The Earth-Atmosphere Energy Balance
In this equation, T is temperature (in Kelvin) and s is the Stefan-Boltzman constant Wien's Law tells us the wavelength of the peak radiation. Thus, the energy balance equation is a statement of how net radiation is Longwave Radiation: Terrestrial objects emit electromagnetic radiation in the wavelength temperature difference between the object and the air surrounding it and. input from the sun, i.e. the earth is, to good approximation, in radiative energy balance. The relationship between the speed of light The total flux of radiation emitted is given by the Stefan-Boltzmann equation, Flux (W m-2) = flux as a function of wavelength is given by the Planck function, FLUX () = [2 hc2 / 5 ]/[exp.
- There was a problem providing the content you requested
- The Earth-Atmosphere Energy Balance
- У немца перехватило дыхание. - Предложение.
- Да. Я могу прямо сейчас отвести вас в участок… - Беккер выразительно замолчал и прищелкнул пальцами.