,000\u00a0mile\u00b2) by definition.\r\n\r\nGlacial bodies larger than 50,000\u00a0km\u00b2 are called ice sheets or continental glaciers.<sup id=\"cite_ref-5\"><a href=\"#cite_note-5\">[5]<\/a><\/sup>\u00a0Several kilometers deep, they obscure the underlying topography. Only\u00a0<i>nunataks<\/i>\u00a0protrude from their surfaces. The only extant ice sheets are the two that cover most of Antarctica and Greenland. They contain vast quantities of fresh water, enough that if both melted, global sea levels would rise by over 70 meters.<sup id=\"cite_ref-6\"><a href=\"#cite_note-6\">[6]<\/a><\/sup>Portions of an ice sheet or cap that extend into water are called\u00a0<i>ice shelves;<\/i>\u00a0they tend to be thin with limited slopes and reduced velocities.<sup id=\"cite_ref-NSIDC_7-0\"><a href=\"#cite_note-NSIDC-7\">[7]<\/a><\/sup>\u00a0Narrow, fast-moving sections of an ice sheet are called\u00a0<i>ice streams.<\/i><sup id=\"cite_ref-8\"><a href=\"#cite_note-8\">[8]<\/a><\/sup><sup id=\"cite_ref-BAS2009_9-0\"><a href=\"#cite_note-BAS2009-9\">[9]<\/a><\/sup>\u00a0In Antarctica, many ice streams drain into large ice shelves. Some drain directly into the sea, often with an ice tongue, like Mertz Glacier.\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Fjordsglacier.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Fjordsglacier.jpg\" alt=\"\" width=\"220\" height=\"144\" \/><\/a>\r\n<div>\r\n\r\nSightseeing boat in front of a tidewater glacier, Kenai Fjords National Park, Alaska\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<i>Tidewater glaciers<\/i>\u00a0are glaciers that terminate in the sea, including most glaciers flowing from Greenland, Antarctica, Baffin and Ellesmere Islands in Canada, Southeast Alaska, and the Northern and Southern Patagonian Ice Fields. As the ice reaches the sea, pieces break off, or\u00a0<i>calve<\/i>, forming icebergs. Most tidewater glaciers calve above sea level, which often results in a tremendous impact as the iceberg strikes the water. Tidewater glaciers undergo centuries-long cycles of advance and retreat that are much less affected by the climate change than those of other glaciers.\r\n\r\nThermally, a\u00a0<i>temperate glacier<\/i>\u00a0is at melting point throughout the year, from its surface to its base. The ice of a\u00a0<i>polar glacier<\/i>\u00a0is always below freezing point from the surface to its base, although the surface snowpack may experience seasonal melting. A\u00a0<i>sub-polar glacier<\/i>includes both temperate and polar ice, depending on depth beneath the surface and position along the length of the glacier. In a similar way, the thermal regime of a glacier is often described by the temperature at its base alone. A\u00a0<i>cold-based<\/i>\u00a0glacier is below freezing at the ice-ground interface, and is thus frozen to the underlying substrate. A\u00a0<i>warm-based<\/i>\u00a0glacier is above or at freezing at the interface, and is able to slide at this contact.<sup id=\"cite_ref-ColdBased_10-0\"><a href=\"#cite_note-ColdBased-10\">[10]<\/a><\/sup>\u00a0This contrast is thought to a large extent to govern the ability of a glacier to effectively erode its bed, as sliding ice promotes plucking at rock from the surface below.<sup id=\"cite_ref-11\"><a href=\"#cite_note-11\">[11]<\/a><\/sup>\u00a0Glaciers which are partly cold-based and partly warm-based are known as\u00a0<i>polythermal<\/i>.<sup id=\"cite_ref-ColdBased_10-1\"><a href=\"#cite_note-ColdBased-10\">[10]<\/a><\/sup>\r\n<h2>Formation<\/h2>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-GornerGlacier_002.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-GornerGlacier_002.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nGorner Glacier in Switzerland\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nGlaciers form where the accumulation of snow and ice exceeds ablation. The area in which a glacier forms is called a cirque (corrie or cwm) - a typically armchair-shaped geological feature (such as a depression between mountains enclosed by ar\u00eates) - which collects and compresses through gravity the snow which falls into it. This snow collects and is compacted by the weight of the snow falling above it forming n\u00e9v\u00e9. Further crushing of the individual snowflakes and squeezing the air from the snow turns it into extremely dense 'glacial ice'. This glacial ice will fill the cirque until it 'overflows' through a geological weakness or vacancy, such as the gap between two mountains. When the mass of snow and ice is sufficiently thick, it begins to move due to a combination of surface slope, gravity and pressure. On steeper slopes, this can occur with as little as 15\u00a0m (50\u00a0ft) of snow-ice.\r\n\r\nIn temperate glaciers, snow repeatedly freezes and thaws, changing into granular ice called firn. Under the pressure of the layers of ice and snow above it, this granular ice fuses into denser and denser firn. Over a period of years, layers of firn undergo further compaction and become glacial ice. Glacier ice is slightly less dense than ice formed from frozen water because it contains tiny trapped air bubbles.\r\n\r\nGlacial ice has a distinctive blue tint because it absorbs some red light due to an overtone of the infrared OH stretching mode of the water molecule. Liquid water is blue for the same reason. The blue of glacier ice is sometimes misattributed to Rayleigh scattering due to bubbles in the ice.<sup id=\"cite_ref-12\"><a href=\"#cite_note-12\">[12]<\/a><\/sup>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-153_-_Glacier_Perito_Moreno_-_Grotte_glaciaire_-_Janvier_2010.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-153_-_Glacier_Perito_Moreno_-_Grotte_glaciaire_-_Janvier_2010.jpg\" alt=\"\" width=\"220\" height=\"151\" \/><\/a>\r\n<div>\r\n\r\nA glacier cave located on the Perito Moreno Glacier in Argentina.\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<h2>Structure<\/h2>\r\nA glacier originates at a location called its\u00a0<i>glacier head<\/i>\u00a0and terminates at its\u00a0<i>glacier foot<\/i>, or terminus.\r\n\r\nGlaciers are broken into zones based on surface snowpack and melt conditions.<sup id=\"cite_ref-13\"><a href=\"#cite_note-13\">[13]<\/a><\/sup>\u00a0The\u00a0<i>ablation zone<\/i>\u00a0is the region where there is a net loss in glacier mass. The\u00a0<i>equilibrium line<\/i>\u00a0separates the ablation zone and the accumulation zone; it is the altitude where the amount of new snow gained by accumulation is equal to the amount of ice lost through ablation. The upper part of a glacier, where accumulation exceeds ablation, is called the\u00a0<i>accumulation zone<\/i>. In general, the accumulation zone accounts for 60\u201370% of the glacier's surface area, more if the glacier calves icebergs. Ice in the accumulation zone is deep enough to exert a downward force that erodes underlying rock. After a glacier melts, it often leaves behind a bowl- or amphitheater-shaped depression that ranges in size from large basins like the Great Lakes to smaller mountain depressions known as cirques.\r\n\r\nThe accumulation zone can be subdivided based on its melt conditions.\r\n<ol>\r\n \t<li>The\u00a0<i>dry snow zone<\/i>\u00a0is a region where no melt occurs, even in the summer, and the snowpack remains dry.<\/li>\r\n \t<li>The\u00a0<i>percolation zone<\/i>\u00a0is an area with some surface melt, causing meltwater to percolate into the snowpack. This zone is often marked by refrozen ice lenses, glands, and layers. The snowpack also never reaches melting point.<\/li>\r\n \t<li>Near the equilibrium line on some glaciers, a\u00a0<i>superimposed ice zone<\/i>\u00a0develops. This zone is where meltwater refreezes as a cold layer in the glacier, forming a continuous mass of ice.<\/li>\r\n \t<li>The\u00a0<i>wet snow zone<\/i>\u00a0is the region where all of the snow deposited since the end of the previous summer has been raised to 0\u00a0\u00b0C.<\/li>\r\n<\/ol>\r\nThe \"health\" of a glacier is usually assessed by determining the glacier mass balance or observing terminus behavior. Healthy glaciers have large accumulation zones, more than 60% of their area snowcovered at the end of the melt season, and a terminus with vigorous flow.\r\n\r\nFollowing the Little Ice Age's end around 1850, glaciers around the Earth have retreated substantially. A slight cooling led to the advance of many alpine glaciers between 1950\u20131985, but since 1985 glacier retreat and mass loss has become larger and increasingly ubiquitous.<sup id=\"cite_ref-14\"><a href=\"#cite_note-14\">[14]<\/a><\/sup><sup id=\"cite_ref-15\"><a href=\"#cite_note-15\">[15]<\/a><\/sup><sup id=\"cite_ref-16\"><a href=\"#cite_note-16\">[16]<\/a><\/sup>\r\n<h2>Motion<\/h2>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Chevron_Crevasses_00.JPG\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Chevron_Crevasses_00.JPG\" alt=\"\" width=\"220\" height=\"147\" \/><\/a>\r\n<div>\r\n\r\nShear or herring-bone crevasses on Emmons Glacier (Mount Rainier); such crevasses often form near the edge of a glacier where interactions with underlying or marginal rock impede flow. In this case, the impediment appears to be some distance from the near margin of the glacier.\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>Main article: Ice sheet dynamics<\/div>\r\nGlaciers move, or flow, downhill due to gravity and the internal deformation of ice.<sup id=\"cite_ref-GreveBlatter2009_17-0\"><a href=\"#cite_note-GreveBlatter2009-17\">[17]<\/a><\/sup>\u00a0Ice behaves like a brittle solid until its thickness exceeds about 50\u00a0m (160\u00a0ft). The pressure on ice deeper than 50\u00a0m causes plastic flow. At the molecular level, ice consists of stacked layers of molecules with relatively weak bonds between layers. When the stress on the layer above exceeds the inter-layer binding strength, it moves faster than the layer below.<sup id=\"cite_ref-18\"><a href=\"#cite_note-18\">[18]<\/a><\/sup>\r\n\r\nGlaciers also move through basal sliding. In this process, a glacier slides over the terrain on which it sits, lubricated by the presence of liquid water. The water is created from ice that melts under high pressure from frictional heating. Basal sliding is dominant in temperate, or warm-based glaciers.\r\n<h3>Fracture zone and cracks<\/h3>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-TitlisIceCracks.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-TitlisIceCracks.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nIce cracks in the Titlis Glacier\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nThe top 50 metres (160\u00a0ft) of a glacier are rigid because they are under low pressure. This upper section is known as the\u00a0<i>fracture zone<\/i>; it mostly moves as a single unit over the plastically flowing lower section. When a glacier moves through irregular terrain, cracks called crevasses develop in the fracture zone. Crevasses form due to differences in glacier velocity. If two rigid sections of a glacier move at different speeds and directions, shear forces cause them to break apart, opening a crevasse. Crevasses are seldom more than 150 feet (46\u00a0m) deep but in some cases can be 1,000 feet (300\u00a0m) or even deeper. Beneath this point, the plasticity of the ice is too great for cracks to form. Intersecting crevasses can create isolated peaks in the ice, called seracs.\r\n\r\nCrevasses can form in several different ways. Transverse crevasses are transverse to flow and form where steeper slopes cause a glacier to accelerate. Longitudinal crevasses form semi-parallel to flow where a glacier expands laterally. Marginal crevasses form from the edge of the glacier, due to the reduction in speed caused by friction of the valley walls. Marginal crevasses are usually largely transverse to flow. Moving glacier ice can sometimes separate from stagnant ice above, forming a\u00a0<i>bergschrund<\/i>. Bergschrunds resemble crevasses but are singular features at a glacier's margins.\r\n\r\nCrevasses make travel over glaciers hazardous, especially when they are hidden by fragile snow bridges.\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/170px-Glaciereaston.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/170px-Glaciereaston.jpg\" alt=\"\" width=\"170\" height=\"227\" \/><\/a>\r\n<div>\r\n\r\nCrossing a crevasse on the Easton Glacier, Mount Baker, in the North Cascades, United States\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nBelow the equilibrium line, glacial meltwater is concentrated in stream channels. Meltwater can pool in proglacial lakes on top of a glacier or descend into the depths of a glacier via moulins. Streams within or beneath a glacier flow in englacial or sub-glacial tunnels. These tunnels sometimes reemerge at the glacier's surface.<sup id=\"cite_ref-19\"><a href=\"#cite_note-19\">[19]<\/a><\/sup>\r\n<h3>Speed<\/h3>\r\nThe speed of glacial displacement is partly determined by friction. Friction makes the ice at the bottom of the glacier move more slowly than ice at the top. In alpine glaciers, friction is also generated at the valley's side walls, which slows the edges relative to the center.\r\n\r\nMean speeds vary greatly, but is typically around 1 meter per day.