Chapter 8 Lecture Waves and WaterDynamics

Essential of Oceanography

Table of Contents

All waves begin as disturbances, and ocean waves form as the result of a disturbing force.

Wave Generation

  • Disturbing force causes waves to form.
  • Wind blowing across ocean surface
  • Interface of fluids with different densities
  • Air – ocean interface
    – Ocean waves
  • Air – air interface
    – Atmospheric waves
  • Water – water interface
    – Internal waves

Types of Waves

Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Internal Waves

  • Associated with pycnocline
  • Larger than surface waves
  • Caused by tides, turbidity currents, winds, ships
Internal Waves
Internal Waves

Wave Movement

All types of waves transmit energy—or propagate—by means of cyclic movement through matter. The medium itself (solid, liquid, or gas) does not actually travel in the direction of the wave that is passing through it. The particles in the medium simply oscillate—or cycle—back and forth, and up and down, transferring energy from one particle to another.

  • Waves transmit energy
  • Cyclic motion of particles in ocean
    – Particles may move
  • Up and down
  • Back and forth
  • Around and around
READ ALSO  What Are the Characteristics of Biogenous Sediment?

Different types of waves move in a variety of ways. Simple progressive waves are waves that oscillate uniformly and progress or travel without breaking. Progressive waves are divided into longitudinal, transverse, or a combination of the two motions, called orbital.

Global distribution of energy in ocean waves.
Graph showing the average annual energy, types, and principal
causes of waves in the world ocean.
Global distribution of energy in ocean waves. Graph showing the average annual energy, types, and principal causes of waves in the world ocean.

Progressive Waves

  • Progressive waves oscillate uniformly and progress without breaking
    – Longitudinal
    – Transverse
    – Orbital
Types of progressive
waves. Diagrammatic view of the
three types of progressive waves.
Examples include 1 longitudinal
waves, 2 transverse waves, and
3 orbital waves.
Types of progressive waves. Diagrammatic view of the three types of progressive waves. Examples include 1 longitudinal
waves, 2 transverse waves, and 3 orbital waves.

Longitudinal Waves

In longitudinal waves (also known as push–pull waves), the particles that vibrate “push and pull” in the same direction that the wave is traveling, like a spring whose coils are alternately compressed and expanded. The shape of the wave (called a waveform) moves through the medium by compressing and decompressing as it goes. Sound, for instance, travels as longitudinal waves

  • Also called push-pull waves
  • Compress and decompress as they travel, like a coiled spring

Transverse Waves

In transverse waves (also known as side-to-side waves), energy travels at right angles to the direction of the vibrating particles. If one end of a rope is tied to a doorknob while the other end is moved up and down (or side to side) by hand, for example, a waveform progresses along the rope and energy is transmitted from the motion of the hand to the doorknob. The waveform moves up and down (or side to side) with the hand, but the motion is at right angles to the direction in which energy is transmitted (from the hand to the doorknob). Generally, transverse waves transmit energy only through solids, because the particles in solids are bound to one another strongly enough to transmit this kind of motion

  • Also called side-to-side waves
  • Energy travels at right angles to direction of moving particles.
  • Generally only transmit through solids, not liquids
READ ALSO  What Features Exist in the Deep-Ocean Basins?

Orbital Waves

Longitudinal and transverse waves are called body waves because they transfer energy through a body of matter. Ocean waves are considered surface waves because they travel along the interface between two different fluids (air and water). The
movement of particles in ocean waves involves components of both longitudinal and transverse waves, so particles move in circular orbits. Thus, waves at the ocean surface are orbital waves (also called interface waves).

  • Also called interface waves
  • Waves on ocean surface

Wave Terminology

As an idealized wave passes a permanent marker (such as a pier piling), a succession of high parts of the waves, called crests, alternate with low parts, called troughs. Halfway between the crests and the troughs is the still water level, or zero energy level. This is the level of the water if there were no waves. The wave height, designated by the symbol H, is the vertical distance between a crest and a trough. The horizontal distance between any two corresponding points on successive waveforms, such as from crest to crest or from trough to trough, is the wavelength, L.

Wave Steepness

Wave steepness is the ratio of wave height to wavelength:


Wave steepness = Wave height (H) / Wave length (L)

If the wave steepness exceeds 1/7, the wave breaks (spills forward) because the wave is too steep to support itself. A wave can break anytime the 1:7 ratio is exceeded, either along the shoreline or out at sea. This ratio also dictates the maximum height of a wave. For example, a wave 7 meters long can only be 1 meter high; if the wave is any higher than that, it will break.

READ ALSO  How does latitude affect solar radiation?

