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description Publicationkeyboard_double_arrow_right Article , Other literature type 2022 France, France, France, France, GermanyPublisher:Copernicus GmbH Funded by:EC | IMMERSE, NSF | EarthCube Data Capabiliti..., NSF | NSFGEO-NERC: Collaborativ... +3 projectsEC| IMMERSE ,NSF| EarthCube Data Capabilities: A Cloud-Native Data Repository for the Geoscience Community ,NSF| NSFGEO-NERC: Collaborative Research: Assessing the influence of sub-annual variability in the AMOC on the Gulf Stream and the atmosphere ,ANR| CONTACTS ,ANR| DEEPER ,EC| ESiWACE2T. Uchida; J. Le Sommer; C. Stern; R. P. Abernathey; C. Holdgraf; A. Albert; L. Brodeau; L. Brodeau; E. P. Chassignet; X. Xu; J. Gula; J. Gula; G. Roullet; N. Koldunov; S. Danilov; Q. Wang; D. Menemenlis; C. Bricaud; B. K. Arbic; J. F. Shriver; F. Qiao; B. Xiao; A. Biastoch; A. Biastoch; R. Schubert; R. Schubert; B. Fox-Kemper; W. K. Dewar; W. K. Dewar; A. Wallcraft;Abstract. With the increase in computational power, ocean models with kilometer-scale resolution have emerged over the last decade. These models have been used for quantifying the energetic exchanges between spatial scales, informing the design of eddy parametrizations, and preparing observing networks. The increase in resolution, however, has drastically increased the size of model outputs, making it difficult to transfer and analyze the data. It remains, nonetheless, of primary importance to assess more systematically the realism of these models. Here, we showcase a cloud-based analysis framework proposed by the Pangeo project that aims to tackle such distribution and analysis challenges. We analyze the output of eight submesoscale-permitting simulations, all on the cloud, for a crossover region of the upcoming Surface Water and Ocean Topography (SWOT) altimeter mission near the Gulf Stream separation. The cloud-based analysis framework (i) minimizes the cost of duplicating and storing ghost copies of data and (ii) allows for seamless sharing of analysis results amongst collaborators. We describe the framework and provide example analyses (e.g., sea-surface height variability, submesoscale vertical buoyancy fluxes, and comparison to predictions from the mixed-layer instability parametrization). Basin- to global-scale, submesoscale-permitting models are still at their early stage of development; their cost and carbon footprints are also rather large. It would, therefore, benefit the community to document the different model configurations for future best practices. We also argue that an emphasis on data analysis strategies would be crucial for improving the models themselves.
OceanRep; Geoscienti... arrow_drop_down Geoscientific Model Development (GMD)Other literature type . 2022Data sources: Copernicus PublicationsElectronic Publication Information CenterArticle . 2022Data sources: Electronic Publication Information CenterArchiMer - Institutional Archive of IfremerOther literature type . 2022Data sources: ArchiMer - Institutional Archive of IfremerINRIA a CCSD electronic archive server; Mémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2022License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routesgold 8 citations 8 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert OceanRep; Geoscienti... arrow_drop_down Geoscientific Model Development (GMD)Other literature type . 2022Data sources: Copernicus PublicationsElectronic Publication Information CenterArticle . 2022Data sources: Electronic Publication Information CenterArchiMer - Institutional Archive of IfremerOther literature type . 2022Data sources: ArchiMer - Institutional Archive of IfremerINRIA a CCSD electronic archive server; Mémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2022License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-15-5829-2022&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:EDP Sciences Funded by:EC | ExoplANETS A, UKRI | Quota Studentship 2012, EC | EXOLIGHTS +6 projectsEC| ExoplANETS A ,UKRI| Quota Studentship 2012 ,EC| EXOLIGHTS ,UKRI| DiRAC 2.5 Operations 2017-2020 ,EC| ATMO ,UKRI| A comprehensive study of stars, disks and exoplanets ,UKRI| DiRAC2: 100 Tflop/s HPC cluster procurement ,UKRI| The DiRAC 2.5x Facility ,EC| ExoAIBenjamin Drummond; Eric Hébrard; Nathan J. Mayne; Olivia Venot; Robert J. Ridgway; Quentin Changeat; Shang-Min Tsai; James Manners; Pascal Tremblin; Nathan Luke Abraham; David K. Sing; Krisztian Kohary;We present results from a set of simulations using a fully coupled three-dimensional (3D) chemistry-radiation-hydrodynamics model and investigate the effect of transport of chemical species by the large-scale atmospheric flow in hot Jupiter atmospheres. We couple a flexible chemical kinetics scheme to the