Knowledge Resource Center for Ecological Environment in Arid Area
DOI | 10.1093/mnras/staa1618 |
Modelling the 3D climate of Venus with OASIS | |
Mendonca, Joao M.; Buchhave, Lars A. | |
通讯作者 | Mendonca, JM |
来源期刊 | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
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ISSN | 0035-8711 |
EISSN | 1365-2966 |
出版年 | 2020 |
卷号 | 496期号:3页码:3512-3530 |
英文摘要 | Flexible 3D models to explore the vast diversity of terrestrial planets and interpret observational data are still in their early stages. In this work, we present OASIS: a novel and flexible 3D virtual planet laboratory. With OASIS we envision a platform that couples self-consistently seven individual modules representing the main physical and chemical processes that shape planetary environments. Additionally, OASIS is capable of producing simulated spectra from different instruments and observational techniques. In this work, we focus on the benchmark test of coupling four of the physical modules: fluid dynamics, radiation, turbulence, and surface/soil. To test the OASIS platform, we produced 3D simulations of the Venus climate and its atmospheric circulation and study how the modelled atmosphere changes with various cloud covers, atmospheric heat capacity, and surface friction. 3D simulations of Venus are challenging because they require long integration times with a computationally expensive radiative transfer code. By comparing OASIS results with observational data, we verify that the new model is able to successfully simulate Venus. With simulated spectra produced directly from the 3D simulations, we explore the capabilities of future missions, like LUVOIR, to observe Venus analogues located at a distance of 10 pc. With OASIS, we have taken the first steps to build a sophisticated and very flexible platform capable of studying the environment of terrestrial planets, which will be an essential tool to characterize observed terrestrial planets and plan future observations. |
英文关键词 | hydrodynamics methods: numerical planets and satellites: atmospheres planets and satellites: terrestrial planets |
类型 | Article |
语种 | 英语 |
收录类别 | SCI-E |
WOS记录号 | WOS:000574919300057 |
WOS关键词 | RUNAWAY GREENHOUSE ; LOWER ATMOSPHERE ; DYNAMICAL CORES ; EARTH ; SURFACE ; TERRESTRIAL ; ABSORPTION ; CLOUDS ; WATER ; SPECTROMETER |
WOS类目 | Astronomy & Astrophysics |
WOS研究方向 | Astronomy & Astrophysics |
资源类型 | 期刊论文 |
条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/326621 |
作者单位 | [Mendonca, Joao M.; Buchhave, Lars A.] Tech Univ Denmark, Natl Space Inst, Elektrovej, DK-2800 Lyngby, Denmark |
推荐引用方式 GB/T 7714 | Mendonca, Joao M.,Buchhave, Lars A.. Modelling the 3D climate of Venus with OASIS[J],2020,496(3):3512-3530. |
APA | Mendonca, Joao M.,&Buchhave, Lars A..(2020).Modelling the 3D climate of Venus with OASIS.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,496(3),3512-3530. |
MLA | Mendonca, Joao M.,et al."Modelling the 3D climate of Venus with OASIS".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 496.3(2020):3512-3530. |
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