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The Processes That Produce the Wind

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Title: The Processes That Produce the Wind


1
The Processes That Produce the Wind
2
Wind
  • Wind is the general term for the movement of
    air.
  • Air moves in three dimensions, but meteorologists
    often separate the motion into the horizontal
    wind and the vertical motion.
  • Our understanding of the movement of air is based
    on Newtons Laws of Motion.

3
First Law of Motion
  • Newtons First Law of Motion states that an
    object at rest will remain at rest and an object
    in motion will remain in motion and travel in a
    straight line at a constant speed unless a force
    is exerted on the object.

4
Newtons First Law of Motion (Cont.)
remains at rest
Force
change of direction
travels in a straight line at a constant speed
5
Newtons Second Law of Motion
  • Newtons Second Law of Motion states that the
    rate of change of momentum of an object with time
    is equal to the sum of the forces acting on the
    object.
  • Newton defined momentum as the mass multiplied
    times the velocity.

6
Newtons Second Law of Motion (Cont.)
  • The equation for Newtons Second Law of Motion is
  • d(mV)/dt Force 1 Force 2 Force 3
  • where
  • m is the mass of the object
  • V is the velocity of the object
  • dt is the change of time

7
Newtons Second Law of Motion (Cont.)
  • If we assume our object is an air parcel and that
    the mass of the air parcel remains constant, then
    we can pull m out of the derivative and write
  • m(dV/dt) Force 1 Force 2 Force 3
  • or if we divide both sides by m we get

8
Newtons Second Law of Motion (Cont.)
  • dV/dt Force 1/m Force 2/m Force 3/m

9
Vertical Motion
  • As we discussed earlier in the course, vertical
    motion is the result of differences between the
    upward directed pressure gradient force and the
    downward directed gravitational force.
  • When the two forces are equal we have the
    hydrostatic balance.

10
Horizontal Motion
  • In the lowest 100 km of the Earths atmosphere,
    horizontal motion is the result of three factors
  • the pressure gradient force
  • the Coriolis effect and
  • the frictional force

11
The Pressure Gradient Force
  • The pressure gradient is defined as the change in
    pressure between two points divided by the
    distance between the two points.
  • Since pressure is force divided by area, the
    difference in pressure is directly related to a
    difference in force.

12
Pressure Gradient
p 1.03x105 Pa (1030 mb)
p 1.00x105 Pa (1000 mb)
106 m
pressure gradient (1.03x105 Pa 1.00x105
Pa)/106 m pressure gradient 0.003 Pa/m
13
Pressure Gradient
More force
less force
p 1.03x105 Pa (1030 mb)
p 1.00x105 Pa (1000 mb)
106 m
The imbalance of forces accelerates the air
parcel from the higher toward the lower pressure.
14
Pressure Gradient Force
  • Suppose we look at the pressure gradient force in
    the x-direction.

y
dx
p dp
p
x
15
Pressure Gradient Force (Cont.)
  • The pressure pushing the parcel in the positive
    x-direction is p.
  • The pressure pushing the parcel in the negative
    x-direction is pdp.
  • The distance between the two sides of the parcel
    is dx.
  • Lets assume our air parcel is a cube and the
    area of each face is A.

16
Pressure Gradient Force (Cont.)
  • In this case the pressure gradient force pushing
    the parcel in the positive x-direction is pA and
    the pressure gradient force pushing the parcel in
    the negative x-direction is (pdp)A.

17
Pressure Gradient Force (Cont.)
  • The net pressure gradient force on the parcel in
    the x-direction is the difference between these
    two forces
  • pA (pdp)A
  • or
  • pA pA dpA -dp A

18
Pressure Gradient Force (Cont.)
  • The volume of the air parcel would be
  • V Adx
  • So,
  • A V/dx

19
Pressure Gradient Force (Cont.)
  • If we substitute into our earlier expression we
    get
  • - dp A - V (dp/dx)
  • This would give us the next pressure gradient
    force in the x-direction.

