Providing water vapour and temperature profiles
The InfraRed Sounder (IRS) is set to revolutionise weather forecasting by tracking the 3-dimensional structure of atmospheric water vapour and temperature, for the first time on an operational basis.
20 June 2022
21 May 2020
The IRS acquires a number of spectral soundings simultaneously over a dwell using a two dimensional detector array. It uses a ‘step-and-stare’ mechanism to probe the Earth´s atmosphere.
The dwell coverage is stepped in an east/west direction to form a line of dwell spectral soundings, before moving northward to form the next line, covering the local area coverage (LAC) within the repeat cycle duration (‘step-and-stare’ principle of probing the atmosphere).
Four separate LAC zones are defined and scanned sequentially (Figure 2). One LAC is acquired within 15 minutes, consisting of overlapping dwells following a step and stare scan pattern. Each dwell consists of 160x160 pixels (spectral soundings), with 4km spatial sampling distance at nadir. Europe (LAC4) is observed every 30 minutes.
The spectral soundings are transmitted to the ground as interferograms and transformed to spectral channels as part of the ground processing, before dissemination to the end users as Level 1 datasets.
The IRS is based on an imaging Fourier-interferometer with a hyperspectral resolution of 0.625cm-1 wave-number, taking measurements in two bands, the Long-Wave Infrared (LWIR) and the Mid-Wave Infrared (MWIR).
Summary of technical specifications
- Two spectral bands: MWIR: 1600 to 2250cm-1 (4.44–6.25µm) and LWIR: 680 to 1210cm-1 (8.26–14.70µm).
- Full disc coverage in 60 min, Europe region (Local Area Coverage) 30 min.
- Spatial resolution of 4km x 4km at nadir.
- Radiometric measurement ranges between 180K and 313K (equivalent black-body temperature.)
- Spectral radiometric noise (excluding spectral calibration) at 280K black body: between 170 and 900mK depending on the considered wave-number inside the band of interest.
The IRS includes the ozone band within LWIR and the carbon monoxide band within MWIR. This will allow measurement within the free troposphere, leading to information on enhanced levels of pollution in the boundary layer below.
Other MTG instruments
Flexible Combined Imager (FCI)
The Flexible Combined Imager (FCI) will fly on the on the MTG-I satellite.
Science studies & meetings
Assimilation of PC-reconstructed radiances in NWP
Hyperspectral missions have been providing key information to numerical weather prediction (NWP) for about two decades, e.g.
IRS mission advisory group (IRS-MAG) January 2022
IRS mission advisory group (IRS-MAG), 24 January 2022, Online
IRS mission advisory group (IRS-MAG) June 2021
IRS mission advisory group (IRS-MAG), 8 June 2021, Online
Hyperspectral sounding for severe storm forecasting
Exploring the potential and requirements of hyperspectral sounding products to severe storm short-range forecasting.
IRS retrievals & applications at high satellite zenith angle
Study to engineer a method aimed at assessing the sensing sensitivity of MTG-IRS at high scanning angles.
IRS mission advisory group (IRS-MAG) November 2020
IRS mission advisory group (IRS-MAG),12 November 2020, Online
IRS mission advisory group (IRS-MAG) June 2020
IRS mission advisory group (IRS-MAG),6 June 2020, Online
IRS mission advisory group (IRS-MAG), May 2019
IRS mission advisory group (IRS-MAG), 16-17 May 2019, EUMETSAT, Germany
IRS mission advisory group (IRS-MAG), May 2018
IRS mission advisory group (IRS-MAG), 24-25 May 2018, EUMETSAT, Darmstadt.
IRS mission advisory group (IRS-MAG), November 2019
IRS mission advisory group (IRS-MAG),18-19 November 2019, EUMETSAT, Germany
Generation of MTG FCI and IRS INR observations
This study focuses on the generation of proxy data for two MTG payloads, FCI and IRS.