Wave Period and Frequency

The time it takes one full wave—one wavelength—to pass a fixed position (such as a pier piling) is the wave period, T. Typical wave periods range between 6 and 16 seconds. The frequency (f) is defined as the number of wave crests passing a fixed location per unit of time and is the inverse of the period:


Frequency (f) = 1 / Period (T)
  • Crest
  • Trough
  • Still water level
    – Zero energy level
  • Wave height (H)

Orbital Wave Characteristics

  • Wave steepness = H/L
    – If wave steepness > 1/7, wave breaks
  • Wave period (T) = time for one wavelength to pass fixed point
  • Wave frequency = inverse of period or 1/T
  • Diameter of orbital motion decreases with depth of water.
  • Wave base = ½ L
  • Hardly any motion below wave base due to wave activity
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Circular Orbital Motion

The water itself doesn’t travel the entire distance, but the waveform does. As the wave travels, the water passes the energy along by moving in a circle. This movement is called circular orbital motion.

  • Wave particles move in a circle.
  • Waveform travels forward.
  • Wave energy advances.
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Deep Water Waves

If the water depth (d) is greater than the wave base (L/2), the waves are called deep-water waves

  • Wave base – depth where orbital movement of water particles stops
  • If water depth is greater than wave base (>½L), wave isa deep water wave.
  • Lack of orbital motion at depth useful for floating runways and other structures
Floating airport runway in waters off
Japan.
Floating airport runway in waters off Japan.
  • All wind-generated waves in open ocean
  • Wave speed = wavelength (L)/period (T)
  • Speed called celerity (C)
Deep-water wave: Circular orbits diminish in size with increasing depth. Water depth is greater than 1/2 wavelength.
Deep-water wave: Circular orbits diminish in size with increasing depth. Water depth is greater than 1/2 wavelength.

Speed of Deep Water Waves

Determining the speed of deep-water
waves. Graph showing the relationships between wavelength
(horizontal axis), period (blue curve), and wave speed (vertical axis)
for deep-water waves.
Determining the speed of deep-water waves. Graph showing the relationships between wavelength (horizontal axis), period (blue curve), and wave speed (vertical axis) for deep-water waves.

Shallow-Water Waves

Waves in which depth (d) is less than 1/20 of the wavelength (L/20) are called shallow-water waves, or long waves . Shallow-water waves are said to touch bottom or feel bottom because they touch the ocean floor, which interferes with the wave’s orbital motion.

  • Water depth (d) is less than 1/20 L
    – Water “feels” seafloor
  • C (meters/sec) = 3.13 √ d(meters) or
  • C (feet/sec) = 5.67 √d (feet)

Transitional Waves

  • Characteristics of both deep- and shallow-water waves
  • Celerity depends on both water depth and wavelength
) Transitional wave: Intermediate between deep-water and shallow-water
waves. Water depth is greater than 1/20 wavelength, but less than 1/2
wavelength.
) Transitional wave: Intermediate between deep-water and shallow-water waves. Water depth is greater than 1/20 wavelength, but less than 1/2 wavelength.

Wind-Generated Wave Development

The “lifecycle” of a wind-generated wave includes its origin in a windy region of the ocean, its movement across great expanses of open water without subsequent aid of wind, and its termination when it breaks and releases its energy, either in the open
ocean or against the shore.

  • Capillary waves : As the wind blows over the ocean surface, it pushes down on and parallel to the surface, causing water to pile up into small wavelets called capillary waves, which are more commonly called ripples.
  • Wind generates stress on sea surface
  • Gravity waves As capillary wave development increases, the sea surface takes on a rougher appearance. The water “catches” more of the wind, allowing the wind and ocean surface to interact more efficiently. As more energy is transferred to the ocean, gravity waves develop
    – Increasing wave energy
  • Capillary Waves
    – Ripples
    – Wind generates initial stress on sea surface
  • Gravity Waves
    – More energy transferred to ocean
    – Trochoidal waveform as crests become pointed
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Sea

The area where wind-driven waves are generated is called the sea, or sea area.

  • Sea
    – Where wind-driven waves are generated
    – Also called sea area

Factors Affecting Wave Energy

  • Wind speed
  • Wind duration
  • Fetch – distance over which wind blows
Factors that contribute to creating large waves
in the “sea” and the origination of swell.
Factors that contribute to creating large waves in the “sea” and the origination of swell.

Wave Height

  • Directly related to wave energy
  • Wave heights usually less than 2 meters (6.6 feet)
  • Breakers called whitecaps form when wave reaches critical steepness.
  • Beaufort Wind Scale describes appearance of sea surface.

