The time required for one full round trip is the same everywhere: $2\pi r/v$. What you need to know is the distance traveled: it is obviously $2\pi r$ at the equator and $0$ at the pole.
At a general latitude $\phi$, trigonometry will tell you that the distance is $2\pi r \cos(\phi)$, so the speed is $$\frac{2\pi r \cos(\phi)}{2\pi r/v}=\cos(\phi) v$$