First Images Press Conference
April 19, 2000
 
introduction / modis / misr / aster / mopitt / ceres / conclusion

CERES, Bruce Barkstrom
Earth in Space   The only way the Earth receives the energy that keeps the surface warm is through sunlight. Some of the incoming sunlight is reflected back up into space by the Earth's surface, atmosphere, and clouds; some of it is absorbed and stored as heat. When the surface and atmosphere warm, they emit heat, or thermal energy, to space. The "radiation budget" is an accounting of these energy flows. If the radiation budget is in balance, then, the surface of the Earth should be neither warming nor cooling, on average.
CERES Shortwave The CERES, or Clouds and the Earth's Radiant Energy System, instrument measures reflected sunlight. In this image, the dark and unreflective ocean is colored blue, while the more reflective land is colored green to grey. Clouds are very reflective. We see them standing out from the dark ocean.
CERES Thermal IR CERES measures the energy emitted by the surface and atmosphere of the Earth. This image shows high emission from warm surfaces in yellow. Where the surface is colder, the image appears blue or white. Over the Sahara, we see through to the very warm surface of the Earth. Nearer the poles, clouds cover the surface and we see them as cold, blue areas in this image.
CERES Thermal Longwave The excess sunlight warms the Tropics. If ths continued over a long time, the Tropics would just keep warming. The Polar regions receive less energy from the sun than they emit to space, and so they cool. The temperature difference between the Tropics and the Poles creates winds and ocean currents that carry excess heat and moisture. When the moisture encounters cooler temp- eratures as it moves to the poles, clouds form and reduce the emission of energy to space. This animation shows the weather systems driven by the distribution of energy measured by CERES.
Cloud Effects on Earth's Radiation Clouds play a complex role in the Earth's radiation budget. Low Clouds reflect much of the sunlight that falls on them, but have little Effect on the emitted energy. Thus, low clouds act to cool the Current climate. High clouds reflect less energy, but trap more of The energy emitted by the surface. About 10 years ago, measure- Ments like those of CERES showed that clouds act to cool the current climate. However, the measurements could not tell us why the clouds in different parts of the Earth were different from one another. CERES cannot answer this question by itself; the other instruments on Terra will make contributions to what CERES measures that will improve our understanding of why clouds act the way they do in the current climate, and what we may expect them to do in the future.
Climate Sensitivity Scientists assessing our understanding of climate have looked at many mechanisms that might change climate: volcanoes, green-house gas changes, aerosols, the properties of the Earth's surface. This chart illustrates our current understanding of the relative importance of these various kinds of climate forcing mechanisms. The uncertainty in what clouds will do in the future remains the largest source of uncertainty in predicting the future climate.
SCOOL This picture shows one of the educational outreach activities that Terra includes: the CERES S'COOL Project, short for Student Cloud Observations On-Line. When the CERES instruments on Terra pass over the schools, the students in S'COOL observe the Clouds and send in their observations to the S'COOL Project at NASA's Langley Research Center. About 500 schools are Currently participating in this international program.

introduction / modis / misr / aster / mopitt / ceres / conclusion