<sup id=\"cite_ref-20\"><a href=\"#cite_note-20\">[20]<\/a><\/sup>\u00a0There may be no motion in stagnant areas; for example, in parts of Alaska, trees can establish themselves on surface sediment deposits. In other cases, glaciers can move as fast as 20\u201330\u00a0m per day, such as in Greenland's Jakobshavn Isbr\u00e6 (Greenlandic:\u00a0<i>Sermeq Kujalleq<\/i>). Velocity increases with increasing slope, increasing thickness, increasing snowfall, increasing longitudinal confinement, increasing basal temperature, increasing meltwater production and reduced bed hardness.\r\n\r\nA few glaciers have periods of very rapid advancement called surges. These glaciers exhibit normal movement until suddenly they accelerate, then return to their previous state. During these surges, the glacier may reach velocities far greater than normal speed.<sup id=\"cite_ref-21\"><a href=\"#cite_note-21\">[21]<\/a><\/sup>\u00a0These surges may be caused by failure of the underlying bedrock, the pooling of meltwater at the base of the glacier<sup id=\"cite_ref-22\"><a href=\"#cite_note-22\">[22]<\/a><\/sup>\u00a0\u2014 perhaps delivered from a supraglacial lake\u00a0\u2014 or the simple accumulation of mass beyond a critical \"tipping point\".<sup id=\"cite_ref-23\"><a href=\"#cite_note-23\">[23]<\/a><\/sup>\r\n\r\nIn glaciated areas where the glacier moves faster than one km per year, glacial earthquakes occur. These are large scale tremblors that have seismic magnitudes as high as 6.1.<sup id=\"cite_ref-people.deas.harvard.edu_24-0\"><a href=\"#cite_note-people.deas.harvard.edu-24\">[24]<\/a><\/sup><sup id=\"cite_ref-TsaiEkstrom_JGR2007_2007_25-0\"><a href=\"#cite_note-TsaiEkstrom_JGR2007_2007-25\">[25]<\/a><\/sup>\u00a0The number of glacial earthquakes in Greenland peaks every year in July, August and September and is increasing over time. In a study using data from January 1993 through October 2005, more events were detected every year since 2002, and twice as many events were recorded in 2005 as there were in any other year. This increase in the numbers of glacial earthquakes in Greenland may be a response to global warming.<sup id=\"cite_ref-people.deas.harvard.edu_24-1\"><a href=\"#cite_note-people.deas.harvard.edu-24\">[24]<\/a><\/sup><sup id=\"cite_ref-TsaiEkstrom_JGR2007_2007_25-1\"><a href=\"#cite_note-TsaiEkstrom_JGR2007_2007-25\">[25]<\/a><\/sup>\r\n<h3>Ogives<\/h3>\r\n<i>Ogives<\/i>\u00a0are alternating wave crests and valleys that appear as dark and light bands of ice on glacier surfaces. They are linked to seasonal motion of glaciers; the width of one dark and one light band generally equals the annual movement of the glacier. Ogives are formed when ice from an icefall is severely broken up, increasing ablation surface area during summer. This creates a swale and space for snow accumulation in the winter, which in turn creates a ridge.<sup id=\"cite_ref-26\"><a href=\"#cite_note-26\">[26]<\/a><\/sup>\u00a0Sometimes ogives consist only of undulations or color bands and are described as wave ogives or band ogives.<sup id=\"cite_ref-27\"><a href=\"#cite_note-27\">[27]<\/a><\/sup>\r\n<h2>Geography<\/h2>\r\n<div>For more details on this topic, see List of glaciers, and Retreat of glaciers since 1850.<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Black-Glacier.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Black-Glacier.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nBlack ice glacier near Aconcagua, Argentina\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nGlaciers are present on every continent and approximately fifty countries, excluding those (Australia, South Africa) that have glaciers only on distant subantarctic island territories. Extensive glaciers are found in Antarctica, Chile, Canada, Alaska, Greenland and Iceland. Mountain glaciers are widespread, especially in the Andes, the Himalayas, the Rocky Mountains, the Caucasus, and the Alps. Mainland Australia currently contains no glaciers, although a small glacier on Mount Kosciuszko was present in the last glacial period.<sup id=\"cite_ref-28\"><a href=\"#cite_note-28\">[28]<\/a><\/sup>\u00a0In New Guinea, small, rapidly diminishing, glaciers are located on its highest summit massif of Puncak Jaya.<sup id=\"cite_ref-29\"><a href=\"#cite_note-29\">[29]<\/a><\/sup>\u00a0Africa has glaciers on Mount Kilimanjaro in Tanzania, on Mount Kenya and in the Rwenzori Mountains. Oceanic islands with glaciers occur on Iceland, Svalbard, New Zealand, Jan Mayen and the subantarctic islands of Marion, Heard, Grande Terre (Kerguelen) and Bouvet. During glacial periods of the Quaternary, Taiwan, Hawaii on Mauna Kea<sup id=\"cite_ref-30\"><a href=\"#cite_note-30\">[30]<\/a><\/sup>\u00a0and Tenerife also had large alpine glaciers, while the Faroe and Crozet Islands<sup id=\"cite_ref-31\"><a href=\"#cite_note-31\">[31]<\/a><\/sup>\u00a0were completely glaciated.\r\n\r\nThe permanent snow cover necessary for glacier formation is affected by factors such as the degree of slope on the land, amount of snowfall and the winds. Glaciers can be found in all latitudes except from 20\u00b0 to 27\u00b0 north and south of the equator where the presence of the descending limb of the Hadley circulation lowers precipitation so much that with high insolation snow lines reach above 6,500 metres (21,330\u00a0ft). Between 19\u02daN and 19\u02daS, however, precipitation is higher and the mountains above 5,000 metres (16,400\u00a0ft) usually have permanent snow.\r\n\r\nEven at high latitudes, glacier formation is not inevitable. Areas of the Arctic, such as Banks Island, and the McMurdo Dry Valleys in Antarctica are considered polar deserts where glaciers cannot form because they receive little snowfall despite the bitter cold. Cold air, unlike warm air, is unable to transport much water vapor. Even during glacial periods of the Quaternary, Manchuria, lowland Siberia,<sup id=\"cite_ref-32\"><a href=\"#cite_note-32\">[32]<\/a><\/sup>and central and northern Alaska,<sup id=\"cite_ref-33\"><a href=\"#cite_note-33\">[33]<\/a><\/sup>\u00a0though extraordinarily cold, had such light snowfall that glaciers could not form.<sup id=\"cite_ref-34\"><a href=\"#cite_note-34\">[34]<\/a><\/sup><sup id=\"cite_ref-35\"><a href=\"#cite_note-35\">[35]<\/a><\/sup>\r\n\r\nIn addition to the dry, unglaciated polar regions, some mountains and volcanoes in Bolivia, Chile and Argentina are high (4,500 metres (14,800\u00a0ft) - 6,900\u00a0m (22,600\u00a0ft)) and cold, but the relative lack of precipitation prevents snow from accumulating into glaciers. This is because these peaks are located near or in the hyperarid Atacama Desert.\r\n<h2>Glacial geology<\/h2>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Arranque_glaciar-en.svg.png\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Arranque_glaciar-en.svg.png\" alt=\"\" width=\"220\" height=\"132\" \/><\/a>\r\n<div>\r\n\r\nDiagram of glacial plucking and abrasion\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-PluckedGraniteAlandIslands.JPG\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-PluckedGraniteAlandIslands.JPG\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nGlacially plucked granitic bedrock near Mariehamn, \u00c5land Islands\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nGlaciers erode terrain through two principal processes:\u00a0<b>abrasion<\/b>\u00a0and\u00a0<b>plucking.<\/b>\r\n\r\nAs glaciers flow over bedrock, they soften and lift blocks of rock into the ice. This process, called plucking, is caused by subglacial water that penetrates fractures in the bedrock and subsequently freezes and expands. This expansion causes the ice to act as a lever that loosens the rock by lifting it. Thus, sediments of all sizes become part of the glacier's load. If a retreating glacier gains enough debris, it may become a rock glacier, like the Timpanogos Glacier in Utah.\r\n\r\nAbrasion occurs when the ice and its load of rock fragments slide over bedrock and function as sandpaper, smoothing and polishing the bedrock below. The pulverized rock this process produces is called rock flour and is made up of rock grains between 0.002 and 0.00625\u00a0mm in size. Abrasion leads to steeper valley walls and mountain slopes in alpine settings, which can cause avalanches and rock slides. These add even more material to the glacier.\r\n\r\nGlacial abrasion is commonly characterized by glacial striations. Glaciers produce these when they contain large boulders that carve long scratches in the bedrock. By mapping the direction of the striations, researchers can determine the direction of the glacier's movement. Similar to striations are chatter marks, lines of crescent-shape depressions in the rock underlying a glacier. They are formed by abrasion when boulders in the glacier are repeatedly caught and released as they are dragged along the bedrock.\r\n\r\nThe rate of glacier erosion is variable. Six factors control erosion rate:\r\n<ul>\r\n \t<li>Velocity of glacial movement<\/li>\r\n \t<li>Thickness of the ice<\/li>\r\n \t<li>Shape, abundance and hardness of rock fragments contained in the ice at the bottom of the glacier<\/li>\r\n \t<li>Relative ease of erosion of the surface under the glacier<\/li>\r\n \t<li>Thermal conditions at the glacier base<\/li>\r\n \t<li>Permeability and water pressure at the glacier base<\/li>\r\n<\/ul>\r\nMaterial that becomes incorporated in a glacier is typically carried as far as the zone of ablation before being deposited. Glacial deposits are of two distinct types:\r\n<ul>\r\n \t<li><i>Glacial till<\/i>: material directly deposited from glacial ice. Till includes a mixture of undifferentiated material ranging from clay size to boulders, the usual composition of a moraine.<\/li>\r\n \t<li><i>Fluvial and outwash sediments<\/i>: sediments deposited by water. These deposits are stratified by size.<\/li>\r\n<\/ul>\r\nLarger pieces of rock that are encrusted in till or deposited on the surface are called \"glacial erratics\". They range in size from pebbles to boulders, but as they are often moved great distances, they may be drastically different from the material upon which they are found. Patterns of glacial erratics hint at past glacial motions.\r\n<h3>Moraines<\/h3>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-MorainesLakeLouise.JPG\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-MorainesLakeLouise.JPG\" alt=\"\" width=\"220\" height=\"158\" \/><\/a>\r\n<div>\r\n\r\nGlacial moraines above Lake Louise, Alberta, Canada\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nGlacial moraines are formed by the deposition of material from a glacier and are exposed after the glacier has retreated. They usually appear as linear mounds of till, a non-sorted mixture of rock, gravel and boulders within a matrix of a fine powdery material. Terminal or end moraines are formed at the foot or terminal end of a glacier. Lateral moraines are formed on the sides of the glacier. Medial moraines are formed when two different glaciers merge and the lateral moraines of each coalesce to form a moraine in the middle of the combined glacier. Less apparent are ground moraines, also called\u00a0<i>glacial drift<\/i>, which often blankets the surface underneath the glacier downslope from the equilibrium line.\r\n\r\nThe term\u00a0<i>moraine<\/i>\u00a0is of French origin. It was coined by peasants to describe alluvial embankments and rims found near the margins of glaciers in the French Alps. In modern geology, the term is used more broadly, and is applied to a series of formations, all of which are composed of till. Moraines can also create moraine dammed lakes.\r\n<h3>Drumlins<\/h3>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/249px-Drumlins_LMB.svg.png\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/249px-Drumlins_LMB.svg.png\" alt=\"\" width=\"249\" height=\"109\" \/><\/a>\r\n<div>A drumlin field forms after a glacier has modified the landscape. The teardrop-shaped formations denote the direction of the ice flow.<\/div>\r\n<\/div>\r\n<\/div>\r\nDrumlins are asymmetrical, canoe shaped hills made mainly of till. Their heights vary from 15 to 50\u00a0meters and they can reach a kilometer in length. The tilted side of the hill faces the direction from which the ice advanced (<i>stoss<\/i>), while the longer slope follows the ice's direction of movement (<i>lee<\/i>).\r\n\r\nDrumlins are found in groups called\u00a0<i>drumlin fields<\/i>\u00a0or\u00a0<i>drumlin camps<\/i>. One of these fields is found east of Rochester, New York; it is estimated to contain about 10,000 drumlins.\r\n\r\nAlthough the process that forms drumlins is not fully understood, their shape implies that they are products of the plastic deformation zone of ancient glaciers. It is believed that many drumlins were formed when glaciers advanced over and altered the deposits of earlier glaciers.\r\n<h3>Glacial valleys, cirques, ar\u00eates, and pyramidal peaks<\/h3>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacial_landscape.svg.png\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacial_landscape.svg.png\" alt=\"\" width=\"220\" height=\"130\" \/><\/a>\r\n<div>\r\n\r\nFeatures of a glacial landscape\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nBefore glaciation, mountain valleys have a characteristic \"V\" shape, produced by eroding water. During glaciation, these valleys are widened, deepened, and smoothed, forming a \"U\"-shaped glacial valley. The erosion that creates glacial valleys eliminates the spurs of earth that extend across mountain valleys, creating triangular cliffs called truncated spurs. Within glacial valleys, depressions created by plucking and abrasion can be filled by lakes, called paternoster lakes. If a glacial valley runs into a large body of water, it forms a fjord.