LECTURES ON
ELECTROMAGNETIC WAVES
AND WAVE PROPAGATION
Assoc. Prof. Yasser Mahmoud Madany
Senior Member, IEEE
URSI Senior Member
Founder and Chair of the IEEE Egypt AP-S/MTT-S Joint Chapter
Founder and Counselor of the IEEE AL Ryada Student Branch
PART ONE
Maxwell’s Equations and
Electromagnetic Waves
INTRODUCTION
❑ Static electric field has applications in:
❖ Cathode ray oscilloscopes for deflecting
charged particles.
❖ Ink jet printers to increase the speed of printing
and improve print quality.
❑ Static magnetic field has applications in:
❖ Magnetic separators to separate magnetic
materials from non-magnetic materials.
❖ Cyclotrons for imparting high energy to charged
particles.
INTRODUCTION
❑ Time-varying fields constitute electromagnetic (EM) waves
which have wide applications in all the communications,
radars and also in Bio-medical engineering.
❑ EM waves are produced by time-varying currents.
❑ In brief, it may be noted that:
❖ Static charges produce electrostatic fields.
❖ Steady currents (DC currents) produce magneto-static
fields.
❖ Static magnetic charges (magnetic dipoles) also
produce magneto-static fields.
❖ Time-varying currents produce EM waves or EM fields.
THE FIELDS ഥ
𝑬, ഥ
𝑯, ഥ
𝑫 AND ഥ
𝑩 IN STATIC FORM
Coordinate
/ Field
Cartesian Cylindrical Spherical
Cartesian
Time-
varying
Electric
Field, ഥ
𝑬
ഥ
𝑬(𝒙, 𝒚, 𝒛) ഥ
𝑬(𝝆, ∅, 𝒛) ഥ
𝑬(𝒓, 𝜽, ∅) ഥ
𝑬(𝒕, 𝒙, 𝒚, 𝒛)
Magnetic
Field, ഥ
𝑯
ഥ
𝑯(𝒙, 𝒚, 𝒛) ഥ
𝑯(𝝆, ∅, 𝒛) ഥ
𝑯(𝒓, 𝜽, ∅) ഥ
𝑯(𝒕, 𝒙, 𝒚, 𝒛)
Electric Flux
Density, ഥ
𝑫
ഥ
𝑫(𝒙, 𝒚, 𝒛) ഥ
𝑫(𝝆, ∅, 𝒛) ഥ
𝑫(𝒓, 𝜽, ∅) ഥ
𝑫(𝒕, 𝒙, 𝒚, 𝒛)
Magnetic
Flux Density,
ഥ
𝑩
ഥ
𝑩(𝒙, 𝒚, 𝒛) ഥ
𝑩(𝝆, ∅, 𝒛) ഥ
𝑩(𝒓, 𝜽, ∅) ഥ
𝑩(𝒕, 𝒙, 𝒚, 𝒛)
EQUATION OF CONTINUITY FOR TIME-VARYING
FIELDS
❑ Consider a closed surface enclosing a charge 𝑸 and
there exists an outward flow of current given by
𝑰 = ර
𝒔
ҧ
𝑱. 𝒅ത
𝒔
❑ The previous equation known as equation of continuity in
integral form, where
𝑰 is the current flowing away through a closed surface
(A).
ҧ
𝑱 is the conduction current density (A/m2).
𝒅ത
𝒔 is the differential area on the surface whose direction
is always outward and normal to the surface.
❑ As there is outward flow of current, there will be a
decrease the rate of charge of which is given by
𝑰 =
−𝒅𝑸
𝒅𝒕
where 𝑸 is the enclosed charge (C).
❑ From the principle of conservative of charge, we have
𝑰 = ර
𝒔
ҧ
𝑱. 𝒅ത
𝒔 =
−𝒅𝑸
𝒅𝒕
❑ From divergence theorem, we have
ර
𝒔
ҧ
𝑱. 𝒅ത
𝒔 = න
𝒗
𝛁. ҧ
𝑱 𝒅𝒗
❑ Hence,
න
𝒗
𝛁. ҧ
𝑱 𝒅𝒗 =
−𝒅𝑸
𝒅𝒕
❑ By definition,
𝑸 = න
𝒗
𝝆𝒗 𝒅𝒗
where 𝝆𝒗 is the volume charge density (C/m3).
❑ So,
න
𝒗
𝛁. ҧ
𝑱 𝒅𝒗 = න
𝒗
−𝝏𝝆𝒗
𝝏𝒕
𝒅𝒗 = න
𝒗
− ሶ
𝝆𝒗 𝒅𝒗
❑ Two volume integrals are equal only if their integrands are
equal. So, the equation of continuity in point form is
𝛁 ∙ ҧ
𝑱 =
−𝝏𝝆𝒗
𝝏𝒕
= − ሶ
𝝆𝒗
MAXWELL’S EQUATIONS FOR TIME-VARYING
FIELDS
❑ Maxwell’s equations in differential form are given by
𝛁 × ഥ
𝑯 =
𝝏ഥ
𝑫
𝝏𝒕
+ ҧ
𝒋 = ሶ
ഥ
𝑫 + ҧ
𝒋 (1)
𝛁 × ഥ
𝑬 =
−𝝏ഥ
𝑩
𝝏𝒕
= − ሶ
ഥ
𝑩 (2)
𝛁 ∙ ഥ
𝑫 = 𝝆𝒗 (3)
𝛁 ∙ ഥ
𝑩 = 𝟎 (4)
where
ഥ
𝑯 is the magnetic field strength (A/m).
ഥ
𝑫 is the electric flux density (C/m2).
