Average Total-Sky Outgoing Longwave Flux

Images & Animations

  • Credit

    NASA/Goddard Space Flight Center Scientific Visualization Studio

Average Total-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 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. The Earth's rotation and the movement of warm air from the equator to the poles make the Earth roughly uniform in temperature. The most visible features are the cold poles in winter and the cold clouds along the equator which trap the outgoing thermal radiation.

This is the legend for the total-sky outgoing longwave flux animation, indicating the magnitude of the energy flux.

Metadata

  • Sensor

    Terra/CERES

  • Animation ID

    3092

  • Start Timecode

    00:00:00:00

  • End Timecode

    00:00:00:00

  • Animator

    Horace Mitchell, Eric Sokolowsky

  • Studio

    SVS

  • Visualization Date

    2005/02/01

  • Scientist

    Bruce Wielicki (NASA/LaRC)

  • Datasets

    Outgoing Longwave Radiation

  • Keywords

    GCMD--EARTH SCIENCE--Atmosphere--Atmospheric Radiation--Outgoing Longwave Radiation, GCMD--EARTH SCIENCE--Oceans--Ocean Heat Budget--Longwave Radiation

  • Georeference Data

    [-180,-90,180,90]

  • Data Date

    2002/07/01-2004/06/30

  • Story URL

    http://asd-www.larc.nasa.gov/ceres/ASDceres.html

  • Animation Type

    Regular