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It might be worthwhile as an exercise to go back to post 74 from @alan123hk ,  where ## E_{induced}=-\frac{\partial{A}}{\partial{t}} ##,  and compute ## E_{induced}  ## from the ## A ##.  I normally like to simply compute ## E_{induced}  ## from the EMF using the symmetry with the path distance being ## 2 \pi r ##.
The vector potential ##A ## is known for a uniform ## B ## to be ## A=(B \times \vec{r})/2 ##.
I think it is also possible to compute ## A ## from the currents of a long solenoid that make up the uniform field, with ## A(x)=\frac{\mu_o}{4 \pi} \int \frac{J(x')}{|x-x'|} \, d^3 x' ##, but perhaps not a simple integral. @vanhees71 Might you have worked through this more difficult computation?
The answer we are looking for for ##E_{induced} ## from using the EMF is ##E_{induced}= \dot{B}(\pi r^2)/(2 \pi r)=\dot{B} r/2 ##, (pointing clockwise),
(Note for ## r>a ##, we should get ## E_{induced}=\dot{B} a^2/(2r) ##, but we don't have an expression for ## A ## for ## r>a ##).
and that's exactly what we get using ## E_{induced}=-\frac{\partial{A}}{\partial{t}} ## with ## A=(B \times \vec{r})/2 ##.
It's nice to see that everything is consistent.
(Note: I omit most vector symbols for brevity=it's difficult to write vectors all the time in Latex).
				
			The vector potential ##A ## is known for a uniform ## B ## to be ## A=(B \times \vec{r})/2 ##.
I think it is also possible to compute ## A ## from the currents of a long solenoid that make up the uniform field, with ## A(x)=\frac{\mu_o}{4 \pi} \int \frac{J(x')}{|x-x'|} \, d^3 x' ##, but perhaps not a simple integral. @vanhees71 Might you have worked through this more difficult computation?
The answer we are looking for for ##E_{induced} ## from using the EMF is ##E_{induced}= \dot{B}(\pi r^2)/(2 \pi r)=\dot{B} r/2 ##, (pointing clockwise),
(Note for ## r>a ##, we should get ## E_{induced}=\dot{B} a^2/(2r) ##, but we don't have an expression for ## A ## for ## r>a ##).
and that's exactly what we get using ## E_{induced}=-\frac{\partial{A}}{\partial{t}} ## with ## A=(B \times \vec{r})/2 ##.
It's nice to see that everything is consistent.
(Note: I omit most vector symbols for brevity=it's difficult to write vectors all the time in Latex).
			
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