MAXWELL’S EQUATIONS FOR TIME-VARYING
FIELDS
where:
ሶ
ഥ
𝑫 =
𝝏ഥ
𝑫
𝝏𝒕
is the displacement electric current density (A/m2).
ҧ
𝑱 is the conduction current density (A/m2).
ഥ
𝑬 is the electric field strength (V/m).
ഥ
𝑩 is the magnetic flux density (wb/m2) or (Tesla).
ሶ
ഥ
𝑩 =
𝝏ഥ
𝑩
𝝏𝒕
is the time-derivative of magnetic flux density (wb/m2
. sec). Also,
ሶ
ഥ
𝑩 is the magnetic current density (V/m2) or (Tesla/sec).
𝝆𝒗 is the volume charge density (C/m3)
MAXWELL’S EQUATIONS FOR TIME-VARYING
FIELDS
❑ Maxwell’s equations in integral form are given by
‫ׯ‬
𝑳
ഥ
𝑯. 𝒅ഥ
𝑳 = ‫ׯ‬
𝒔
ሶ
ഥ
𝑫 + ҧ
𝒋 . 𝒅ത
𝒔 (1)
‫ׯ‬
𝑳
ഥ
𝑬. 𝒅ഥ
𝑳 = − ‫ׯ‬
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔 (2)
‫ׯ‬
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = ‫׬‬
𝒗
𝝆𝒗 𝒅𝒗 (3)
‫ׯ‬
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎 (4)
where
𝒅ഥ
𝑳 is the differential length.
𝒅ത
𝒔 is the differential surface area whose direction is always
outward and normal to the surface.
CONVERSION OF DIFFERENTIAL FORM OF
MAXWELL’S EQUATIONS TO INTEGRAL FORM
❑ Consider the first Maxwell’s equation
𝛁 × ഥ
𝑯 = ሶ
ഥ
𝑫 + ҧ
𝒋
❑ Take surface integral on both sides
‫ׯ‬
𝒔
𝛁 × ഥ
𝑯 . 𝒅ത
𝒔 = ‫ׯ‬
𝒔
ሶ
ഥ
𝑫 + ҧ
𝒋 . 𝒅ത
𝒔
❑ Applying Stokes’ theorem, we can write
ර
𝒔
𝛁 × ഥ
𝑯 . 𝒅ത
𝒔 = ර
𝑳
ഥ
𝑯. 𝒅ത
𝑳
❑ Therefore, the first low
ර
𝑳
ഥ
𝑯. 𝒅ത
𝑳 = ර
𝒔
ሶ
ഥ
𝑫 + ҧ
𝒋 . 𝒅ത
𝒔
❑ Consider the second Maxwell’s equation
𝛁 × ഥ
𝑬 = − ሶ
ഥ
𝑩
❑ Take surface integral on both sides
‫ׯ‬
𝒔
𝛁 × ഥ
𝑬 . 𝒅ത
𝒔 = − ‫ׯ‬
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔
❑ Applying Stokes’ theorem, we can write
ර
𝒔
𝛁 × ഥ
𝑬 . 𝒅ത
𝒔 = ර
𝑳
ഥ
𝑬. 𝒅ത
𝑳
❑ Therefore, the second low
ර
𝑳
ഥ
𝑬. 𝒅ത
𝑳 = − ර
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔
❑ Consider the third Maxwell’s equation
𝛁 ∙ ഥ
𝑫 = 𝝆𝒗
❑ Take volume integral on both sides
න
𝒗
𝛁 ∙ ഥ
𝑫 𝒅𝒗 = න
𝒗
𝝆𝒗 𝒅𝒗
❑ Applying divergence theorem, we can write
න
𝒗
𝛁 ∙ ഥ
𝑫 𝒅𝒗 = ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔
❑ Therefore, the third low
ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = න
𝒗
𝝆𝒗 𝒅𝒗
❑ Consider the fourth Maxwell’s equation
𝛁 ∙ ഥ
𝑩 = 𝟎
❑ Take volume integral on both sides
න
𝒗
𝛁 ∙ ഥ
𝑩 𝒅𝒗 = 𝟎
❑ Applying divergence theorem, we can write
න
𝒗
𝛁 ∙ ഥ
𝑩 𝒅𝒗 = ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔
❑ Therefore, the fourth low
ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎
MAXWELL’S EQUATIONS FOR STATIC FIELDS
𝛁 × ഥ
𝑯 = ҧ
𝒋
⇔ ර
𝑳
ഥ
𝑯. 𝒅ത
𝑳 = ර
𝒔
ҧ
𝒋. 𝒅ത
𝒔
𝛁 × ഥ
𝑬 = 𝟎 ⇔ ර
𝑳
ഥ
𝑬. 𝒅ത
𝑳 = 𝟎
𝛁 ∙ ഥ
𝑫 = 𝝆𝒗 ⇔ ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = න
𝒗
𝝆𝒗 𝒅𝒗
𝛁 ∙ ഥ
𝑩 = 𝟎 ⇔ ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎
CHARACTERISTICS OF FREE SPACE
Parameter Symbol Value
Relative permittivity 𝜺𝒓 1
Relative permeability 𝝁𝒓 1
Conductivity 𝝈 0
Conduction current density ҧ