Met Office Unified Model which enables the study of the interaction of chemistry, radiative transfer and fluid dynamics. We use a newly-released "reduced" chemical network comprising 30 chemical species that has been specifically developed for application in 3D atmosphere models. We simulate the atmospheres of the well-studied hot Jupiters HD~209458b and HD~189733b which both have dayside--nightside temperature contrasts of several hundred Kelvin and superrotating equatorial jets. We find qualitatively quite different chemical structures between the two planets, particularly for methane (CH$_4$), when advection of chemical species is included. Our results show that consideration of 3D chemical transport is vital in understanding the chemical composition of hot Jupiter atmospheres. 3D mixing leads to significant changes in the abundances of absorbing gas-phase species compared with what would be expected by assuming local chemical equilibrium, or from models including 1D - and even 2D - chemical mixing. We find that CH$_4$, carbon dioxide (CO$_2$) and ammonia (NH$_3$) are particularly interesting as 3D mixing of these species leads to prominent signatures of out-of-equilibrium chemistry in the transmission and emission spectra, detectable with near-future instruments. Comment: Accepted in A&A
arXiv.org e-Print Ar... arrow_drop_down Astronomy and AstrophysicsOther literature type . Article . 2020 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937153&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 55 citations 55 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Astronomy and AstrophysicsOther literature type . Article . 2020 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937153&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:American Astronomical Society Funded by:EC | ATMO, EC | ExoAI, UKRI | Quota Studentship 2012 +1 projectsEC| ATMO ,EC| ExoAI ,UKRI| Quota Studentship 2012 ,EC| ExoplANETS AOlivia Venot; Vivien Parmentier; Jasmina Blecic; Patricio E. Cubillos; Ingo Waldmann; Quentin Changeat; Julianne I. Moses; Pascal Tremblin; Nicolas Crouzet; Peter Gao; Diana Powell; Pierre Olivier Lagage; Ian Dobbs-Dixon; Maria Steinrueck; Laura Kreidberg; Natalie M. Batalha; Jacob L. Bean; Kevin B. Stevenson; Sarah L. Casewell; Ludmila Carone;The James Webb Space Telescope (JWST) is expected to revolutionize the field of exoplanets. The broad wavelength coverage and the high sensitivity of its instruments will allow characterization of exoplanetary atmospheres with unprecedented precision. Following the Call for the Cycle 1 Early Release Science Program, the Transiting Exoplanet Community was awarded time to observe several targets, including WASP-43b. The atmosphere of this hot Jupiter has been intensively observed but still harbors some mysteries, especially concerning the day-night temperature gradient, the efficiency of the atmospheric circulation, and the presence of nightside clouds. We will constrain these properties by observing a full orbit of the planet and extracting its spectroscopic phase curve in the 5--12 $\mu$m range with JWST/MIRI. To prepare for these observations, we performed an extensive modeling work with various codes: radiative transfer, chemical kinetics, cloud microphysics, global circulation models, JWST simulators, and spectral retrieval. Our JWST simulations show that we should achieve a precision of 210 ppm per 0.1 $\mu$m spectral bin on average, which will allow us to measure the variations of the spectrum in longitude and measure the night-side emission spectrum for the first time. If the atmosphere of WASP-43b is clear, our observations will permit us to determine if its atmosphere has an equilibrium or disequilibrium chemical composition, providing eventually the first conclusive evidence of chemical quenching in a hot Jupiter atmosphere. If the atmosphere is cloudy, a careful retrieval analysis will allow us to identify the cloud composition. Comment: 26 pages, 16 figures, accepted in The Astrophysical Journal
The Astrophysical Jo... arrow_drop_down The Astrophysical JournalOther literature type . Article . 2020 . Peer-reviewedLicense: IOP Copyright PoliciesHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ab6a94&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 50 citations 50 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert The Astrophysical Jo... arrow_drop_down The Astrophysical JournalOther literature type . Article . 