Monday, 9 January 2012

Introduction to Climate

There are two major aspects of global climate, both related to latitude: variation in the distribution of solar radiation with respect to time (seasonal) and space.  

First:  Variation in TIME – the seasons

Since the earth's axis of spin always points in +/- the same direction relative to the cosmos at large (the N. pole always points towards the Pole Star – which is why that star never seems to move in the sky, either through the night or across the seasons) and the same spin axis is not perpendicular to the plane of earth's orbit around the sun (it's ~23.5° from the vertical), then the effective latitude of any given point on earth cyclically increases and decreases as the earth moves around the sun.  This means that daylength and radiation levels increase and decrease throughout the year, these effects being most marked at higher latitudes (see the diagram a little lower, to the right) - that is, we experience seasons.  Longer days and stronger radiation we call summer, and so on.  



The four main landmarks on earth's orbit (shown in the figure above right) are:  

two solstices (northern summer, ~June 21, to the left; northern winter, ~December 21, to the right), when the axis tilt is normal with respect to the orbit – one pole is tilted either 23.5° towards or 23.5° away from the sun – and daylength is a maximum or minimum, depending on which hemisphere you're in;  

two equinoxes (~March 20; ~September 22), when the axis tilt is tangential to the orbit – tilted neither towards nor away from the sun – and daylength is exactly 12h. everywhere, from pole to pole, because the sun rises due east and sets due west everywhere on those two days.  The two solstices, mid-winter and mid-summer, are separated by two equinoxes, either the spring (vernal) or fall (autumnal) equinox. 

As well as thus dictating seasonality, the axis tilt of ~23.5° from the vertical also defines: 

latitudes above which the sun is permanently above the horizon at midsummer solstice and permanently below it at midwinter solstice:  these are the Arctic and Antarctic Circles – at (90°- 23.5°) = 66.5°.  The Arctic Circle is visible in the diagram above; 

latitudes  below which the sun is directly overhead on at least one day a year:  the Tropics of Cancer and Capricorn – at 23.5° either side of the equator.  Within the tropic latitudes, the sun is directly overhead twice a year – exactly every six months on the equator.  This means that, in the tropic latitudes, the mid-day sun is part of the year in the southern sky and the rest of the year in the northern sky.

Second: Variation in SPACE – latitudinal patterns.   

Major global patterns in climate are driven by latitudinal variation in the amount of solar energy that impinges on the planet's surface and the effects of this variation in solar heating on the behaviour of the atmosphere.  

This variation in heating has three primary causes:

1. Lower latitudes receive more radiation per unit area (see diagram at left), because any given-sized "packet" of radiation hits earth at angles close to 90° (i.e. it arrives ~perpendicular to the earth's  surface), but that same energy impinges much more obliquely at higher latitudes - it gets spread over a larger area

2.  At low latitudes the arriving energy passes directly through a minimum depth of absorbing and scattering atmosphere, while at higher latitudes, the energy's oblique path through the atmosphere is longer, meaning that more energy is scattered away into the cosmos. 

3.  At lower latitudes, incoming radiation suffers minimal reflection from the atmosphere and from the earth's surface, whereas the low angle of incidence at higher latitudes means that more energy is reflected away.  

The sum of these sources of variation in irradiation according to latitude (see diagram to the right) is a corresponding variation in the heating of the earth's surface, as short-wave solar radiation is absorbed by the earth.  This energy heats the earth, and then gets re-radiated as long-wave radiation, and this form of the energy heats the atmosphere.  

The relatively great heating of the earth's surface around the equatorial belt sets up a massive upward convection current in the atmosphere in the equatorial region (see diagram immediately below, left), and this broad belt of strongly rising air, which girdles the equator, takes lots of water vapour up to high altitudes (about 10,000 m), where it cools, and the vapour condenses, falling back to earth as rain.  Thus, much of the equatorial zone is both hot and humid, and typically with low atmospheric pressure.
The mass of air, now much colder and drier, cannot fall straight back down to earth, but must move out of the way to make way for the next day's strong updraft.  So it must move away from the equator, either north or south (the diagram at left only shows the northern hemisphere).  Meanwhile, at ground level, the upward convection current, centred on the equator, produces a lowered air-pressure (at L) which draws surface air towards the equator from higher latitudes, either north or south.  At about 20-30° north and south of the equator, this equator-wards movement of surface air begins to pull down the air mass from higher altitudes, which, if you recall, has just traveled up from the equator......  and this air mass, now cooled and dried out, descends towards the earth, making a high-pressure zone  (H, above).  As it descends, it warms, both through compression (ever wondered why your bicycle pump gets so hot? - it isn't just friction), and from radiant heat from the earth's surface.  This descending air mass was dry to start with (most of its moisture was lost as tropical rain), but as it heats up on the way down, it develops a serious water debt, and hits the ground very dry. 

