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Non-Rationalised Geography NCERT Notes, Solutions and Extra Q & A (Class 6th to 12th)
6th 7th 8th 9th 10th 11th 12th

Class 11th Chapters
Fundamentals of Physical Geography
1. Geography As A Discipline 2. The Origin And Evolution Of The Earth 3. Interior Of The Earth
4. Distribution Of Oceans And Continents 5. Minerals And Rocks 6. Geomorphic Processes
7. Landforms And Their Evolution 8. Composition And Structure Of Atmosphere 9. Solar Radiation, Heat Balance And Temperature
10. Atmospheric Circulation And Weather Systems 11. Water In The Atmosphere 12. World Climate And Climate Change
13. Water (Oceans) 14. Movements Of Ocean Water 15. Life On The Earth
16. Biodiversity And Conservation
India Physical Environment
1. India — Location 2. Structure And Physiography 3. Drainage System
4. Climate 5. Natural Vegetation 6. Soils
7. Natural Hazards And Disasters
Practical Work in Geography
1. Introduction To Maps 2. Map Scale 3. Latitude, Longitude And Time
4. Map Projections 5. Topographical Maps 6. Introduction To Aerial Photographs
7. Introduction To Remote Sensing 8. Weather Instruments, Maps And Charts



Chapter 14 Movements Of Ocean Water



Ocean water is constantly in motion. The dynamic nature of ocean water is influenced by its physical characteristics, such as temperature, salinity, and density, as well as external forces exerted by the sun, moon, and winds.

Ocean water exhibits both horizontal and vertical movements:


Waves

Ocean waves are essentially the movement of energy across the surface of the water, not the mass movement of water itself over large distances. As a wave passes, water particles move in circular orbits, returning close to their original position (Figure 14.1).

Diagram illustrating the motion of waves and the circular movement of water molecules

Diagram showing how waves propagate energy horizontally while water particles move in circular orbits beneath the surface, with the orbit size decreasing with depth.

The primary source of energy for most ocean waves is the wind. Wind blowing over the water surface transfers energy to the water, generating waves. This energy is carried across the ocean and ultimately released onto coastlines as waves break.

The motion of waves is mainly confined to the surface layers and typically does not significantly affect the calm water found in the deep ocean below. As a wave approaches shallow water near the shore, it slows down due to friction with the seabed. When the water depth becomes less than half the wave's wavelength, the wave becomes unstable and breaks, forming surf.

Waves start as small ripples on calm water when a light breeze blows. As wind speed increases and blows over a greater distance and for a longer duration, these ripples grow into larger waves. Larger waves accumulate more energy from the wind and can travel thousands of kilometers across the open ocean before breaking on shore.

The size and shape of a wave can give clues about its origin. Steep waves are generally younger and created by local winds, whereas smoother, more regular waves (swells) have traveled long distances from their generation area. The maximum height a wave can reach is determined by the wind's strength, how long it blows (duration), and the distance over which it blows in a consistent direction (fetch).

Waves travel because wind pushes the water, and gravity acts on the water to pull the crests down. The falling water pushes the water in the preceding trough upwards, allowing the wave form to propagate forward.


Characteristics Of Waves

Waves are described using several standard characteristics:




Tides

Tides are the periodic, rhythmic rise and fall of the sea level. This phenomenon occurs once or twice daily and is primarily caused by the gravitational attraction of the moon and, to a lesser extent, the sun on the Earth's ocean waters. Wind and atmospheric pressure changes can also cause short-term sea level changes called surges, but these are not regular tidal movements.

The study of tides is complex due to variations in their frequency, height, and timing depending on location and time. The key forces driving tides are the gravitational pull of the moon and sun and the centrifugal force generated by the Earth-moon system's rotation around a common center of mass.

These forces create two major tidal bulges on the Earth. One bulge forms on the side of the Earth directly facing the moon, where the moon's gravitational pull is strongest. A second bulge forms on the opposite side of the Earth. Although the moon's gravitational pull is weakest here, the centrifugal force (an outward-acting inertial force) is dominant, pulling water away from the Earth's center and creating a bulge (Figure 14.2).

Diagram illustrating the gravitational and centrifugal forces causing tidal bulges

Diagram showing how the gravitational attraction of the Moon and the centrifugal force of the Earth-Moon system combine to create two tidal bulges on opposite sides of the Earth.

