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Atmospheric Circulation (Air-Sea Interaction)

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Title: Atmospheric Circulation (Air-Sea Interaction)


1
Atmospheric Circulation (Air-Sea Interaction)
  • We live at the bottom of an ocean of air, the
    atmosphere
  • The atmosphere and the ocean are interdependent
    what happens in one system causes changes in the
    other
  • Surface currents in the oceans are directly
    caused by atmospheric winds

2
Air-Sea Interaction
  • Differences in solar energy (heating) across the
    Earth combined with the Earths spin create
    winds
  • Winds drive surface currents and create waves
  • Likewise, certain atmospheric phenomena are
    manifested (originate) in the oceans
  • El Niño Southern Oscillation
  • Hurricanes, cyclones

3
Air-Sea Interaction
  • Earths atmosphere is composed mainly of
    Nitrogen, Oxygen, and Water Vapor
  • Nitrogen 78
  • Oxygen 21
  • Argon, CO2, Neon, Helium, Methane, others 1
  • Air is never completely dry, however, and water
    vapor (H2O) can occupy as much as 4 of the airs
    volume
  • Visible as clouds and fog invisible as water
    vapor
  • Enters atmosphere via evaporation, exits via
    condensation

4
Air-Sea Interaction
  • Temperature and humidity determine the density of
    air masses, which in turn determines whether
    these air masses will rise or sink
  • Air containing water vapor is less dense than dry
    air at the same temperature and density
  • Also, when heated, air expands and becomes less
    dense
  • This means that cold air is denser than warm air
    and cold, dry air is much denser than warm, moist
    air

5
Say what?
  • Warm air is less dense than cold air because
    increasing temperature results in greater
    molecular dispersion
  • ? Increasing Temperature

6
Say what? (Continued)
  • Moist air is less dense than cold air because the
    weight of water vapor (H2O) is less than that of
    Nitrogen (N2) and Oxygen (O2)
  • When water vapor increases, the amount of O2 and
    N2 decreases per unit volume
  • Molecular weight of O2 16 16 32
  • Molecular weight of N2 14 14 28
  • Molecular weight of H2O 1 1 16 18

7
Atmospheric Circulation
  • Air masses will move from regions of high
    pressure (dense air) to regions of low pressure
    (less dense air)
  • A low pressure zone results from moist and/or
    warm air
  • A high pressure zone results from dry and/or cold
    air
  • The flow of air from regions of high to low
    pressure create the winds

8
Atmospheric Circulation
  • Because warm and/or moist air is less dense, it
    rises (heat rises)
  • Likewise, cool and/or dry air is more dense and
    so it sinks
  • As air rises, it expands and cools water vapor
    in rising, expanding air will condense into
    clouds because the cooler air is no longer able
    to hold as much water vapor
  • Precipitation transfers water vapor (AND HEAT!!)
    from low to high latitudes

9
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10
Solar Heating Varies with Latitude
  • The Earth revolves around the sun in an
    elliptical path
  • The Earth itself is tilted at an angle of 23.5
  • The tilt of Earths rotational axis results in
    the seasons

11
Solar Heating Varies with Latitude
  • Approximately half of the solar energy reaching
    the Earth is absorbed, but this heat is not
    evenly absorbed
  • The amount of solar energy reaching the Earths
    surface varies with latitude and season
  • Because of the Earths tilt, solar energy
    reaching the equator strikes at a low angle,
    concentrating the radiation in a small area
    solar energy reaching the poles, however, does so
    at a lower angle and so less heat is absorbed in
    polar zones

12
Near the poles, light filters through more
atmosphere and approaches at a low angle,
favoring reflection rather than absorption
13
Got albedo?
  • Albedo is the measure of solar radiation that is
    reflected back into space
  • A high albedo indicates that more energy is
    reflected back into space, while a low albedo
    indicates that less energy is reflected back to
    space
  • Ice and snow (even clouds) increases albedo, and
    so much of the light that reaches the polar
    regions is reflected back into space

14
Uneven solar heating and atmospheric circulation
  • Air is warmed in the tropics and rises
  • Air is cooled near the poles and falls
  • It seems logical to suspect then, that air heated
    in the tropics expands and becomes less dense as
    it moves towards the poles, where it will cool
    (and condense) sinking back towards the poles.
  • BUT, THIS IS NOT WHAT HAPPENS!

