- I-Learn, Class Pictures, Learning Targets, Text Book Practice
- Prep Tasks: Unit 1 - Motion, Unit 2 - Derivatives, Unit 3 - Integration, Unit 4 - Vector Calculus
We still have some tasks from Day 39 to finish discussing in class.
Day 39 - Prep
There are no new tasks for this day. Work on the tasks from previous days that we have not yet discussed in class.
Day 40 - Prep
Learning Target Checkoff
A learning target quiz will appear in I-Learn. Complete and submit the quiz before the due date.
Day 40 - In class
There is no class. Complete the quiz in I-Learn.
Day 41 - Prep
Task 41.1
We've already learned how to draw parametric space curves, such as $\vec r(t)=(2\cos t, 2\sin t, t)$ for $0\leq t\leq 4\pi$. We pick several values of $t$, plot the corresponding points in space, and then connect the dots. We can draw this function in Mathematica using the following code.
ParametricPlot3D[{2 Cos[t], 2 Sin[t], t}, {t, 0, 4 Pi}]
The example above draws a wire, or path, in space. It's an example of a parametrization that uses only one parameter. Because only one parameter is used, the graph represents an object for which it makes sense to compute lengths. It's like we've wrapped a straight line up in space, using the parametrization. What happens if we increase the number of parameters. That's what this task explores.
- Suppose a jet begins spiraling upwards to gain height. The position of the jet after $t$ seconds is modeled by the equation $\vec r(t)=(2\cos t, 2\sin t, t).$ The jet is accompanied by several jets flying side by side. As all the jets fly, they leave a smoke trail behind them (it's an air show). The smoke from each jet spreads outwards to mix together, so that it looks like the jets are leaving a wide sheet of smoke behind them as they spiral upwards. The position of two of the many other jets is given by $\vec r_3(t)=(3\cos t, 3\sin t, t)$ and $\vec r_4(t)=(4\cos t,4\sin t,t)$. A function which represents the smoke stream from these jets is $\vec r(a,t)=(a\cos t, a\sin t, t)$ for $0\leq t\leq 4\pi$ and $2\leq a\leq 4$.
- Graph the position of the three jets $\vec r(2,t)=(2\cos t, 2\sin t, t)$, $\vec r(3,t)=(3\cos t, 3\sin t, t)$, and $\vec r(4,t)=(4\cos t,4\sin t,t)$ in the same 3D plot.
- Let $t=0$ and graph the curve $r(a,0)=(a,0,0)$ for $a\in[2,4]$ (so $2\leq a\leq 4$), which represents a segment along which the smoke has spread. Then repeat this for $t=\pi/2$, then $t=\pi$, and then $t=3\pi/2$.
- Describe the resulting surface. Then use Mathematica to view the surface (all it requires is adding another parameter to the code).
ParametricPlot3D[{a Cos[t], a Sin[t], t}, {t, 0, 4 Pi}, {a, 2, 4}]
We call the surface you drew above a parametric surface. The vector equation describing the smoke screen is a parametrization of this surface.
A parametrization of a surface is a collection of three equations to tell us the position $$x=x(u,v), y=y(u,v), z=z(u,v)$$ of a point $(x,y,z)$ on the surface. We call $u$ and $v$ parameters, and these parameters give us a two dimensional pair $(u,v)$, the input, needed to obtain a specific location $(x,y,z)$, the output, on the surface. We can also write a parametrization in vector form as $$\vec r(u,v) = (x(u,v), y(u,v), z(u,v)).$$ We'll often give bounds on the parameters $u$ and $v$, which help us describe specific portions of the surface. A parametric surface is a surface together with a parametrization.
We draw parametric surfaces by joining together many parametric space curves. Pick one variable, hold it constant, and draw the resulting space curve. Repeat this several times, and you'll have a 3D surface plot. Most of 3D computer animation is done using parametric surfaces. Car companies create computer models of vehicles using parametric surfaces, and then use those parametric surfaces to study collisions. Often the mathematics behind these models is hidden in the software program, but parametric surfaces are at the heart of just about every 3D model.