Global Wave Heights

Global Wave Heights
Global Wave Heights

Beaufort Wind Scale

Beaufort wind scale and the state of the sea
Beaufort numberDescriptive termWind speed  Appearance of the sea
km/hrmi/hr
0Calm<1<1Like a mirror
1Light air1–51–3Ripples with the appearance of scales, no foam crests
2Light breeze6–114–7Small wavelets; crests of glassy appearance, no breaking
3Gentle breeze12–198–12Large wavelets; crests begin to break, scattered whitecaps
4Moderate breeze20–2813–18Small waves, becoming longer; numerous whitecaps
5Fresh breeze29–3819–24Moderate waves, taking longer form; many whitecaps, some spray
6Strong breeze39–4925–31Large waves begin to form, whitecaps everywhere, more spray
7Near gale50–6132–38Sea heaps up and white foam from breaking waves begins to be blown in streaks
8Gale62–7439–46Moderately high waves of greater length, edges of crests begin to break into spindrift, foam is blown in well-marked streaks
9Strong gale75–8847–54High waves, dense streaks of foam and sea begins to roll, spray may affect visibility
10Storm89–10255–63Very high waves with overhanging crests; foam is blown in dense white streaks, causing the sea to appear white; the rolling of the sea becomes heavy; visibility reduced
11Violent storm103–11764–72Exceptionally high waves (small and medium-sized ships might for a time be lost from view behind the waves), the sea is covered with white patches of foam, everywhere the edges of the wave crests are blown into froth, visibility further reduced
12Hurricane118+73+The air is filled with foam and spray, sea completely white with driving spray, visibility greatly reduced

Maximum Wave Height

  • USS Ramapo (1933): 152-meters (500 feet) long ship caught in Pacific typhoon
  • Waves 34 meters (112 feet) high
  • Previously thought waves could not exceed 60 feet
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Wave Damage

  • USS Ramapo undamaged
  • Other craft not as lucky
  • Ships damaged or disappear annually due to high storm waves
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Wave Energy

  • Fully developed sea
    – Equilibrium condition
    – Waves can grow no further
  • Swell
    – Uniform, symmetrical waves that travel outward from storm area
    – Long crests
    – Transport energy long distances

Fully Developed Sea

CONDITIONS NECESSARY TO PRODUCE A FULLY DEVELOPED SEA AT VARIOUS WIND SPEEDS AND THE CHARACTERISTICS OF THE RESULTING WAVES
These conditions . . .. . . produce these waves
Wind speed in km/hr (mi/hr)Fetch in km (mi)Duration in hoursAverage height in m (ft)Average wave- length in m (ft)Average period in secondsHighest 10% of waves in m (ft)
20 (12)24 (15)2.80.3 (1.0)10.6 (34.8)3.20.8 (2.5)
30 (19)77 (48)7.00.9 (2.9)22.2 (72.8)4.62.1 (6.9)
40 (25)176 (109)11.51.8 (5.9)39.7 (130.2)6.23.9 (12.8)
50 (31)380 (236)18.53.2 (10.5)61.8 (202.7)7.76.8 (22.3)
60 (37)660 (409)27.55.1 (16.7)89.2 (292.6)9.110.5 (34.4)
70 (43)1093 (678)37.57.4 (24.3)121.4 (398.2)10.815.3 (50.2)
80 (50)1682 (1043)50.010.3 (33.8)158.6 (520.2)12.421.4 (70.2)
90 (56)2446 (1517)65.213.9 (45.6)201.6 (661.2)13.928.4 (93.2)

Swells

As waves generated in a sea area move toward its margins, wind speeds diminish and the waves eventually move faster than the wind. When this occurs, wave steepness decreases and waves become long-crested waves called swells (swellan = swollen), which are uniform, symmetrical waves that have traveled out of their area of origination.

  • Longer wavelength waves travel faster and outdistance other waves.
    – Wave train – a group of waves with similar characteristics
    – Wave dispersion – sorting of waves by wavelengths
    – Decay distance – distance over which waves change from choppy sea to uniform swell
  • Wave train speed is ½ speed of individual wave.

Wave Train Movement

Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Wave Interference Patterns

When swells from different storms run together, the waves clash, or interfere with one another, giving rise to interference patterns. An interference pattern produced when two or more wave systems collide is the sum of the disturbance that each wave would have produced individually.

  • Collision of two or more wave systems
  • Constructive interference
    – In-phase wave trains with about the same wavelengths
  • Destructive interference
    – Out-of-phase wave trains with about the same wavelengths
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
  • Mixed interference
    – Two swells with different wavelengths and different wave heights
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Rogue Waves

  • Massive, spontaneous, solitary ocean waves
  • Reach abnormal heights, enormous destructive power
  • Luxury liner Michelangelo damaged in 1966
  • Basis of The Perfect Storm
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics
  • Difficult to forecast
  • Occur more near weather fronts and downwind of islands
  • Strong ocean currents amplify opposing swells
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Waves in Surf Zone

  • Surf zone – zone of breaking waves near shore
  • Shoaling water – water becoming gradually more shallow
  • When deep water waves encounter shoaling water less than ½ their wavelength, they become transitional waves.

