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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_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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## 3D_radiative_disk
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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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* **Boundaries**: reflecting in both radial and vertical direction, recommended when disk is studied without planets like in this case
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## **3D_radiative_disk_restart**: TBD
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## 3D_radiative_disk_restart
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TBD
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## 3D_stellar_radiation_disk
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## **3D_stellar_radiation_disk**: similar to the previous example considering also the radiation emitted from the star. This example is provided in a restart mode, this configuration requires a physical time of about 50 orbits at r=1 to reach a flared disk in equilibrium
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similar to the previous example considering also the radiation emitted from the star. This example is provided in a restart mode, this configuration requires a physical time of about 50 orbits at r=1 to reach a flared disk in equilibrium
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* **Half**: true, simulations with StarRadiation require a large radial and vertical domain to obtain a flared disk, it is therefore recommended to simulate only half of the disk (the code has a reflecting condition at midplane in this case)
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* **FullEnergyEos**: true to have a disk description with thermal effects
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* **StarRadiation**: true to consider also the radiation from the star
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* **Epsilon**: 5.e-5 this value is larger than typically used values 5.e-7-1.e-6 but it is recommended for a first approach to equilibrium, then one can refine by reducing epsilon
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* **Output**: 1 output after 1/10 of orbit at r=1 (PhysicalTime=0.628)
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## **3D_accreting_bywind**: TBD
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## 3D_accreting_bywind
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TBD
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