... | ... | @@ -12,7 +12,17 @@ |
|
|
The **FARGOCA** code is a 3D version of FARGO, developed in 2011 in its isothermal version,
|
|
|
has evolved since then with the addition of the treatment of energy equation with energy provided by the viscous and compressional heating and by the energy irradiated from the star.
|
|
|
|
|
|
In 2017 we have started a code re-factorization with the main purpose of reorganize and optimize it in view of future developments.
|
|
|
FARGOCA is a grid-based hydrodynamical code that run on CPU clusters (MPI+OpenMP parallelization) specifically designed for the study of protoplanetary disks and for planets-disk interactions.
|
|
|
|
|
|
The main features of FARGOCA are:
|
|
|
1) Spherical geometry
|
|
|
2) 2 and 3 dimensional calculations
|
|
|
3) FARGO algorithm for orbital advection calculations
|
|
|
4) Full Energy equation taking into account viscous heating, star radiation, radiation from planets accreting solids and radiative cooling with multiple opacity prescriptions
|
|
|
|
|
|
The code has been re-factorized from its original version (Lega et al. 2014) by A. Miniussi (main developper) and E. Lega
|
|
|
A set of integration test provides code validation as well as suitably selected examples that provide a starting point for code usage.
|
|
|
|
|
|
|
|
|
<!-- ![density](uploads/bc957fc3f6ce78a714aa5d97b34d701e/density.png) -->
|
|
|
<img src="uploads/bc957fc3f6ce78a714aa5d97b34d701e/density.png" width="220" height="220">
|
... | ... | |