Survey of Mathematics

6.5 Surfaces, area and flux

A surface is the image of a rectangle or disc under a map r(u, v); the cross product of its two tangent vectors is a normal whose length is the stretching factor from parameter area to surface area, and that one vector gives the area of the surface, the integral of a scalar over it, and the flux of a vector field through it.

Taught in 375/376Beyond the courseApostol Vol. 2, 12.1 to 12.9 (12.7 surface integrals, 12.8 change of parametric representation, 12.9 other notations)MATH 376 Weeks 5 and 6: lectures of 23, 25 and 27 February and 2 March, worksheets 11 to 15, 17 and 27, homework 5, Midterm 2 problems 1 and 2, Final problem 2 and its practice siblingSchwarz, the lantern counterexample (1880)

A wire is a curve and has one parameter. A sheet of metal, a soap film or the skin of a balloon is a surface and has two. This chapter answers three questions about a surface. How big is it? What is the total of some quantity spread over it, such as mass? And how much of a flow, such as water or heat, crosses it? One vector, built from two tangent vectors, answers all three, and it is the object that Stokes’ theorem and the divergence theorem in 6.6 are written with.

Before you start

2.7: a 2×22\times 2 determinant is ad−bcad - bc, and a 3×33\times 3 one is expanded along a row. 2.9: two vectors are orthogonal when their dot product is 00. 5.2: a partial derivative treats the other variables as constants. 6.1: the line integral, and the idea of an oriented curve. 6.3 and 6.4: double integrals over a region, polar coordinates, and the change of variables.

Quick checkWhat is det⁡[2−134]\det\begin{bmatrix}2 & -1\\ 3 & 4\end{bmatrix}?
Quick checkAre (1,2,2)(1, 2, 2) and (2,1,−2)(2, 1, -2) orthogonal?
Quick checkFor r(u,v)=(ucos⁡v, usin⁡v, u2)r(u, v) = (u\cos v,\ u\sin v,\ u^2), what is ∂r∂v\dfrac{\partial r}{\partial v}?

The picture: patches, normals and flux

Start with the paraboloid and F=(x,y,z)F = (x, y, z). Slide include strips and watch the green patches fill in: the flux so far is climbing. Each short orange arrow is the vector N=ru×rvN = r_u \times r_v of one patch, drawn with length 11. Now tick flip the normal: every sign changes, and so does the total. Change the field to (0,0,1)(0, 0, 1) and the cone: the flux comes out as 4π4\pi, the area of the disc under the cone, because a field that points straight up only sees the shadow of the surface. Choose the Moebius strip last and read the sentence under the picture.

The idea, in words

A curve is traced by one number tt, and r′(t)r'(t) is the velocity. A surface is traced by two numbers (u,v)(u, v). Fix vv and move uu: the point slides along a curve on the surface with velocity rur_u. Fix uu and move vv: it slides along another curve with velocity rvr_v. A tiny square of the parameter plane with sides dudu and dvdv is sent to a tiny patch of the surface, and the patch looks like a parallelogram with sides ru dur_u\,du and rv dvr_v\,dv. The area of that parallelogram is the cross product’s length ∥ru×rv∥ du dv\lVert r_u \times r_v \rVert\,du\,dv. Add up the patches and you have the area. Put a number on each patch and add, and you have a scalar surface integral. Put a field on each patch and ask how much of it goes through the parallelogram, and you have the flux.

Why· Why a cross product, and why the same vector three times

Think of a rubber sheet stretched over a frame. The parameter square is the unstretched sheet. The vector ru×rvr_u \times r_v records two things about how the sheet is stretched at one point: how much (its length) and which way the stretched patch faces (its direction, perpendicular to the patch). Area needs only the first. A scalar quantity such as density needs the first. A flow needs both, because the part of a flow that crosses a patch depends on how the patch is tilted against the flow, and a patch lying along the flow lets nothing through. So one vector, N=ru×rvN = r_u \times r_v, serves all three jobs, and the entire chapter is learning to compute it and to use it with the right sign.

Where this came from· Why area of a surface was harder than length of a curve

You can find the length of a curve by laying a polygon with corners on the curve and letting the corners get closer together. In the 1860s a standard French textbook, Serret’s Cours de calcul différentiel et intégral, said the area of a curved surface is likewise the limit of the areas of inscribed polyhedra. Around 1880 Hermann Schwarz found a cylinder for which this fails: stack thin rings of triangles with the rings twisted against each other (the shape is called Schwarz’s lantern) and the area of the polyhedron can approach a number larger than the cylinder’s area, or grow without bound, even though every corner lies on the cylinder. Peano found the same example independently around 1882. The reason is that very thin, tilted triangles can hug the cylinder at their corners while leaning far away from its tangent planes. So a definition of area must use tangent planes, not only points, and that is exactly what the fundamental vector product does. The lab in the area section runs the lantern.

The cross product

Everything below needs one operation on two vectors in space. It is worth building it from what it does, because the formula is easy to misremember.

Definition T

Cross product

The cross product of aa and bb is the vector

a×b=(a2b3−a3b2,  a3b1−a1b3,  a1b2−a2b1).a \times b = (a_2b_3 - a_3b_2,\ \ a_3b_1 - a_1b_3,\ \ a_1b_2 - a_2b_1).

It is remembered as the determinant of a 3×33\times 3 table with e1=(1,0,0)e_1 = (1,0,0), e2=(0,1,0)e_2 = (0,1,0), e3=(0,0,1)e_3 = (0,0,1) in the first row, aa in the second and bb in the third, expanded along the first row (2.7):

a×b=det⁡[e1e2e3a1a2a3b1b2b3]=e1(a2b3−a3b2)−e2(a1b3−a3b1)+e3(a1b2−a2b1).a \times b = \det\begin{bmatrix} e_1 & e_2 & e_3 \\ a_1 & a_2 & a_3 \\ b_1 & b_2 & b_3\end{bmatrix} = e_1(a_2b_3 - a_3b_2) - e_2(a_1b_3 - a_3b_1) + e_3(a_1b_2 - a_2b_1).

The middle term carries a minus sign from the cofactor expansion, which is why the middle component of the formula reads a3b1−a1b3a_3b_1 - a_1b_3 and not the other way round. Unlike the dot product, it needs three dimensions, and the result is a vector, not a number.

In one lineFor a=(a1,a2,a3)a = (a_1, a_2, a_3) and b=(b1,b2,b3)b = (b_1, b_2, b_3) in R3\mathbb R^3, a×b=(a2b3−a3b2, a3b1−a1b3, a1b2−a2b1)a \times b = (a_2b_3 - a_3b_2,\ a_3b_1 - a_1b_3,\ a_1b_2 - a_2b_1): a vector perpendicular to both, whose length is the area of the parallelogram with sides aa and bb.

Why it existsArea and direction of a tilted patch in one vector. Both are needed to measure a surface and to say which way it faces.

Why· Where the formula comes from

The lecture does not start from the formula. It starts from what the cross product must do: it is linear in each slot, a×b=− b×aa\times b = -\,b\times a (so a×a=0a\times a = 0), and e1×e2=e3e_1\times e_2 = e_3, e2×e3=e1e_2\times e_3 = e_1, e3×e1=e2e_3\times e_1 = e_2. Write a=∑aieia = \sum a_ie_i and b=∑bjejb = \sum b_je_j and multiply out using linearity: a×b=∑i,jaibj ei×eja\times b = \sum_{i,j}a_ib_j\,e_i\times e_j. The three terms with i=ji = j are 00. Pair the term (i,j)(i, j) with (j,i)(j, i), which has the opposite sign, to get ∑i<j(aibj−ajbi) ei×ej\sum_{i<j}(a_ib_j - a_jb_i)\,e_i\times e_j. The pair (1,2)(1, 2) gives (a1b2−a2b1) e3(a_1b_2 - a_2b_1)\,e_3, the pair (2,3)(2, 3) gives (a2b3−a3b2) e1(a_2b_3 - a_3b_2)\,e_1, and the pair (1,3)(1, 3) gives (a1b3−a3b1) e1×e3=(a3b1−a1b3) e2(a_1b_3 - a_3b_1)\,e_1\times e_3 = (a_3b_1 - a_1b_3)\,e_2, because e1×e3=−e3×e1=−e2e_1\times e_3 = -e_3\times e_1 = -e_2. That last minus sign is the flipped middle component.

Theorem T MATH 376 lectures of 23 and 25 February

Length and direction of the cross product

Let θ∈[0,π]\theta \in [0, \pi] be the angle between aa and bb. Then the facts in the statement hold. The sign rule e1×e2=e3e_1\times e_2 = e_3, e2×e3=e1e_2\times e_3 = e_1, e3×e1=e2e_3\times e_1 = e_2 is the right-hand rule: curl the fingers of your right hand from aa towards bb and the thumb points along a×ba\times b.

In one linea×ba \times b is orthogonal to aa and to bb; ∥a×b∥2=∥a∥2∥b∥2−(a⋅b)2\lVert a \times b\rVert^2 = \lVert a\rVert^2\lVert b\rVert^2 - (a\cdot b)^2; so ∥a×b∥=∥a∥∥b∥sin⁡θ\lVert a\times b\rVert = \lVert a\rVert\lVert b\rVert\sin\theta is the area of the parallelogram with sides aa and bb. Also b×a=−a×bb \times a = -a \times b and e1×e2=e3e_1\times e_2 = e_3.

Why it is trueIt says what the cross product is for: the direction is perpendicular to the plane of aa and bb and the length is the area, so the formula is the right vector to measure and to orient a patch.

ProofMATH 376 lecture of 25 February
The idea: Perpendicularity is a dot product that cancels term by term. The length comes from an identity that both sides expand to the same six products; then the formula for the dot product in terms of the angle turns it into the area of a parallelogram: base times height.
a⋅(a×b)=a1(a2b3−a3b2)+a2(a3b1−a1b3)+a3(a1b2−a2b1)a\cdot(a\times b) = a_1(a_2b_3 - a_3b_2) + a_2(a_3b_1 - a_1b_3) + a_3(a_1b_2 - a_2b_1).
Dot the formula with aa and multiply out.
=a1a2b3−a1a3b2+a2a3b1−a1a2b3+a1a3b2−a2a3b1=0= a_1a_2b_3 - a_1a_3b_2 + a_2a_3b_1 - a_1a_2b_3 + a_1a_3b_2 - a_2a_3b_1 = 0.
Collect: each of the six products appears once with a plus and once with a minus.Doing the same with bb shows it is perpendicular to bb. A cross product that fails these two dot products has a sign error in it.
∥a×b∥2=∑i≠jai2bj2−2 (a1a2b1b2+a1a3b1b3+a2a3b2b3)\lVert a\times b\rVert^2 = \sum_{i\ne j} a_i^2b_j^2 - 2\,(a_1a_2b_1b_2 + a_1a_3b_1b_3 + a_2a_3b_2b_3), where the sum has the six terms with i≠ji \ne j.
Square the three components. Each square gives two squared terms and one cross term.
∥a∥2∥b∥2=∑iai2bi2+∑i≠jai2bj2\lVert a\rVert^2\lVert b\rVert^2 = \sum_i a_i^2b_i^2 + \sum_{i\ne j}a_i^2b_j^2 and (a⋅b)2=∑iai2bi2+2 (a1a2b1b2+a1a3b1b3+a2a3b2b3)(a\cdot b)^2 = \sum_i a_i^2b_i^2 + 2\,(a_1a_2b_1b_2 + a_1a_3b_1b_3 + a_2a_3b_2b_3).
Multiply out the product of the two squared lengths, and the square of the dot product.
∥a∥2∥b∥2−(a⋅b)2=∥a×b∥2\lVert a\rVert^2\lVert b\rVert^2 - (a\cdot b)^2 = \lVert a\times b\rVert^2.
Subtract. The terms ∑iai2bi2\sum_i a_i^2b_i^2 cancel and what is left is the line above.
∥a×b∥2=∥a∥2∥b∥2sin⁡2θ\lVert a\times b\rVert^2 = \lVert a\rVert^2\lVert b\rVert^2\sin^2\theta.
The dot product is a⋅b=∥a∥∥b∥cos⁡θa\cdot b = \lVert a\rVert\lVert b\rVert\cos\theta (2.9), and 1−cos⁡2θ=sin⁡2θ1 - \cos^2\theta = \sin^2\theta.
∥a×b∥=∥a∥∥b∥sin⁡θ\lVert a\times b\rVert = \lVert a\rVert\lVert b\rVert\sin\theta.
Take square roots. sin⁡θ≥0\sin\theta \ge 0 on [0,π][0, \pi], so no sign is needed.
∥a×b∥\lVert a\times b\rVert is the area of the parallelogram. ■\blacksquare
A parallelogram has area base times height: the base is ∥a∥\lVert a\rVert and the height is ∥b∥sin⁡θ\lVert b\rVert\sin\theta. Swapping aa and bb flips the sign of each component in the formula.The sign claim b×a=−a×bb \times a = -a\times b is the same swap: b2a3−b3a2=−(a2b3−a3b2)b_2a_3 - b_3a_2 = -(a_2b_3 - a_3b_2), and likewise for the other two components.
Proof workshopRebuild the proof that the length of a x b is the parallelogram areaMATH 376 lecture of 25 February

Tap the lines in the order a proof would write them. Each line can only use what is already above it.

    Worked example MATH 376 worksheet 12 problems 1 and 2
    Compute (2,−1,3)×(1,4,−2)(2, -1, 3) \times (1, 4, -2), check that it is orthogonal to both vectors, and find the area of the parallelogram and of the triangle they span.

    Solution.

    1. First component. a2b3−a3b2=(−1)(−2)−(3)(4)=2−12=−10a_2b_3 - a_3b_2 = (-1)(-2) - (3)(4) = 2 - 12 = -10. Rows 22 and 33 of the pattern: ignore a1a_1 and b1b_1.
    2. Second component. a3b1−a1b3=(3)(1)−(2)(−2)=3+4=7a_3b_1 - a_1b_3 = (3)(1) - (2)(-2) = 3 + 4 = 7. Remember the flipped order: third times first, minus first times third.
    3. Third component. a1b2−a2b1=(2)(4)−(−1)(1)=8+1=9a_1b_2 - a_2b_1 = (2)(4) - (-1)(1) = 8 + 1 = 9. Ignore a3a_3 and b3b_3.
    4. Check with two dot products. (−10,7,9)⋅(2,−1,3)=−20−7+27=0(-10, 7, 9)\cdot(2, -1, 3) = -20 - 7 + 27 = 0 and (−10,7,9)⋅(1,4,−2)=−10+28−18=0(-10, 7, 9)\cdot(1, 4, -2) = -10 + 28 - 18 = 0. A cross product must be orthogonal to both factors. This catches the usual sign slip in the middle component.
    5. Length. ∥(−10,7,9)∥=100+49+81=230\lVert(-10, 7, 9)\rVert = \sqrt{100 + 49 + 81} = \sqrt{230}. The length of a×ba\times b is the parallelogram area.
    6. Triangle. The triangle with sides aa and bb is half the parallelogram, so its area is 12230\frac12\sqrt{230}.

