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Andrew Rosen Chapter 14 - Vector Calculus, Part II (LATEX) 14.4 - Green's Theorem Green's Theorem - Circulation Form: ˛ − → − F · d→ r = ˛ ¨ f dx + g dy = ∂g ∂x − ∂f dA ∂y R Note: The partial derivatives that are subtracted in the double integrand are collectively known as the two-dimensional curl Note: From here on out, the positive direction is counterclockwise. If the curve is oriented clockwise, negate the answer → − If the two-dimensional curl of a vector eld, F = hf, gi, is zero then it is said to be irrotational → − → − → − If the 2-D curl is zero, F is conservative ( F = ∇φ) because ¸→ − → F · d− r will also be zero Area of a Plane Region by Line Integrals: ˛ ˛ x dy = − C y dx = C 1 ˛ (x dy − y dx) 2 C Green's Theorem - Flux Form: ˛ − → F · n̂ ds = ˛ ¨ f dy − g dx = ∂f ∂x + ∂g ∂y dA R C Note: The partial derivatives that are added in the double integrand are collectively known as the dimensional divergence two- → − If the two-dimensional divergence of a vector eld, F = hf, gi, is zero then it is said to be source-free 14.5 - Divergence and Curl ∂g ∂h ∂f − → − → − → div F = ∇ · F = + + ∂x ∂y ∂z ∂h ∂g ∂f ∂h ∂g ∂f − → − → − → curl F = ∇ × F = h − , − , − i ∂y ∂z ∂z ∂x ∂x ∂y Properties of a Conservative Vector Field: → − → − 1. There exists a potential function, φ, such that F = ∇φ 2. ´→ − → F · d− r = φ(B) − φ(A) for all points on a smooth, oriented curve, C , from A to B C 3. ¸→ − → F · d− r = 0 on all simple, smooth, close oriented curves C C → − → − → − 4. 1 ∇ × F = 0 Note: Rule #4 only applies if −→ F has continuous partial derivatives on all of R3 , so if there is a singularity anywhere then the theorem cannot be used 1 1 → − → − → − → − Curl of a Gradient: If F is conservative then ∇ × ( ∇φ) = 0 → − → − → − Divergence of the Curl: ∇ · ( ∇ × F ) = 0 14.6 - Surface Integrals A general description for a parametric surface is the following, → − r (u, v) = hx(u, v), y(u, v), z(u, v)i A general description for parameterizing a cylinder with its axis along the z axis with radius, r: → − r (θ, z) = hr cos θ, r sin θ, zi A general description for parameterizing a cone with its vertex at the origin with radius, r, and height, h: rz rz → − r (θ, z) = h cos θ, sin θ, zi h h A general description for parameterizing a sphere with radius, ρ, centered at the origin2 : → − r (φ, θ) = hρ sin φ cos θ, ρ sin φ sin θ, ρ cos φi Surface Integral of Scalar Functions: ¨ ¨ f (x, y, z) dS = S − → − → f (x(u, v), y(u, v), z(u, v)) | t u × t v | dA R Surface Integral of Vector Fields: ¨ F lux = − → F · n̂ dS = ¨ S − → − → − → F · ( t u × t v ) dA R Average value of a function on a surface: ˜ Average = R → − → − f (x(u, v), y(u, v), z(u, v)) | t u × t v | dA ˜ → − → − | t u × t v | dA R Finding the magnitude of the cross product of the two partial derivative vectors can be dicult here, but it will usually be , which is exactly what is used for a spherical coordinate triple integral! This will be dA here. Even though the sphere is parameterized with spherical coordinates, do not multiply in another factor of ρ2 sin φ. It's a regular, rectangular double integral with bounds for φ and θ 2 ρ2 sin φ 2 Example for nding the equation of a tangent plane at a point on a surface: → − Find the equation of the tangent plane at (1, 1, 3) of t (u, v) = hu2 , v 2 , u + 2vi Step 1: Calculate the cross product of the partial derivatives → − → − t u = h2u, 0, 1i and t v = h0, 2v, 2i → − → − t u × t v = h2u, 0, 1i × h0, 2v, 2i = h−2v, −4u, 4uvi Step 2: Solve for the normal vector by nding u, v and substituting into the cross product x = 1 = u2 → u = ±1 y = 1 = v 2 → v = ±1 z = 3 = u + 2v ∴ u, v = 1 → − n (1, 1, 3) = h−2, −4, 4i Step 3: Set up the tangent plane equation at that point −2(x − 1) − 4(y − 1) + 4(z − 3) = 0 → −2x − 4y + 4z = 6 14.7 - Stokes' Theorem → − Assuming that F is a vector eld show components have continuous rst partial derivatives on S , ˛ − → − F · d→ r = ¨ − → − → ( ∇ × F ) · n̂ dS S Note: The normal vector for an explicitly dened surface z = g(x, y) is h−zx , −zy , 1i [Might help to solve some problems] Note: If the surface is in the xy plane, the unit normal vector is k̂ 14.8 - Divergence Theorem ¨ − → F · n̂ dS = S ˚ D 3 − → − → ∇ · F dV