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    RB IITG NPTEL

    Web CourseOn

    ELECTROMAGNETIC THEORY

    Ratnajit BhattacharjeeDepartment of ECE IIT Guwahati

    Guwahati- 781039

    Syllabus

    1 Mathematical Fundamentals

    Coordinate Systems and Transformations

    Vector Analysis

    Differential Length, Area and Volume

    Line, Surface and Volume Integrals

    Gradient, Divergence and Curl

    Divergence Theorem and Stokes Theorem

    2

    3

    Static Electric Fields

    Coulombs Law

    Electric Field & Electric Flux Density

    Gausss Law with Application

    Electrostatic Potential, Equipotential Surfaces

    Boundary Conditions for Static Electric Fields

    Capacitance and Capacitors

    Electrostatic Energy

    Laplaces and Poissons Equations

    Uniqueness of Electrostatic Solutions

    Method of Images

    Solution of Boundary Value Problems in Different

    Coordinate Systems.

    Steady Electric Currents

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    4

    Current Density and Ohms Law

    Electromotive Force and Kirchhoffs Voltage Law,

    Continuity Equation and Kirchhoffs Current Law

    Power Dissipation and Joules Law Boundary Conditions for Current Density.

    Static Magnetic Fields

    Biot-Savart Law and its Application

    Amperes Law and its Application

    Magnetic Dipole

    Behavior of Magnetic Materials

    Vector Magnetic Potential

    Magnetic Boundary Conditions

    Inductances and Inductors, Inductance Calculation for

    Common Geometries

    Energy Stored in a Magnetic Field.

    5 Time Varying Fields & Maxwells Equations

    Faradays law of Electromagnetic Induction

    Maxwells Equations

    Electromagnetic Boundary Conditions

    Wave Equations and Their Solutions

    Time Harmonic Fields.

    6 Electromagnetic Waves

    Plane Waves in Lossless Media

    Plane Waves in Lossy Media

    Poynting Vector and Power Flow in Electromagnetic

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    Field

    Skin Effect

    Wave Polarisation

    Normal and Oblique Incidence of Plane wave at a(i) Plane Conducting Boundary

    (ii) Plane Dielectric Boundary

    7 Fundamentals of Antennas and Radiating systems

    Fundamentals of Radiation

    Radiation Field of an Hertzian Dipole Basic Antenna Parameters like Directivity, Gain,

    Beamwidth, Radiation Resistance, Effective Aperture

    and Effective Height etc.

    Half-wave Dipole Antenna

    Quarter-wave Monopole Antenna

    Small-Loop Antennas

    Basics of Antenna Arrays

    .8 Introduction to Numerical Techniques in

    Electromagnetics

    Finite Difference Equivalent of Laplaces and Poissons

    Equation and Solution of Boundary-Value Problems.

    Basic Concepts of the Method of Moments

    Formulation of Integral Equations

    Application of Method of Moments to Wire Antennas

    and Scatterers.

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    CHAPTER-1

    1. Introduction

    Electromagnetic theory is a discipline concerned with the study ofcharges at rest and in motion. Electromagnetic principles arefundamental to the study of electrical engineering and physics.Electromagnetic theory is also indispensable to the understanding,analysis and design of various electrical, electromechanical andelectronic systems. Some of the branches of study whereelectromagnetic principles find application are:

    RF communicationMicrowave EngineeringAntennasElectrical MachinesSatellite CommunicationAtomic and nuclear researchRadar TechnologyRemote sensingEMI EMCQuantum ElectronicsVLSI

    Electromagnetic theory is a prerequisite for a wide spectrum of studiesin the field of Electrical Sciences and Physics. Electromagnetic theorycan be thought of as generalization of circuit theory. There are certainsituations that can be handled exclusively in terms of field theory. Inelectromagnetic theory, the quantities involved can be categorized assource quantities and field quantities. Source of electromagneticfield is electric charges: either at rest or in motion. However anelectromagnetic field may cause a redistribution of charges that in turnchange the field and hence the separation of cause and effect is notalways visible.

    Electric charge is a fundamental property of matter. Charge exist only inpositive or negative integral multiple of electronic charge, -e,

    191.60 10e = coulombs. [It may be noted here that in 1962, Murray Gell-Mann hypothesized Quarks as the basic building blocks of matters.Quarks were predicted to carry a fraction of electronic charge and theexistence of Quarks have been experimentally verified.] Principle ofconservation of charge states that the total charge (algebraic sum ofpositive and negative charges) of an isolated system remainsunchanged, though the charges may redistribute under the influence of

    electric field. Kirchhoffs Current Law (KCL) is an assertion of the

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    conservative property of charges under the implicit assumption thatthere is no accumulation of charge at the junction.

