GGR100H1 Lecture : Earth's energy balance

41 views2 pages
3 Mar 2011
School
Department
Course
Professor

Document Summary

Earth"s energy balance the sun emits radiation in a spectrum- uv, infared, etc. different gasses absorb different types of radiation clouds have the property of reflecting radiation to space- wave hits the cloud and bounces back up to space, doesn"t change wavelength, just reflects back. Fate of incoming solar radiation (short wave) scattering: gas molecules and dust change direction of radiation without altering wavelength-> diffuse radiation reflection: bounce back to space. which is why a cloudy day still allows daylight to be seen. we reflect 31% of the radiation [known as albedo] absorption: assimilation of radiation by molecules of matter, converted into other forms of energy. earth is pretty bright in space because we are reflecting 31% the moon reflects 6% Aerosols tiny droplets that reflect radiation they are small particles that exist in the atompshere. we produce a lot of aerosols in our industrial activities.

Get access

Grade+20% off
$8 USD/m$10 USD/m
Billed $96 USD annually
Grade+
Homework Help
Study Guides
Textbook Solutions
Class Notes
Textbook Notes
Booster Class
40 Verified Answers
Class+
$8 USD/m
Billed $96 USD annually
Class+
Homework Help
Study Guides
Textbook Solutions
Class Notes
Textbook Notes
Booster Class
30 Verified Answers

Related Documents

Related Questions