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Surface Integral 1 Sk/EUM114/ Vector 3 Lecture/2015 Surface Integral

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  • Surface Integral

    1

    Sk/EUM114/ Vector 3 Lecture/2015

    Surface Integral

  • Surface Integral

    2

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    3

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    4

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    5

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    6

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    7

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    8

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    9

    Sk/EUM114/ Vector 3 Lecture/2015

    Stokes Theorem

  • Surface Integral

    10

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    11

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    12

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    13

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    14

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    15

    Sk/EUM114/ Vector 3 Lecture/2015

  • Surface Integral

    16

    Sk/EUM114/ Vector 3 Lecture/2015

    Triple Integrals - Divergence Theorem of Gauss (1777-1855)

    The triple integral is a generalization of the double integral introduced above. For defining this integral,

    one considers a function , ,f x y z defined in a bounded closed region T of space. One subdivides T by

    planes parallel to the three coordinate planes. Then, one numbers the parallelepipeds inside T from 1 to n.

  • Surface Integral

    17

    Sk/EUM114/ Vector 3 Lecture/2015

    In each such parallelepiped, one chooses an arbitrary point, say , ,k k kx y z in the kth

    parallelepiped, and form the sum

    1

    , ,n

    n k k k k

    k

    J f x y z v

    (1)

    wherekv is the volume of the kth parallelepiped. This limit is called the triple integral of

    , ,f x y z over the region T, and is denoted by

    , , or , ,T T

    f x y z dxdydz f x y z dv (2)

    S T T

    F nd div Fdxdydz div Fdv (3)

    Example

  • Surface Integral

    18

    Sk/EUM114/ Vector 3 Lecture/2015

    Compute ,S

    F n d where 2 2 , , 2 4F x y z x i yj z k and S is the surface of the cylinder

    2 2 4, 0 2x y z .

    Solution

    div 2 2 8F x z , so

    2 2

    2 2 2 2

    2

    04

    2

    4 4

    2 2 8 2 2 8

    z=2 2 2 4 4 20

    z=0

    S T x y

    x y x y

    F n x z dzdxdy x z dzdxdy

    xz z z dxdy x dxdy

    Let cosx r and siny r , then 2 2 2 2 2 2 24 cos sin 2x y r r r r .

    The differential area in the polar coordinate system becomes dA dxdy rdrd .)

    2 2 2 2

    2

    0 0 0 0

    2

    0

    4 cos 20) 4 cos 5

    8 4 cos 10 80

    3

    r rdrd r r drd

    d

  • Surface Integral

    19

    Sk/EUM114/ Vector 3 Lecture/2015

    Example

    By transforming to a triple integral, evaluate

    3 2 2S

    I x dydz x y dxdz x z dxdy

    where S is the closed surface consisting of the cylinder 2 2 2 0 z bx y a and the dicks z=0

    and z=b. From (6), it is evident that

    3 2 2, ,P x Q x y R x z

    Hence, by taking advantage of the symmetry of the circle (evaluate only 1/4 of the circle), the

    corresponding triple integral takes the from by (6)

    2 2

    3/22 2 2 2 2 2

    0 0 0 0 0

    13 4 5 20

    3

    b a a y b a

    T

    I x x x dxdydz x dxdydz a y dydz

    Let sin , cosy a dy a d , then

    3/23/2 3/2

    2 2 2 2 2 2 3 31 sin cos cosa y a a a

    and

    43/2 /2

    2 2 4 4 4

    0 0

    1 1 1 3cos

    3 3 3 8 2 16

    a aa y dy a d a

    Hence, the integral I becomes

  • Surface Integral

    20

    Sk/EUM114/ Vector 3 Lecture/2015

    44

    0

    520

    16 4

    b aI dz a b

    Example

    If F and n are expressed in terms of their Cartesian components such that

    cos , cos , cos ,x y z

    F n x n i y n j z n k i j kr r r

    where

    2 2 2r x y z and the region T is the sphere 2 2 2 2x y z a

    Evaluate the triple integral :

    Solution

    Assuming that 0r

    2 2 2 2 2 2 2 2 2

    2 2 2 32 2 2

    /x y z x x y zP x r x

    x x x y z rx y z

    Likewise,

    2 2

    3

    Q r y

    y r

    and

    2 2

    3

    R r z

    z r

    Hence,

    2 2

    3

    3 20

    r rdiv F if r

    r r

    and

    2

    T

    dxdydzr

    Since the triple integral is discontinuous when r=0, care must be exercised. Returning back to

    the equivalent surface integral reveals that

    2 2 22

    2 2 2 1 4

    S S S

    x y zF nd d d a

    r r r

    The integral is simply the surface area of a sphere of radius a, thus avoiding an integral

    containing a discontinuity at r=0.

