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Jim Lambers MAT 280 Spring Semester 2009-10 Lecture 21 Notes

These notes correspond to Section 13.6 in Stewart and Sections 7.3 and 7.4 in Marsden and Tromba.

Parametric Surfaces and Their

We have learned that Green’s Theorem can be used to relate a line of a two-dimensional vector field F over a closed plane C to a double integral of a component of curl F over the region D that is enclosed by C. Our goal is to generalize this result in such a way as to relate the line integral of a three-dimensional vector field F over a closed space curve C to the integral of a component of curl F over a enclosed by C. We have also learned that Green’s Theorem relates the integral of the component of a two-dimensional vector field over a closed curve C to the double integral of div F over the region D that it encloses. We wish to generalize this result in order to relate the integral of the normal component of a three-dimensional vector field F over a closed surface S to the triple integral of div F over the solid E contained within S. In order to realize either of these generalizations, we need to be able to integrate functions over piecewise smooth surfaces, just as we now know how to integrate functions over piecewise smooth . Whereas a smooth curve C, being a curved one-dimensional entity, is most conveniently described by a parameterization r(t), where a ≤ t ≤ b and r(t) is a differentiable function of one vari- able, a smooth surface S, being a curved two-dimensional entity, is most conveniently described by a parametriation r(u, v), where (u, v) lies within a 2-D region, and r(u, v) = ⟨x(u, v), y(y, v), z(u, v)⟩ is a differentiable function of two variables. We say that S is a parametric surface, and x = x(u, v), y = y(u, v), z = z(u, v) are the parametric equations of S. Example The M¨obiusstrip is a surface that is famous for being a nonorientable surface; that is, it “has only one side”. It can be parameterized by  v u  v u v u x(u, v) = 1 + cos cos u, y(u, v) = 1 + cos sin u, z(u, v) = sin , 2 2 2 2 2 2 where 0 ≤ u ≤ 2 and −1 ≤ v ≤ 1. It is shown in Figure 1. □ Example The paraboloid defined by the equation x = 4y2 + 4z2, 0 ≤ x ≤ 4, can also be defined by the parametric equations √ √ x x x = x, y = cos , z = sin , 2 2

1 Figure 1: The M¨obiusstrip where 0 ≤  ≤ 2, since for each x, a point (x, y, z) on the paraboloid must lie on a circle centered at (x, 0, 0) with radius px/4, parallel to the yz-plane. This is an example of a , since the surface is obtained by revolving the curve y = f(x) around the x-axis. □

Let P0 = (x0, y0, z0) = r(u0, v0) be a point on a parametric surface S. A curve defined by g(v) = r(u0, v) that lies within S and passes through P0 has the vector ∂x ∂y ∂z  r = g′(v) = (u , v ), (u , v ), (u , v ) v ∂v 0 0 ∂v 0 0 ∂v 0 0 at P0. Similarly, the tangent vector at P0 of the curve h(u) = r(u, v0), that also lies within S and passes through P0, is ∂x ∂y ∂z  r = h′(u) = (u , v ), (u , v ), (u , v ) . u ∂u 0 0 ∂u 0 0 ∂u 0 0

If these vectors are not parallel, then together they define the tangent plane of S at P0. Its normal vector is ru × rv = ⟨a, b, c⟩ which yields the equation a(x − x0) + b(y − y0) + c(z − z0) = 0

2 of the tangent plane. Example (Stewart, Section 13.6, Exercise 30) Consider the surface defined by the parametric equations x = u2, y = v2, z = uv, 0 ≤ u, v ≤ 10.

At the point (x0, y0, z0) = (1, 1, 1), which corresponds to u0 = 1, v0 = 1, the equation of the tangent plane can be obtained by first computing the partial derivatives of the coordinate functions. We have xu = 2u, yu = 0, zu = v,

xv = 0, yv = 2v, zv = u.

Evaluating at (u0, v0) yields

ru = ⟨xu, yu, zu⟩ = ⟨2, 0, 1⟩, rv = ⟨xv, yv, zv⟩ = ⟨0, 2, 1⟩.

It follows that the normal to the tangent plane is

n = ru × rv = ⟨2, 0, 1⟩ × ⟨0, 2, 1⟩ = ⟨−2, −2, 4⟩.

We conclude that the equation of the tangent plane is

−2(x − 1) − 2(y − 1) + 4(z − 1) = 0.