    Answer. a×b=(−10,7,9)a\times b = (-10, 7, 9); parallelogram area 230≈15.17\sqrt{230}\approx 15.17; triangle area 12230≈7.58\frac12\sqrt{230}\approx 7.58. Worksheet 12 problem 2 is (1,2,2)×(2,0,1)=(2,3,−4)(1, 2, 2)\times(2, 0, 1) = (2, 3, -4), and the same two dot products give 2+6−8=02 + 6 - 8 = 0 and 4+0−4=04 + 0 - 4 = 0.

    Worked example MATH 376 worksheet 12 problem 3
    Find a normal vector to the plane through A=(1,0,2)A = (1, 0, 2), B=(3,−1,1)B = (3, -1, 1), C=(2,2,0)C = (2, 2, 0), and the area of the triangle ABCABC.

    Solution.

    1. Two edges from one corner. AB→=B−A=(2,−1,−1)\overrightarrow{AB} = B - A = (2, -1, -1) and AC→=C−A=(1,2,−2)\overrightarrow{AC} = C - A = (1, 2, -2). Both lie in the plane, and they are not parallel.
    2. Cross them. AB→×AC→=((−1)(−2)−(−1)(2), (−1)(1)−(2)(−2), (2)(2)−(−1)(1))=(4,3,5)\overrightarrow{AB}\times\overrightarrow{AC} = ((-1)(-2) - (-1)(2),\ (-1)(1) - (2)(-2),\ (2)(2) - (-1)(1)) = (4, 3, 5). The cross product is orthogonal to two vectors in the plane, so it is a normal to the plane.
    3. Area. 12∥(4,3,5)∥=1216+9+25=1250=522\frac12\lVert(4, 3, 5)\rVert = \frac12\sqrt{16 + 9 + 25} = \frac12\sqrt{50} = \frac{5\sqrt2}{2}. Half the parallelogram.

    Answer. A normal is (4,3,5)(4, 3, 5) and the area is 522≈3.54\frac{5\sqrt2}{2}\approx 3.54. The plane is 4(x−1)+3y+5(z−2)=04(x - 1) + 3y + 5(z - 2) = 0.

    Your answerFind the area of the triangle with vertices A=(1,1,0)A = (1, 1, 0), B=(3,1,2)B = (3, 1, 2) and C=(1,4,2)C = (1, 4, 2).
    Quick checkWhat is (1,2,3)×(2,4,6)(1, 2, 3)\times(2, 4, 6)?
    Quick checkYou compute a×ba\times b and get a vector whose dot product with aa is not 00. What happened?

    Parametric surfaces

    Definition T

    Parametric surface

    A curve needs one parameter, running over an interval. A surface needs two, running over a region TT of the plane, such as a rectangle or a disc. The map r:T→R3r: T \to \mathbb R^3 is a parametrization and S=r(T)S = r(T) is a parametric surface. When r(x,y)=(x,y,g(x,y))r(x, y) = (x, y, g(x, y)) the parametrization is explicit: SS is the graph z=g(x,y)z = g(x, y). The number of parameters is the dimension: a circle and a helix have one, a disc (even though it is flat), a cylinder and a sphere have two.

    In one lineA surface SS given by a map r(u,v)=(x(u,v), y(u,v), z(u,v))r(u, v) = (x(u, v),\ y(u, v),\ z(u, v)) from a parameter region TT in the uvuv-plane; SS is the set of points r(u,v)r(u, v) with (u,v)(u, v) in TT.

    Why it existsIt turns a two-dimensional object in space into two ordinary variables, so every question about the surface becomes a double integral over a flat region.

    Memorize this table. Each row is used all through the chapter and the next.

    SurfaceParametrizationParameter region
    graph z=g(x,y)z = g(x, y)r(x,y)=(x, y, g(x,y))r(x, y) = (x,\ y,\ g(x, y))the region DD of the xyxy-plane under it
    cylinder x2+y2=R2x^2 + y^2 = R^2r(θ,z)=(Rcos⁡θ, Rsin⁡θ, z)r(\theta, z) = (R\cos\theta,\ R\sin\theta,\ z)0≤θ≤2π0 \le \theta \le 2\pi, zz in an interval
    cone z=x2+y2z = \sqrt{x^2 + y^2}r(r,θ)=(rcos⁡θ, rsin⁡θ, r)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ r)r≥0r \ge 0, 0≤θ≤2π0 \le \theta \le 2\pi
    paraboloid z=4−x2−y2z = 4 - x^2 - y^2r(r,θ)=(rcos⁡θ, rsin⁡θ, 4−r2)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ 4 - r^2)0≤r≤20 \le r \le 2, 0≤θ≤2π0 \le \theta \le 2\pi
    sphere of radius RRr(φ,θ)=R(sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)r(\varphi, \theta) = R(\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi)0≤φ≤π0 \le \varphi \le \pi, 0≤θ≤2π0 \le \theta \le 2\pi
    ellipsoid x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1r(u,v)=(asin⁡vcos⁡u, bsin⁡vsin⁡u, ccos⁡v)r(u, v) = (a\sin v\cos u,\ b\sin v\sin u,\ c\cos v)0≤u≤2π0 \le u \le 2\pi, 0≤v≤π0 \le v \le \pi
    torus: circle of radius aa swept round a circle of radius R>aR > ar(u,v)=((R+acos⁡v)cos⁡u, (R+acos⁡v)sin⁡u, asin⁡v)r(u, v) = ((R + a\cos v)\cos u,\ (R + a\cos v)\sin u,\ a\sin v)0≤u,v≤2π0 \le u, v \le 2\pi
    plane through PP with sides a,ba, br(u,v)=P+ua+vbr(u, v) = P + ua + vb0≤u≤10 \le u \le 1, 0≤v≤10 \le v \le 1 for the parallelogram

    On the sphere, φ\varphi is the angle measured down from the north pole (the positive zz-axis) and θ\theta is the angle around the zz-axis. In the cone and paraboloid rows the letter rr is both the radius coordinate and the name of the map; the name of the map is r(⋅,⋅)r(\cdot,\cdot) with two arguments.

    Watch out· The triangle is not the parallelogram

    The set {ua+vb:0≤u,v≤1}\{ua + vb : 0\le u, v\le 1\} is the parallelogram. The set with the extra condition u+v≤1u + v \le 1 is only the triangle with corners 00, aa, bb. A wrong parameter region gives a different set, and a different answer.

    Worked example MATH 376 worksheet 11 problems 1 to 4
    Parametrize the unit sphere, the cylinder x2+y2=9x^2 + y^2 = 9 with 0<z<50 < z < 5, the slanted triangle x+2y+z=2x + 2y + z = 2 in the first octant, and the punctured disc z=xz = x with 0<x2+y2<10 < x^2 + y^2 < 1. In each case find the infimum and supremum of the coordinate xx and say whether they are attained.

    The infimum of the values of xx is the largest number that is at most every value, the supremum is the smallest number that is at least every value, and a bound is attained if some point of the surface has exactly that value of xx.

    Solution.

    1. Sphere. r(φ,θ)=(sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)r(\varphi, \theta) = (\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi), 0≤φ≤π0\le\varphi\le\pi, 0≤θ≤2π0\le\theta\le2\pi. Then x=sin⁡φcos⁡θx = \sin\varphi\cos\theta has ∣x∣≤1\lvert x\rvert \le 1, and φ=π/2\varphi = \pi/2, θ=0\theta = 0 gives x=1x = 1, while θ=π\theta = \pi gives x=−1x = -1. Both bounds are reached, so the supremum 11 and infimum −1-1 are attained.
    2. Cylinder. r(θ,z)=(3cos⁡θ, 3sin⁡θ, z)r(\theta, z) = (3\cos\theta,\ 3\sin\theta,\ z), θ∈[0,2π)\theta\in[0, 2\pi), z∈(0,5)z\in(0, 5). Then x=3cos⁡θ∈[−3,3]x = 3\cos\theta\in[-3, 3], and θ=0\theta = 0 and θ=π\theta = \pi reach both ends for any zz. Attained. The missing end circles z=0z = 0 and z=5z = 5 do not matter for xx. For the coordinate zz instead, the infimum 00 and the supremum 55 would not be attained.
    3. Triangle. The plane meets the axes at (2,0,0)(2, 0, 0), (0,1,0)(0, 1, 0), (0,0,2)(0, 0, 2). Solve for zz: r(u,v)=(u, v, 2−u−2v)r(u, v) = (u,\ v,\ 2 - u - 2v) with 0≤u≤20\le u\le2, 0≤v≤1−u/20\le v\le 1 - u/2 (this is z≥0z \ge 0). Then x=u∈[0,2]x = u\in[0, 2], with u=2u = 2 at the vertex (2,0,0)(2, 0, 0) and u=0u = 0 along the edge x=0x = 0. Both are attained: the triangle contains its edges.
    4. Punctured disc. r(r,θ)=(rcos⁡θ, rsin⁡θ, rcos⁡θ)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ r\cos\theta) with 0<r<10 < r < 1, 0≤θ≤2π0\le\theta\le2\pi. Then ∣x∣≤r<1\lvert x\rvert\le r < 1 with values arbitrarily close to 11 and −1-1 (take θ=0\theta = 0 or π\pi and r→1r\to1). The bound 11 would need r=1r = 1, which was removed, so the supremum 11 and the infimum −1-1 are not attained.

    Answer. Sphere: ±1\pm1, attained. Cylinder: ±3\pm3, attained. Triangle: 00 and 22, attained. Punctured disc: ±1\pm1, not attained. (The worksheet calls a surface ‘closed’ when it has no boundary curve, like the sphere, and ‘open’ when it has one. That is a different use of the words from the point-set words in 4.1.)

    Worked example MATH 376 worksheet 15 problem 1
    Parametrize each of: a circle of radius RR, a disc of radius RR, a helix of radius RR and one turn of height HH, and a cylinder of radius RR and height hh. How many parameters does each need?

    Solution.

    1. Circle. (Rcos⁡t, Rsin⁡t)(R\cos t,\ R\sin t), 0≤t≤2π0\le t\le2\pi: one parameter, an interval.
    2. Disc. (rcos⁡θ, rsin⁡θ)(r\cos\theta,\ r\sin\theta), 0≤r≤R0\le r\le R, 0≤θ≤2π0\le\theta\le2\pi: two parameters. The disc is flat and lives in the plane, but it is a surface: it takes two numbers to name a point.
    3. Helix. (Rcos⁡t, Rsin⁡t, Ht/(2π))(R\cos t,\ R\sin t,\ Ht/(2\pi)), 0≤t≤2π0\le t\le2\pi: one parameter. It is a curve in space.
    4. Cylinder. (Rcos⁡θ, Rsin⁡θ, z)(R\cos\theta,\ R\sin\theta,\ z), 0≤θ≤2π0\le\theta\le2\pi, 0≤z≤h0\le z\le h: two parameters.

    Answer. One, two, one, two. A curve has a one-dimensional parameter set and a surface a two-dimensional one, whatever space they sit in.

    The fundamental vector product

    Fix a point (u0,v0)(u_0, v_0) of the parameter region. The partial derivatives ru=∂r/∂ur_u = \partial r/\partial u and rv=∂r/∂vr_v = \partial r/\partial v are two vectors at the point r(u0,v0)r(u_0, v_0). Moving uu by a little bit δ\delta moves the point by about δ ru\delta\,r_u (the linear approximation of 5.3), and moving vv by δ\delta moves it by about δ rv\delta\,r_v. So the small square [u0,u0+δ]×[v0,v0+δ][u_0, u_0 + \delta]\times[v_0, v_0+\delta] is sent to a patch that is, to first order, the parallelogram with sides δ ru\delta\,r_u and δ rv\delta\,r_v. By the theorem above, its area is ∥ru×rv∥ δ2\lVert r_u\times r_v\rVert\,\delta^2.

    Definition T

    Fundamental vector product

    The fundamental vector product of rr at (u,v)(u, v) is

    N(u,v)=ru×rv.N(u, v) = r_u \times r_v.

    The parametrization is regular at (u,v)(u, v) if N(u,v)≠0N(u, v) \ne 0, and smooth if it is regular at every point (and rr is continuously differentiable). Where N=0N = 0 the two tangent vectors are parallel or one of them is zero, the patch collapses to a segment or a point, there is no tangent plane and no unit normal.

    In one lineFor a parametrization r(u,v)r(u, v) the vector N(u,v)=ru×rvN(u, v) = r_u \times r_v. It is normal to the surface and ∥N∥\lVert N\rVert is the area of the image of a unit parameter square. The parametrization is regular where N≠0N \ne 0 and smooth if it is regular everywhere.

    Why it existsIt is the one vector that carries the facing direction and the stretching factor of a surface patch, so every surface integral is written with it.

    Theorem T MATH 376 lectures of 23 to 27 February; Apostol 12.1 to 12.5

    Normal and area element of a parametrized surface

    At a regular point, NN is orthogonal to rur_u and rvr_v, which span the tangent plane, so it is a normal vector to the surface. The unit normal is n=N/∥N∥n = N/\lVert N\rVert. A small parameter rectangle of area du dvdu\,dv is sent to a patch of area ∥N∥ du dv\lVert N\rVert\,du\,dv to first order, so we write dS=∥N∥ du dvdS = \lVert N\rVert\,du\,dv.

    In one lineN=ru×rvN = r_u \times r_v is perpendicular to the tangent plane at each regular point, and the area element is dS=∥ru×rv∥ du dvdS = \lVert r_u\times r_v\rVert\,du\,dv.

    Why it is trueThis is the whole reason the cross product enters surface integrals: its direction is the normal and its length is the area stretching factor.

    The theorem is the computation above: the first sentence is the perpendicularity part of the cross product theorem, and the second is its length part applied to the patch with sides ru dur_u\,du and rv dvr_v\,dv. The ideas of linear approximation in 5.3 are what turn “to first order” into a limit, and it is the same limit that defines the surface area in the next section.

    Proposition T MATH 376 lecture of 2 March and worksheet 12; Apostol 12.5

    Normal of a graph

    For a graph of a continuously differentiable function gg, the parametrization r(x,y)=(x,y,g(x,y))r(x, y) = (x, y, g(x, y)) has the stated fundamental vector product, and it is regular everywhere.

    In one lineFor the graph z=g(x,y)z = g(x, y) with r(x,y)=(x,y,g(x,y))r(x, y) = (x, y, g(x, y)): rx×ry=(−gx,−gy,1)r_x \times r_y = (-g_x, -g_y, 1), which points upward, and ∥rx×ry∥=1+gx2+gy2\lVert r_x\times r_y\rVert = \sqrt{1 + g_x^2 + g_y^2}.

    Why it is trueGraphs are the most common surfaces, and this formula turns most flux and area problems about them into a one-line computation.

