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    10. Method of Moments

    .

    1/3/20141 Electromagnetic Field Theory by R. S. Kshetrimayum

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    10.1 Introduction

    learn how to use method of moments (MoM) to solve

    electrostatic problems

    advanced & challenging problems in time-varying fields

    brief discussion on the basic steps of MoM

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum2

    so ve a s mp e eren a equa on us ng o in order to elucidate the steps involved

    MoM tfor 1-D and 2-D electrostatic problems

    MoM for electrodynamic problems

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    10.2 Basic Steps in Method of Moments Method of Moments (MoM) transforms

    integro-differential equations into matrix systems of linear equations

    which can be solved using computers

    Consider the following inhomogeneous equation

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum3

    where L is a linear integro-differential operator,

    u is an unknown function (to be solved) and

    k is a known function (excitation)

    kuL =

    ( ) 0= kuL

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    10.2 Basic Steps in Method of Moments For example,

    (a) consider the integral equation for a line charge density

    0

    0

    ( ') '

    4 ( , ')

    x dxV

    r x x

    =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum4

    Then ( )

    'u x=

    0k V=

    0

    '4 ( , ')

    dxLr x x

    =

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    10.2 Basic Steps in Method of Moments (b) consider the differential equation of the form

    Then

    2

    22( ) 3 2d f x x

    dx = +

    =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum5

    23 2k x= +

    2

    2

    dL

    dx=

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    10.2 Basic Steps in Method of Moments To solve u, approximate it by sum of weighted known

    basis functions or

    expansion functions

    as given belowN N

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum6

    where is the expansion function,

    is its unknown complex coefficients to be determined, Nis the total number of expansion functions

    1 1, 1, 2,...,n n n

    n nu u I b n N

    = = = =

    nb

    nI

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    10.2 Basic Steps in Method of Moments Since L is linear, substitution of the above equation in the

    integro-differential equation,

    we get,

    N

    n nL I b k

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum7

    where the error or residual is given by

    1n=

    1

    N

    n n

    n

    R k L I b=

    =

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    10.2 Basic Steps in Method of Moments Mathematicians name this method as Method of Weighted

    Residuals

    Why?

    Next step in MoM

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum8

    n orc ng t e oun ary con t on Make inner product of the above equation with each of the

    testing or

    weighting functions should make residual or error zero

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    10.2 Basic Steps in Method of Moments

    By replacing u by where n=1,2,,N

    taking inner product with a set of

    n

    u

    mw

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum9

    we g ng or

    testing functions

    in the range of L, we have,

    ( )( ), 0, 1, 2,...,m nw L u k m M = =

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    10.2 Basic Steps in Method of Moments

    Since In is a constant we can take it outside the inner product and

    write

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum10

    M and N should be infinite theoretically

    but practically it should be a finite number

    ( )1

    , , , 1, 2,...,N

    n m n m

    n

    I w L b w k m M=

    = =

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    10.2 Basic Steps in Method of Moments Note that a scalar product is defined to be a scalar

    satisfying

    , , ( ) ( )w g g w g x w x dx= =

    gw,

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum11

    b and c are scalars and * indicates complex conjugation

    wgcwwcg ,,,

    +=+

    00,*

    > gifgg 00,*

    == gifgg

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    10.2 Basic Steps in Method of Moments In matrix form

    with each matrix and vector defined by

    [ ][ ] [ ]VIZ =

    [ ] [ ]TNIIII ...21= [ ] 1 2, , ... ,T

    MV k w k w k w =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum12

    [ ]

    ( ) ( ) ( )

    ( ) ( ) ( )

    ( ) ( ) ( )

    ( ) ( ) ( )

    1 1 1 2 1

    2 1 2 2 2

    3 1 3 2 3

    1 2

    , , ,

    , , ... ,

    , , ,...