\r\n\r\nMany glaciers deepen their valleys more than their smaller tributaries. Therefore, when glaciers recede, the valleys of the tributary glaciers remain above the main glacier's depression and are called hanging valleys.\r\n\r\nAt the start of a classic valley glacier is a bowl-shaped cirque, which has escarped walls on three sides but is open on the side that descends into the valley. Cirques are where ice begins to accumulate in a glacier. Two glacial cirques may form back to back and erode their backwalls until only a narrow ridge, called an ar\u00eate is left. This structure may result in a mountain pass. If multiple cirques encircle a single mountain, they create pointed pyramidal peaks; particularly steep examples are called horns.\r\n<h3>Roche moutonn\u00e9e<\/h3>\r\nSome rock formations in the path of a glacier are sculpted into small hills called\u00a0<i>roche moutonn\u00e9e,<\/i>\u00a0or \"sheepback\" rock. Roche moutonn\u00e9e are elongated, rounded, and asymmetrical bedrock knobs can be produced by glacier erosion. They range in length from less than a meter to several hundred meters long.<sup id=\"cite_ref-36\"><a href=\"#cite_note-36\">[36]<\/a><\/sup>\u00a0Roche moutonn\u00e9e have a gentle slope on their up-glacier sides and a steep to vertical face on their down-glacier sides. The glacier abrades the smooth slope on the upstream side as it flows along, but tears loose and carries away rock from the downstream side via plucking.\r\n<h3>Alluvial stratification<\/h3>\r\nAs the water that rises from the ablation zone moves away from the glacier, it carries fine eroded sediments with it. As the speed of the water decreases, so does its capacity to carry objects in suspension. The water thus gradually deposits the sediment as it runs, creating an alluvial plain. When this phenomenon occurs in a valley, it is called a\u00a0<i>valley train<\/i>. When the deposition is in an estuary, the sediments are known as bay mud.\r\n\r\nOutwash plains and valley trains are usually accompanied by basins known as \"kettles\". These are small lakes formed when large ice blocks that are trapped in alluvium melt and produce water-filled depressions. Kettle diameters range from 5\u00a0m to 13\u00a0km, with depths of up to 45\u00a0meters. Most are circular in shape because the blocks of ice that formed them were rounded as they melted.<sup id=\"cite_ref-britannica_37-0\"><a href=\"#cite_note-britannica-37\">[37]<\/a><\/sup>\r\n<h3>Glacial deposits<\/h3>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Receding_glacier-en.svg.png\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Receding_glacier-en.svg.png\" alt=\"\" width=\"220\" height=\"103\" \/><\/a>\r\n<div>\r\n\r\nLandscape produced by a receding glacier\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\nWhen a glacier's size shrinks below a critical point, its flow stops and it becomes stationary. Meanwhile, meltwater within and beneath the ice leaves stratified alluvial deposits. These deposits, in the forms of columns, terraces and clusters, remain after the glacier melts and are known as \"glacial deposits\".\r\n\r\nGlacial deposits that take the shape of hills or mounds are called\u00a0<i>kames<\/i>. Some kames form when meltwater deposits sediments through openings in the interior of the ice. Others are produced by fans or deltas created by meltwater. When the glacial ice occupies a valley, it can form terraces or kames along the sides of the valley.\r\n\r\nLong, sinuous glacial deposits are called\u00a0<i>eskers<\/i>. Eskers are composed of sand and gravel that was deposited by meltwater streams that flowed through ice tunnels within or beneath a glacier. They remain after the ice melts, with heights exceeding 100\u00a0meters and lengths of as long as 100\u00a0km.\r\n<h3>Loess deposits<\/h3>\r\nVery fine glacial sediments or rock flour is often picked up by wind blowing over the bare surface and may be deposited great distances from the original fluvial deposition site. These eolian loess deposits may be very deep, even hundreds of meters, as in areas of China and the Midwestern United States of America. Katabatic winds can be important in this process.\r\n<h2>Isostatic rebound<\/h2>\r\n<div>Main article: Isostatic rebound<\/div>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/Glacier_weight_effects_LMB.png\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/Glacier_weight_effects_LMB.png\" alt=\"\" width=\"482\" height=\"174\" \/><\/a>\r\n<div>Isostatic pressure by a glacier on the Earth's crust<\/div>\r\n<\/div>\r\n<\/div>\r\nLarge masses, such as ice sheets or glaciers, can depress the crust of the Earth into the mantle. The depression usually totals a third of the ice sheet or glacier's thickness. After the ice sheet or glacier melts, the mantle begins to flow back to its original position, pushing the crust back up. This post-glacial rebound, which proceeds very slowly after the melting of the ice sheet or glacier, is currently occurring in measurable amounts in Scandinavia and the Great Lakes region of North America.\r\n\r\nA geomorphological feature created by the same process on a smaller scale is known as\u00a0<i>dilation-faulting<\/i>. It occurs where previously compressed rock is allowed to return to its original shape more rapidly than can be maintained without faulting. This leads to an effect similar to what would be seen if the rock were hit by a large hammer. Dilation faulting can be observed in recently de-glaciated parts of Iceland and Cumbria.\r\n<h2>On Mars<\/h2>\r\n<div>\r\n<div>\r\n\r\n<a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Mars_north_pole.jpg\"><img src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Mars_north_pole.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a>\r\n<div>\r\n\r\nNorthern polar ice cap on Mars\r\n\r\n<\/div>\r\n<\/div>\r\n<\/div>\r\n<div>Main article: Glaciers on Mars<\/div>\r\nThe polar ice caps of Mars show geologic evidence of glacial deposits. The south polar cap is especially comparable to glaciers on Earth.<sup id=\"cite_ref-38\"><a href=\"#cite_note-38\">[38]<\/a><\/sup>\u00a0Topographical features and computer models indicate the existence of more glaciers in Mars' past.<sup id=\"cite_ref-39\"><a href=\"#cite_note-39\">[39]<\/a><\/sup>\r\n\r\nAt mid-latitudes, between 35\u00b0 and 65\u00b0 north or south, Martian glaciers are affected by the thin Martian atmosphere. Because of the low atmospheric pressure, ablation near the surface is solely due to sublimation, not melting. As on Earth, many glaciers are covered with a layer of rocks which insulates the ice. A radar instrument on board the Mars Reconnaissance Orbiter found ice under a thin layer of rocks in formations called Lobate Debris Aprons (LDAs).<sup id=\"cite_ref-40\"><a href=\"#cite_note-40\">[40]<\/a><\/sup><sup id=\"cite_ref-41\"><a href=\"#cite_note-41\">[41]<\/a><\/sup><sup id=\"cite_ref-42\"><a href=\"#cite_note-42\">[42]<\/a><\/sup><sup id=\"cite_ref-43\"><a href=\"#cite_note-43\">[43]<\/a><\/sup><sup id=\"cite_ref-44\"><a href=\"#cite_note-44\">[44]<\/a><\/sup>\r\n<h2>Notes<\/h2>\r\n<div>\r\n<ol>\r\n \t<li id=\"cite_note-Post_2000-1\"><b><a href=\"#cite_ref-Post_2000_1-0\">^<\/a><\/b>\u00a0Post, Austin; LaChapelle, Edward R (2000).\u00a0<i>Glacier ice<\/i>. Seattle, Washington: University of Washington Press. ISBN\u00a00-295-97910-0.<\/li>\r\n \t<li id=\"cite_note-IMS-2\"><b><a href=\"#cite_ref-IMS_2-0\">^<\/a><\/b>\u00a0Brown, Molly Elizabeth; Ouyang, Hua; Habib, Shahid; Shrestha, Basanta; Shrestha, Mandira; Panday, Prajjwal; Tzortziou, Maria; Policelli, Frederick; Artan, Guleid; Giriraj, Amarnath; Bajracharya, Sagar R.; Racoviteanu, Adina.\u00a0<a href=\"http:\/\/hdl.handle.net\/2060\/20110015312\" rel=\"nofollow\">\"HIMALA: Climate Impacts on Glaciers, Snow, and Hydrology in the Himalayan Region\"<\/a>.\u00a0<i>Mountain Research and Development<\/i>. International Mountain Society. Retrieved 16 September 2011.<\/li>\r\n \t<li id=\"cite_note-3\"><b><a href=\"#cite_ref-3\">^<\/a><\/b>\u00a0Simpson, D.P. (1979).\u00a0<i>Cassell's Latin Dictionary<\/i>\u00a0(5 ed.). London: Cassell Ltd. p.\u00a0883. ISBN\u00a00-304-52257-0.<\/li>\r\n \t<li id=\"cite_note-4\"><b><a href=\"#cite_ref-4\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nichols.edu\/departments\/glacier\/juneau%20icefield.htm\" rel=\"nofollow\">\"Retreat of Alaskan glacier Juneau icefield\"<\/a>. Nichols.edu. Retrieved 2009-01-05.<\/li>\r\n \t<li id=\"cite_note-5\"><b><a href=\"#cite_ref-5\">^<\/a><\/b>\u00a0<a href=\"http:\/\/amsglossary.allenpress.com\/glossary\/search?id=ice-sheet1\" rel=\"nofollow\">\"American Meteorological Society, Glossary of Meteorology\"<\/a>. Amsglossary.allenpress.com. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-6\"><b><a href=\"#cite_ref-6\">^<\/a><\/b>\u00a0<a href=\"http:\/\/pubs.usgs.gov\/fs\/fs2-00\/\" rel=\"nofollow\">\"Sea Level and Climate\"<\/a>.\u00a0<i>USGS FS 002-00<\/i>. USGS. 2000-01-31. Retrieved 2009-01-05.<\/li>\r\n \t<li id=\"cite_note-NSIDC-7\"><b><a href=\"#cite_ref-NSIDC_7-0\">^<\/a><\/b>\u00a0*\u00a0National Snow and Ice Data Center.\u00a0<a href=\"http:\/\/www.nsidc.org\/glaciers\/questions\/types.html\" rel=\"nofollow\">\"Types of Glacier\"<\/a>.<\/li>\r\n \t<li id=\"cite_note-8\"><b><a href=\"#cite_ref-8\">^<\/a><\/b>\u00a0Bindschadler, R.A. and T.A. Scambos. Satellite-image-derived velocity field of an Antarctic ice stream.\u00a0<i>Science<\/i>, 252(5003), 242-246, 1991<\/li>\r\n \t<li id=\"cite_note-BAS2009-9\"><b><a href=\"#cite_ref-BAS2009_9-0\">^<\/a><\/b>\u00a0British Antarctic Survey.\u00a0<a href=\"http:\/\/www.antarctica.ac.uk\/\/about_antarctica\/geography\/ice\/streams.php\" rel=\"nofollow\">\"Description of Ice Streams\"<\/a>. Retrieved 2009-01-26.<\/li>\r\n \t<li id=\"cite_note-ColdBased-10\">^\u00a0<a href=\"#cite_ref-ColdBased_10-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-ColdBased_10-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/link.springer.com\/referenceworkentry\/10.1007%2F978-90-481-2642-2_72\/fulltext.html\" rel=\"nofollow\">http:\/\/link.springer.com\/referenceworkentry\/10.1007%2F978-90-481-2642-2_72\/fulltext.html<\/a><\/li>\r\n \t<li id=\"cite_note-11\"><b><a href=\"#cite_ref-11\">^<\/a><\/b>\u00a0Boulton, G.S. [1974] \"Processes and patterns of glacial erosion\", (In Coates, D.R. ed.,\u00a0<i>Glacial Geomorphology<\/i>. A Proceedings Volume of the fifth Annual Geomorphology Symposia series, held at Binghamton, New York, September 26\u201328, 1974. Binghamton, N.Y., State University of New York, p. 41-87. (Publications in Geomorphology))<\/li>\r\n \t<li id=\"cite_note-12\"><b><a href=\"#cite_ref-12\">^<\/a><\/b>\u00a0<a href=\"http:\/\/webexhibits.org\/causesofcolor\/5C.html\" rel=\"nofollow\">\"What causes the blue color that sometimes appears in snow and ice\u00a0?\"<\/a>. Webexhibits.org. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-13\"><b><a href=\"#cite_ref-13\">^<\/a><\/b>\u00a0Benson, C.S., 1961, \"Stratigraphic studies in the snow and firn of the Greenland Ice Sheet\",\u00a0<i>Res. Rep. 70<\/i>, U.S. Army Snow, Ice and Permafrost Res Establ., Corps of Eng., 120 pp<\/li>\r\n \t<li id=\"cite_note-14\"><b><a href=\"#cite_ref-14\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.grid.unep.ch\/activities\/global_change\/switzerland.php\" rel=\"nofollow\">\"Glacier change and related hazards in Switzerland\"<\/a>. UNEP. Retrieved 2009-01-05.<\/li>\r\n \t<li id=\"cite_note-15\"><b><a href=\"#cite_ref-15\">^<\/a><\/b>\u00a0<a href=\"http:\/\/folk.uio.no\/kaeaeb\/publications\/grl04_paul.pdf\" rel=\"nofollow\">\"Frank Paul, et al., 2004, Rapid disintegration of Alpine glaciers observed with satellite data, GEOPHYSICAL RESEARCH LETTERS, VOL. 31, L21402, {{doi|10.1029\/2004GL020816}}\"<\/a>\u00a0(PDF). 2004.<\/li>\r\n \t<li id=\"cite_note-16\"><b><a href=\"#cite_ref-16\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nichols.edu\/departments\/Glacier\/glacier_retreat.htm\" rel=\"nofollow\">\"Recent Global Glacier Retreat Overview\"<\/a>\u00a0(PDF). Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-GreveBlatter2009-17\"><b><a href=\"#cite_ref-GreveBlatter2009_17-0\">^<\/a><\/b>\u00a0Greve, R.; Blatter, H. (2009).\u00a0<i>Dynamics of Ice Sheets and Glaciers<\/i>. Springer. doi:<a href=\"http:\/\/dx.doi.org\/10.1007%2F978-3-642-03415-2\" rel=\"nofollow\">10.1007\/978-3-642-03415-2<\/a>. ISBN\u00a0978-3-642-03414-5.<\/li>\r\n \t<li id=\"cite_note-18\"><b><a href=\"#cite_ref-18\">^<\/a><\/b>\u00a0W.S.B. Paterson, Physics of ice<\/li>\r\n \t<li id=\"cite_note-19\"><b><a href=\"#cite_ref-19\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nasa.gov\/vision\/earth\/lookingatearth\/moulin-20061211.html\" rel=\"nofollow\">\"Moulin 'Blanc': NASA Expedition Probes Deep Within a Greenland Glacier\"<\/a>. NASA. 2006-12-11. Retrieved 2009-01-05.<\/li>\r\n \t<li id=\"cite_note-20\"><b><a href=\"#cite_ref-20\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.geo.hunter.cuny.edu\/tbw\/ncc\/Notes\/chap3.landforms\/erosion.deposition\/glaciers.htm\" rel=\"nofollow\">Glacier properties Hunter College CUNY lectures<\/a><\/li>\r\n \t<li id=\"cite_note-21\"><b><a href=\"#cite_ref-21\">^<\/a><\/b>\u00a0<a href=\"http:\/\/earth.esa.int\/pub\/ESA_DOC\/gothenburg\/154stroz.pdf\" rel=\"nofollow\">T. Strozzi et al.:\u00a0<i>The Evolution of a Glacier Surge Observed with the ERS Satellites<\/i><\/a>\u00a0(pdf, 1.3 Mb)<\/li>\r\n \t<li id=\"cite_note-22\"><b><a href=\"#cite_ref-22\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.hi.is\/~oi\/bruarjokull_project.htm\" rel=\"nofollow\">\"The Br\u00faarj\u00f6kull Project: Sedimentary environments of a surging glacier. The Br\u00faarj\u00f6kull Project research idea\"<\/a>. Hi.is. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-23\"><b><a href=\"#cite_ref-23\">^<\/a><\/b>\u00a0Meier &amp; Post (1969)<\/li>\r\n \t<li id=\"cite_note-people.deas.harvard.edu-24\">^\u00a0<a href=\"#cite_ref-people.deas.harvard.edu_24-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-people.deas.harvard.edu_24-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/people.deas.harvard.edu\/~vtsai\/files\/EkstromNettlesTsai_Science2006.pdf\" rel=\"nofollow\">http:\/\/people.deas.harvard.edu\/~vtsai\/files\/EkstromNettlesTsai_Science2006.pdf<\/a>\u00a0Ekstr\u00f6m, G., M. Nettles, and V. C. Tsai (2006)\"Seasonality and Increasing Frequency of Greenland Glacial Earthquakes\",\u00a0<i>Science<\/i>, 311, 5768, 1756-1758, doi:<a href=\"http:\/\/dx.doi.org\/10.1126%2Fscience.1122112\" rel=\"nofollow\">10.1126\/science.1122112<\/a><\/li>\r\n \t<li id=\"cite_note-TsaiEkstrom_JGR2007_2007-25\">^\u00a0<a href=\"#cite_ref-TsaiEkstrom_JGR2007_2007_25-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-TsaiEkstrom_JGR2007_2007_25-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/people.deas.harvard.edu\/~vtsai\/files\/TsaiEkstrom_JGR2007.pdf\" rel=\"nofollow\">http:\/\/people.deas.harvard.edu\/~vtsai\/files\/TsaiEkstrom_JGR2007.pdf<\/a>\u00a0Tsai, V. C. and G. Ekstr\u00f6m (2007). \"Analysis of Glacial Earthquakes\", J. Geophys. Res., 112, F03S22, doi:<a href=\"http:\/\/dx.doi.org\/10.1029%2F2006JF000596\" rel=\"nofollow\">10.1029\/2006JF000596<\/a><\/li>\r\n \t<li id=\"cite_note-26\"><b><a href=\"#cite_ref-26\">^<\/a><\/b>\u00a0Easterbrook, D.J. (1999).\u00a0<i>Surface Processes and Landforms<\/i>\u00a0(2 ed.). New Jersey: Prentice-Hall, Inc. p.\u00a0546. ISBN\u00a00-13-860958-6.<\/li>\r\n \t<li id=\"cite_note-27\"><b><a href=\"#cite_ref-27\">^<\/a><\/b>\u00a0<a href=\"http:\/\/pubs.usgs.gov\/of\/2004\/1216\/no\/no.html\" rel=\"nofollow\">\"Glossary of Glacier Terminology\"<\/a>. Pubs.usgs.gov. 2012-06-20. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-28\"><b><a href=\"#cite_ref-28\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.ga.gov.au\/education\/facts\/landforms\/auslform.htm\" rel=\"nofollow\">\"C.D. Ollier: ''Australian Landforms and their History'', National Mapping Fab, Geoscience Australia\"<\/a>. Ga.gov.au. 2010-11-18. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-29\"><b><a href=\"#cite_ref-29\">^<\/a><\/b>\u00a0KINCAID, JONI L.; KLEIN, ANDREW G. (2004).\u00a0<a href=\"http:\/\/www.easternsnow.org\/proceedings\/2004\/kincaid_and_klein.pdf\" rel=\"nofollow\">\"Retreat of the Irian Jaya Glaciers from 2000 to 2002 as Measured from IKONOS Satellite Images\"<\/a>. Portland, Maine, USA. pp.\u00a0147\u2013157. Retrieved 2009-01-05.<\/li>\r\n \t<li id=\"cite_note-30\"><b><a href=\"#cite_ref-30\">^<\/a><\/b>\u00a0<a href=\"http:\/\/geology.com\/press-release\/hawiian-glaciers\/\" rel=\"nofollow\">\"Hawaiian Glaciers Reveal Clues to Global Climate Change\"<\/a>. Geology.com. 2007-01-26. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-31\"><b><a href=\"#cite_ref-31\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.discoverfrance.net\/Colonies\/Crozet.shtml\" rel=\"nofollow\">\"French Colonies - Crozet Archipelago\"<\/a>. Discoverfrance.net. 2010-12-09. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-32\"><b><a href=\"#cite_ref-32\">^<\/a><\/b>\u00a0Collins, Henry Hill;\u00a0<b>Europe and the USSR<\/b>; p. 263. ISBN 1-256-35000-3<\/li>\r\n \t<li id=\"cite_note-33\"><b><a href=\"#cite_ref-33\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.beringia.com\/centre_info\/exhibit.html\" rel=\"nofollow\">\"Yukon Beringia Interpretive Center\"<\/a>. Beringia.com. 1999-04-12. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-34\"><b><a href=\"#cite_ref-34\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.eas.slu.edu\/People\/KChauff\/earth_history\/4EH-posted.pdf\" rel=\"nofollow\">Earth History 2001<\/a>\u00a0(page 15)<\/li>\r\n \t<li id=\"cite_note-35\"><b><a href=\"#cite_ref-35\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.wku.edu\/~smithch\/biogeog\/SCHM1946.htm\" rel=\"nofollow\">\"On the Zoogeography of the Holarctic Region\"<\/a>. Wku.edu. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-36\"><b><a href=\"#cite_ref-36\">^<\/a><\/b>\u00a0'Glaciers &amp; Glaciation' (Arnold, London 1998) Douglas Benn and David Evans, pp324-326<\/li>\r\n \t<li id=\"cite_note-britannica-37\"><b><a href=\"#cite_ref-britannica_37-0\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.britannica.com\/EBchecked\/topic\/315739\/kettle\" rel=\"nofollow\">\"Kettle geology\"<\/a>. Britannica Online. Retrieved 2009-03-12.<\/li>\r\n \t<li id=\"cite_note-38\"><b><a href=\"#cite_ref-38\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.lpi.usra.edu\/meetings\/polar2003\/pdf\/8112.pdf\" rel=\"nofollow\">\"Kargel, J.S. et al.:''Martian Polar Ice Sheets and Mid-Latitude Debris-Rich Glaciers, and Terrestrial Analogs'', Third International Conference on Mars Polar Science and Exploration, Alberta, Canada, October 13-17, 2003 (pdf 970 Kb)\"<\/a>\u00a0(PDF). Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-39\"><b><a href=\"#cite_ref-39\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.esa.int\/SPECIALS\/Mars_Express\/SEMS3PMZCIE_0.html\" rel=\"nofollow\">\"Martian glaciers: did they originate from the atmosphere? ESA Mars Express, 20 January 2006\"<\/a>. Esa.int. 2006-01-20. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-40\"><b><a href=\"#cite_ref-40\">^<\/a><\/b>\u00a0Head, J. et al. 2005. Tropical to mid-latitude snow and ice accumulation, flow and glaciation on Mars. Nature: 434. 346-350<\/li>\r\n \t<li id=\"cite_note-41\"><b><a href=\"#cite_ref-41\">^<\/a><\/b>\u00a0Source: Brown University Posted Monday, October 17, 2005 (2005-10-17).\u00a0<a href=\"http:\/\/www.marstoday.com\/news\/viewpr.html?pid=18050\" rel=\"nofollow\">\"Mars' climate in flux: Mid-latitude glaciers | SpaceRef - Your Space Reference\"<\/a>. Marstoday.com. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-42\"><b><a href=\"#cite_ref-42\">^<\/a><\/b>\u00a0Richard Lewis (2008-04-23).\u00a0<a href=\"http:\/\/news.brown.edu\/pressreleases\/2008\/04\/martian-glaciers\" rel=\"nofollow\">\"Glaciers Reveal Martian Climate Has Been Recently Active | Brown University News and Events\"<\/a>. News.brown.edu. Retrieved 2013-01-04.<\/li>\r\n \t<li id=\"cite_note-43\"><b><a href=\"#cite_ref-43\">^<\/a><\/b>\u00a0Plaut, J. et al. 2008. Radar Evidence for Ice in Lobate Debris Aprons in the Mid-Northern Latitudes of Mars. Lunar and Planetary Science XXXIX. 2290.pdf<\/li>\r\n \t<li id=\"cite_note-44\"><b><a href=\"#cite_ref-44\">^<\/a><\/b>\u00a0Holt, J. et al. 2008. Radar Sounding Evidence for Ice within Lobate Debris Aprons near Hellas Basin, Mid-Southern Latitudes of Mars. Lunar and Planetary Science XXXIX. 2441.pdf<\/li>\r\n<\/ol>\r\n<\/div>\r\n<h2>References<\/h2>\r\n<ul>\r\n \t<li><i>This article draws heavily on the corresponding article in the Spanish-language Wikipedia, which was accessed in the version of 24 July 2005.<\/i><\/li>\r\n \t<li>Hambrey, Michael; Alean, J\u00fcrg (2004).\u00a0<i>Glaciers<\/i>\u00a0(2nd ed.). Cambridge University Press. ISBN\u00a00-521-82808-2. OCLC\u00a054371738.\u00a0An excellent less-technical treatment of all aspects, with superb photographs and firsthand accounts of glaciologists' experiences. All images of this book can be found online (see Weblinks: Glaciers-online)<\/li>\r\n \t<li>Benn, Douglas I.; Evans, David J. A. (1999).\u00a0<i>Glaciers and Glaciation<\/i>. Arnold. ISBN\u00a00-470-23651-5. OCLC\u00a038329570.<\/li>\r\n \t<li>Bennett, M. R.; Glasser, N. F. (1996).\u00a0<i>Glacial Geology: Ice Sheets and Landforms<\/i>. John Wiley &amp; Sons. ISBN\u00a00-471-96344-5. OCLC\u00a033359888 37536152.<\/li>\r\n \t<li>Hambrey, Michael (1994).\u00a0<i>Glacial Environments<\/i>. University of British Columbia Press, UCL Press. ISBN\u00a00-7748-0510-2. OCLC\u00a030512475.\u00a0An undergraduate-level textbook.<\/li>\r\n \t<li>Knight, Peter G (1999).\u00a0<i>Glaciers<\/i>. Cheltenham: Nelson Thornes. ISBN\u00a00-7487-4000-7. OCLC\u00a042656957 63064183 77294832.\u00a0A textbook for undergraduates avoiding mathematical complexities<\/li>\r\n \t<li>Walley, Robert (1992).\u00a0<i>Introduction to Physical Geography<\/i>. Wm. C. Brown Publishers.\u00a0A textbook devoted to explaining the geography of our planet.<\/li>\r\n \t<li>W. S. B. Paterson (1994).\u00a0<i>Physics of Glaciers<\/i>\u00a0(3rd ed.). Pergamon Press. ISBN\u00a00-08-013972-8. OCLC\u00a026188.\u00a0A comprehensive reference on the physical principles underlying formation and behavior.<\/li>\r\n<\/ul>\r\n<h2>External links<\/h2>\r\n<ul>\r\n \t<li><a href=\"http:\/\/danbbs.dk\/~stst\/glaciologi\/\" rel=\"nofollow\">Glacial structures - photo atlas<\/a><\/li>\r\n \t<li><a href=\"http:\/\/www.glaciares.org\/\" rel=\"nofollow\">Glaciers of the Pyrenees<\/a><\/li>\r\n \t<li><a href=\"http:\/\/www.pbs.org\/now\/shows\/516\/index.html\" rel=\"nofollow\">NOW on PBS \"On Thin Ice\"<\/a><\/li>\r\n \t<li><a href=\"http:\/\/www.asiasociety.org\/onthinnerice\" rel=\"nofollow\">Photo project tracks changes in Himalayan glaciers since 1921<\/a><\/li>\r\n \t<li>Short radio episode\u00a0<i><b><a href=\"http:\/\/californialegacy.org\/radio_anthology\/scripts\/muir.html\" rel=\"nofollow\">California Glaciers<\/a><\/b><\/i>\u00a0from\u00a0<i>The Mountains of California<\/i>\u00a0by John Muir, 1894. California Legacy Project<\/li>\r\n \t<li><a href=\"http:\/\/donlehmanjr.com\/Mountain\/08%20The%20Dynamics%20of%20Glaciers.htm\" rel=\"nofollow\">Dyanamics of Glaciers<\/a><\/li>\r\n<\/ul>\r\n<\/div>","rendered":"<p>A\u00a0<b>glacier<\/b>\u00a0(<small>US<\/small>\u00a0\/\u02c8\u0261le\u026a\u0283\u0259r\/\u00a0or\u00a0<small>UK<\/small>\u00a0\/\u02c8\u0261l\u00e6si\u0259\/) is a persistent body of dense ice that is constantly moving under its own weight; it forms where the accumulation of snow exceeds its ablation (melting and sublimation) over many years, often centuries. Glaciers slowly deform and flow due to stresses induced by their weight, creating crevasses, seracs, and other distinguishing features. They also abrade rock and debris from their substrate to create landforms such as cirques and moraines. Glaciers form only on land and are distinct from the much thinner sea ice and lake ice that form on the surface of bodies of water.<\/p>\n<p><a style=\"line-height: 1.5em;\" href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Baltoro_glacier_from_air.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Baltoro_glacier_from_air.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div id=\"mw-content-text\" dir=\"ltr\" lang=\"en\">\n<div>\n<div>\n<div>\n<p>The Baltoro Glacier in the Karakoram, Baltistan, Northern Pakistan. At 62 kilometres (39\u00a0mi) in length, it is one of the longest alpine glaciers on earth.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Perito_Moreno_Glacier_Patagonia_Argentina_Luca_Galuzzi_2005.JPG\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Perito_Moreno_Glacier_Patagonia_Argentina_Luca_Galuzzi_2005.JPG\" alt=\"\" width=\"220\" height=\"147\" \/><\/a><\/p>\n<div>\n<p>Ice calving from the terminus of the Perito Moreno Glacier in western Patagonia, Argentina<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Grosser_Aletschgletscher_3178.JPG\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Grosser_Aletschgletscher_3178.JPG\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>The Aletsch Glacier, the largest glacier of the Alps, in Switzerland<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Quelccaya_Glacier.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Quelccaya_Glacier.jpg\" alt=\"\" width=\"220\" height=\"147\" \/><\/a><\/p>\n<div>\n<p>The Quelccaya Ice Cap is the largest glaciated area in the tropics, in Peru<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p><span style=\"line-height: 1.5em;\">On Earth, 99% of glacial ice is contained within vast ice sheets in the polar regions, but glaciers may be found in mountain ranges on every continent except Australia, and on a few high-latitude oceanic islands. Between 35\u00b0N and 35\u00b0S, glaciers occur only in the Himalayas, Andes, Rocky Mountains, a few high mountains in East Africa, Mexico, New Guinea and on Zard Kuh in Iran.<\/span><sup id=\"cite_ref-Post_2000_1-0\" style=\"line-height: 1.5em;\"><a href=\"#cite_note-Post_2000-1\">[1]<\/a><\/sup><\/p>\n<p>Glacial ice is the largest reservoir of freshwater on Earth.<sup id=\"cite_ref-IMS_2-0\"><a href=\"#cite_note-IMS-2\">[2]<\/a><\/sup>\u00a0Many glaciers from temperate, alpine and seasonal polar climates store water as ice during the colder seasons and release it later in the form of meltwater as warmer summer temperatures cause the glacier to melt, creating a water source that is especially important for plants, animals and human uses when other sources may be scant. Within high altitude and Antarctic environments, the seasonal temperature difference is often not sufficient to release meltwater.<\/p>\n<p>Because glacial mass is affected by long-term climate changes, e.g., precipitation, mean temperature, and cloud cover, glacial mass changes are considered among the most sensitive indicators of climate change and are a major source of variations in sea level.