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TRANSCRIPT
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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