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## [3D Unperturbed Disk](Examples/3D Unperturbed Disk)
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In [examples/3D_unperturbed_disk](/../tree/master/examples/3D_unperturbed_disk).
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## [3D Isothermal Disk](Examples/3D Isothermal Disk)
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In [examples/3D_isothermal_disk](/../tree/master/examples/3D_isothermal_disk).
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* **3D_isothermal_non_uniform_grid** : locally isothermal Equation of State
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* **Planet** : 20 Earth mass planet embedded in a 3D disk without masstaper, the grid is nonuniform, resolution is highest close to the planet, the configuration
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file provides the name of the files containing the grid
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* **Output** : 1 output file after 1/100 of orbit
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* **Transport**: normal, we can not use FARGO algorithm with non uniform grid geometry in azimuth
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* **Boundaries**: reflecting in both radial and vertical direction, commonly used for small mass planets (below 30 Earth masses)
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* **3D_radiative_disk**: evolution of a disk without planet (r-z disk thanks to azimuthal symmetry) with Full energy equation of state, useful to find thermal equilibrium before expanding the disk in 3D and inserting planet(s)
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* **FullEnergyEos**: true to have a disk description with thermal effects
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* **Output**: 1 output after 10 orbits at r=1 (PhysicalTime=100*0.628)
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