Actually, if you ask about radial dependace of time-avaraged Poynting flux vector, then it depends on where the observer is (far field or near field). If you assume that the observer is far away (more than $\frac{2D^2}{\lambda}$, where $D$ - is the maximum size of your source and $\lambda$ - is the walength (I see you use monocromatic case)) than the intensity should degrade as $\frac{1}{r^2}$ (in case there is no absorbtion in medium, if yes, then it should be a little faster, for example $\frac{1}{r^{2+\alpha}}, \alpha>0$). In the near field region electric and magnetic field components have several terms: $\frac{1}{r},\frac{1}{r^2},\frac{1}{r^3}$, so the Poynting vector should have several components too and they all degrade as $\frac{1}{r^5}$ (and that's even without absorbtion).