Waves Approaching Shore

  • As a deep-water wave becomes a shallowwater wave:
    – Wave speed decreases
    – Wavelength decreases
    – Wave height increases
    – Wave steepness (height/wavelength) increases
    – When steepness > 1/7, wave breaks
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Breakers in Surf Zone

  • Surf as swell from distant storms
    – Waves break close to shore
    – Uniform breakers
  • Surf generated by local winds
    – Choppy, high energy, unstable water
  • Shallow water waves

Three Types of Breakers

  • Spilling
  • Plunging
  • Surging

Spilling Breakers

  • Gently sloping sea floor
  • Wave energy expended over longer distance
  • Water slides down front slope of wave
Spilling breaker, resulting from a gradual beach slope
Spilling breaker, resulting from a gradual beach slope

Plunging Breakers

  • Moderately steep sea floor
  • Wave energy expended over shorter distance
  • Best for board surfers
  • Curling wave crest
 Plunging breaker, resulting from a steep beach slope; these  are the best waves for surfing.
Plunging breaker, resulting from a steep beach slope; these are the best waves for surfing.

Surging Breakers

  • Steepest sea floor
  • Energy spread over shortest distance
  • Best for body surfing
  • Waves break on the shore
 Surging breaker, resulting from an abrupt beach slope
Surging breaker, resulting from an abrupt beach slope

Surfing

  • Like riding a gravity-operated water sled
  • Balance of gravity and buoyancy
  • Skilled surfers position board on wave front
    – Can achieve speeds up to 40 km/hour (25 miles/hour)

Wave Refraction

  • Waves rarely approach shore at a perfect 90-degree angle.
  • As waves approach shore, they bend so wave crests are nearly parallel to shore.
  • Wave speed is proportional to the depth of water (shallow-water wave).
  • Different segments of the wave crest travel at different speeds.
Wave Refraction
Wave Refraction
  • Wave energy unevenly distributed on shore
  • Orthogonal lines or wave rays – drawn perpendicular to wave crests
    – More energy released on headlands
    – Energy more dissipated in bays
Perspective view of wave refraction along an irregular shoreline
Perspective view of wave refraction along an irregular shoreline
  • Gradually erodes headlands
  • Sediment accumulates in bays
Photo of wave refraction at Rincon Point, California (looking west).
Photo of wave refraction at Rincon Point, California (looking west).

Wave Reflection

  • Waves and wave energy bounced back from barrier
  • Reflected wave can interfere with next incoming wave.
  • With constructive interference, can create dangerous plunging breakers
 Wave reflection and constructive interference
at The Wedge, Newport Harbor, California
Wave reflection and constructive interference at The Wedge, Newport Harbor, California

Standing Waves

  • Two waves with same wavelength moving in opposite directions
  • Water particles move vertically and horizontally.
  • Water sloshes back and forth.
  • Nodes have no vertical movement
  • Antinodes are alternating crests and troughs.
Sequence of motion in a standing wave. I
Sequence of motion in a standing wave.

Tsunami

  • Seismic sea waves
  • Originate from sudden sea floor topography changes
    – Earthquakes – most common cause
    – Underwater landslides
    – Underwater volcano collapse
    – Underwater volcanic eruption
    – Meteorite impact – splash waves

Tsunami Characteristics

  • Long wavelengths (> 200 km or 125 miles)
    • Behaves as a shallow-water wave
      – Encompasses entire water column, regardless of ocean depth
      – Can pass undetected under boats in open ocean
  • Speed proportional to water depth
    – Very fast in open ocean
 How a tsunami is generated, propagated, and surges to extreme heights at the shore.
How a tsunami is generated, propagated, and surges to extreme heights at the shore.

Tsunami Destruction

  • Sea level can rise up to 40 meters (131 feet) when a tsunami reaches shore.

Tsunami

  • Most occur in Pacific Ocean
    – More earthquakes and volcanic eruptions
  • Damaging to coastal areas
  • Loss of human lives
Tsunami damage in Hilo, Hawaii.
Flattened parking meters in Hilo, Hawaii, caused by the 1946 tsunami
that resulted in more than $25 million in damage and 159 deaths.
Tsunami damage in Hilo, Hawaii. Flattened parking meters in Hilo, Hawaii, caused by the 1946 tsunami that resulted in more than $25 million in damage and 159 deaths.

