On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions
The long-term comparison between simulated and observed spectrally resolved outgoing longwave radiation (OLR) can represent a stringent test for the direct verification and improvement of general circulation models (GCMs), which are regularly tuned by adjusting parameters related to subgrid processe...
Published in: | Geoscientific Model Development |
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ftcopernicus:oai:publications.copernicus.org:gmd104464 2023-05-15T18:18:49+02:00 On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions Fera, Stefano Fabiano, Federico Raspollini, Piera Ridolfi, Marco Cortesi, Ugo Barbara, Flavio Hardenberg, Jost 2023-02-28 application/pdf https://doi.org/10.5194/gmd-16-1379-2023 https://gmd.copernicus.org/articles/16/1379/2023/ eng eng doi:10.5194/gmd-16-1379-2023 https://gmd.copernicus.org/articles/16/1379/2023/ eISSN: 1991-9603 Text 2023 ftcopernicus https://doi.org/10.5194/gmd-16-1379-2023 2023-03-06T17:23:11Z The long-term comparison between simulated and observed spectrally resolved outgoing longwave radiation (OLR) can represent a stringent test for the direct verification and improvement of general circulation models (GCMs), which are regularly tuned by adjusting parameters related to subgrid processes not explicitly represented in the model to constrain the integrated OLR energy fluxes to observed values. However, a good agreement between simulated and observed integrated OLR fluxes may be obtained from the cancellation of opposite-in-sign systematic errors localized in specific spectral ranges. Since the mid-2000s, stable hyperspectral observations of the mid-infrared region (667 to 2750 cm −1 ) of the Earth emission spectrum have been provided by different sensors (e.g. AIRS, IASI and CrIS). Furthermore, the FORUM (Far-infrared Outgoing Radiation Understanding and Monitoring) mission, selected to be the ninth ESA Earth Explorer, will measure, starting from 2027, the terrestrial radiation emitted to space at the top of the atmosphere (TOA) from 100 to 1600 cm −1 , filling the observational gap in the far-infrared (FIR) region, from 100 to 667 cm −1 . In this work, in anticipation of FORUM measurements, we compare Infrared Atmospheric Sounding Interferometer (IASI) Metop-A observations to radiances simulated on the basis of the atmospheric fields predicted by the EC-Earth Global Climate Model (version 3.3.3) in clear-sky conditions. To simulate spectra based on the atmospheric and surface state provided by the climate model, the radiative transfer model σ-IASI has been integrated in the Cloud Feedback Model Intercomparison Project (COSP) package. Therefore, online simulations, provided by the EC-Earth model equipped with the new COSP–σ-IASI module, have been performed in clear-sky conditions with prescribed sea surface temperature and sea ice concentration, every 6 h, over a time frame consistent with the availability of IASI data. Systematic comparisons between observed and simulated brightness temperature (BT) ... Text Sea ice Cris Copernicus Publications: E-Journals Geoscientific Model Development 16 4 1379 1394 |
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Open Polar |
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Copernicus Publications: E-Journals |
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ftcopernicus |
language |
English |
description |
The long-term comparison between simulated and observed spectrally resolved outgoing longwave radiation (OLR) can represent a stringent test for the direct verification and improvement of general circulation models (GCMs), which are regularly tuned by adjusting parameters related to subgrid processes not explicitly represented in the model to constrain the integrated OLR energy fluxes to observed values. However, a good agreement between simulated and observed integrated OLR fluxes may be obtained from the cancellation of opposite-in-sign systematic errors localized in specific spectral ranges. Since the mid-2000s, stable hyperspectral observations of the mid-infrared region (667 to 2750 cm −1 ) of the Earth emission spectrum have been provided by different sensors (e.g. AIRS, IASI and CrIS). Furthermore, the FORUM (Far-infrared Outgoing Radiation Understanding and Monitoring) mission, selected to be the ninth ESA Earth Explorer, will measure, starting from 2027, the terrestrial radiation emitted to space at the top of the atmosphere (TOA) from 100 to 1600 cm −1 , filling the observational gap in the far-infrared (FIR) region, from 100 to 667 cm −1 . In this work, in anticipation of FORUM measurements, we compare Infrared Atmospheric Sounding Interferometer (IASI) Metop-A observations to radiances simulated on the basis of the atmospheric fields predicted by the EC-Earth Global Climate Model (version 3.3.3) in clear-sky conditions. To simulate spectra based on the atmospheric and surface state provided by the climate model, the radiative transfer model σ-IASI has been integrated in the Cloud Feedback Model Intercomparison Project (COSP) package. Therefore, online simulations, provided by the EC-Earth model equipped with the new COSP–σ-IASI module, have been performed in clear-sky conditions with prescribed sea surface temperature and sea ice concentration, every 6 h, over a time frame consistent with the availability of IASI data. Systematic comparisons between observed and simulated brightness temperature (BT) ... |
format |
Text |
author |
Fera, Stefano Fabiano, Federico Raspollini, Piera Ridolfi, Marco Cortesi, Ugo Barbara, Flavio Hardenberg, Jost |
spellingShingle |
Fera, Stefano Fabiano, Federico Raspollini, Piera Ridolfi, Marco Cortesi, Ugo Barbara, Flavio Hardenberg, Jost On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
author_facet |
Fera, Stefano Fabiano, Federico Raspollini, Piera Ridolfi, Marco Cortesi, Ugo Barbara, Flavio Hardenberg, Jost |
author_sort |
Fera, Stefano |
title |
On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
title_short |
On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
title_full |
On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
title_fullStr |
On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
title_full_unstemmed |
On the use of Infrared Atmospheric Sounding Interferometer (IASI) spectrally resolved radiances to test the EC-Earth climate model (v3.3.3) in clear-sky conditions |
title_sort |
on the use of infrared atmospheric sounding interferometer (iasi) spectrally resolved radiances to test the ec-earth climate model (v3.3.3) in clear-sky conditions |
publishDate |
2023 |
url |
https://doi.org/10.5194/gmd-16-1379-2023 https://gmd.copernicus.org/articles/16/1379/2023/ |
genre |
Sea ice Cris |
genre_facet |
Sea ice Cris |
op_source |
eISSN: 1991-9603 |
op_relation |
doi:10.5194/gmd-16-1379-2023 https://gmd.copernicus.org/articles/16/1379/2023/ |
op_doi |
https://doi.org/10.5194/gmd-16-1379-2023 |
container_title |
Geoscientific Model Development |
container_volume |
16 |
container_issue |
4 |
container_start_page |
1379 |
op_container_end_page |
1394 |
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1766195531060609024 |