𝑱 0
Volume charge density 𝝆𝒗 0
Intrinsic or characteristic
impedance
𝜼 𝟏𝟐𝟎 𝝅 𝑶𝑹 𝟑𝟕𝟕
MAXWELL’S EQUATIONS FOR FREE SPACE
𝛁 × ഥ
𝑯 = ሶ
ഥ
𝑫 ⇔ ර
𝑳
ഥ
𝑯. 𝒅ത
𝑳 = ර
𝒔
ሶ
ഥ
𝑫. 𝒅ത
𝒔
𝛁 × ഥ
𝑬 = − ሶ
ഥ
𝑩 ⇔ ර
𝑳
ഥ
𝑬. 𝒅ത
𝑳 = − ර
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔
𝛁 ∙ ഥ
𝑫 = 𝟎 ⇔ ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = 𝟎
𝛁 ∙ ഥ
𝑩 = 𝟎 ⇔ ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎
MAXWELL’S EQUATIONS FOR STATIC FIELDS IN
FREE SPACE
𝛁 × ഥ
𝑯 = 𝟎
⇔ ර
𝑳
ഥ
𝑯. 𝒅ത
𝑳 = 𝟎
𝛁 × ഥ
𝑬 = 𝟎 ⇔ ර
𝑳
ഥ
𝑬. 𝒅ത
𝑳 = 𝟎
𝛁 ∙ ഥ
𝑫 = 𝟎 ⇔ ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = 𝟎
𝛁 ∙ ഥ
𝑩 = 𝟎 ⇔ ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎
PROOF OF MAXWELL’S EQUATIONS
❑ First, from Ampere’s circuital law , we have
𝛁 × ഥ
𝑯 = ҧ
𝒋
❑ Take dot product on both sides
𝛁. 𝛁 × ഥ
𝑯 = 𝛁. ҧ
𝒋
❑ As the divergence of curl of a vector is zero,
𝛁. ҧ
𝒋 = 𝟎
❑ But the equation of continuity in point form
𝛁 ∙ ҧ
𝑱 =
−𝝏𝝆𝒗
𝝏𝒕
= − ሶ
𝝆𝒗
❑ This means that if 𝛁 × ഥ
𝑯 = ҧ
𝒋 is true, we get 𝛁. ҧ
𝒋 = 𝟎.
❑ As the equation of continuity is more fundamental, Ampere’s
circuital law should be modified.
❑ Modifying Ampere’s circuital law , we have
𝛁 × ഥ
𝑯 = ҧ
𝒋 + ഥ
𝑭
❑ Take dot product on both sides
𝛁. 𝛁 × ഥ
𝑯 = 𝛁. ҧ
𝒋 + 𝛁. ഥ
𝑭
❑ As the divergence of curl of a vector is zero,
𝛁. ҧ
𝒋 + 𝛁. ഥ
𝑭 = 𝟎
❑ Substituting the value of 𝛁. ҧ
𝒋 from the equation of
continuity in the previous equation,
𝛁 ∙ ഥ
𝑭 + − ሶ
𝝆𝒗 = 𝟎 OR 𝛁 ∙ ഥ
𝑭 = ሶ
𝝆𝒗
❑ But the point form of Gauss’s law
𝛁. ഥ
𝑫 = 𝝆𝒗 OR 𝛁. ሶ
ഥ
𝑫 = ሶ
𝝆𝒗
❑ Then,
𝛁. ഥ
𝑭 = 𝛁. ሶ
ഥ
𝑫
❑ The divergence of two vectors are equal only if the
vectors are identical.
ഥ
𝑭 = ሶ
ഥ
𝑫
❑ Substituting the value of ഥ
𝑭,
𝛁 × ഥ
𝑯 = ሶ
ഥ
𝑫 + ҧ
𝒋
❑ Second, according to Faraday’s law
𝒆𝒎𝒇 = −
𝒅∅
𝒅𝒕
, ∅ ∶ 𝒎𝒂𝒈𝒏𝒆𝒕𝒊𝒄 𝒇𝒍𝒖𝒙 𝒊𝒏 𝒘𝒃
❑ By definition,
𝒆𝒎𝒇 = ර
𝑳
ഥ
𝑬. 𝒅ഥ
𝑳
❑ Then,
ර
𝑳
ഥ
𝑬. 𝒅ഥ
𝑳 = −
𝒅∅
𝒅𝒕
❑ But,
∅ = ‫ׯ‬
𝒔
ഥ
𝑩. 𝒅ത
𝒔 OR −
𝒅∅
𝒅𝒕
= − ‫ׯ‬
𝒔
𝝏ഥ
𝑩
𝝏𝒕
. 𝒅ത
𝒔
❑ So,
ර
𝑳
ഥ
𝑬. 𝒅ഥ
𝑳 = − ර
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔
❑ Applying Stokes’ theorem, we get
ර
𝒔
𝛁 × ഥ
𝑬 . 𝒅ത
𝒔 = ර
𝑳
ഥ
𝑬. 𝒅ഥ
𝑳
❑ Hence,
ර
𝒔
𝛁 × ഥ
𝑬 . 𝒅ത
𝒔 = − ර
𝒔
ሶ
ഥ
𝑩. 𝒅ത
𝒔
❑ Two surface integrals are equal only if their integrands are
equal,
𝛁 × ഥ
𝑬 = − ሶ
ഥ
𝑩
❑ Third, from Gauss’s law in electric field
‫ׯ‬
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = 𝑸 = ‫׬‬𝒗
𝝆𝒗 𝒅𝒗
❑ Applying divergence theorem, we get
ර
𝒔
ഥ
𝑫. 𝒅ത
𝒔 = න
𝒗
𝛁 ∙ ഥ
𝑫 𝒅𝒗 = න
𝒗
𝝆𝒗 𝒅𝒗
❑ Two volume integrals are equal only if their integrands are
equal,
𝛁 ∙ ഥ
𝑫 = 𝝆𝒗
❑ Fourth, from Gauss’s law for magnetic field [the magnetic flux
lines are a closed loop]
ර
𝒔
ഥ
𝑩. 𝒅ത
𝒔 = 𝟎
❑ Applying divergence theorem, we get
‫׬‬𝒗
𝛁 ∙ ഥ
𝑩 𝒅𝒗 = 𝟎 OR 𝛁 ∙ ഥ
𝑩 = 𝟎
SINUSOIDAL TIME-VARYING FIELDS
❑ In practice, electric and magnetic fields vary
sinusoidally.