<\/p>\n<p>&nbsp;<\/p>\n<h2>Etymology and related terms<\/h2>\n<p>The word\u00a0<i>glacier<\/i>\u00a0comes from French. It is derived from the Vulgar Latin\u00a0<i>glacia<\/i>\u00a0and ultimately from Latin\u00a0<i>glacies<\/i>\u00a0meaning &#8220;ice&#8221;.<sup id=\"cite_ref-3\"><a href=\"#cite_note-3\">[3]<\/a><\/sup>\u00a0The processes and features caused by glaciers and related to them are referred to as\u00a0<b>glacial<\/b>. The process of glacier establishment, growth and flow is called\u00a0<b>glaciation<\/b>. The corresponding area of study is called glaciology. Glaciers are important components of the global cryosphere.<\/p>\n<h2>Types<\/h2>\n<div>Main article: Glacier morphology<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacier_mouth.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacier_mouth.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Mouth of the Schlatenkees Glacier near Innergschl\u00f6\u00df, Austria<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Glaciers are categorized by their morphology, thermal characteristics, and behavior.\u00a0<i>Alpine glaciers,<\/i>\u00a0also known as\u00a0<i>mountain glaciers<\/i>or\u00a0<i>cirque glaciers<\/i>, form on the crests and slopes of mountains. An alpine glacier that fills a valley is sometimes called a\u00a0<i>valley glacier<\/i>. A large body of glacial ice astride a mountain, mountain range, or volcano is termed an ice cap or ice field.<sup id=\"cite_ref-4\"><a href=\"#cite_note-4\">[4]<\/a><\/sup>\u00a0Ice caps have an area less than 50,000\u00a0km\u00b2 (20,000\u00a0mile\u00b2) by definition.<\/p>\n<p>Glacial bodies larger than 50,000\u00a0km\u00b2 are called ice sheets or continental glaciers.<sup id=\"cite_ref-5\"><a href=\"#cite_note-5\">[5]<\/a><\/sup>\u00a0Several kilometers deep, they obscure the underlying topography. Only\u00a0<i>nunataks<\/i>\u00a0protrude from their surfaces. The only extant ice sheets are the two that cover most of Antarctica and Greenland. They contain vast quantities of fresh water, enough that if both melted, global sea levels would rise by over 70 meters.<sup id=\"cite_ref-6\"><a href=\"#cite_note-6\">[6]<\/a><\/sup>Portions of an ice sheet or cap that extend into water are called\u00a0<i>ice shelves;<\/i>\u00a0they tend to be thin with limited slopes and reduced velocities.<sup id=\"cite_ref-NSIDC_7-0\"><a href=\"#cite_note-NSIDC-7\">[7]<\/a><\/sup>\u00a0Narrow, fast-moving sections of an ice sheet are called\u00a0<i>ice streams.<\/i><sup id=\"cite_ref-8\"><a href=\"#cite_note-8\">[8]<\/a><\/sup><sup id=\"cite_ref-BAS2009_9-0\"><a href=\"#cite_note-BAS2009-9\">[9]<\/a><\/sup>\u00a0In Antarctica, many ice streams drain into large ice shelves. Some drain directly into the sea, often with an ice tongue, like Mertz Glacier.<\/p>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Fjordsglacier.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Fjordsglacier.jpg\" alt=\"\" width=\"220\" height=\"144\" \/><\/a><\/p>\n<div>\n<p>Sightseeing boat in front of a tidewater glacier, Kenai Fjords National Park, Alaska<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p><i>Tidewater glaciers<\/i>\u00a0are glaciers that terminate in the sea, including most glaciers flowing from Greenland, Antarctica, Baffin and Ellesmere Islands in Canada, Southeast Alaska, and the Northern and Southern Patagonian Ice Fields. As the ice reaches the sea, pieces break off, or\u00a0<i>calve<\/i>, forming icebergs. Most tidewater glaciers calve above sea level, which often results in a tremendous impact as the iceberg strikes the water. Tidewater glaciers undergo centuries-long cycles of advance and retreat that are much less affected by the climate change than those of other glaciers.<\/p>\n<p>Thermally, a\u00a0<i>temperate glacier<\/i>\u00a0is at melting point throughout the year, from its surface to its base. The ice of a\u00a0<i>polar glacier<\/i>\u00a0is always below freezing point from the surface to its base, although the surface snowpack may experience seasonal melting. A\u00a0<i>sub-polar glacier<\/i>includes both temperate and polar ice, depending on depth beneath the surface and position along the length of the glacier. In a similar way, the thermal regime of a glacier is often described by the temperature at its base alone. A\u00a0<i>cold-based<\/i>\u00a0glacier is below freezing at the ice-ground interface, and is thus frozen to the underlying substrate. A\u00a0<i>warm-based<\/i>\u00a0glacier is above or at freezing at the interface, and is able to slide at this contact.<sup id=\"cite_ref-ColdBased_10-0\"><a href=\"#cite_note-ColdBased-10\">[10]<\/a><\/sup>\u00a0This contrast is thought to a large extent to govern the ability of a glacier to effectively erode its bed, as sliding ice promotes plucking at rock from the surface below.<sup id=\"cite_ref-11\"><a href=\"#cite_note-11\">[11]<\/a><\/sup>\u00a0Glaciers which are partly cold-based and partly warm-based are known as\u00a0<i>polythermal<\/i>.<sup id=\"cite_ref-ColdBased_10-1\"><a href=\"#cite_note-ColdBased-10\">[10]<\/a><\/sup><\/p>\n<h2>Formation<\/h2>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-GornerGlacier_002.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-GornerGlacier_002.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Gorner Glacier in Switzerland<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Glaciers form where the accumulation of snow and ice exceeds ablation. The area in which a glacier forms is called a cirque (corrie or cwm) &#8211; a typically armchair-shaped geological feature (such as a depression between mountains enclosed by ar\u00eates) &#8211; which collects and compresses through gravity the snow which falls into it. This snow collects and is compacted by the weight of the snow falling above it forming n\u00e9v\u00e9. Further crushing of the individual snowflakes and squeezing the air from the snow turns it into extremely dense &#8216;glacial ice&#8217;. This glacial ice will fill the cirque until it &#8216;overflows&#8217; through a geological weakness or vacancy, such as the gap between two mountains. When the mass of snow and ice is sufficiently thick, it begins to move due to a combination of surface slope, gravity and pressure. On steeper slopes, this can occur with as little as 15\u00a0m (50\u00a0ft) of snow-ice.<\/p>\n<p>In temperate glaciers, snow repeatedly freezes and thaws, changing into granular ice called firn. Under the pressure of the layers of ice and snow above it, this granular ice fuses into denser and denser firn. Over a period of years, layers of firn undergo further compaction and become glacial ice. Glacier ice is slightly less dense than ice formed from frozen water because it contains tiny trapped air bubbles.<\/p>\n<p>Glacial ice has a distinctive blue tint because it absorbs some red light due to an overtone of the infrared OH stretching mode of the water molecule. Liquid water is blue for the same reason. The blue of glacier ice is sometimes misattributed to Rayleigh scattering due to bubbles in the ice.<sup id=\"cite_ref-12\"><a href=\"#cite_note-12\">[12]<\/a><\/sup><\/p>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-153_-_Glacier_Perito_Moreno_-_Grotte_glaciaire_-_Janvier_2010.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-153_-_Glacier_Perito_Moreno_-_Grotte_glaciaire_-_Janvier_2010.jpg\" alt=\"\" width=\"220\" height=\"151\" \/><\/a><\/p>\n<div>\n<p>A glacier cave located on the Perito Moreno Glacier in Argentina.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<h2>Structure<\/h2>\n<p>A glacier originates at a location called its\u00a0<i>glacier head<\/i>\u00a0and terminates at its\u00a0<i>glacier foot<\/i>, or terminus.<\/p>\n<p>Glaciers are broken into zones based on surface snowpack and melt conditions.<sup id=\"cite_ref-13\"><a href=\"#cite_note-13\">[13]<\/a><\/sup>\u00a0The\u00a0<i>ablation zone<\/i>\u00a0is the region where there is a net loss in glacier mass. The\u00a0<i>equilibrium line<\/i>\u00a0separates the ablation zone and the accumulation zone; it is the altitude where the amount of new snow gained by accumulation is equal to the amount of ice lost through ablation. The upper part of a glacier, where accumulation exceeds ablation, is called the\u00a0<i>accumulation zone<\/i>. In general, the accumulation zone accounts for 60\u201370% of the glacier&#8217;s surface area, more if the glacier calves icebergs. Ice in the accumulation zone is deep enough to exert a downward force that erodes underlying rock. After a glacier melts, it often leaves behind a bowl- or amphitheater-shaped depression that ranges in size from large basins like the Great Lakes to smaller mountain depressions known as cirques.<\/p>\n<p>The accumulation zone can be subdivided based on its melt conditions.<\/p>\n<ol>\n<li>The\u00a0<i>dry snow zone<\/i>\u00a0is a region where no melt occurs, even in the summer, and the snowpack remains dry.<\/li>\n<li>The\u00a0<i>percolation zone<\/i>\u00a0is an area with some surface melt, causing meltwater to percolate into the snowpack. This zone is often marked by refrozen ice lenses, glands, and layers. The snowpack also never reaches melting point.<\/li>\n<li>Near the equilibrium line on some glaciers, a\u00a0<i>superimposed ice zone<\/i>\u00a0develops. This zone is where meltwater refreezes as a cold layer in the glacier, forming a continuous mass of ice.<\/li>\n<li>The\u00a0<i>wet snow zone<\/i>\u00a0is the region where all of the snow deposited since the end of the previous summer has been raised to 0\u00a0\u00b0C.<\/li>\n<\/ol>\n<p>The &#8220;health&#8221; of a glacier is usually assessed by determining the glacier mass balance or observing terminus behavior. Healthy glaciers have large accumulation zones, more than 60% of their area snowcovered at the end of the melt season, and a terminus with vigorous flow.<\/p>\n<p>Following the Little Ice Age&#8217;s end around 1850, glaciers around the Earth have retreated substantially. A slight cooling led to the advance of many alpine glaciers between 1950\u20131985, but since 1985 glacier retreat and mass loss has become larger and increasingly ubiquitous.<sup id=\"cite_ref-14\"><a href=\"#cite_note-14\">[14]<\/a><\/sup><sup id=\"cite_ref-15\"><a href=\"#cite_note-15\">[15]<\/a><\/sup><sup id=\"cite_ref-16\"><a href=\"#cite_note-16\">[16]<\/a><\/sup><\/p>\n<h2>Motion<\/h2>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Chevron_Crevasses_00.JPG\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Chevron_Crevasses_00.JPG\" alt=\"\" width=\"220\" height=\"147\" \/><\/a><\/p>\n<div>\n<p>Shear or herring-bone crevasses on Emmons Glacier (Mount Rainier); such crevasses often form near the edge of a glacier where interactions with underlying or marginal rock impede flow. In this case, the impediment appears to be some distance from the near margin of the glacier.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>Main article: Ice sheet dynamics<\/div>\n<p>Glaciers move, or flow, downhill due to gravity and the internal deformation of ice.<sup id=\"cite_ref-GreveBlatter2009_17-0\"><a href=\"#cite_note-GreveBlatter2009-17\">[17]<\/a><\/sup>\u00a0Ice behaves like a brittle solid until its thickness exceeds about 50\u00a0m (160\u00a0ft). The pressure on ice deeper than 50\u00a0m causes plastic flow. At the molecular level, ice consists of stacked layers of molecules with relatively weak bonds between layers. When the stress on the layer above exceeds the inter-layer binding strength, it moves faster than the layer below.<sup id=\"cite_ref-18\"><a href=\"#cite_note-18\">[18]<\/a><\/sup><\/p>\n<p>Glaciers also move through basal sliding. In this process, a glacier slides over the terrain on which it sits, lubricated by the presence of liquid water. The water is created from ice that melts under high pressure from frictional heating. Basal sliding is dominant in temperate, or warm-based glaciers.<\/p>\n<h3>Fracture zone and cracks<\/h3>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-TitlisIceCracks.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-TitlisIceCracks.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Ice cracks in the Titlis Glacier<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>The top 50 metres (160\u00a0ft) of a glacier are rigid because they are under low pressure. This upper section is known as the\u00a0<i>fracture zone<\/i>; it mostly moves as a single unit over the plastically flowing lower section. When a glacier moves through irregular terrain, cracks called crevasses develop in the fracture zone. Crevasses form due to differences in glacier velocity. If two rigid sections of a glacier move at different speeds and directions, shear forces cause them to break apart, opening a crevasse. Crevasses are seldom more than 150 feet (46\u00a0m) deep but in some cases can be 1,000 feet (300\u00a0m) or even deeper. Beneath this point, the plasticity of the ice is too great for cracks to form. Intersecting crevasses can create isolated peaks in the ice, called seracs.<\/p>\n<p>Crevasses can form in several different ways. Transverse crevasses are transverse to flow and form where steeper slopes cause a glacier to accelerate. Longitudinal crevasses form semi-parallel to flow where a glacier expands laterally. Marginal crevasses form from the edge of the glacier, due to the reduction in speed caused by friction of the valley walls. Marginal crevasses are usually largely transverse to flow. Moving glacier ice can sometimes separate from stagnant ice above, forming a\u00a0<i>bergschrund<\/i>. Bergschrunds resemble crevasses but are singular features at a glacier&#8217;s margins.