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Temperature Balances Simplified Revision Notes

Revision notes with simplified explanations to understand Temperature Balances quickly and effectively.

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6.4.2 Temperature Balances

Earth (Physics only)

  • Sun's Energy:
    • Sun's energy is mostly absorbed by the earth's atmosphere, and some is reflected.
    • The amount of energy re-radiated and absorbed leads to Earth's temperature.
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The Greenhouse Effect

  • Solar Radiation:
    • 343 Watts per m² from the sun.
    • Some of the solar radiation is reflected by the atmosphere and the Earth's surface.
    • Some of the infrared radiation passes through the atmosphere and out into space.
    • Outgoing solar radiation: 103 Watts per m².
    • Outgoing infrared radiation: 240 Watts per m².
  • Absorption:
    • About half the solar radiation is absorbed by the Earth's surface.
    • Radiation is converted to heat energy, causing the emission of longwave (infrared) radiation back into the atmosphere.
  • Atmospheric Interaction:
    • Some of the infrared radiation is absorbed and re-emitted by the greenhouse gas molecules.
    • The atmosphere is responsible for keeping the Earth at a constant temperature by absorbing IR radiation from the sun and trapping IR re-radiated from the Earth.
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