The "tide-generating force" at any point on Earth is the difference between the gravitational attraction of a celestial body (moon or sun) and the average centrifugal force acting on the Earth as a whole. On the side closest to the moon, gravity dominates, causing a bulge. On the opposite side, the weaker gravity is overcome by the stronger centrifugal force, also causing a bulge. Water flows horizontally across the Earth's surface towards these bulges.

The magnitude of tides can be influenced by local factors such as the shape of the coastline and the seafloor. Wide continental shelves can amplify tidal bulges, while mid-oceanic islands have smaller tides. Funnel-shaped bays or estuaries can significantly increase tidal ranges. When tidal flow is channeled through narrow passages or into bays, these are called tidal currents.

The Bay of Fundy in Canada is famous for having the highest tides in the world, reaching 15-16 meters due to its specific shape and the resonance of tidal movements.


Types Of Tides

Tides are classified based on their frequency of occurrence per day or their height variations.


Tides Based On Frequency


Tides Based On The Sun, Moon And The Earth Positions

The relative positions of the Sun, Moon, and Earth significantly influence the height of the tides because the Sun's gravity also contributes to the tide-generating force. Tides based on these alignments are:

Other astronomical factors also slightly affect tidal range:

The period when the tide is falling (from high to low tide) is called the ebb tide or ebb. The period when the tide is rising (from low to high tide) is called the flow tide or flood tide.


Importance Of Tides

Tides are predictable phenomena because the positions of the Earth, Moon, and Sun are known in advance. This predictability makes tides important for various human activities:




Ocean Currents

Ocean currents are continuous, directed movements of seawater within ocean basins. They are like vast rivers flowing through the ocean, carrying massive amounts of water over long distances in defined paths and directions. Ocean currents are influenced by a combination of primary forces that initiate water movement and secondary forces that modify their flow.

Primary forces that initiate ocean currents:

Secondary forces that influence current flow include friction (resistance from surrounding water and the seabed), and the shape of coastlines and ocean floor topography which can deflect or channel currents. Differences in water density, caused by variations in temperature and salinity, drive deep-water currents. Cold water is denser than warm water, and saltier water is denser than less salty water. Denser water tends to sink, while lighter water rises, creating vertical water movements and driving deep ocean circulation (thermohaline circulation).


Types Of Ocean Currents

Ocean currents can be classified based on their depth or temperature:

Based on Depth:

Based on Temperature:

The speed or strength of a current is referred to as its "drift", measured in knots. Currents are generally strongest near the surface and their speed decreases with depth. Fast currents are considered strong; most currents have speeds less than or equal to 5 knots ($< 9.3 \, km/h$).


Major Ocean Currents

The large-scale patterns of major ocean currents (Figure 14.3) are strongly influenced by prevailing winds and the Coriolis force. The overall ocean circulation pattern broadly mimics the pattern of atmospheric circulation (the major wind belts). In the middle latitudes, the large circular currents (gyres) often follow the anticyclonic (clockwise in NH, anticlockwise in SH) circulation patterns of the subtropical atmospheric highs, while in higher latitudes, they may follow the cyclonic patterns associated with subpolar lows. In monsoon regions, seasonal wind reversals can cause seasonal reversals in ocean currents.

World map showing major warm and cold ocean currents

Map illustrating the general pattern and names of major warm (red arrows) and cold (blue arrows) ocean currents in the Pacific, Atlantic, and Indian Oceans.

Due to the Coriolis force, warm currents originating from low latitudes tend to be deflected to the right in the Northern Hemisphere and to the left in the Southern Hemisphere. Conversely, cold currents originating from high latitudes are also deflected, contributing to the gyre circulation.

Major ocean currents play a vital role in transporting heat globally, moving energy from the energy-surplus regions in the tropics towards the energy-deficit polar regions, complementing the heat transport by atmospheric circulation. Cold waters from the Arctic and Antarctic move towards the tropics, and warm waters from the tropics move polewards.

Examples of currents influenced by prevailing winds (Figure 14.3):


Effects Of Ocean Currents

Ocean currents have significant impacts on coastal climates, marine ecosystems, and human activities:




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