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The Earth Radiation Budget Experiment (ERBE)

ERBE Image


The radiation budget represents the balance between incoming energy from the Sun and outgoing thermal (longwave) and reflected (shortwave) energy from the Earth. In the 1970’s, NASA recognized the importance of improving our understanding of the radiation budget and its effects on the Earth’s climate. Langley Research Center 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 Center 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 weather monitoring satellites, NOAA 9 and NOAA 10 in 1984 and 1986.

Science Team

An international team of scientists was selected from proposals to an Announcement of Opportunity in 1978 to participate in the design and development of ERBE. Dr Bruce Barkstrom, of the Radiation Sciences Branch of Langley’s Atmospheric Sciences Competency, was selected as the ERBE Principal Investigator. He led the team through 30 meetings to guide the development of the instrumentation and the ground processing software for analyzing the data.

Instrument Development

Langley formed a team of electronic, thermal, and mechanical experts to develop the ERBE instruments. Led by Jack Cooper, Experiment Manager, and Glenn Taylor, Instrument Manager, this team developed the specifications for two types of instruments:

  • Scanner – A set of three co-planar detectors (longwave, shortwave and total energy), all of which scan from one limb of the Earth to the other, across the satellite track (in it’s normal operational mode).
  • Nonscanner – A set of five detectors; one which measures the total energy from the Sun, two which measure the shortwave and total energy from the entire Earth disk, and two of which measure the shortwave and total energy from a medium resolution area beneath the satellite.

TRW, of Redondo Beach, California, was selected to build the instruments, calibrate them in a unique thermal/vacuum radiometric calibration facility, and help integrate the instruments with the ERBS and NOAA satellite platforms.

Data Management System Development

The ERBE Data Management Team was formed to design and develop the ground data processing system based on algorithms from the Science Team. Jim Kibler, Head of the Data Management Office in Langley’s Atmospheric Sciences Competency, led the team through three iterative releases of the system to be ready for processing at the first launch. The system design included several subsystems to produce archival science products for study by the science community:

  • Telemetry – Process data from NOAA and GSFC to a common format, interpret the instrument and spacecraft housekeeping data, and analyze instrument commands and in-orbit environment.
  • Ephemeris – Analyze orbit position data from GSFC for each of the three satellite platforms.
  • Merge/Count Conversion – Combine telemetry and ephemeris data to produce Earth location geometry and convert radiometric counts produced by the instruments into satellite-altitude radiances.
  • Inversion – Identify the scene viewed by the instruments and interpret the measurements at the top of the Earth’s atmosphere using shape factor and numerical filter inversion techniques.
  • Daily and Monthly Time/Space Averaging – Convert from time-ordered to regionally-accessible data sets and apply diurnal models to estimate hourly, daily, and monthly averages of radiation budget components.
  • Data Products – Generate well-documented science archival products in an easily accessible format.

Data Archival and Access

Since the ERBS launch in 1984, the ERBE Project has been validating the instrument results and producing data products for use by the science community. These products range from instantaneous time-sequenced instrument measurements to monthly-averaged regional, zonal, and global estimates of radiation budget parameters:

  • S-2 Solar Incidence
  • S-4 Regional, Zonal, and Global Averages
  • S-4G Regional, Zonal, and Global Gridded Averages
  • S-7 Medium-Wide Field of View Nonscanner Data
  • S-8 Instantaneous Scanner and Nonscanner Data
  • S-9 Scanner Earth Radiant Flux and Albedo
  • S-10 Nonscanner Earth Radiant Flux and Albedo

These data products are now available from the Langley Distributed Active Archive Center. Data, programs for reading the data, and user’s guides can be obtained through the on-line system.

ERBE Science Lead: Takmeng Wong

Team Satellite Sensor G/L Dates Number of obs Phase angle range (°)
CMA FY-3C MERSI LEO 2013-2014 9 [43 57]
CMA FY-2D VISSR GEO 2007-2014
CMA FY-2E VISSR GEO 2010-2014
CMA FY-2F VISSR GEO 2012-2014
JMA MTSAT-2 IMAGER GEO 2010-2013 62 [-138,147]
JMA GMS5 VISSR GEO 1995-2003 50 [-94,96]
JMA Himawari-8 AHI GEO 2014- -
EUMETSAT MSG1 SEVIRI GEO 2003-2014 380/43 [-150,152]
EUMETSAT MSG2 SEVIRI GEO 2006-2014 312/54 [-147,150]
EUMETSAT MSG3 SEVIRI GEO 2013-2014 45/7 [-144,143]
EUMETSAT MET7 MVIRI GEO 1998-2014 128 [-147,144]
CNES Pleiades-1A PHR LEO 2012 10 [+/-40]
CNES Pleiades-1B PHR LEO 2013-2014 10 [+/-40]
NASA-MODIS Terra MODIS LEO 2000-2014 136 [54,56]
NASA-MODIS Aqua MODIS LEO 2002-2014 117 [-54,-56]
NASA-VIIRS NPP VIIRS LEO 2012-2014 20 [50,52]
NASA-OBPG SeaStar SeaWiFS LEO 1997-2010 204 (<10, [27-66])
NASA/USGS Landsat-8 OLI LEO 2013-2014 3 [-7]
NOAA-STAR NPP VIIRS LEO 2011-2014 19 [-52,-50]
NOAA GOES-10 IMAGER GEO 1998-2006 33 [-66, 81]
NOAA GOES-11 IMAGER GEO 2006-2007 10 [-62, 57]
NOAA GOES-12 IMAGER GEO 2003-2010 49 [-83, 66]
NOAA GOES-15 IMAGER GEO 2012-2013 28 [-52, 69]
VITO Proba-V VGT-P LEO 2013-2014 25 [-7]
KMA COMS MI GEO 2010-2014 60
AIST Terra ASTER LEO 1999-2014 1 -27.7
ISRO OceanSat2 OCM-2 LEO 2009-2014 2

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