- Consider the parametric surface $\vec r(u,v)=(u\cos v, u\sin v, u^2)$ for $0\leq u\leq 3$ and $0\leq v\leq 2 \pi$. Construct a graph of this function.
- Remember, to do so we just let $u$ equal a constant (such as 1, 2, 3) and then graph the resulting space curve where we let $v$ vary. After doing this for several values of $u$, swap and let $v$ equal a constant (such as 0, $\pi/2$, etc.) and graph the resulting space curve as $u$ varies.
- Did you get a satellite dish? Modify the Mathematica code above to have software construct the surface.
Task 41.2
When a vector has no potential, there is a generalization of the fundamental theorem of calculus that can simplify work computations. To discuss this version (called Green's theorem), we first need a few definitions.
When a curve $C$ is a closed curve (starts and ends at the same point), we call the work done by vector field $\vec F$ along $C$ the circulation of $\vec F$ along $C$.
A simple closed curve is a closed curve that does not cross itself.
Let $\vec F(x,y)=\left<M,N\right>$ be a continuously differentiable vector field. At the point $(x,y)$ in the plane, create a circle $C_a$ of radius $a$ centered at $(x,y)$, oriented counterclockwise. The area inside of $C_a$ is $A_a=\pi a^2$. The quotient $\ds \frac{1}{A_a}\oint_{C_a} \vec F \cdot d\vec r$ is a circulation per area. The counterclockwise circulation density of $\vec F$ at $(x,y)$ we define to be $$\lim_{a\to 0} \frac{1}{A_a}\oint_{C_a} \vec F \cdot d\vec r = \lim_{a\to 0} \frac{1}{A_a}\oint_{C_a} Mdx+Ndy =\frac{\partial N}{\partial x}-\frac{\partial M}{\partial y}=N_x-M_y.$$
In the definition above, we could have replaced the circle $C_a$ with a square of side lengths $a$ centered at $(x,y)$ with interior area $A_a$. Alternately, we could have chosen any collection of curves $C_a$ which "shrink nicely" to $(x,y)$ and have area $A_a$ inside. Regardless of which curves you chose, it can be shown that $$N_x-M_y=\lim_{a\to 0} \frac{1}{A_a}\oint_{C_a} Mdx+Ndy.$$
To understand what the circulation density mean in a physical sense, think of $\vec F$ as the velocity field of some fluid (a liquid or gas). The circulation density tells us the rate at which the vector field $\vec F$ causes objects to rotate around points. If circulation density is positive, then particles near $(x,y)$ would tend to circulate around the point in a counterclockwise direction. The larger the circulation density, the faster the rotation. The velocity field of a fluid could have some regions where the fluid is swirling clockwise, and some regions where the fluid is swirling counterclockwise.
We are now ready to state Green's Theorem. Ask me in class to give an informal proof as to why this theorem is valid.
Let $\vec F(x,y)=(M,N)$ be a continuously differentiable vector field, which is defined on an open region in the plane that contains a simple closed curve $C$ and the region $R$ inside the curve $C$. Then we can compute the counterclockwise circulation of $\vec F$ along $C$ using $$ \oint_{C} M dx+Ndy=\iint_R N_x-M_y dA %\quad \text{ and } \quad %\oint_{C} \vec F \cdot \vec n ds=\iint_R M_x+N_y dA. $$
Let's use this theorem to find circulation (work on a closed curve).
- Consider the vector field $\vec F=(2x+3y,4x+5y)$.
- Start by computing $N_x-M_y$.
- If $C$ is the boundary of the rectangle $2\leq x\leq 7$ and $0\leq y\leq 3$, find the circulation of $\vec F$ along $C$. [Doing this without Green's theorem requires we parametrize 4 line segments, compute 4 integrals, and then sum the results. Green's theorem can make this really fast. ]
- Let $R$ be the region inside a circle of radius 3 that is centered at the origin. Compute the work done by $\vec F$ to move an object once, counterclockwise, around this circle. (In other words, compute the circulation of $\vec F$ along $C$ - use Green's theorem to make this fast.)