15
HYPOTHETICAL CIRCULATION ON A NON-SPINNING EARTH
16
Enter the Coriolis Effect
  • Experience will tell us, however, that winds in
    the mid-latitudes of the northern hemisphere do
    NOT flow out of the north, but rather the west
  • The hypothetical winds described do not resemble
    the actual wind patterns of the Earth because we
    have neglected the effect of the Earths rotation

17
Enter the Coriolis Effect
  • The rotation of the Earth strongly influences the
    motion of air and water
  • This effect is named the Coriolis effect after
    its discoverer, Gaspard Gustave de Coriolis
  • The Coriolis effect changes the intended path of
    a moving body
  • Causes moving objects on Earth to follow curved
    paths

18
Coriolis The Example
  • Imagine you and your friend are on a carousel
  • You are sitting on the inside of the carousel and
    your friend is sitting on the outside
  • You throw a ball to your friend, but are amazed
    to find that the ball curves sharply to the right
    and your friend is unable to catch it (and this
    is not because you throw like a girl)
  • Other friends watching from a hot air balloon
    hovering over the carousel confirm that the path
    of the ball was in fact straight

19
Coriolis The Example
  • If we compare our carousel to the Earth, we know
    that the Earth will complete a full rotation
    every 24 hours
  • People living on the equator however must
    complete a much larger circumference of rotation
    than would people in middle and high latitudes
  • In order for every part of the Earth to complete
    a rotation in 24 hours, points on the equator
    MUST travel faster than points near the poles

20
Back to the carousel
  • When you throw the ball to your friend on the
    carousel, YOU are traveling slower than he/she is
    riding on the outside of the carousel
  • In order for you and your friend to complete a
    rotation within the same time, the inner riders
    on the carousel must travel slower than those
    riding on the outside who must cover more ground
    in the same amount of time

21
The Coriolis Effect
  • The equator must travel faster
    than higher latitudes must travel
    in order for all regions of
    the Earth to complete
    1 full rotation in 24
    hours (people in Anchorage, AK and Equator all
    experience the same 24-hour day)
  • Therefore as objects travel from one region of
    the globe to another, they are subject to
    changing speeds of travel

rst.gsfc.nasa.gov/Sect14Sect14_1c.html
22
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23
The Coriolis Effect Will Keep You Up At Night.
24
The Coriolis Effect
Your friend, rotating faster to cover more
distance (red line) in same time
15 mph
8 mph
You, rotating slower to cover less distance (blue
line) in same time
25
15 mph
8 mph
You throw ball while moving at 8mph in what you
consider to be a straight path
26
15 mph
As ball travels, it carries with it this slower
motion with it
The carousel beneath the ball is traveling
faster than it
8 mph
27
15 mph
As ball travels, it carries with it this slower
motion with it
The carousel beneath the ball is traveling
faster than it
8 mph
28
15 mph
As ball travels, it carries with it this slower
motion with it
The carousel beneath the ball is traveling
faster than it
8 mph
29
My art is WAY better, but just in case you want
the books version
30
The Coriolis Effect
  • Now imagine that you are at the North Pole and
    your friend is in Rio de Janeiro, Brazil near the
    equator
  • You toss a ball to your friend (yes, use your
    imagination) and the same principles apply you
    are traveling around the world slower than your
    friend is. The ball will be deflected to the
    right due to the rotation of the Earth

31
  • The rotation of the Earth is counter-clockwise
  • In the northern hemisphere, objects are deflected
    to the right relative to their path of motion

32
  • In the southern hemisphere, objects are deflected
    to the left for the same reason (poles are moving
    slower than equator)

33
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34
Coriolis Effect
  • As a plane travels from Antarctica towards the
    equator, it will veer to the left along its path
    (if it did not alter its course) due to Coriolis
    effect
  • During its northern journey, the plane is flying
    over land that is rotating eastward at a slower
    and ever decreasing rate compared to that of
    the jet
  • Objects are deflected to the right in the
    Northern Hemisphere and to the left in the
    Southern Hemisphere regardless of what direction
    (N,S,E,W) they are moving in

35
The Coriolis Effect Influences the Movement of
Air in the Atmosphere
  • Lets return to our hypothetic model of
    atmospheric circulation on the Earth
  • Air does warm, expand and rise along the equator
  • But, instead of traveling continuously from the
    equator to the poles, rising air moves poleward
    and is deflected eastward (to the right) in the
    Northern Hemisphere, and westward (to the left)
    in the Southern Hemisphere

36
The Coriolis Effect Influences the Movement of
Air in the Atmosphere
  • Note that the Coriolis effect does not cause the
    winds it only influences the winds direction
  • As air rises at the equator, it will lose water
    vapor by precipitation caused by the expansion
    (there is decreasing atmospheric pressure
    w/increasing altitude) and cooling. This drier
    air travels north or south of the equator and
    grows denser as it cools

37
The Coriolis Effect Influences the Movement of
Air in the Atmosphere
  • When the air has traveled one third of the way
    from the equator to the pole to about 30N or
    30S latitude, the air becomes dense enough to
    sink back towards the surface, completing the
    loop
  • The Coriolis Effect influences the direction of
    the resulting winds

38
At the equator, warm, moist air rises, resulting
in a low pressure zone
Deflected to the right
As the rising air becomes colder drier,
its density increases, resulting in a high
pressure zone
39
Descending air towards equator is deflected to
the right of its path of motion
Descending air towards equator is deflected to
the left (Southern H.) of its path of motion
40
Throwing a monkey wrench into the Coriolis
concept
  • The tendency of wind to deflect because of the
    Coriolis effect increases with its speed and with
    distance from the equator
  • This means that winds in high latitudes deviate
    much moreso than do tropical winds occurring at
    low latitudes moving at the same speed
  • Likewise, faster winds will be deflected moreso
    than slower winds in either region

41
General Wind Patterns
  • This means that there is, in fact, no Coriolis
    effect at the equator, and hence, no deflection
    of wind
  • This is because the change in velocity (speed) of
    the Earth changes very little near the equator,
    but changes muchy more at higher latitudes ?
    greater Coriolis effect

42
General Wind Patterns
  • A column of warm, low density air rises away from
    the surface and creates a band of low pressure at
    the equator
  • The weather in areas of low pressure is
    characterized by cloudy conditions with lots of
    precipitation because rising air cools and cannot
    retain (hold onto) its water vapor
  • This region is clothed in tropical rain forests

43
General Wind Patterns
  • A column of cool, dense air moves towards the
    surface and creates high pressure zones.
    Descending air is quite dry and so these regions
    are characterized by dry, clear, fair conditions
  • Sinking air is very arid (dry) and the great
    deserts of the world are centered along this band
    of high pressure (30N and 30S)

44
General Wind Patterns
  • Sailors have a special term for the calm,
    equatorial regions where low pressure persists
    and little winds exist the doldrums
  • Sailors also have a special term for the regions
    within the high pressure band, where winds are
    light and variable the horse latitudes
  • Places between the high and low pressure bands,
    on the other hand, experience rapidly moving air,
    and are characterized by strong, dependable winds

45
(Horse latitudes)
46
Winds are named for the direction in which they
originate
47
Storms and fronts
  • Different air masses meet at fronts
  • When warm air meets cold air, the warm air rises
    gently, resulting in mild precipitation

48
Storms and fronts
  • When cold air moves into warm, the warm air rises
    quickly, resulting in LOTS of precipitation

49
Tropical Cyclones (Hurricanes)
  • Tropical cyclones are huge rotating masses of low
    pressure characterized by strong winds and
    torrential rain
  • In North and South America, tropical cyclones are
    commonly called hurricanes
  • In the western North Pacific, they are called
    typhoons
  • In the Indian Ocean, they are called cyclones

50
Tropical Cyclones (Hurricanes)
  • Tropical cyclones carry tremendous amounts of
    heat from one region of the world to another
  • The energy contained in a single hurricane is
    greater than that generated by all energy sources
    in the United States in one year!
  • Hurricanes are powered by the release of waters
    latent heat of condensation (when water
    evaporates, it stores tremendous amounts of heat
    when water condenses into a liquid, it releases
    this stored heat into the surrounding atmosphere)

51
Tropical Cyclones (Hurricanes)
  • The conditions required to form a hurricane are
    as follows
  • Ocean temperature greater than 25C (77F), which
    provides an abundance of water vapor to the
    atmosphere via evaporation (summer and fall)
  • Warm, moist air, which supplies vast amounts of
    heat as the water vapor condenses and fuels the
    storm
  • The Coriolis Effect, which causes the hurricane
    to rotate counterclockwise in the Northern
    Hemisphere, and clockwise in the Southern
    Hemisphere

52
More hurricanes in Northern Hemisphere warmer
weather in tropics there b/c greater amount of
land
53
Tropical Cyclones (Hurricanes)
  • In fact, there are no hurricanes that can occur
    directly over the equator because the Coriolis
    Effect is zero there
  • Hurricanes can not form below 8 N or S latitude
    Coriolis effect is not strong enough to cause
    deflection
  • Hurricane season June 1 Nov 30 97 of
    cyclones (hurricanes) occur during this time

54
Tropical Cyclones (Hurricanes)
  • As air rises (in the northern hemisphere), it is
    deflected to the right
  • This results in a counter-clockwise rotation

Pressure gradient (moving towards the low
pressure center) is represented by blue arrows
the Coriolis deflection is represented by red
arrows
L
http//en.wikipedia.org/wiki/FileHurricane_isabel
_and_coriolis_force.jpg
55
Sinking of air occurs at the eye as dry air moves
in from the atmosphere
EYE
56
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57
The 2005 Hurricane Season
  • The 2005 hurricane season was the most extensive
    on record, and actually persisted into January
    2006!
  • A record 27 tropical storms formed, a record 15
    of which became hurricanes
  • 5 became Category 4
  • 4 became Category 5 (the highest category)
  • 100 billion in damages and gt2000 deaths
  • Coincidentally, 2005 was the hottest year on
    record!

58
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