Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation-Reference-Cited by-同舟云学术

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Venus’ upper atmosphere revealed by a GCM: I. Structure and variability of the circulation

Published:2021-09 Issue: Volume:366 Page:114400
ISSN:0019-1035
Container-title:Icarus
language:en
Short-container-title:Icarus

Author:

Navarro Thomas^ORCID,Gilli Gabriella,Schubert Gerald^ORCID,Lebonnois Sébastien^ORCID,Lefèvre Franck^ORCID,Quirino Diogo^ORCID

Funder

EU Framework Programme for Research and Innovation Marie Sklodowska-Curie Actions

Fundação para a Ciência e a Tecnologia

Grand Equipement National De Calcul Intensif

NASA

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference107 articles.

1. The puzzling Venusian polar atmospheric structure reproduced by a general circulation model;Ando;Nature Commun.,2016

2. Cloud patterns, waves and convection in the Venus atmosphere;Belton;J. Atmos. Sci.,1976

3. Influence of venus topography on the zonal wind and UV albedo at cloud top level: The role of stationary gravity waves;Bertaux;J. Geophys. Res. (Planets),2016

4. A warm layer in venus’ cryosphere and high-altitude measurements of HF, HCl, H2O and HDO;Bertaux;Nature,2007

5. Upper atmosphere dynamics: Global circulation and gravity waves;Bougher,1997

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1. The Venus Global Ionosphere‐Thermosphere Model (V‐GITM): A Coupled Thermosphere and Ionosphere Formulation;Journal of Geophysical Research: Planets;2024-07

2. Venus water loss is dominated by HCO+ dissociative recombination;Nature;2024-05-06

3. One-dimensional Microphysics Model of Venusian Clouds from 40 to 100 km: Impact of the Middle-atmosphere Eddy Transport and SOIR Temperature Profile on the Cloud Structure;The Planetary Science Journal;2024-03-01

4. Mountain Waves in the Upper Atmosphere of Venus;Geophysical Research Letters;2024-02-09

5. O2 (а1Δg) Airglow at 1.27 μM and upper Mesosphere Dynamics on the Night Side of Venus;Solar System Research;2023-06

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