- Consider the vector field $\vec F=(x^2+y^2,3x+5y)$.
- Start by computing $N_x-M_y$.
- If $C$ is the circle $x^2+y^2=4$ (oriented counterclockwise), then find the circulation of $\vec F$ along $C$.
- Let $R$ be the rectangular region with bounds $0\leq x\leq 4$ and $0\leq y\leq 6$. Compute the counterclockwise circulation of $\vec F$ along the boundary of $R$.
Task 41.3
Given a parametric surface, such as $\vec r(u,v) = (u\cos v, u\sin v, v)$ for $2\leq u\leq 4$ and $0\leq v\leq 2\pi$, we can compute the partial derivatives $\vec r_u = \frac{\partial \vec r}{\partial u}$ and $\vec r_v = \frac{\partial \vec r}{\partial v}$, both of which are 3D vectors. Their cross product $\vec n = \vec r_u\times \vec r_v = \dfrac{\partial \vec r}{\partial u}\times \dfrac{\partial \vec r}{\partial v}$ is a vector that is orthogonal to both partial derivatives. The Mathematica code below creates a Module which plots the surface, along with $\vec r_u$, $\vec r_v$, and $\vec n$, using the colors red, blue, and green, respectively.
Module[{r, u, v, ru, rv, n, uBounds, vBounds},
r[u_, v_] := {u Cos[v], u Sin[v], v};
uBounds = {u, 2, 4};
vBounds = {v, 0, 2 Pi};
ru[u_, v_] := Derivative[1, 0][r][u, v];
rv[u_, v_] := Derivative[0, 1][r][u, v];
n[u_, v_] := Cross[ru[u, v], rv[u, v]];
Manipulate[Show[
ParametricPlot3D[r[u, v], uBounds, vBounds, PlotStyle -> Opacity[0.5]],
Graphics3D[{Thick,
Red, Arrow[{r[u1, v1], r[u1, v1] + ru[u1, v1]}],
Blue, Arrow[{r[u1, v1], r[u1, v1] + rv[u1, v1]}],
Green, Arrow[{r[u1, v1], r[u1, v1] + n[u1, v1]}]}],
PlotRange -> All],
{{u1, (uBounds[[2]] + uBounds[[3]])/2}, uBounds[[2]], uBounds[[3]]},
{{v1, (vBounds[[2]] + vBounds[[3]])/2}, vBounds[[2]], vBounds[[3]]}]]
When you run the code above, you'll see two sliders (created using the Manipulate[] command) which allow you to pick the parameter values $(u_1,v_1)$ at which all three vectors are shown.
- How do you interpret the vectors $\vec r_u$, $\vec r_v$, and $\vec n$? How do they physically relate to the surface?
- Run the code above on your own computer. After playing with the sliders a bit, write down an interpretation.
- Let's swap to a different surface. In the code above, change the parametric surface and bounds (lines 2-4) to the following. Run the code and you should see a donut (torus). Play with the sliders again. Does your interpretation of the vectors $\vec r_u$, $\vec r_v$, and $\vec n$ change any, or does this help confirm your interpretation?
r[u_, v_] := {(2 - Cos[u]) Cos[v], (2 - Cos[u]) Sin[v], Sin[u]}; uBounds = {u, 0, 2 Pi}; vBounds = {v, 0, 2 Pi}; - Here are more surfaces to explore. Rerun the code with some of these surfaces, and update your interpretation as needed. If you present in class, then you'll only need to share one of the surfaces you chose to work with (from above, or below).
