Overview of the Venus PCM - Revision history

Mlefevre: /* POULDP Venus */

2026-03-23T16:08:26Z

‎POULDP Venus

2026-03-23T11:13:30Z

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‎Bibliography

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‎2025

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‎Bibliography

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‎Bibliography

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 == POULDP Venus ==
 A POULDP meeting, for Point Organisé et Utile LMDZ Dynamico Planéto (apologies to non-French speakers), is organized between the developers to discuss the development of the model and plan improvements.
 To subscribe to the POULDP mailing list (and/or browse through past messages): https://groupes.renater.fr/sympa/info/pouldp_venus

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 == Getting started ==
 The traditional Venus PCM - LMDZ (formerly know as the IPSL Venus GCM) is the most commonly used version. For a first try at installing running the Venus PCM we recommend you start from the [[Quick Install and Run Venus PCM]] page. You will also most likely be interested in all the pages tagged as "Venus-Model" or "Venus-LMDZ" in the [[Special:Categories|Categories]] section.
 == Bibliography ==

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 Some recent reference articles:
 ==== 2025 ====
 *Lai, D., T. Li, S. Lebonnois, and M. Lefèvre, '''Stationary wave dynamics in Venus's upper clouds: Morphology and forcing from Akatsuki/LIR and Venus planetary climate model analyses''', Astronomy and Astrophysics, 704, A286 (2025). DOI: https://doi.org/10.1051/0004-6361/202557330

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 Some recent reference articles:
 ==== 2025 ====
 *Cohen, M., J. Holmes, S. Lewis, M. Patel, and S. Lebonnois, '''Three Worlds in One: Venus as a Natural Laboratory for the Effect of Rotation Period on Atmospheric Circulation''', The Astrophysical Journal, 980, L11 (2025). DOI: https://doi.org/10.3847/2041-8213/adade9
 ==== 2024 ====
 *Martinez, A., J.-Y. Chaufray, S. Lebonnois, F. Gonzàlez-Galindo, F. Lefèvre, and G. Gilli, '''Three-dimensional Venusian ionosphere model''', Icarus, 415, 116035 (2024). DOI: https://doi.org/10.1016/j.icarus.2024.116035

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 Some recent reference articles:
 ==== 2023 ====
 * Stolzenbach, A.; Lefèvre, F.; Lebonnois, S. and Määttänen, A., '''Three-dimensional modeling of Venus photochemistry and clouds''', Icarus, vol.395, pp.115447 (2023). DOI: https://doi.org/10.1016/j.icarus.2023.115447

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 == The Venus PCM (Planetary Climate Model) ==
-In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core).
+In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or [[WRF dynamical core for LES/mesoscale simulations|'''WRF''']] (limited area dynamical core).
 == Getting started ==

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 * Stolzenbach, A.; Lefèvre, F.; Lebonnois, S. and Määttänen, A., '''Three-dimensional modeling of Venus photochemistry and clouds''', Icarus, vol.395, pp.115447 (2023). DOI: https://doi.org/10.1016/j.icarus.2023.115447
 * Martinez, A.; Lebonnois, S.; Millour, E.; Pierron, T.; Moisan, E.; Gilli, G. and Lefèvre, F., '''Exploring the variability of the venusian thermosphere with the IPSL Venus GCM''', Icarus, vol.389, pp.115272 (2023). DOI: https://doi.org/10.1016/j.icarus.2022.115272
 ==== 2021 ====
 * Navarro, T.; Gilli, G.; Schubert, G.; Lebonnois, S.; Lefèvre, F. and Quirino, D., '''Venus' upper atmosphere revealed by a GCM: I. Structure and variability of the circulation''', Icarus, vol.366, pp.114400 (2021). DOI: https://doi.org/10.1016/j.icarus.2021.114400

← Older revision		Revision as of 13:23, 26 May 2023
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	In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core).		In a nutshell the Venus PCM is a suite of models combining the Venus physics package and a dynamical core which may be LMDZ (the historical lon-lat grid), DYNAMICO (a more recent icosahedral dynamical core) or WRF (limited area dynamical core).

		+	The traditional Venus PCM - LMDZ (formerly know as the IPSL Venus GCM) is the most commonly used version.
		+
		+	== Bibliography ==
		+
		+	TODO: Add reference articles here

−	[Category:Venus-Model]	+	[[Category:Venus-Model]]