❑ Any periodic variation can be described in terms of
sinusoidal variations.
❑ The fields can be represented by
෩
ഥ
𝑬 = 𝑬𝒎 𝐜𝐨𝐬 𝝎𝒕 OR ෩
ഥ
𝑬 = 𝑬𝒎 𝒄𝒐𝒔 𝝎𝒕
where
𝝎 : Angular frequency, 𝝎 = 𝟐𝝅𝒇
𝒇 : Frequency variation of the field.
𝑬𝒎 : The maximum field strength.
❑ It is also possible to represent the fields using the
phasor notation.
❑ The time-varying field ෩
ഥ
𝑬(𝒓, 𝒕) is related to phasor field
ഥ
𝑬(𝒓) as
෩
ഥ
𝑬(𝒓, 𝒕) = 𝑹𝒆 ഥ
𝑬 𝒓 𝒆𝒋𝝎𝒕
OR
෩
ഥ
𝑬(𝒓, 𝒕) = 𝑰𝒎 ഥ
𝑬 𝒓 𝒆𝒋𝝎𝒕
where
𝝎 : Angular frequency.
MAXWELL’S EQUATIONS IN PHASOR FORM
❑ Consider the first Maxwell’s equation
𝛁 × ෩
ഥ
𝑯 =
෩ሶ
ഥ
𝑫 + ሚҧ
𝒋
❑ If
෩
ഥ
𝑯 = 𝑹𝒆 ഥ
𝑯𝒆𝒋𝝎𝒕
෩
ഥ
𝑫 = 𝑹𝒆 ഥ
𝑫𝒆𝒋𝝎𝒕
෨ҧ
𝑱 = 𝑹𝒆 ҧ
𝑱𝒆𝒋𝝎𝒕
Then
𝛁 × 𝑹𝒆 ഥ
𝑯𝒆𝒋𝝎𝒕
=
𝝏
𝝏𝒕
𝑹𝒆 ഥ
𝑫𝒆𝒋𝝎𝒕
+ 𝑹𝒆 ҧ
𝑱𝒆𝒋𝝎𝒕
❑ Interchanging the operation of taking the real part, we get
𝑹𝒆 𝛁 × ഥ
𝑯 − 𝒋𝝎ഥ
𝑫 − ҧ
𝑱 𝒆𝒋𝝎𝒕 = 𝟎
∴ 𝛁 × ഥ
𝑯 = 𝒋𝝎ഥ
𝑫 + ҧ
𝑱
❑ Consider the second Maxwell’s equation
𝛁 × ෩
ഥ
𝑬 = −
෩ሶ
ഥ
𝑩
❑ If
෩
ഥ
𝑬 = 𝑹𝒆 ഥ
𝑬𝒆𝒋𝝎𝒕
෩
ഥ
𝑩 = 𝑹𝒆 ഥ
𝑩𝒆𝒋𝝎𝒕
❑ Then
𝛁 × 𝑹𝒆 ഥ
𝑬𝒆𝒋𝝎𝒕 = −
𝝏
𝝏𝒕
𝑹𝒆 ഥ
𝑩𝒆𝒋𝝎𝒕
❑ Interchanging the operation of taking the real part, we
get
𝑹𝒆 𝛁 × ഥ
𝑬 + 𝒋𝝎ഥ
𝑩 𝒆𝒋𝝎𝒕 = 𝟎
∴ 𝛁 × ഥ
𝑬 = −𝒋𝝎ഥ
𝑩
❑ Consider the third Maxwell’s equation
𝛁 ∙ ෩
ഥ
𝑫 = 𝝆𝒗
❑ If
෩
ഥ
𝑫 = 𝑹𝒆 ഥ
𝑫𝒆𝒋𝝎𝒕
❑ Then
𝛁 ∙ 𝑹𝒆 ഥ
𝑫𝒆𝒋𝝎𝒕 = 𝝆𝒗
❑ Interchanging the operation of taking the real part, we
get
𝑹𝒆 𝛁 ∙ ഥ
𝑫 𝒆𝒋𝝎𝒕 = 𝝆𝒗
∴ 𝛁 ∙ ഥ
𝑫 = 𝝆𝒗
❑ Consider the fourth Maxwell’s equation
𝛁 ∙ ෩
ഥ
𝑩 = 𝟎
❑ If
෩
ഥ
𝑩 = 𝑹𝒆 ഥ
𝑩𝒆𝒋𝝎𝒕
❑ Then
𝛁 ∙ 𝑹𝒆 ഥ
𝑩𝒆𝒋𝝎𝒕 = 𝟎
❑ Interchanging the operation of taking the real part, we
get
𝑹𝒆 𝛁 ∙ ഥ
𝑩 𝒆𝒋𝝎𝒕 = 𝟎
∴ 𝛁 ∙ ഥ
𝑩 = 𝟎
❑ In summary, Maxwell’s equations in phasor form are
as follows:
𝛁 × ഥ
𝑯 = 𝒋𝝎ഥ
𝑫 + ҧ
𝑱
𝛁 × ഥ
𝑬 = −𝒋𝝎ഥ
𝑩
𝛁 ∙ ഥ
𝑫 = 𝝆𝒗
𝛁 ∙ ഥ
𝑩 = 𝟎
The Part (1) will be
continued …
Thanks

2_Electromagnetic waves and propagation Lectures_part1_1.pdf

  • 1.
