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2024-12-10T11:12:24Z

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2024-11-29T16:06:46Z

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2023-05-26T13:03:10Z

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** Overview_of_the_Generic_PCM|Overview of the Generic PCM
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2023-04-06T12:53:01Z

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** Overview_of_the_Generic_PCM|Overview of the Generic PCM
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2023-04-06T12:49:05Z

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** Overview_of_the_Generic_PCM|Overview of the Generic PCM
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2023-03-30T07:31:32Z

Adminplanets:

Main Page

2023-03-27T14:35:54Z

Adminplanets:

Welcome to the wiki of the Planetary Climate Models (PCM) family! Use the menu on the left to navigate across our webpages.

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2023-03-27T14:34:26Z

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2023-03-27T14:33:49Z

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2023-03-27T14:33:06Z

Adminplanets:

* Generic Models (exoplanets, giant planets)
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Overview of the Generic PCM

2022-07-20T11:41:25Z

Adminplanets: Created page with "== What is a GCM? == Our Global Climate Model (GCM) calculates the temporal evolution of the different variables (temperature, pressure, mass, mixing ratio of tracers/gas/clo..."

== What is a GCM? ==

Our Global Climate Model (GCM) calculates the temporal evolution of the different variables (temperature, pressure, mass, mixing ratio of tracers/gas/clouds, winds, etc.) that control or describe the planetary meteorology and climate at different points of a 3D “grid” that covers the entire atmosphere.

From an initial state, the model calculates the temporal evolution of these variables, one timestep after another:
* At instant t, variables Xt (temperature for example) are known at every grid point of the atmosphere.
* We calculate the evolution (the tendencies) (δX/δt)1, (δX/δt)2, etc.) due to each physical phenomenon, calculated via the parameterization thereof (e.g., heating due to absorption of solar radiation, mixing due to turbulence in the planetary boundary layer, etc.).
* In order to move on to the next time step, t + δt, we can calculate Xt+δt from Xt and (δX/δt). This is formally known as the time integration of the variables. (For example, Xt+δt = Xt + (δX/δt)1δt + (δX/δt)2δt + ...)

The main task of the model is to calculate these tendencies (δX/δt) arising from the different parameterized phenomena.

TO BE MODIFIED (AND COMPLETED) by Jeremy

[[File:Didi-eps-converted-to-1.png|thumb|Physics / Dynamics interface]]

== Physical vs dynamical core ==

In practice, the 3D model is split in two components:

* '''a dynamical core''' containing the numerical solution of the general equations for atmospheric circulation. This component (including source code) is common to all terrestrial-type atmospheres, and applicable in certain cases to the upper atmospheres of gas giant planets.
* '''a physical package''' that is specific to the planet in question (as it takes into account dedicated parametrizations representative of ongoing physical processes) and which computes atmospheric processes in each atmospheric column (which are sub-grid-scale from the point of view of the dynamical core).

In practice, we do have several '''dynamical cores''' available with the model: LMDZ (global longitude/latitude grid), DYNAMICO (icosaedric grid) and WRF (rectangular box for local/regional studies)

TO BE MODIFIED (AND COMPLETED) by Aymeric

== GCM inputs and outputs ==

[[File:Inout-eps-converted-to-1.png|thumb|input/output data]]

The input files are the files needed to initialize the model (state of the atmosphere at instant t0 as well as a dataset of boundary conditions). The output files are “historical files”, archives of the atmospheric flow history as simulated by the model, the “diagfi files”, the “stats files”, the daily averages, and so on.

