Part 1: The Planetary Energy Budget
Earth's climate is governed by a simple thermodynamic balance: energy in must equal energy out. Sunlight arrives as high-energy visible light; Earth must radiate an equal amount of energy back out into cold space as low-energy infrared heat.
- Shortwave Solar Radiation vs Longwave Outgoing Terrestrial Infrared
- Blackbody Radiation (Stefan-Boltzmann Law)
- Radiative Forcing (imbalance between incoming sunlight and outgoing heat, measured in W/m²)