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EG1204: Earth Systems: an introduction

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EG1204: Earth Systems: an introduction Meteorology and Climate Lecture 6 The oceans and winds Topics we will cover Ocean structure and circulation Sea surface ... – PowerPoint PPT presentation

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Title: EG1204: Earth Systems: an introduction


1
EG1204 Earth Systems an introduction
  • Meteorology and Climate
  • Lecture 6
  • The oceans and winds

2
Topics we will cover
  • Ocean structure and circulation
  • Sea surface temperatures (and ENSO)
  • Salinity
  • Global winds
  • Local winds
  • Assignment 2 tips

3
Ocean structure and circulation
  • At the ocean surface, winds produce a thermally
    mixed surface layer averaging a few tens of
    metres deep poleward of latitude 60º, 400 m at
    latitude 40º and 100-200 m at the equator

4
Ocean structure and circulation
  • Below the (relatively) warm, thermally mixed
    layer is the thermocline
  • The thermocline is a layer in which (vertically)
    temperature decreases and density increases
  • The thermocline layer exhibits a stable
    stratification which tends to inhibit vertical
    mixing and and acts as a barrier to warmer water
    above and colder water below

5
Ocean structure and circulation
  • The ocean currents of the world are thought to
    move in accordance with a conveyor belt paradigm
  • This deep ocean thermohaline circulation system
    has been accepted theory for some time
  • The theory has recently come under close scrutiny
    - and may soon be revised
  • (see Wunsch (2000) NATURE 405 (6788) 743-744 JUN
    15 2000)

6
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7
Sea surface temperature
  • Sea surface temperatures (SSTs) were first mapped
    by Alexander von Humboldt in 1817
  • SSTs vary from about -1.9ºC at the poles to over
    30ºC in the Persian Gulf and the Red Sea in july.
  • Differences in temperature between oceans near
    the coast and areas inland lead to the creation
    of coastal breezes

8
Sea surface temperature
  • Isotherms of SST generally change as a function
    of latitude - although variations occur at coasts
    where the isotherms bend poleward on East coasts
    and equatorward on West coasts
  • Changes in SST greatly influence pressure,
    evaporation and hence wind and rainfall patterns
  • Sometimes relationships between SST patterns and
    pressure/precipitation anomalies occur over a
    great distance from each other and are called
    teleconnections

9
Sea surface temperature
  • The most well known SST anomaly is ENSO
  • Normally easterly trade winds prevents eastward
    movement of warm water from western Pacific to
    eastern Pacific
  • When trade winds weaken, warm water propagates
    eastward, the low pressure over Indonesia breaks
    down and so too does the Walker circulation with
    its downward branch over the eastern Pacific
  • It is essentially a change in SST brought about
    by a change in circulation

10
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11
TOPEX-POSEIDON
  • For much of our oceans, temperature is not
    measured directly but by proxy
  • Warmer water expands if surrounded by cooler
    water it rises. Its height is therefore an
    indication of its temperature

12
TOPEX-POSEIDON
  • TOPEX is an altimetric satellite
  • Return time of pulses of energy sent by TOPEX to
    the ocean surface are measured
  • Distance between satellite and water surface can
    be accurately measured
  • TOPEX used to measure El Niño

13
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14
Salinity
  • There are normally about 34.5 grams of salts
    dissolved in each kilogram of sea water - written
    as 34.50
  • The salinity affects climate by altering the
    density of the sea - thus changing the patterns
    of pressures which govern ocean currents and
    hence heat transport around the globe

15
The global winds
  • The driving force of ANY wind is the local
    pressure gradient expressed as
  • ?p/ ?n where
  • ?p is the difference between the pressures at
    points separated horizontally by a distance ?n

16
The global winds
  • Where there is a chain of centres of convergence
    associated with convective storms air moves
    vertically into the upper atmosphere
  • The raised air increases upper level pressure
    which creates poleward winds
  • The Coriolis deflection prevents the upper winds
    from reaching beyond 30º creating a belt of
    subtropical highs

17
The global winds
  • The accumulated air gradually cools, then sinks
    and creates surface high pressure
  • The descending air then replaces air moving
    equatorward at the surface to feed convection
    their - thus forming a circuit of motion we call
    a Hadley Cell

18
Hadley Cells
19
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20
The global winds
  • Winds between the tropics converge on a line
    called the Inter-Tropical Convergence Zone (ITCZ)
  • This line of convergence can be discerned on a
    map of streamlines and visualised on a satellite
    image from space

21
ITCZ (Inter-Tropical Convergence Zone)
22
The global winds
  • The ITCZ lies about 5º North on average - known
    as the meteorological equator and matching the
    equators of radiation
  • ITCZ movement across southern Africa is
    complicated by land characteristics

23
The global winds
  • Winds are mainly easterly at latitudes between
    10-30º - these are known as the trade winds or
    trades
  • Westerly winds prevail at about 35-60º and are
    known as the midlatitude winds
  • There are polar easterlies at latitudes above 60º

24
The global winds
  • The seasonal Monsoon circulation (West African,
    Asian and Northern Australian) result from moist
    south westerlies converging with dry north
    easterlies at special regions
  • Monsoon winds bring large amounts of rainfall to
    their respective regions
  • Desert winds can be vigourous - generating winds
    such as the Harmattan, Scirocco, Haboob and Willy
    willies

25
The local winds
  • Sea breezes due to SST varying each day by only
    a degree or so - whilst surface air temperatures
    onshore change by around ten times as much
  • Land breeze the opposite of a sea breeze happens
    at night when the land has cooled below that of
    SSTs
  • Mountain winds the foehn effect, when the
    warming of winds blowing down mountains after
    there has been rainfall on the windward side
  • Katabatic and Anabatic winds katabatic winds are
    downhill flows of cold air driven by gravity

26
The local winds
  • The daytime counterparts of katabatic winds are
    anabatic winds - they flow up sunny slopes
    fuelled by solar convectional heating and provide
    thermals for gliders
  • Anabatic winds are deeper and more gusty than
    katabatic winds

27
Assignment 2 Tips
  • Show evidence of reading
  • Avoid websites, Wikipedias and partisan
    organisations
  • Summarise your data statistically
  • Means
  • Standard deviation
  • Minimum and Maximum values
  • Use field photos or sketches
  • Use an annotated map
  • Think carefully about how you display data in a
    graph

28
Assignment 2 Tips
29
Assignment 2 Tips
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