    Electromagnetic theory deals directly with the electric and magnetic fieldvectors where as circuit theory deals with the voltages and currents.

    Voltages and currents are integrated effects of electric and magneticfields respectively. Electromagnetic field problems involve three spacevariables along with the time variable and hence the solution tends tobecome correspondingly complex. Vector analysis is a mathematical toolwith which electromagnetic concepts are more conveniently expressedand best comprehended. Since use of vector analysis in the study ofelectromagnetic field theory results in real economy of time andthought, we first introduce the concept of vector analysis.

    2. Vector Analysis

    The quantities that we deal in electromagnetic theory may be eitherscalar or vectors [There are other class of physical quantities calledTensors: scalars and vectors are special cases]. Scalars are quantitiescharacterized by magnitude only and algebraic sign. A quantity that hasdirection as well as magnitude is called a vector. Both scalar and vectorquantities are function of time and position. A field is a function thatspecifies a particular quantity everywhere in a region. Depending uponthe nature of the quantity under consideration, the field may be a vectoror a scalar field. Example of scalar field is the electric potential in a

    region while electric or magnetic fields at any point is the example ofvector field.

    Fundamentals Vector Algebra:

    A vector is represented by a directed line segment: length of the line isproportional to magnitude and the orientation of the directed linesegment with respect to some reference gives the vector.

    A vector A can be written as A aA= , where A A= is the magnitude and

    A

    aA

    = is the unit vector which has unit magnitude and direction same as

    that ofA .

    Two vectors A and B are added together to give another vector C. We

    have:

    C A B= +

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    Figure 1: Vector addition

    Vector subtraction is similarly carried out as:

    ( )D A B A B= = +

    Figure 2: Vector subtraction

    Scaling of a vector is defined as C B= , where C is a scaled version ofvector B and is a scalar.

    Some important laws of vector algebra are:

    A B B A+ = + Commutative law

    ( ) ( )A B C A B C+ + = + + Associative law

    ( )A B A B + = + Distributive law

    The position vector Pr of a point P is the directed distance from theorigin (O ) to P i.e. Pr OP=

    r.

    Figure 3: Distant vector

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    If Pr OP=r

    and Qr OQ=r

    are the position vectors of the points P and Q

    then the distance vector Q PPQ OQ OP r r= = r r

    Product of Vectors

    When two vectors A and B are multiplied, the result is either a scalar ora vector depending how the two vectors were multiplied. The two typesof vector multiplication are:

    Scalar product (or dot product) A Bg gives a scalarVector product (or cross product) A B gives a vector

    The dot product between two vectors is defined as cos ABA B AB =g .

    Figure: Dot productThe dot product is commutative i.e. A B B A=g g and distributive i.e.

    ( )A B C A B A C+ = +g g g . Associative law does not apply to scalar product.

    The vector or cross product of two vectors A and B is denoted by A B .

    A B is a vector perpendicular to the plane containing

    Aand

    B, the

    magnitude is given by ABABSin and direction is given by right hand ruleas explained in Figure.

    Figure: Vector cross product

    n AB

    A B a ABSin = , where na is the unit vector given by

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    A Bn A B

    a

    = r r

    The following relations hold for vector product.

    A B B A = i.e. cross product is non commutative

    ( )A B C A B A C + = + i.e. cross product is distributive

    ( ) ( )A B C A B C i.e. cross product is non associative

    Scalar and vector triple product

    Scalar triple product ( ) ( ) ( )A B C B C A C A B = = g g g

    Vector triple product ( ) ( ) ( )A B C B A C C A B = g g

    3. COORDINATE SYSTEMS

    In order to describe the spatial variations of the quantities, we requireusing appropriate co-ordinate system. A point or vector can berepresented in a curvilinear coordinate system that may beorthogonal or non-orthogonal. An orthogonal system is one in whichthe co-ordinates are mutually perpendicular. Non-orthogonal co-ordinate

    systems are also possible, but their usage is very limited in practice.

    Let u =constant, v =constant and w =constant represent surfaces in aco-ordinate system, the surfaces may be curved surfaces in general.Further, let ua , va and wa be the unit vectors in the three co-ordinatedirections (base vectors). In a general right-handed orthogonalcurvilinear system, the vectors satisfy the following relations.

    u v w

    v w u

    w u v

    a a a

    a a a

    a a a

    =

    =

    =

    These equations are not independent and specification of one willautomatically imply the other two.Furthermore, the following relations hold

    . . . 0

    . . . 1

    u v v w w u

    u u v v w w

    a a a a a a

    a a a a a a

    = = =

    = = =

    A vector can be represented as sum of its orthogonal components

    u u v v w wA A a A a A a= + +

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    In general u ,v and w may not represent length. We multiply u ,v and w by conversion factors 1h , 2h and 3h respectively to convert differential

    changes du , dv and dw to corresponding changes in length 1dl , 2dl and

    3dl . Therefore

    1 2 3

    1 2 3

    u v w

    u v w

    dl a dl a dl a dl

    h dua h dva h dwa

    = + +

    = + +

    In the same manner, differential volume dv can be written as

    1 2 3dv h h h dudvdw= and differential area 1ds normal to ua is given by

    1 2 3ds dl dl = = 2 3h h dvdw and 1 2 3 uds h h dvdwa= . In the same manner, differential

    areas normal to unit vectors va and wa can be defined.

