Читать книгу Materials for Solar Energy Conversion - Группа авторов - Страница 21

1.5 Basic Laws of Radiation 1.5.1 Stefan-Boltzmann Law

Оглавление

The Stefan-Boltzmann law is as the emissive power of a black body that is directly proportional to fourth power of its absolute temperature.


where Eb - Black body emissive power (W/m2)

σ - Stefan Boltzmann constant—5.67 × 10–8 W/m2 K4

T - Absolute temperature (K)

Materials for Solar Energy Conversion

Подняться наверх