    , , ... ,

    N

    N

    N

    M M M N

    w L b w L b w L b

    w L b w L b w L b

    Z w L b w L b w L b

    w L b w L b w L b

    =

    K

    OM M M

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    10.2 Basic Steps in Method of Moments For [Z] is non-singular,

    Solve the unknown matrix [I] of amplitudes of basis functionas[ ] [ ] [ ] [ ][ ]

    1I Z V Y V

    = =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum13

    a er in s met o

    Point matching or Collocation

    The testing function is a delta function

    nn wb =

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    10.2 Basic Steps in Method of Moments Methods for calculating inverse of a matrix

    Seldom find the inverse of matrix directly , because, if we have ill-conditioned matrices,

    it can give highly erroneous results

    [ ] 1

    Z

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum14

    comman p nv n s pseu o nverse o a ma r x

    using the singular value decomposition

    For a matrix equation of the form AX=B,

    if small changes in B leads to large changes in the solution X, then we call A is ill-conditioned

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    10.2 Basic Steps in Method of Moments The condition number of a matrix is the

    ratio of the largest singular value of a matrix to the smallest

    singular value

    Larger is this condition value

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum15

    It is always

    greater than or equal to 1

    If it is close to one,

    the matrix is well conditioned

    which means its inverse can be computed with good accuracy

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    10.2 Basic Steps in Method of Moments If the condition number is large,

    then the matrix is said to be ill-conditioned

    Practically,

    such a matrix is almost singular, and

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum16

    e compu a on o s nverse, or

    solution of a linear system of equations is

    prone to large numerical errors

    A matrix that is not invertible has the condition number equal to infinity

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    10.2 Basic Steps in Method of Moments Sometimes pseudo inverse is also used for finding

    approximate solutions to ill-conditioned matrices

    Preferable to use LU decomposition

    to solve linear matrix equations

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum17

    ac or za on un e auss an e m na on,

    do not make any modifications in the matrix B

    in solving the matrix equation

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    10.2 Basic Steps in Method of Moments Try to solving a matrix equation

    using LU factorization

    First express the matrix

    [ ] [ ][ ]A L U=

    [ ][ ] [ ]A X B=

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum18

    [ ] [ ]

    11 11 12 13 1

    21 22 22 23 2

    31 32 33 33 3

    1 2 3 1

    0 0 0

    0 0 0

    0 0 0

    ... 0 0 0 ...

    N

    N

    N

    N N N N NN

    l u u u u

    l l u u u

    L l l l and U u u

    l l l l u

    = =

    L L

    L L

    L L

    M M M O M M M M O M

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    10.2 Basic Steps in Method of Moments

    through the forward substitution

    [ ][ ][ ] [ ] [ ][ ] [ ]L U X B L Y B = =

    11 1

    ib = =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum19

    through the backward substitution

    1

    111

    ,i i ik k

    kiil l =

    [ ][ ] [ ]U X Y=

    1

    1; ,

    NN

    N i i ik k

    k iNN ii

    yx x y u x i N

    u u = +

    = =

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    10.2 Basic Steps in Method of Moments This is more efficient than Gaussian elimination

    since the RHS remain unchanged during the whole process

    The main issue here is to

    find the lower and upper triangular matrices.

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum20

    comman or ac or za on o a ma r x s

    [L U] = lu(A)

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    10.2 Basic Steps in Method of MomentsExample 10.1

    Consider a 1-D differential equation2

    2

    2

    ( )3 2

    d f xx

    dx = +

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum21

    subject to the boundary condition f(0)=f(1)=0 Solve this differential equation using Galerkins MoM

    Solution:

    Note that for this case,

    ( )u f x=

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    10.2 Basic Steps in Method of Moments

    According to the nature of the known function ,

    23 2k x= +

    2

    2dL dx=

    23 2k x= +

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum22

    it is natural to choose the basis function as However,

    the boundary condition f(1)=0

    cant be satisfied with such a basis function

    ( ) nn

    b x x=

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    10.2 Basic Steps in Method of Moments A suitable basis function for this differential equation

    taking into account of this boundary condition is

    ( ) 1; 1,2, ...,nnb x x x n N +

    = =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum23

    ssume = t e tota num er o su sections on t einterval [0,1])

