Temperature Balances Simplified Revision Notes for GCSE AQA Physics
Revision notes with simplified explanations to understand Temperature Balances quickly and effectively.
Learn about Black Body Radiation for your GCSE Physics Exam. This Revision Note includes a summary of Black Body Radiation for easy recall in your Physics exam
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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.
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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