Consider the following closed curve in the x y plane (curve x y coordinates are in meters).
r ( θ ) x ( θ ) y ( θ ) z 0 ≤ = = = = θ 1 + 2 1 sin ( 4 θ ) r ( θ ) cos θ r ( θ ) sin θ 0 ≤ 2 π
There is a magnetic flux density B throughout all of space. The field is perpendicular to the x y plane.
B = ( B x , B y , B z ) = ( 0 , 0 , 3 x 2 ) 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
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In hindsight, this problem could have been solved without invoking the concept of the vector potential. I have added a much shorter solution at the end of my already posted solution.
Greetings! I could use a helpful hint to compute the curve of intersection in your latest problem. I am struggling to solve it.
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First, the magnetic vector potential is computed using the relation:
∇ × A = B ∂ y ∂ A z − ∂ z ∂ A y = 0 ∂ z ∂ A x − ∂ x ∂ A z = 0 ∂ x ∂ A y − ∂ y ∂ A x = 3 x 2
From the above relations, with a little bit of trial and error, it is seen that the following vector satisfies the above relations.
A = 0 i ^ + x 3 j ^ + 0 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 ^ d θ d R = d θ d ( r ( θ ) cos θ ) i ^ + d θ d ( r ( θ ) sin θ ) j ^
Plugging in the given parameterization:
⟹ Φ = ∮ C A ⋅ d R = ∫ 0 2 π ( x 3 ( θ ) d θ d ( r ( θ ) sin θ ) ) d θ
Simplifying the integrand leads to:
Φ = ∮ C A ⋅ d R = ∫ 0 2 π ( 1 + 0 . 5 sin 4 θ ) 3 cos 3 θ ( 2 sin θ cos 4 θ + cos θ ( 1 + 0 . 5 sin 4 θ ) ) d θ
Φ = 5 1 2 6 8 1 π ≈ 4 . 1 7 8 5 6 3 6 6 6 2 0 0 4 8 7
Shorter method:
B = 3 r 2 cos 2 θ k ^ d S = r d r d θ k ^
Φ = ∫ ∫ S B ⋅ d S = ∫ 0 2 π ∫ 0 1 + 0 . 5 sin 4 θ ( 3 r 2 cos 2 θ ) r d r d θ ≈ 4 . 1 7 8 5 6 3 6 6 6 2 0 0 4 8 7