The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT

Atmospheric Motion Vectors (AMVs) are an important input to many Numerical Weather Prediction (NWP) models. EUMETSAT derives AMVs from several of its orbiting satellites, including the geostationary satellites (Meteosat), and its Low-Earth Orbit (LEO) satellites. The algorithm extracting the AMVs us...

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Main Authors: Kévin Barbieux, Olivier Hautecoeur, Maurizio De Bartolomei, Manuel Carranza, Régis Borde
Format: Article
Language:English
Published: MDPI AG 2021-04-01
Series:Remote Sensing
Subjects:
Online Access:https://www.mdpi.com/2072-4292/13/9/1702
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author Kévin Barbieux
Olivier Hautecoeur
Maurizio De Bartolomei
Manuel Carranza
Régis Borde
author_facet Kévin Barbieux
Olivier Hautecoeur
Maurizio De Bartolomei
Manuel Carranza
Régis Borde
author_sort Kévin Barbieux
collection DOAJ
description Atmospheric Motion Vectors (AMVs) are an important input to many Numerical Weather Prediction (NWP) models. EUMETSAT derives AMVs from several of its orbiting satellites, including the geostationary satellites (Meteosat), and its Low-Earth Orbit (LEO) satellites. The algorithm extracting the AMVs uses pairs or triplets of images, and tracks the motion of clouds or water vapour features from one image to another. Currently, EUMETSAT LEO satellite AMVs are retrieved from georeferenced images from the Advanced Very-High-Resolution Radiometer (AVHRR) on board the Metop satellites. EUMETSAT is currently preparing the operational release of an AMV product from the Sea and Land Surface Temperature Radiometer (SLSTR) on board the Sentinel-3 satellites. The main innovation in the processing, compared with AVHRR AMVs, lies in the co-registration of pairs of images: the images are first projected on an equal-area grid, before applying the AMV extraction algorithm. This approach has multiple advantages. First, individual pixels represent areas of equal sizes, which is crucial to ensure that the tracking is consistent throughout the processed image, and from one image to another. Second, this allows features that would otherwise leave the frame of the reference image to be tracked, thereby allowing more AMVs to be derived. Third, the same framework could be used for every LEO satellite, allowing an overall consistency of EUMETSAT AMV products. In this work, we present the results of this method for SLSTR by comparing the AMVs to the forecast model. We validate our results against AMVs currently derived from AVHRR and the Spinning Enhanced Visible and InfraRed Imager (SEVIRI). The release of the operational SLSTR AMV product is expected in 2022.
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spelling doaj.art-d96f4c39de68420a9994d61e658c2edf2023-11-21T17:37:41ZengMDPI AGRemote Sensing2072-42922021-04-01139170210.3390/rs13091702The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSATKévin Barbieux0Olivier Hautecoeur1Maurizio De Bartolomei2Manuel Carranza3Régis Borde4EUMETSAT, 64295 Darmstadt, GermanyEXOSTAFF, 64404 Bickenbach, GermanyEUMETSAT, 64295 Darmstadt, GermanyGMV GmbH, 64293 Darmstadt, GermanyEUMETSAT, 64295 Darmstadt, GermanyAtmospheric Motion Vectors (AMVs) are an important input to many Numerical Weather Prediction (NWP) models. EUMETSAT derives AMVs from several of its orbiting satellites, including the geostationary satellites (Meteosat), and its Low-Earth Orbit (LEO) satellites. The algorithm extracting the AMVs uses pairs or triplets of images, and tracks the motion of clouds or water vapour features from one image to another. Currently, EUMETSAT LEO satellite AMVs are retrieved from georeferenced images from the Advanced Very-High-Resolution Radiometer (AVHRR) on board the Metop satellites. EUMETSAT is currently preparing the operational release of an AMV product from the Sea and Land Surface Temperature Radiometer (SLSTR) on board the Sentinel-3 satellites. The main innovation in the processing, compared with AVHRR AMVs, lies in the co-registration of pairs of images: the images are first projected on an equal-area grid, before applying the AMV extraction algorithm. This approach has multiple advantages. First, individual pixels represent areas of equal sizes, which is crucial to ensure that the tracking is consistent throughout the processed image, and from one image to another. Second, this allows features that would otherwise leave the frame of the reference image to be tracked, thereby allowing more AMVs to be derived. Third, the same framework could be used for every LEO satellite, allowing an overall consistency of EUMETSAT AMV products. In this work, we present the results of this method for SLSTR by comparing the AMVs to the forecast model. We validate our results against AMVs currently derived from AVHRR and the Spinning Enhanced Visible and InfraRed Imager (SEVIRI). The release of the operational SLSTR AMV product is expected in 2022.https://www.mdpi.com/2072-4292/13/9/1702atmospheric motion vectorAMVSentinel-3SLSTRcross-correlationcloud
spellingShingle Kévin Barbieux
Olivier Hautecoeur
Maurizio De Bartolomei
Manuel Carranza
Régis Borde
The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
Remote Sensing
atmospheric motion vector
AMV
Sentinel-3
SLSTR
cross-correlation
cloud
title The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
title_full The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
title_fullStr The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
title_full_unstemmed The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
title_short The Sentinel-3 SLSTR Atmospheric Motion Vectors Product at EUMETSAT
title_sort sentinel 3 slstr atmospheric motion vectors product at eumetsat
topic atmospheric motion vector
AMV
Sentinel-3
SLSTR
cross-correlation
cloud
url https://www.mdpi.com/2072-4292/13/9/1702
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