    In the following sections we discuss three most commonly used

    orthogonal co-ordinate systems, viz:

    1. Cartesian (or rectangular) co-ordinate system2. Cylindrical co-ordinate system3. Spherical polar co-ordinate system

    Cartesian Co-ordinate System

    In Cartesian co-ordinate system, we have, ( , , ) ( , , )u v w x y z = . A point

    0 0 0( , , )P x y z in Cartesian co-ordinate system is represented as intersection

    of three planes 0x x= , 0y y= and 0z z= . The unit vectors satisfies thefollowing relation:

    x y z

    y z x

    z x y

    a a a

    a a a

    a a a

    =

    =

    = . . . 0

    . . . 1

    x y y z z x

    x x y y z z

    a a a a a a

    a a a a a a

    = = =

    = = =

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    Figure: Cartesian coordinate system

    0 0 0

    x y zOP a x a y a z = + +

    In cartesian coordinate system, a vector A can be written as

    x x y y z zA a A a A a A= + + . The dot and cross product of two vectors A and B can be written as follows:

    ( ) ( ) ( )

    x x y y z z

    x y z z y y z x x z z x y y x

    x y z

    x y z

    x y z

    A B A B A B A B

    A B a A B A B a A B A B a A B A B

    a a a

    A A A

    B B B

    = + +

    = + +

    =

    gr r

    Since x , y and z all represent lengths, 1 2 3 1h h h= = = . The differentiallength, are and volume are defined respectively as

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    x y z

    x x

    y y

    z x

    dl dxa dya dza

    ds dydzads dxdza

    ds dxdya

    dv dxdydz

    = + +

    ==

    =

    =

    uur

    uur

    uur

    Cylindrical Co-ordinate System

    For cylindrical coordinate systems we have ( , , ) ( , , )u v w z = and a point

    0, 0 0( , )P z is determined as the point of intersection of a cylindrical

    surface 0 = , half plane containing the z-axis and making an angle

    0 = with the xz plane and a plane parallel to xy plane located at 0z z=

    as shown in figure.

    Fig.

    In cylindrical coordinate system, the unit vectors satisfy the followingrelations:

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    z

    z

    z

    a a a

    a a a

    a a a

    =

    =

    =A vector A can be written as z zA A a A a A a = + + .

    The differential length is defined as

    1 2 3 1, 1zdl a d d a dza h h h = + + = = =

    Differential volume element in cylindrical coordinates

    Differential areas are

    z z

    ds d dza

    ds d dza

    ds d d a

    =

    =

    =

    uuur

    uuur

    Differential volume dv d d dz =

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    Transformation between Cartesian and Cylindrical coordinates

    Let us consider a vector z zA a A a A a A = + + is to be expressed in

    Cartesian coordinates as x x y y z zA a A a A a A= + + . In doing so we note that

    ( )x x z z x

    A A a a A a A a A a = = + +g g and it applies for other components as

    well.

    Unit vectors in Cartesian and Cylindrical coordinates

    From the figure we note that:

    cos

    sin

    cos( ) sin2

    cos

    x

    y

    x

    y

    a a

    a a

    a a

    a a

    =

    =

    = + =

    =

    g

    g

    g

    g

    Therefore we can write

    cos sin

    sin cos

    x x

    y x

    z z z

    A A a A A

    A A a A A

    A A a A

    = =

    = = +

    = =

    gr

    gr

    g

    These relations can be put conveniently in the matrix form as:

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    cos sin 0

    sin cos 0

    0 0 1

    x

    y

    z z

    A A

    A A

    A A

    =

    A , zA and zA themselves may be functions of , and z. These

    variables are transformed in terms ofx , y and z as:

    cos

    sin

    x

    y

    z z

    =

    =

    =The inverse relation ships are:

    2 2

    1tan

    x y

    y

    x

    z z

    = +

    =

    =

    Thus we see that a vector in one coordinate system is transformed toanother coordinate system through two-step process: Finding thecomponent vectors and then variable transformation.

    Spherical polar coordinate

    For spherical polar coordinate system, we have, ( , , ) ( , , )u v w r = . A point

    0 0 0( , , )P r is represented as the intersection of

    (i) Spherical surface 0r r=

    (ii) Conical surface 0 = , and

    (iii) Half plane containing z-axis making angle 0 = with the xz

    plane as shown in the figure.