Historical Tsunami

  • Krakatau – 1883
    – Indonesian volcanic eruption
  • Scotch Cap, Alaska/Hilo, Hawaii – 1946
    – Magnitude 7.3 earthquake in Aleutian Trench
  • Papua New Guinea – 1998
    – Pacific Ring of Fire magnitude 7.1 earthquake

Historical Large Tsunami

Global locations and corresponding table showing significant
tsunami (those with large tsunami height and/or responsible for
a large number of fatalities) since 1990. Tsunami have claimed
more than 300,000 lives worldwide since 1990. These killer waves
are most often generated by earthquakes along colliding tectonic
plates of the Pacific Rim, although the most deadly tsunami in
history was the 2004 Indian Ocean Tsunami (number 8). Locations
of ocean trenches are shown by dark red lines; Pacific Ring of Fire
is shown by red shading.
Significant tsunami since 1990.
Global locations and corresponding table showing significant tsunami (those with large tsunami height and/or responsible for
a large number of fatalities) since 1990. Tsunami have claimed more than 300,000 lives worldwide since 1990. These killer waves are most often generated by earthquakes along colliding tectonic plates of the Pacific Rim, although the most deadly tsunami in history was the 2004 Indian Ocean Tsunami (number 8). Locations of ocean trenches are shown by dark red lines; Pacific Ring of Fire is shown by red shading.

Indian Ocean Tsunami

  • December 26, 2004
    – Magnitude 9.2 earthquake off coast of Sumatra
    – 1200 km seafloor displaced between two tectonic plates
    – Deadliest tsunami in history
    – Coastal villages completely wiped out
  • Detected by Jason-1 satellite
  • Traveled more than 5000 km (3000 mi)
  • Wavelength about 500 km (300 mi)
  • 230,000–300,000 people in 11 countries killed
  • Lack of warning system in Indian Ocean
Jason-1 satellite detects the Indian Ocean Tsunami.
The Indian Ocean Tsunami was initiated by a large earthquake offshore
Sumatra on December 26, 2004 (red star). By a fortuitous circumstance, the
Jason-1 satellite passed over the Indian Ocean (black line) two hours after the
tsunami was generated. Its radar altimeter detected the crests and troughs of
the tsunami (colors), which showed a wave height of about 1 meter (3.3 feet)
in the open ocean. The graph of the satellite’s overpass (below) shows the
difference between the measured sea level from satellite data (black line) and
the modeled wave height (blue curve).
Jason-1 satellite detects the Indian Ocean Tsunami.
The Indian Ocean Tsunami was initiated by a large earthquake offshore Sumatra on December 26, 2004 (red star). By a fortuitous circumstance, the Jason-1 satellite passed over the Indian Ocean (black line) two hours after the tsunami was generated. Its radar altimeter detected the crests and troughs of the tsunami (colors), which showed a wave height of about 1 meter (3.3 feet) in the open ocean. The graph of the satellite’s overpass (below) shows the difference between the measured sea level from satellite data (black line) and the modeled wave height (blue curve).

Japan Tsunami

  • March 11, 2011 – Tohoku Earthquake
    – Magnitude 9.0 earthquake in Japan Trench
    – Felt throughout Pacific basin
    – Most expensive tsunami in history
  • Initial surge 15 meters (49 ft)
    – Topped harbor-protecting tsunami walls
    – Amplified by local topography
  • Killed 19,508 people
  • Disrupted power at Fukushima Daiichi nuclear power plant
    – Reactors exploded
    – Radioactivity problem initiated

Tsunami Warning System

  • Pacific Tsunami Warning Center (PTWC) – Honolulu, HI – Uses seismic wave recordings to forecast tsunami
  • Deep Ocean Assessment and Reporting of Tsunami (DART)
    – System of buoys
    – Detects pulse of tsunami passing
Deep-ocean Assessment and Reporting of
Tsunamis (DART). The DART system consists of a deep-ocean
pressure sensor that can detect a tsunami passing above. The
pressure sensor relays information to a buoy at the surface that
transmits the data via satellite, allowing oceanographers to detect
the passage of a tsunami in the open ocean.
Deep-ocean Assessment and Reporting of Tsunamis (DART).
The DART system consists of a deep-ocean pressure sensor that can detect a tsunami passing above. The pressure sensor relays information to a buoy at the surface that transmits the data via satellite, allowing oceanographers to detect the passage of a tsunami in the open ocean.

Tsunami Watches and Warnings

  • Tsunami Watch
    • issued when potential for tsunami exists
  • Tsunami Warning
    • unusual wave activity verified
      – Evacuate people
      – Move ships from harbors
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Waves as Source of Energy

  • Lots of energy associated with waves
  • Mostly with large storm waves
    – How to protect power plants
    – How to produce power consistently
  • Environmental issues
    – Building power plants close to shore
    – Interfering with life and sediment movement

Wave Power Plant

  • First commercial wave power plant began operating in 2000.
  • LIMPET 500 – Land Installed Marine Powered Energy Transformer
    – Coast of Scotland
    – 500 kilowatts of power under peak operating capacity
How a wave power
plant works.
How a wave power plant works.

Wave Farms

  • Portugal – 2008
    – Ocean Power Delivery
    – First wave farm
  • About 50 wave power development projects globally
Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Global Wave Energy Resources

Chapter 8 Lecture Waves and WaterDynamics
Chapter 8 Lecture Waves and WaterDynamics

Reference: All images and content are taken from Essentials of Oceanography by Alan P. Trujillo and Harold V. Thurman, 12th Edition.