Thus, most of the world's deserts are to be found at 20-30°N. and 20-30°S. latitude, underlying this belt of high atmospheric pressure.

 

 

From this belt, some of the air moves back towards the equator, as we have seen, but some moves pole-wards, towards temperate latitudes.  Thus there are rolling doughnut-shaped belts of air around the earth's middle, between 0° and 30° latitude (one in the northern and one in the southern hemisphere), accompanied by  similar ones, rolling over in the opposite direction, between ~30° and ~60° N & S. 

That's why temperate mid-latitudes are dominated by low-pressure (L) sytems (rising air mass), and are humid (but usually with much less rainfall than the tropics) though cooler than tropical regions, because there's less radiant energy per unit area at higher latitudes.  These major features of earth's climate are shown in the map below.  
 
Note the equatorial belt of high (>1500mm annually) rainfall areas (diagonal hatching) and the smaller similarly very rainy areas in western north and south America.  Mid-temperate latitudes, though damp, are generally not so massively wet as this.  Also note the subtropical and polar belts of arid (<250mm rain) lands (dotted).  Finally, note the high pressure zones (H), where the subtropical dry air masses descend to earth's surface, spreading out either towards the equator or higher latitudes, where troughs of low pressure (L) lie.  Now, why don't the resulting winds move simply north or south? 
 
 
This is because of the Coriolis Effect, which is an apparent force due to the earth's rotation.  The earth spins from west to east (anticlockwise as viewed from the north pole), and this has the effect of making anything that moves (such as an air mass) veer, with respect to the earth's surface, towards the right in the northern hemisphere and towards the left in the s. hemisphere.  
 
Thus the subtropical winds (the Trade Winds) are from the northeast and southeast, while the prevailing winds in temperate latitudes are primarily westerlies, bringing oceanic air onto continents from their western margins.  The dominance of these westerly winds is what lies behind the fact that, in temperate latitudes, westerly continental locations are milder and moister than easterly ones at the same latitude, since they get the moisture of the mild oceanic air masses.  Coastal B.C. is much milder and moister than Newfoundland.  Korea is much colder than Spain.  
 
London, England is much milder than Kamchatka.  At the temperate latitude (40-50°) low pressure zones, there is a continuous "conflict" between the air masses converging on them from the south and the north, and this generates the great climatic instabilities that are typical of the region.  This instability contrasts with the high pressure zones at ~30° and ~60°.  The main atmospheric circulation picture is completed by a third cell, rotating equatorwards at ground level, bringing very cold dry air down to earth in the polar regions.  That's why polar regions are not only very cold but also very dry.

Local climate 

Is affected by anything else that moves the air mass up and down or affects its water-load, such as mountain ranges or the proximity of oceans and large lakes.  As a relatively moist, moving, air mass hits high mountains, it is forced to rise, gets cooler, and the moisture condenses, dropping rain on the lower and mid slopes of the windward side of the mountain-range.  As the air descends on the other side, it gets warmer, and its moisture debt increases.  Thus, in the lee of mountains, it is often especially dry e.g. the Mojave desert, in the lee of the very high Sierra Nevada in s. California (see below). 

The deep interiors of large continents (e.g. east-central Asia, Mongolia - see world map above), are so far downwind from sources of moisture that most of that moisture has already been lost from the air-mass - thus the air is dried, and there can be little rain, and often desertic conditions prevail outside of the main subtropical desert belt, in this case giving the Gobi Desert of northern China and adjacent parts of Mongolia, and the other central Asian deserts around the Caspian and Aral Seas. 

 








North America 

both the high mountains in the far west and the huge size of the continental mass itself have dramatic effects on the simple latitudinal climatic systems discussed earlier, such that, when we focus on the continent alone, and ignore the planet as a whole, the major latitudinal belts are only somewhat in evidence.  Rather, the major precipitation regimes seem largely to be disposed longitudinally (see map of North American precipitation regimes left;  or a more vivid one of the USA.  You will appreciate this steadily drying climate as we drive west from London towards the Rockies. 

A primary message in this map is that local conditions can impose important distortions on the overall global latitudinal pattern;  the other side of this coin is that, if we simply look at such local patterns, we can gain a completely erroneous impression of the nature of the global picture, and the factors which govern it.  Note in the map particularly the high rainfall generated along the mountainous west coast, the arid lands beyond those mountains, the semi-arid and subhumid prairies in the continent's interior, and the generally humid temperate eastern regions.  On other continents, different individual local patterns are generated by the major features of their local topographies. 