<\/p>\n<p>Crevasses make travel over glaciers hazardous, especially when they are hidden by fragile snow bridges.<\/p>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/170px-Glaciereaston.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/170px-Glaciereaston.jpg\" alt=\"\" width=\"170\" height=\"227\" \/><\/a><\/p>\n<div>\n<p>Crossing a crevasse on the Easton Glacier, Mount Baker, in the North Cascades, United States<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Below the equilibrium line, glacial meltwater is concentrated in stream channels. Meltwater can pool in proglacial lakes on top of a glacier or descend into the depths of a glacier via moulins. Streams within or beneath a glacier flow in englacial or sub-glacial tunnels. These tunnels sometimes reemerge at the glacier&#8217;s surface.<sup id=\"cite_ref-19\"><a href=\"#cite_note-19\">[19]<\/a><\/sup><\/p>\n<h3>Speed<\/h3>\n<p>The speed of glacial displacement is partly determined by friction. Friction makes the ice at the bottom of the glacier move more slowly than ice at the top. In alpine glaciers, friction is also generated at the valley&#8217;s side walls, which slows the edges relative to the center.<\/p>\n<p>Mean speeds vary greatly, but is typically around 1 meter per day.<sup id=\"cite_ref-20\"><a href=\"#cite_note-20\">[20]<\/a><\/sup>\u00a0There may be no motion in stagnant areas; for example, in parts of Alaska, trees can establish themselves on surface sediment deposits. In other cases, glaciers can move as fast as 20\u201330\u00a0m per day, such as in Greenland&#8217;s Jakobshavn Isbr\u00e6 (Greenlandic:\u00a0<i>Sermeq Kujalleq<\/i>). Velocity increases with increasing slope, increasing thickness, increasing snowfall, increasing longitudinal confinement, increasing basal temperature, increasing meltwater production and reduced bed hardness.<\/p>\n<p>A few glaciers have periods of very rapid advancement called surges. These glaciers exhibit normal movement until suddenly they accelerate, then return to their previous state. During these surges, the glacier may reach velocities far greater than normal speed.<sup id=\"cite_ref-21\"><a href=\"#cite_note-21\">[21]<\/a><\/sup>\u00a0These surges may be caused by failure of the underlying bedrock, the pooling of meltwater at the base of the glacier<sup id=\"cite_ref-22\"><a href=\"#cite_note-22\">[22]<\/a><\/sup>\u00a0\u2014 perhaps delivered from a supraglacial lake\u00a0\u2014 or the simple accumulation of mass beyond a critical &#8220;tipping point&#8221;.<sup id=\"cite_ref-23\"><a href=\"#cite_note-23\">[23]<\/a><\/sup><\/p>\n<p>In glaciated areas where the glacier moves faster than one km per year, glacial earthquakes occur. These are large scale tremblors that have seismic magnitudes as high as 6.1.<sup id=\"cite_ref-people.deas.harvard.edu_24-0\"><a href=\"#cite_note-people.deas.harvard.edu-24\">[24]<\/a><\/sup><sup id=\"cite_ref-TsaiEkstrom_JGR2007_2007_25-0\"><a href=\"#cite_note-TsaiEkstrom_JGR2007_2007-25\">[25]<\/a><\/sup>\u00a0The number of glacial earthquakes in Greenland peaks every year in July, August and September and is increasing over time. In a study using data from January 1993 through October 2005, more events were detected every year since 2002, and twice as many events were recorded in 2005 as there were in any other year. This increase in the numbers of glacial earthquakes in Greenland may be a response to global warming.<sup id=\"cite_ref-people.deas.harvard.edu_24-1\"><a href=\"#cite_note-people.deas.harvard.edu-24\">[24]<\/a><\/sup><sup id=\"cite_ref-TsaiEkstrom_JGR2007_2007_25-1\"><a href=\"#cite_note-TsaiEkstrom_JGR2007_2007-25\">[25]<\/a><\/sup><\/p>\n<h3>Ogives<\/h3>\n<p><i>Ogives<\/i>\u00a0are alternating wave crests and valleys that appear as dark and light bands of ice on glacier surfaces. They are linked to seasonal motion of glaciers; the width of one dark and one light band generally equals the annual movement of the glacier. Ogives are formed when ice from an icefall is severely broken up, increasing ablation surface area during summer. This creates a swale and space for snow accumulation in the winter, which in turn creates a ridge.<sup id=\"cite_ref-26\"><a href=\"#cite_note-26\">[26]<\/a><\/sup>\u00a0Sometimes ogives consist only of undulations or color bands and are described as wave ogives or band ogives.<sup id=\"cite_ref-27\"><a href=\"#cite_note-27\">[27]<\/a><\/sup><\/p>\n<h2>Geography<\/h2>\n<div>For more details on this topic, see List of glaciers, and Retreat of glaciers since 1850.<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Black-Glacier.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Black-Glacier.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Black ice glacier near Aconcagua, Argentina<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Glaciers are present on every continent and approximately fifty countries, excluding those (Australia, South Africa) that have glaciers only on distant subantarctic island territories. Extensive glaciers are found in Antarctica, Chile, Canada, Alaska, Greenland and Iceland. Mountain glaciers are widespread, especially in the Andes, the Himalayas, the Rocky Mountains, the Caucasus, and the Alps. Mainland Australia currently contains no glaciers, although a small glacier on Mount Kosciuszko was present in the last glacial period.<sup id=\"cite_ref-28\"><a href=\"#cite_note-28\">[28]<\/a><\/sup>\u00a0In New Guinea, small, rapidly diminishing, glaciers are located on its highest summit massif of Puncak Jaya.<sup id=\"cite_ref-29\"><a href=\"#cite_note-29\">[29]<\/a><\/sup>\u00a0Africa has glaciers on Mount Kilimanjaro in Tanzania, on Mount Kenya and in the Rwenzori Mountains. Oceanic islands with glaciers occur on Iceland, Svalbard, New Zealand, Jan Mayen and the subantarctic islands of Marion, Heard, Grande Terre (Kerguelen) and Bouvet. During glacial periods of the Quaternary, Taiwan, Hawaii on Mauna Kea<sup id=\"cite_ref-30\"><a href=\"#cite_note-30\">[30]<\/a><\/sup>\u00a0and Tenerife also had large alpine glaciers, while the Faroe and Crozet Islands<sup id=\"cite_ref-31\"><a href=\"#cite_note-31\">[31]<\/a><\/sup>\u00a0were completely glaciated.<\/p>\n<p>The permanent snow cover necessary for glacier formation is affected by factors such as the degree of slope on the land, amount of snowfall and the winds. Glaciers can be found in all latitudes except from 20\u00b0 to 27\u00b0 north and south of the equator where the presence of the descending limb of the Hadley circulation lowers precipitation so much that with high insolation snow lines reach above 6,500 metres (21,330\u00a0ft). Between 19\u02daN and 19\u02daS, however, precipitation is higher and the mountains above 5,000 metres (16,400\u00a0ft) usually have permanent snow.<\/p>\n<p>Even at high latitudes, glacier formation is not inevitable. Areas of the Arctic, such as Banks Island, and the McMurdo Dry Valleys in Antarctica are considered polar deserts where glaciers cannot form because they receive little snowfall despite the bitter cold. Cold air, unlike warm air, is unable to transport much water vapor. Even during glacial periods of the Quaternary, Manchuria, lowland Siberia,<sup id=\"cite_ref-32\"><a href=\"#cite_note-32\">[32]<\/a><\/sup>and central and northern Alaska,<sup id=\"cite_ref-33\"><a href=\"#cite_note-33\">[33]<\/a><\/sup>\u00a0though extraordinarily cold, had such light snowfall that glaciers could not form.<sup id=\"cite_ref-34\"><a href=\"#cite_note-34\">[34]<\/a><\/sup><sup id=\"cite_ref-35\"><a href=\"#cite_note-35\">[35]<\/a><\/sup><\/p>\n<p>In addition to the dry, unglaciated polar regions, some mountains and volcanoes in Bolivia, Chile and Argentina are high (4,500 metres (14,800\u00a0ft) &#8211; 6,900\u00a0m (22,600\u00a0ft)) and cold, but the relative lack of precipitation prevents snow from accumulating into glaciers. This is because these peaks are located near or in the hyperarid Atacama Desert.<\/p>\n<h2>Glacial geology<\/h2>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Arranque_glaciar-en.svg.png\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Arranque_glaciar-en.svg.png\" alt=\"\" width=\"220\" height=\"132\" \/><\/a><\/p>\n<div>\n<p>Diagram of glacial plucking and abrasion<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-PluckedGraniteAlandIslands.JPG\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-PluckedGraniteAlandIslands.JPG\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Glacially plucked granitic bedrock near Mariehamn, \u00c5land Islands<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Glaciers erode terrain through two principal processes:\u00a0<b>abrasion<\/b>\u00a0and\u00a0<b>plucking.<\/b><\/p>\n<p>As glaciers flow over bedrock, they soften and lift blocks of rock into the ice. This process, called plucking, is caused by subglacial water that penetrates fractures in the bedrock and subsequently freezes and expands. This expansion causes the ice to act as a lever that loosens the rock by lifting it. Thus, sediments of all sizes become part of the glacier&#8217;s load. If a retreating glacier gains enough debris, it may become a rock glacier, like the Timpanogos Glacier in Utah.<\/p>\n<p>Abrasion occurs when the ice and its load of rock fragments slide over bedrock and function as sandpaper, smoothing and polishing the bedrock below. The pulverized rock this process produces is called rock flour and is made up of rock grains between 0.002 and 0.00625\u00a0mm in size. Abrasion leads to steeper valley walls and mountain slopes in alpine settings, which can cause avalanches and rock slides. These add even more material to the glacier.<\/p>\n<p>Glacial abrasion is commonly characterized by glacial striations. Glaciers produce these when they contain large boulders that carve long scratches in the bedrock. By mapping the direction of the striations, researchers can determine the direction of the glacier&#8217;s movement. Similar to striations are chatter marks, lines of crescent-shape depressions in the rock underlying a glacier. They are formed by abrasion when boulders in the glacier are repeatedly caught and released as they are dragged along the bedrock.<\/p>\n<p>The rate of glacier erosion is variable. Six factors control erosion rate:<\/p>\n<ul>\n<li>Velocity of glacial movement<\/li>\n<li>Thickness of the ice<\/li>\n<li>Shape, abundance and hardness of rock fragments contained in the ice at the bottom of the glacier<\/li>\n<li>Relative ease of erosion of the surface under the glacier<\/li>\n<li>Thermal conditions at the glacier base<\/li>\n<li>Permeability and water pressure at the glacier base<\/li>\n<\/ul>\n<p>Material that becomes incorporated in a glacier is typically carried as far as the zone of ablation before being deposited. Glacial deposits are of two distinct types:<\/p>\n<ul>\n<li><i>Glacial till<\/i>: material directly deposited from glacial ice. Till includes a mixture of undifferentiated material ranging from clay size to boulders, the usual composition of a moraine.<\/li>\n<li><i>Fluvial and outwash sediments<\/i>: sediments deposited by water. These deposits are stratified by size.<\/li>\n<\/ul>\n<p>Larger pieces of rock that are encrusted in till or deposited on the surface are called &#8220;glacial erratics&#8221;. They range in size from pebbles to boulders, but as they are often moved great distances, they may be drastically different from the material upon which they are found. Patterns of glacial erratics hint at past glacial motions.<\/p>\n<h3>Moraines<\/h3>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-MorainesLakeLouise.JPG\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-MorainesLakeLouise.JPG\" alt=\"\" width=\"220\" height=\"158\" \/><\/a><\/p>\n<div>\n<p>Glacial moraines above Lake Louise, Alberta, Canada<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Glacial moraines are formed by the deposition of material from a glacier and are exposed after the glacier has retreated. They usually appear as linear mounds of till, a non-sorted mixture of rock, gravel and boulders within a matrix of a fine powdery material. Terminal or end moraines are formed at the foot or terminal end of a glacier. Lateral moraines are formed on the sides of the glacier. Medial moraines are formed when two different glaciers merge and the lateral moraines of each coalesce to form a moraine in the middle of the combined glacier. Less apparent are ground moraines, also called\u00a0<i>glacial drift<\/i>, which often blankets the surface underneath the glacier downslope from the equilibrium line.<\/p>\n<p>The term\u00a0<i>moraine<\/i>\u00a0is of French origin. It was coined by peasants to describe alluvial embankments and rims found near the margins of glaciers in the French Alps. In modern geology, the term is used more broadly, and is applied to a series of formations, all of which are composed of till. Moraines can also create moraine dammed lakes.<\/p>\n<h3>Drumlins<\/h3>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/249px-Drumlins_LMB.svg.png\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/249px-Drumlins_LMB.svg.png\" alt=\"\" width=\"249\" height=\"109\" \/><\/a><\/p>\n<div>A drumlin field forms after a glacier has modified the landscape. The teardrop-shaped formations denote the direction of the ice flow.