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10'2 Energy Transfer in the Atmosphere

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Exosphere: The layers of Earth's atmosphere. See pages 438 - 439 (c) McGraw ... Exosphere: 500 km to 700 km above Earth. Atmosphere merges with outer space. ... – PowerPoint PPT presentation

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Title: 10'2 Energy Transfer in the Atmosphere


1
10.2 Energy Transfer in the Atmosphere
  • Earths atmosphere is key in allowing life to
    survive
  • Has the right ingredients and maintains the
    correct temperature

The composition of Earths atmosphere
See pages 436 - 437
2
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3
The Layers of the Atmosphere
  • Earths atmosphere is made up of five layers.
  • Troposphere
  • Closest to Earths surface, 8 km to 16 km thick
  • Highest density - all other layers compress it
  • Almost all water vapour in the atmosphere is
    found here.
  • Where most weather takes place
  • Solar energy and thermal energy from Earth keep
    air moving
  • Radiation from the sun heats the earth
  • 15ºC (near the ground) to 55ºC at the top

See pages 438 - 439
4
The Layers of the Atmosphere
  • Earths atmosphere is made up of five layers.
  • Stratosphere
  • Second layer (10 km to 50 km above Earth)
  • Ozone layer is found here
  • Absorbs harmful UV radiation
  • Absorbs more UV at the top, therefore..
  • Temperature warms from 55ºC as altitude increases

See pages 438 - 439
5
The Layers of the Atmosphere
  • The remaining three layers are known as the upper
    atmosphere.
  • Mesosphere
  • Thermosphere
  • Exosphere

See pages 438 - 439
The layers of Earths atmosphere
6
The Layers of the Atmosphere
  • The remaining three layers are known as the upper
    atmosphere.
  • Mesosphere
  • 50 km to 80 km above Earth
  • Temperatures decrease with altitude to 100ºC
  • No ozone to absorb UV
  • This layer is where space debris (dust, meteors)
    burns up when it begins to hit particles.

See pages 438 - 439
The layers of Earths atmosphere
7
The Layers of the Atmosphere
  • The remaining three layers are known as the upper
    atmosphere.
  • Thermosphere
  • 80 km to 500 km above Earth
  • Temperatures can reach 1500ºC to 3000ºC
  • Trace O2 absorbs solar radiation
  • This is where the Northern Lights, aurora
    borealis, are found.
  • Charged particles in Earths magnetic field
    collide with particles in the thermosphere.

See pages 438 - 439
The layers of Earths atmosphere
8
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9
The Layers of the Atmosphere
  • The remaining three layers are known as the upper
    atmosphere.
  • Exosphere
  • 500 km to 700 km above Earth
  • Atmosphere merges with outer space.

See pages 438 - 439
The layers of Earths atmosphere
10
Radiation and Conduction in the Atmosphere
  • Almost all of the thermal energy on Earth comes
    from the Sun.
  • Only a small fraction of the solar radiation that
    reaches Earth.
  • Most thermal energy is transferred near the
    equator
  • Direct source of solar radiation
  • Insolation
  • Amount of solar radiation an area receives (
    W/m2)
  • Decreases if
  • Dust and smoke in the way
  • Angle of incidence of the solar radiation is too
    great.

Angle of incidence
See pages 440 - 441
11
Radiation and Conduction in the Atmosphere
  • Solar radiation does NOT heat the atmosphere
    directly
  • Earths surface absorbs radiation, heats up, then
  • radiates the thermal energy into the atmosphere.
  • Provides 70 of the airs thermal energy
  • Convection currents in the air spread thermal
    energy
  • (See Figure 10.19 on Page 441)

See pages 440 - 441
12
The Radiation Budget and Albedo
  • Radiation budget
  • Explains where the solar radiation goes
  • Earths radiation budget heat gained heat
    lost
  • Incoming Outgoing radiation balanced
  • If all 342 W/m2 of solar radiation that reaches
    Earth was stored in the atmosphere, it would be
    far too hot

13
The Radiation Budget and Albedo
  • Radiation budget
  • Earths radiation budget heat gained heat
    lost
  • Of the solar radiation that goes towards Earth
  • 58 reaches Earths surface
  • 9 reflected by surface
  • Reflected
  • 15 by clouds
  • 7 by particles
  • Absorbed
  • 20 is absorbed by clouds
  • and the atmosphere
  • Radiation that comes to Earth
  • 23 drives the water cycle
  • 7 creates wind
  • 19 re-radiated from Earths surface

14
The Radiation Budget and Albedo
  • Albedo - amount of energy reflected by a surface.
  • Light-coloured surfaces (snow, sand) have a high
    albedo and reflect energy.
  • Dark-coloured surfaces (soil, water) have a low
    albedo and absorb energy.

See pages 442 - 443
15
Prevailing Winds
  • Prevailing winds - winds that are typical for a
    location
  • Winds in B.C. usually blow in from the ocean.
  • Warm air rises, cools and condenses ? causing
    rain as it is forced up the mountain slopes
  • Air gets drier as it moves inland, continuing to
    drop precipitation.
  • Dry air rushes down the far side of the mountains
    into the prairies.

See pages 448 - 449
The prevailing winds off British Columbias
coast, crossing into Alberta.
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