Average Clear-sky Outgoing Longwave Flux (WMS)
The Earth's climate is determined by energy transfer from the sun to the Earth's land, oceans, and atmosphere. As the Earth rotates, the sun lights up only part of the Earth at a time, and some of that incoming solar energy is reflected and some is absorbed, depending on type of area it lights. The average amount of reflection and absorption is critical to the climate, because the absorbed energy heats up the Earth until it is radiated away as thermal radiation. This animation shows the monthly average clear-sky outgoing longwave radiation from July, 2002 through June, 2004 as measured by the CERES instrument. This is the thermal radiation given off by the warm Earth when the sky is cloud free. The Earth's rotation and the movement of warm air from the equator to the poles make the Earth roughly uniformin temperature. The most visible features are the cold poles in winter and the significant regions of snow coverage in the northern hemisphere, also in winter.
This animation shows the monthly average clear-sky outgoing
longwave flux from CERES for July 2002 through June 2004.
This product is available through our Web Map Service.
This is the legend for the clear-sky outgoing longwave flux
animation, indicating the magnitude of the energy flux.
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Credits
Please give credit for this item to:
NASA/Goddard Space Flight Center
Scientific Visualization Studio
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Animators
- Horace Mitchell (NASA/GSFC)
- Eric Sokolowsky (Global Science and Technology, Inc.)
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Scientist
- Bruce A. Wielicki (NASA/LaRC)
Release date
This page was originally published on Tuesday, February 1, 2005.
This page was last updated on Wednesday, May 3, 2023 at 1:56 PM EDT.
Series
This page can be found in the following series:Datasets used
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Outgoing Longwave Radiation Flux [Aqua: CERES]
ID: 247
Note: While we identify the data sets used on this page, we do not store any further details, nor the data sets themselves on our site.