WRF dynamical core for LES/mesoscale simulations

WRF is a mesoscale numerical weather prediction system designed for both atmospheric research and operational forecasting applications over the Earth's atmosphere: see WRF presentation.

In the PCM, we take advantage of the dynamical core of the WRF model to run LES (large-eddy simulations) or mesoscale simulations.

To do so, we take the WRF model, remove all its physical packages related to the Earth's atmosphere, and plug in the physical package from the PCM (either Venus, Mars, Titan, or Generic).

A description of the various equations solved by WRF can be found here: Skamarock et al. (2019, 2021).

Descriptions of the application of WRF dynamical core with the PCM can be found in:

- Noé CLEMENT's PhD thesis (chapter 3) for the Generic PCM.

- Maxence Lefevre's PhD thesis for the Venus PCM.

Studies with the PCM coupled to the WRF dynamical core have been done using WRF V2, WRF V3, WRF V4.

Our aim is now to use WRF V4 as much as possible, which offers significant improvements in terms of numerical schemes in particular.

Here is a list of studies using the PCM coupled to the WRF dynamical core:

Planet	Reference	Physical package	Dynamical core
Mars	Spiga and Forget (2009)	Mars PCM	WRF V2
Mars	Spiga et al. (2010)	Mars PCM	WRF V3
Venus	Lefèvre et al. (2017)	Venus PCM	WRF V3
Exoplanets	Lefèvre et al. (2021)	Generic PCM	WRF V3
Exoplanets	Leconte et al. (2024)	Generic PCM	WRF V4
Uranus, Neptune	Clément et al. (2024)	Generic PCM	WRF V4

For advanced users:

When compiling the model, the flags:

#ifndef MESOSCALE
      use ...
#else
      use ...

select lines compiled depending on the configuration.

Below is a synthesis of equations solved by WRF.