Leave a Reply

CSIR NET Exam: EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES

Exam Pattern: EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES 

 PART APART BPART CTOTAL
Total questions205080150
Max No. of Questions to attempt15352575
Marks for each correct answer224200
Marks for each incorrect answer (Negative marking for part A & B is @ 25%, and part C is @ 33%)0.50.51.32

The candidate is required to answer a maximum of 15, 35, and 25 questions from Part-A, Part-B, and Part-C, respectively. If more than the required number of questions are answered, only the first 15, 35, and 25 questions in Part A, Part B, and Part C, respectively, will be taken up for evaluation.

Below each question in Part A, Part B, and Part C, four alternatives or responses are given. Only one of these alternatives is the “correct” option to the question. The candidate has to find, for each question, the correct or the best answer.

Syllabus

EARTH, ATMOSPHERIC, OCEAN AND PLANETARY SCIENCES

PAPER I (PART B)

  1. The Earth and the Solar System

    • Milky Way and the solar system.
    • Modern theories on the origin of the Earth and planetary bodies.
    • Earth’s orbital parameters, Kepler’s laws of planetary motion.
    • Geological Time Scale; space and time scales of processes in the solid Earth, atmosphere, and oceans.
    • Radioactive isotopes and their applications.
    • Meteorites: chemical composition and primary differentiation of the Earth.
    • Basic principles of stratigraphy.
    • Theories about the origin of life and fossil records.
    • Earth’s gravity, magnetic fields, and thermal structure: Geoid and spheroid concepts; Isostasy.
  2. Earth Materials, Surface Features, and Processes

    • Gross composition and physical properties of important minerals and rocks.
    • Properties and processes responsible for mineral concentrations.
    • Distribution of rocks and minerals in Earth’s units and India.
    • Physiography of the Earth; weathering, erosion, and soil formation.
    • Energy balance of Earth’s surface processes.
    • Physiographic features and river basins in India.
  3. Interior of the Earth, Deformation, and Tectonics

    • Basic concepts of seismology and Earth’s internal structure.
    • Physico-chemical and seismic properties of Earth’s interior.
    • Stress and strain concepts; rock deformation.
    • Folds, joints, and faults; causes and measurement of earthquakes.
    • Interplate and intraplate seismicity; paleomagnetism.
    • Sea-floor spreading and plate tectonics.
  4. Oceans and Atmosphere

    • Hypsography of continents and ocean floors: continental shelves, slopes, abyssal plains.
    • Physical and chemical properties of seawater; residence times of elements.
    • Ocean currents, waves, tides, thermohaline circulation, and conveyor belts.
    • Major water masses, biological productivity, and fluid motion.
    • Atmospheric structure and heat budget; greenhouse gases and global warming.
    • General circulation, monsoon systems, ENSO, cyclones, and local systems in India.
    • Marine and atmospheric pollution, ozone depletion.
  5. Environmental Earth Sciences

    • Properties of water and the hydrological cycle.
    • Energy resources: uses, degradation, alternatives, and management.
    • Ecology, biodiversity, and natural resource conservation.
    • Natural hazards and remote sensing applications.

PAPER I (PART C)

I. Geology

  1. Mineralogy and Petrology

    • Point group, space group, and lattice concepts.
    • Crystal field theory, mineralogical spectroscopy, and bonding in mineral structures.
    • Genesis, properties, and crystallization of magmas.
    • Metamorphic structures, textures, and thermobarometry.
    • Petrogenesis of Indian rock suites: Deccan Traps, charnockites, ophiolites, and more.
  2. Structural Geology and Geotectonics

    • Stress and strain analysis; Mohr circles.
    • Geometry and mechanics of folds, faults, and ductile shear zones.
    • Plate boundaries, mantle plumes, and Himalayan orogeny.
  3. Paleontology and Applications

    • Life origin theories, evolution models, and mass extinctions.
    • Applications of fossils in age determination, paleoecology, and paleogeography.
    • Micropaleontology in hydrocarbon exploration.
  4. Sedimentology and Stratigraphy

    • Classification of sediments and sedimentary rocks.
    • Sedimentary environments and basin evolution.
    • Stratigraphic principles, correlation methods, and sequence stratigraphy.
    • Phanerozoic stratigraphy of India.
  5. Marine Geology and Paleoceanography

    • Ocean floor morphology, ocean circulation, and thermohaline processes.
    • Factors influencing oceanic sediments and paleoceanographic reconstruction.
  6. Geochemistry

    • Atomic properties, periodic table, thermodynamics of reactions, and isotopes in geochronology.
    • Applications of stable isotopes in Earth processes.
  7. Economic Geology

    • Ore formation processes, mineral deposit studies, and petroleum geology.
    • Coal and unconventional energy resources.
  8. Precambrian Geology and Crustal Evolution

    • Evolution of Earth systems and Precambrian characteristics of India.
    • Precambrian–Cambrian boundary.
  9. Quaternary Geology

    • Quaternary stratigraphy, climate variability, and human evolution.
    • Dating methods and tectonic geomorphology.
  10. Applied Geology

  • Remote sensing and GIS.
  • Engineering properties of rocks; construction investigations.
  • Methods of mineral exploration and groundwater studies.

II. Physical Geography

  1. Geomorphology: Landform processes, DEM analysis, extraterrestrial geomorphology.
  2. Climatology: Radiation balance, wind systems, ENSO, and climate classification.
  3. Biogeography: Plant and animal associations, Indian biogeography, and conservation.
  4. Environmental Geography: Man-land relationships, hazards, and ecological balance.
  5. Geography of India: Physical geography, climatology, agriculture, and population characteristics.

III. Geophysics

  1. Signal Processing: Fourier transforms, filters, and signal analysis.
  2. Field Theory: Newtonian potential, Green’s theorem, and seismic wave propagation.
  3. Numerical Analysis and Inversion: Least squares, optimization, and pattern recognition.
  4. Gravity and Magnetic Methods: Data interpretation and anomaly analysis.
  5. Seismic Methods: Ray theory, reflection/refraction techniques, seismic stratigraphy.
  6. Well Logging: Techniques for lithology, porosity, and fluid saturation interpretation.

(IV) METEOROLOGY

1) Climatology

  • Same as under Geography.

2) Physical Meteorology

  • Thermal Structure of the Atmosphere and Its Composition.
  • Radiation:
    • Basic laws – Rayleigh and Mie scattering, multiple scattering.
    • Radiation from the sun, solar constant, effect of clouds, surface and planetary albedo.
    • Emission and absorption of terrestrial radiation, radiation windows, radiative transfer, Greenhouse effect, net radiation budget.
  • Thermodynamics of Dry and Moist Air:
    • Specific gas constant, adiabatic and isentropic processes, entropy and enthalpy.
    • Moisture variables, virtual temperature, Clausius–Clapeyron equation.
    • Adiabatic processes of moist air, thermodynamic diagrams.
  • Hydrostatic Equilibrium:
    • Hydrostatic equation, variation of pressure with height, geopotential, standard atmosphere, altimetry.
  • Vertical Stability of the Atmosphere:
    • Dry and moist air parcel and slice methods, tropical convection.
  • Atmospheric Optics:
    • Visibility and optical phenomena – rainbows, haloes, corona, mirage, etc.

3) Atmospheric Electricity

  • Fair weather electric field in the atmosphere and potential gradients.
  • Ionization in the atmosphere, electrical fields in thunderstorms.
  • Theories of thunderstorm electrification, structure of lightning flash, mechanisms of earth-atmospheric charge balance, and the role of thunderstorms.

4) Cloud Physics

  • Cloud classification, condensation nuclei, growth of cloud drops and ice-crystals.
  • Precipitation mechanisms: Bergeron–Findeisen process, coalescence process.
  • Precipitation of warm and mixed clouds, artificial precipitation, hail suppression, fog and cloud dissipation.
  • Radar observation of clouds and precipitation:
    • Radar equation, rain drop spectra, radar echoes of hailstorms, tornadoes, hurricanes, and rainfall measurements.

5) Dynamic Meteorology

  • Basic Equations and Fundamental Forces:
    • Pressure, gravity, centripetal and Coriolis forces.
    • Continuity and momentum equations (Cartesian and spherical coordinates).
    • Scale analysis, inertial flow, geostrophic and gradient winds, thermal wind.
    • Divergence and vertical motion, Rossby, Richardson, Reynolds, and Froude numbers.
  • Atmospheric Turbulence:
    • Mixing length theory, planetary boundary layer equations, Ekman layer, eddy transport of heat, moisture, and momentum.
  • Linear Perturbation Theory:
    • Internal and external gravity waves, inertia waves, gravity waves, Rossby waves, wave motion in the tropics, barotropic and baroclinic instabilities.
  • Atmospheric Energetics:
    • Kinetic, potential, and internal energies; conversion into kinetic energy; available potential energy.

6) Numerical Weather Prediction (NWP)

  • Computational instability, filtering of sound and gravity waves.
  • Filtered forecast equations, barotropic and baroclinic models.
  • Objective analysis, data assimilation techniques, satellite applications in NWP.

7) General Circulation and Climate Modelling

  • Observed zonally symmetric circulations, meridional circulation models.
  • General circulation modelling principles: grid-point and spectral GCMs.
  • Climate variability phenomena: ENSO, QBO, MJO, etc.
  • Ocean-atmosphere coupled models.

8) Synoptic Meteorology

  • Weather observations and transmission, synoptic charts.
  • Synoptic weather forecasting, prediction of weather elements, and hazardous weather phenomena.
  • Tropical Meteorology:
    • ITCZ, monsoons, tropical cyclones, jet streams.
  • Extra-Tropical Features:
    • Jet streams, extratropical cyclones, anticyclones.
  • Air masses and fronts: sources, classification, frontogenesis, and associated weather.

9) Aviation Meteorology

  • Meteorological role in aviation, weather hazards during takeoff, cruising, and landing.
  • In-flight hazards: icing, turbulence, visibility issues, gusts, wind shear, thunderstorms.

10) Satellite Meteorology

  • Polar orbiting and geostationary satellites.
  • Applications in identifying synoptic systems, cyclones, temperature estimation, rainfall prediction, and temperature/humidity soundings.

(V) OCEAN SCIENCES

1) Physical Oceanography

  • T-S diagrams, mixing processes, characteristics of water masses.
  • Wind-generated waves, shallow and deep-water wave dynamics.
  • Coastal processes: wave reflection, refraction, diffraction, littoral currents, rip currents, tsunami, and more.
  • Ocean Circulation:
    • Global conveyor belt circulation, Ekman’s theory, upwelling processes.

2) Chemical Oceanography

  • Composition of seawater, chemical exchanges, and classification of elements.
  • Element chemistry under special conditions (estuaries, vents, etc.).
  • Carbonate chemistry, biological pumps, and sedimentary deposit factors.

3) Geological Oceanography

  • Topics as listed under “Marine Geology & Paleoceanography.”

4) Biological Oceanography

  • Classification of marine environments and organisms.
  • Primary and secondary production, factors affecting biodiversity.
  • Human impacts on marine communities and climate change effects.

 

How Study Hub Can Help You Prepare for the Earth, Atmospheric, Ocean, and Planetary Sciences Syllabus

Preparing for the extensive and demanding syllabus of Earth, Atmospheric, Ocean, and Planetary Sciences (702) requires a strategic approach and access to comprehensive study resources. Study Hub (accessible at studyhub.net.in) offers unparalleled support to help candidates excel in this challenging domain. Here’s how Study Hub can guide your preparation:


Comprehensive Coverage of Topics

At Study Hub, we provide in-depth study materials, mock tests, and curated articles to help candidates grasp even the most complex topics. Our resources are designed to address every aspect of the syllabus, including:

  1. Meteorology: Understand critical concepts like the thermal structure of the atmosphere, radiative transfer, vertical stability, numerical weather prediction, general circulation and climate modelling, and the role of satellite meteorology in observing weather systems such as cyclones, monsoons, and thunderstorms.

  2. Ocean Sciences: Dive into topics such as physical oceanography, chemical oceanography, geological oceanography, and biological oceanography. Study Hub’s resources emphasize key aspects like upwelling processes, estuarine circulation, ocean eddies, Ekman theory, and global conveyor belt circulation—helping you understand the intricate processes of ocean systems.

  3. Atmospheric Dynamics and Energetics: Through articles, conceptual guides, and practice questions, candidates gain a strong grasp of fundamental equations, vorticity, geostrophic winds, Rossby waves, atmospheric turbulence, and barotropic and baroclinic instabilities.

  4. Planetary Sciences: Our expertly crafted content helps students explore planetary structures, processes, and phenomena with precision, complementing other topics under Earth Sciences for an interdisciplinary understanding.


Mock Tests and Evaluation Framework

We align our mock tests and sample papers with the pattern of the Earth Sciences examination:

  • Objective Analysis for Numerical Weather Prediction (NWP): Test your knowledge of filtered forecasting models and data assimilation techniques.
  • Synoptic Meteorology Practices: Work on real-world weather data and forecast exercises involving tropical cyclones, ITCZ systems, monsoon depressions, and jet streams.
  • Topic-specific tests ensure mastery in areas like atmospheric optics, biochemical nutrient cycling, and the impact of human activities on ecosystems.

Why Study Hub is the Perfect Partner for Your Earth Sciences Preparation

  1. Academic Rigor: Study Hub maintains an academic tone throughout its resources, ensuring in-depth coverage of essential keywords such as radiative budget, MJO (Madden-Julian Oscillation), Quasi-Biennial Oscillation (QBO), and ENSO phenomena.
  2. Focused on Practical Applications: Be it radar observations, wave refraction techniques, or the impact of anthropogenic inputs on marine biodiversity, we emphasize the practical relevance of each topic for better comprehension.
  3. Adaptive Materials: From simple T-S diagrams to advanced topics like geopotential variation and numerical baroclinic models, we tailor our resources to match both beginner and advanced levels of understanding.
Scroll to Top