    Approximation of the unknown function

    ( ) ( )2 3

    1 1 2 2 1 2( ) ( ) ( )f x I b x I b x I x x I x x + = +

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    10.2 Basic Steps in Method of Moments For Galerkins MoM, the weighting functions are

    Choosing a square [Z] matrix where M=N=2

    ( ) 1

    ; 1, 2,...,m

    mw x x x m M +

    = =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum24

    ( ) ( ) ( )1 1

    211 1 1 1 1

    0 0

    1, ( ) ( ) ( ) 23

    Z w L b w x L b x dx x x dx= = = =

    ( ) ( ) ( )

    1 1

    2

    12 1 2 1 2

    0 0

    1, ( ) ( ) ( ) 6 2Z w L b w x L b x dx x x x dx= = = =

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    10.2 Basic Steps in Method of Moments Therefore,

    [ ][ ] [ ] 1

    2

    1 1 3

    3 2 5

    1 4 112 5 12

    IZ I V

    I

    = =

    13

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum26

    The unknown function f(x)

    [ ]

    1

    2 1

    3

    I I = =

    ( ) ( ) ( ) ( )2 3 2 31 213 1

    ( )10 3

    f x I x x I x x x x x x + = +

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    10.2 Basic Steps in Method of Moments The above function satisfies the given boundary conditions

    f(0)=f(1)=0

    The analytical solution for this differential equation is

    2 45 3 1( )f x x x x=

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum27

    Check whether the above solution using MoM is

    different from the analytical solution obtained by direct

    integration (see Fig. 10.1)

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    10.2 Basic Steps in Method of Moments

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum28

    Fig. 10.1 Comparison of exact solution (analytical) and approximatesolution (MoM) of Example 10.1

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    10.3 Introductory examples from electrostatics In electrostatics, the problem of finding the potential

    due to a given charge distribution is often considered

    In practical scenario, it is very difficult to specify a charge distribution

    We usually connect a conductor to a voltage source

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum29

    and thus the voltage on the conductor is specified We will consider MoM

    to solve for the electric charge distribution

    when an electric potential is specified

    Examples 2 and 3 discuss about calculation of inverse using LUdecomposition and SVD

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    10.3 Introductory examples from electrostatics 1-D Electrostatic case: Charge density of a straight wire

    Consider a straight wire of length l and radius a (assume

    a

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    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum31

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    10.3 Introductory examples from electrostaticsFig. 10.2

    (a) Straight wire of length l and radius a applied with a

    constant potential of 1V

    (b) Its segmentation: y1, y2, , yN are observation points and

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum32

    (c) Division of the charged strip into N sections

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    10.3 Introductory examples from electrostatics where

    It is necessary to solve the integral equation

    ' ' ' 2 ' 2 ' 2 ' 2 2

    0( , ) ( , ) ( ) ( ) ( ) ( ) ( )x zR y y R r r y y x z y y a= == = + + = +

    r r

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum33

    to find the unknown function

    (y)

    The solution may be obtained numerically by

    reducing the integral equation into a series of linear algebraic

    equations

    that may be solved by conventional matrix techniques

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    10.3 Introductory examples from electrostatics (a) Approximate the unknown charge density (y)

    by an expansion of N known basis functions with unknown

    coefficients

    =

    =

    N

    n

    nn ybIy

    1

    '' )()(

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum34

    Integral equation after substituting this is

    =

    = ==

    l

    n

    l N

    n

    n

    N

    n

    nn

    yyR

    dyybIyyR

    dyybI

    0'

    ''

    0 1'

    '

    1

    '

    0),(

    )(

    ),(

    )(

    4

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    10.3 Introductory examples from electrostatics Now we have divided the wire into N uniform segments each

    of length as shown in Fig. 10.2 (b)

    We will choose our basis functions as pulse functions

    ( )

    = nynfor

    ybn

    '' )1(1

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum35

    b) Applying the testing or weighting functions

    Let us apply the testing functions as delta functions

    for point matching

    ( )my y

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    10.3 Introductory examples from electrostatics Integration of any function with this delta function

    will give us the function value at

    Replacing observation variable y by a fixed point such as ym,

    results in an integrand that is solely a function of y

    my y=

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum36

    so e n egra may e eva ua e .

