Lecture 7

October 17
Radiation or What We Get From the Sun
  1. Solar energy warms the earth and powers life through photosynthesis
  2. Energy radiates from the sun as electromagnetic waves
    • waves, frequency, wavelength
    • electromagnetic spectrum
    • visible spectrum
  3. Bodies of different temperature radiate energy of different wavelengths
    • demo - temperature of body varies as color changes
    • model system - black body
      • black body absorbs and emits electromanetic radiation without favouring a particular wavelength
      • peak wavelength is inversely proportional to temperature
      • energy emitted increases as temperture to the power of 4
    • form of spectrum is characteristic
      • description of form requires quantum picture of em radiation
  4. Spectrum of solar radiation
    • peak wavelength appropriate for electronic excitation
      • photosynthesis - Ron
  5. Earth's temperature
    • absorbtion of solar energy
    • reflectance of solar energy - albedo
    • emission of radiation from earth
    • greenhouse effect
      • why water and CO2 absorb short wavelength radiation - Derek
    • demo - greenhouse effect

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Modified: 17/10/1995 by goddyn@sfu.ca (Luis Goddyn)