Global heating and earth's rotation set up comparable global movements in the enormous body of the earth's oceans.  Again, the moving masses are influenced by the Coriolis Effect, to give major surface currents (largely driven by surface winds) that are usually clockwise in the northern hemisphere (e.g. the Gulf Stream-Canaries current system in the N. Atlantic, or the Kuroshio-California system in the N. Pacific) and anticlockwise in the s. hemisphere e.g. the Benguela-Brazil current in the S. Atlantic). 

Until recently, we only knew about these surface ocean currents, but now we recognize that there is a very important 3-D oceanic system called the Thermohaline Circulation (driven primarily by density differences through variation in temperature and salinity), which provides for massive heat redistribution about the globe.  This complex oceanic circulation, taking place at all depths, with upwellings and downwellings, profoundly affects the temperature of the ocean surface, in turn affecting conditions on nearby land-masses e.g. subtropical coastal upwellings of very cold water off Baja California, Peru and Namibia generate peculiarly high aridity onshore, making some of the world's most arid deserts, such as the Vizcaino of Baja California, the Atacama of Peru and the Namib of s.western Africa. 

A convenient way to summarize much information about the climate of a locality is a Climate Diagram.  These diagrams were invented by Walter & Lieth , and have been widely adopted by most ecologists, geographers and others as an efficient tool.  With a bit of practice you can make a pretty good guess at the vegetation of a locality just from inspection of the climate diagram.  A key to the interpretation of climate diagrams is to be found below, to be used in conjunction with the sample diagrams opposite, and those shown on the rainfall map of the Sonoran desert.

 
Ankara and Odessa are grasslands (steppe);  Douala is tropical rainforest;  Hohenheim is deciduous forest. 

X-axis:  months (N. Hemisphere Jan.-Dec.;  S. Hemisphere July-June).
Y-axis: one div. = 10°C or 20mm rain.  a = locality;  b = altitude above sea-level;  c = length of record (if two, first = temp.;  second = rainfall);  d = mean annual temp. °C;  e = mean annual ppn. in mm;  f = mean daily min. temp. of coldest month;  g = lowest temp. recorded;  h = mean daily max. of warmest month;  i = highest temp. recorded;  j = mean daily temp. variation;  k = curve of mean monthly temp.;  l = curve of mean monthly ppn.;  m = period of relative drought;  n = period of water excess;  o = mean monthly ppn. >100mm. on 1/10 scale;  q = months with daily min. temp. <0°C;  r = late or early frosts;  s = mean duration of frost-free period in days.
Not all the information is shown in all diagrams. 

Whittaker (who popularized the Five Kingdom classification system) noted that the major vegetation types of the world are substantially predicted by two primary climatic variables:  mean annual temperature and total annual precipitation.  

A simplified version of a diagram with these two axes and the various major biomes mapped onto it is shown below (all these biomes are represented in North America and Mexico):
  • Tundra - Arctic and Alpine
  • Taiga - boreal (largely conifer) forest
  • Temperate deciduous (broadleaf) forest
  • Temperate grassland ("prairie" - part of the "woodland, shrubland, grassland" unit)
  • Desert scrub  (cold to hot)
  • Savannahs and thornscrub
  • Tropical forests (including dry seasonal, monsoon, and evergreen "rainforests")

The number of biomes differs according to the authority, but the seven shown in the diagram are commonly recognised.  Often, the tropical forest group is split into a)  the superhumid "rainforest" biome and b)  the seasonal (drought-deciduous) forest biome, while the relatively warm and highly humid temperate conifer (and sometimes deciduous) forests are recognised as Temperate Rainforest, such as those of the northwestern American coast (conifer), the southeastern coast of Australia and the southwestern coasts of New Zealand and Chile (mixed conifer and broadleaf).  Finally, a maritime, summer-drought/winter-rain assemblage called chaparral is often acknowledged, which is typified by woody shrubs with leathery evergreen foliage.  This is found in coastal central Chile, southern California, southwestern Australia, the Cape region of S. Africa, and around the margins of the Mediterranean Sea. 

When we plot the geographic occurence of biomes (variously defined) about the globe we see patterns that strongly recall that of climate.  This is no surprise, given the close integration between climate and vegetation.  Similarly, soils and primary production shows very similar distributions, as we have seen.  So now we have described, from several directions, the phenomena lying behind the fact that, for example, the low-latitude (equatorial) zone is humid, very highly productive and occupied by a very large number of species of plants, largely trees.  

A closer look at those trees will show that, when adult, many of them have the same overall morphology, through evolutionary adaptive convergence:  they are very tall, have a smooth, almost limbless trunk, and a dense canopy at the top;  they usually have large, simply-shaped, somewhat leathery leaves, which persist for several years.  In similar fashion, boreal forests are characterised by trees which are conical in shape, often with branches to the ground, and evergreen, drought-adapted, needle-leaves.  Again, arctic regions are extremely cold and dry and occupied by low-statured, often evergreen plants.  

