home.md

@@ -15,45 +15,10 @@ In 2017 we have started a code re-factorization with the main purpose of reorgan
 ## [Supported Boundaries Conditions](supported-boundary-condition)
 ## [Meetings](Meetings)
 
-## [Code Content](CodeContent)
+## [Code Content](Code-Content)
+## [Plots and Post Process](Plots and Post Process)
  
 
-## Plots and Post Process
- 
-In order to '''compile the program for the plot''' of the gas quantities:
-```
-./PostProces/make
-```
-
-
-In order to '''make the plot of gas density and velocities ''':
-```
-./fargo3Dplot -h
-./streamlines -h for streamlines
-./average-cylindric for the analysis of flow in a cylindric frame centred on the planet
-etc ... (see README in fargo3D/PostProces)
-```
-
-for the help on using fargo3Dplot. fargo3Dplot prepares different files for plot, it must be followed ./gnuexe in order to plot them with gnuplot 
-
-The output file containing the orbital parameters at each DT is orbit''i''.dat where ''i'' is the planet number.
-The columns contain respectively:
-``` 
-the date
-the eccentricity
-the semi-major axis
-the inclination
-the planet mean anomaly
-the argument of pericenter
-the longitude of the node
-```
-
-![Cress](/uploads/1ce4238ed6d32b6464053c4bfb50fad0/Cress.jpeg)
-
-
-Revision e [71]  in [source:/fargo3D/src@71 ] corresponds to the full 3D isothermal model with gas + planets. 
-The figure shows  the evolution of semi-major axis eccentricity and inclination for a 20 Earth mass planets.
-The parameter are those in Cresswell et al. 2007, and the results are in good agreement (see Fig.16 of Cresswell et al. paper). 
 
 <!---
 In revision [82]   in [source:/fargo3DAD/src@82 ]  the adiabatic part is completed.