The magnetic field in radiation that travels a long way is usually not due to magnetic dipoles such as the dipole moments of elementary particles. It is usually caused by the magnetic field from accelerating charges.
So let's talk about what the field at a point $\vec r$ at time $t$ is equal to due to a charge. You start at your point $\vec r$ and you go out to a sphere of radius $d$ and then ask yourself if there were any charges there at time $t-d/c$ (if there wasn't then do out to a different radius) and if there was that means you'd be able to see that charge at $\vec r$ at time $t$ so that's what you are looking for. If so let $\vec w$ be the position of that charge, let $q$ be the amount of charge, let $\vec a$ be the acceleration of the charge, and let $\vec v$ be the velocity of the charge and make sure all of them are evaluated at time $t-d/c$ then you have what you need.
Now we can compute the electric and magnetic fields due to that charge based on those three vectors. To compute the fields you can use $\vec d=\vec r -\vec w$ and $\vec u=c\hat d-\vec v$ and get (adapted from Griffiths' Introduction to electrodynamics):
$$\vec E(\vec r,t)=\frac{q}{4\pi\epsilon_0}\frac{d}{(\vec d\cdot \vec u)^3}\left[(c^2-v^2)\vec u+\vec d\times(\vec u\times \vec a)\right]$$
and $$\vec B(\vec r,t)=\frac{1}{c}\hat d\times
\vec E(\vec r,t).$$
Recall that the $t$ is not the time when the charge had the position $\vec w,$ velocity $\vec v,$ and acceleration $\vec a.$ Those are at an earlier time, the time back when the charge broadcasted its position $\vec w,$ velocity $\vec v,$ and acceleration $\vec a$ just in time to arrive at $\vec r$ at time $t.$
Now, we see that it is term with the acceleration $\vec a$ that falls off the least, so while it might start off small, when you are super far away, that's the term that dominates.