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Lesson6b Atmosphere Weather patterns on the Planets
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Lesson6b Atmosphere

Feb 23, 2016

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Lesson6b Atmosphere. Weather patterns on the Planets. Figuring out weather patterns. Here in Kentucky we are moving about 700 MPH, due to the Earth’s rotation on its axis. Which direction is the Earth turning?. - PowerPoint PPT Presentation
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Page 1: Lesson6b Atmosphere

Lesson6b Atmosphere

Weather patterns on the Planets

Page 2: Lesson6b Atmosphere

Figuring out weather patterns.

Page 3: Lesson6b Atmosphere

• Here in Kentucky we are moving about 700 MPH, due to the Earth’s rotation on its axis.

• Which direction is the Earth turning?

Page 4: Lesson6b Atmosphere

• Here in Kentucky we are moving about 700 MPH, due to the Earth’s rotation on its axis.

• Which direction is the Earth turning?

• It turns from west to east. That is why the sun comes up in the east.

Page 5: Lesson6b Atmosphere

Image a trip from Lexington to Rome, Italy and back. Assume no wind on the trip.

Direction of Earth’s Rotation

Page 6: Lesson6b Atmosphere

• How does the Earth’s rotation affect this trip?

• (Remember we are not considering wind effects here. Just imagine a windless day)

Page 7: Lesson6b Atmosphere

.1. The trip to Rome will take

less time than the trip back to Lexington.

2. The trip back from Rome takes less time than the trip to Rome.

3. No effect

Page 8: Lesson6b Atmosphere

• It has no effect.• The plane flight is the same both ways.• The plane before take-off is already moving

700 MPH, due to the Earth’s rotation. When it is flying it is traveling around 500 MPH relative to the ground plus the 700 MPH it had at take off.

• Same thing for the return trip. When the plane is flying back to Lexington, from outer space the plane will appear to be moving 200 MPH to the East. Lexington is approaching at 500 MPH

Page 9: Lesson6b Atmosphere

• Ancient Greeks used this kind of idea to say that the Earth was NOT rotating.

• What happens when you jump in the air?• If you are in the air for one second, here in

Kentucky, the Earth would rotate underneath you at 700 MPH.

• For one second you would land 300 meters to the west. That’s 3 football fields.

Page 10: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

Page 11: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

Page 12: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

Page 13: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

700 MPH

Page 14: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

700 MPH700 MPH

Page 15: Lesson6b Atmosphere

You land in the same spot.

700 MPH

700 MPH

700 MPH

700 MPH700 MPH

Page 16: Lesson6b Atmosphere

Canada launches an attack on the Panama Canal by firing a cannon ball. They aim directly at

Panama.

Page 17: Lesson6b Atmosphere

• Where will the cannonball land?

Page 18: Lesson6b Atmosphere

.

1 2 3

0% 0%0%

1. It should hit the target.2. It will hit West of the target3. It will hit East of the target.

Page 19: Lesson6b Atmosphere

• The first thing we need to consider is the rotation speed of the launch site in Canada.

• Let’s assume the launch site is at a latitude of 55o North.

• We know that everyone on Earth has the same length day, 24 hours. But not everyone is moving at the same speed.

• At the equator the rotational speed is v = Circumference/time v = 24,901 miles/24 hours = 1037 MPH.

Page 20: Lesson6b Atmosphere

• What about the Canadian launch site?

55o

35o

Radius of Earth

Radiu

s of E

arth

Distance to rotation axis

Page 21: Lesson6b Atmosphere

• The radius of the circle that Canada is making is given by:

Sin(θ) = (opposite side)/(hypotenuse) Sin(35o) = (opposite side)/(Radius of the Earth)

Opposite side = (3959 miles)*sin(35o)

radius of circle for Canada = 2,270 miles.

Page 22: Lesson6b Atmosphere

• What about the Canadian launch site?

55o

35o

Radius of Earth

Radiu

s of E

arth

2270 miles

Page 23: Lesson6b Atmosphere

Speed at Canadian launch site

v = (circumference of circle)/length of day v = (2π(2270 miles))/24 hours v = 14,268 miles/ 24 hours v = 594 MPH or about 600 MPH.

Panama is moving at about 1,000 MPH.Now let’s see what this means.

Page 24: Lesson6b Atmosphere

From outer space.• Let’s assume the cannon ball travels 500 MPH

and it was pointed due south.

• So, from outer space the cannon ball has a sideways component.

600 MPH East500 MPH

South

Real Velocity

Page 25: Lesson6b Atmosphere

• This wouldn’t matter if Panama was traveling at 600 MPH also. By the time the cannon ball arrives, Panama would have moved right into the path. BUT Panama is moving at 1,000 MPH.

Missed to the West.

Page 26: Lesson6b Atmosphere

What do we see on Earth?

• We know that Canada isn’t falling behind Panama on the surface of the Earth.

Missed to the West.

Page 27: Lesson6b Atmosphere

Panama returns fire.

• Panama laughs and thinks Canadians are a bad shot. So they aim directly at the launch site and fire due North.

• What will happen?

Page 28: Lesson6b Atmosphere

.

1 2 3

0% 0%0%

1. Panama will miss the target and hit East of it.

2. Panama will miss the target and hit West of it.

3. Panama will hit the target.

Page 29: Lesson6b Atmosphere

What do we see on Earth?

• Panama is traveling 1000 MPH and Canada only 600 MPH.

Missed to the East.

Page 30: Lesson6b Atmosphere

• The curved path that is witnessed on the surface of the Earth makes it look like there is a force pushing the cannon ball off course.