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    Figure:

    The unit vectors satisfy the following relations

    r

    r

    a a a

    a a a

    a a a

    =

    =

    =

    The orientation of the unit vectors are shown in the figure

    Figure:

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    A vector in spherical polar co-ordinate is written as:

    r rA A a A a A a = + + and sinrdl a dr a rd a r d = + + . For

    spherical polar coordinate system we have 1 1h = , 2 sinh r = and 3h r= .

    Figure:

    With reference to the Figure, the elemental areas are:

    2 sin

    sin

    r rds r d d a

    ds r drd a

    ds rdrd a

    =

    =

    =

    uuur

    uuur

    and elemental volume is given by2 sindv r drd d =

    Coordinate transformation between rectangular and sphericalpolar

    With reference to the Figure we can write the following:

    sin cos

    sin sin

    cos

    r x

    r y

    r z

    a a

    a a

    a a

    =

    =

    =

    g

    g

    g

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    cos cos

    cos sin

    cos( ) sin2

    x

    y

    z

    a a

    a a

    a a

    =

    =

    = + =

    g

    g

    g

    cos( ) sin2

    cos

    0

    x

    y

    z

    a a

    a a

    a a

    = + =

    =

    =

    g

    g

    g

    Figure

    Given a vector r rA A a A a A a = + + in the Spherical Polar coordinate

    system, its component in the Cartesian coordinate system can befound out as follows:

    . sin cos cos cos sinx x rA A a A A A = = +

    Similarly,

    . sin sin cos sin cosy y rA A a A A A = = + +

    . cos sinz z rA A a A A = = The above expressions may be put in a compact form:

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    sin cos cos cos sin

    sin sin cos sin cos

    cos sin 0

    Ax Ar

    Ay A

    Az A

    =

    The components rA ,A and A themselves will be function of r, and

    . r, and are related to x ,y and z as

    sin cos

    sin sin

    cos

    x r

    y r

    z r

    =

    =

    =and conversely,

    2 2 2

    1

    2 2 2

    1

    cos

    tan

    r x y z

    z

    x y z

    y

    x

    = + +

    =+ +

    =

    Using the variable transformation listed above, the vectorcomponents, which are functions of variables of one coordinatesystem, can be transformed to functions of variables of othercoordinate system and a total transformation can be done.

    Line, surface and volume integrals

    In electromagnetic theory we come across integrals, which containvector functions. Some representative integrals are listed below:

    VFdv C dl .CF dl .SF ds etc.

    In the above integrals, Fand respectively represent vector and

    scalar function of space coordinates. , &C S V represent path, surface

    and volume of integration. All these integrals are evaluated usingextension of the usual one-dimensional integral as the limit of a sum,

    i.e., if a function ( )f x is defined over arrange a to b of values of x,

    then the integral is given by

    1

    ( )b n

    i i

    ia

    Limf x dx f x

    n

    =

    =

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    where the interval ( , )a b is subdivided into n continuous interval of

    lengths 1........... nx x .

    Line integral

    Line integral.

    C

    E dl is the dot product of a vector with a specifiedpath C; in other words it is the integral of the tangential component

    ofE along the curve C.

    Figure: Line integral

    As shown in the figure, given a vector field Earound C, we define

    the integral cosb

    aC

    E dl E dl= r

    g as the line integral of E along the

    curve C. If the path of integration is a closed path as shown inFigure, the line integral becomes a closed line integral and is called

    the circulation ofE around C and denoted asC

    E dl g

    Figure: Closed line integral

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    Surface integral

    Given a vector field A , continuous in a region containing the smooth

    surface S, we define the surface integral or the flux of A through S

    as

    cos nS S S

    A ds A a ds A ds = = = g g

    Figure: Computation of surface integral

    If the surface integral is carried out over a closed surface, then we

    write:S

    A ds = g which gives the net outward flux of A from S.Volume integrals

    We defineV

    fdv orv

    fdv as the volume integral of the scalar function f(function of spatial coordinates) over the volume V . Evaluation of

    integral of the formV

    Fdv can be carried out as a sum of three scalarvolume integrals, where each scalar volume integral is a component of

    the vector F.

    The Del Operator

    The vector differential operator was introduced by Sir W. R. Hamiltonand later on developed by P. G. Tait.

    Mathematically the vector differential operator can be written in thegeneral form as:

    1 2 3

    1 1 1

    u v wa a ah u h v h w

    = + +

    In Cartesian coordinates:

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    x y za a a

    x y z

    = + +

    In cylindrical coordinates:

    1

    za a az

    = + +

    and in spherical polar coordinates:

    1 1 sin

    ra a ar r r

    = + +

    Gradient of a Scalar