The Sentinel-4 mission builds upon the heritage of a series of spectrometer instruments which have been or are currently measuring atmospheric properties since 1995; namely:
- The Global Ozone Monitoring Experiment (GOME) on ESA's ERS-2 satellite which operated between 1995 and 2011.
- The GOME-2 instrument on-board EUMETSAT's MetOp-A satellite, launched in 2006, still in service. A second GOME-2 is operating since 2012 on MetOp-B.
- The SCanning Imaging Absorption spectroMeter for Atmospheric CartograpHY (SCIAMACHY) instrument onboard ESA's Envisat mission which operated between 2002 and 2012.
- The Ozone Monitoring Instrument (OMI) instrument onboard NASA's AURA spacecraft, operating since 2004 and still in service.
- The Tropospheric Ozone Monitoring (TROPOMI) instrument onboard ESA's Sentinel-5P spacecraft expected to be launched in 2016.
As shown in the table, among these five heritage instruments, the one which has the best global performances (e.g. spatial resolution, Signal-to-Noise Ratio, spectral coverage) is TROPOMI as it reunites several of the best characteristics of its predecessors, even going beyond them like for example an unprecedented on-ground spatial resolution of 7 x 7 km.
All Sentinel-4 heritage missions are passive backscatter spectrometers operating in Low Earth Orbits (LEO) which allow performing Earth global coverage measurements with a daily revisit time.
Sentinel-4 on the other hand will be the first imaging spectrometer instrument which will be embarked on-board a satellite in a geostationary (GEO) orbit.
The GEO orbit, although limiting the geographic coverage (for Sentinel-4 only to Europe and parts of North Africa and the Atlantic), will allow for the first time an extremely frequent (about 1hour) delivery of accurate atmospheric data: twenty to hundred times better than the LEO missions.
In terms of spatial sampling, Sentinel-4 will be roughly equivalent to Sentinel-5 and Sentinel-5P.
The wide spectral range covered by Sentinel-4 is narrower as compared to Sentinel-5 and Sentinel-5P, and has been chosen to cover the signatures of fast varying tropospheric constituents.
The main characteristics of the five heritage instruments are summarised in the table.
Instrument | Technical Concept | Spectral Range | Spatial resolution (km x km) | Earth Coverage | Revisit time | Operational |
GOME | Whisk-broom (scanning) | UV-VIS-NIR (240-790 nm) | 320 x 40 | Global | 1 ½ day | 1995-2011 |
GOME-2 | Whisk-broom (scanning) | UV-VIS-NIR (240-790 nm) | 80 x 40 | Global | 1 ½ day | 2006-present |
SCIAMACHY | Whisk-broom (scanning) | UV to SWIR (240-2400 nm) | 30 x 215 | Global | 6 days | 2002-2012 |
OMI | Push-broom (staring) | UV-VIS (270-500 nm) | 13 x 24 | Global | 1 day | 2004-present |
TROPOMI | Push-broom (staring) | UV-VIS-NIR-SWIR (270 – 2385 nm) | 7 x 7 | Global | 1 day | Launch scheduled in 2016 |
Sentinel-4/UVN | Push-Broom (scanning) | UV-VIS-NIR (305- 775 nm) | 8 x 8 | Europe + parts of North Africa and the Atlantic | 1 hour | Launch scheduled in 2021 |