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IntroductionThe Earth Radiation Budget Experiment is designed around three Earth-orbiting satellites: the NASA Earth
Radiation Budget Satellite (ERBS), and two NOAA satellites. The data from these satellites is being used
to study the radiation budget, which
represents the balance between incoming energy from the Sun and outgoing thermal (longwave) and reflected
(shortwave) energy from the Earth. The Earth's radiation budget is the primary indicator of global climate
change. The absorbed shortwave radiation (incident minus reflected) fuels the earth's climate and biosphere
systems. The longwave radiation represents the exhaust heat emitted to space. It can be used to estimate
the insulating effect of the atmosphere (the greenhouse effect). It is also a useful indicator of cloud
amount and activity. Consequently the ERBE has helped scientists worldwide better understand how clouds
and aerosols, as well as some chemical compounds in the atmosphere (greenhouse gases), affect the Earth's
daily and long-term weather (the Earth's climate). In addition, the ERBE data has helped scientists
better understand how the amount of energy emitted by the Earth varies from day to night. These diurnal
changes are also very important aspects of our daily weather and climate.
In the 1970's, NASA recognised the importance of the radiation budget and
its effects on the Earth's climate. Langley Research Centre was charged with developing a new generation of
instrumentation to make accurate regional and global measurements of the components of the radiation
budget. The Goddard Space Flight Centre built the Earth
Radiation Budget Satellite (ERBS) on which the
first ERBE instruments were launched by the Space Shuttle Challenger in 1984. ERBE instruments were also
launched on two National Oceanic and Atmospheric Administration (NOAA) weather monitoring satellites; NOAA
9 and NOAA 10, in 1984 and 1986.
The ERBE instrument aboard ERBS, launched from the Space Shuttle Challenger in October 1984 (STS-41G), had
the main aim of providing accurate measurements of incoming solar energy and shortwave and longwave radiation
reflected or emitted from the Earth back into space. The other goals of the Earth Radiation Budget
Experiment (ERBE) are:
All of the initial goals were met, and the ERBE instrument continues to provide valuable data. Earth
Radiation Budget Experiment (ERBE) data are fundamental to the development of
realistic climate models and for studying natural and anthropogenic perturbations of the climate system.
This CD-ROM contains data and colour images from scanning radiometers on the three ERBE satellites and for
combined satellite cases. The CD-ROM is written using the ISO-9660 standard. Monthly average values are
included for the time periods during which the scanners were operational.
Access to DataThe ERBE data are held on a CD-ROM at the BADC and are made available for browsing purposes. If you want to use the data in earnest you should order a copy of the CD from the contact address below. The CD-ROM holds a few directories, including the ERBE data.
DocumentationReadme documentation can be found on the ERBE CD-ROM. More extensive documentation is available on the ERBE datasets web page, and includes the following topics:
A sample image is
available from the ERBE
total solar irradiance data, on the
ERBE datasets web site.
Links and ReferencesA list of references has been
extracted from the ERBE web pages.
You may visit the ERBE
datasets information page, which has links to the
ERBE CD-ROM information page and
the NASA ERBE home page.
Citation
Who to ContactGeneral queries about these pages or browsing the data should be directed to the
BADC support line.
If you would like to obtain a copy of the Earth Radiation Budget Experiment (ERBE) CD-ROM you should
contact the
NASA Langley Atmospheric Sciences Data Centre User Services. The
CD-ROM set may be ordered through the web from the NASA Langley Centre.
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