Wien’s Displacement Law describes the relationship between the temperature of a blackbody and the wavelength at which its emission is most intense. According to the law, the wavelength of peak emission is inversely proportional to the absolute temperature of the blackbody.
This law is used to predict the color of objects based on their temperature, such as the red-hot glow of a heated metal.
The article discusses the laws and fundamental principles of heat transfer through conduction, convection, and radiation. It explains Fourier’s law for conduction, Newton’s law of cooling for convection, and Stefan-Boltzmann, Planck, and Wien’s laws for radiation. Applications span engineering, meteorology, cooking, energy efficiency, and medicine.
We have detected that you are using extensions to block ads. Please support us by disabling these ads blocker.
