GOES-R is scheduled launch from Cape Canaveral Air Force Station, Florida atop an Atlas V rocket on November 19, 2016. The current GOES-East and GOES-West have been faithfully providing continuous imagery and data on atmospheric conditions, Earth weather, and space weather, and even aiding in search and rescue missions for almost a decade. So, with the launch of the first of the next generation of GOES satellites, GOES-R, what is NOAA trying to accomplish?
Artist's rendering of GOES-R
The GOES fleet
Since 1975, the National Oceanographic and Atmospheric Administration (NOAA) has operated the Geostationary Operational Environmental Satellites (GOES). At any given time, there are two of them in operation: GOES-East, which covers the Eastern Hemisphere at 75° W longitude, and GOES-West, which covers the Western Hemisphere at 135°W longitude. In case of trouble, a third satellite is usually in orbit, too, standing by until some anomaly occurs.
The GOES fleet
Schematic of the spatial coverage and longitudinal positions of the current GOES fleet.
These satellites sit in geostationary orbit, which is 35,786 kilometers above Earth's equator. At this altitude, their orbital period is equal to Earth’s rotational period, so the satellite appears to hover in a fixed position over Earth’s surface.
When GOES-R arrives in orbit, it will sit at a fixed location of 89.5°W while it undergoes further in-orbit testing. Once operational, its environmental data products will support short-term weather forecasts, hazardous weather announcements, maritime forecasts, seasonal forecasts, drought forecasts, hurricane and storm intensity and tracking forecasts, and space weather predictions. In total it will provide 34 atmospheric, land, ocean, solar, and space weather data products for the scientific community!
Better, faster, stronger
The current GOES-East and GOES-West satellites were launched in 2006 and 2010, respectively. While they carry useful instruments and provide world-class data, the technology upon which they were built is now at least 2 decades old. GOES-R represents the first major technological advancement since then.
Most GOES satellites carry a large suite of instruments. The most important ones are the sounder, the imager, and the solar x-ray imager. GOES-R will introduce a massive new 16-channel imager called the Advanced Baseline Imager (ABI), a Geostationary Lightning Mapper (GLM), and a Solar UV Imager (SUVI) as a step up from previous GOES instruments.
Artist’s rendition of GOES-R
ABI is unique because it will scan 5 times faster with 4 times the spatial resolution of the current GOES. This means ABI can scan an entire hemisphere every 5 minutes, or as fast as every 30 seconds in subregions where there is severe weather. Previous iterations of GOES could only provide hemispherical data every 30 minutes, and hazardous weather data every 5 minutes. In addition, ABI has 3 times the number of spectral channels from which weather data can be derived. For reference, here’s a list of all of ABI’s spectral channels, the part of the electromagnetic spectrum each covers, and what those data can be used to study.
Center Wavelength (μm)
Portion of Spectrum
Observed Environmental Parameters
Fog, solar insolation, cloud behavior, snow/ice cover, severe weather detection, low-level cloud-drift winds, smoke, volcanic ash, hurricanes, winter storm
Clouds, fog, aerosols, normalized difference vegetation index (NDVI)
Thin cirrus clouds
Cloud, snow, ice, total cloud cover estimation, smoke detection from fires with low burn rates
Tropospheric air temperature estimation, cloud products
GLM will detect both cloud-to-ground and cloud-to-cloud lightning from geostationary orbit. Research has uncovered a relationship between lightning activity and intensification of storms. Data from GLM will help to identify changes in lightning activity in tropical cyclones, and forecasters may then be able to determine whether a storm will have bad wind, hail, or rain.
SUVI will keep a watchful eye on the environment around Earth in the extreme ultraviolet portion of the electromagnetic spectrum. Despite being in space, space weather directly impacts life on Earth. The sun periodically releases strong bursts of charged particles that interact with Earth’s magnetic field and can disrupt satellite operations, GPS, and telecommunications. SUVI’s job is to observe solar flares and coronal mass ejections, providing early warnings to forecasters of possible impacts to the Earth-space environment, and, subsequently, on the ground.
Looking for data?
Meanwhile, if you’re a scientist or citizen scientist looking for GOES-13 (East) or GOES-15 (West) data or imagery, here are the resources you’ll want to check out. Note that you may have to write your own data readers using some kind of scientific software like MATLAB, IDL, or Fortran, if you’re not looking for pre-processed imagery. NOAA’s data guides are also available at these websites: