Curated OER
An Overview of Solar Radiation
Students examine the Stefan-Boltzmann Law. Students compute basic radiative "constants" of the sun-Earth-atomosphere system. They examine the wavelength of maximum radiation emission.
University Corporation for Atmospheric Research
Ucar: Earth's Energy Balance
See how Earth's temperature would change if the Sun's brightness increased or dimmed or if Earth's albedo was different.
Science Struck
Science Struck: Conduction, Convection, and Radiation
Explains the concept of heat transfer and describes conduction, convection, and radiation which are the three modes of heat transfer. Includes formulas, examples, and applications.