Now we need a functional form for ψ to solve the PDE. Look at vrpsi above and realize that we need it to have a cos dependence. Thus C[r] Sin[
] looks like a good choice.
![[Graphics:../Images/inviscid_sphere_gr_68.gif]](../Images/inviscid_sphere_gr_68.gif)
![[Graphics:../Images/inviscid_sphere_gr_69.gif]](../Images/inviscid_sphere_gr_69.gif)
Things are going well, the theta dependence divides out
![[Graphics:../Images/inviscid_sphere_gr_71.gif]](../Images/inviscid_sphere_gr_71.gif)
This can be solved readily with a solution of the form A[r] = rα because it is an Euler equation.
![[Graphics:../Images/inviscid_sphere_gr_73.gif]](../Images/inviscid_sphere_gr_73.gif)
Here is the far away boundary condition, we match the r velocity to the free stream , @ r-->∞
![[Graphics:../Images/inviscid_sphere_gr_75.gif]](../Images/inviscid_sphere_gr_75.gif)
The boundary condition on the sphere must be
[r=R] = 0
![[Graphics:../Images/inviscid_sphere_gr_78.gif]](../Images/inviscid_sphere_gr_78.gif)
Now solve for the constants
![[Graphics:../Images/inviscid_sphere_gr_80.gif]](../Images/inviscid_sphere_gr_80.gif)
Now replace the constants in the answer to get the expression for the streamlines.
![[Graphics:../Images/inviscid_sphere_gr_82.gif]](../Images/inviscid_sphere_gr_82.gif)