  • Surface Integral

    21

    Sk/EUM114/ Vector 3 Lecture/2015

    The triple integral may be evaluated by transforming the Cartesian coordinates into the spherical

    coordinates. From the sketch, it is clear that

    In this case, r . 2 sindv dxdydz r drd d

    2 22 2

    0 0 0 0 0

    22 2 2

    0

    2 12 sin sin

    cos 2 1 1 40

    a

    T

    dxdydz r drd d a d dr r

    a d a a

    As expected, it yields the same result.

  • Surface Integral

    22

    Sk/EUM114/ Vector 3 Lecture/2015

    Hints on Surface Itegrals

    Case 1. Parametrize and Integrate

    Write the parametric equation r(u,v) of the surface. Find dS = (ru x rv) du dv. Take the dot

    product with F and integrate over u and v.

    Case 2. Use the Divergence (Gausss) Theorem a) The Divergence Theorem has exactly the same flavor as Stokes Theorem.

    You go up one dimension

    You take some kind of derivative of the integrand

    You integrate over the region bounded by the closed shape

    b) In the xz plane, ( ) ( ) ( )dS dx i dz k dxdz j

    c) In the yz plane, ( ) ( ) ( )dS dy j dz k dydz i

    Case 3.

    In Stokes theorem, Curl (F ) =0, implies that F = Grad (f.) for some f.

    Then it is easy to find the potential f and evaluate at the end points. Another way of saying this is that the

    integral depends only on the boundary of the curve, namely the end points. Thus, one could replace the

    curve by the simplest curve with the same boundary, namely a line joining the end points. In practice one

    never does this since it is simpler to evaluate f at the end points.

    Is

    No

    Is S closed?

    No

    Parametrize and Integrate

    Yes

    Yes

    Is S closed?

    No

    Choose simplest surface S with the

    same boundary

    Yes

    =0

  • Surface Integral

    23

    Sk/EUM114/ Vector 3 Lecture/2015

    In Gausss theorem, if Div(F)=0, implies that F=Curl(A) for some A.

    Now it is not easy to find the vector potential A. But the situation is similar. The integral depends only on

    the boundary, so one can replace the original surface S with the simplest surface that has the same

    boundary. So, for example, if the surface is the upper hemisphere z=sqrt(a^2-x^2-y^2), where the

    computation of the differential of surface is nasty, one could use the surface z=0, (where dS = dx dy k)

    and integrate over a circle of radius a.

    Think of this as the butterfly net catcher theorem. If Div (F) =0 then there are no sources or sinks inside

    the surface, the flux of butterflies coming into the surface net depends only on the Rim of the net.

    Case 4.

    If Div(F)=0 and the surface is closed, then there are no sources or sinks inside the surface, so the net Flux

    is zero! Whatever goo comes in, must come out..

    So Why is this Important?

    Gausss and Stokes theorem are central to Physics. Without Gradients, Curls and Divergences, one could not give a full quantitative description of Gravitation, Electrodynamics, Fluid Dynamics, Aerospace

    Engineering, Atmospheric Sciencesyou get the point.

  • Surface Integral

    24

    Sk/EUM114/ Vector 3 Lecture/2015

    Summary of Surface Integrals

    Type

    of Int. Notation

    Definition and

    Interpretations/Applications Standard/Direct Way to Compute

    Major Theorems that

    Indicate How to Compute

    Indirectly

    surf

    ace

    in

    teg

    ral

    of

    a

    real-

    valu

    ed f

    un

    ctio

    n

    ( , , )S

    f x y z dS

    *

    ,1 1

    lim ( )m n

    ij ijm n

    i j

    f P S

    (mass/moments of a surface)

    22

    ( , , ) 1D

    dz dzf x y z dA

    dx dy

    , where

    ( , )z g x y is the function whose graph is the

    surface S of integration and D is the

    projection of S; OR ( ( , )) u vD

    f u v dA r r r where D is the pre-image (in the uv-plane) of

    S

    Su

    rface

    (or

    flu

    x)

    inte

    gra

    l of

    a v

    ecto

    r

    fiel

    d

    S dSF , OR

    S dSnF (this notation infers

    outward orientation

    if S is closed and

    upward orientation

    if S is not closed)

    m

    i

    n

    j

    ijijijnm

    SPP1 1

    **

    ,lim nF

    (rate of flow through a surface)

    ( , , ) ( , , ) ( , , )D

    g gP x y z Q x y z R x y z dA

    x y

    where z = g(x,y) is the function whose graph

    is the surface S of integration and D is the

    projection of S; OR

    D vu dA)( rrF , where D is the pre-image (in the uv-plane) of S

    Stokes Theorem:

    SC dd SFrF curl where C is the boundary of S

    Divergence Theorem:

    ES dVd FSF div where S is the boundary of E

    Note: There are analogous notations, definitions, and formulas for situations in which the roles of x, y, and/or z are swapped.

    Based on an upward

    orientation of S