    ProofMATH 376 lecture of 2 March
    The idea: Differentiate, then cross. The first two components of the cross product each have one zero factor, and the third is a determinant of a matrix with $1, 0, 0, 1$ in it.
    rx=(1,0,gx)r_x = (1, 0, g_x) and ry=(0,1,gy)r_y = (0, 1, g_y).
    Differentiate each coordinate of r(x,y)=(x,y,g(x,y))r(x, y) = (x, y, g(x, y)) with respect to xx and then yy.
    rx×ry=(0⋅gy−gx⋅1,  gx⋅0−1⋅gy,  1⋅1−0⋅0)r_x\times r_y = (0\cdot g_y - g_x\cdot1,\ \ g_x\cdot0 - 1\cdot g_y,\ \ 1\cdot1 - 0\cdot0).
    The cross product formula with a=rxa = r_x and b=ryb = r_y.
    =(−gx, −gy, 1)= (-g_x,\ -g_y,\ 1).
    Evaluate each component.The third component is +1+1 for every graph: that is why rx×ryr_x\times r_y always points up, and why we say 'upward' for a graph without checking anything else.
    ∥rx×ry∥=gx2+gy2+1\lVert r_x\times r_y\rVert = \sqrt{g_x^2 + g_y^2 + 1}. ■\blacksquare
    Length of a vector: square root of the sum of squares. It is at least 11, so never zero.
    Why· The same fact seen from the side

    The factor 1+gx2+gy2\sqrt{1 + g_x^2 + g_y^2} equals 1/cos⁡γ1/\cos\gamma, where γ\gamma is the angle between the upward normal and the vertical. A steep patch has a large γ\gamma and its true area is its shadow on the xyxy-plane divided by cos⁡γ\cos\gamma: a roof of slope 11 (gx=1g_x = 1, gy=0g_y = 0) has 2\sqrt2 times the area of the floor under it. This is also why a flat piece of paper held at an angle shades less of the table than it covers.

    Worked example MATH 376 worksheet 11 problem 5
    Find the tangent vectors and the fundamental vector product of r(u,v)=(u2, sin⁡(uv), ev)r(u, v) = (u^2,\ \sin(uv),\ e^v) at (u,v)=(1,0)(u, v) = (1, 0).

    Solution.

    1. Differentiate in uu. ru=(2u, vcos⁡(uv), 0)r_u = (2u,\ v\cos(uv),\ 0). Chain rule on sin⁡(uv)\sin(uv): the derivative of uvuv in uu is vv. The last coordinate has no uu.
    2. Differentiate in vv. rv=(0, ucos⁡(uv), ev)r_v = (0,\ u\cos(uv),\ e^v).
    3. Evaluate at (1,0)(1, 0). ru=(2,0,0)r_u = (2, 0, 0) and rv=(0,1,1)r_v = (0, 1, 1). vcos⁡(uv)=0v\cos(uv) = 0 and ucos⁡(uv)=cos⁡0=1u\cos(uv) = \cos 0 = 1, e0=1e^0 = 1.
    4. Cross. N=(0⋅1−0⋅1, 0⋅0−2⋅1, 2⋅1−0⋅0)=(0,−2,2)N = (0\cdot1 - 0\cdot1,\ 0\cdot0 - 2\cdot1,\ 2\cdot1 - 0\cdot0) = (0, -2, 2).
    5. Check. N⋅ru=0N\cdot r_u = 0 and N⋅rv=−2+2=0N\cdot r_v = -2 + 2 = 0. The free check from the cross product theorem.

    Answer. ru=(2,0,0)r_u = (2, 0, 0), rv=(0,1,1)r_v = (0, 1, 1), N=(0,−2,2)N = (0, -2, 2).

    Worked example new (compare 5.3)
    Find the equation of the tangent plane to the paraboloid z=x2+y2z = x^2 + y^2 at (1,1,2)(1, 1, 2) from the fundamental vector product.

    Solution.

    1. Normal of a graph. g=x2+y2g = x^2 + y^2 has gx=2x=2g_x = 2x = 2 and gy=2y=2g_y = 2y = 2 at the point, so N=(−2,−2,1)N = (-2, -2, 1). The graph formula.
    2. Plane through the point with this normal. −2(x−1)−2(y−1)+(z−2)=0-2(x - 1) - 2(y - 1) + (z - 2) = 0, that is z=2x+2y−2z = 2x + 2y - 2. The tangent plane is the set of points XX with N⋅(X−p)=0N\cdot(X - p) = 0.
    3. Check against 5.3. The level-surface gradient of f=x2+y2−zf = x^2 + y^2 - z is (2x,2y,−1)=(2,2,−1)(2x, 2y, -1) = (2, 2, -1), which is −N-N. Same line, opposite direction: both are normals, so both describe the same plane.

    Answer. z=2x+2y−2z = 2x + 2y - 2.

    Worked example MATH 376 Midterm 2 problem 1(a); see [A.3](/vol2/a3-midterm-2/)
    Find the normal field of the surface S={(u,v,eu):0≤u,v≤1}S = \{(u, v, e^u) : 0 \le u, v \le 1\} pointing in the positive zz direction.

    Solution.

    1. Parametrize. r(u,v)=(u,v,eu)r(u, v) = (u, v, e^u). It is the graph of z=exz = e^x over the unit square, with u=xu = x and v=yv = y.
    2. Tangent vectors. ru=(1,0,eu)r_u = (1, 0, e^u) and rv=(0,1,0)r_v = (0, 1, 0).
    3. Cross. N=ru×rv=(0⋅0−eu⋅1, eu⋅0−1⋅0, 1⋅1−0⋅0)=(−eu,0,1)N = r_u\times r_v = (0\cdot0 - e^u\cdot1,\ e^u\cdot0 - 1\cdot0,\ 1\cdot1 - 0\cdot0) = (-e^u, 0, 1). The third component is +1>0+1 > 0, so it points in the positive zz direction as the problem asks. No sign flip.
    4. Length. ∥N∥=e2u+1\lVert N\rVert = \sqrt{e^{2u} + 1}.
    5. Normalize. n=(−eu, 0, 1)e2u+1n = \dfrac{(-e^u,\ 0,\ 1)}{\sqrt{e^{2u} + 1}}. The unit normal is NN divided by its length.

    Answer. n=(−eu,0,1)/e2u+1n = (-e^u, 0, 1)/\sqrt{e^{2u} + 1}. The practice exam asks the same for (u,v,v−u3)(u, v, v - u^3) (A.5), where ru=(1,0,−3u2)r_u = (1, 0, -3u^2), rv=(0,1,1)r_v = (0, 1, 1) and N=(3u2,−1,1)N = (3u^2, -1, 1) come out the same way.

    Quick checkFor the surface r(u,v)=(u,v,u2+v2)r(u, v) = (u, v, u^2 + v^2), which is the fundamental vector product?

    Surface area

    Definition T

    Surface area

    For a smooth parametrization r:T→Sr: T\to S of a surface SS, the surface area of SS is

    area⁡(S)=∬T∥ru×rv∥ du dv.\operatorname{area}(S) = \iint_T \lVert r_u\times r_v\rVert\,du\,dv.

    For a graph z=g(x,y)z = g(x, y) over a region DD this becomes ∬D1+gx2+gy2 dx dy\iint_D \sqrt{1 + g_x^2 + g_y^2}\,dx\,dy.

    In one lineThe area of S=r(T)S = r(T) for a smooth parametrization is ∬T∥ru×rv∥ du dv\iint_T \lVert r_u \times r_v\rVert\,du\,dv.

    Why it existsIt adds up the areas ∥N∥ du dv\lVert N\rVert\,du\,dv of the parallelogram patches, and is the only definition that survives the Schwarz lantern.

    Method: (1) parametrize, using the constraints of the problem to set the parameter ranges; (2) compute rur_u, rvr_v and N=ru×rvN = r_u\times r_v; (3) take the length; (4) integrate over the parameter region.

    Worked example MATH 376 Midterm 2 problem 2, 6 points; see [A.3](/vol2/a3-midterm-2/)
    Find the area of the part of the paraboloid z=34−x2−y2z = \frac34 - x^2 - y^2 above the plane z=0z = 0, using cylindrical coordinates. (Hint: ddr(1+4r2)3/2=12 r1+4r2\frac{d}{dr}(1 + 4r^2)^{3/2} = 12\,r\sqrt{1 + 4r^2}.)

    Solution.

    1. Parameter ranges. z≥0z\ge0 means 34−r2≥0\frac34 - r^2\ge0, so 0≤r≤320\le r\le\frac{\sqrt3}2 and 0≤θ≤2π0\le\theta\le2\pi. The constraint of the problem is what sets the limits.
    2. Parametrize. r(r,θ)=(rcos⁡θ, rsin⁡θ, 34−r2)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ \frac34 - r^2).
    3. Tangent vectors. rr=(cos⁡θ, sin⁡θ, −2r)r_r = (\cos\theta,\ \sin\theta,\ -2r) and rθ=(−rsin⁡θ, rcos⁡θ, 0)r_\theta = (-r\sin\theta,\ r\cos\theta,\ 0).
    4. Cross. rr×rθ=(sin⁡θ⋅0−(−2r)(rcos⁡θ), (−2r)(−rsin⁡θ)−cos⁡θ⋅0, cos⁡θ⋅rcos⁡θ+sin⁡θ⋅rsin⁡θ)=(2r2cos⁡θ, 2r2sin⁡θ, r)r_r\times r_\theta = (\sin\theta\cdot0 - (-2r)(r\cos\theta),\ (-2r)(-r\sin\theta) - \cos\theta\cdot0,\ \cos\theta\cdot r\cos\theta + \sin\theta\cdot r\sin\theta) = (2r^2\cos\theta,\ 2r^2\sin\theta,\ r).
    5. Length. 4r4cos⁡2θ+4r4sin⁡2θ+r2=4r4+r2=r1+4r2\sqrt{4r^4\cos^2\theta + 4r^4\sin^2\theta + r^2} = \sqrt{4r^4 + r^2} = r\sqrt{1 + 4r^2}. cos⁡2+sin⁡2=1\cos^2 + \sin^2 = 1, then pull r2r^2 out of the root; this is allowed because r≥0r\ge0.
    6. Integrate in rr. By the hint, ∫03/2r1+4r2 dr=112[(1+4r2)3/2]03/2=112(43/2−1)=712\int_0^{\sqrt3/2}r\sqrt{1 + 4r^2}\,dr = \frac1{12}\big[(1 + 4r^2)^{3/2}\big]_0^{\sqrt3/2} = \frac1{12}(4^{3/2} - 1) = \frac7{12}. At r=3/2r = \sqrt3/2: 1+4⋅34=41 + 4\cdot\frac34 = 4 and 43/2=84^{3/2} = 8. At r=0r = 0 the value is 11. If there were no hint, you would guess a multiple of (1+4r2)3/2(1+4r^2)^{3/2} and differentiate it to find the multiple.
    7. Integrate in θ\theta. The inner integral does not depend on θ\theta, so multiply by 2π2\pi: 2π⋅712=7π62\pi\cdot\frac7{12} = \frac{7\pi}6.

    Answer. 7π6≈3.665\dfrac{7\pi}{6}\approx3.665. The flat disc under it has area π⋅34=2.356\pi\cdot\frac34 = 2.356, and the cap is bigger because it is tilted.

    Worked example MATH 376 practice Midterm 2 problem 2; see [A.5](/vol2/a5-practice-exams/)
    Find the area of the cone z=x2+y2z = \sqrt{x^2 + y^2} between the planes z=0z = 0 and z=21/4z = 2^{1/4}, using cylindrical coordinates.

    Solution.

    1. Parametrize. r(r,θ)=(rcos⁡θ, rsin⁡θ, r)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ r) with 0≤r≤21/40\le r\le2^{1/4}, 0≤θ≤2π0\le\theta\le2\pi. On the cone z=rz = r, so 0≤z≤21/40\le z\le2^{1/4} is 0≤r≤21/40\le r\le2^{1/4}.
    2. Cross. rr=(cos⁡θ,sin⁡θ,1)r_r = (\cos\theta, \sin\theta, 1) and rθ=(−rsin⁡θ,rcos⁡θ,0)r_\theta = (-r\sin\theta, r\cos\theta, 0), so rr×rθ=(−rcos⁡θ, −rsin⁡θ, r)r_r\times r_\theta = (-r\cos\theta,\ -r\sin\theta,\ r).
    3. Length. ∥⋅∥=r2cos⁡2θ+r2sin⁡2θ+r2=r2\lVert\cdot\rVert = \sqrt{r^2\cos^2\theta + r^2\sin^2\theta + r^2} = r\sqrt2.
    4. Integrate. ∫02π ⁣ ⁣∫021/42 r dr dθ=2π2⋅(21/4)22=2π2⋅22=2π\displaystyle\int_0^{2\pi}\!\!\int_0^{2^{1/4}}\sqrt2\,r\,dr\,d\theta = 2\pi\sqrt2\cdot\frac{(2^{1/4})^2}{2} = 2\pi\sqrt2\cdot\frac{\sqrt2}2 = 2\pi.
    5. Check with geometry. The lateral area of a cone is π⋅radius⋅slant height=π⋅21/4⋅2⋅21/4=π2⋅2=2π\pi\cdot\text{radius}\cdot\text{slant height} = \pi\cdot2^{1/4}\cdot\sqrt2\cdot2^{1/4} = \pi\sqrt2\cdot\sqrt2 = 2\pi. A second method, from high-school geometry, agrees.

    Answer. 2π2\pi. At the apex r=0r = 0 the vector NN is 00, so the parametrization is not regular there. The apex is a single point, so it changes no integral.

    Worked example Apostol 12.5 (sphere); new (torus)
    Find the area of a sphere of radius RR, and of the torus with radii R>aR > a.

    Solution.

    1. Sphere, tangent vectors. r(φ,θ)=R(sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)r(\varphi,\theta) = R(\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi) has rφ=R(cos⁡φcos⁡θ, cos⁡φsin⁡θ, −sin⁡φ)r_\varphi = R(\cos\varphi\cos\theta,\ \cos\varphi\sin\theta,\ -\sin\varphi) and rθ=R(−sin⁡φsin⁡θ, sin⁡φcos⁡θ, 0)r_\theta = R(-\sin\varphi\sin\theta,\ \sin\varphi\cos\theta,\ 0).
    2. Sphere, cross. rφ×rθ=R2sin⁡φ (sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)r_\varphi\times r_\theta = R^2\sin\varphi\,(\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi). The first component is 0−(−sin⁡φ)(sin⁡φcos⁡θ)R2=R2sin⁡2φcos⁡θ0 - (-\sin\varphi)(\sin\varphi\cos\theta)R^2 = R^2\sin^2\varphi\cos\theta, and similarly for the others. The third is R2sin⁡φcos⁡φ(cos⁡2θ+sin⁡2θ)R^2\sin\varphi\cos\varphi(\cos^2\theta + \sin^2\theta).
    3. Sphere, length. The vector in brackets has length 11, and sin⁡φ≥0\sin\varphi\ge0 on [0,π][0, \pi], so ∥N∥=R2sin⁡φ\lVert N\rVert = R^2\sin\varphi.
    4. Sphere, integrate. ∫02π ⁣∫0πR2sin⁡φ dφ dθ=2πR2⋅2=4πR2\int_0^{2\pi}\!\int_0^\pi R^2\sin\varphi\,d\varphi\,d\theta = 2\pi R^2\cdot2 = 4\pi R^2.
    5. Torus. With r(u,v)=((R+acos⁡v)cos⁡u, (R+acos⁡v)sin⁡u, asin⁡v)r(u, v) = ((R + a\cos v)\cos u,\ (R + a\cos v)\sin u,\ a\sin v) the cross product ru×rv=a(R+acos⁡v) (cos⁡ucos⁡v, sin⁡ucos⁡v, sin⁡v)r_u\times r_v = a(R + a\cos v)\,(\cos u\cos v,\ \sin u\cos v,\ \sin v), which has length a(R+acos⁡v)a(R + a\cos v) since R>aR > a. Same pattern as the sphere: a scalar times an outward unit vector.
    6. Torus, integrate. ∫02π ⁣∫02πa(R+acos⁡v) du dv=2π⋅a⋅(2πR+0)=4π2Ra\int_0^{2\pi}\!\int_0^{2\pi}a(R + a\cos v)\,du\,dv = 2\pi\cdot a\cdot(2\pi R + 0) = 4\pi^2Ra. ∫02πcos⁡v dv=0\int_0^{2\pi}\cos v\,dv = 0.

