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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](Examples/3D Radiative Disk)
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In [examples/3D_radiative_disk_restart](/../tree/master/examples/3D_radiative_disk).
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In [examples/3D_radiative_disk](/../tree/master/examples/3D_radiative_disk).
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## [3D Radiative Disk Restart](Examples/3D Radiative Disk Restart)
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In [examples/3D_radiative_disk_restart](/../tree/master/examples/3D_radiative_disk_restart).
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## 3D_stellar_radiation_disk
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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 Stellar Radiation Disk](Examples/3D Stellar Radiation Disk)
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In [example/#D_stellar_radiation_disk](/../tree/master/examples/3D_stellar_radiation_disk).
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## [3D Accreting By Wind](Examples/3D Accreting By Wind)
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In [examples/2D_isothermal_disk](/../tree/master/examples/3D_accreting_bywind). |
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