    LECTURES ON ELECTROMAGNETIC WAVES ANDWAVE PROPAGATION Assoc. Prof. Yasser Mahmoud Madany Senior Member, IEEE URSI Senior Member Founder and Chair of the IEEE Egypt AP-S/MTT-S Joint Chapter Founder and Counselor of the IEEE AL Ryada Student Branch
  • 2.
    PART ONE Maxwell’s Equationsand Electromagnetic Waves
  • 3.
    INTRODUCTION ❑ Static electricfield has applications in: ❖ Cathode ray oscilloscopes for deflecting charged particles. ❖ Ink jet printers to increase the speed of printing and improve print quality. ❑ Static magnetic field has applications in: ❖ Magnetic separators to separate magnetic materials from non-magnetic materials. ❖ Cyclotrons for imparting high energy to charged particles.
  • 4.
    INTRODUCTION ❑ Time-varying fieldsconstitute electromagnetic (EM) waves which have wide applications in all the communications, radars and also in Bio-medical engineering. ❑ EM waves are produced by time-varying currents. ❑ In brief, it may be noted that: ❖ Static charges produce electrostatic fields. ❖ Steady currents (DC currents) produce magneto-static fields. ❖ Static magnetic charges (magnetic dipoles) also produce magneto-static fields. ❖ Time-varying currents produce EM waves or EM fields.
  • 5.
    THE FIELDS ഥ 𝑬,ഥ 𝑯, ഥ 𝑫 AND ഥ 𝑩 IN STATIC FORM Coordinate / Field Cartesian Cylindrical Spherical Cartesian Time- varying Electric Field, ഥ 𝑬 ഥ 𝑬(𝒙, 𝒚, 𝒛) ഥ 𝑬(𝝆, ∅, 𝒛) ഥ 𝑬(𝒓, 𝜽, ∅) ഥ 𝑬(𝒕, 𝒙, 𝒚, 𝒛) Magnetic Field, ഥ 𝑯 ഥ 𝑯(𝒙, 𝒚, 𝒛) ഥ 𝑯(𝝆, ∅, 𝒛) ഥ 𝑯(𝒓, 𝜽, ∅) ഥ 𝑯(𝒕, 𝒙, 𝒚, 𝒛) Electric Flux Density, ഥ 𝑫 ഥ 𝑫(𝒙, 𝒚, 𝒛) ഥ 𝑫(𝝆, ∅, 𝒛) ഥ 𝑫(𝒓, 𝜽, ∅) ഥ 𝑫(𝒕, 𝒙, 𝒚, 𝒛) Magnetic Flux Density, ഥ 𝑩 ഥ 𝑩(𝒙, 𝒚, 𝒛) ഥ 𝑩(𝝆, ∅, 𝒛) ഥ 𝑩(𝒓, 𝜽, ∅) ഥ 𝑩(𝒕, 𝒙, 𝒚, 𝒛)
  • 6.
    EQUATION OF CONTINUITYFOR TIME-VARYING FIELDS ❑ Consider a closed surface enclosing a charge 𝑸 and there exists an outward flow of current given by 𝑰 = ර 𝒔 ҧ 𝑱. 𝒅ത 𝒔 ❑ The previous equation known as equation of continuity in integral form, where 𝑰 is the current flowing away through a closed surface (A). ҧ 𝑱 is the conduction current density (A/m2). 𝒅ത 𝒔 is the differential area on the surface whose direction is always outward and normal to the surface.
  • 7.
    ❑ As thereis outward flow of current, there will be a decrease the rate of charge of which is given by 𝑰 = −𝒅𝑸 𝒅𝒕 where 𝑸 is the enclosed charge (C). ❑ From the principle of conservative of charge, we have 𝑰 = ර 𝒔 ҧ 𝑱. 𝒅ത 𝒔 = −𝒅𝑸 𝒅𝒕 ❑ From divergence theorem, we have ර 𝒔 ҧ 𝑱. 𝒅ത 𝒔 = න 𝒗 𝛁. ҧ 𝑱 𝒅𝒗
  • 8.
    ❑ Hence, න 𝒗 𝛁. ҧ 𝑱𝒅𝒗 = −𝒅𝑸 𝒅𝒕 ❑ By definition, 𝑸 = න 𝒗 𝝆𝒗 𝒅𝒗 where 𝝆𝒗 is the volume charge density (C/m3). ❑ So, න 𝒗 𝛁. ҧ 𝑱 𝒅𝒗 = න 𝒗 −𝝏𝝆𝒗 𝝏𝒕 𝒅𝒗 = න 𝒗 − ሶ 𝝆𝒗 𝒅𝒗 ❑ Two volume integrals are equal only if their integrands are equal. So, the equation of continuity in point form is 𝛁 ∙ ҧ 𝑱 = −𝝏𝝆𝒗 𝝏𝒕 = − ሶ 𝝆𝒗
  • 9.
    MAXWELL’S EQUATIONS FORTIME-VARYING FIELDS ❑ Maxwell’s equations in differential form are given by 𝛁 × ഥ 𝑯 = 𝝏ഥ 𝑫 𝝏𝒕 + ҧ 𝒋 = ሶ ഥ 𝑫 + ҧ 𝒋 (1) 𝛁 × ഥ 𝑬 = −𝝏ഥ 𝑩 𝝏𝒕 = − ሶ ഥ 𝑩 (2) 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗 (3) 𝛁 ∙ ഥ 𝑩 = 𝟎 (4) where ഥ 𝑯 is the magnetic field strength (A/m). ഥ 𝑫 is the electric flux density (C/m2).
  • 10.
