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## [Supported Boundaries Conditions](supported-boundary-condition)
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## [Meetings](Meetings)
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## [Code Content](CodeContent)
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## Plots and Post Process
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## [Code Content](Code-Content)
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## [Plots and Post Process](Plots and Post Process)
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In order to '''compile the program for the plot''' of the gas quantities:
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```
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./PostProces/make
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```
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In order to '''make the plot of gas density and velocities ''':
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```
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./fargo3Dplot -h
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./streamlines -h for streamlines
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./average-cylindric for the analysis of flow in a cylindric frame centred on the planet
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etc ... (see README in fargo3D/PostProces)
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```
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for the help on using fargo3Dplot. fargo3Dplot prepares different files for plot, it must be followed ./gnuexe in order to plot them with gnuplot
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The output file containing the orbital parameters at each DT is orbit''i''.dat where ''i'' is the planet number.
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The columns contain respectively:
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```
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the date
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the eccentricity
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the semi-major axis
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the inclination
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the planet mean anomaly
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the argument of pericenter
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the longitude of the node
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```
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![Cress](/uploads/1ce4238ed6d32b6464053c4bfb50fad0/Cress.jpeg)
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Revision e [71] in [source:/fargo3D/src@71 ] corresponds to the full 3D isothermal model with gas + planets.
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The figure shows the evolution of semi-major axis eccentricity and inclination for a 20 Earth mass planets.
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The parameter are those in Cresswell et al. 2007, and the results are in good agreement (see Fig.16 of Cresswell et al. paper).
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<!---
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In revision [82] in [source:/fargo3DAD/src@82 ] the adiabatic part is completed.
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