    It leads to an equation with N unknowns

    +++++=

    2

    )1( )1(

    '

    ''

    '

    ''

    '

    ''2

    2

    0

    '

    ''1

    10

    ),(

    )(...

    ),(

    )(...

    ),(

    )(

    ),(

    )(4

    n

    n

    l

    N m

    NN

    m

    nn

    mm yyR

    dyybI

    yyR

    dyybI

    yyR

    dyybI

    yyR

    dyybI

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    10.3 Introductory examples from electrostatics

    Solution for these N unknown constants,

    N linearly independent equations are required

    N equations may be produced

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum37

    y c oos ng an o serva on po n ym on e w re an

    at the center of each length element

    as shown in Fig. 10.2 (c)

    Result in an equation of the form of the previous equation

    corresponding to each observation point

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    10.3 Introductory examples from electrostatics

    For N such observation points we have

    +++++=

    2

    )1( )1('

    1

    ''

    '1

    ''

    '1

    ''

    22

    0'

    1

    ''

    110),(

    )(...),(

    )(...),(

    )(),(

    )(4

    n

    n

    l

    N

    NNnnyyRdyybI

    yyRdyybI

    yyRdyybI

    yyRdyybI

    2 '''''''' n l

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum38

    +++++=

    )1( )1('2'2'2

    2

    20

    '2

    1

    10 ),(...

    ),(...

    ),(),(4

    n N

    N

    N

    n

    n yyR

    yyI

    yyR

    yyI

    yyR

    yyI

    yyR

    yyI

    +++++=

    2

    )1( )1( '

    ''

    '

    ''

    '

    ''2

    2

    0 '

    ''1

    10

    ),(

    )(...

    ),(

    )(...

    ),(

    )(

    ),(

    )(4

    n

    n

    l

    N N

    NN

    N

    nn

    NN yyR

    dyybI

    yyR

    dyybI

    yyR

    dyybI

    yyR

    dyybI

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    10.3 Introductory examples from electrostatics(c) We may write the above equations in matrix form as

    [ ][ ] [ ]

    11 12 1 1 0

    21 22 2 2 0

    31 32 3 3 0

    ...

    ...

    N

    N

    N mn n m

    Z Z Z I V

    Z Z Z I V

    Z Z Z I V Z I V

    = =

    K

    OM M M M M

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum39

    where

    1 2 0...N N NN NZ Z Z I V

    [ ] [ ]04=mV

    1

    1 1

    ' ' '

    ' 2 2 ' 2 2

    0

    ' '

    '' 2

    ( )

    ( ) ( )

    ( )

    n

    n

    n n

    n n

    yl

    n

    mn

    ym m

    y y

    m m ny ym

    b y dy dyZ

    y y a y y ady dy

    for m ny y y yy y

    = =

    + +

    =

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    10.3 Introductory examples from electrostatics Special care for calculating the Zmn for m=n case

    since the expression for Zmn is infinite for this case

    Extraction of this singularity

    Substitute ' 'm

    y y d dy = =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum40

    ( )0

    2 2

    2 2 2 20

    0

    log ( )( ) ( )

    mnd dZ a

    a a

    = = = + +

    + +

    2 2

    ln a

    a

    + +=

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    10.3 Introductory examples from electrostatics Self or diagonal terms are the

    most dominant elements in the [Z] matrix

    Note that linear geometry of this problem

    yields a matrix that is symmetric toeplitz, i.e.,

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum41

    [ ]

    11 12 1

    12 11 1 1

    1 1 1 11

    ...

    ...

    . . . .