    Answer. Sphere 4πR24\pi R^2. Torus 4π2Ra4\pi^2Ra: the length of the core circle, 2πR2\pi R, times the circumference of the tube, 2πa2\pi a.

    Worked example Apostol 12.5 (surfaces of revolution)
    Derive the high-school formula 2π∫y1+y′2 dx2\pi\int y\sqrt{1 + y'^2}\,dx for the area of a surface of revolution, and use it to show that the part of a sphere of radius RR between two parallel planes at distance hh has area 2πRh2\pi Rh.

    Solution.

    1. Parametrize the surface of revolution. Rotate the graph y=f(x)≥0y = f(x)\ge0, a≤x≤ba\le x\le b, about the xx-axis: r(x,θ)=(x, f(x)cos⁡θ, f(x)sin⁡θ)r(x, \theta) = (x,\ f(x)\cos\theta,\ f(x)\sin\theta).
    2. Cross. rx=(1, f′cos⁡θ, f′sin⁡θ)r_x = (1,\ f'\cos\theta,\ f'\sin\theta) and rθ=(0, −fsin⁡θ, fcos⁡θ)r_\theta = (0,\ -f\sin\theta,\ f\cos\theta), so rx×rθ=(ff′, −fcos⁡θ, −fsin⁡θ)r_x\times r_\theta = (ff',\ -f\cos\theta,\ -f\sin\theta). First: f′cos⁡θ⋅fcos⁡θ+f′sin⁡θ⋅fsin⁡θ=ff′f'\cos\theta\cdot f\cos\theta + f'\sin\theta\cdot f\sin\theta = ff'. Second: f′sin⁡θ⋅0−1⋅fcos⁡θf'\sin\theta\cdot0 - 1\cdot f\cos\theta. Third: 1⋅(−fsin⁡θ)−01\cdot(-f\sin\theta) - 0.
    3. Length. f2f′2+f2=f1+f′2\sqrt{f^2f'^2 + f^2} = f\sqrt{1 + f'^2}.
    4. Area. ∫ab∫02πf1+f′2 dθ dx=2π∫abf1+f′2 dx\int_a^b\int_0^{2\pi}f\sqrt{1 + f'^2}\,d\theta\,dx = 2\pi\int_a^bf\sqrt{1 + f'^2}\,dx. That is the formula from JEE: the rule you used is this computation with the angle already integrated.
    5. The sphere. For f=R2−x2f = \sqrt{R^2 - x^2}, f′=−x/ff' = -x/f, so f1+f′2=f2+x2=Rf\sqrt{1 + f'^2} = \sqrt{f^2 + x^2} = R.
    6. The zone. The area between x=ax = a and x=bx = b is 2πR (b−a)=2πRh2\pi R\,(b - a) = 2\pi Rh. It does not depend on where the planes cut: slices of equal thickness have equal area (Archimedes).

    Answer. The zone has area 2πRh2\pi Rh; the whole sphere (h=2Rh = 2R) has area 4πR24\pi R^2.

    Your answerFind the area of the part of the paraboloid z=x2+y2z = x^2 + y^2 with z≤1z \le 1.
    Your answerFind the area of the torus whose core circle has radius 33 and whose tube has radius 11.
    Beyond the course: for understanding· Label B: the lantern and the torus

    Schwarz’s lantern, the surface of revolution formula and the torus are beyond MATH 376, which set area problems only for graphs, the cone and the paraboloid cap. They are here to show why the definition of area uses tangent planes and to give more surfaces to practise the cross product on.

    Python labArea of a surface by a mesh of triangles, and Schwarz's lantern
    import numpy as np
    
    def mesh_area(r, a, b, c, d, n):
        u = np.linspace(a, b, n + 1); v = np.linspace(c, d, n + 1)
        U, V = np.meshgrid(u, v, indexing="ij")
        P = np.stack(r(U, V), axis=-1)
        A, B, C, D = P[:-1, :-1], P[1:, :-1], P[1:, 1:], P[:-1, 1:]
        tri = lambda p, q, s: 0.5 * np.linalg.norm(np.cross(q - p, s - p), axis=-1).sum()
        return tri(A, B, C) + tri(A, C, D)
    
    sphere = lambda ph, th: (np.sin(ph) * np.cos(th), np.sin(ph) * np.sin(th), np.cos(ph))
    print("n   mesh area of unit sphere   error")
    for n in (4, 8, 16, 32, 64):
        A = mesh_area(sphere, 0, np.pi, 0, 2 * np.pi, n)
        print(f"{n:3d}  {A:.6f}  {abs(A - 4 * np.pi):.6f}")
    
    def lantern(m, n):   # m slabs, n points per ring, neighbouring rings twisted by pi/n
        return 2 * n * m * np.sin(np.pi / n) * np.sqrt(1 / m**2 + (1 - np.cos(np.pi / n))**2)
    
    print("true area of the cylinder:", round(2 * np.pi, 4))
    for n in (10, 20, 40):
        print(n, " m=n:", round(lantern(n, n), 4), " m=n^2:", round(lantern(n**2, n), 4), " m=n^3:", round(lantern(n**3, n), 1))

    Try this. Run it. The first table cuts the sphere into n by n parameter squares, each into two flat triangles, and adds the triangle areas (half the length of a cross product). The error against 4*pi shrinks by a factor of about 4 each time n doubles, so it falls like 1/n^2 and the mesh area converges. The second part is Schwarz's lantern: a cylinder of radius 1 and height 1, true area 2*pi = 6.2832, replaced by a polyhedron with m rings of n points, every corner on the cylinder. With m = n the area goes to 2*pi. With m = n^2 it goes to about 31.6, five times too big. With m = n^3 it grows without bound. All three have more and more triangles and every corner on the cylinder. Change m to 2*n or to n**2.5 and predict before you run.

    Quick checkA cylinder of radius 33 is parametrized by r(θ,z)=(3cos⁡θ,3sin⁡θ,z)r(\theta, z) = (3\cos\theta, 3\sin\theta, z) on the rectangle [0,2π]×[0,3][0, 2\pi]\times[0, 3]. Which is the area of the cylinder?
    Quick checkThe apex of the cone r(r,θ)=(rcos⁡θ,rsin⁡θ,r)r(r, \theta) = (r\cos\theta, r\sin\theta, r) is the point r=0r = 0. What is rr×rθr_r\times r_\theta there?

    Integrating a scalar over a surface

    Definition T

    Surface integral

    The surface integral of a continuous scalar field ff over S=r(T)S = r(T) is

    ∬Sf dS=∬Tf(r(u,v)) ∥ru×rv∥ du dv.\iint_S f\,dS = \iint_T f(r(u, v))\,\lVert r_u\times r_v\rVert\,du\,dv.

    The parametrization must be smooth, so that ∥N∥>0\lVert N\rVert > 0 and dSdS is a genuine area element, and ff must be continuous on a set containing SS. With f=1f = 1 this is the area; if f=ρf = \rho is a mass per unit area, it is the mass of the sheet.

    In one lineFor a continuous scalar field ff and a smooth parametrization r:T→Sr: T \to S, ∬Sf dS=∬Tf(r(u,v)) ∥ru×rv∥ du dv\iint_S f\,dS = \iint_T f(r(u, v))\,\lVert r_u\times r_v\rVert\,du\,dv.

    Why it existsIt adds up ff times area over the patches. With f=1f = 1 it is the area, with ff a density it is the mass.

    Watch out· The factor that cannot be dropped

    The parameter region has area ∬Tdu dv\iint_T du\,dv and the surface has area ∬T∥N∥ du dv\iint_T\lVert N\rVert\,du\,dv. They agree only when ∥N∥=1\lVert N\rVert = 1. For a scalar integral you need ∥N∥\lVert N\rVert, once, as a factor. Never replace dSdS by du dvdu\,dv.

    Worked example MATH 376 worksheet 13 problems 3 and 4
    Compute ∬Sz2 dS\iint_S z^2\,dS over the cylinder x2+y2=9x^2 + y^2 = 9, 0≤z≤30\le z\le3, and ∬S(x+y+z) dS\iint_S(x + y + z)\,dS over the top face z=1z = 1 of the unit cube.

    Solution.

    1. Cylinder, parametrize. r(θ,z)=(3cos⁡θ, 3sin⁡θ, z)r(\theta, z) = (3\cos\theta,\ 3\sin\theta,\ z), 0≤θ≤2π0\le\theta\le2\pi, 0≤z≤30\le z\le3. Then rθ×rz=(3cos⁡θ, 3sin⁡θ, 0)r_\theta\times r_z = (3\cos\theta,\ 3\sin\theta,\ 0), of length 33.
    2. Cylinder, integrate. ∫02π ⁣∫03z2⋅3 dz dθ=3⋅2π⋅9=54π\int_0^{2\pi}\!\int_0^3z^2\cdot3\,dz\,d\theta = 3\cdot2\pi\cdot9 = 54\pi. The integrand does not depend on θ\theta. ∫03z2 dz=9\int_0^3z^2\,dz = 9.
    3. Top face. r(x,y)=(x,y,1)r(x, y) = (x, y, 1) has N=(0,0,1)N = (0, 0, 1) and ∥N∥=1\lVert N\rVert = 1, so dS=dAdS = dA. A flat horizontal face is not stretched.
    4. Top face, integrate. ∫01 ⁣∫01(x+y+1) dx dy=∫01(12+y+1) dy=12+12+1=2\int_0^1\!\int_0^1(x + y + 1)\,dx\,dy = \int_0^1(\tfrac12 + y + 1)\,dy = \tfrac12 + \tfrac12 + 1 = 2.

    Answer. 54π54\pi and 22.

    Worked example MATH 376 homework 5 problem 2
    Compute ∬S(x2+y2+z2) dS\iint_S(x^2 + y^2 + z^2)\,dS over the triangle with vertices (1,0,0)(1, 0, 0), (0,1,0)(0, 1, 0), (0,0,1)(0, 0, 1).

    Solution.

    1. Plane and graph. The triangle lies in x+y+z=1x + y + z = 1, so z=1−x−yz = 1 - x - y over D={x,y≥0, x+y≤1}D = \{x, y\ge0,\ x + y\le1\}.
    2. Normal. N=(−gx,−gy,1)=(1,1,1)N = (-g_x, -g_y, 1) = (1, 1, 1), so ∥N∥=3\lVert N\rVert = \sqrt3, a constant, and dS=3 dAdS = \sqrt3\,dA.
    3. Use symmetry. Swapping the names of two coordinates maps the triangle onto itself and keeps dSdS, so ∬x2 dS=∬y2 dS=∬z2 dS\iint x^2\,dS = \iint y^2\,dS = \iint z^2\,dS. This turns a three-term integral into three times one.
    4. Integrate one term. 33∬Dx2 dA=33∫01x2(1−x) dx=33(13−14)=33⋅112=343\sqrt3\iint_Dx^2\,dA = 3\sqrt3\int_0^1x^2(1 - x)\,dx = 3\sqrt3\big(\tfrac13 - \tfrac14\big) = 3\sqrt3\cdot\tfrac1{12} = \tfrac{\sqrt3}4.

    Answer. 34\dfrac{\sqrt3}4.

    Worked example MATH 376 worksheet 12 problem 8
    Find the mass of the surface z=x2+y2z = x^2 + y^2, x2+y2≤1x^2 + y^2\le1, with density ρ=2+z\rho = 2 + z.

    Solution.

    1. Normal. N=(−2x,−2y,1)N = (-2x, -2y, 1), ∥N∥=1+4r2\lVert N\rVert = \sqrt{1 + 4r^2} in polar coordinates, and ρ=2+r2\rho = 2 + r^2.
    2. Set up. M=∫02π ⁣∫01(2+r2)1+4r2 r dr dθM = \int_0^{2\pi}\!\int_0^1(2 + r^2)\sqrt{1 + 4r^2}\,r\,dr\,d\theta. Here dA=r dr dθdA = r\,dr\,d\theta is the Jacobian of polar coordinates (6.4), separate from the ∥N∥\lVert N\rVert factor.
    3. Substitute. s=1+4r2s = 1 + 4r^2, r dr=ds/8r\,dr = ds/8, r2=(s−1)/4r^2 = (s-1)/4, 2+r2=(s+7)/42 + r^2 = (s + 7)/4, limits s=1s = 1 to 55. Then M=2π⋅14⋅18∫15(s+7)s1/2 ds=π16∫15(s3/2+7s1/2) dsM = 2\pi\cdot\frac14\cdot\frac18\int_1^5(s + 7)s^{1/2}\,ds = \frac\pi{16}\int_1^5(s^{3/2} + 7s^{1/2})\,ds.
    4. Integrate. π16[25s5/2+143s3/2]15=π16(10053−7615)\frac\pi{16}\big[\frac25s^{5/2} + \frac{14}3s^{3/2}\big]_1^5 = \frac\pi{16}\Big(\frac{100\sqrt5}{3} - \frac{76}{15}\Big). At s=5s = 5: 25⋅255+143⋅55=105+7053\frac25\cdot25\sqrt5 + \frac{14}3\cdot5\sqrt5 = 10\sqrt5 + \frac{70\sqrt5}3. At s=1s = 1: 25+143=7615\frac25 + \frac{14}3 = \frac{76}{15}.
    5. Simplify. π16⋅5005−7615=π(1255−19)60≈13.64\frac\pi{16}\cdot\frac{500\sqrt5 - 76}{15} = \dfrac{\pi(125\sqrt5 - 19)}{60}\approx13.64.

    Answer. π(1255−19)60≈13.64\dfrac{\pi(125\sqrt5 - 19)}{60}\approx13.64. The same method gives ∬Sz dS=π(1755−41)60≈18.34\iint_S z\,dS = \frac{\pi(175\sqrt5 - 41)}{60}\approx18.34 for z=4−x2−y2z = 4 - x^2 - y^2 over r≤1r\le1 (worksheet 27 problem 8; the course solution stops at the antiderivative, and this value was recomputed).

    Your answerCompute ∬Sz dS\iint_S z\,dS over the upper unit hemisphere x2+y2+z2=1x^2 + y^2 + z^2 = 1, z≥0z\ge0.