Finally, deserts show vegetation which is often spiny, succulent, and with great capacities for sustaining high levels of temperature and drought. Though most of us start out with the image of deserts as endless, pitilessly-hot, wastes of sand and rock, and though there are such deserts, this picture is nothing like true of many.  Much desert land is covered by low-diversity scrubby vegetation (albeit sparse) of short bushes and small trees, but some deserts have a quite luxuriant and very diverse vegetation, including good-sized trees e.g. the Sonoran desert of s.w. U.S. and Mexico. 

Major desert systems of the world:

 

Africa

- Kalahari/Namib  (~0.6 x 106 km2);  Sahara (~9 x 106 km2); 
 

Asia

-  Arabian  (~2.6 x 106 km2);  Turkestan/Iranian/Thar (~2.9 x 106 km2);  Takla-Makan (Tarim Basin)/Gobi (~0.8 x 106 km2); 
 

Australia

- Central Desert System (~3.4 x 106 km2); 
 

South America

- Patagonia/Monte(~1 x 106 km2);  Atacama; 
 

North America

- Chihuahuan/Sonoran/Mojave(~0.8 x 106 km2). 
 

Climate

 

     Most very arid deserts are in the subtropical zone of descending dry air masses (see earlier in these notes), but other deserts outside this zone may be caused , or augmented,  by rain-shadow effects (e.g. the Mojave desert) and interior-continental conditions (remote from oceanic moisture - e.g. much of the central Asian desert system).Deserts may be both hot and cold ;  what defines them is their precipitation regime (approx. 200 mm rain or less annually), though the irregularity of the amount and its timing are also typical. 
 
The amount of rain needed to turn a desert into something else, such as desert grassland or thornscrub, depends upon mean annual temperature - the higher the temperature, the more rain you need to compensate for evaporation.  The seasonality of rainfall varies greatly, and has a profound effect on the diversity of the vegetation.  
 
For example, the Mojave desert is a winter-rain (from Pacific) desert, the Chihuahuan has only summer rains (from Gulf of Mexico), and the Sonoran has both winter and summer rains:  the Sonoran desert has a far richer and more complex flora.  Because of the low humidity of the atmosphere, and rare cloud-cover, the diurnal temperature range can be enormous (>30°C) with night-time temperatures below freezing.  Deserts are also typically very windy places, enhancing the effects of a desiccating atmosphere. 
 

Soils

 

    Desert soils are typically poorly developed, because of the low rate of accumulation of organic matter, and because of the periodic cessation of biological activity (due to high temperatures and low soil moisture.  Low availability of N2 favours plant species with N-fixing bacteria in root nodules, such as members of Leguminosae.  Under many conditions, there is an accumulation of salts and CaCO3 at or near the surface. 
 
The carbonate sometimes forms a distict, impervious layer, called caliche or "hard-pan", which profoundly affects the distribution of plants.  In North American deserts, presence of high levels of CaCO3 favours the prototypical American desert plant, creosote bush, Larrea tridentata.  Saline soils are common on flats, in valley bottoms and in basins, and they support characteristic plant communities.   Subject to pronounced wind-erosion (probably the main cause of "desert pavement" on level areas), and severe water erosion from occasional torrential downpours.  
 
Under certain conditions, airborne sediments accumulate in dunes, which have a characteristic flora.  Mountain and hill slopes or bajadas show a regular downhill trend from large rock, stones and coarse gravel to fine gravel and sand (often somewhat saline) on the flats.  This dramatically affects rain percolation and runoff, and provides very different opportunities for root anchorage;  this affects the plant asemblages (see next section).  Surfaces of fine soils are often stabilized by crusts formed by communities of cyanobacteria, algae and lichens. 
 

Vegetation

 

    Plants face the twin problems of high heat load and low, unpredictable, availability of water.  Many striking adaptations to these exacting conditions are found.  In most deserts, there are four major ways of being a plant:  by escaping drought (i.e. by being dormant during the dry period);  by resisting the drought;  by enduring the dought;  and by accessing other sources of water besides local rainfall.  Heat load is often combatted by finely-divided or tiny leaves and/or by near-vertical orientation of leaf-surfaces.  Most plants are drought-deciduous, dropping leaves and even branches, though some are evergreen (notably Larrea).  Because of the scarcity of vegetation, there is also high herbivore pressure, and there are many adaptations to discourage it, including thorns, spines, and chemical compounds, such as tannins and resins. 
 

Drought-escaping

 

commonly means the ephemeral   habit, whereby the plant passes the dry period as fruit/seed (therophyte);  germination, growth & fruiting are accomplished extremely rapidly whenever rain may come.  These desert ephemerals have a very ordinary appearance, since they show no aridity-adaptations except for the dormant seed-stage itself.  Examples from the N. American deserts are:  Baileya, Astragalus, Plantago, Phacelia. 
 

