Solar Radiation and Blackbody Emission

In course

Dolore consequat ut commodo voluptate dolor tempor nostrud esse cillum labore. Esse consectetur nulla sint commodo laboris eiusmod. Est ea velit enim id adipisicing amet cillum enim dolor ut pariatur laboris ipsum. Ex do officia et pariatur irure elit excepteur excepteur qui qui amet fugiat ut. Consectetur elit sunt excepteur culpa labore esse. Duis proident aliquip ipsum occaecat commodo non elit cillum reprehenderit est ex.

Description

This lecture covers the resolution of exercise 3 related to the solar radiation and blackbody emission. It discusses the intensity of solar radiation at ground level, the temperature of the ground, the emission intensity by the ground, the addition of a glass pane between the ground and the observer, and the calculation of temperatures using Stefan-Boltzmann's law.

Instructor

non ad aute

Cupidatat reprehenderit non commodo non consectetur eiusmod ipsum amet mollit non sint ex nisi dolore. Duis cillum ut incididunt ut in exercitation nisi cillum voluptate incididunt anim ullamco. Ex do anim veniam eiusmod dolore velit. Aute id Lorem qui dolor labore aute consectetur. Consequat veniam Lorem velit occaecat. Sint nulla Lorem incididunt laborum reprehenderit laboris ut do irure.

Official source

https://mediaspace.epfl.ch/media/0_p7lw755t

About this result

This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.

Ontological neighbourhood

Physics

Electromagnetism: Electromagnetic radiation

Related lectures (35)