    MAXWELL’S EQUATIONS FORTIME-VARYING FIELDS where: ሶ ഥ 𝑫 = 𝝏ഥ 𝑫 𝝏𝒕 is the displacement electric current density (A/m2). ҧ 𝑱 is the conduction current density (A/m2). ഥ 𝑬 is the electric field strength (V/m). ഥ 𝑩 is the magnetic flux density (wb/m2) or (Tesla). ሶ ഥ 𝑩 = 𝝏ഥ 𝑩 𝝏𝒕 is the time-derivative of magnetic flux density (wb/m2 . sec). Also, ሶ ഥ 𝑩 is the magnetic current density (V/m2) or (Tesla/sec). 𝝆𝒗 is the volume charge density (C/m3)
  • 11.
    MAXWELL’S EQUATIONS FORTIME-VARYING FIELDS ❑ Maxwell’s equations in integral form are given by ‫ׯ‬ 𝑳 ഥ 𝑯. 𝒅ഥ 𝑳 = ‫ׯ‬ 𝒔 ሶ ഥ 𝑫 + ҧ 𝒋 . 𝒅ത 𝒔 (1) ‫ׯ‬ 𝑳 ഥ 𝑬. 𝒅ഥ 𝑳 = − ‫ׯ‬ 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔 (2) ‫ׯ‬ 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = ‫׬‬ 𝒗 𝝆𝒗 𝒅𝒗 (3) ‫ׯ‬ 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎 (4) where 𝒅ഥ 𝑳 is the differential length. 𝒅ത 𝒔 is the differential surface area whose direction is always outward and normal to the surface.
  • 12.
    CONVERSION OF DIFFERENTIALFORM OF MAXWELL’S EQUATIONS TO INTEGRAL FORM ❑ Consider the first Maxwell’s equation 𝛁 × ഥ 𝑯 = ሶ ഥ 𝑫 + ҧ 𝒋 ❑ Take surface integral on both sides ‫ׯ‬ 𝒔 𝛁 × ഥ 𝑯 . 𝒅ത 𝒔 = ‫ׯ‬ 𝒔 ሶ ഥ 𝑫 + ҧ 𝒋 . 𝒅ത 𝒔 ❑ Applying Stokes’ theorem, we can write ර 𝒔 𝛁 × ഥ 𝑯 . 𝒅ത 𝒔 = ර 𝑳 ഥ 𝑯. 𝒅ത 𝑳 ❑ Therefore, the first low ර 𝑳 ഥ 𝑯. 𝒅ത 𝑳 = ර 𝒔 ሶ ഥ 𝑫 + ҧ 𝒋 . 𝒅ത 𝒔
  • 13.
    ❑ Consider thesecond Maxwell’s equation 𝛁 × ഥ 𝑬 = − ሶ ഥ 𝑩 ❑ Take surface integral on both sides ‫ׯ‬ 𝒔 𝛁 × ഥ 𝑬 . 𝒅ത 𝒔 = − ‫ׯ‬ 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔 ❑ Applying Stokes’ theorem, we can write ර 𝒔 𝛁 × ഥ 𝑬 . 𝒅ത 𝒔 = ර 𝑳 ഥ 𝑬. 𝒅ത 𝑳 ❑ Therefore, the second low ර 𝑳 ഥ 𝑬. 𝒅ത 𝑳 = − ර 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔
  • 14.
    ❑ Consider thethird Maxwell’s equation 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗 ❑ Take volume integral on both sides න 𝒗 𝛁 ∙ ഥ 𝑫 𝒅𝒗 = න 𝒗 𝝆𝒗 𝒅𝒗 ❑ Applying divergence theorem, we can write න 𝒗 𝛁 ∙ ഥ 𝑫 𝒅𝒗 = ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 ❑ Therefore, the third low ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = න 𝒗 𝝆𝒗 𝒅𝒗
  • 15.
    ❑ Consider thefourth Maxwell’s equation 𝛁 ∙ ഥ 𝑩 = 𝟎 ❑ Take volume integral on both sides න 𝒗 𝛁 ∙ ഥ 𝑩 𝒅𝒗 = 𝟎 ❑ Applying divergence theorem, we can write න 𝒗 𝛁 ∙ ഥ 𝑩 𝒅𝒗 = ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 ❑ Therefore, the fourth low ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎
  • 16.
    MAXWELL’S EQUATIONS FORSTATIC FIELDS 𝛁 × ഥ 𝑯 = ҧ 𝒋 ⇔ ර 𝑳 ഥ 𝑯. 𝒅ത 𝑳 = ර 𝒔 ҧ 𝒋. 𝒅ത 𝒔 𝛁 × ഥ 𝑬 = 𝟎 ⇔ ර 𝑳 ഥ 𝑬. 𝒅ത 𝑳 = 𝟎 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗 ⇔ ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = න 𝒗 𝝆𝒗 𝒅𝒗 𝛁 ∙ ഥ 𝑩 = 𝟎 ⇔ ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎
  • 17.
    CHARACTERISTICS OF FREESPACE Parameter Symbol Value Relative permittivity 𝜺𝒓 1 Relative permeability 𝝁𝒓 1 Conductivity 𝝈 0 Conduction current density ҧ 𝑱 0 Volume charge density 𝝆𝒗 0 Intrinsic or characteristic impedance 𝜼 𝟏𝟐𝟎 𝝅 𝑶𝑹 𝟑𝟕𝟕
  • 18.
    MAXWELL’S EQUATIONS FORFREE SPACE 𝛁 × ഥ 𝑯 = ሶ ഥ 𝑫 ⇔ ර 𝑳 ഥ 𝑯. 𝒅ത 𝑳 = ර 𝒔 ሶ ഥ 𝑫. 𝒅ത 𝒔 𝛁 × ഥ 𝑬 = − ሶ ഥ 𝑩 ⇔ ර 𝑳 ഥ 𝑬. 𝒅ത 𝑳 = − ර 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔 𝛁 ∙ ഥ 𝑫 = 𝟎 ⇔ ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = 𝟎 𝛁 ∙ ഥ 𝑩 = 𝟎 ⇔ ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎
  • 19.
