Atmosphere structure, Solar Inputs and the Transport of Heat.

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Atmosphere structure, Solar Inputs and the Transport of Heat
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Transcript of Atmosphere structure, Solar Inputs and the Transport of Heat.

Page 1: Atmosphere structure, Solar Inputs and the Transport of Heat.

Atmosphere structure, Solar Inputs and the Transport of Heat

Page 2: Atmosphere structure, Solar Inputs and the Transport of Heat.

Heat, winds, and currents

We will address the following topics....

• Why do the winds blow?The source of the winds is ultimately the Sun. We’ll discuss how heating by the Sun generates air flow.

• What influence does the Earth’s rotation have on winds?Earth’s rotation causes the winds and currents to turn…without this rotation the climate would be very different.

Solar Insolation controls almost everything: But it is not just what we get, it is what we keep that defines the thermal balances.

Page 3: Atmosphere structure, Solar Inputs and the Transport of Heat.

Structure of the Modern Atmosphere

• Pressure: force exerted per unit area by the weight of overlying air (1 mb = 100 Pa; 1000 mb ~ 1bar ~1 atm)

• Temperature: measure of the molecular kinetic energy.

Page 4: Atmosphere structure, Solar Inputs and the Transport of Heat.

Thermosphere

Thermosphere: upper atmospheric layer with temperature increasing with altitude

• Heated by absorption of high-energy radiation by oxygen• Atmosphere is extremely thin, nearly a vacuum. As a result,

Sun’s energy can heat air molecules to very high temperatures (2500 °C) during the day. But there are so few, it doesn’t reallymatter Auroras occur in thermosphere

Page 5: Atmosphere structure, Solar Inputs and the Transport of Heat.

Mesosphere

• Temperatures as low as -100 C

• Million of meteors burn up daily in the mesosphere, due to collision with air molecules

Mesosphere: middle atmospheric layers where temperature decreases with altitude

Noctilucent clouds (blue-white) over Finland.

Page 6: Atmosphere structure, Solar Inputs and the Transport of Heat.

Stratosphere

• Ozone is concentrated around an altitude of 25 km in the “ozone layer”

• Ozone layer protects surface from harmful UV radiation

Stratosphere: temperature increases with altitude due to absorption of UV by ozone

Page 7: Atmosphere structure, Solar Inputs and the Transport of Heat.

Troposphere

• Temperature determined by surface heating

• Well mixed by weather

Troposphere: lowest layer in atmosphere, temperature decreases with altitude

Page 8: Atmosphere structure, Solar Inputs and the Transport of Heat.

ANNUAL

Shortwave radiation• Earth receives more solar radiation at low latitudes than high

latitudes.• Ultimately, it is this solar insolation that provides the heat

that controls weather and climate. It is the imbalance across the Earth’s surface that controls winds and currents.

Page 9: Atmosphere structure, Solar Inputs and the Transport of Heat.

Shortwave radiation

• Beam spreading: each unit of shortwave radiation is spread over a larger area away from the equator

3 factors influence the shortwave radiation received at Earth’s surface

Page 10: Atmosphere structure, Solar Inputs and the Transport of Heat.

Shortwave radiation

• Beam spreading: each unit of shortwave radiation is spread over a larger area away from the equator

• Beam depletion: radiation is absorbed and reflected as it passes through atmosphere

3 factors influence the shortwave radiation received at Earth’s surface

Page 11: Atmosphere structure, Solar Inputs and the Transport of Heat.

Shortwave radiation

• Beam spreading: each unit of shortwave radiation is spread over a larger area away from the equator

• Beam depletion: radiation is absorbed and reflected as it passes through atmosphere

• Day length: hours of daylight varies with latitude and season

3 factors influence the shortwave radiation received at Earth’s surface

Page 12: Atmosphere structure, Solar Inputs and the Transport of Heat.

No tilt Tilted

Shortwave radiation

Earth has seasons because its axis is tilted 23.5º with respect to the plane of the ecliptic

Page 13: Atmosphere structure, Solar Inputs and the Transport of Heat.

Why do we have seasons?

Seasonal variations in insolation are greatest at high latitudes

Page 14: Atmosphere structure, Solar Inputs and the Transport of Heat.

Dec-Jan-Feb. Jun-Jul-Aug

Shortwave radiation

Earth receives more solar radiation at low latitudes than high latitudes

Page 15: Atmosphere structure, Solar Inputs and the Transport of Heat.

Longwave radiation

Earth emits more longwave radiation at low latitudes than high latitudes

Page 16: Atmosphere structure, Solar Inputs and the Transport of Heat.

Dec-Jan-Feb. Jun-Jul-Aug

Longwave radiation

Earth emits more longwave radiation at low latitudes than high latitudes

Why is there a difference between Winter and Summer?

Page 17: Atmosphere structure, Solar Inputs and the Transport of Heat.

Net radiation

Net radiation: total radiation• Net radiation: shortwave - longwave• There is an energy imbalance!

Page 18: Atmosphere structure, Solar Inputs and the Transport of Heat.

Global Energy Balance

Page 19: Atmosphere structure, Solar Inputs and the Transport of Heat.

Global Energy Balance

Page 20: Atmosphere structure, Solar Inputs and the Transport of Heat.

Global Energy Balance

Page 21: Atmosphere structure, Solar Inputs and the Transport of Heat.