TO BE COMPLETED

==== start and startfi files ====

TO BE COMPLETED

==== start vs restart files ====

TO BE COMPLETED

==== .def files ====

List of needed .def files:
<ul>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_callphys.def_Input_File ''callphys.def'']: Physical parameters</li>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_run.def_Input_File ''run.def'']: Numerical parameters</li>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_gases.def_Input_File ''gases.def'']: List of gases</li>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_traceur.def_Input_File ''traceur.def'']: Numerical traceurs in the atmosphere</li>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_z2sig.def_Input_File ''z2sig.def'']: Pseudo-altitudes (in km) at which the user wants to set the vertical levels</li>
<li> [https://lmdz-forge.lmd.jussieu.fr/mediawiki/Planets/index.php/The_diagfi.def_Input_File ''diagfi.def''] (optionnal): List of wanted outputs</li>
</ul>

==== input data ====

TO BE COMPLETED

==== output files ====

diagfi.nc
diagspec_IR.nc / diagspec_VI.nc
stats.nc
etc.

TO BE COMPLETED

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2022-07-20T11:40:12Z

Adminplanets:

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2022-07-20T11:39:50Z

Adminplanets:

Useful Examples

2022-07-20T11:38:23Z

Adminplanets:

== Editing convention ==
*Name of the files: ''italic''

== To Edit Sidebar (as admin only!!!) ==
Go to [[MediaWiki:Sidebar]]

== To write some LateX ==
See e.g. [https://lmdz-forge.lmd.jussieu.fr/mediawiki/LMDZPedia/index.php/ExempleMaths LMDZPedia]
And check out this page in "edit" mode!

$$\newcommand{\Re}{\mathrm{Re}\,}
\newcommand{\pFq}[5]{{}_{#1}\mathrm{F}_{#2} \left( \genfrac{}{}{0pt}{}{#3}{#4} \bigg| {#5} \right)}$$

We consider, for various values of $$s$$, the $$n$$-dimensional integral
\begin{align}
\label{def:Wns}
W_n (s)
&:=
\int_{[0, 1]^n}
\left| \sum_{k = 1}^n \mathrm{e}^{2 \pi \mathrm{i} \, x_k} \right|^s \mathrm{d}\boldsymbol{x}
\end{align}
which occurs in the theory of uniform random walk integrals in the plane,
where at each step a unit-step is taken in a random direction. As such,
the integral \eqref{def:Wns} expresses the $$s$$-th moment of the distance
to the origin after $$n$$ steps.

By experimentation and some sketchy arguments we quickly conjectured and
strongly believed that, for $$k$$ a nonnegative integer
\begin{align}
\label{eq:W3k}
W_3(k) &= \Re \, \pFq32{\frac12, -\frac k2, -\frac k2}{1, 1}{4}.
\end{align}

Appropriately defined, \eqref{eq:W3k} also holds for negative odd integers.
The reason for \eqref{eq:W3k} was long a mystery, but it will be explained
at the end of the paper.

== Miscellaneous ==
* HTML like syntax works! e.g. comments with

<pre>

which you see because between "pre" tags
</pre>

* Some special features:
Link to the internal page with all special features: [[Special:Version]]

* Examples of Syntax Highlighting:
Some Fortran Code:
<syntaxhighlight lang="fortran" line>
program truc
implicit none
integer :: i
do i=1,10
write(*,*) "i=",i," for each hello planeto world"
end do
end program
</syntaxhighlight>

Some Python Code:
<syntaxhighlight lang="python" line>
import numpy
import matplotlib as plt
for i in range(0,5,1):
print('hello planeto world")
plt.show()
</syntaxhighlight>

Some bash code:
<syntaxhighlight lang="bash" line>
echo 'hello planeto world'
</syntaxhighlight>

== How to create a new page ==
Option 1: Make a link to that page from a currently existing page, and when you click on that link (will be displayed in red as the system notices that it is a broken link) and the system will ask you if you want to create the page. A reminder on how to add (code-wise) a link to another MediaWiki page (try to follow CamelCase formatting, see option 2 below):
<pre>
[[Link_To_Some_Page|some descriptive text]]
</pre>
which will be rendered as:
[[Link_To_Some_Page|some descriptive text]]

Option 2: Look for it via the search bar! Advice: you should use CamelCase formating (with a "_" between words) as this page name will end up also being the title of the page (with the "_" replaced by spaces), e.g. The_Best_Page_Ever

== Link to the Generic PCM user manual ==

link to the one on the trac which is what is on svn and thus will always be up to date:
https://trac.lmd.jussieu.fr/Planeto/browser/trunk/LMDZ.GENERIC/ManualGCM_GENERIC.pdf

How to Cite

2022-07-20T11:37:32Z

Adminplanets:

= Main reference to cite the Generic PCM =

* Wordsworth et al. 2011 ?
* Forget et al., in preparation ?