    ...

    N

    N

    mn

    N N

    Z Z Z

    Z Z ZZ

    Z Z Z

    =

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    10.3 Introductory examples from electrostatics All other rows are a rearranged version of the first row

    Required to calculate the first row of the matrix only

    Remaining elements can be obtained by the rearrangement

    formula:

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum42

    Therefore the unknown [I] matrix could be solved as

    1, 1, ,mn m n m n +=

    [ ] [ ] [ ]mmnn VZI 1

    =

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    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum43

    Fig. 10.3 (a) Convergence plot of Z11 and Z21 (b) Plot of line charge density ofthe wire (MATLAB program provided in the book)

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    10.3 Introductory examples from electrostatics Let us see the convergence of these two types of elements of

    the Z matrix say,

    Z11 and Z21

    Fig. 10.3 (a) shows the convergence plot of two elements of

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum44

    for number of sub-sections varying from 5 to 100

    The graph of Z21 (dashed line) versus number of sub-sections

    is a straight line

    so any number of sub-sections between 5 and 100 should givethe same result

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    10.3 Introductory examples from electrostatics But the graph of Z11 versus number of sub-sections is

    decreasing quite fast at the initial values of number of sub-

    sections and it is decreasing more slowly for larger values of number of sub-

    sections

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum45

    This shows that at higher values of number of sub-sections,

    we will get a more convergent result

    Choose the maximum number of sub-sections and plot the line charge density as depicted in the Fig. 10.3 (b)

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    10.3 Introductory examples from electrostatics See the condition number of the [Z] matrix in order to see

    whether the [Z] matrix is well-behaved or not

    The condition number of [Z] matrix

    (=7.1409) for maximum number of sub-sections is good

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum46

    o pro em n a ng e nverse

    Fig. 10.3 (b) line charge density is

    maximum at the two end points of the wire and

    minimum at the center of the wire

    2-D Electrostatic case: Charge density of a square conducting

    plate discussed in the book

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    10.4 Some commonly used basis functions The weighted sum of basis functions is

    used to represent the unknown function in MoM

    Choose a basis function that reasonably approximates

    the unknown function over the given interval

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum47

    as s unc ons common y use n an enna or sca er ng

    problems are of two types:

    entire domain functions and

    sub-domain functions

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    10.4 Some commonly used basis functions10.4.1 Entire domain basis functions

    The entire domain functions exist over the full domain

    -l/2

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    10.4 Some commonly used basis functions Chebyshev's differential equation

    where n is a real number

    01 2'''2

    =+ ynxyyx

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum49

    Solutions Chebyshev functions of degree n

    n is a non-negative integer, i.e., n=0,1,2,3,,

    the Chebyshev functions are called Chebyshev polynomials

    denoted by Tn(x)

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    10.4 Some commonly used basis functions A Chebyshev polynomial at one point can be

    expressed by neighboring Chebyshev polynomials at the same

    point

    ( ) ( ) ( )xTxxTxT nnn 11 2 + =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum50

    0 , 1

    Legendre's differential equation

    where n is a real number

    ( ) 0121 '''2 =++ ynnxyyx

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    10.4 Some commonly used basis functions Disadvantage: entire domain basis function may not be

    applicable of any general problem

    Choose a particular basis function for a particular problem Crucial and only experts in the area could do it efficiently

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    ,

    software for analyzing almost every problem inelectromagnetics

    this is not feasible

    Sub-domain basis functions could achieve this purpose

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    10.4 Some commonly used basis functions10.4.2 Sub-domain basis functions

    Sub-domain basis functions exist only on one of the N

    overlapping segments

    into which the domain is divided

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    :

    Piecewise constant function (pulse)

    1 [ 1] [ ]( )

    0n

    x n x x nb x

    otherwise

    <

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    10.4 Some commonly used basis functions Piecewise triangular function

    [ 1] [ 1]( )

    0

    n

    n

    x xx n x x n

    b x

    otherwise

    < < +

    =

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum54

    1

    1

    1

    1

    [ 1] [ ]

