Consider the following closed curve in x y z space (coordinates are in meters).
r ( θ ) x ( θ ) y ( θ ) z ( θ ) 0 ≤ = = = = θ 1 + 2 1 sin ( 4 θ ) r ( θ ) cos θ r ( θ ) sin θ θ 2 − 2 π θ ≤ 2 π
There is a magnetic flux density B throughout all of space.
B = ( B x , B y , B z ) = ( 1 , 1 , 1 ) m 2 Wb
Determine the absolute value of the magnetic flux (in Wb ) through the interior surface bounded by the curve.
∬ S B ⋅ d S
Note: The image shows the projection of the curve and interior surface onto the x y plane
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@Karan Chatrath
Hello sir.
How we will post problems now . Community will not accept more problems after 1 month
I am very worried regarding this ,share your views ?
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First, the magnetic vector potential is computed using the relation:
∇ × A = B ∂ y ∂ A z − ∂ z ∂ A y = 1 ; ∂ z ∂ A x − ∂ x ∂ A z = 1 ; ∂ x ∂ A y − ∂ y ∂ A x = 1
With a little bit of trial and error, it is seen that the following vector satisfies the above relations.
A = z ( θ ) i ^ + x ( θ ) j ^ + y ( θ ) k ^
Now, by applying Stokes' theorem
Φ = ∫ ∫ S B ⋅ d S = ∫ ∫ S ( ∇ × A ) ⋅ d S = ∮ C A ⋅ d R
R = r ( θ ) cos θ i ^ + r ( θ ) sin θ j ^ + z ( θ ) k ^ d θ d R = d θ d ( r ( θ ) cos θ ) i ^ + d θ d ( r ( θ ) sin θ ) j ^ + d θ d z ( θ ) k ^ d R = ( d θ d ( r ( θ ) cos θ ) i ^ + d θ d ( r ( θ ) sin θ ) j ^ + d θ d z ( θ ) k ^ ) d θ
With the parameterisation complete, the next step is to evaluate the integrand. Here, simplifications have been left out and may be attempted by anyone interested.
Φ = ∫ 0 2 π A ⋅ d R = ∫ 0 2 π f ( θ ) d θ ⟹ ∣ Φ ∣ ≈ 7 . 3 5 6 6
The integral can be solved by outsourcing to Wolfram-Alpha or by using a script of code.