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## Presentation
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The **FARGOCA** code is a 3D version of FARGO, developed in 2011 in its isothermal version,
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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.
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**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.
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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.
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The main features of FARGOCA are:
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The main features of **FARGOCA** are:
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1) Spherical geometry
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2) 2 and 3 dimensional calculations
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3) FARGO algorithm for orbital advection calculations
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4) Full Energy equation taking into account viscous heating, star radiation, radiation from planets accreting solids and radiative cooling with multiple opacity prescriptions
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The code has been re-factorized from its original version (Lega et al. 2014) by A. Miniussi (main developper) and E. Lega
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The code has been re-factorized from its original version (Lega et al. 2014) by A. Miniussi (main developper) and E. Lega.
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A set of integration test provides code validation as well as suitably selected examples that provide a starting point for code usage.
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