3.4.1 Black-Body Radiation скачать в хорошем качестве

3.4.1 Black-Body Radiation

This video introduces the concept of black-body readiation. An ideal black body absorbs all incident radiation and has a temperature-dependent radiation emission. The power on the surface for black-body radiation at a given temperature is given by the Planck distribution. The video considers the formulas for the spectral irradiance as a function of frequency and wavelength and converts the two. This video is a prerequesite for understanding the Shockley-Queisser efficiency limit of solar cells. Therefore, the calculation results are presented for the radiation of the sun and the earth. This video is part of a course offered at Kiel University for advanced engineering bachelor students. Additional videos and exercise material are available in the course "Renewable Energy" on the Digital Learning Campus platform dlc.sh : https://dlc.sh/lernangebot/728 DLC registration is free of charge not only for students already registered at Kiel University, but also for prospective students who want to get to know Kiel University and consider transferring to Kiel University.