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ATMOSPHERE Air Circulation

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ATMOSPHERE Air Circulation UNIT 7 Meteorology and Climate Atmosphere-Ocean Coupling Why study atmospheric circulation? Atmosphere and ocean processes are intertwined ... – PowerPoint PPT presentation

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Title: ATMOSPHERE Air Circulation


1
ATMOSPHERE Air Circulation
  • UNIT 7
  • Meteorology and Climate

2
Atmosphere-Ocean Coupling
  • Why study atmospheric circulation?
  • Atmosphere and ocean processes are intertwined
  • Atmosphere-ocean interaction moderates surface
    temperatures, weather and climate
  • Weather local atmospheric conditions
  • Climate regional long-term weather
  • Atmosphere drives most ocean surface waves and
    currents

3
Composition of the Atmosphere
  • Dry Air 78 Nitrogen, 21 Oxygen
  • BUT it is never completely dry
  • Typically contains about 1 water vapor
  • Chemical residence time of water vapor in the air
    is about 10 days
  • Warm air holds much more water vapor than cold
    air

http//www.nature.com/scitable/knowledge/library/t
he-global-climate-system-74649049
4
Density of Air
  • Typical air density 1 mg/cm3
  • Temperature and pressure affect the density of
    air
  • Temperature Hot air is less dense than cold air
  • Pressure Air expands with elevation above sea
    level

http//www.physicalgeography.net/fundamentals/7d.h
tml
5
Density and Temperature
  • Rising air expands and cools
  • Vapor condenses into clouds and precipitation
  • Sinking air is compressed and warms
  • Clear air

6
Expanding Air Cools and Condenses
  • Like opening a pressurized bottle of soda
  • Air expands and cools
  • Water vapor condenses cloud formation

7
Solar Heating of the Earth
  • Solar energy absorbed unevenly over Earths
    surface why is air rising?
  • Energy absorbed / unit surface area varies with
  • Angle of the Sun
  • Reflectivity of the surface (i.e., ice versus
    ocean)
  • Transparency of the atmosphere (i.e. clouds)

8
Solar Insolation Variations with Latitude
9
(No Transcript)
10
Solar Heating of the Earth
  • Sunlight heats the ground more intensely in the
    tropics than near poles

July
January
11
Solar Heating and Seasons
  • Seasons are caused by Earths 23.5 tilt

http//astro.unl.edu/naap/motion1/animations/seaso
ns_ecliptic.html
12
Solar Heat Energy
  • Equator absorbs more heat from the sun than it
    radiates away
  • Polar regions radiates much more heat than they
    absorb from the sun
  • Energy in at equator and heat out at poles
  • Heat transfer from
  • E.g. Equator isnt that hot Poles arent that
    cold
  • Evidence that the atmosphere (2/3) and oceans
    (1/3) redistribute heat (wind and ocean currents)
  • Convective heat transfer moderates Earth climate

http//oceanmotion.org/html/resources/solar.htmvi
shead
13
Convective Heat
  • Convective heat transfer models Earth climate
  • Heated air expands and rises, then cools and sinks

Equator
Poles
14
Atmospheric Circulation
Cold, more dense air sinks near the Poles
Warm, less dense air rises near the Equator
Cold, more dense air sinks near the Poles
Wind from the north
15
Actual Atmospheric Circulation
  • Air rises and sinks
  • More than one convection cell
  • Earth spins once per day that amounts to a speed
    for us at the surface of Earth of 100s of miles/
    hour
  • Coriolis Effect

16
Coriolis Effect Movies
http//earthsciweb.org/GeoMod/index.php?titleCori
olis
http//science.nasa.gov/science-news/science-at-na
sa/2004/23jul_spin/
http//ww2010.atmos.uiuc.edu/28Gh29/guides/mtr/f
w/gifs/coriolis.mov
17
The Coriolis Effect on Earth
  • Surface velocity increases from poles to equator
  • Points on the equator must move faster than
    points near the poles to go around once a day
  • Latitude velocity differences land to curving
    paths
  • Northern hemisphere deflected to right

18
The Coriolis Effect
  • Strength of Deflection varies with latitude
  • Maximum at the poles
  • Zero(!) at equator
  • Faster a planet rotates, the stronger the
    Coriolis effects
  • The larger the planet, the stronger the Coriolis
    effects (Jupiter spins once every 10 hours)

19
Hurricanes
  • A storm with lots of clouds has rising air thus
    low-pressure at the surface!
  • Converging air sets up counter-rotation
    (cyclonic)

Spinning clockwise Bending to the right
Spinning counter clockwise Bending to the left
20
Hurricanes Low Pressure
  • Hurricane is rising and already has moisture in
    it
  • Low pressure system at the surface air rising
    so that means air is being sucked in at the base
  • Arrows get defected by Coriolis to the right
  • Set up a counter clockwise circulation in the
    northern hemisphere

L
21
High Pressure
  • Air sinks and compresses and it gets warmer and
    dry
  • See clear air not clouds
  • Pushes air away
  • Rotate clockwise in northern hemisphere

H
22
Atmospheric Circulation
  • Sinking air at 30 deserts
  • Easterly winds trade winds
  • Westerly winds at 30 and 60

23
Atmospheric Circulation
  • 3 convection cells in each hemisphere
  • Each cell 30 latitudinal width
  • Veritcal Motions
  • Rising Air 0 and 60 Latitude
  • Sinking Air 30 and 90 Latitude
  • Horizontal Motions
  • Zonal winds flow nearly along latitude lines
  • Zonal winds within each cell band
  • DUE to DEFLECTIONS BY CORIOLIS!

24
Sea Breeze
  • Land warms fastest during the day. Air during the
    day expands and rises
  • Ocean surface temperature changes slowly. Air
    cools and becomes more dense, sinks then begins
    to rise over the land.
  • Result wind from sea towards land

25
Land Breeze
  • Land cools fastest at night. Low heat capacity.
    Air contracts and sinks
  • Ocean surface temperature changes slowly. Air is
    pushed away and up by cooler denser land air.
  • Result wind from land towards sea

26
Marine Layer
  • Cold waters, warm air think cloud layer on ocean
    surface
  • Subtropics H pressure, regional subsidence
  • Cloud layer flows onto land at night
  • Evaporates over land by day

LAND
OCEAN
27
Marine Layer
  • Cold waters, warm air think cloud layer on ocean
    surface
  • Subtropics H pressure, regional subsidence
  • Cloud layer flows onto land at night
  • Evaporates over land by day

LAND
OCEAN
28
Marine Layer
  • Cold waters, warm air think cloud layer on ocean
    surface
  • Subtropics H pressure, regional subsidence
  • Cloud layer flows onto land at night
  • Evaporates over land by day

LAND
OCEAN
29
Marine Layer
  • Cold waters, warm air think cloud layer on ocean
    surface
  • Subtropics H pressure, regional subsidence
  • Cloud layer flows onto land at night
  • Evaporates over land by day

LAND
OCEAN
30
Marine Layer
  • Cold waters, warm air think cloud layer on ocean
    surface
  • Subtropics H pressure, regional subsidence
  • Cloud layer flows onto land at night
  • Evaporates over land by day

LAND
OCEAN
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