r[u_, v_] := {u, v, 4 - u^2 - v^2};
uBounds = {u, -2, 2};
vBounds = {v, -2, 2};
r[u_, v_] := {u Cos[v], u Sin[v], 4 - u^2};
uBounds = {u, 0, 2};
vBounds = {v, 0, 2 Pi};
r[u_, v_] := {u Cos[v], u, u Sin[v]};
uBounds = {u, 0, 2};
vBounds = {v, 0, 2 Pi};
r[u_, v_] := {2 Sin[u] Cos[v], 3 Sin[u] Sin[v], 5 Cos[u]};
uBounds = {u, 0, Pi};
vBounds = {v, 0, 2 Pi};
r[u_, v_] := {2 Cos[v], u, 2 Sin[v]};
uBounds = {u, -2, 5};
vBounds = {v, 0, 2 Pi};
The two partial derivatives appear in the differential $d\vec r = \vec r_u du+\vec r_v dv$. The vectors $\vec r_u$ and $\vec r_v$ form the edges of a parallelogram, as do the vectors $\vec r_u du$ and $\vec r_v dv$. The Mathematica code below shows the surface (a torus) and partial derivatives at a chosen point $(u_1,v_1)$. The parallelogram whose edges are $\vec r_u$ and $\vec r_v$ is shaded green, and the parallelogram whose edges are $\vec r_u du$ and $\vec r_v dv$ is shaded black. You can easily change the surface to any of the other surfaces above, by adjusting lines 2-4 of the code.
Module[{r, u, v, ru, rv, n, uBounds, vBounds},
r[u_, v_] := {(2 - Cos[u]) Cos[v], (2 - Cos[u]) Sin[v], Sin[u]};
uBounds = {u, 0, 2 Pi};
vBounds = {v, 0, 2 Pi};
ru[u_, v_] := Derivative[1, 0][r][u, v];
rv[u_, v_] := Derivative[0, 1][r][u, v];
n[u_, v_] := Cross[ru[u, v], rv[u, v]];
Manipulate[Show[
ParametricPlot3D[r[u, v], uBounds, vBounds, PlotStyle -> Opacity[0.5]],
Graphics3D[{Thick,
Red, Arrow[{r[u1, v1], r[u1, v1] + ru[u1, v1]}],
Blue, Arrow[{r[u1, v1], r[u1, v1] + rv[u1, v1]}],
Opacity[0.5], Green, Polygon[{r[u1, v1], r[u1, v1] + ru[u1, v1], r[u1, v1] + ru[u1, v1] + rv[u1, v1], r[u1, v1] + rv[u1, v1]}],
Opacity[1], Black, Polygon[{r[u1, v1], r[u1, v1] + ru[u1, v1] du, r[u1, v1] + ru[u1, v1] du + rv[u1, v1] dv, r[u1, v1] + rv[u1, v1] dv}]}],
PlotRange -> All, ImageSize -> Large],
{{u1, (uBounds[[2]] + uBounds[[3]])/2}, uBounds[[2]], uBounds[[3]]},
{{v1, (vBounds[[2]] + vBounds[[3]])/2}, vBounds[[2]], vBounds[[3]]},
{{du, 0.5}, 0, 1},
{{dv, 0.5}, 0, 1}
]]
When you run the code above, you will find 4 sliders. The first two allow you to pick a point on the surface by choosing values for the parameters $u$ and $v$. The other two allow you to pick values for $du$ and $dv$.
- For a parametric surface $\vec r(u,v)$ with $a\leq u\leq b$ and $c\leq v\leq d$, explain why the surface area is given by $$S=\iint_S dS = \int_{a}^{b}\int_{c}^{d}|\vec r_u\times \vec r_v|dvdu.$$ The items below may help you do this.
- How do you find the area of the green parallelogram?
- How do you find the area of the black parallelogram?
- Explain why $|\vec r_u du \times \vec r_v dv|=|\vec r_u \times \vec r_v |dudv$ (did you notice this was the area of the black parallelogram?).
- Explain why a little bit of surface area is given by $dS = |\vec r_u \times \vec r_v |dudv$.
- To get total surface area, what should we do with the little surface areas $dS$?
- For the surface $\vec r(u,v) = (u\cos v, u\sin v, v)$ for $2\leq u\leq 4$ and $0\leq v\leq 2\pi$, compute the surface area using the formula above.
Task 41.4
Pick some problems related to the topics we are discussing from the Text Book Practice page.
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