Top Banner

of 30

01 Electromagnetic Radiation

Jun 04, 2018

Download

Documents

ekosatria004
Welcome message from author
This document is posted to help you gain knowledge. Please leave a comment to let me know what you think about it! Share it to your friends and learn new things together.
Transcript
  • 8/13/2019 01 Electromagnetic Radiation

    1/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    1

    Electromagnetic Radiation

    1. Radiation Mechanism

    When electric charges undergo acceleration or

    deceleration, electromagnetic radiation will be

    produced. Hence it is the motion of charges (i.e.,

    currents) that is the source of radiation.

    Yet not all current distributions will produce a strong

    enough radiation for communication. We will firststudy some typical current distributions and the

    radiation fields that they produce.

  • 8/13/2019 01 Electromagnetic Radiation

    2/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    2

    2. Vector and Scalar PotentialsFrom Maxwells fourth equation:

    0

    0 A

    For any vector function A,

    AB

    So we can write:

  • 8/13/2019 01 Electromagnetic Radiation

    3/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    3

    ABE

    j

    jFrom Maxwells first equation:

    Then,

    0 AE j

    For any scalar function ,

    0

    So we can write:j E A

    That is, j E A

  • 8/13/2019 01 Electromagnetic Radiation

    4/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    4

    From Maxwells second equation:

    2 2

    2 2

    1

    j

    j j

    j

    k j

    H J D

    A J A

    A A J A

    A A J A

    We can further specify the divergence of A according to

    Lorentzs gauge as:

    j A

    2 2k

  • 8/13/2019 01 Electromagnetic Radiation

    5/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    5

    Using Lorentzs gauge, we have:2 2k A A J

    Now, the first, the second, and the last Maxwells

    equations have been satisfied. To satisfy the third one,put into the third equation,j E A

    2 2

    j

    k

    D

    E

    A

  • 8/13/2019 01 Electromagnetic Radiation

    6/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    6

    A and are called vector and scalar potentials and theysatisfy the following inhomogeneous Helmholtz equations:

    2 2

    2 2

    2 2

    k

    k

    k

    A A J

    Note that each component ofA is governed by the same

    scalar equation as that for . Hence it suffices to solve

    only one scalar equation, namely, the inhomogeneous

    Helmholtz equation.

  • 8/13/2019 01 Electromagnetic Radiation

    7/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    7

    3. Solutions to the Vector and Scalar PotentialsSolutions to the vector and scalar potentials are (see

    Supplementary Notes):

    '

    '

    1 '4

    ( ) '4

    jkR

    v

    jkR

    v

    e' dvR

    e

    ' dvR

    R R

    A R J R

    R'R

    R

    R= field point

    R = source point

    R = |R-R|

  • 8/13/2019 01 Electromagnetic Radiation

    8/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    8

    1

    1

    j

    H A

    E H

    Once the potentials are known, the electric and magneticfields can be found from:

  • 8/13/2019 01 Electromagnetic Radiation

    9/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    9

    4. Hertzian Dipole (length

  • 8/13/2019 01 Electromagnetic Radiation

    10/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    10

    '''42

    2

    dzdydxR

    eAI

    x,y,z

    d

    d

    jkR

    A

    zA

    r

    zyx

    zzyyxx'R

    222

    222RR

    Here x = y = 0 & z 0

    (source at origin)

    Very short dipoleIndependent of primed coordinate!

    constant/ AIAzz zIJCurrent density:

  • 8/13/2019 01 Electromagnetic Radiation

    11/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    11

    A has only thezcomponent. ConvertAz to spherical (Ar,

    A,A) components first.