<\/div>\n<\/div>\n<\/div>\n<p>Drumlins are asymmetrical, canoe shaped hills made mainly of till. Their heights vary from 15 to 50\u00a0meters and they can reach a kilometer in length. The tilted side of the hill faces the direction from which the ice advanced (<i>stoss<\/i>), while the longer slope follows the ice&#8217;s direction of movement (<i>lee<\/i>).<\/p>\n<p>Drumlins are found in groups called\u00a0<i>drumlin fields<\/i>\u00a0or\u00a0<i>drumlin camps<\/i>. One of these fields is found east of Rochester, New York; it is estimated to contain about 10,000 drumlins.<\/p>\n<p>Although the process that forms drumlins is not fully understood, their shape implies that they are products of the plastic deformation zone of ancient glaciers. It is believed that many drumlins were formed when glaciers advanced over and altered the deposits of earlier glaciers.<\/p>\n<h3>Glacial valleys, cirques, ar\u00eates, and pyramidal peaks<\/h3>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacial_landscape.svg.png\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Glacial_landscape.svg.png\" alt=\"\" width=\"220\" height=\"130\" \/><\/a><\/p>\n<div>\n<p>Features of a glacial landscape<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>Before glaciation, mountain valleys have a characteristic &#8220;V&#8221; shape, produced by eroding water. During glaciation, these valleys are widened, deepened, and smoothed, forming a &#8220;U&#8221;-shaped glacial valley. The erosion that creates glacial valleys eliminates the spurs of earth that extend across mountain valleys, creating triangular cliffs called truncated spurs. Within glacial valleys, depressions created by plucking and abrasion can be filled by lakes, called paternoster lakes. If a glacial valley runs into a large body of water, it forms a fjord.<\/p>\n<p>Many glaciers deepen their valleys more than their smaller tributaries. Therefore, when glaciers recede, the valleys of the tributary glaciers remain above the main glacier&#8217;s depression and are called hanging valleys.<\/p>\n<p>At the start of a classic valley glacier is a bowl-shaped cirque, which has escarped walls on three sides but is open on the side that descends into the valley. Cirques are where ice begins to accumulate in a glacier. Two glacial cirques may form back to back and erode their backwalls until only a narrow ridge, called an ar\u00eate is left. This structure may result in a mountain pass. If multiple cirques encircle a single mountain, they create pointed pyramidal peaks; particularly steep examples are called horns.<\/p>\n<h3>Roche moutonn\u00e9e<\/h3>\n<p>Some rock formations in the path of a glacier are sculpted into small hills called\u00a0<i>roche moutonn\u00e9e,<\/i>\u00a0or &#8220;sheepback&#8221; rock. Roche moutonn\u00e9e are elongated, rounded, and asymmetrical bedrock knobs can be produced by glacier erosion. They range in length from less than a meter to several hundred meters long.<sup id=\"cite_ref-36\"><a href=\"#cite_note-36\">[36]<\/a><\/sup>\u00a0Roche moutonn\u00e9e have a gentle slope on their up-glacier sides and a steep to vertical face on their down-glacier sides. The glacier abrades the smooth slope on the upstream side as it flows along, but tears loose and carries away rock from the downstream side via plucking.<\/p>\n<h3>Alluvial stratification<\/h3>\n<p>As the water that rises from the ablation zone moves away from the glacier, it carries fine eroded sediments with it. As the speed of the water decreases, so does its capacity to carry objects in suspension. The water thus gradually deposits the sediment as it runs, creating an alluvial plain. When this phenomenon occurs in a valley, it is called a\u00a0<i>valley train<\/i>. When the deposition is in an estuary, the sediments are known as bay mud.<\/p>\n<p>Outwash plains and valley trains are usually accompanied by basins known as &#8220;kettles&#8221;. These are small lakes formed when large ice blocks that are trapped in alluvium melt and produce water-filled depressions. Kettle diameters range from 5\u00a0m to 13\u00a0km, with depths of up to 45\u00a0meters. Most are circular in shape because the blocks of ice that formed them were rounded as they melted.<sup id=\"cite_ref-britannica_37-0\"><a href=\"#cite_note-britannica-37\">[37]<\/a><\/sup><\/p>\n<h3>Glacial deposits<\/h3>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Receding_glacier-en.svg.png\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Receding_glacier-en.svg.png\" alt=\"\" width=\"220\" height=\"103\" \/><\/a><\/p>\n<div>\n<p>Landscape produced by a receding glacier<\/p>\n<\/div>\n<\/div>\n<\/div>\n<p>When a glacier&#8217;s size shrinks below a critical point, its flow stops and it becomes stationary. Meanwhile, meltwater within and beneath the ice leaves stratified alluvial deposits. These deposits, in the forms of columns, terraces and clusters, remain after the glacier melts and are known as &#8220;glacial deposits&#8221;.<\/p>\n<p>Glacial deposits that take the shape of hills or mounds are called\u00a0<i>kames<\/i>. Some kames form when meltwater deposits sediments through openings in the interior of the ice. Others are produced by fans or deltas created by meltwater. When the glacial ice occupies a valley, it can form terraces or kames along the sides of the valley.<\/p>\n<p>Long, sinuous glacial deposits are called\u00a0<i>eskers<\/i>. Eskers are composed of sand and gravel that was deposited by meltwater streams that flowed through ice tunnels within or beneath a glacier. They remain after the ice melts, with heights exceeding 100\u00a0meters and lengths of as long as 100\u00a0km.<\/p>\n<h3>Loess deposits<\/h3>\n<p>Very fine glacial sediments or rock flour is often picked up by wind blowing over the bare surface and may be deposited great distances from the original fluvial deposition site. These eolian loess deposits may be very deep, even hundreds of meters, as in areas of China and the Midwestern United States of America. Katabatic winds can be important in this process.<\/p>\n<h2>Isostatic rebound<\/h2>\n<div>Main article: Isostatic rebound<\/div>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/Glacier_weight_effects_LMB.png\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/Glacier_weight_effects_LMB.png\" alt=\"\" width=\"482\" height=\"174\" \/><\/a><\/p>\n<div>Isostatic pressure by a glacier on the Earth&#8217;s crust<\/div>\n<\/div>\n<\/div>\n<p>Large masses, such as ice sheets or glaciers, can depress the crust of the Earth into the mantle. The depression usually totals a third of the ice sheet or glacier&#8217;s thickness. After the ice sheet or glacier melts, the mantle begins to flow back to its original position, pushing the crust back up. This post-glacial rebound, which proceeds very slowly after the melting of the ice sheet or glacier, is currently occurring in measurable amounts in Scandinavia and the Great Lakes region of North America.<\/p>\n<p>A geomorphological feature created by the same process on a smaller scale is known as\u00a0<i>dilation-faulting<\/i>. It occurs where previously compressed rock is allowed to return to its original shape more rapidly than can be maintained without faulting. This leads to an effect similar to what would be seen if the rock were hit by a large hammer. Dilation faulting can be observed in recently de-glaciated parts of Iceland and Cumbria.<\/p>\n<h2>On Mars<\/h2>\n<div>\n<div>\n<p><a href=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Mars_north_pole.jpg\"><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/s3-us-west-2.amazonaws.com\/candimgs\/9CUkzn\/220px-Mars_north_pole.jpg\" alt=\"\" width=\"220\" height=\"165\" \/><\/a><\/p>\n<div>\n<p>Northern polar ice cap on Mars<\/p>\n<\/div>\n<\/div>\n<\/div>\n<div>Main article: Glaciers on Mars<\/div>\n<p>The polar ice caps of Mars show geologic evidence of glacial deposits. The south polar cap is especially comparable to glaciers on Earth.<sup id=\"cite_ref-38\"><a href=\"#cite_note-38\">[38]<\/a><\/sup>\u00a0Topographical features and computer models indicate the existence of more glaciers in Mars&#8217; past.<sup id=\"cite_ref-39\"><a href=\"#cite_note-39\">[39]<\/a><\/sup><\/p>\n<p>At mid-latitudes, between 35\u00b0 and 65\u00b0 north or south, Martian glaciers are affected by the thin Martian atmosphere. Because of the low atmospheric pressure, ablation near the surface is solely due to sublimation, not melting. As on Earth, many glaciers are covered with a layer of rocks which insulates the ice. A radar instrument on board the Mars Reconnaissance Orbiter found ice under a thin layer of rocks in formations called Lobate Debris Aprons (LDAs).<sup id=\"cite_ref-40\"><a href=\"#cite_note-40\">[40]<\/a><\/sup><sup id=\"cite_ref-41\"><a href=\"#cite_note-41\">[41]<\/a><\/sup><sup id=\"cite_ref-42\"><a href=\"#cite_note-42\">[42]<\/a><\/sup><sup id=\"cite_ref-43\"><a href=\"#cite_note-43\">[43]<\/a><\/sup><sup id=\"cite_ref-44\"><a href=\"#cite_note-44\">[44]<\/a><\/sup><\/p>\n<h2>Notes<\/h2>\n<div>\n<ol>\n<li id=\"cite_note-Post_2000-1\"><b><a href=\"#cite_ref-Post_2000_1-0\">^<\/a><\/b>\u00a0Post, Austin; LaChapelle, Edward R (2000).\u00a0<i>Glacier ice<\/i>. Seattle, Washington: University of Washington Press. ISBN\u00a00-295-97910-0.<\/li>\n<li id=\"cite_note-IMS-2\"><b><a href=\"#cite_ref-IMS_2-0\">^<\/a><\/b>\u00a0Brown, Molly Elizabeth; Ouyang, Hua; Habib, Shahid; Shrestha, Basanta; Shrestha, Mandira; Panday, Prajjwal; Tzortziou, Maria; Policelli, Frederick; Artan, Guleid; Giriraj, Amarnath; Bajracharya, Sagar R.; Racoviteanu, Adina.\u00a0<a href=\"http:\/\/hdl.handle.net\/2060\/20110015312\" rel=\"nofollow\">&#8220;HIMALA: Climate Impacts on Glaciers, Snow, and Hydrology in the Himalayan Region&#8221;<\/a>.\u00a0<i>Mountain Research and Development<\/i>. International Mountain Society. Retrieved 16 September 2011.<\/li>\n<li id=\"cite_note-3\"><b><a href=\"#cite_ref-3\">^<\/a><\/b>\u00a0Simpson, D.P. (1979).\u00a0<i>Cassell&#8217;s Latin Dictionary<\/i>\u00a0(5 ed.). London: Cassell Ltd. p.\u00a0883. ISBN\u00a00-304-52257-0.<\/li>\n<li id=\"cite_note-4\"><b><a href=\"#cite_ref-4\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nichols.edu\/departments\/glacier\/juneau%20icefield.htm\" rel=\"nofollow\">&#8220;Retreat of Alaskan glacier Juneau icefield&#8221;<\/a>. Nichols.edu. Retrieved 2009-01-05.<\/li>\n<li id=\"cite_note-5\"><b><a href=\"#cite_ref-5\">^<\/a><\/b>\u00a0<a href=\"http:\/\/amsglossary.allenpress.com\/glossary\/search?id=ice-sheet1\" rel=\"nofollow\">&#8220;American Meteorological Society, Glossary of Meteorology&#8221;<\/a>. Amsglossary.allenpress.com. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-6\"><b><a href=\"#cite_ref-6\">^<\/a><\/b>\u00a0<a href=\"http:\/\/pubs.usgs.gov\/fs\/fs2-00\/\" rel=\"nofollow\">&#8220;Sea Level and Climate&#8221;<\/a>.\u00a0<i>USGS FS 002-00<\/i>. USGS. 2000-01-31. Retrieved 2009-01-05.<\/li>\n<li id=\"cite_note-NSIDC-7\"><b><a href=\"#cite_ref-NSIDC_7-0\">^<\/a><\/b>\u00a0*\u00a0National Snow and Ice Data Center.\u00a0<a href=\"http:\/\/www.nsidc.org\/glaciers\/questions\/types.html\" rel=\"nofollow\">&#8220;Types of Glacier&#8221;<\/a>.<\/li>\n<li id=\"cite_note-8\"><b><a href=\"#cite_ref-8\">^<\/a><\/b>\u00a0Bindschadler, R.A. and T.A. Scambos. Satellite-image-derived velocity field of an Antarctic ice stream.\u00a0<i>Science<\/i>, 252(5003), 242-246, 1991<\/li>\n<li id=\"cite_note-BAS2009-9\"><b><a href=\"#cite_ref-BAS2009_9-0\">^<\/a><\/b>\u00a0British Antarctic Survey.\u00a0<a href=\"http:\/\/www.antarctica.ac.uk\/\/about_antarctica\/geography\/ice\/streams.php\" rel=\"nofollow\">&#8220;Description of Ice Streams&#8221;<\/a>. Retrieved 2009-01-26.<\/li>\n<li id=\"cite_note-ColdBased-10\">^\u00a0<a href=\"#cite_ref-ColdBased_10-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-ColdBased_10-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/link.springer.com\/referenceworkentry\/10.1007%2F978-90-481-2642-2_72\/fulltext.html\" rel=\"nofollow\">http:\/\/link.springer.com\/referenceworkentry\/10.1007%2F978-90-481-2642-2_72\/fulltext.html<\/a><\/li>\n<li id=\"cite_note-11\"><b><a href=\"#cite_ref-11\">^<\/a><\/b>\u00a0Boulton, G.S. [1974] &#8220;Processes and patterns of glacial erosion&#8221;, (In Coates, D.R. ed.,\u00a0<i>Glacial Geomorphology<\/i>. A Proceedings Volume of the fifth Annual Geomorphology Symposia series, held at Binghamton, New York, September 26\u201328, 1974. Binghamton, N.Y., State University of New York, p. 41-87. (Publications in Geomorphology))<\/li>\n<li id=\"cite_note-12\"><b><a href=\"#cite_ref-12\">^<\/a><\/b>\u00a0<a href=\"http:\/\/webexhibits.org\/causesofcolor\/5C.html\" rel=\"nofollow\">&#8220;What causes the blue color that sometimes appears in snow and ice\u00a0?&#8221;<\/a>. Webexhibits.org. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-13\"><b><a href=\"#cite_ref-13\">^<\/a><\/b>\u00a0Benson, C.S., 1961, &#8220;Stratigraphic studies in the snow and firn of the Greenland Ice Sheet&#8221;,\u00a0<i>Res. Rep. 70<\/i>, U.S. Army Snow, Ice and Permafrost Res Establ., Corps of Eng., 120 pp<\/li>\n<li id=\"cite_note-14\"><b><a href=\"#cite_ref-14\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.grid.unep.ch\/activities\/global_change\/switzerland.php\" rel=\"nofollow\">&#8220;Glacier change and related hazards in Switzerland&#8221;<\/a>. UNEP. Retrieved 2009-01-05.