PMF IAS Current Affairs
PMF IAS Current Affairs

Vertical & Horizontal Temperature Distribution of Oceans

Subscribe to Never Miss an Important Update! Assured Discounts on New Products!

Temperature Distribution of Oceans

  • The study of the temperature of the oceans is important for determining the
  1. movement of large volumes of water (vertical and horizontal ocean currents),
  2. type and distribution of marine organisms at various depths of oceans,
  3. climate of coastal lands, etc.

Source of Heat in Oceans

  • The sun is the principal source of energy (Insolation).
  • The ocean is also heated by the inner heat of the ocean itself (earth’s interior is hot. At the sea surface, the crust is only about 5 to 30 km thick). But this heat is negligible compared to that received from sun.

How does deep water marine organisms survive in spite of absence of sunlight?

  • Photic zone is only about few hundred meters. It depends on lot of factors like turbidity, presence of algae etc..
  • There are no enough primary producers below few hundred meters till the ocean bottom.
  • At the sea bottom, there are bacteria that make use of heat supplied by earth’s interior to prepare food. So, they are the primary producers.
  • Other organisms feed on these primary producers and subsequent secondary producers.
  • So, the heat from earth supports wide ranging deep water marine organisms.

But the productivity is too low compared to ocean surface.

Why is diurnal range of ocean temperatures too small?, Why oceans take more time to heat or cool?

  • The process of heating and cooling of the oceanic water is slower than land due to vertical and horizontal mixing and high specific heat of water.
  • (More time required to heat up a Kg of water compared to heating the same unit of a solid at same temperatures and with equal energy supply).

The ocean water is heated by three processes.

  1. Absorption of sun’s radiation.
  2. The conventional currents: Since the temperature of the earth increases with increasing depth, the ocean water at great depths is heated faster than the upper water layers. So, convectional oceanic circulations develop causing circulation of heat in water.
  3. Heat is produced due to friction caused by the surface wind and the tidal currents which increase stress on the water body.

The ocean water is cooled by

  1. Back radiation (heat budget) from the sea surface takes place as the solar energy once received is reradiated as long wave radiation (terrestrial radiation or infrared radiation) from the seawater.
  2. Exchange of heat between the sea and the atmosphere if there is temperature difference.
  3. Evaporation: Heat is lost in the form of latent heat of evaporation (atmosphere gains this heat in the form of latent heat of condensation).

Factors Affecting Temperature Distribution of Oceans

  • Insolation: The average daily duration of insolation and its intensity.
  • Heat loss: The loss of energy by reflection, scattering, evaporation and radiation.
  • Albedo: The albedo of the sea (depending on the angle of sun rays).
  • The physical characteristics of the sea surface: Boiling point of the sea water is increased in the case of higher salinity and vice versa [Salinity increased == Boiling point increased == Evaporation decreased].
  • The presence of submarine ridges and sills [Marginal Seas]: Temperature is affected due to lesser mixing of waters on the opposite sides of the ridges or sills.
  • The shape of the ocean: The latitudinally extensive seas in low latitude regions have warmer surface water than longitudinally extensive sea [Mediterranean Sea records higher temperature than the longitudinally extensive Gulf of California].
  • The enclosed seas (Marginal Seas – Gulf, Bay etc.) in the low latitudes record relatively higher temperature than the open seas; whereas the enclosed seas in the high latitudes have lower temperature than the open seas.
  • Local weather conditions such as cyclones.
  • Unequal distribution of land and water: The oceans in the northern hemisphere receive more heat due to their contact with larger extent of land than the oceans in the southern hemisphere.
  • Prevalent winds generate horizontal and sometimes vertical ocean currents: The winds blowing from the land towards the oceans (off-shore winds-moving away from the shore) drive warm surface water away from the coast resulting in the upwelling of cold water from below (This happens near Peruvian Coast in normal years. El-Nino).
  • Contrary to this, the onshore winds (winds flowing from oceans into continents) pile up warm water near the coast and this raises the temperature (This happens near the Peruvian coast during El Nino event)(In normal years, North-eastern Australia and Western Indonesian islands see this kind of warm ocean waters due to Walker Cell or Walker Circulation).
  • Ocean currents: Warm ocean currents raise the temperature in cold areas while the cold currents decrease the temperature in warm ocean areas. Gulf stream (warm current) raises the temperature near the eastern coast of North America and the West Coast of Europe while the Labrador current (cold current) lowers the temperature near the north-east coast of North America (Near Newfoundland). All these factors influence the temperature of the ocean currents locally.

Vertical Temperature Distribution of Oceans

  • Photic or euphotic zone extends from the upper surface to ~200 m. The photic zone receives adequate solar insolation.
  • Aphotic zone extends from 200 m to the ocean bottom; this zone does not receive adequate sunrays.

Thermocline

  • The profile shows a boundary region between the surface waters of the ocean and the deeper layers.
  • The boundary usually begins around 100 – 400 m below the sea surface and extends several hundred of meters downward.
  • This boundary region, from where there is a rapid decrease of temperature, is called the thermocline. About 90 per cent of the total volume of water is found below the thermocline in the deep ocean. In this zone, temperatures approach 0° C.

thermocline - Temperature Distribution of Oceans

Three-Layer System

  • The temperature structure of oceans over middle and low latitudes can be described as a three-layer system from surface to the bottom.
  • The first layer represents the top layer of warm oceanic water and it is about 500m thick with temperatures ranging between 20° and 25° C. This layer, within the tropical region, is present throughout the year but in mid-latitudes it develops only during summer.
  • The second layer called the thermocline layer lies below the first layer and is characterized by rapid decrease in temperature with increasing depth. The thermocline is 500 -1,000 m thick.
  • The third layer is very cold and extends up to the deep ocean floor. Here the temperature becomes almost stagnant.

