Lecture 7
- October 17
- Radiation or What We Get From the Sun
- Solar energy warms the earth and powers life through photosynthesis
- Energy radiates from the sun as electromagnetic waves
- waves, frequency, wavelength
- electromagnetic spectrum
- visible spectrum
- 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
- Spectrum of solar radiation
- peak wavelength appropriate for electronic excitation
- 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
Back to Sci 010 home page.
.../010lec7.html
Modified: 17/10/1995
by goddyn@sfu.ca (Luis Goddyn)