    Orientation and flux

    For a flow we need more than area. A surface has two sides, and flux counts a crossing as positive when it goes one way and negative when it goes the other. We must say which way is positive.

    Definition T

    Oriented surface

    An orientation of a surface SS is a continuous choice of unit normal nn at every point of SS. A surface with an orientation is an oriented surface. A given smooth surface that has one orientation has exactly two, nn and −n-n. A problem tells you which: ‘upward’ for a graph, ‘outward’ for a closed surface such as a sphere, ‘downward’, ‘inward’, or ‘in the direction of ru×rvr_u\times r_v’.

    In one lineA surface together with a continuous choice of unit normal vector nn at every point.

    Why it existsFlux changes sign if the normal is reversed, so a flux problem is meaningless until a normal has been chosen: upward, outward, downward, inward.

    Definition T

    Orientable surface

    A surface is orientable if a continuous unit normal field exists on it. A Moebius strip (a band of paper with one half twist, glued) is not: carry a normal vector once around the band and it comes back reversed, so no continuous choice exists. In the picture at the top of the chapter, choose the Moebius strip and compare NN at u=0u = 0 and u=2πu = 2\pi. A parametrization such as r(u,v)=((1+vcos⁡u2)cos⁡u, (1+vcos⁡u2)sin⁡u, vsin⁡u2)r(u, v) = \big((1 + v\cos\tfrac u2)\cos u,\ (1 + v\cos\tfrac u2)\sin u,\ v\sin\tfrac u2\big), 0≤u≤2π0\le u\le2\pi, −12≤v≤12-\frac12\le v\le\frac12 traces it, and ru×rvr_u\times r_v at u=0u = 0 is the negative of ru×rvr_u\times r_v at u=2πu = 2\pi at the same point.

    In one lineA surface that admits an orientation. Spheres, cylinders, graphs, tori and flat pieces are orientable; the Moebius strip is not.

    Why it existsFlux and Stokes' theorem both need a normal, so they only make sense on orientable surfaces.

    Definition T

    Flux

    The flux of a continuous vector field FF through the oriented surface SS with unit normal nn is

    ∬SF⋅n dS.\iint_S F\cdot n\,dS.

    Only the component of FF along nn crosses the surface, so the integrand F⋅nF\cdot n is the flux density: the rate of crossing per unit area. If FF is the velocity of a fluid, the flux is the volume of fluid crossing the surface per unit time, positive in the direction of nn.

    In one lineThe flux of a vector field FF through an oriented surface SS with unit normal nn is ∬SF⋅n dS\iint_S F\cdot n\,dS.

    Why it existsIt measures how much of the field crosses the surface, counted positive in the direction of nn and negative against it.

    Why the dot product with nn and not something else? Try a flat square of area AA in the plane x=0x = 0, with normal n=(1,0,0)n = (1, 0, 0). If F=(1,0,0)F = (1, 0, 0) the field goes straight through, and in one second a column of fluid of volume 1⋅A1\cdot A crosses. If F=(0,2,0)F = (0, 2, 0) the field slides along the square and nothing crosses. For a constant F=vF = v the volume crossing in one second is the volume of the slanted column on the square with edge vv, which is (v⋅n) A(v\cdot n)\,A.

    Theorem T MATH 376 lectures of 25 and 27 February; Apostol 12.7 and 12.9

    Flux as a double integral

    Let r:T→Sr: T\to S be a smooth parametrization and FF continuous on SS. If N=ru×rvN = r_u\times r_v points in the direction of the required normal nn, then ∬SF⋅n dS=∬TF(r(u,v))⋅N(u,v) du dv\iint_SF\cdot n\,dS = \iint_TF(r(u, v))\cdot N(u, v)\,du\,dv. If NN points the other way, then n=−N/∥N∥n = -N/\lVert N\rVert and the flux is −∬TF(r)⋅N du dv-\iint_TF(r)\cdot N\,du\,dv.

    In one lineIf ru×rvr_u\times r_v points the same way as nn, then ∬SF⋅n dS=∬TF(r(u,v))⋅(ru×rv) du dv\iint_S F\cdot n\,dS = \iint_TF(r(u, v))\cdot(r_u\times r_v)\,du\,dv; if it points the opposite way, the right side has the opposite sign.

    Why it is trueThe length of the normal cancels, so a flux integral never contains a square root. This one identity is the working formula for every flux problem.

    ProofMATH 376 lecture of 27 February
    The idea: The unit normal divides by the length of N and the area element multiplies by the length of N. They cancel.
    ∬SF⋅n dS=∬TF(r)⋅n ∥N∥ du dv\iint_SF\cdot n\,dS = \iint_TF(r)\cdot n\,\lVert N\rVert\,du\,dv.
    Surface integral formula with f=F⋅nf = F\cdot n.
    n ∥N∥=N∥N∥∥N∥=Nn\,\lVert N\rVert = \dfrac{N}{\lVert N\rVert}\lVert N\rVert = N.
    If NN points the way nn does, then n=N/∥N∥n = N/\lVert N\rVert at every point.This is where the direction check matters. For 'upward', look at the sign of the third component of NN. For 'outward' from a sphere or cylinder, test NN against the position vector at one point.
    =∬TF(r)⋅N du dv= \iint_TF(r)\cdot N\,du\,dv.
    Substitute. The normalization has vanished.
    The integral is −∬TF(r)⋅N du dv-\iint_TF(r)\cdot N\,du\,dv. ■\blacksquare
    If instead NN points against nn, then n=−N/∥N∥n = -N/\lVert N\rVert and the same cancellation gives n ∥N∥=−Nn\,\lVert N\rVert = -N.Do not flip the sign by taking an absolute value at the end: a flux can truly be negative.

    The method for flux: (1) parametrize; (2) compute N=ru×rvN = r_u\times r_v; (3) compare its direction with the required orientation, and replace NN by −N-N if they disagree; (4) substitute the surface into FF; (5) dot with NN; (6) integrate over the parameter region. Nothing is normalized.

    Why· Another way to write the same flux: Apostol 12.9

    Apostol writes the flux of F=(P,Q,R)F = (P, Q, R) as ∬SP dy∧dz+Q dz∧dx+R dx∧dy\iint_SP\,dy\wedge dz + Q\,dz\wedge dx + R\,dx\wedge dy. The symbol ∬SP dy∧dz\iint_SP\,dy\wedge dz means ∬TP(r(u,v)) ∂(y,z)∂(u,v) du dv\iint_TP(r(u, v))\,\dfrac{\partial(y, z)}{\partial(u, v)}\,du\,dv, where ∂(y,z)∂(u,v)=yuzv−yvzu\dfrac{\partial(y, z)}{\partial(u, v)} = y_uz_v - y_vz_u is a 2×22\times2 determinant. These three determinants are exactly the three components of ru×rvr_u\times r_v: the first component of NN is yuzv−zuyvy_uz_v - z_uy_v, the second is zuxv−xuzvz_ux_v - x_uz_v and the third is xuyv−yuxvx_uy_v - y_ux_v. So the notation says nothing new. It says that PP is paired with the shadow of the patch on the yzyz-plane, QQ with its shadow on the zxzx-plane and RR with its shadow on the xyxy-plane. 6.7 explains what dy∧dzdy\wedge dz is.

    Why· The picture behind the cancellation: a slanted box

    During a short time Δt\Delta t, the fluid that crosses a small patch is the fluid in a slanted box. The box has sides FΔtF\Delta t (how far the fluid moves), ruΔur_u\Delta u and rvΔvr_v\Delta v (the patch). The volume of a box is the triple product FΔt⋅(ruΔu×rvΔv)F\Delta t\cdot(r_u\Delta u\times r_v\Delta v): base area times height, where the height is the component of FΔtF\Delta t along the normal. Divide by Δt\Delta t and add the boxes: ∬F⋅(ru×rv) du dv\iint F\cdot(r_u\times r_v)\,du\,dv, with no square root anywhere. The length of NN is the base area and the unit normal only extracts the height.

    Worked example MATH 376 Midterm 2 problem 1(b), 4 points; see [A.3](/vol2/a3-midterm-2/)
    Find the flux of F=(x,y,z)F = (x, y, z) through S={(u,v,eu):0≤u,v≤1}S = \{(u, v, e^u) : 0\le u, v\le1\} with the normal pointing in the positive zz direction.

    Solution.

    1. Normal. N=ru×rv=(−eu,0,1)N = r_u\times r_v = (-e^u, 0, 1), with positive third component. From the previous example. It already points the required way.
    2. Substitute. F(r(u,v))=(u,v,eu)F(r(u, v)) = (u, v, e^u). x=ux = u, y=vy = v, z=euz = e^u.
    3. Dot. F⋅N=−ueu+0+eu=(1−u)euF\cdot N = -ue^u + 0 + e^u = (1 - u)e^u. No square root: n dS=N du dvn\,dS = N\,du\,dv.
    4. Set up. ∫01 ⁣∫01(1−u)eu dv du=∫01(1−u)eu du\int_0^1\!\int_0^1(1 - u)e^u\,dv\,du = \int_0^1(1 - u)e^u\,du. The integrand has no vv, so the vv integral over [0,1][0,1] is 11.
    5. Antiderivative. Integration by parts with g=1−ug = 1 - u and dh=eu dudh = e^u\,du gives ∫(1−u)eu du=(1−u)eu+∫eu du=(2−u)eu\int(1 - u)e^u\,du = (1 - u)e^u + \int e^u\,du = (2 - u)e^u. Check by differentiating: ddu(2−u)eu=−eu+(2−u)eu=(1−u)eu\frac d{du}(2 - u)e^u = -e^u + (2 - u)e^u = (1 - u)e^u.
    6. Evaluate. [(2−u)eu]01=1⋅e−2⋅1=e−2\big[(2 - u)e^u\big]_0^1 = 1\cdot e - 2\cdot1 = e - 2.

    Answer. e−2≈0.718e - 2\approx0.718. The practice exam version has S={(u,v,v−u3):(u,v)∈[0,1]×[0,2]}S = \{(u, v, v - u^3) : (u, v)\in[0,1]\times[0,2]\} and F=(x,2y,z)F = (x, 2y, z). There N=(3u2,−1,1)N = (3u^2, -1, 1) (positive third component again), F(r)⋅N=3u3−2v+v−u3=2u3−vF(r)\cdot N = 3u^3 - 2v + v - u^3 = 2u^3 - v, and ∫01 ⁣∫02(2u3−v) dv du=∫01(4u3−2) du=1−2=−1\int_0^1\!\int_0^2(2u^3 - v)\,dv\,du = \int_0^1(4u^3 - 2)\,du = 1 - 2 = -1.

    Worked example MATH 376 lecture of 25 February, Example 5.5
    Find the flux of F=(x,0,2z)F = (x, 0, 2z) through the paraboloid patch S={(u,v,u2+v2):(u,v)∈[0,1]2}S = \{(u, v, u^2 + v^2) : (u, v)\in[0, 1]^2\} with the orientation of ru×rvr_u\times r_v.

    Solution.

    1. Tangent vectors and cross. ru=(1,0,2u)r_u = (1, 0, 2u), rv=(0,1,2v)r_v = (0, 1, 2v), N=(−2u,−2v,1)N = (-2u, -2v, 1). Graph formula with g=u2+v2g = u^2 + v^2.
    2. Substitute and dot. F(r)=(u,0,2(u2+v2))F(r) = (u, 0, 2(u^2 + v^2)) and F⋅N=−2u2+0+2u2+2v2=2v2F\cdot N = -2u^2 + 0 + 2u^2 + 2v^2 = 2v^2. The u2u^2 terms cancel.
    3. Integrate. ∫01 ⁣∫012v2 du dv=∫012v2 dv=23\int_0^1\!\int_0^12v^2\,du\,dv = \int_0^12v^2\,dv = \frac23.

    Answer. 23\dfrac23.

    Worked example MATH 376 worksheet 11 problem 6; worksheet 12 problem 5 is the field $(0, 0, z)$
    Find the upward flux of F=(y,−x,z)F = (y, -x, z) through the cap z=4−x2−y2z = 4 - x^2 - y^2, z≥0z\ge0, using polar coordinates.

    Solution.

    1. Parametrize. r(r,θ)=(rcos⁡θ, rsin⁡θ, 4−r2)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ 4 - r^2), 0≤r≤20\le r\le2, 0≤θ≤2π0\le\theta\le2\pi.
    2. Cross. N=rr×rθ=(2r2cos⁡θ, 2r2sin⁡θ, r)N = r_r\times r_\theta = (2r^2\cos\theta,\ 2r^2\sin\theta,\ r). The same computation as in the area example: the constant in zz disappears on differentiating. The third component r≥0r\ge0, so it points up.
    3. Substitute. F(r)=(rsin⁡θ, −rcos⁡θ, 4−r2)F(r) = (r\sin\theta,\ -r\cos\theta,\ 4 - r^2).
    4. Dot. F⋅N=2r3sin⁡θcos⁡θ−2r3cos⁡θsin⁡θ+(4−r2)r=4r−r3F\cdot N = 2r^3\sin\theta\cos\theta - 2r^3\cos\theta\sin\theta + (4 - r^2)r = 4r - r^3. The field (y,−x,0)(y, -x, 0) circles the axis and is tangent to every horizontal circle, so it contributes nothing.
    5. Integrate. ∫02π ⁣∫02(4r−r3) dr dθ=2π[2r2−r44]02=2π(8−4)=8π\int_0^{2\pi}\!\int_0^2(4r - r^3)\,dr\,d\theta = 2\pi\big[2r^2 - \tfrac{r^4}4\big]_0^2 = 2\pi(8 - 4) = 8\pi.

    Answer. 8π8\pi. For F=(0,0,z)F = (0, 0, z) the graph shortcut n dS=(2x,2y,1) dAn\,dS = (2x, 2y, 1)\,dA gives the integrand 4−x2−y24 - x^2 - y^2 and the same 8π8\pi.

    Worked example MATH 376 worksheet 12 problems 6 and 7
    Find the outward flux of F=(x,y,0)F = (x, y, 0) through the lateral surface of the cylinder x2+y2=1x^2 + y^2 = 1, 0≤z≤20\le z\le2, and the outward flux of F=(x,y,z)F = (x, y, z) through the upper unit hemisphere by a shortcut.

    Solution.

    1. Cylinder. r(θ,z)=(cos⁡θ, sin⁡θ, z)r(\theta, z) = (\cos\theta,\ \sin\theta,\ z) gives N=rθ×rz=(cos⁡θ, sin⁡θ, 0)N = r_\theta\times r_z = (\cos\theta,\ \sin\theta,\ 0), which points away from the axis: outward. Test at θ=0\theta = 0: the point is (1,0,z)(1, 0, z) and N=(1,0,0)N = (1, 0, 0).
    2. Cylinder, dot. F(r)=(cos⁡θ,sin⁡θ,0)F(r) = (\cos\theta, \sin\theta, 0), so F⋅N=cos⁡2θ+sin⁡2θ=1F\cdot N = \cos^2\theta + \sin^2\theta = 1, and the flux is ∫02π ⁣∫021 dz dθ=4π\int_0^{2\pi}\!\int_0^21\,dz\,d\theta = 4\pi.
    3. Hemisphere, shortcut. On the unit sphere the outward unit normal at (x,y,z)(x, y, z) is (x,y,z)(x, y, z) itself, so F⋅n=x2+y2+z2=1F\cdot n = x^2 + y^2 + z^2 = 1, constant. If F⋅nF\cdot n is constant cc on SS, the flux is c⋅area⁡(S)c\cdot\operatorname{area}(S).
    4. Area. Half of 4π4\pi, so the flux is 1⋅2π=2π1\cdot2\pi = 2\pi.

