back to running the whole simulation

Author: pancetta

pySDC/projects/Hamiltonian/README.rst

@@ -21,6 +21,5 @@ For this, only six planets are modeled, namely the Sun (which in its mass contai
 The acceleration due to gravitational forces are computed using a simple N^2 solver.
 All this is implemented within the ``OuterSolarSystem`` problem class.
 Coarsening can be done using only the sun for computing the acceleration.
-Note that the tests/autogenerated results only run the visualization to save time.
 
 .. include:: doc_solar_system.rst

pySDC/projects/Hamiltonian/data/outer_solar_system.dat

@@ -80,7 +80,7 @@ def run_simulation(prob=None):
         description, controller_params = setup_outer_solar_system()
         # set time parameters
         t0 = 0.0
-        Tend = 100000.0
+        Tend = 20000.0
         num_procs = 100
     else:
         raise NotImplemented('Problem type not implemented, got %s' % prob)

pySDC/projects/Hamiltonian/solar_system.py

@@ -1,5 +1,4 @@
-from pySDC.projects.Hamiltonian.solar_system import show_results
+from pySDC.projects.Hamiltonian.solar_system import main
 
 def test_main():
-    prob = 'outer_solar_system'
-    show_results(prob, cwd='pySDC/projects/Hamiltonian/')
+    main()