Reanalyzing Jupiter ISO/SWS Data through a More Recent Atmospheric Model
dc.contributor.author | Ribeiro, José | |
dc.contributor.author | Machado, Pedro | |
dc.contributor.author | Pérez Hoyos, Santiago ![]() | |
dc.contributor.author | Dias, João A. | |
dc.contributor.author | Irwin, Patrick G.J. | |
dc.date.accessioned | 2024-01-22T16:48:57Z | |
dc.date.available | 2024-01-22T16:48:57Z | |
dc.date.issued | 2023-11-24 | |
dc.identifier.citation | Atmosphere 14(12) : (2023) // Article ID 1731 | es_ES |
dc.identifier.issn | 2073-4433 | |
dc.identifier.uri | http://hdl.handle.net/10810/64207 | |
dc.description.abstract | The study of isotopic ratios in planetary atmospheres gives an insight into the formation history and evolution of these objects. The more we can constrain these ratios, the better we can understand the history and future of our solar system. To help in this endeavour, we used Infrared Space Observatory Short Wavelength Spectrometer (ISO/SWS) Jupiter observations in the 793–1500 cm−1 region together with the Nonlinear Optimal Estimator for MultivariatE Spectral analySIS (NEMESIS) radiative transfer suite to retrieve the temperature–pressure profile and the chemical abundances for various chemical species. We also used the 1500–2499 cm−1 region to determine the cloud and aerosol structure of the upper troposphere. We obtained a best-fit simulated spectrum with 𝜒2/𝑁=0.47 for the 793–1500 cm−1 region and 𝜒2/𝑁=0.71 for the 1500–2499 cm−1 region. From the retrieved methane abundances, we obtained, within a 1𝜎 uncertainty, a 12C/13C ratio of 84 ± 27 and a D/H ratio of (3.5 ± 0.6) × 10−5, and these ratios are consistent with other published results from the literature. | es_ES |
dc.description.sponsorship | This research was funded by the Portuguese Fundação Para a Ciência e Tecnologia through the research grants UIDB/04434/2020 and UIDP/04434/2020 as well as a fellowship grants 2021.04584.BD and 2022.09859.BD. | es_ES |
dc.language.iso | eng | es_ES |
dc.publisher | MDPI | |
dc.rights | info:eu-repo/semantics/openAccess | es_ES |
dc.rights.uri | http://creativecommons.org/licenses/by/4.0/es/ | |
dc.subject | Jupiter | es_ES |
dc.subject | vertical structure | es_ES |
dc.subject | spectroscopy | es_ES |
dc.subject | radiative transfer | es_ES |
dc.title | Reanalyzing Jupiter ISO/SWS Data through a More Recent Atmospheric Model | es_ES |
dc.type | info:eu-repo/semantics/article | es_ES |
dc.date.updated | 2023-12-22T13:45:25Z | |
dc.rights.holder | © 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/ 4.0/). | es_ES |
dc.relation.publisherversion | https://www.mdpi.com/2073-4433/14/12/1731 | es_ES |
dc.identifier.doi | 10.3390/atmos14121731 | |
dc.departamentoes | Física aplicada I | |
dc.departamentoeu | Fisika aplikatua I |
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Except where otherwise noted, this item's license is described as © 2023 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (https://creativecommons.org/licenses/by/ 4.0/).