Resisting the drought

 

commonly means the succulent habit, and both stems and leaves are used for water-storage.  Virtually all cacti are stem-succulents;  leaf-succulents include agaves and aloes.  Succulents commonly show CAM metabolism, a photosynthetic pathway which is extremely water-conserving, though providing for only very slow growth.  Examples:  Cereus, Opuntia, Mamillaria (cacti);  Agave, Dudleya, Mesembryanthemum. 
 

Drought-enduring

 

plants are extremely efficient at absorbing rainfall whenever available with a dense mat of adventitious surface roots.  They continue to be active into the dry period as long as possible, using a diversity of water-conserving mechanisms and morphologies, such as sunken stomata, thick, waxy cuticles, dense surface hairs, small leaves.  Some can tolerate an astonishing degree of tissue-water loss e,g Larrea leaves can recover after 50% water loss. 
 
Many trees are capable of accessing deep ground-water, and are thereby independent of local rainfall.  Such plants are called phreatophytes:  a mesquite tree (Prosopis) will have as much or more woody growth below ground as above.  Examples are:  Cercidium, Acacia, Prosopis, Mimosa, Olneya. 

Some plants can absorb dew, and a diversity of plants and lichens that do this are epiphytic, sitting in the branches of trees and shrubs e.g. Tillandsia. 

Upper slopes occupied by a diverse vegetation, including trees, bushes and larger cacti (when present);  middle slopes dominated by bushes (including Ambrosia, Krameria), including bush-type cacti;  lower slopes and flats typically occupied by smaller bushes (including Ambrosia, Larrea);  water courses support larger bushes and trees, even out on the flats.  Saline flats and basins are occupied by halophytes, which are capable of tolerating higher concentrations of salt in the tissues (e.g. Atriplex);  some are capable of excreting salt through special glands (e.g. Tamarix).

Animals

 

    Most animals evade rather than endure the desert extremes.  Thus, much of the smaller animal life (rodents, lizards, snakes) is subterranean during the day (burrows >50 cm deep remain cool and moist), emerging to the surface at night.  Many have the capacity to exist on metabolic (from food) water alone and to excrete solid uric acid (e.g. kangaroo rats, Dipodomys).  Some animals remain dormant during rainless periods e.g. snails, frogs and toads.  Though active during much of the daytime, even birds and larger mammals seek shade and inactivity during the hottest times.  Saline waters are occupied by a diversity of bacteria, and fed upon by a few invertebrates, notably brine-shrimp, Artemia.

Sunday, 8 January 2012

Introduction to Earth's Surface

Location

 

Wherever you are on Earth's surface, in order to describe your location, you need some point of reference. Right now you are probably reading this chapter at your computer. But where is your computer? It may set up in a certain place or you may be on a laptop computer, which means you can change where you are. In order to describe your location, you could name other items around you to give a more exact position of your computer. Or you could measure the distance and direction that you are from a reference point. For example, you may be sitting in a chair that is one meter to the right of the door. This statement provides more precise information for someone to locate your position within the room.

Similarly, when studying the Earth's surface, Earth scientists must be able to pinpoint any feature that they observe and be able to tell other scientists where this feature is on the Earth’s surface. Earth scientists have a system to describe the location of any feature. To describe your location to a friend when you are trying to get together, you could do what we did with describing the location of the computer in the room. You would give her a reference point, a distance from the reference point, and a direction, such as, "I am at the corner of Maple Street and Main Street, about two blocks north of your apartment." Another way is to locate the feature on a coordinate system, using latitude and longitude. Lines of latitude and longitude form a grid that measures distance from a reference point. You will learn about this type of grid when we discuss maps later in this chapter.

Direction

 

If you are at a laptop, you can change your location. When an object is moving, it is not enough to describe its location; we also need to know direction. Direction is important for describing moving objects.

For example, a wind blows a storm over your school. Where is that storm coming from? Where is it going? The most common way to describe direction in relation to the Earth’s surface is by using a compass.

(Figure 2.1). The compass is a device with a floating needle that is a small magnet.


 
Figure 2.1: A compass is a device that is used to determine direction. The needle points to the Earth's magnetic north pole.
 
(Figure 2.2). The needle aligns itself with the Earth's magnetic field, so that the compass needle points to magnetic north. Once you find north, you can then describe any other direction, such as east, south, west, etc., on a compass rose (Figure 2.2).

 
Figure 2.2: A compass rose shows the various directions, such as North (N), East (E), South (S), West (W), and various combinations.
 
(Figure 2.3) A compass needle aligns to the Earth's magnetic North Pole, not the Earth’s geographic North Pole or true north. The geographic North Pole is the top of the imaginary axis upon which the Earth’s rotates, much like the spindle of a spinning top. The magnetic North Pole shifts in location over time. Depending on where you live, you can correct for this difference when you use a map and a compass .