    Answer. 4π4\pi (check: F⋅n=1F\cdot n = 1 times the area 2π⋅1⋅2=4π2\pi\cdot1\cdot2 = 4\pi) and 2π2\pi. Two more shortcuts in the same worksheets: on a flat horizontal piece with n=(0,0,1)n = (0, 0, 1) only the third component of FF matters, since the first two are tangent to the piece. So the flux of (0,0,5)(0, 0, 5) upward through the disc x2+y2≤16x^2 + y^2\le16 in z=2z = 2 is 5⋅16π=80π5\cdot16\pi = 80\pi, and that of (x,y,5)(x, y, 5) through x2+y2≤4x^2 + y^2\le4 in z=3z = 3 is 5⋅4π=20π5\cdot4\pi = 20\pi.

    Worked example MATH 376 worksheet 11 problem 7; worksheet 13 problem 6 is $F = (x, y, 0)$, $0\le z\le4$, oriented upward and inward
    Find the flux of F=(0,0,z2)F = (0, 0, z^2) through the cone z=x2+y2z = \sqrt{x^2 + y^2}, 1≤z≤21\le z\le2, oriented downward.

    Solution.

    1. Parametrize. r(r,θ)=(rcos⁡θ, rsin⁡θ, r)r(r, \theta) = (r\cos\theta,\ r\sin\theta,\ r) with 1≤r≤21\le r\le2. On the cone z=rz = r.
    2. Cross. rr×rθ=(−rcos⁡θ, −rsin⁡θ, r)r_r\times r_\theta = (-r\cos\theta,\ -r\sin\theta,\ r). Its third component is r>0r>0: it points up (and in). The problem wants downward: the wrong way.
    3. Flip. Use N=−rr×rθ=(rcos⁡θ, rsin⁡θ, −r)N = -r_r\times r_\theta = (r\cos\theta,\ r\sin\theta,\ -r). By the theorem, the flux is the integral with −N-N.
    4. Dot. F⋅N=z2⋅(−r)=r2(−r)=−r3F\cdot N = z^2\cdot(-r) = r^2(-r) = -r^3. z=rz = r on the cone.
    5. Integrate. ∫02π ⁣∫12−r3 dr dθ=2π[−r44]12=2π(−4+14)=−15π2\int_0^{2\pi}\!\int_1^2-r^3\,dr\,d\theta = 2\pi\big[-\tfrac{r^4}4\big]_1^2 = 2\pi\big(-4 + \tfrac14\big) = -\dfrac{15\pi}2.

    Answer. −15π2-\frac{15\pi}2. It is negative because the field points up and the surface is oriented down. For the worksheet 13 version the vector rr×rθr_r\times r_\theta already points up and inward, so there is no flip: F⋅N=(rcos⁡θ)(−rcos⁡θ)+(rsin⁡θ)(−rsin⁡θ)=−r2F\cdot N = (r\cos\theta)(-r\cos\theta) + (r\sin\theta)(-r\sin\theta) = -r^2, and the flux is 2π[−r33]04=−128π32\pi\big[-\frac{r^3}3\big]_0^4 = -\frac{128\pi}3.

    Worked example MATH 376 homework 5 problem 1
    Parametrize the ellipsoid x2a2+y2b2+z2c2=1\frac{x^2}{a^2} + \frac{y^2}{b^2} + \frac{z^2}{c^2} = 1, find its normal field, and decide whether it points in or out.

    Solution.

    1. Parametrize. r(u,v)=(asin⁡vcos⁡u, bsin⁡vsin⁡u, ccos⁡v)r(u, v) = (a\sin v\cos u,\ b\sin v\sin u,\ c\cos v), 0≤u≤2π0\le u\le2\pi, 0≤v≤π0\le v\le\pi. The sphere parametrization with each coordinate stretched. It satisfies the equation: sin⁡2v(cos⁡2u+sin⁡2u)+cos⁡2v=1\sin^2v(\cos^2u + \sin^2u) + \cos^2v = 1.
    2. Tangent vectors. ru=(−asin⁡vsin⁡u, bsin⁡vcos⁡u, 0)r_u = (-a\sin v\sin u,\ b\sin v\cos u,\ 0) and rv=(acos⁡vcos⁡u, bcos⁡vsin⁡u, −csin⁡v)r_v = (a\cos v\cos u,\ b\cos v\sin u,\ -c\sin v).
    3. Cross. N=(−bcsin⁡2vcos⁡u, −acsin⁡2vsin⁡u, −absin⁡vcos⁡v)N = (-bc\sin^2v\cos u,\ -ac\sin^2v\sin u,\ -ab\sin v\cos v).
    4. Test the direction. At u=0u = 0, v=π/2v = \pi/2 the point is (a,0,0)(a, 0, 0) and N=(−bc,0,0)N = (-bc, 0, 0), which points toward the origin. One test point is enough for a continuous normal that never vanishes inside the region.

    Answer. The normal ru×rvr_u\times r_v points inward. For a flux problem that says ‘outward’, use −N=(bcsin⁡2vcos⁡u, acsin⁡2vsin⁡u, absin⁡vcos⁡v)-N = (bc\sin^2v\cos u,\ ac\sin^2v\sin u,\ ab\sin v\cos v).

    Worked example MATH 376 practice final problem 2; see [A.5](/vol2/a5-practice-exams/)
    Find the upward flux of f=(y,x,1)f = (y, x, 1) through S={(x,y,x2−y2):x,y∈[0,1]}S = \{(x, y, x^2 - y^2) : x, y\in[0, 1]\}.

    Solution.

    1. Cross. rx=(1,0,2x)r_x = (1, 0, 2x), ry=(0,1,−2y)r_y = (0, 1, -2y), so N=(−2x, 2y, 1)N = (-2x,\ 2y,\ 1). Graph formula: −gx=−2x-g_x = -2x, −gy=2y-g_y = 2y.
    2. Direction. The third component is 1>01>0: upward, as required.
    3. Dot. f(r)⋅N=y(−2x)+x(2y)+1=1f(r)\cdot N = y(-2x) + x(2y) + 1 = 1. ff does not depend on zz. The xyxy terms cancel.
    4. Integrate. ∫01 ⁣∫011 dy dx=1\int_0^1\!\int_0^1 1\,dy\,dx = 1.

    Answer. 11.

    Your answerFind the outward flux of F=(x,y,z)F = (x, y, z) through the lateral surface of the cylinder x2+y2=4x^2 + y^2 = 4, 0≤z≤30\le z\le3.
    Quick checkYou parametrize a surface and ru×rvr_u\times r_v points downward at a point, but the problem asks for the upward flux. What do you do?
    Quick checkIn a flux integral through a surface parametrized by r(u,v)r(u, v), what happens to ∥ru×rv∥\lVert r_u\times r_v\rVert?
    Quick checkThe Moebius strip is not orientable. Which statement about it is correct?

    The integral does not depend on the parametrization

    The same surface has many parametrizations. The answer must not depend on the one you picked, or the computation would not measure the surface.

    Proposition T MATH 376 lecture of 27 February, Proposition 5.11 and Lemma 5.12; Apostol 12.8

    Surface integrals do not depend on the parametrization

    Let r:T→Sr: T\to S be smooth and g=(u,v):τ→Tg = (u, v): \tau\to T a one-to-one continuously differentiable map with det⁡Jg≠0\det Jg\neq0, so that ρ=r∘g\rho = r\circ g is another parametrization of SS with parameters (s,t)(s, t). Here JgJg is the Jacobian matrix with entries us,ut,vs,vtu_s, u_t, v_s, v_t (5.3).

    In one lineIf ρ=r∘g\rho = r\circ g with gg one-to-one and continuously differentiable, then ρs×ρt=(det⁡Jg) (ru×rv)∘g\rho_s\times\rho_t = (\det Jg)\,(r_u\times r_v)\circ g; so a scalar surface integral is the same for rr and ρ\rho, and the flux is the same if det⁡Jg>0\det Jg>0 and changes sign if det⁡Jg<0\det Jg<0.

    Why it is trueIt justifies computing a surface integral with whichever parametrization is easiest, and it shows that orientation is the one thing that depends on the choice.

    ProofMATH 376 lecture of 27 February
    The idea: The chain rule says each new tangent vector is a combination of the old ones. Crossing two such combinations leaves exactly the determinant of the combination coefficients times the old cross product. Then the change of variables formula (6.4) absorbs the determinant into the area element.
    ρs=us ru+vs rv\rho_s = u_s\,r_u + v_s\,r_v and ρt=ut ru+vt rv\rho_t = u_t\,r_u + v_t\,r_v.
    Chain rule for ρ(s,t)=r(u(s,t),v(s,t))\rho(s, t) = r(u(s, t), v(s, t)); ru,rvr_u, r_v are evaluated at g(s,t)g(s, t).
    ρs×ρt=usut ru×ru+usvt ru×rv+vsut rv×ru+vsvt rv×rv\rho_s\times\rho_t = u_su_t\,r_u\times r_u + u_sv_t\,r_u\times r_v + v_su_t\,r_v\times r_u + v_sv_t\,r_v\times r_v.
    Cross product is linear in each slot, so multiply out the four terms.
    ρs×ρt=(usvt−vsut) ru×rv\rho_s\times\rho_t = (u_sv_t - v_su_t)\,r_u\times r_v.
    A vector crossed with itself is 00 (zero area), and rv×ru=−ru×rvr_v\times r_u = -r_u\times r_v (anti-symmetry).The lecture notes print a slip on this line; the factor is usvt−vsutu_sv_t - v_su_t, which is what the four-term expansion gives.
    usvt−vsut=det⁡Jgu_sv_t - v_su_t = \det Jg, so ρs×ρt=(det⁡Jg) (ru×rv)∘g\rho_s\times\rho_t = (\det Jg)\,(r_u\times r_v)\circ g.
    Definition of the determinant of the Jacobian matrix of gg.
    ∥ρs×ρt∥=∣det⁡Jg∣ ∥(ru×rv)∘g∥\lVert\rho_s\times\rho_t\rVert = \lvert\det Jg\rvert\,\lVert(r_u\times r_v)\circ g\rVert.
    Take lengths. The absolute value appears because a length is not negative.
    ∬Tf(r)∥ru×rv∥ du dv=∬τf(ρ) ∣det⁡Jg∣ ∥(ru×rv)∘g∥ ds dt=∬τf(ρ)∥ρs×ρt∥ ds dt\displaystyle\iint_Tf(r)\lVert r_u\times r_v\rVert\,du\,dv = \iint_\tau f(\rho)\,\lvert\det Jg\rvert\,\lVert(r_u\times r_v)\circ g\rVert\,ds\,dt = \iint_\tau f(\rho)\lVert\rho_s\times\rho_t\rVert\,ds\,dt.
    Change of variables (6.4) for the continuous function f(r(u,v))∥ru×rv∥f(r(u,v))\lVert r_u \times r_v\rVert and the map gg, with the factor ∣det⁡Jg∣\lvert\det Jg\rvert.
    The scalar integrals are equal, and the flux integrals are equal or opposite according to the sign of det⁡Jg\det Jg. ■\blacksquare
    For flux, the same chain gives ρs×ρt\rho_s\times\rho_t equal to det⁡Jg\det Jg times the old vector. If det⁡Jg>0\det Jg>0 it points the same way and the flux is unchanged; if det⁡Jg<0\det Jg<0 it points the opposite way and the flux changes sign.So a surface integral depends on the surface and on the orientation, not on the parametrization. Swapping the names of uu and vv has det⁡Jg=−1\det Jg = -1 and reverses the orientation.
    Proof workshopGive the reason for each line: the new normal is the Jacobian determinant times the old oneMATH 376 lecture of 27 February

    Each line of the proof is shown in order. Choose the reason that justifies it, then press Check.

    1. ρs=us ru+vs rv\rho_s = u_s\,r_u + v_s\,r_v and ρt=ut ru+vt rv\rho_t = u_t\,r_u + v_t\,r_v.
    2. ρs×ρt=usut ru×ru+usvt ru×rv+vsut rv×ru+vsvt rv×rv\rho_s\times\rho_t = u_su_t\,r_u\times r_u + u_sv_t\,r_u\times r_v + v_su_t\,r_v\times r_u + v_sv_t\,r_v\times r_v.
    3. ru×ru=0r_u\times r_u = 0 and rv×rv=0r_v\times r_v = 0.
    4. rv×ru=− ru×rvr_v\times r_u = -\,r_u\times r_v.
    5. ρs×ρt=(usvt−vsut) ru×rv\rho_s\times\rho_t = (u_sv_t - v_su_t)\,r_u\times r_v.
    6. usvt−vsut=det⁡Jgu_sv_t - v_su_t = \det Jg.

    Where it is used

    Used inside maths· Inside maths: Archimedes, mean curvature and the divergence theorem

    The area of the sphere 4πR24\pi R^2 is on the one hand a computation with rφ×rθr_\varphi\times r_\theta, and on the other the number Archimedes found by comparing a sphere with the cylinder around it: the zone between two parallel planes has the same area as the corresponding band of the cylinder, 2πRh2\pi Rh. The word ‘area’ also leads to curvature: the cross product’s length squared is EG−F2EG - F^2, with E=ru⋅ruE = r_u\cdot r_u, F=ru⋅rvF = r_u\cdot r_v, G=rv⋅rvG = r_v\cdot r_v, the first fundamental form of the surface, which is where differential geometry begins. And flux is the left side of the divergence theorem in 6.6, where the whole surface integral for a closed surface becomes a volume integral. The flux of F=(x,y,z)F = (x, y, z) out of a torus of radii RR and aa is 6π2Ra26\pi^2Ra^2 (dot FF with the outward normal a(R+acos⁡v)(cos⁡ucos⁡v,sin⁡ucos⁡v,sin⁡v)a(R + a\cos v)(\cos u\cos v, \sin u\cos v, \sin v) found above and integrate), exactly three times its volume 2π2Ra22\pi^2Ra^2. Why a factor of exactly 33 is the subject of 6.6.

    Used in the real world· Used in the real world: a solar panel and a mesh

    Sunlight delivers about 10001000 W per square metre on a surface facing the sun; the field is F=1000 dF = 1000\,d, with dd the unit vector along the rays, and the power on a panel is the flux through it. A flat roof panel of 1.71.7 m2^2 with upward unit normal n=(0,0,1)n = (0, 0, 1) sees the sun 30∘30^\circ from the vertical, so the rays travel along d=(−12,0,−32)d = (-\tfrac12, 0, -\tfrac{\sqrt3}2), and the power on the panel is ∣F⋅n∣⋅area=1000⋅32⋅1.7≈1472\lvert F\cdot n\rvert\cdot\text{area} = 1000\cdot\tfrac{\sqrt3}2\cdot1.7\approx1472 W, about 87%87\% of the full 17001700 W: the tilt costs cos⁡30∘\cos30^\circ. Tilting the panel to face the sun turns the dot product into 10001000 and the power into 17001700 W.

