Earth-facing The Advanced Baseline Imager (ABI) and Geostationary Lightning Mapper (GLM) make up GOES-16's Earth-facing, or
nadir-pointing, instruments. These are positioned on a stable precision-pointed platform isolated from the rest of the spacecraft. all electronics and the
sensor array are redundant to ensure operation longetivity. Several other companies were involved in the development and fabrication of the ABI, including
BAE Systems, BEI Technologies,
Babcock Corporation,
DRS Technologies,
L3 Technologies SSG-Tinsley, and
Northrop Grumman Space Technology. The ABI takes images with three different geographic extents, In the default "flex" mode (scan mode 3) of operation, the ABI produces full-disk images of the Earth every 15 minutes, with a spatial resolution of . The instrument also images a area centered on the
continental United States every five minutes at a resolution of . Where possible, the ABI can also image
mesoscale phenomena over two selected areas every 60 seconds at a resolution of . The ABI onboard GOES-16 represents a significant improvement over the imager onboard previous GOES satellites. The sixteen spectral bands on the ABI, as opposed to the five on the previous GOES generation, represents a two-fold increase in spectral information. In addition, the ABI features up to four times greater spatial resolution and five times greater temporal resolution over the previous GOES imager. The ABI is nearly identical to the Advanced Himawari Imager (AHI) first used on the
Japan Meteorological Agency's
Himawari 8, which launched on 7 October 2014. The two instruments share 15 of the same spectral bands and have one spectral band unique to either instrument, with the ABI featuring a 1.37 μm near-infrared band for
cirrus cloud detection while the AHI uses a 0.51 μm band optimized for reflectance around the green portion of the
visible spectrum. Lacking an explicit band for green light,
true-color imagery for ABI is created using the combination of the ABI's red and blue visible bands along with a synthesized green band; the simulated green band is created by applying algorithms based on
MODIS and AHI onto existing ABI spectral bands.
Geostationary Lightning Mapper (GLM) The GOES-16 Geostationary Lightning Mapper (GLM) is a single-channel
near-infrared detector that monitors for the short-lived light emitted by
lightning. by extension, such information can also reduce false alarm rates of
severe thunderstorm and tornado warnings. The GLM can detect both
cloud-to-cloud and
cloud-to-ground lightning during daytime and nighttime, complementing land-based
lightning detection. GLM's sensitivity results in a detection rate of 70–90% of all lightning strikes in its viewing area. The camera is a 1372 × 1300 pixel
staring CCD sensitive to 777.4 nm light with a spatial resolution of at the nadir and near the edge of the instrument's field-of-view, resulting in a spatial resolution averaging roughly . The latitudinal coverage of the instrument is limited to between 52°N and 52°S. To limit interference of undesired light, a solar blocking filter and solar rejection filter are affixed to the front of the instrument's aperture. Data from the GLM can be mapped in real-time using
open-source software that has also been adapted by the United States
National Weather Service Development of the GLM was contracted by the Lockheed Martin Advanced Technology Center in
Palo Alto, California.
Sun-facing The Sun-facing, or solar-pointing, components of GOES-16 include the EXIS and SUVI, which are located on a Sun Pointing Platform (SPP) on the spacecraft's solar array
yoke; the SPP tracks the seasonal and daily movement of the sun relative to GOES-16, and also supports GOES-16's Unique Payload Services. Together, the EXIS instrument weighs and consumes 40 W of power.
Solar Ultraviolet Imager (SUVI) The Solar Ultraviolet Imager (SUVI) is an
ultraviolet telescope onboard GOES-16 that produces full-disk images of the sun in the
extreme ultraviolet range, succeeding the former GOES Solar X-ray Imager instrument onboard previous GOES satellite generations. The goals of SUVI are to locate
coronal holes, detect and locate solar flares, monitor changes that indicate
coronal mass ejections, detect active regions beyond the Sun's east limb, and analyze the complexity of active regions on the sun. The telescope is composed of six different wavelength bands centered between 94–304
Å specialized for different solar features. The GOES-16's ultraviolet imager is analogous to the
Extreme ultraviolet Imaging Telescope on the
Solar and Heliospheric Observatory.
Space environment GOES-16 features two instruments, the Magnetometer (MAG) and Space Environment In-Situ Suite (SEISS), that provide localized in-situ observations of high-energy particles and magnetic fields in geostationary orbit.
Magnetometer (MAG) The GOES-16 Magnetometer (MAG) is a tri-axial
fluxgate magnetometer that measures the
Earth's magnetic field at the outer extents of the
magnetosphere from geostationary orbit. MAG provides general data on
geomagnetic activity, which can be used to detect
solar storms and validate large-scale space environment modelling; The magnetometer samples the magnetic field at a resolution of 0.016
nT at a frequency of 2.5 Hz. The electronic and sensor components of MAG were built by Macintyre Electronic Design Associates, Inc. (MEDA) in
Sterling, Virginia, while the deployable boom was built by ATK in
Goleta, California.
Space Environment In-Situ Suite (SEISS) The Space Environment In-Situ Suite (SEISS) consists of four sensors with a wide variance in
field-of-view that monitor
proton,
electron, and heavy
ion fluxes in the magnetosphere. Electrons at these energies easily penetrate spacecraft and may cause internal
dielectric breakdown or discharge damage. Development of SEISS was contracted by
Assurance Technology Corporation in
Carlisle, Massachusetts, and subcontracted to the
University of New Hampshire. ==Launch and mission profile==