On the magnetic dipole radiation in Griffith's book

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Magnetic dipole radiation in Griffith's "Introduction to Electrodynamics" indicates that there is no magnetic field along the axis of a wire loop when theta equals zero. However, the magnetic flux density can still be at its maximum due to the time-varying nature of alternating current. In a time-independent current loop, the magnetic field is strongest at theta equals zero, but it decreases rapidly with distance as 1/r^3. Griffith's analysis in section 11.1.3 focuses on a radiating current loop, where radiation terms for the magnetic and electric fields decrease more slowly, at 1/r. To deepen understanding, working through problem 11.5 is recommended to explore the fields without relying on approximation 3.
a1titude
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Homework Statement
It's not a homework. I just saw the resultant equation to find that it's strange.
Relevant Equations
$$\mathbf{B} = \mathbf{\nabla} \times \mathbf{A} = - \frac {\mu_0 m_0 \omega^2} {4 \pi c^2} \left( \frac {\sin \theta} {r} \right) \cos [\omega (t - r/c)] \hat{\mathbf{\theta}}$$
In 11.1.3 of Griffith's "Introduction to Electrodynamics 4Ed" appears magnetic dipole radiation, which results in the equation above. According to the resultant equation, there is no magnetic field in the axis of the wire loop because theta=0. However, I think the magnetic flux density is at maximum value there although its time-varying due to the alternating current. What am I missing now? Thanks for your concerns in advance.
 

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a1titude said:
In 11.1.3 of Griffith's "Introduction to Electrodynamics 4Ed" appears magnetic dipole radiation, which results in the equation above. According to the resultant equation, there is no magnetic field in the axis of the wire loop because theta=0. However, I think the magnetic flux density is at maximum value there although its time-varying due to the alternating current. What am I missing now? Thanks for your concerns in advance.
For a time-independent current loop, the B-field is strongest for ##\theta = 0## (for a given ##r##), as you are thinking. But recall that the field falls off rapidly with distance as ##1/r^3##.

In Griffiths' calculation in section 11.1.3, he is considering a radiating, harmonically oscillating current loop. In this case, you get "radiation terms" in the results for B and E that decrease much more slowly with distance as ##1/r##. So for "large ##r##", only the radiation terms are significant. Note, in particular, Griffiths' "approximation 3" given as relation (11.34) on page 475; namely, assume ##r \gg c/\omega##.

It would probably be helpful for you to work problem 11.5 on page 477 (at least the first part where you are asked to find the fields without making approximation 3.)
 
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