• This is often called the Coriolis “Force”. But there is no force acting on the cannon ball. The path is the result of us on the surface thinking that we are not rotating. It is a perspective issue. From outer space the path makes perfect sense.

• Therefore, the correct name is the Coriolis Effect.

Page 31: Lesson6b Atmosphere

• Note, the faster a planet rotates, the more extreme the Coriolis Effect.

• Coriolis Effect video

Page 32: Lesson6b Atmosphere

Hadley Cell

Motion

Hot air on the

equator, rises and

moves North or South.

Page 33: Lesson6b Atmosphere

Hadley Cell

Motion

When it cools it sinks down and

heads back to

the equator

Page 34: Lesson6b Atmosphere

If we add a little

rotation the wind motion

looks like this.

Page 35: Lesson6b Atmosphere

Venus is rotating very slowly.

Page 36: Lesson6b Atmosphere

Venus is rotating very slowly.

Page 37: Lesson6b Atmosphere

• We would expect that the clouds moving northward from the equator should bend to the East. Instead they are bending to the West.

• What’s up with Venus?

Page 38: Lesson6b Atmosphere

.

1 2 3 4

0% 0%0%0%

1. It is too hot for a Hadley cell to form2. There is no Coriolis Effect on Venus3. Venus is rotating the opposite

direction4. Venus doesn’t have water clouds so

the effect is different

Page 39: Lesson6b Atmosphere

• Venus has just two Hadley cells, one moving North and one moving South.

• But Venus rotates slowly in the opposite direction of the Earth. It actually spins clockwise when viewed from the North Pole.

• This makes the Coriolis Effect reversed on Venus.

Page 40: Lesson6b Atmosphere

On Earth the rotation is

so rapid that the Hadley cell turns

east before it reaches the North

pole.

Page 41: Lesson6b Atmosphere
Page 42: Lesson6b Atmosphere

There are three major cells

• The Hadley Cell, that moves from the Equator• The Polar Cell, that moves from the poles• And the Ferrell Cell, (or mid-latitude cell) that

isn’t really a cell at all. It is the boundary region between the Hadley and Polar cells. This transition region is dominated by either the Hadley or the Polar cells. It is turbulent and has many different weather patterns.

Page 43: Lesson6b Atmosphere

The Ferrel cell

• Many things can happen between the latitudes of 30o and 60o.

• For example, warm air from the south can collide with cold air from the north. The warm air can ride up on top of the cold air. And the two streams will mix and produce turbulence.

• Or one cell can over power the other cell and cause a front to move up into the Ferrel region.

Page 44: Lesson6b Atmosphere

Downward flow of the Hadley cell

• In the region where the Hadley cell sinks, the air pressure is normally high.

• High pressure in a region means that the air tends to flow outward from the region to places where the pressure is lower.

Page 45: Lesson6b Atmosphere

As air sinks into the more dense air near the surface, it takes on the speed of the air in that

region

Earth surface

Equator Northward

Hadley Cell Ferrel CellNorthward

Equator

HIGH PRESSURE

Page 46: Lesson6b Atmosphere
Page 47: Lesson6b Atmosphere

High Pressure region in the Northern Hemisphere.

What will happen as the air leaves this region?

North

Equator

H

Page 48: Lesson6b Atmosphere

.

1 2 3

0% 0%0%

1. The northern air flow will bend east, and the southern flow will bend west.

2. The Northern air flow will bend west and the southern air flow will bend east

3. The air will move straight out of the region.

Page 49: Lesson6b Atmosphere

High Pressure region in the Northern Hemisphere.

Coriolis Effect bends the air flow.

North

Equator

H

Page 50: Lesson6b Atmosphere

High Pressure region in the Northern Hemisphere.

Air circulation is clockwise around a high pressure region.

North

Equator

H

Page 51: Lesson6b Atmosphere

High Pressure region in the Southern Hemisphere.

What will happen as the air leaves this region?

South

Equator

H

Page 52: Lesson6b Atmosphere

High Pressure region in the Southern Hemisphere.

Rotation is counter-clockwise for high pressure.

South

Equator

H

Page 53: Lesson6b Atmosphere

High Pressure regions

• High pressure regions on Earth are fair weather regions.

• In order to form clouds, air currents must raise up to altitudes where water vapor turns into water droplets and forms clouds.

• High pressure stops the ability for these type of air currents to form.

• The result is sunny weather.

Page 54: Lesson6b Atmosphere

Regions of low pressure in the Northern Hemisphere.

• When a region develops where the air pressure is lower than in surrounding regions the air flow is into the low pressure region.

Equator

L

North

Page 55: Lesson6b Atmosphere

• What about low pressure in the Northern Hemisphere?

Page 56: Lesson6b Atmosphere

.

1 2 3

0% 0%0%

1. The southern air flow will bend west and the northern flow east.

2. The southern air flow will bend east and the northern flow west.

3. The air will flow directly in, collide and make a storm.

Page 57: Lesson6b Atmosphere

In Northern Hemisphere, low pressure systems rotate counter-clockwise.

L

Equator

North

Page 58: Lesson6b Atmosphere

Low Pressure Systems

• In the Southern Hemisphere, lows rotate clockwise.

• Low pressure means that air is flowing into the region and can develop air currents that move upwards, where the air is cooler.

• When this happens, water vapor condenses to from droplets and clouds form

Page 59: Lesson6b Atmosphere

Hurricane

Page 60: Lesson6b Atmosphere

Jupiter

Page 61: Lesson6b Atmosphere

Jupiter