    MAXWELL’S EQUATIONS FORSTATIC FIELDS IN FREE SPACE 𝛁 × ഥ 𝑯 = 𝟎 ⇔ ර 𝑳 ഥ 𝑯. 𝒅ത 𝑳 = 𝟎 𝛁 × ഥ 𝑬 = 𝟎 ⇔ ර 𝑳 ഥ 𝑬. 𝒅ത 𝑳 = 𝟎 𝛁 ∙ ഥ 𝑫 = 𝟎 ⇔ ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = 𝟎 𝛁 ∙ ഥ 𝑩 = 𝟎 ⇔ ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎
  • 20.
    PROOF OF MAXWELL’SEQUATIONS ❑ First, from Ampere’s circuital law , we have 𝛁 × ഥ 𝑯 = ҧ 𝒋 ❑ Take dot product on both sides 𝛁. 𝛁 × ഥ 𝑯 = 𝛁. ҧ 𝒋 ❑ As the divergence of curl of a vector is zero, 𝛁. ҧ 𝒋 = 𝟎 ❑ But the equation of continuity in point form 𝛁 ∙ ҧ 𝑱 = −𝝏𝝆𝒗 𝝏𝒕 = − ሶ 𝝆𝒗 ❑ This means that if 𝛁 × ഥ 𝑯 = ҧ 𝒋 is true, we get 𝛁. ҧ 𝒋 = 𝟎. ❑ As the equation of continuity is more fundamental, Ampere’s circuital law should be modified.
  • 21.
    ❑ Modifying Ampere’scircuital law , we have 𝛁 × ഥ 𝑯 = ҧ 𝒋 + ഥ 𝑭 ❑ Take dot product on both sides 𝛁. 𝛁 × ഥ 𝑯 = 𝛁. ҧ 𝒋 + 𝛁. ഥ 𝑭 ❑ As the divergence of curl of a vector is zero, 𝛁. ҧ 𝒋 + 𝛁. ഥ 𝑭 = 𝟎 ❑ Substituting the value of 𝛁. ҧ 𝒋 from the equation of continuity in the previous equation, 𝛁 ∙ ഥ 𝑭 + − ሶ 𝝆𝒗 = 𝟎 OR 𝛁 ∙ ഥ 𝑭 = ሶ 𝝆𝒗
  • 22.
    ❑ But thepoint form of Gauss’s law 𝛁. ഥ 𝑫 = 𝝆𝒗 OR 𝛁. ሶ ഥ 𝑫 = ሶ 𝝆𝒗 ❑ Then, 𝛁. ഥ 𝑭 = 𝛁. ሶ ഥ 𝑫 ❑ The divergence of two vectors are equal only if the vectors are identical. ഥ 𝑭 = ሶ ഥ 𝑫 ❑ Substituting the value of ഥ 𝑭, 𝛁 × ഥ 𝑯 = ሶ ഥ 𝑫 + ҧ 𝒋
  • 23.
    ❑ Second, accordingto Faraday’s law 𝒆𝒎𝒇 = − 𝒅∅ 𝒅𝒕 , ∅ ∶ 𝒎𝒂𝒈𝒏𝒆𝒕𝒊𝒄 𝒇𝒍𝒖𝒙 𝒊𝒏 𝒘𝒃 ❑ By definition, 𝒆𝒎𝒇 = ර 𝑳 ഥ 𝑬. 𝒅ഥ 𝑳 ❑ Then, ර 𝑳 ഥ 𝑬. 𝒅ഥ 𝑳 = − 𝒅∅ 𝒅𝒕 ❑ But, ∅ = ‫ׯ‬ 𝒔 ഥ 𝑩. 𝒅ത 𝒔 OR − 𝒅∅ 𝒅𝒕 = − ‫ׯ‬ 𝒔 𝝏ഥ 𝑩 𝝏𝒕 . 𝒅ത 𝒔 ❑ So, ර 𝑳 ഥ 𝑬. 𝒅ഥ 𝑳 = − ර 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔
  • 24.
    ❑ Applying Stokes’theorem, we get ර 𝒔 𝛁 × ഥ 𝑬 . 𝒅ത 𝒔 = ර 𝑳 ഥ 𝑬. 𝒅ഥ 𝑳 ❑ Hence, ර 𝒔 𝛁 × ഥ 𝑬 . 𝒅ത 𝒔 = − ර 𝒔 ሶ ഥ 𝑩. 𝒅ത 𝒔 ❑ Two surface integrals are equal only if their integrands are equal, 𝛁 × ഥ 𝑬 = − ሶ ഥ 𝑩
  • 25.
    ❑ Third, fromGauss’s law in electric field ‫ׯ‬ 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = 𝑸 = ‫׬‬𝒗 𝝆𝒗 𝒅𝒗 ❑ Applying divergence theorem, we get ර 𝒔 ഥ 𝑫. 𝒅ത 𝒔 = න 𝒗 𝛁 ∙ ഥ 𝑫 𝒅𝒗 = න 𝒗 𝝆𝒗 𝒅𝒗 ❑ Two volume integrals are equal only if their integrands are equal, 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗 ❑ Fourth, from Gauss’s law for magnetic field [the magnetic flux lines are a closed loop] ර 𝒔 ഥ 𝑩. 𝒅ത 𝒔 = 𝟎 ❑ Applying divergence theorem, we get ‫׬‬𝒗 𝛁 ∙ ഥ 𝑩 𝒅𝒗 = 𝟎 OR 𝛁 ∙ ഥ 𝑩 = 𝟎
  • 26.
