Ch. 8 Equations Flashcards
Power radiated by a grey body (Stefan-Boltzmann law)
Note: For a black body, e = 1.
Albedo (of planet)
Total scattered power/total incident power
Emissivity
power per unit area radiated by object / power per unit area radiated by a black body at the same temperature
Intensity*
Power/area
Specific energy (of fuel)
Energy per unit mass
Energy density (of fuel)
Energy per unit volume
Maximum power generated by wind turbine
P = 1/2ρAv^3
Power generated by hydroelectric power station
P = mgΔh/Δt or (ρV/Δt)gΔh
Wavelength of peak radiation emission of a black body
Wavelength (metres) = (2.90 * 10^-3)/T (Kelvin)
Emissivity (definition)
The ratio of the power per unit area radiated by a body to the power per unit area radiated by a black body at the same temperature.