 
Figure 2.3: Earth's magnetic north pole (B) is about 11 degrees offset from its geographic north pole (A) on the axis of rotation.

(Figure 2.4) When you study maps later, you will see that certain types of maps have a double compass rose to make the corrections between magnetic north and true north. An example of this type is a nautical chart that sailors and boaters use to chart their positions at sea or offshore 

 
Figure 2.4: Nautical maps include a double compass rose that shows both magnetic directions (inner circle) and geographic compass directions (outer circle).
 

Topography

 

As you know, the surface of the Earth is not flat. Some places are high and some places are low. 

For example, mountain ranges like the Sierra Nevada in California or the Andes mountains in South America are high above the surrounding areas. 

(Figure 2.5) We can describe the topography of a region by measuring the height or depth of that feature relative to sea level . 

You might measure your height relative to your best friend or classmate. When your class lines up, some kids make high "mountains" and others are more like small hills!What scientists call relief or terrain includes all the major features or landforms of a region. A topographic map of an area shows the differences in height or elevation for mountains, craters, valleys, and rivers. 

Figure 2.6 The San Francisco Mountain area in northern Arizona as well as some nearby lava flows and craters. We will talk about some different landforms in the next section.

 
Figure 2.6: This image was made from data of the Landsat satellite and shows the topography of the San Francisco Mountain and surrounding areas in northern Arizona. You can see the differences in elevation of the mountain and surrounding lava flows.
 

Landforms 

 

(Figure 2.7),the Earth's surface and take away the water in the oceans , you will see that the surface has two distinctive features, continents and the ocean basins. 


The continents are large land areas extending from high elevations to sea level. The ocean basins extend from the edges of the continents down steep slopes to the ocean floor and into deep trenches.

 
Figure 2.7: This image shows examples of some of the main features found on the ocean floor, as well as their above-water continuations. The red areas are high elevations (mountains). Yellow and green areas are lower elevations and blue areas are the lowest on the ocean floor.
 
Both the continents and the ocean floor have many features with different elevations. Some areas of the continents are high. These are the mountains we have already talked about. Even on the ocean floor there are mountains! Let's discuss each.

 
Figure 2.8: Features of continents include mountain ranges, plateaus, and plains.
 

Continents

 

Continents are relatively old (billions of years) compared to the ocean basins (millions of years). Because the continents have been around for billions of years, a lot has happened to them! As continents move over the Earth's surface, mountains are formed when continents collide. Once a mountain has formed, it gradually wears down by weathering and erosion. 

(Figure 2.8) Every continent has mountain ranges with high elevations . Some mountains formed a very long time ago and others are still forming today:
  • Young mountains (<100 million years) – Mountains of the Western United States (Rocky Mountains, Sierra Nevada, Cascades), Mountains around the edge of the Pacific Ocean, Andes Mountains (South America), Alps (Europe), Himalayan Mountains (Asia)
  • Old mountains (>100 million years) – Appalachian Mountains (Eastern United States), Ural Mountains (Russia).
Mountains can be formed when the Earth's crust pushes up, as two continents collide, like the Appalachian Mountains in the eastern United States and the Himalayas in Asia. Mountains can also be formed by a long chain of volcanoes at the edge of a continent, like the Andes Mountains in South America.

Over millions of years, mountains are worn down by rivers and streams to form high flat areas called plateaus or lower lying plains. Interior plains are in the middle of continents while coastal plains are on the edge of a continent, where it meets the ocean.

 
Figure 2.9: Summary of major landforms on continents and features of coastlines.As rivers and streams flow across continents, they cut away at rock, forming river valleys (Figure 2.9). The bits and pieces of rock carried by rivers are deposited where rivers meet the oceans. These can form deltas, like the Mississippi River delta and barrier islands, like Padre Island in Texas. Our rivers bring sand to the shore which forms our beaches.

Ocean Basins

 

The ocean basins begin where the ocean meets the land. The names for the parts of the ocean nearest to the shore still have the word “continental” attached to them because the continents form the edge of the ocean. The continental margin is the part of the ocean basin that begins at the coastline and goes down to the ocean floor. It starts with the continental shelf, which is a part of the continent that is underwater today.

(Figure 2.10)  The continental shelf usually goes out about 100 – 200 kilometers and is about 100-200 meters deep, which is a very shallow area of the ocean

Figure 2.10: Diagram of the continental shelf and slope of the southeastern United States leading down to the ocean floor.
 
From the edge of the continental shelf, the continental slope is the hill that forms the edge of the continent. As we travel down the continental slope, before we get all the way to the ocean floor, there is often a large pile of sediments brought from rivers, which forms the continental rise. The continental rise ends at the ocean floor, which is called the abyssal plain.