Temperature Distribution of Oceans

General behavior

  • In the Arctic and Antarctic circles, the surface water temperatures are close to 0° C and so the temperature change with the depth is very slight (ice is a very bad conductor of heat). Here, only one layer of cold water exists, which extends from surface to deep ocean floor.

The rate of decrease of temperature with depths is greater at the equator than at the poles.

  • The surface temperature and its downward decrease is influenced by the upwelling of bottom water (Near Peruvian coast during normal years).
  • In cold Arctic and Antarctic regions, sinking of cold water and its movement towards lower latitudes is observed.
  • In equatorial regions the surface, water sometimes exhibits lower temperature and salinity due to high rainfall, whereas the layers below it have higher temperatures.
  • The enclosed seas in both the lower and higher latitudes record higher temperatures at the bottom.
  • The enclosed seas of low latitudes like the Sargasso Sea, the Red Sea and the Mediterranean Sea have high bottom temperatures due to high insolation throughout the year and lesser mixing of the warm and cold’ waters.
  • In the case of the high latitude enclosed seas, the bottom layers of water are warmer as water of slightly higher salinity and temperature moves from outer ocean as a sub-surface current.
  • The presence of submarine barriers may lead to different temperature conditions on the two sides of the barrier. For example, at the Strait of Bab-el-Mandeb, the submarine barrier (sill) has a height of about 366 m. The subsurface water in the strait is at high temperature compared to water at same level in Indian ocean. The temperature difference is greater than nearly 20° C.

Horizontal Temperature Distribution of Oceans

  • The average temperature of surface water of the oceans is about 27°C and it gradually decreases from the equator towards the poles.
  • The rate of decrease of temperature with increasing latitude is generally 0.5°C per latitude.
  • The horizontal temperature distribution is shown by isothermal lines, i.e., lines joining places of equal temperature.
  • Isotherms are closely spaced when the temperature difference is high and vice versa.
  • For example, in February, isothermal lines are closely spaced in the south of Newfoundland, near the west coast of Europe and North Sea and then isotherms widen out to make; a bulge towards north near the coast of Norway. The cause of this phenomenon lies in the cold Labrador Current flowing southward along the north American coast which reduces the temperature of the region more sharply than in other places in the same latitude; at the same time the warm Gulf Stream proceeds towards the western coast of Europe and raises the temperature of the west coast of Europe.

Seasonal Temperature Distribution – January

Range of Ocean Temperature

  • The oceans and seas get heated and cooled slower than the land surfaces. Therefore, even if the solar insolation is maximum at noon, the ocean surface temperature is highest at 2 p.m.
  • The average diurnal or daily range of temperature is barely 1 degree in oceans and seas.
  • The highest temperature in surface water is attained at 2 p.m. and the lowest, at 5 a.m.
  • The diurnal range of temperature is highest in oceans if the sky is free of clouds and the atmosphere is calm.
  • The annual range of temperature is influenced by the annual variation of insolation, the nature of ocean currents and the prevailing winds.
  • The maximum and the minimum temperatures in oceans are slightly delayed than those of land areas (the maximum being in August and the minimum in February [Think why intense tropical cyclones occur mostly between August and October – case is slightly different in Indian Ocean due to its shape]).
  • The northern Pacific and northern Atlantic oceans have a greater range of temperature than their southern parts due to a difference in the force of prevailing winds from the land and more extensive ocean currents in the southern parts of oceans.
  • Besides annual and diurnal ranges of temperature, there are periodic fluctuations of sea temperature also. For example, the 11-year sunspot cycle causes sea temperatures to rise after a 11- year gap.

Sunspot

  • Sunspots are temporary phenomena on the photosphere of the Sun that appear visibly as dark spots compared to surrounding regions.
  • They correspond to concentrations of magnetic field that inhibit convection and result in reduced surface temperature compared to the surrounding photosphere.
  • Sunspots usually appear as pairs, with each spot having the opposite magnetic polarity of the other.
  • Although they are at temperatures of roughly 3,000–4,500 K (2,700–4,200 °C), the contrast with the surrounding material at about 5,780 K (5,500 °C) leaves them clearly visible as dark spots.
  • Sunspot activity cycles about every eleven years. The point of highest sunspot activity during this cycle is known as Solar Maximum, and the point of lowest activity is Solar Minimum.

Primary References: NCERT Geography,  Spectrum’s Geography [Amazon and Flipkart] and Savindra Singh [Amazon and Flipkart]

Sharing is Caring !!

Newsletter Updates

Subscribe to our newsletter and never miss an important update!

Assured Discounts on our New Products!

4 Comments

  1. The ocean water is heated by three processes :

    2. The conventional currents: Since the temperature of the earth increases with increasing depth, the ocean water at great depths is heated faster than the upper water layers. So, convectional oceanic circulations develop causing circulation of heat in water.

    ^Can someone please elaborate the above statement? Does that mean the ocean water at depth is hotter (which is not true)?

    Thanks!

    • Hi !

      By conventional current they mean that The HEAT received by TOP LAYER is distributed to below layer by Conventional currents and capacity of water at depths is more to absorb the heat from TOP LAYER. So the statement is not saying that depth waters are more hotter , it only emphasis on the way how temperature is received at depth that is Conventional currents.

    • The average temperature of oceans at depth is
      2 degree. Which means its heated not cooled up

Leave a Reply

Your email address will not be published. Required fields are marked *

Newsletter

Never miss an important update!