= How to cite? (process by process) =

== slab ocean ==

Codron 2012 https://link.springer.com/article/10.1007/s00382-011-1031-3
Charnay, B.; Forget, F.; Wordsworth, R.; Leconte, J.; Millour, E.; Codron, F. and Spiga, A., Exploring the faint young Sun problem and the possible climates of the Archean Earth with a 3-D GCM, Journal of Geophysical Research (Atmospheres), vol.118, pp.10,414 (2013)

== CO2 ice clouds ==

Forget, F.; Wordsworth, R.; Millour, E.; Madeleine, J. B.; Kerber, L.; Leconte, J.; Marcq, E. and Haberle, R. M., 3D modelling of the early martian climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds, Icarus, vol.222, pp.81 (2013)

== etc. ==

= List of all references (using the Generic PCM) =

=== terrestrial exoplanets ===

Wordsworth, R. D.; Forget, F.; Selsis, F.; Millour, E.; Charnay, B. and Madeleine, J.-B., Gliese 581d is the First Discovered Terrestrial-mass Exoplanet in the Habitable Zone, The Astrophysical Journal, vol.733, pp.L48 (2011)

Leconte, J.; Forget, F.; Charnay, B.; Wordsworth, R.; Selsis, F.; Millour, E. and Spiga, A., 3D climate modeling of close-in land planets: Circulation patterns, climate moist bistability, and habitability, Astronomy and Astrophysics, vol.554, pp.A69 (2013)

Emeline's paper on eccentric exoplanets

Turbet, M.; Leconte, J.; Selsis, F.; Bolmont, E.; Forget, F.; Ribas, I.; Raymond, S. N. and Anglada-Escudé, G., The habitability of Proxima Centauri b. II. Possible climates and observability, Astronomy and Astrophysics, vol.596, pp.A112 (2016)

Turbet, M.; Forget, F.; Leconte, J.; Charnay, B. and Tobie, G., CO2 condensation is a serious limit to the deglaciation of Earth-like planets, Earth and Planetary Science Letters, vol.476, pp.11 (2017)

Turbet, M.; Bolmont, E.; Leconte, J.; Forget, F.; Selsis, F.; Tobie, G.; Caldas, A.; Naar, J. and Gillon, M., Modeling climate diversity, tidal dynamics and the fate of volatiles on TRAPPIST-1 planets, Astronomy and Astrophysics, vol.612, pp.A86 (2018)

Fauchez, T. J.; Turbet, M.; Villanueva, G. L.; Wolf, E. T.; Arney, G.; Kopparapu, R. K.; Lincowski, A.; Mandell, A.; de Wit, J.; Pidhorodetska, D.; Domagal-Goldman, S. D. and Stevenson, K. B., Impact of Clouds and Hazes on the Simulated JWST Transmission Spectra of Habitable Zone Planets in the TRAPPIST-1 System, The Astrophysical Journal, vol.887, pp.194 (2019)

=== super-Earths ===

Leconte, J.; Forget, F.; Charnay, B.; Wordsworth, R.; Selsis, F.; Millour, E. and Spiga, A., 3D climate modeling of close-in land planets: Circulation patterns, climate moist bistability, and habitability, Astronomy and Astrophysics, vol.554, pp.A69 (2013)

