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TOPIC 3 GLOBAL CYCLES AND PHYSICAL SYSTEMS

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If winds reach 33 m/s: CYCLONE / HURRICANE! Different names depending on location: 'Hurricane' - North Atlantic, NE Pacific 'Typhoon' - NE Pacific ' ... – PowerPoint PPT presentation

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Title: TOPIC 3 GLOBAL CYCLES AND PHYSICAL SYSTEMS


1
TOPIC 3 - GLOBAL CYCLES AND PHYSICAL SYSTEMS
  • Atmosphere - envelope of gases surrounding Earth
    (Ch. 21 Env. Sci.)
  • Structure and function (3.1)
  • Depletion of Stratospheric Ozone (3.2)
  • Tropospheric Ozone (3.3)
  • Issue of Global Warming (3.4)
  • Acid Deposition (3.5)
  • Hydrosphere - liquid envelope (3.6)
  • Lithosphere - solid earth (3.7)
  • Soil System (3.8)

2
ATMOSPHERE
  • Composed mostly of gases but also some small
    solid particles (ash, dust, salt, pollen) and
    liquid solid water
  • Main gases

3
Atmospheric structure
  • About 1000 km thick
  • Held in place by gravity
  • More than 99 of mass is in first 40 km of
    earths surface
  • Above 100 km it is virtually a vacuum
  • Five layers characterized by differences in
    temperature, composition, movement and density

4
Five layers
  • Troposphere (0 to 8 -16 km)
  • Starts at earths surface
  • Most dense layer - contains most of atmospheres
    mass, water vapour and dust
  • Site and source of almost all weather
  • Upper boundary called tropopause ranges in height
    from 8 km in high latitudes to 16 km above the
    equator
  • Tropopause also varies with seasons - highest in
    summer and lowest in winter

5
Temperature profile of the atmosphere
  • Temperature decreases from 17 to -75oC in
    troposphere as the distance from earth increases
  • lapse rate rate at which temperature declines
    with increasing altitude in the troposphere (6oC
    per km)

6
More on the troposphere
  • Contains most of water vapour and clouds in
    atmosphere
  • Troposphere means region of mixing
  • Wind speeds increase with height due to decreased
    friction

7
2. Stratosphere (8-16 to 50 km)
  • stratopause at 50 km
  • Dry - very low water vapour content
  • Lacks dust
  • Less dense than troposphere
  • Temperature remains constant up to 25 km then it
    increases to -3oC due to UV absorption by ozone
    layer (at 20-30 km)
  • 90 of ozone in atmosphere is the stratosphere
    (10 ppm compared to 0.04 ppm in troposphere)
  • Little vertical mixing - movement by diffusion
    only

8
3. Mesosphere (50-80 km)
  • Mesopause at 80 km
  • Temperatures fall to -90oC due to decreasing
    density and inability to absorb energy

9
4. Ionosphere (80-600 km)
  • Ionosphere exosphere thermosphere
  • Temperature increases with altitude up to 1200oC
    due to absorption of intense solar energy by O2
    and N2 which break apart into ions, releasing
    energy
  • 5. Exosphere (600 - 1000 km)
  • Relatively undefined
  • Transitional zone between atmosphere and space
  • Helium and hydrogen are major components

10
Global warming and atmospheric layers
  • http//www.ghcc.msfc.nasa.gov/MSU/atmos_layers.htm
    l

11
Functions of the atmosphere
  • Recycling of water and other chemicals
  • Temperature regulation - moderates climate on
    earth (greenhouse effect)
  • Protection from high energy short-wave radiation
    (UV) from sun
  • Protection from small meteors
  • Reservoir of oxygen, carbon dioxide and nitrogen

12
Global atmospheric energy budget
  • Solar radiation (short wave UltraViolet (UV)
    radiation) entering the atmosphere can take
    several paths
  • 30 reflected by atmosphere - never makes it to
    earth
  • 19 is absorbed by atmosphere
  • 51 is absorbed by earths surface (land and
    oceans)

13
Global energy budget
14
Of the 51 absorbed by the earths surface
  • 21 is re-radiated to space as long wave InfraRed
    (IR) radiation (directly or via the atmosphere)
  • 23 is transferred to the atmosphere through
    evaporation (latent heat flux heat required for
    a material to change state)
  • 7 is transferred by conduction and re-radiation
    (sensible heat flux heat transfer due to
    conduction and convection)
  • Finally the atmosphere re-radiates heat as long
    wave (IR) radiation into space

15
Weather
  • Weather is caused by the transfer of energy
  • Energy is transferred wherever there is a
    temperature difference between two objects
  • Three main ways energy can be transferred
  • Radiation e.g. visible light, UV, IR
  • Conduction - contact between objects
  • Convection - movement

16
Energy movement
  • Solar radiation (UV) enters the atmosphere - some
    is absorbed by the earth
  • The energy is transferred by conduction to a thin
    layer of air above the earth
  • Convection occurs because warmer air is less
    dense than colder air so it rises - taking the
    energy with it