The vectors ru and rv are helpful for computing the of a smooth surface S. For simplicity, we assume that S is parametrized by a function r(u, v) with domain D, where D = [a, b] × [c, d] is a rectangle in the uv-plane. We divide [a, b] into n subintervals [ui−1, ui] of width Δu = (b − a)/n, and divide [c, d] into m subintervals [vj−1, vj] of width Δv = (d − c)/m. Then, r approximately maps the rectangle Rij with lower left corner (ui−1, vj−1) into a paral- lelogram with adjacent edges defined by the vectors

r(ui, vj−1) − r(ui−1, vj−1) ≈ ruΔu and r(ui−1, vj) − r(ui−1, vj−1) ≈ rvΔv. The area of this parallelogram is Aij = ∥ru × rv∥ΔuΔv. Adding all of these areas approximates the area of S, which we denote by A(S). If we let m, n → ∞, we obtain n m X X ZZ A(S) = lim Aij = ∥ru × rv∥ dA. m,n→∞ i=1 j=1 D

3 Example (Stewart, Section 13.6, Exercise 34) We wish to find the area of the surface S that is the part of the plane 2x + 5y + z = 10 that lies inside the x2 + y2 = 9. First, we must find parametric equations for this surface. Because x and y are restricted to the circle of radius 3 centered at the origin, it makes sense to use polar coordinates for x and y. We then have the parametric equations

x = u cos v, y = u sin v, z = 10 − u(2 cos v + 5 sin v), where 0 ≤ u ≤ 3 and 0 ≤ v ≤ 2. We then have

ru = ⟨xu, yu, zu⟩ = ⟨cos v, sin v, −2 cos v − 5 sin v⟩,

rv = ⟨xv, yv, zv⟩ = ⟨−u sin v, u cos v, u(2 sin v − 5 cos v)⟩.

We then have √ ∥ru × rv∥ = ∥⟨2u, 5u, u⟩∥ = ∣u∣ 30. It follows that Z 3 Z 2 √ √ Z 3 √ A(S) = u 30 du dv = 2 30 u du = 9 30. 0 0 0

It should be noted that it is to be expected that the direction of ru × rv is parallel to the normal vector of the plane 2x + 5y + z = 10, since it is normal to the surface at every point. □ Often, a surface is defined to be the graph of a function z = f(x, y). Such a surface can be parametrized by x = u, y = v, z = f(u, v), (u, v) ∈ D. It follows that ru = ⟨1, 0, fu⟩, rv = ⟨0, 1, fv⟩.

We then have rv × ru = ⟨fu, fv, 1⟩, which yields the equation of the tangent plane ∂f ∂f (u , v )(x − x ) + (u , v )(y − y ) + (z − z ) = 0, ∂u 0 0 0 ∂v 0 0 0 0 which, using the relations x = u and y = v, can be rewritten as ∂f ∂f (x , y )(x − x ) + (x , y )(y − y ) + (z − z ) = 0. ∂x 0 0 0 ∂y 0 0 0 0 Recall that this is the equation of the tangent plane of a surface defined by an equation of the form z = f(x, y) that had been previously defined. It follows that the area of such a surface is given by the double integral s ZZ  df 2  df 2 A(S) = 1 + + dA. D dx dy

4 Example (Stewart, Section 13.6, Exercise 38) To find the area A(S) of the surface z = 1+3x+2y2 that lies above the triangle with vertices (0, 0), (0, 1) and (2, 1), we compute ∂z ∂z = 3, = 4y, ∂x ∂y and then evaluate the double integral s Z 1 Z 2y  ∂z 2 ∂z 2 A(S) = 1 + + dx dy 0 0 ∂x ∂y Z 1 Z 2y p = 10 + 16y2 dx dy 0 0 Z 1 p = 2y 10 + 16y2 dy 0 1 Z 26 = u1/2 du 16 10 26 1 3/2 = u 24 10 1 = (263/2 − 103/2) 24 ≈ 4.206. □ A surface of revolution S that is obtained by revolving the curve y = f(x), a ≤ x ≤ b, around the x-axis has parametric equations x = u, y = f(u) cos v, z = f(u) sin v, where a ≤ u ≤ b and 0 ≤ v ≤ 2. From these equations, we obtain

p ′ 2 ∥ru × rv∥ = ∣f(u)∣ 1 + [f (u)] , which yields Z b p A(S) = 2 ∣f(u)∣ 1 + [f ′(u)]2 du. a If y = f(x) is revolved around the y-axis instead, then the area is

Z b p A(S) = 2 ∣u∣ 1 + [f ′(u)]2 du, a which can be obtained by considering the case of revolving x = f −1(y) around the y-axis and proceeding with a parametrization similar to the case of revolving around the x-axis.

5 Practice Problems

Practice problems from the recommended textbooks are:

∙ Stewart: Section 13.6, Exercises 29-43 odd

∙ Marsden/Tromba: Section 7.3, Exercises 1, 3, 11; Section 7.4, Exercises 1, 3, 5, 11, 13

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