=== mini-Neptunes ===

Benjamin's two papers on GJ1214b

Charnay, B.; Blain, D.; Bézard, B.; Leconte, J.; Turbet, M. and Falco, A., Formation and dynamics of water clouds on temperate sub-Neptunes: the example of K2-18b, Astronomy and Astrophysics, vol.646, pp.A171 (2021)

=== LES ===
Lefèvre, M.; Turbet, M. and Pierrehumbert, R., 3D Convection-resolving Model of Temperate, Tidally Locked Exoplanets, The Astrophysical Journal, vol.913, pp.101 (2021)

== paleoclimates ==

=== Earth ===

Charnay, B.; Forget, F.; Wordsworth, R.; Leconte, J.; Millour, E.; Codron, F. and Spiga, A., Exploring the faint young Sun problem and the possible climates of the Archean Earth with a 3-D GCM, Journal of Geophysical Research (Atmospheres), vol.118, pp.10,414 (2013)

Charnay, B.; Le Hir, G.; Fluteau, F.; Forget, F. and Catling, D. C., A warm or a cold early Earth? New insights from a 3-D climate-carbon model, Earth and Planetary Science Letters, vol.474, pp.97 (2017)

Turbet, M.; Bolmont, E.; Chaverot, G.; Ehrenreich, D.; Leconte, J. and Marcq, E., Day-night cloud asymmetry prevents early oceans on Venus but not on Earth, Nature, vol.598, pp.276 (2021)

=== Mars ===

Forget, F.; Wordsworth, R.; Millour, E.; Madeleine, J. B.; Kerber, L.; Leconte, J.; Marcq, E. and Haberle, R. M., 3D modelling of the early martian climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds, Icarus, vol.222, pp.81 (2013)

Wordsworth, R.; Forget, F.; Millour, E.; Head, J. W.; Madeleine, J. B. and Charnay, B., Global modelling of the early martian climate under a denser CO2 atmosphere: Water cycle and ice evolution, Icarus, vol.222, pp.1 (2013)

Wordsworth, R. D.; Kerber, L.; Pierrehumbert, R. T.; Forget, F. and Head, J. W., Comparison of "warm and wet" and "cold and icy" scenarios for early Mars in a 3-D climate model, Journal of Geophysical Research (Planets), vol.120, pp.1201 (2015)

Kerber, L.; Forget, F. and Wordsworth, R., Sulfur in the early martian atmosphere revisited: Experiments with a 3-D Global Climate Model, Icarus, vol.261, pp.133 (2015)

Turbet, M.; Forget, F.; Head, J. W. and Wordsworth, R., 3D modelling of the climatic impact of outflow channel formation events on early Mars, Icarus, vol.288, pp.10 (2017)

Turbet, M. and Forget, F., The paradoxes of the Late Hesperian Mars ocean, Scientific Reports, vol.9, pp.5717 (2019)

Turbet, M.; Gillmann, C.; Forget, F.; Baudin, B.; Palumbo, A.; Head, J. and Karatekin, O., The environmental effects of very large bolide impacts on early Mars explored with a hierarchy of numerical models, Icarus, vol.335, pp.113419 (2020)

=== Venus ===

Turbet, M.; Bolmont, E.; Chaverot, G.; Ehrenreich, D.; Leconte, J. and Marcq, E., Day-night cloud asymmetry prevents early oceans on Venus but not on Earth, Nature, vol.598, pp.276 (2021)

=== Titan ===

Charnay, B.; Forget, F.; Tobie, G.; Sotin, C. and Wordsworth, R., Titan's past and future: 3D modeling of a pure nitrogen atmosphere and geological implications, Icarus, vol.241, pp.269 (2014)
DOI: 10.1016/j.icarus.2014.07.009

== future climates ==

=== Earth ===

Leconte, J.; Forget, F.; Charnay, B.; Wordsworth, R. and Pottier, A., Increased insolation threshold for runaway greenhouse processes on Earth-like planets, Nature, vol.504, pp.268 (2013)