    [ ] [ 1]

    0

    n

    n n

    n

    n n

    x xx n x x nx x

    x xx n x x n

    x x

    otherwise

    +

    +

    <

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    10.4 Some commonly used basis functions

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum56

    Fig. 10.5 Sub-domain basis functions (a) Piecewise constant

    function (b) Piecewise triangular function (c) Piecewisesinusoidal function

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    10.4 Some commonly used basis functions Since the derivative of the pulse function is impulsive

    we cannot employ it for MoM problems

    o where the linear operator L consists of derivatives

    Piecewise triangular and sinusoidal functions

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum57

    may be used for such kinds of problems Piecewise sinusoidal functions are generally used

    for analysis of wire antennas since

    they can approximate sinusoidal currents in the wireantennas

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    10.5 Wire Antennas and Scatterers For Piece-wise triangular and sinusoidal functions

    when we have N points in an interval

    we will have N-1 sub-sections and

    N-2 basis functions may be used

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    10.5 Wire Antennas and Scatterers

    Consider application of MoM techniques

    to wire antennas and scatterers

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    10.5 Wire Antennas and Scatterers Antennas can be distinguished from scatterers

    in terms of the location of the source

    If the source is on the wire

    it is regarded as antenna

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum59

    W en t e wire is ar rom t e source

    it acts as scatterer

    For the wire objects (antenna or scatterer)

    we require to know the current distribution accurately

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    10.5 Wire Antennas and Scatterers Integral equations are derived and

    solved for this purpose

    Wire antennas

    Feed voltage to an antenna is known

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    an t e current istri ution cou e ca cu ate

    other antenna parameters such as

    impedance,

    radiation pattern, etc.

    can be calculated

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    10.5 Wire Antennas and ScatterersWire scatterers

    Wave impinges upon surface of a wire scatterer

    it induces current density

    which in turn is used to generate the scattered fields

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    e w cons er

    how to find the current distribution on a

    thin wire or

    cylindrical antenna

    using the MoM

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    10.5 Wire Antennas and Scatterers10.5.1 Electric field integral equation (EFIE)

    On perfect electric conductor like metal

    the total tangential electric field is zero

    Centrally excited cylindrical antenna (Fig. 10.6)

    1/3/2014Electromagnetic Field Theory by R. S. Kshetrimayum62

    ave two in s o e ectric ie s viz.,

    incident and

    scattered electric fields

    t

    tan tan tan tan tan0 0ot inc scat inc scat

    E E E E E= + = =

    r r r r r

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    2

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    Fig. 10.6 A thin wire antenna of length L, radius a (a

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    10.5 Wire Antennas and Scatterers where the is the source or impressed field and

    can be computed from the

    current density induced on the cylindrical wire antenna due to the

    incident or

    incE

    r

    scatE

    r

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    mpresse e

    10.5.2 Hallens and Pocklington's Integro-differential equation

    Let us consider a perfectly conducting wire of

    length L and

    radius a such that a

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    10.5 Wire Antennas and Scatterers Consider the wire to be a hollow metal tube

    open at both ends

    Let us assume that an incident wave impinges on the surface of a wire

    ( )incE rr r

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    en e w re s an an enna

    the incident field is produced by the feed at the gap (see Fig.10.6)

    The impressed field is required

    to be known on the surface of the wire

    inc

    zE

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    10.5 Wire Antennas and Scatterers Simplest excitation

    delta-gap excitation

    For delta gap excitation (assumption) excitation voltage at the feed terminal is constant and

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    66

    Implies incident field constant over the feed gap and

    zero elsewhere

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    10.5 Wire Antennas and Scatterers 2V0 (from + V0 to -V0) voltage source applied

    across the feed gap 2,

    Incident field on the wire antenna can be expressed as

    0V

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    67

    Induced current density

    due to the incident or impressed electric field produces the scattered electric field

    0;2

    inc

    zE Lz

    =


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