20
Pressure Gradient Force (Cont.)
  • In our form of Newtons Second Law of Motion, we
    divided the forces by the mass.
  • So, if we divide the pressure gradient force by
    the mass we get
  • (-V/m)(dp/dx)

21
Pressure Gradient Force (Cont.)
  • Now,
  • volume/mass 1/density specific volume
  • V/m 1/? a
  • So,
  • - (V/m)(dp/dx) - (1/?)(dp/dx)
  • or - a(dp/dx)
  • which gives the acceleration caused by the
    pressure gradient force acting in the x-direction.

22
Pressure Gradient Force (Cont.)
  • The strength of the pressure gradient force is
    determined by the pressure difference.
  • A large pressure difference creates a large force
    and usually produces higher wind speeds.
  • A smaller pressure difference creates a smaller
    force and usually produces lighter winds.

23
Isobar Analysis
  • Meteorologist evaluate the pressure gradient
    force and locate centers of higher and lower
    pressure on surface weather maps by drawing
    isobars.
  • An isobar is a curve connecting points that have
    the same pressure.

24
Isobar Analysis of the Surface Map
  • Perhaps the most fundamental synoptic analysis is
    the drawing of isobars on a surface weather map.
  • An isobar is a curve connecting places that have
    the same pressure. On the surface synoptic map
    isobars connect places that have the same sea
    level pressure,

25
Isobar Analysis (cont.)
  • On a surface weather map the standard practice is
    to draw isobars at an interval of 4 hPa (4 mb)
    beginning with 1000 hPa (1000 mb) or the closest
    appropriate isobar.
  • In cases where the pressure gradients are weak
    supplemental isobars are drawn every 2 hPa (2 mb).

26
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27
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28
Getting Started
  • First, locate all of the places on the map where
    the sea level pressure is 1000 hPa (mb) and draw
    an X at those locations.

29
X
X
X
X
X
X
X
X
X
X
X
X
X
X
X
30
The 1000 hPa (mb) Isobar
  • Now draw a curve connecting all of the Xs. You
    have just drawn the 1000 hPa (mb). isobar.
  • Repeat the process by going up and down at a 4
    hPa interval until you have drawn all of the
    isobars.

31
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32
Local Wind Systems
  • Several local wind systems are the direct result
    of the pressure gradient force.
  • sea/land (lake/shore) breezes
  • anabatic/katabatic winds

33
Sea (lake) Breeze
  • Recall that water has a higher specific heat than
    the land surface.
  • Thus, water surfaces warm and cool more slowly
    than land.
  • On a sunny day the water will typically be cooler
    than the land surface.

34
Sea (lake) Breeze (Cont.)
Sunny Day
The pressure gradient force pushes a cooler sea
(lake) breeze toward land.
Lower pressure
Higher pressure
Water surface is cooler
Land surface is warmer
35
Land (shore) Breeze
Night
The pressure gradient force pushes a cooler land
(shore) breeze toward land.
Higher pressure
Lower pressure
Water surface is warmer
Land surface is cooler
36
Mountain and Valley Winds
  • Differential heating and cooling can also produce
    local winds in mountainous regions.

37
Anabatic Winds
  • During the daytime the higher parts of mountains
    warm more quickly than the valleys because they
    receive more solar radiation.
  • The warming of the higher elevations produces
    flows up the slopes called anabatic winds.

38
Anabatic Winds (Cont.)
Warmer, lower pressure
Warmer, lower pressure
Anabatic winds up the slopes
Cooler, higher pressure
39
Katabatic Winds
  • At night the tops of the mountains cool off much
    more quickly because they emit more terrestrial
    radiation down to space.
  • The cooler denser air is affected more by the
    gravitational force and flows down the slope
    creating katabatic winds.

40
Anabatic Winds (Cont.)
Cooler, denser air
Cooler, denser air
Katabatic winds drain down the slopes at night.
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