== gas giants ==

=== Saturn ===

==== Saturn radiative transfer model ====
Guerlet, S.; Spiga, A.; Sylvestre, M.; Indurain, M.; Fouchet, T.; Leconte, J.; Millour, E.; Wordsworth, R.; Capderou, M.; Bézard, B. and Forget, F., Global climate modeling of Saturn’s atmosphere. Part I: Evaluation of the radiative transfer model, Icarus, vol.238, pp.110 (2014)
DOI: 10.1016/j.icarus.2014.05.010

==== Saturn DYNAMICO GCM tropospheric dynamics ====
Spiga, A.; Guerlet, S.; Millour, E.; Indurain, M.; Meurdesoif, Y.; Cabanes, S.; Dubos, T.; Leconte, J.; Boissinot, A.; Lebonnois, S.; Sylvestre, M. and Fouchet, T., Global climate modeling of Saturn's atmosphere. Part II: Multi-annual high-resolution dynamical simulations, Icarus, vol.335, pp.113377 (2020)
DOI: 10.1016/j.icarus.2019.07.011

==== Saturn DYNAMICO GCM statistical analysis of the zonostrophic dynamics ====
Cabanes, S.; Spiga, A. and Young, R. M. B ., Global climate modeling of Saturn's atmosphere. Part III: Global statistical picture of zonostrophic turbulence in high-resolution 3D-turbulent simulations, Icarus, vol.345, pp. 113705 (2020)
DOI: 10.1016/j.icarus.2020.113705

==== Saturn DYNAMICO GCM stratospheric dynamics ====
Bardet, D.; Spiga, A.; Guerlet, S.; Cabanes, S.; Millour, E. and Boissinot, A., Global climate modeling of Saturn's atmosphere. Part IV: Stratospheric equatorial oscillation, Icarus, vol.354, pp. 114042 (2021)
DOI: 10.1016/j.icarus.2020.114042

Bardet, D.; Spiga, A. and Guerlet, S., Joint evolution of equatorial oscillation and inter-hemispheric circulation in Saturn’s stratosphere, Nature Astronomy (2022)
DOI: 10.1038/s41550-022-01670-7

=== Jupiter ===
==== Jupiter radiative transfer model ====
Guerlet, S.; Spiga, A.; Delattre, H. and Fouchet, T., Radiative-equilibrium model of Jupiter's atmosphere and application to estimating stratospheric circulations, Icarus, vol.351, pp. 113935 (2020)
DOI: 10.1016/j.icarus.2020.113935

=== Uranus ===

=== Neptune ===

MediaWiki:Sidebar

2022-05-11T10:41:22Z

Adminplanets:

MediaWiki:Sidebar

2022-04-08T12:05:36Z

Adminplanets:

MediaWiki:Sidebar

2022-04-08T12:04:35Z

Adminplanets:

How to Cite

2022-04-06T20:13:05Z

Adminplanets: /* Other references */

= Main reference to cite the LMD Generic GCM =

= Other (more specialized) references =

== exoplanets ==

=== terrestrial exoplanets ===

=== super-Earths ===

=== mini-Neptunes ===

== paleoclimates ==

=== Earth ===

=== Mars ===

=== Venus ===

=== Titan ===

== gas giants ==

=== Jupiter ===

==== Saturn ====

==== Uranus ====

==== Neptune ====

Tool Box

2022-04-06T20:10:04Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|thumb|Screenshot of panoply showing here LMD Generic results for the exoplanet TRAPPIST-1e]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:09:32Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|thumb|Screenshot of panoply]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:08:53Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|thumb]]

[[File:Example panoply.png|thumb|Légende de l'image.]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:08:01Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|thumb]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:07:50Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|test]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:06:10Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example panoply.png|thumb]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:05:37Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example.jpg|thumb]]

[[File:Example panoply.png|thumb]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T20:05:02Z

Adminplanets: /* Panoply */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===

[[File:Example.jpg|thumb]]

[[File:Example.jpg|thumb]]

=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

File:Example panoply.png

2022-04-06T20:03:51Z

Adminplanets:

How to Cite

2022-04-06T19:58:40Z

Adminplanets:

= Main reference to cite the LMD Generic GCM =

= Other references =

== exoplanets ==

=== terrestrial exoplanets ===

=== super-Earths ===

=== mini-Neptunes ===

== paleoclimates ==

=== Earth ===

=== Mars ===

=== Venus ===

=== Titan ===

== gas giants ==

=== Jupiter ===

==== Saturn ====

==== Uranus ====

==== Neptune ====

How to Cite

2022-04-06T19:57:51Z

Adminplanets:

== Main reference to cite the LMD Generic GCM ==

== Other references ==

=== exoplanets ===

==== terrestrial exoplanets ====

==== super-Earths ====

==== mini-Neptunes ====

=== paleoclimates ===

==== Earth ====

==== Mars ====

==== Venus ====

==== Titan ====

=== gas giants ===

==== Jupiter ====

==== Saturn ====

==== Uranus ====

==== Neptune ====

Advanced Use of the GCM

2022-04-06T19:53:36Z

Adminplanets:

== Running in parallel ==

== Distinctions beween ifort, mpi, etc. ==

== Distinction between using IOIPSL or XIOS ==

== How to Change Vertical and Horizontal Resolutions ==

== How to Change the Topography (or remove it) ==

== How to Change the Opacity Tables ==

== How to Manage Tracers ==

Tool Box

2022-04-06T19:52:53Z

Adminplanets: /* Post-processing tools */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast ===
=== mass stream function ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===
=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T19:52:25Z

Adminplanets: /* scripts */

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast, mass stream function, etc. ===

== Continuing Simulations ==
=== bash scripts ===

== Visualization software ==
=== Panoply ===
=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Tool Box

2022-04-06T19:52:11Z

Adminplanets:

== Pre-processing Tools ==
=== newstart ===
=== start2archive ===
=== visualization tools ===
=== other third party scripts and tools ===

== Post-processing tools ==
=== zrecast, mass stream function, etc. ===

== Continuing Simulations ==
=== scripts ===

== Visualization software ==
=== Panoply ===
=== ncview ===
=== paraview ===
=== planetoplot ===
=== python scripts ===

Other GCM Configurations worth knowing about

2022-04-06T19:50:52Z

Adminplanets:

== 3D lon-lat LMDZ setup ==
=== Earth with slab ocean ===
=== TRAPPIST-1e ===
=== mini-Neptune GJ1214b ===

== 3D DYNAMICO setup ==
=== Jupiter with DYNAMICO ===
=== Hot Jupiter with DYNAMICO ===

== 1D setup ==

=== rcm1d test case ===
=== kcm1d test case ===

Quick Install and Run

2022-04-06T19:50:23Z

Adminplanets:

== Tools and Libraries ==
* Fortran compiler (install with gfortran)
* NetCDF + references to visualization tools (ncview, paraview, grads, etc.)
* svn
* FCM
* IOIPSL

== Data ==
* datadir + starts + other GCM data for test case early Mars (desert planet with a CO2 atmosphere)

== Compiling ==
* prepare and explain arch files
* compiling a test case (early Mars)

== Running ==
* run your first simulation

== Checking the Results ==
* everything is cool in the .out file
* tools to visualize the produced diagfi.nc file: panoply, ncview, paraview, etc.

Quick Install and Run

2022-04-06T19:49:59Z

Adminplanets:

= Prerequisites and Download Instructions =

== Tools and Libraries ==
* Fortran compiler (install with gfortran)
* NetCDF + references to visualization tools (ncview, paraview, grads, etc.)
* svn
* FCM
* IOIPSL

== Data ==
* datadir + starts + other GCM data for test case early Mars (desert planet with a CO2 atmosphere)

== Compiling ==
* prepare and explain arch files
* compiling a test case (early Mars)

== Running ==
* run your first simulation

== Checking the Results ==
* everything is cool in the .out file
* tools to visualize the produced diagfi.nc file: panoply, ncview, paraview, etc.