The ocean floor itself is not totally flat. Small hills rise above the thick layers of mud that cover the ocean floor. In many areas, small undersea volcanoes, called

seamounts 

(Figure 2.11) rise more than 1000 m above the seafloor. Besides seamounts, there are long, very tall (about 2 km) mountain ranges that form along the middle parts of all the oceans.

(Figure 2.12) They are connected in huge ridge systems called mid-ocean ridges  The mid-ocean ridges are formed from volcanic eruptions, when molten rock from inside the Earth breaks through the crust, flows out as lava and forms the mountains.

New England Seamounts
Bear Seamount
 
 
Figure 2.12: Map of the mid-ocean ridge system (yellow-green) in the Earth’s oceans.
 
 
Figure 2.13: This map shows the location of the Mariana Trench in the Pacific Ocean.
 
The deepest places of the ocean are the ocean trenches. There are many trenches in the world's oceans, especially around the edge of the Pacific Ocean.

(Figure 2.13) The Mariana Trench, which is located east of Guam in the Pacific Ocean, is the deepest place in the ocean, about 11 kilometers deep.

To compare the deepest place in the ocean with the highest place on land, Mount Everest is less than 9 kilometers tall. In these trenches, the ocean floor sinks deep inside the Earth. The ocean floor gets constantly recycled. New ocean floor is made at the mid-ocean ridges and older parts are destroyed at the trenches. This recycling is why the ocean basins are so much younger than the continents.

The Earth’s surface is constantly changing over long periods of time. For example, new mountains get formed by volcanic activity or uplift of the crust. Existing mountains and continental landforms get worn away by erosion.

Rivers and streams cut into the continents and create valleys, plains, and deltas. Underneath the oceans, new crust forms at the mid-ocean ridges, while old crust gets destroyed at the trenches. Wave activity erodes the tops of some seamounts and volcanic activity creates new ones. You will explore the ways that the Earth's surface changes as you proceed through this book.

OCEAN BASINS and CONTINENTAL MARGINS

There are two types of continental margins:

  • passive, and

  • active margins.

Passive margins, which are common around the Atlantic Ocean, consist of:
  • Continental Shelves,
  • Continental Slopes, and
  • Continental Rises.

Active margins, which are common around the Pacific Ocean, consist of:

  • Continental Shelves,

  • Continental Slopes,
  • Ocean or Submarine Trenches.

The Continental Shelf

 The continental shelf (CS) is a gently-sloping submerged edge of the continents that makes up 18% of the continental surface area. The slope is about 2m per km. The CS is covered by a thick blanket of sediment, eroded from the land and trapped behind natural dams of ancient coral reefs, or fractured ridges of granite. This sediment in some areas is up to 15 km thick. A result of such a massive accumulation of sediment, the seaward edge of the CS has been depressed slowly into a gently inclined slope. Passive CS are generally much wider (up to 1200 km in some areas), and active margins CS are narrower. Typically, the shelf width depends on marine processes such as currents, and sea level fluctuations.

The Shelf Break represents the seaward edge of the CS, which is consistently located at ~ 140 m depth below msl. The only exception is the shelf break around Antarctica which are at depths greater than 140 m (in some areas, at 600 m below msl) because of the massive ice sheets that has depressed the CS around Antartica.

The Continental Slope

The continental slope (CSL) begins seaward of the CS break, and it is identified by an abrupt increase in slope from an average of 2m/km to 70 m/km (or 4 degrees slope). Slopes as steep as 25 degrees has been identified at active margins. The average width is 20 km. Geologically, the seaward edge of the CSL represents the boundary between the continents and the ocean basins.
Associated with the CS and the CSL are a major feature cutting through the CS/CSL at right angle to the shorelines. This feature is known as SUBMARINE CANYONS. Along some passive margins, they appear to be seaward extensions of major river valleys ( examples are the Hudson River, Congo River, and Chesapeake Bay) that deepened during low sea level periods. However, the canyons are generally explained as erosion caused by turbidity currents. Turbidity currents are a consistent slurry of seawater/sediment mixture (like freshly mixed concrete). These currents are occasionally activated by submarine earthquakes, which mobilizes the slurry to move downslope at speeds that can attain up to 17 mph.


Continental Rise

The CRs are present only along passive margins. In other words,they are present only where ocean trenches are absent. They typically form at the base of the CSL, where gradient decreases sharply to an average of 6m/km. The feature is formed by accumulating sediment that is delivered downslope by turbidity currents. The CR materials may be moved around by deep ocean currents particularly around western ocean margins where the currents are relatively stronger. The width of CRs can vary from 0.1 to 1000 km.

