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Let \(F (x,y, z) \) be a space vector field, \(p \) a point in the domain of \(F\), and \(\rm {v}\) a unit vector based at \(p\).
Let \(C\subset \mathbb {R}^2 \) be a very small circle centered at \(p\), around \(\rm {v}\), which travels counterclockwise when
seen from the tip of \(\rm {v}\). Then the integral
\[ \int _C F \cdot d \gamma \]
measures how much rotation is generated by \(F\)
around the axis \(\rm {v}\). It turns out we have another quantity that measures precisely that:
\[ \text {Curl}(F)(p) \cdot \rm {v} . \]
Overall, if we have an oriented surface \( \Sigma \subset \mathbb {R}^3\) with boundary \(\partial \Sigma \) oriented counterclockwise, the
two integrals
\begin{gather*} \int _{\partial \Sigma } F \cdot d \gamma \\ \iint _{\Sigma } ( \text {Curl}(F) \cdot N )\, dS \end{gather*}
measure how much rotation the vector field \(F\) generates over \(\Sigma \)
(with axis perpendicular to the surface). Stokes Theorem states that they
agree.
Stokes Theorem Let \(F(x,y, z)\) be a space vector field, and \( \Sigma \subset \mathbb {R}^3\) an oriented surface with
boundary \(\partial \Sigma \), oriented counterclockwise, when seen from the tip of \(N\). Then
\[ \int _{\partial \Sigma } F \cdot d \gamma = \iint _{\Sigma } \text {Curl}(F) \cdot dS \]
Let \(C \subset \mathbb {R}^3\) be the circle \(x^2 + y^2 = 25\) in the \(xy\)-plane, oriented counterclockwise, when seen from above.
Compute
\[ \text {Curl} (F) = \langle - x , -2 + y , 3 \rangle \]
If we define \(\Sigma \) to be disk \(x^2 + y^2 \leq 25 \) in the \(xy\)-plane, oriented
upward, we have \(\partial \Sigma = C\), and by Stokes Theorem,
Let \(C\subset \mathbb {R}^3\) be the curve that travels along straight lines first from \((1,0,0)\) to \((0,0,1)\), then from \((0,0,1)\) to \((0,1,0)\),
and then from \((0,1,0)\) to \((1,0,0)\). Compute
\[ \int _C \langle 3x + y, e^y - 2x , 5 z - 4x - 1 \rangle \cdot d \gamma \]
Set \(F = \langle 3x + y, e^y - 2x , 5 z - 4x - 1 \rangle \) and compute
where the minus
sign appears because when we look at \(C\) from the tip of \(N = \langle 1,1,1\rangle \), it goes clockwise.
Note that \(\langle 0,4,-3 \rangle \cdot N = 4-3 = 1\), so
The triangle is equilateral with side \(\sqrt {2}\), so its area is \(\frac {1}{2}\), and
\[ \int _C \langle 3x + y, e^y - 2x , 5 z - 4x - 1 \rangle \cdot d \gamma = - \frac {1}{2} \]
Let \(C\subset \mathbb {R}^3\) be the curve that goes from \((1,0)\) to \((-1,0)\) along the arc \(x^2 + y^2 = 1\), \(y \geq 0\), in the \(xy\)-plane, followed by the
curve that goes back to \((1,0)\) along the arc \(x^2 + z^2 = 1\), \(z\geq 0\), in the \(xz\)-plane. Compute
If we define \(\Sigma \) to be the portion of the sphere \(x^2 + y^2 + z^2 = 1\) with \(y \geq 0\), \(z \geq 0\), oriented
upward, we get \(\partial \Sigma = C\). Then by Stokes Theorem,
Parametrizing \(\Sigma \), we use \(\varphi : [0, \pi ] \times [0, \pi / 2] \to \Sigma \) with
\[ \varphi (u,v) = ( \cos u \sin v , \sin u \sin v , \cos v ) , \]
then
\begin{align*} \frac {\partial \varphi }{\partial u } & = \langle -\sin u \sin v , \cos u \sin v , 0 \rangle \\ \frac {\partial \varphi }{\partial v } & = \langle \cos u \cos v , \sin u \cos v , - \sin v \rangle \\ \frac {\partial \varphi }{\partial u } \times \frac {\partial \varphi }{\partial v } & = \langle - \cos u \sin ^2 v , - \sin u \sin ^2 v , - \sin v \cos v \rangle \end{align*}
Note that \( \frac {\partial \varphi }{\partial u } \times \frac {\partial \varphi }{\partial v } \) points inwards, so \(\varphi \) is NOT compatible with the orientation. The integrand
becomes
\begin{align*} \langle 2 , 2 \cos v ,0 \rangle & \cdot \langle - \cos u \sin ^2 v , - \sin u \sin ^2 v , - \sin v \cos v \rangle \\ & = -2 \cos u \sin ^2 v - 2 \sin u \cos v \sin ^2 v \end{align*}
Then (recalling that \(\varphi \) was not compatible with the orientation), we conclude
\begin{align*} \iint _{\Sigma } \langle 2 , 2z , 0 \rangle \cdot dS & = - \int _{0 }^{\pi } \int _0 ^{\pi /2} [-2 \cos u \sin ^2 v - 2 \sin u \cos v \sin ^2 v ] \, d v du \\ & = 0 + 4 \int _0 ^{ \pi / 2 } \cos v \sin ^2 v \, dv \\ & = 4 \left [ \frac {\sin ^3 v}{3 } \right ] _{v = 0} ^{ \pi /2} \\ & = \frac {4}{3} \end{align*}