Other GCM Configurations worth knowing about

2022-04-06T19:47:39Z

Adminplanets:

=== 3D lon-lat LMDZ setup ===
==== Earth with slab ocean ====
==== TRAPPIST-1e ====
==== mini-Neptune GJ1214b ====

=== 3D DYNAMICO setup ===
==== Jupiter with DYNAMICO ====
==== Hot Jupiter with DYNAMICO ====

=== 1D setup ===

==== rcm1d test case ====
==== kcm1d test case ====

Other GCM Configurations worth knowing about

2022-04-06T19:46:30Z

Adminplanets:

=== 3D lon-lat LMDZ setup ===
* Earth with slab ocean
* TRAPPIST-1e
* mini-Neptune GJ1214b

=== 3D DYNAMICO setup ===
* Jupiter with DYNAMICO
* Hot Jupiter with DYNAMICO

=== 1D setup ===

==== rcm1d test case ====
==== kcm1d test case ====

Other GCM Configurations worth knowing about

2022-04-06T19:45:57Z

Adminplanets:

Other GCM Configurations worth knowing about

2022-04-06T19:45:39Z

Adminplanets: Created page with "== List of other Configurations wotrh knowing about == === 3D lon-lat LMDZ setup === * Earth with slab ocean * TRAPPIST-1e * mini-Neptune GJ1214b === 3D DYNAMICO setup === *..."

== List of other Configurations wotrh knowing about ==

=== 3D lon-lat LMDZ setup ===
* Earth with slab ocean
* TRAPPIST-1e
* mini-Neptune GJ1214b

=== 3D DYNAMICO setup ===
* Jupiter with DYNAMICO
* Hot Jupiter with DYNAMICO

=== 1D setup ===
* rcm1d test case
* kcm1d test case

Tool Box

2022-04-06T19:45:13Z

Adminplanets: Created page with "= Tool Box = == Pre-processing Tools == * newstart * start2archive * visualization tools * other third party scripts and tools == Post-processing tools == * zrecast, mass s..."

= Tool Box =

== Pre-processing Tools ==
* newstart
* start2archive
* visualization tools
* other third party scripts and tools

== Post-processing tools ==
* zrecast, mass stream function, etc.

== Continuing Simulations ==
* scripts

== Visualization software ==
* Panoply, ncview, paraview, planetoplot, python scripts, etc.

Advanced Use of the GCM

2022-04-06T19:44:40Z

Adminplanets: Created page with "== Advanced Use of the GCM == === Running in parallel === === Distinctions beween ifort, mpi, etc. === === Distinction between using IOIPSL or XIOS === === How to Change V..."

== Advanced Use of the GCM ==

=== Running in parallel ===

=== Distinctions beween ifort, mpi, etc. ===

=== Distinction between using IOIPSL or XIOS ===

=== How to Change Vertical and Horizontal Resolutions ===

=== How to Change the Topography (or remove it) ===

=== How to Change the Opacity Tables ===

=== How to Manage Tracers ===

How to Cite

2022-04-06T19:44:14Z

Adminplanets: Created page with "This is a new page * Citation 1 * Citation 2"

This is a new page

* Citation 1
* Citation 2

Help

2022-04-06T19:43:41Z

Adminplanets: Created page with "ask Ehouarn Also, use the '''Search Box''' at the top of the page !!!"

ask Ehouarn

Also, use the '''Search Box''' at the top of the page !!!

MediaWiki:Sidebar

2022-04-06T19:42:42Z

Adminplanets:

MediaWiki:Sidebar

2022-04-06T15:04:44Z

Adminplanets:

MediaWiki:Sidebar

2022-04-06T15:03:22Z

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MediaWiki:Sidebar

2022-04-06T14:54:38Z

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MediaWiki:Sidebar

2022-04-06T14:52:41Z

Adminplanets: