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The radiative-convective equilibrium structures and thermodynamic properties of the Venus atmosphere

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posted on 2023-09-29, 15:04 authored by Yoshiyuki Takahashi, Yoshi-Yuki Hayashi, George Hashimoto, Kiyoshi Kuramoto, Masaki Ishiwatari, Hiroki Kashimura

This is a dataset for the one-dimensional radiative-convective equilibrium structures of the Venus atmosphere calculated with several thermodynamic models. Associated thermodynamic properties of the Venus atmosphere are also included. 

These data can be used to reproduce figures of Takahashi et al. (2024) (https://doi.org/10.2151/jmsj.2024-001). The NetCDF file named data_FigXX_*.nc includes data for Figure XX of Takahashi et al. (2024) except for data which appeared in other sources. 

Funding

Modeling of water and material circulations in the solar system objects

Japan Society for the Promotion of Science

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Comprehensive picture of atmospheric circulation of Venus revealed by AKATSUKI data assimilation

Japan Society for the Promotion of Science

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Numerical exploration of the thermal structure of the lower atmosphere of Venus

Japan Society for the Promotion of Science

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History

Corresponding author email address

yot@gfd-dennou.org

Title (in Japanese)

金星大気の放射対流平衡構造と熱力学特性

Manuscript title (in Japanese)

金星下層大気の放射対流平衡構造の熱力学モデル依存性

Authors (in Japanese)

高橋芳幸, 林祥介, はしもとじょーじ, 倉本圭, 石渡正樹, 樫村博基

Copyright

© The Author(s) 2023

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    気象集誌/Journal of the Meteorological Society of Japan

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