2020 . Peer-reviewedLicense: IOP Copyright PoliciesHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ab6a94&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Article , Other literature type 2022 France, France, France, France, GermanyPublisher:Copernicus GmbH Funded by:EC | IMMERSE, NSF | EarthCube Data Capabiliti..., NSF | NSFGEO-NERC: Collaborativ... +3 projectsEC| IMMERSE ,NSF| EarthCube Data Capabilities: A Cloud-Native Data Repository for the Geoscience Community ,NSF| NSFGEO-NERC: Collaborative Research: Assessing the influence of sub-annual variability in the AMOC on the Gulf Stream and the atmosphere ,ANR| CONTACTS ,ANR| DEEPER ,EC| ESiWACE2T. Uchida; J. Le Sommer; C. Stern; R. P. Abernathey; C. Holdgraf; A. Albert; L. Brodeau; L. Brodeau; E. P. Chassignet; X. Xu; J. Gula; J. Gula; G. Roullet; N. Koldunov; S. Danilov; Q. Wang; D. Menemenlis; C. Bricaud; B. K. Arbic; J. F. Shriver; F. Qiao; B. Xiao; A. Biastoch; A. Biastoch; R. Schubert; R. Schubert; B. Fox-Kemper; W. K. Dewar; W. K. Dewar; A. Wallcraft;Abstract. With the increase in computational power, ocean models with kilometer-scale resolution have emerged over the last decade. These models have been used for quantifying the energetic exchanges between spatial scales, informing the design of eddy parametrizations, and preparing observing networks. The increase in resolution, however, has drastically increased the size of model outputs, making it difficult to transfer and analyze the data. It remains, nonetheless, of primary importance to assess more systematically the realism of these models. Here, we showcase a cloud-based analysis framework proposed by the Pangeo project that aims to tackle such distribution and analysis challenges. We analyze the output of eight submesoscale-permitting simulations, all on the cloud, for a crossover region of the upcoming Surface Water and Ocean Topography (SWOT) altimeter mission near the Gulf Stream separation. The cloud-based analysis framework (i) minimizes the cost of duplicating and storing ghost copies of data and (ii) allows for seamless sharing of analysis results amongst collaborators. We describe the framework and provide example analyses (e.g., sea-surface height variability, submesoscale vertical buoyancy fluxes, and comparison to predictions from the mixed-layer instability parametrization). Basin- to global-scale, submesoscale-permitting models are still at their early stage of development; their cost and carbon footprints are also rather large. It would, therefore, benefit the community to document the different model configurations for future best practices. We also argue that an emphasis on data analysis strategies would be crucial for improving the models themselves.
OceanRep; Geoscienti... arrow_drop_down Geoscientific Model Development (GMD)Other literature type . 2022Data sources: Copernicus PublicationsElectronic Publication Information CenterArticle . 2022Data sources: Electronic Publication Information CenterArchiMer - Institutional Archive of IfremerOther literature type . 2022Data sources: ArchiMer - Institutional Archive of IfremerINRIA a CCSD electronic archive server; Mémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2022License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-15-5829-2022&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesgold 8 citations 8 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert OceanRep; Geoscienti... arrow_drop_down Geoscientific Model Development (GMD)Other literature type . 2022Data sources: Copernicus PublicationsElectronic Publication Information CenterArticle . 2022Data sources: Electronic Publication Information CenterArchiMer - Institutional Archive of IfremerOther literature type . 2022Data sources: ArchiMer - Institutional Archive of IfremerINRIA a CCSD electronic archive server; Mémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2022License: CC BYadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.5194/gmd-15-5829-2022&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:EDP Sciences Funded by:EC | ExoplANETS A, UKRI | Quota Studentship 2012, EC | EXOLIGHTS +6 projectsEC| ExoplANETS A ,UKRI| Quota Studentship 2012 ,EC| EXOLIGHTS ,UKRI| DiRAC 2.5 Operations 2017-2020 ,EC| ATMO ,UKRI| A comprehensive study of stars, disks and exoplanets ,UKRI| DiRAC2: 100 Tflop/s HPC cluster procurement ,UKRI| The DiRAC 2.5x Facility ,EC| ExoAIBenjamin Drummond; Eric Hébrard; Nathan J. Mayne; Olivia Venot; Robert J. Ridgway; Quentin Changeat; Shang-Min Tsai; James Manners; Pascal Tremblin; Nathan Luke Abraham; David K. Sing; Krisztian Kohary;We present results from a set of simulations using a fully coupled three-dimensional (3D) chemistry-radiation-hydrodynamics model and investigate the effect of transport of chemical species by the large-scale atmospheric flow in hot Jupiter atmospheres. We couple a flexible chemical kinetics scheme to the Met Office Unified Model which enables the study of the interaction of chemistry, radiative transfer and fluid dynamics. We use a newly-released "reduced" chemical network comprising 30 chemical species that has been specifically developed for application in 3D atmosphere models. We simulate the atmospheres of the well-studied hot Jupiters HD~209458b and HD~189733b which both have dayside--nightside temperature contrasts of several hundred Kelvin and superrotating equatorial jets. We find qualitatively quite different chemical structures between the two planets, particularly for methane (CH$_4$), when advection of chemical species is included. Our results show that consideration of 3D chemical transport is vital in understanding the chemical composition of hot Jupiter atmospheres. 