File:NASA Earth radiation thermal balance energy budget atmosphere.jpg

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NASA_Earth_radiation_thermal_balance_energy_budget_atmosphere.jpg(720 × 507 pixels, file size: 86 KB, MIME type: image/jpeg)

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English: The atmosphere radiates the equivalent of 59% of incoming sunlight back to space as thermal infrared energy, or heat. Where does the atmosphere get its energy? The atmosphere directly absorbs about 23% of incoming sunlight, and the remaining energy is transferred from the Earth’s surface by evaporation (25%), convection (5%), and thermal infrared radiation (a net of 5-6%). The remaining thermal infrared energy from the surface (12%) passes through the atmosphere and escapes to space. (NASA illustration by Robert Simmon. Astronaut photograph ISS017-E-13859.) See also NASA Earth’s Energy Budget and The NASA Earth's Energy Budget Poster
Source http://earthobservatory.nasa.gov/Features/EnergyBalance/page6.php
Author NASA Earth Observatory

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Public domain This file is in the public domain in the United States because it was solely created by NASA. NASA copyright policy states that "NASA material is not protected by copyright unless noted". (See Template:PD-USGov, NASA copyright policy page or JPL Image Use Policy.)
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current14:54, 20 April 2014Thumbnail for version as of 14:54, 20 April 2014720 × 507 (86 KB)Prokaryotes (talk | contribs){{subst:Upload marker added by en.wp UW}} {{Information |Description = {{en|Just as the major atmospheric gases (oxygen and nitrogen) are transparent to incoming sunlight, they are also transparent to outgoing thermal infrared. However, water vapor, ca...

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