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The course uses a simplified model of Earth without an atmosphere to calculate its surface temperature. It introduces electromagnetic waves, energy, intensity, blackbody radiation, and the Stefan-Boltzmann law.
Syllabus
- Intro to electromagnetic waves
- Energy and Power
- Intensity
- Blackbody radiation
- Stefan-Boltzman
- Power into the Earth
- Power out of Earth
- Temperature
Taught by
Dot Physics