17
Unequal heating of earths surface by sun
  • An area at the equator receives more solar
    radiation than an equal area at the poles because
    of
  • The angle of exposure
  • The distance the radiation travels through the
    atmosphere is less at the equator (the atmosphere
    absorbs part of the energy)

18
Atmospheric circulation
  • High solar radiation at the equator produces hot
    air which rises because of its low density
  • In contrast, air at the poles is cold because of
    low solar radiation - the cold air sinks because
    of its high density which results in a high
    pressure zone near the poles
  • Fluids flow from High Pressure Zones to Low
    Pressure Zones so we would expect surface winds
    to flow from the poles (high P) to the equator
    (low P) - single cell

19
Coriolis Effect
  • We dont see this simple pattern of air
    circulation (a single cell in each hemisphere)
    due to the CORIOLIS EFFECT
  • Objects that are moving relative to the ground
    are deflected to the right in the northern
    hemisphere and to the left in the southern
    hemisphere
  • The amount of deflection increases with speed of
    the moving object and with latitude (no Coriolis
    Effect at the equator)

20
Global Wind Pattern
  • Result of the effects of pressure (uneven heating
    of the earths surface) and Coriolis Effect
    (rotation of the earth)
  • Heating at equator (0o latitude) causes air to
    warm - this air expands resulting in a low
    pressure zone
  • Warm air rises, expands and cools (lapse rate!) -
    losing moisture by precipitation and resulting in
    a high pressure zone
  • Air flows toward low pressure zone and as it
    becomes cooler and drier its density increases,
    so at 30oN and 30oS the air sinks

21
  • Much of this air returns to the equator along
    the surface becoming warmer and picking up
    moisture along the way - as it travels the air is
    deflected by the Coriolis Effect resulting in
    Northeast Trade Winds and Southeast Trade Winds
  • These trade winds converge at the equator
    resulting in light and variable winds called the
    Doldrums where wind is being convected upwards
  • Similarly there is little wind at 30oN and S
    (Horse Latitudes) because air is moving downwards

22
Tricellular Model
  • Hadley Cell - wind flow pattern of air rising at
    the equator and descending at 30oN and 30oS
  • Ferrel Cell - at 30oN and 30oS some of the
    descending air travels pole-ward - these surface
    winds are deflected by the Coriolis Effect to
    become the Westerlies of both hemispheres
  • Surface winds travel pole-ward until about 50oN
    and 50oS where they encounter cold dense air
    coming from the poles
  • Air is forced upwards where it diverges so that
    some goes equator ward to complete Ferrel cell
    and some pole ward

23
Tricellular model
  • Polar Cell -upper air moving pole ward cools,
    becomes dense and sinks back to the surface at
    the poles

24
Atmospheric circulation
  • Is responsible for distributing energy (heat)
    from the equator to the poles
  • Gives rise to climatic zones and biomes
  • Tropical rainforests near the equator
  • Deserts at 30o where dry air descends

25
Tropical cyclones
  • non-frontal low-pressure system over tropical or
    sub-tropical waters with organized convection and
    cyclonic surface wind circulation
  • Vortex-like centres of very low pressure,
    associated with extremely high, often destructive
    winds blowing toward the centre or eye (IB)
  • Disc shaped
  • Vertical dimension - tens of kilometres
  • Horizontal dimension - hundreds of kilometres
  • http//www.aoml.noaa.gov/hrd/weather_sub/faq.html
  • http//www.hko.gov.hk/informtc/nature.htm

26
Tropical cyclones
  • Tropical cyclones with maximum sustained surface
    winds of less than 17 m/s (34 kt, 39 mph, 63
    km/h) are called tropical depressions
  • If maximum sustained wind is greater than 17 m/s
    then they are called tropical storms
  • If winds reach 33 m/s CYCLONE / HURRICANE!
  • Different names depending on location
  • Hurricane - North Atlantic, NE Pacific
  • Typhoon - NE Pacific
  • Tropical cyclone - SW Indian Ocean
  • Naming of hurricanes / cyclones
  • http//www.aoml.noaa.gov/hrd/tcfaq/B2.html

27
How do cyclones form?
  • Requirements
  • Warm water (26.5oC or more) - energy source
  • Moist atmosphere
  • Low wind shear - wind must be blowing in the same
    direction and at the same speed up to 9,000
    metres above the sea
  • Air cools very quickly with vertical distance
  • Minimum distance of 500 km from equator (Coriolis
    effect)
  • Dissipate when they reach land as their energy
    source (warm water) is gone
  • Cyclones and depressions have an important role
    in the distribution of energy

28
Depression (temperate cyclone)
  • A region of relatively low pressure (up to 2000
    km across) in middle latitudes in which winds
    spiral inwards and counterclockwise in the
    northern hemisphere and clockwise in the southern
    hemisphere (IB)
  • Associated with windy, cloudy and wet weather
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