    A 3D model in a game engine or a 3D printer file is a list of flat triangles. The software finds the area of each triangle as half the length of the cross product of two edges, exactly as in the worked example, and adds: a 10 cm cube stored as 1212 triangles has area 12⋅12⋅100=60012\cdot\frac12\cdot100 = 600 cm2^2, which is what determines the amount of paint or resin for the skin. The unit normal of each triangle, the cross product divided by its length, is what the shading uses: the brightness of a pixel on a triangle is proportional to the dot product of that normal with the direction to the light. A hemispherical dome of radius 1212 m has roof area 2π⋅122≈904.82\pi\cdot12^2\approx904.8 m2^2, the number that matters for the cost of the roofing.

    Your answerA flat solar panel of 1.71.7 m2^2 lies on a horizontal roof. Sunlight of intensity 10001000 W/m2^2 arrives along the direction (−12,0,−32)(-\frac12, 0, -\frac{\sqrt3}2). How many watts reach the panel?

    Traps

    Watch out· Midterm 2 problem 1(b) lost two of four points: three mistakes in one flux integral

    On the 376 midterm, a student wrote dS=du dvdS = du\,dv but kept the unit normal n=N/e2u+1n = N/\sqrt{e^{2u} + 1} in the integrand, so the stray square root stayed. The real area element is dS=e2u+1 du dvdS = \sqrt{e^{2u} + 1}\,du\,dv, and it cancels the denominator of nn. They then pulled the factor 1/e2u+11/\sqrt{e^{2u} + 1} out of the integral over uu, which is never allowed for a factor that depends on uu. A sign that something went wrong is that their boxed answer still contained the variable uu: a definite integral over the whole surface is a number. And they integrated ueuue^u as u22eu−eu\frac{u^2}2e^u - e^u, which is not integration by parts; the antiderivative is ueu−euue^u - e^u. Differentiate every antiderivative before they use it. The rubric item applied was ‘correct except for a major computational mistake’. The full solution is in A.3 and A.1.

    Watch out· Compare the sign of the cross product with the orientation, every time

    The formula ∬F⋅n dS=∬F⋅(ru×rv) du dv\iint F\cdot n\,dS = \iint F\cdot(r_u\times r_v)\,du\,dv holds only when ru×rvr_u\times r_v points the way nn does. Test it at one point: the sign of the third component for upward or downward, the direction relative to the axis or the centre for outward or inward. The cone (rcos⁡θ,rsin⁡θ,r)(r\cos\theta, r\sin\theta, r) gives a vector pointing up and inward, and the ellipsoid parametrization gives a vector pointing inward. Both are traps in the worksheets.

    Watch out· Do not normalize, and do not drop the length, whichever integral it is

    Scalar integral: f ∥N∥ du dvf\,\lVert N\rVert\,du\,dv, with the length. Flux: F⋅N du dvF\cdot N\,du\,dv, with no length and no unit vector. Writing the unit normal and also the length (the other way round from the exam mistake) gives the right answer but is slow and invites arithmetic slips with the square root.

    Watch out· Let the problem's constraints set the parameter limits

    For the paraboloid cap above the plane z=0z = 0 the limit is r≤3/2r\le\sqrt3/2, from z≥0z\ge0, not r≤1r\le1 or r≤3/4r\le3/4. For the cone between z=0z = 0 and z=21/4z = 2^{1/4} the limit is on rr, not on θ\theta. Write the constraint as an inequality before you integrate. A dropped absolute value is the same kind of slip in a different place: the set max⁡(∣x∣,∣y∣,∣z∣)=1\max(\lvert x\rvert, \lvert y\rvert, \lvert z\rvert) = 1 is the surface of the cube [−1,1]3[-1, 1]^3, not of a cube in one octant. 6.6 returns to it.

    Watch out· Cone apex, sphere poles

    At the apex of the cone and at the poles of the sphere (φ=0,π\varphi = 0, \pi) the vector NN is 00 and the parametrization is not regular. These are points or curves that do not carry area, so they change no integral. What you must not do is divide by ∥N∥\lVert N\rVert there.

    Problems

    checknew (MATH 376 worksheet 12 style)

    Compute (1,2,−1)×(3,0,2)(1, 2, -1)\times(3, 0, 2) and verify that it is orthogonal to both vectors.

    Solution

    Components: 2⋅2−(−1)⋅0=42\cdot2 - (-1)\cdot0 = 4; (−1)⋅3−1⋅2=−5(-1)\cdot3 - 1\cdot2 = -5; 1⋅0−2⋅3=−61\cdot0 - 2\cdot3 = -6. So the cross product is (4,−5,−6)(4, -5, -6). Check: (4,−5,−6)⋅(1,2,−1)=4−10+6=0(4, -5, -6)\cdot(1, 2, -1) = 4 - 10 + 6 = 0 and (4,−5,−6)⋅(3,0,2)=12+0−12=0(4, -5, -6)\cdot(3, 0, 2) = 12 + 0 - 12 = 0.

    checknew (MATH 376 worksheet 11 problem 5 style)

    Find ru×rvr_u\times r_v for r(u,v)=(u+v, u−v, uv)r(u, v) = (u + v,\ u - v,\ uv) at (u,v)=(1,1)(u, v) = (1, 1).

    Solution

    ru=(1,1,v)=(1,1,1)r_u = (1, 1, v) = (1, 1, 1) and rv=(1,−1,u)=(1,−1,1)r_v = (1, -1, u) = (1, -1, 1) at the point. ru×rv=(1⋅1−1⋅(−1), 1⋅1−1⋅1, 1⋅(−1)−1⋅1)=(2,0,−2)r_u\times r_v = (1\cdot1 - 1\cdot(-1),\ 1\cdot1 - 1\cdot1,\ 1\cdot(-1) - 1\cdot1) = (2, 0, -2). Check: dotted with rur_u gives 2−2=02 - 2 = 0, with rvr_v gives 2−2=02 - 2 = 0.

    checknew (Midterm 2 problem 1(b) mistake)

    A cylinder of radius 44 and height 55 is parametrized on [0,2π]×[0,5][0, 2\pi]\times[0, 5]. What is the area of the parameter rectangle, and what is the area of the cylinder? What is ∥rθ×rz∥\lVert r_\theta\times r_z\rVert?

    Solution

    The rectangle has area 10π10\pi. r=(4cos⁡θ,4sin⁡θ,z)r = (4\cos\theta, 4\sin\theta, z) has rθ×rz=(4cos⁡θ,4sin⁡θ,0)r_\theta\times r_z = (4\cos\theta, 4\sin\theta, 0), of length 44. So the cylinder has area 4⋅10π=40π4\cdot10\pi = 40\pi, which is 2π⋅4⋅52\pi\cdot4\cdot5, circumference times height.

    check

    True or false: if you reparametrize a surface by swapping the roles of uu and vv, the flux of FF through it stays the same.

    Solution

    It depends on what is held fixed. Swapping uu and vv replaces ru×rvr_u\times r_v by rv×ru=−ru×rvr_v\times r_u = -r_u\times r_v, so if you keep using ∬F⋅(ru×rv) du dv\iint F\cdot(r_u\times r_v)\,du\,dv without comparing the direction with the required orientation, the sign of the answer flips: false. If you do compare, and use −N-N when NN points the wrong way, the flux through the oriented surface does not depend on the parametrization: true. What changes is which of ±N\pm N equals nn.

    usenew (MATH 376 worksheet 12 problem 3 style)

    Find the area of the part of the plane x+2y+3z=6x + 2y + 3z = 6 in the first octant.

    Solution

    The plane meets the axes at A=(6,0,0)A = (6, 0, 0), B=(0,3,0)B = (0, 3, 0), C=(0,0,2)C = (0, 0, 2). AB→=(−6,3,0)\overrightarrow{AB} = (-6, 3, 0) and AC→=(−6,0,2)\overrightarrow{AC} = (-6, 0, 2), so AB→×AC→=(3⋅2−0, 0⋅(−6)−(−6)⋅2, (−6)⋅0−3⋅(−6))=(6,12,18)\overrightarrow{AB}\times\overrightarrow{AC} = (3\cdot2 - 0,\ 0\cdot(-6) - (-6)\cdot2,\ (-6)\cdot0 - 3\cdot(-6)) = (6, 12, 18), of length 6146\sqrt{14}. The area is 314≈11.223\sqrt{14}\approx11.22. Check by the graph formula: z=(6−x−2y)/3z = (6 - x - 2y)/3, ∥N∥=1+19+49=143\lVert N\rVert = \sqrt{1 + \frac19 + \frac49} = \frac{\sqrt{14}}3, and the region DD under it has area 12⋅6⋅3=9\frac12\cdot6\cdot3 = 9, giving 3143\sqrt{14}.

    usenew (symmetry, compare MATH 376 homework 5 problem 2)

    Compute ∬Sx2 dS\iint_Sx^2\,dS over the unit sphere.

    Solution

    By symmetry (swapping coordinate names maps the sphere to itself), ∬x2 dS=∬y2 dS=∬z2 dS\iint x^2\,dS = \iint y^2\,dS = \iint z^2\,dS. Their sum is ∬(x2+y2+z2) dS=∬1 dS=4π\iint(x^2 + y^2 + z^2)\,dS = \iint1\,dS = 4\pi. So each is 4π3\frac{4\pi}3.

    usenew (compare MATH 376 worksheet 12 problem 7)

    Find the outward flux of the constant field F=(1,2,3)F = (1, 2, 3) through the upper hemisphere of radius 22.

    Solution

    Use r(φ,θ)=2(sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)r(\varphi, \theta) = 2(\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi), 0≤φ≤π/20\le\varphi\le\pi/2. N=rφ×rθ=4sin⁡φ (sin⁡φcos⁡θ, sin⁡φsin⁡θ, cos⁡φ)N = r_\varphi\times r_\theta = 4\sin\varphi\,(\sin\varphi\cos\theta,\ \sin\varphi\sin\theta,\ \cos\varphi), which points outward. F⋅N=4sin⁡φ (sin⁡φcos⁡θ+2sin⁡φsin⁡θ+3cos⁡φ)F\cdot N = 4\sin\varphi\,(\sin\varphi\cos\theta + 2\sin\varphi\sin\theta + 3\cos\varphi). The θ\theta integral of the first two terms over [0,2π][0, 2\pi] is 00. What is left is 12sin⁡φcos⁡φ12\sin\varphi\cos\varphi, and 2π∫0π/212sin⁡φcos⁡φ dφ=2π⋅6=12π2\pi\int_0^{\pi/2}12\sin\varphi\cos\varphi\,d\varphi = 2\pi\cdot6 = 12\pi. This is 3⋅π⋅223\cdot\pi\cdot2^2, the third component times the area of the disc under the hemisphere, as it must be: only the vertical part of a constant field sees the shadow.

    useMATH 376 homework 5 problem 3

    Find the outward flux of F=(x2,y2,z2)F = (x^2, y^2, z^2) through the cylinder x2+y2=1x^2 + y^2 = 1, −1≤z≤1-1\le z\le1 (lateral surface only).

    Solution

    r=(cos⁡θ,sin⁡θ,z)r = (\cos\theta, \sin\theta, z), N=(cos⁡θ,sin⁡θ,0)N = (\cos\theta, \sin\theta, 0) (outward). F⋅N=cos⁡3θ+sin⁡3θF\cdot N = \cos^3\theta + \sin^3\theta, with no zz and no third-component term. ∫−11∫02π(cos⁡3θ+sin⁡3θ) dθ dz=2(∫02π(1−sin⁡2θ)cos⁡θ dθ+∫02π(1−cos⁡2θ)sin⁡θ dθ)\int_{-1}^1\int_0^{2\pi}(\cos^3\theta + \sin^3\theta)\,d\theta\,dz = 2\big(\int_0^{2\pi}(1 - \sin^2\theta)\cos\theta\,d\theta + \int_0^{2\pi}(1 - \cos^2\theta)\sin\theta\,d\theta\big). The first is [sin⁡θ−sin⁡3θ3]02π=0\big[\sin\theta - \frac{\sin^3\theta}3\big]_0^{2\pi} = 0 and the second is [−cos⁡θ+cos⁡3θ3]02π=0\big[-\cos\theta + \frac{\cos^3\theta}3\big]_0^{2\pi} = 0. The flux is 00.

    useMATH 376 worksheet 12 problem 4

    Find the upward flux of F=(x,2y,z)F = (x, 2y, z) through the part of the plane z=4−x−2yz = 4 - x - 2y over 0≤x≤20\le x\le2, 0≤y≤10\le y\le1.

    Solution

    r(x,y)=(x,y,4−x−2y)r(x, y) = (x, y, 4 - x - 2y), N=(−gx,−gy,1)=(1,2,1)N = (-g_x, -g_y, 1) = (1, 2, 1), third component +1+1 so upward as required. F(r)=(x,2y,4−x−2y)F(r) = (x, 2y, 4 - x - 2y), so F⋅N=x+4y+4−x−2y=4+2yF\cdot N = x + 4y + 4 - x - 2y = 4 + 2y. The xx terms cancel. ∫01 ⁣∫02(4+2y) dx dy=∫01(8+4y) dy=8+2=10\int_0^1\!\int_0^2(4 + 2y)\,dx\,dy = \int_0^1(8 + 4y)\,dy = 8 + 2 = 10.

    useMATH 376 worksheet 27 problem 9

    Find the upward flux of F=(x,y,z)F = (x, y, z) through z=4−x2−y2z = 4 - x^2 - y^2 over the disc x2+y2≤1x^2 + y^2\le1.

    Solution

    N=(2x,2y,1)N = (2x, 2y, 1) (upward), F⋅N=2x2+2y2+(4−x2−y2)=4+x2+y2F\cdot N = 2x^2 + 2y^2 + (4 - x^2 - y^2) = 4 + x^2 + y^2. In polar coordinates ∫02π ⁣∫01(4+r2) r dr dθ=2π[2r2+r44]01=2π⋅94=9π2\int_0^{2\pi}\!\int_0^1(4 + r^2)\,r\,dr\,d\theta = 2\pi\big[2r^2 + \tfrac{r^4}4\big]_0^1 = 2\pi\cdot\tfrac94 = \tfrac{9\pi}2. Compare the cap over r≤2r\le2, where the same field gives 24π24\pi in the picture at the top of the chapter.

    useMATH 376 worksheet 14 problem 3

    The field B=(−y,x,0)x2+y2B = \dfrac{(-y, x, 0)}{x^2 + y^2} is defined away from the zz-axis. Find its upward flux through the part of the plane z=y+5z = y + 5 inside the cylinder x2+y2=1x^2 + y^2 = 1.