<\/li>\n<li id=\"cite_note-15\"><b><a href=\"#cite_ref-15\">^<\/a><\/b>\u00a0<a href=\"http:\/\/folk.uio.no\/kaeaeb\/publications\/grl04_paul.pdf\" rel=\"nofollow\">&#8220;Frank Paul, et al., 2004, Rapid disintegration of Alpine glaciers observed with satellite data, GEOPHYSICAL RESEARCH LETTERS, VOL. 31, L21402, {{doi|10.1029\/2004GL020816}}&#8221;<\/a>\u00a0(PDF). 2004.<\/li>\n<li id=\"cite_note-16\"><b><a href=\"#cite_ref-16\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nichols.edu\/departments\/Glacier\/glacier_retreat.htm\" rel=\"nofollow\">&#8220;Recent Global Glacier Retreat Overview&#8221;<\/a>\u00a0(PDF). Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-GreveBlatter2009-17\"><b><a href=\"#cite_ref-GreveBlatter2009_17-0\">^<\/a><\/b>\u00a0Greve, R.; Blatter, H. (2009).\u00a0<i>Dynamics of Ice Sheets and Glaciers<\/i>. Springer. doi:<a href=\"http:\/\/dx.doi.org\/10.1007%2F978-3-642-03415-2\" rel=\"nofollow\">10.1007\/978-3-642-03415-2<\/a>. ISBN\u00a0978-3-642-03414-5.<\/li>\n<li id=\"cite_note-18\"><b><a href=\"#cite_ref-18\">^<\/a><\/b>\u00a0W.S.B. Paterson, Physics of ice<\/li>\n<li id=\"cite_note-19\"><b><a href=\"#cite_ref-19\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.nasa.gov\/vision\/earth\/lookingatearth\/moulin-20061211.html\" rel=\"nofollow\">&#8220;Moulin &#8216;Blanc&#8217;: NASA Expedition Probes Deep Within a Greenland Glacier&#8221;<\/a>. NASA. 2006-12-11. Retrieved 2009-01-05.<\/li>\n<li id=\"cite_note-20\"><b><a href=\"#cite_ref-20\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.geo.hunter.cuny.edu\/tbw\/ncc\/Notes\/chap3.landforms\/erosion.deposition\/glaciers.htm\" rel=\"nofollow\">Glacier properties Hunter College CUNY lectures<\/a><\/li>\n<li id=\"cite_note-21\"><b><a href=\"#cite_ref-21\">^<\/a><\/b>\u00a0<a href=\"http:\/\/earth.esa.int\/pub\/ESA_DOC\/gothenburg\/154stroz.pdf\" rel=\"nofollow\">T. Strozzi et al.:\u00a0<i>The Evolution of a Glacier Surge Observed with the ERS Satellites<\/i><\/a>\u00a0(pdf, 1.3 Mb)<\/li>\n<li id=\"cite_note-22\"><b><a href=\"#cite_ref-22\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.hi.is\/~oi\/bruarjokull_project.htm\" rel=\"nofollow\">&#8220;The Br\u00faarj\u00f6kull Project: Sedimentary environments of a surging glacier. The Br\u00faarj\u00f6kull Project research idea&#8221;<\/a>. Hi.is. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-23\"><b><a href=\"#cite_ref-23\">^<\/a><\/b>\u00a0Meier &amp; Post (1969)<\/li>\n<li id=\"cite_note-people.deas.harvard.edu-24\">^\u00a0<a href=\"#cite_ref-people.deas.harvard.edu_24-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-people.deas.harvard.edu_24-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/people.deas.harvard.edu\/~vtsai\/files\/EkstromNettlesTsai_Science2006.pdf\" rel=\"nofollow\">http:\/\/people.deas.harvard.edu\/~vtsai\/files\/EkstromNettlesTsai_Science2006.pdf<\/a>\u00a0Ekstr\u00f6m, G., M. Nettles, and V. C. Tsai (2006)&#8221;Seasonality and Increasing Frequency of Greenland Glacial Earthquakes&#8221;,\u00a0<i>Science<\/i>, 311, 5768, 1756-1758, doi:<a href=\"http:\/\/dx.doi.org\/10.1126%2Fscience.1122112\" rel=\"nofollow\">10.1126\/science.1122112<\/a><\/li>\n<li id=\"cite_note-TsaiEkstrom_JGR2007_2007-25\">^\u00a0<a href=\"#cite_ref-TsaiEkstrom_JGR2007_2007_25-0\"><sup><i><b>a<\/b><\/i><\/sup><\/a>\u00a0<a href=\"#cite_ref-TsaiEkstrom_JGR2007_2007_25-1\"><sup><i><b>b<\/b><\/i><\/sup><\/a>\u00a0<a href=\"http:\/\/people.deas.harvard.edu\/~vtsai\/files\/TsaiEkstrom_JGR2007.pdf\" rel=\"nofollow\">http:\/\/people.deas.harvard.edu\/~vtsai\/files\/TsaiEkstrom_JGR2007.pdf<\/a>\u00a0Tsai, V. C. and G. Ekstr\u00f6m (2007). &#8220;Analysis of Glacial Earthquakes&#8221;, J. Geophys. Res., 112, F03S22, doi:<a href=\"http:\/\/dx.doi.org\/10.1029%2F2006JF000596\" rel=\"nofollow\">10.1029\/2006JF000596<\/a><\/li>\n<li id=\"cite_note-26\"><b><a href=\"#cite_ref-26\">^<\/a><\/b>\u00a0Easterbrook, D.J. (1999).\u00a0<i>Surface Processes and Landforms<\/i>\u00a0(2 ed.). New Jersey: Prentice-Hall, Inc. p.\u00a0546. ISBN\u00a00-13-860958-6.<\/li>\n<li id=\"cite_note-27\"><b><a href=\"#cite_ref-27\">^<\/a><\/b>\u00a0<a href=\"http:\/\/pubs.usgs.gov\/of\/2004\/1216\/no\/no.html\" rel=\"nofollow\">&#8220;Glossary of Glacier Terminology&#8221;<\/a>. Pubs.usgs.gov. 2012-06-20. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-28\"><b><a href=\"#cite_ref-28\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.ga.gov.au\/education\/facts\/landforms\/auslform.htm\" rel=\"nofollow\">&#8220;C.D. Ollier: &#8221;Australian Landforms and their History&#8221;, National Mapping Fab, Geoscience Australia&#8221;<\/a>. Ga.gov.au. 2010-11-18. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-29\"><b><a href=\"#cite_ref-29\">^<\/a><\/b>\u00a0KINCAID, JONI L.; KLEIN, ANDREW G. (2004).\u00a0<a href=\"http:\/\/www.easternsnow.org\/proceedings\/2004\/kincaid_and_klein.pdf\" rel=\"nofollow\">&#8220;Retreat of the Irian Jaya Glaciers from 2000 to 2002 as Measured from IKONOS Satellite Images&#8221;<\/a>. Portland, Maine, USA. pp.\u00a0147\u2013157. Retrieved 2009-01-05.<\/li>\n<li id=\"cite_note-30\"><b><a href=\"#cite_ref-30\">^<\/a><\/b>\u00a0<a href=\"http:\/\/geology.com\/press-release\/hawiian-glaciers\/\" rel=\"nofollow\">&#8220;Hawaiian Glaciers Reveal Clues to Global Climate Change&#8221;<\/a>. Geology.com. 2007-01-26. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-31\"><b><a href=\"#cite_ref-31\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.discoverfrance.net\/Colonies\/Crozet.shtml\" rel=\"nofollow\">&#8220;French Colonies &#8211; Crozet Archipelago&#8221;<\/a>. Discoverfrance.net. 2010-12-09. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-32\"><b><a href=\"#cite_ref-32\">^<\/a><\/b>\u00a0Collins, Henry Hill;\u00a0<b>Europe and the USSR<\/b>; p. 263. ISBN 1-256-35000-3<\/li>\n<li id=\"cite_note-33\"><b><a href=\"#cite_ref-33\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.beringia.com\/centre_info\/exhibit.html\" rel=\"nofollow\">&#8220;Yukon Beringia Interpretive Center&#8221;<\/a>. Beringia.com. 1999-04-12. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-34\"><b><a href=\"#cite_ref-34\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.eas.slu.edu\/People\/KChauff\/earth_history\/4EH-posted.pdf\" rel=\"nofollow\">Earth History 2001<\/a>\u00a0(page 15)<\/li>\n<li id=\"cite_note-35\"><b><a href=\"#cite_ref-35\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.wku.edu\/~smithch\/biogeog\/SCHM1946.htm\" rel=\"nofollow\">&#8220;On the Zoogeography of the Holarctic Region&#8221;<\/a>. Wku.edu. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-36\"><b><a href=\"#cite_ref-36\">^<\/a><\/b>\u00a0&#8216;Glaciers &amp; Glaciation&#8217; (Arnold, London 1998) Douglas Benn and David Evans, pp324-326<\/li>\n<li id=\"cite_note-britannica-37\"><b><a href=\"#cite_ref-britannica_37-0\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.britannica.com\/EBchecked\/topic\/315739\/kettle\" rel=\"nofollow\">&#8220;Kettle geology&#8221;<\/a>. Britannica Online. Retrieved 2009-03-12.<\/li>\n<li id=\"cite_note-38\"><b><a href=\"#cite_ref-38\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.lpi.usra.edu\/meetings\/polar2003\/pdf\/8112.pdf\" rel=\"nofollow\">&#8220;Kargel, J.S. et al.:&#8221;Martian Polar Ice Sheets and Mid-Latitude Debris-Rich Glaciers, and Terrestrial Analogs&#8221;, Third International Conference on Mars Polar Science and Exploration, Alberta, Canada, October 13-17, 2003 (pdf 970 Kb)&#8221;<\/a>\u00a0(PDF). Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-39\"><b><a href=\"#cite_ref-39\">^<\/a><\/b>\u00a0<a href=\"http:\/\/www.esa.int\/SPECIALS\/Mars_Express\/SEMS3PMZCIE_0.html\" rel=\"nofollow\">&#8220;Martian glaciers: did they originate from the atmosphere? ESA Mars Express, 20 January 2006&#8221;<\/a>. Esa.int. 2006-01-20. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-40\"><b><a href=\"#cite_ref-40\">^<\/a><\/b>\u00a0Head, J. et al. 2005. Tropical to mid-latitude snow and ice accumulation, flow and glaciation on Mars. Nature: 434. 346-350<\/li>\n<li id=\"cite_note-41\"><b><a href=\"#cite_ref-41\">^<\/a><\/b>\u00a0Source: Brown University Posted Monday, October 17, 2005 (2005-10-17).\u00a0<a href=\"http:\/\/www.marstoday.com\/news\/viewpr.html?pid=18050\" rel=\"nofollow\">&#8220;Mars&#8217; climate in flux: Mid-latitude glaciers | SpaceRef &#8211; Your Space Reference&#8221;<\/a>. Marstoday.com. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-42\"><b><a href=\"#cite_ref-42\">^<\/a><\/b>\u00a0Richard Lewis (2008-04-23).\u00a0<a href=\"http:\/\/news.brown.edu\/pressreleases\/2008\/04\/martian-glaciers\" rel=\"nofollow\">&#8220;Glaciers Reveal Martian Climate Has Been Recently Active | Brown University News and Events&#8221;<\/a>. News.brown.edu. Retrieved 2013-01-04.<\/li>\n<li id=\"cite_note-43\"><b><a href=\"#cite_ref-43\">^<\/a><\/b>\u00a0Plaut, J. et al. 2008. Radar Evidence for Ice in Lobate Debris Aprons in the Mid-Northern Latitudes of Mars. Lunar and Planetary Science XXXIX. 2290.pdf<\/li>\n<li id=\"cite_note-44\"><b><a href=\"#cite_ref-44\">^<\/a><\/b>\u00a0Holt, J. et al. 2008. Radar Sounding Evidence for Ice within Lobate Debris Aprons near Hellas Basin, Mid-Southern Latitudes of Mars. Lunar and Planetary Science XXXIX. 2441.pdf<\/li>\n<\/ol>\n<\/div>\n<h2>References<\/h2>\n<ul>\n<li><i>This article draws heavily on the corresponding article in the Spanish-language Wikipedia, which was accessed in the version of 24 July 2005.<\/i><\/li>\n<li>Hambrey, Michael; Alean, J\u00fcrg (2004).\u00a0<i>Glaciers<\/i>\u00a0(2nd ed.). Cambridge University Press. ISBN\u00a00-521-82808-2. OCLC\u00a054371738.\u00a0An excellent less-technical treatment of all aspects, with superb photographs and firsthand accounts of glaciologists&#8217; experiences. All images of this book can be found online (see Weblinks: Glaciers-online)<\/li>\n<li>Benn, Douglas I.; Evans, David J. A. (1999).\u00a0<i>Glaciers and Glaciation<\/i>. Arnold. ISBN\u00a00-470-23651-5. OCLC\u00a038329570.<\/li>\n<li>Bennett, M. R.; Glasser, N. F. (1996).\u00a0<i>Glacial Geology: Ice Sheets and Landforms<\/i>. John Wiley &amp; Sons. ISBN\u00a00-471-96344-5. OCLC\u00a033359888 37536152.<\/li>\n<li>Hambrey, Michael (1994).\u00a0<i>Glacial Environments<\/i>. University of British Columbia Press, UCL Press. ISBN\u00a00-7748-0510-2. OCLC\u00a030512475.\u00a0An undergraduate-level textbook.<\/li>\n<li>Knight, Peter G (1999).\u00a0<i>Glaciers<\/i>. Cheltenham: Nelson Thornes. ISBN\u00a00-7487-4000-7. OCLC\u00a042656957 63064183 77294832.\u00a0A textbook for undergraduates avoiding mathematical complexities<\/li>\n<li>Walley, Robert (1992).\u00a0<i>Introduction to Physical Geography<\/i>. Wm. C. Brown Publishers.\u00a0A textbook devoted to explaining the geography of our planet.<\/li>\n<li>W. S. B. Paterson (1994).\u00a0<i>Physics of Glaciers<\/i>\u00a0(3rd ed.). Pergamon Press. ISBN\u00a00-08-013972-8. OCLC\u00a026188.\u00a0A comprehensive reference on the physical principles underlying formation and behavior.<\/li>\n<\/ul>\n<h2>External links<\/h2>\n<ul>\n<li><a href=\"http:\/\/danbbs.dk\/~stst\/glaciologi\/\" rel=\"nofollow\">Glacial structures &#8211; photo atlas<\/a><\/li>\n<li><a href=\"http:\/\/www.glaciares.org\/\" rel=\"nofollow\">Glaciers of the Pyrenees<\/a><\/li>\n<li><a href=\"http:\/\/www.pbs.org\/now\/shows\/516\/index.html\" rel=\"nofollow\">NOW on PBS &#8220;On Thin Ice&#8221;<\/a><\/li>\n<li><a href=\"http:\/\/www.asiasociety.org\/onthinnerice\" rel=\"nofollow\">Photo project tracks changes in Himalayan glaciers since 1921<\/a><\/li>\n<li>Short radio episode\u00a0<i><b><a href=\"http:\/\/californialegacy.org\/radio_anthology\/scripts\/muir.html\" rel=\"nofollow\">California Glaciers<\/a><\/b><\/i>\u00a0from\u00a0<i>The Mountains of California<\/i>\u00a0by John Muir, 1894. California Legacy Project<\/li>\n<li><a href=\"http:\/\/donlehmanjr.com\/Mountain\/08%20The%20Dynamics%20of%20Glaciers.htm\" rel=\"nofollow\">Dyanamics of Glaciers<\/a><\/li>\n<\/ul>\n<\/div>\n","protected":false},"author":5,"menu_order":6,"template":"","meta":{"_candela_citation":"[]","CANDELA_OUTCOMES_GUID":"","pb_show_title":"on","pb_short_title":"","pb_subtitle":"","pb_authors":[],"pb_section_license":""},"chapter-type":[],"contributor":[],"license":[],"class_list":["post-71","chapter","type-chapter","status-publish","hentry"],"part":948,"_links":{"self":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapters\/71","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapters"}],"about":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/wp\/v2\/types\/chapter"}],"author":[{"embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/wp\/v2\/users\/5"}],"version-history":[{"count":4,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapters\/71\/revisions"}],"predecessor-version":[{"id":950,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapters\/71\/revisions\/950"}],"part":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/parts\/948"}],"metadata":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapters\/71\/metadata\/"}],"wp:attachment":[{"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/wp\/v2\/media?parent=71"}],"wp:term":[{"taxonomy":"chapter-type","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/pressbooks\/v2\/chapter-type?post=71"},{"taxonomy":"contributor","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/wp\/v2\/contributor?post=71"},{"taxonomy":"license","embeddable":true,"href":"https:\/\/courses.lumenlearning.com\/suny-earthscience\/wp-json\/wp\/v2\/license?post=71"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}