    0

    sin4

    sin

    cos4

    cos

    A

    reIdAA

    r

    eIdAA

    jkr

    z

    jkr

    zr

    Therefore:

    re

    Idzd

    r

    e

    Ix,y,z

    jkr

    d

    d

    jkr

    4

    4

    2

    2

    zzA

  • 8/13/2019 01 Electromagnetic Radiation

    12/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    12

    r

    e

    krjkr

    kIdjE

    r

    e

    jkrr

    IdE

    r

    e

    jkr

    jkIdH

    EHH

    jkr

    jkr

    r

    jkr

    r

    2

    2

    1114

    sin

    11

    2

    cos

    11

    4

    sin

    0

    E and H fields can now calculated and expressed inspherical coordinates as:

    1

    1

    j

    H A

    E H

  • 8/13/2019 01 Electromagnetic Radiation

    13/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    13

    Near fields: When kr

  • 8/13/2019 01 Electromagnetic Radiation

    14/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    14

    Far fields:

    (important case)

    When kr>> 1, all terms vary with the

    factors 1/r2 and 1/r3 vanish.

    r

    ekIdjH

    r

    ekIdjE

    jkr

    jkr

    sin4

    sin

    4

    Note that for far fields:

    1. Er=Hr=E = 0.

    2. E

    H

    and transverse to the rdirection, a TEM wave.

    3. BothE andH are in phase..4. In free space, the wave impedance =E/H is equal

    to 0, i.e., = 0 = 120 = 377.

  • 8/13/2019 01 Electromagnetic Radiation

    15/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    15

    Electric field lines surrounding a Hertzian dipole at a given instant

    See animation Far Field Electric 2D See animation Far Field Electric 3D

  • 8/13/2019 01 Electromagnetic Radiation

    16/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    16

    5. Half-Wave Dipole (length = 0.5

    )

    R

    Dipole

    R= r -zcos

    R

    r

    0forsin

    0forsinsin)(

    z'z'hkI

    z'z'hkIz'hkIz'I

    m

    m

    m

    Assumption: zI )(z'I

    h = /4

    Far Field point R

    (r,,)

    y

    x

    z

    z

    See Supplementary Notes

    for the exact derivation ofR.

  • 8/13/2019 01 Electromagnetic Radiation

    17/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    17

    That is, the current distribution is a sinusoidal function asshown below:

    I(z)

    z

    Im

    z'hkIz'I m sin)(

    0

  • 8/13/2019 01 Electromagnetic Radiation

    18/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    18

    For a half-wave dipole, the exact field solutions are toocomplicated. Hence only the far fields will be

    determined. The half-wave dipole can be considered as

    an assembly of many Hertzian dipoles joined together.The far fields of the half-wave dipole are then the

    summations of the far fields of the Hertizan dipoles.

    r

    edzIk

    jdE

    jkr

    z sin4

    )'(0'

    Far-zone electric field of a Hertzian dipole at the origin:

  • 8/13/2019 01 Electromagnetic Radiation

    19/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    19

    Far-zone electric field of a Hertzian dipole at an arbitraryposition R:

    R

    edzkI

    jdE

    jkR

    sin4

    )'(

    Far-zone electric field of a half-wave dipole:

    h

    h

    jkR

    h

    h

    jkR

    dR

    ezI

    kj

    dR

    ezkIjdEE

    )'(4

    sin

    sin4

    )'(

  • 8/13/2019 01 Electromagnetic Radiation

    20/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    20

    Now put in the current expression for I(z) and use the

    following substitutions forR (far-field approximation):

    cos'

    11

    jkzjkrjkR eee

    rR

    Note:R = r -zcos

    h

    jkzjkr

    m

    h

    h

    jkzjkr

    m

    dzezhkr

    ekIj

    dzezhkr

    ekIjE

    0

    cos'

    cos'

    ')'(sin24

    sin

    ')'(sin4

    sin

    We have,

  • 8/13/2019 01 Electromagnetic Radiation

    21/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    21

    The integration can be performed to yield the following

    result:

    60jkr

    m

    eE j I Fr

    EH

    sin

    cos2cos)( F

    where

  • 8/13/2019 01 Electromagnetic Radiation

    22/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    22

    6. Quarter-Wave Monopole

    Equivalent to

    (image theorem)

    h = /4

    h = /2

    Large conducting plane

  • 8/13/2019 01 Electromagnetic Radiation

    23/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    23

    6.1 Image Theorem

    For antennas mounted over or near a ground plane (a

    very large perfectly conducting plane), virtual

    sources (images) can be place below the groundplane to account for reflections from the ground

    plane. After introducing the image sources, the

    electromagnetic field above the ground plane can beconsidered as a sum of the electromagnetic fields

    due to the real sources (above the ground plane) and

    the image sources (below the ground plane), with the

    ground plane removed. This is the image theory.

  • 8/13/2019 01 Electromagnetic Radiation

    24/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    24

    Note that the image theory can only be applied to find

    the fields above the ground plane but not below the

    ground plane. Below the ground plane, the

    electromagnetic field is strictly zero.

    6.2 Method to place the image currents

    1. The image currents are at the same perpendicular

    distances (for example along the z axis) from theground plane as the real currents.

    2. The image currents have the same parallel

    coordinates (for example the x and y coordinates)as the real currents.

  • 8/13/2019 01 Electromagnetic Radiation

    25/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    25

    3. For vertical real currents, the image currents havethe same direction as the real currents. But for

    horizontal real currents, the image currents have

    the opposite directions as the real currents.

    z

    z

    z

    z

    real current real current

    image currrent image current

  • 8/13/2019 01 Electromagnetic Radiation

    26/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    26

    Using the image theorem, a /4 monopole antenna fed by

    a source at its base radiates the same far fields in the

    region above the ground plane as a /2 dipole antenna.

    But there is no radiation below the ground plane. This

    situation applies to other vertical wire antennas placed

    above a large conducting pane, such as a Hertzian dipole.

  • 8/13/2019 01 Electromagnetic Radiation

    27/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    27

    Example 1

    Find the maximum electric field intensity E of a half-wave

    dipole at a distance of 10 km from the dipole. What is the

    direction for maximum field intensity? Assume that thedipole carries a current whose maximum value is Im at the

    middle point of the dipole and the current varies at a

    frequency of 3 GHz.

    Solution

    For a half-wave dipole, the electric field intensity in the farfield region is:

  • 8/13/2019 01 Electromagnetic Radiation

    28/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    28

    sin

    cos2cos60

    reIjE

    jkr

    m

    It has only the component.

    This field is maximum when = /2.

    r

    eIjE

    jkr

    m 602/

    At 3 GHz, = 0.1 m, k= 2/= 20. Therefore at r= 10

    km,

    1000060

    200000

    2/

    j

    m

    eIjE

  • 8/13/2019 01 Electromagnetic Radiation

    29/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    29

    The variation ofE with time at r= 10 km is:

    2000001032sin10000

    60

    10000

    60Rekm10,

    9

    200000

    2/

    tI

    ee

    IjrtE

    m

    tjj

    m

  • 8/13/2019 01 Electromagnetic Radiation

    30/30

    Hon Tat Hui Electromagnetic Radiation

    NUS/ECE EE4101

    30

    References:

    1. David K. Cheng, Field and Wave Electromagnetic, Addison-

    Wesley Pub. Co., New York, 1989.

    2. John D. Kraus,Antennas, McGraw-Hill, New York, 1988.

    3. C. A. Balanis, Antenna Theory, Analysis and Design, John Wiley& Sons, Inc., New Jersey, 2005.

    4. W. L. Stutzman and G. A. Thiele, Antenna Theory and Design,

    Wiley, New York, 1998.

    5. Fawwaz T. Ulaby, Applied Electromagnetics, Prentice-Hall, Inc.,

    New Jersey, 2007.

    6. Joseph A. Edminister, Schaums Outline of Theory and Problems

    of Electromagnetics, McGraw-Hill, Singapore, 1993.7. Yung-kuo Lim (Editor), Problems and solutions on

    electromagnetism, World Scientific, Singapore, 1993.