OCEAN BASINS

Ocean basins typically include the following features:

  • Ocean Trenches,

  • Island Arcs,
  • Abyssal Plains and Hills,
  • Seamounts and Guyots
  • Oceanic Ridge Systems, and
  • Hydrothermal Vents.

OCEAN/SUBMARINE TRENCH

Ocean trenches are long, arc-shaped troughs at the foot of the CSLs, along Active Margins. Trenches also mark the locations of convergent plate boundaries (see Plate Tectonic Chapter), where older oceanic plates plunge into the Asthenosphere. Ocean trenches are also associated with earthquakes, high heat flow, and volcanic activity. Trenches are indeed the deepest areas of the earth surface ( 3 to 6 km below the average ocean floor). The Marianas Trench is 7 km below the adjacent Pacific Ocean floor. Typically, the deepest part of a trench is given a separate name. Ex. the Challenger Deep is the deepest part of the Marianas Trench.

 

ISLAND ARCS

The volcanic activity associated with trenches build up a chain of bow-shaped submarine volcanoes directly above the ocean floor, and landward of the particular trench. These chain of volcanoes become islands over million of years. They also follow the orientation of the trench by producing a set of arc-shaped islands. So the origins of these two oceanic features (trenches, and island arcs) are intimately associated. Typically the trenches that produce a particular island arc is inclined at an angle beneath the island arc. Examples include Japan, Indonesia, Phillipines, and the Aleutian Islands.

ABYSSAL PLAINS/HILLS

The abyssal plains are the flatest, or the most level areas on the Earth's surface. The levelling is a result of fine sediments from the continents covering up most of the volcanic irregularities on the ocean floor. Overall abyssal plains cover 25% of the earth's surface. They are virtually featureless, except near the oceanic ridge areas, where small volcanic hills protruding through the sedimentary layers become common. These abyssal hills are on average less than 200 meters high. The abyssal hills have a complementary relationship to the abyssal plains. Oceans with few abyssal hills tend to have more extensive abyssal plains. Hence abyssal hills are less common in the Atlantic, and Indian Oceans, but common in the Pacific Ocean. Why?

SEAMOUNTS AND GUYOTS

Seamounts are small, relatively steep-sided volcanoes rising to heights of at least 1 km above the average ocean floor. In general, they are submerged volcanoes that may be isolated or organized in chains. In a few places, they are sufficiently elevated to become islands. Many of them form over areas that have highly concentrated heat energy known as hotspots. But a few may form near the ocean ridges. Hence, both types are carried along in the direction of moving tectonic plates. Seamounts are most common in the Pacific Ocean, or any plate with rapid seafloor spreading rates. The Hawaiian Islands are the classic example of a chain of seamounts. A chained set of seamounts indicate the direction of plate movement.

Guyots are flat-topped seamounts whose tops were eroded by surface ocean waves in the past. Because seamounts sink below the ocean water surface as they become older, they are basement or foundations for coral islands in tropical areas.

HYDROTHERMAL VENTS

These are volcanic chimney rocks on the ocean floor where hot, steamy, dark water discharges after being heated below the ocean floor. In a sense, they are submarine hotsprings that were first discovered in 1977 on the East Pacific Rise. Since then, several more have been discovered including one in a deep water lake called Lake Baikal, Russia. Typically, most of them are on or near the ocean ridges. Water temperatures around the vents average 8 - 16 degrees Celcius, which is 100 to 200% higher than the sorrounding deep ocean water (averages at 4 degrees Celcius) away from hydrothermal vents.

These blacksmokers, as they are sometimes referred to, originate from circulating seawater, superheated by very hot volcanic rocks, in active areas of seafloor spreading. The superheated water dissloves minerals from the hot rocks, rises upwards and escape through vents or cracks. The minerals are then deposited as chimneys similar to stalagmites seen in limestone caves.

 

MID-OCEAN RIDGES (MOR)

These are linear, elevated parts of the ocean floor that typically mark the divergent plate boundaries. The MORs are known as the most extensive features on the Earth's surface. Indeed, they are present in all ocean basins. Their total length is estimated worldwide to be 65,000 km or about 40,000 miles, and they can be as wide as 500 km in some areas. Their elevation may vary from 2.5 km above the average ocean floor, to elevations above the ocean water surface. Islands such as Iceland, Easter Island, the Azores, are all examples of MORs built up above msl (into islands).

The active areas of MORs are the mid-section known as the Rift Zone. Within the rift zone are deep, narrow valleys offset in many places by perpendicular faults known as Transform Faults. Also, the following properties are typical of the rift zone:

  • heat flow is high.

  • valley walls are elevated. Why?
  • earthquakes are frequent. Why?
  • volcanic eruptions are frequent. Why?
As this elevated, hot part of the lithosphere cools, it shrinks and sinks. Over millions of years, it becomes more like the flatter, gently sloping abyssal plains, and hills.
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