    Solution

    Graph of g=y+5g = y + 5 over the unit disc, so N=(−gx,−gy,1)=(0,−1,1)N = (-g_x, -g_y, 1) = (0, -1, 1), upward. B⋅N=−xx2+y2B\cdot N = \dfrac{-x}{x^2 + y^2}. In polar coordinates ∫02π ⁣∫01−rcos⁡θr2 r dr dθ=∫02π ⁣∫01(−cos⁡θ) dr dθ=∫02π(−cos⁡θ) dθ=0\int_0^{2\pi}\!\int_0^1\dfrac{-r\cos\theta}{r^2}\,r\,dr\,d\theta = \int_0^{2\pi}\!\int_0^1(-\cos\theta)\,dr\,d\theta = \int_0^{2\pi}(-\cos\theta)\,d\theta = 0. The rr from the area element cancels one power of r2r^2. The plane passes through the zz-axis at (0,0,5)(0, 0, 5), where BB is not defined. The integrand times rr is bounded, so the integral exists, but the field is undefined at that one point.

    useMATH 376 worksheet 14 problem 4

    A bowl is the part of the sphere x2+y2+z2=4x^2 + y^2 + z^2 = 4 with z≤0z\le0. Fluid of pressure 10−z10 - z pushes on it. Find the vertical force Fz=∬S(10−z)(−nz) dSF_z = \iint_S(10 - z)(-n_z)\,dS, where nn is the outward normal.

    Solution

    On the sphere of radius 22, n=(x,y,z)/2n = (x, y, z)/2, so nz=z/2=cos⁡φn_z = z/2 = \cos\varphi, and z=2cos⁡φz = 2\cos\varphi. By the sphere computation, dS=4sin⁡φ dφ dθdS = 4\sin\varphi\,d\varphi\,d\theta. The lower half is π/2≤φ≤π\pi/2\le\varphi\le\pi. The integrand is (10−2cos⁡φ)(−cos⁡φ)=−10cos⁡φ+2cos⁡2φ(10 - 2\cos\varphi)(-\cos\varphi) = -10\cos\varphi + 2\cos^2\varphi. So Fz=∫02π∫π/2π(−10cos⁡φ+2cos⁡2φ) 4sin⁡φ dφ dθF_z = \int_0^{2\pi}\int_{\pi/2}^{\pi}(-10\cos\varphi + 2\cos^2\varphi)\,4\sin\varphi\,d\varphi\,d\theta. Put c=cos⁡φc = \cos\varphi, dc=−sin⁡φ dφdc = -\sin\varphi\,d\varphi, limits c=0c = 0 to −1-1, which reverses to ∫−10(−10c+2c2) dc=[−5c2+23c3]−10=0−(−5−23)=173\int_{-1}^0(-10c + 2c^2)\,dc = \big[-5c^2 + \frac23c^3\big]_{-1}^0 = 0 - (-5 - \frac23) = \frac{17}3. So Fz=2π⋅4⋅173=136π3F_z = 2\pi\cdot4\cdot\frac{17}3 = \frac{136\pi}3. (The course solution as extracted shows 1363\frac{136}3 with the π\pi lost; 136π3\frac{136\pi}3 is correct.)

    provenew (the triple product and flux of a constant field)

    Let a,ba, b be vectors in space and P={ua+vb:0≤u,v≤1}P = \{ua + vb : 0\le u, v\le1\} the parallelogram with normal n=(a×b)/∥a×b∥n = (a\times b)/\lVert a\times b\rVert. Show that the flux of a constant field cc through PP is c⋅(a×b)c\cdot(a\times b).

    Solution

    Parametrize r(u,v)=ua+vbr(u, v) = ua + vb on [0,1]2[0, 1]^2. Then ru=ar_u = a, rv=br_v = b, N=a×bN = a\times b is constant and points the way nn does. By the flux theorem, ∬PF⋅n dS=∬[0,1]2c⋅(a×b) du dv=c⋅(a×b)⋅1\iint_PF\cdot n\,dS = \iint_{[0,1]^2}c\cdot(a\times b)\,du\,dv = c\cdot(a\times b)\cdot1. This is the volume of the parallelepiped on a,b,ca, b, c (up to sign), which is the slanted-column picture.

    provenew (Archimedes' hat-box, Apostol 12.5)

    Prove that the area of the zone of the sphere of radius RR between the planes z=z1z = z_1 and z=z2z = z_2 (with −R≤z1<z2≤R-R\le z_1<z_2\le R) is 2πR(z2−z1)2\pi R(z_2 - z_1).

    Solution

    Use r(φ,θ)r(\varphi, \theta) of radius RR. ∥N∥=R2sin⁡φ\lVert N\rVert = R^2\sin\varphi for 0≤φ≤π0\le\varphi\le\pi, as in the example. The zone is φ1≤φ≤φ2\varphi_1\le\varphi\le\varphi_2 with z=Rcos⁡φz = R\cos\varphi, so φ1<φ2\varphi_1<\varphi_2 correspond to z2>z1z_2>z_1. The area is 2π∫φ1φ2R2sin⁡φ dφ=2πR2(cos⁡φ1−cos⁡φ2)=2πR(z2−z1)2\pi\int_{\varphi_1}^{\varphi_2}R^2\sin\varphi\,d\varphi = 2\pi R^2(\cos\varphi_1 - \cos\varphi_2) = 2\pi R(z_2 - z_1) since Rcos⁡φ1=z2R\cos\varphi_1 = z_2 and Rcos⁡φ2=z1R\cos\varphi_2 = z_1. The area depends only on the thickness.

    provenew (graphs, Apostol 12.5)

    For a graph z=g(x,y)z = g(x, y) over a region DD, prove that area⁡(S)=∬D1+gx2+gy2 dA\operatorname{area}(S) = \iint_D\sqrt{1 + g_x^2 + g_y^2}\,dA, and that if gg is linear, z=px+qy+cz = px + qy + c, then area⁡(S)=1+p2+q2area⁡(D)\operatorname{area}(S) = \sqrt{1 + p^2 + q^2}\operatorname{area}(D).

    Solution

    The graph formula gives N=(−gx,−gy,1)N = (-g_x, -g_y, 1) and ∥N∥=1+gx2+gy2\lVert N\rVert = \sqrt{1 + g_x^2 + g_y^2}, so the definition of area gives the first statement. If g=px+qy+cg = px + qy + c then gx=pg_x = p and gy=qg_y = q are constants, so ∥N∥\lVert N\rVert is a constant that comes out of the integral, leaving area⁡(D)\operatorname{area}(D).

    provenew (orientation reverses under swapping the parameters)

    Show that if ρ(s,t)=r(t,s)\rho(s, t) = r(t, s) (swap the parameters), then ρs×ρt=−(ru×rv)\rho_s\times\rho_t = -(r_u\times r_v) at corresponding points, and conclude that the flux integral changes sign unless one also flips the required normal.

    Solution

    ρs=rv\rho_s = r_v and ρt=ru\rho_t = r_u at the point (t,s)(t, s), so ρs×ρt=rv×ru=−ru×rv\rho_s\times\rho_t = r_v\times r_u = -r_u\times r_v by anti-symmetry. This is also the case g(s,t)=(t,s)g(s, t) = (t, s) with det⁡Jg=−1\det Jg = -1 in the independence theorem. If the problem requires nn and the new ρs×ρt\rho_s\times\rho_t points against it, the flux is −∬F(ρ)⋅(ρs×ρt) ds dt-\iint F(\rho)\cdot(\rho_s\times\rho_t)\,ds\,dt, which equals the flux computed with rr. The two parametrizations give the same oriented flux once each is compared with nn.

    stretchApostol 12.5, the helicoid

    Find the area of the helicoid r(u,v)=(ucos⁡v, usin⁡v, v)r(u, v) = (u\cos v,\ u\sin v,\ v) for 0≤u≤10\le u\le1, 0≤v≤2π0\le v\le2\pi.

    Solution

    ru=(cos⁡v,sin⁡v,0)r_u = (\cos v, \sin v, 0) and rv=(−usin⁡v, ucos⁡v, 1)r_v = (-u\sin v,\ u\cos v,\ 1), so ru×rv=(sin⁡v, −cos⁡v, u)r_u\times r_v = (\sin v,\ -\cos v,\ u) and ∥⋅∥=1+u2\lVert\cdot\rVert = \sqrt{1 + u^2}. The area is 2π∫011+u2 du=2π⋅12[u1+u2+ln⁡(u+1+u2)]01=π(2+ln⁡(1+2))≈7.212\pi\int_0^1\sqrt{1 + u^2}\,du = 2\pi\cdot\frac12\big[u\sqrt{1 + u^2} + \ln(u + \sqrt{1 + u^2})\big]_0^1 = \pi\big(\sqrt2 + \ln(1 + \sqrt2)\big)\approx7.21.

    stretchnew (Schwarz's lantern)

    Derive the area of Schwarz’s lantern with mm slabs and nn points per ring on a cylinder of radius 11 and height 11, and show that for m=nm = n it tends to 2π2\pi as n→∞n\to\infty while for m=n2m = n^2 it does not.

    Solution

    Neighbouring rings are rotated by π/n\pi/n relative to each other, so each triangle has two corners on one ring, joined by a chord of length 2sin⁡(π/n)2\sin(\pi/n), and a third corner on the next ring, directly over the middle of the chord in angle. The horizontal distance from that third corner to the chord’s midpoint is 1−cos⁡(π/n)1 - \cos(\pi/n), and the vertical distance is 1/m1/m, so the height of the triangle (the distance from the apex to the chord’s midpoint) is m−2+(1−cos⁡(π/n))2\sqrt{m^{-2} + (1 - \cos(\pi/n))^2}. A triangle has area sin⁡(π/n)m−2+(1−cos⁡(π/n))2\sin(\pi/n)\sqrt{m^{-2} + (1 - \cos(\pi/n))^2}, and there are 2nm2nm of them. So the area is 2nmsin⁡(π/n)m−2+(1−cos⁡(π/n))22nm\sin(\pi/n)\sqrt{m^{-2} + (1 - \cos(\pi/n))^2}. Rewrite it as 2nsin⁡(π/n)1+m2(1−cos⁡(π/n))22n\sin(\pi/n)\sqrt{1 + m^2(1 - \cos(\pi/n))^2}. As n→∞n\to\infty, 2nsin⁡(π/n)→2π2n\sin(\pi/n)\to2\pi and 1−cos⁡(π/n)≈π22n21 - \cos(\pi/n)\approx\frac{\pi^2}{2n^2}. If m=nm = n then m2(1−cos⁡)2≈π44n2→0m^2(1 - \cos)^2\approx\frac{\pi^4}{4n^2}\to0 and the area tends to 2π2\pi. If m=n2m = n^2 then m2(1−cos⁡)2→π44m^2(1 - \cos)^2\to\frac{\pi^4}4 and the area tends to 2π1+π4/4≈31.62\pi\sqrt{1 + \pi^4/4}\approx31.6, five times the cylinder’s area. The lab confirms both.

    Summary

    • The cross product a×b=(a2b3−a3b2, a3b1−a1b3, a1b2−a2b1)a\times b = (a_2b_3 - a_3b_2,\ a_3b_1 - a_1b_3,\ a_1b_2 - a_2b_1) is orthogonal to aa and bb, and its length is the area of the parallelogram they span. Check every cross product with two dot products.
    • A parametric surface is r(u,v)r(u, v) on a parameter region. Learn the table: graph, cylinder, cone, paraboloid, sphere, ellipsoid, torus, parallelogram. The problem’s constraints set the parameter limits.
    • The fundamental vector product N=ru×rvN = r_u\times r_v is normal to the surface and ∥N∥\lVert N\rVert is the stretching factor from parameter area to surface area. For a graph N=(−gx,−gy,1)N = (-g_x, -g_y, 1) points up.
    • Area is ∬∥N∥ du dv\iint\lVert N\rVert\,du\,dv; a scalar integral is ∬f(r)∥N∥ du dv\iint f(r)\lVert N\rVert\,du\,dv (mass if ff is a density). The sphere has area 4πR24\pi R^2, the cone and paraboloid cap are Midterm 2 problems, the torus has 4π2Ra4\pi^2Ra.
    • Flux through an oriented surface is ∬F⋅n dS=∬F(r)⋅N du dv\iint F\cdot n\,dS = \iint F(r)\cdot N\,du\,dv, where NN must point the way nn does; otherwise use −N-N. The length of NN cancels, so a flux integral has no square root.
    • Compare the sign of NN with ‘upward’, ‘outward’, ‘downward’ or ‘inward’ at one test point, every time. If F⋅nF\cdot n is constant the flux is that constant times the area.
    • The integral does not depend on the parametrization except through orientation, because ρs×ρt=(det⁡Jg) ru×rv\rho_s\times\rho_t = (\det Jg)\,r_u\times r_v. A Moebius strip is not orientable, so it has an area but no flux.
    • Area needs tangent planes, not only points: Schwarz’s lantern shows inscribed polyhedra can fail to converge to the area.

    Watch and read

    The same ideas explained by someone else. Use these when an explanation here does not land.

    Where this sits

    Comes from
    2.7 Determinants
    2.9 Inner products, orthogonality, Gram–Schmidt, projection
    5.3 The total derivative, the Jacobian matrix and tangent planes
    5.4 The chain rule for fields
    6.1 Paths and line integrals
    6.3 Multiple integrals
    6.4 Green's theorem and change of variables
    Leads to
    6.6 Curl, divergence, Stokes' theorem and Gauss's theorem
    6.7 Differential forms and the one big theorem
    6.8 Maxwell's equations, conservation laws and heat
    Same idea elsewhere
    MATH 376: Weeks 5 and 6, Apostol 12.1 to 12.9. Every type of problem the course set is worked below: the cross product and the area of a parallelogram and a triangle (worksheet 12 problems 1 to 3), parametrizing curves, surfaces and the sphere, with the infimum and supremum of a coordinate (worksheet 11 problems 1 to 4 and worksheet 15 problem 1), the fundamental vector product at a point (worksheet 11 problem 5), surface area in cylindrical coordinates (Midterm 2 problem 2 and its sibling), scalar surface integrals and mass (worksheet 12 problem 8, worksheet 13 problems 3 and 4, homework 5 problem 2, worksheet 27 problem 8), flux through graphs, paraboloids, cylinders, cones, discs and the hemisphere (worksheets 11 to 13 and 17, worksheet 27 problem 9, homework 5 problems 1 and 3, Midterm 2 problem 1, Final problem 2 and the practice final), and the bowl under pressure (worksheet 14 problem 4). The exam problems themselves are in 9.3, 9.4 and 9.5.
    MATH 521 and 561: The number E G minus F squared under the root in the area element is the determinant of the first fundamental form of the surface. Area, curvature and geodesics all start from the inner products of r_u and r_v, which is differential geometry.
    CS 559 and computer graphics: A triangle mesh stores a surface as a list of flat triangles. The normal of each triangle is the cross product of two of its edges, its area is half the length of that cross product, and the lighting at a pixel is the dot product of the unit normal with the direction to the light.
    Physics: Flux through a surface is how much of a flow, a heat current or an electric field crosses it. Gauss's law in 6.8 says the electric flux through a closed surface is the enclosed charge divided by a constant.