    SINUSOIDAL TIME-VARYING FIELDS ❑In practice, electric and magnetic fields vary sinusoidally. ❑ Any periodic variation can be described in terms of sinusoidal variations. ❑ The fields can be represented by ෩ ഥ 𝑬 = 𝑬𝒎 𝐜𝐨𝐬 𝝎𝒕 OR ෩ ഥ 𝑬 = 𝑬𝒎 𝒄𝒐𝒔 𝝎𝒕 where 𝝎 : Angular frequency, 𝝎 = 𝟐𝝅𝒇 𝒇 : Frequency variation of the field. 𝑬𝒎 : The maximum field strength.
  • 27.
    ❑ It isalso possible to represent the fields using the phasor notation. ❑ The time-varying field ෩ ഥ 𝑬(𝒓, 𝒕) is related to phasor field ഥ 𝑬(𝒓) as ෩ ഥ 𝑬(𝒓, 𝒕) = 𝑹𝒆 ഥ 𝑬 𝒓 𝒆𝒋𝝎𝒕 OR ෩ ഥ 𝑬(𝒓, 𝒕) = 𝑰𝒎 ഥ 𝑬 𝒓 𝒆𝒋𝝎𝒕 where 𝝎 : Angular frequency.
  • 28.
    MAXWELL’S EQUATIONS INPHASOR FORM ❑ Consider the first Maxwell’s equation 𝛁 × ෩ ഥ 𝑯 = ෩ሶ ഥ 𝑫 + ሚҧ 𝒋 ❑ If ෩ ഥ 𝑯 = 𝑹𝒆 ഥ 𝑯𝒆𝒋𝝎𝒕 ෩ ഥ 𝑫 = 𝑹𝒆 ഥ 𝑫𝒆𝒋𝝎𝒕 ෨ҧ 𝑱 = 𝑹𝒆 ҧ 𝑱𝒆𝒋𝝎𝒕 Then 𝛁 × 𝑹𝒆 ഥ 𝑯𝒆𝒋𝝎𝒕 = 𝝏 𝝏𝒕 𝑹𝒆 ഥ 𝑫𝒆𝒋𝝎𝒕 + 𝑹𝒆 ҧ 𝑱𝒆𝒋𝝎𝒕 ❑ Interchanging the operation of taking the real part, we get 𝑹𝒆 𝛁 × ഥ 𝑯 − 𝒋𝝎ഥ 𝑫 − ҧ 𝑱 𝒆𝒋𝝎𝒕 = 𝟎 ∴ 𝛁 × ഥ 𝑯 = 𝒋𝝎ഥ 𝑫 + ҧ 𝑱
  • 29.
    ❑ Consider thesecond Maxwell’s equation 𝛁 × ෩ ഥ 𝑬 = − ෩ሶ ഥ 𝑩 ❑ If ෩ ഥ 𝑬 = 𝑹𝒆 ഥ 𝑬𝒆𝒋𝝎𝒕 ෩ ഥ 𝑩 = 𝑹𝒆 ഥ 𝑩𝒆𝒋𝝎𝒕 ❑ Then 𝛁 × 𝑹𝒆 ഥ 𝑬𝒆𝒋𝝎𝒕 = − 𝝏 𝝏𝒕 𝑹𝒆 ഥ 𝑩𝒆𝒋𝝎𝒕 ❑ Interchanging the operation of taking the real part, we get 𝑹𝒆 𝛁 × ഥ 𝑬 + 𝒋𝝎ഥ 𝑩 𝒆𝒋𝝎𝒕 = 𝟎 ∴ 𝛁 × ഥ 𝑬 = −𝒋𝝎ഥ 𝑩
  • 30.
    ❑ Consider thethird Maxwell’s equation 𝛁 ∙ ෩ ഥ 𝑫 = 𝝆𝒗 ❑ If ෩ ഥ 𝑫 = 𝑹𝒆 ഥ 𝑫𝒆𝒋𝝎𝒕 ❑ Then 𝛁 ∙ 𝑹𝒆 ഥ 𝑫𝒆𝒋𝝎𝒕 = 𝝆𝒗 ❑ Interchanging the operation of taking the real part, we get 𝑹𝒆 𝛁 ∙ ഥ 𝑫 𝒆𝒋𝝎𝒕 = 𝝆𝒗 ∴ 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗
  • 31.
    ❑ Consider thefourth Maxwell’s equation 𝛁 ∙ ෩ ഥ 𝑩 = 𝟎 ❑ If ෩ ഥ 𝑩 = 𝑹𝒆 ഥ 𝑩𝒆𝒋𝝎𝒕 ❑ Then 𝛁 ∙ 𝑹𝒆 ഥ 𝑩𝒆𝒋𝝎𝒕 = 𝟎 ❑ Interchanging the operation of taking the real part, we get 𝑹𝒆 𝛁 ∙ ഥ 𝑩 𝒆𝒋𝝎𝒕 = 𝟎 ∴ 𝛁 ∙ ഥ 𝑩 = 𝟎
  • 32.
    ❑ In summary,Maxwell’s equations in phasor form are as follows: 𝛁 × ഥ 𝑯 = 𝒋𝝎ഥ 𝑫 + ҧ 𝑱 𝛁 × ഥ 𝑬 = −𝒋𝝎ഥ 𝑩 𝛁 ∙ ഥ 𝑫 = 𝝆𝒗 𝛁 ∙ ഥ 𝑩 = 𝟎
  • 33.
    The Part (1)will be continued … Thanks