3D mixing leads to significant changes in the abundances of absorbing gas-phase species compared with what would be expected by assuming local chemical equilibrium, or from models including 1D - and even 2D - chemical mixing. We find that CH$_4$, carbon dioxide (CO$_2$) and ammonia (NH$_3$) are particularly interesting as 3D mixing of these species leads to prominent signatures of out-of-equilibrium chemistry in the transmission and emission spectra, detectable with near-future instruments. Comment: Accepted in A&A
arXiv.org e-Print Ar... arrow_drop_down Astronomy and AstrophysicsOther literature type . Article . 2020 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937153&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 55 citations 55 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down Astronomy and AstrophysicsOther literature type . Article . 2020 . Peer-reviewedLicense: EDP Sciences Copyright and Publication Licensing PolicyHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1051/0004-6361/201937153&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Preprint 2020 FrancePublisher:American Astronomical Society Funded by:EC | ATMO, EC | ExoAI, UKRI | Quota Studentship 2012 +1 projectsEC| ATMO ,EC| ExoAI ,UKRI| Quota Studentship 2012 ,EC| ExoplANETS AOlivia Venot; Vivien Parmentier; Jasmina Blecic; Patricio E. Cubillos; Ingo Waldmann; Quentin Changeat; Julianne I. Moses; Pascal Tremblin; Nicolas Crouzet; Peter Gao; Diana Powell; Pierre Olivier Lagage; Ian Dobbs-Dixon; Maria Steinrueck; Laura Kreidberg; Natalie M. Batalha; Jacob L. Bean; Kevin B. Stevenson; Sarah L. Casewell; Ludmila Carone;The James Webb Space Telescope (JWST) is expected to revolutionize the field of exoplanets. The broad wavelength coverage and the high sensitivity of its instruments will allow characterization of exoplanetary atmospheres with unprecedented precision. Following the Call for the Cycle 1 Early Release Science Program, the Transiting Exoplanet Community was awarded time to observe several targets, including WASP-43b. The atmosphere of this hot Jupiter has been intensively observed but still harbors some mysteries, especially concerning the day-night temperature gradient, the efficiency of the atmospheric circulation, and the presence of nightside clouds. We will constrain these properties by observing a full orbit of the planet and extracting its spectroscopic phase curve in the 5--12 $\mu$m range with JWST/MIRI. To prepare for these observations, we performed an extensive modeling work with various codes: radiative transfer, chemical kinetics, cloud microphysics, global circulation models, JWST simulators, and spectral retrieval. Our JWST simulations show that we should achieve a precision of 210 ppm per 0.1 $\mu$m spectral bin on average, which will allow us to measure the variations of the spectrum in longitude and measure the night-side emission spectrum for the first time. If the atmosphere of WASP-43b is clear, our observations will permit us to determine if its atmosphere has an equilibrium or disequilibrium chemical composition, providing eventually the first conclusive evidence of chemical quenching in a hot Jupiter atmosphere. If the atmosphere is cloudy, a careful retrieval analysis will allow us to identify the cloud composition. Comment: 26 pages, 16 figures, accepted in The Astrophysical Journal
The Astrophysical Jo... arrow_drop_down The Astrophysical JournalOther literature type . Article . 2020 . Peer-reviewedLicense: IOP Copyright PoliciesHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ab6a94&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen hybrid 50 citations 50 popularity Top 1% influence Average impulse Top 1% Powered by BIP!more_vert The Astrophysical Jo... arrow_drop_down The Astrophysical JournalOther literature type . Article . 2020 . Peer-reviewedLicense: IOP Copyright PoliciesHAL - UPEC / UPEM; Hal-DiderotArticle . 2020https://doi.org/10.48550/arxiv...Article . 2020License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/1538-4357/ab6a94&type=result"></script>'); --> </script>
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