Global Energy Balance

Page 22: Atmosphere structure, Solar Inputs and the Transport of Heat.

• To make the energy balance, there must be a transport of energy from low to high latitudes.

• Radiation is converted to other forms of energy that can be transported by winds and currents

• Sensible heat: heat that you can feel (stored in a substance as a change in temperature)

• Latent heat: heat required to changes phases (solid --> liquid --> gas)

Energy Transport

Page 23: Atmosphere structure, Solar Inputs and the Transport of Heat.

Newton’s first law: A body at rest remains at rest and a body in motion remains in constant motion unless acted upon by an external force

Fluid Flow

• Fluid flow is driven by forces

• Forces include- Pressure- Coriolis- Friction

Page 24: Atmosphere structure, Solar Inputs and the Transport of Heat.

• Pressure gradient force: fluid flows from high pressure to low pressure

Fluid Flow

Pressure: force exerted against a surface due to the weight of air

Page 25: Atmosphere structure, Solar Inputs and the Transport of Heat.

Fluid Flow

• Pressure gradient force: fluid flows from high pressure to low pressure

- Flow in direction from H to L- Larger gradient = faster flow

Pressure: force exerted against a surface due to the weight of air

Page 26: Atmosphere structure, Solar Inputs and the Transport of Heat.

Heating air causes it to expand

In this example, the masses ofthe 2 air columns, A and B, are equal

Equal masses of air

SURFACE

HOTCOLD

A B

Pressure DifferencesPressure differences arise from temperature differences.

Page 27: Atmosphere structure, Solar Inputs and the Transport of Heat.

SURFACE

HOTCOLD

Top of Atmos.

COLD COLD

The mass of air overlying column A is greater than that overlying column B

> mass< mass

A B

Pressure DifferencesPressure differences arise from temperature differences.

Page 28: Atmosphere structure, Solar Inputs and the Transport of Heat.

HOTCOLD

COLD COLD

BONUS!

HIGH LOW

Because the massis greater in column A, the surfacepressure (i.e., the weightof the overlying air) isgreater.

Top of Atmos.A B

Pressure DifferencesPressure differences arise from temperature differences.

Page 29: Atmosphere structure, Solar Inputs and the Transport of Heat.

Pressure DifferencesPressure differences arise from temperature differences.

Page 30: Atmosphere structure, Solar Inputs and the Transport of Heat.

General Circulation of the Atmosphere

Circulation on a non-rotating Earth

Page 31: Atmosphere structure, Solar Inputs and the Transport of Heat.

Coriolis force is an artificial forcethat arises because we are ridingon a rotating rock.

Fluid Flow

Coriolis force: an apparent deflection of moving objects when observed from a rotating reference frame

Page 32: Atmosphere structure, Solar Inputs and the Transport of Heat.

Consider two children throwinga ball on a moving merry-go-round.

Stationary Observer’s Perspective

Rotating Observer’s Perspective

Fluid Flow

Coriolis force: an apparent deflection of moving objects when observed from a rotating reference frame

Page 33: Atmosphere structure, Solar Inputs and the Transport of Heat.

The stationary observer sees the ball moving in a straight line, and Johnny and Jill moving in a circle.

Stationary observer

Fluid Flow

Coriolis force: an apparent deflection of moving objects when observed from a rotating reference frame

Page 34: Atmosphere structure, Solar Inputs and the Transport of Heat.

Johnny and Jill on the merry-go-round perceive that they arestationary. They see the ballmove to the right.

Moving observer

Fluid Flow

Coriolis force: an apparent deflection of moving objects when observed from a rotating reference frame

Page 35: Atmosphere structure, Solar Inputs and the Transport of Heat.

Fluid Flow

Coriolis force: an apparent deflection of moving objects when observed from a rotating reference frame

http://ww2010.atmos.uiuc.edu/(Gh)/guides/mtr/fw/crls.rxml

Page 36: Atmosphere structure, Solar Inputs and the Transport of Heat.

General Circulation of the Atmosphere

• Trade winds• Mid-latitude westerlies• Polar easterlies

Circulation on a rotating Earth

Page 37: Atmosphere structure, Solar Inputs and the Transport of Heat.
Page 38: Atmosphere structure, Solar Inputs and the Transport of Heat.

DESERTS – THE CONVERGENCE OF ATMOSPHERIC CIRCULATION CELLS AND THE SURFACE OF THE EARTH

Page 39: Atmosphere structure, Solar Inputs and the Transport of Heat.

Net radiation

Net radiation: total radiation• Net radiation: shortwave - longwave• There is an energy imbalance! • Cold Poles and Hot Tropics – the drive for circulation in both

the atmosphere and the ocean systems

Page 40: Atmosphere structure, Solar Inputs and the Transport of Heat.

Circulation of the OceanThermohaline Driving Mechanism

Page 41: Atmosphere structure, Solar Inputs and the Transport of Heat.

THE ATLANTIC GULF STREAMWARMING THE POLES – COOLING THE TROPICS

Page 42: Atmosphere structure, Solar Inputs and the Transport of Heat.

MAJOR OCEAN CURRENT SYSTEMS

Page 43: Atmosphere structure, Solar Inputs and the Transport of Heat.

GLOBAL SCALE CIRCULATION OF OCEANS – A THERMAL TRANSFER.

Page 44: Atmosphere structure, Solar Inputs and the Transport of Heat.

SURFACE TEMPERATURE ANOMOLIES