Unit 7 | unit 7 electromagnetic waves

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EMF

Unit 7

Electromagnetic Waves

7.1 Derivation of wave equation

Maxwell’s equations in empty space (free of charges and currents) are :

Gauss’s Law for electricity . d =0

Gauss’s Law for magnetism . d =0

Faraday’s law of induction . d = d ɸB/dt

Ampere’s law . d = μo dɸꙴ / dt

According to Faraday’s Law changing magnetic fields make electric fields and according to Ampere’s law changing electric fields make magnetic fields . This is the essence of the propagation of electromagnetic waves. The fields produce each other as they change in space and time.

Consider a rectangular path in the x-z plane of height h and width dz as shown.

Apply Faraday’s Law . d = d ɸB/dt  . d = -d/dt

The path integral only has contributions along vertical portions of the path

. d = (E + dE) h – Eh = hdE

The flux integral can be done because the B-field is nearly constant over the rectangle.

= Bhdz

Putting these results in Faraday’s law hdE = -d/dt (Bhdz)

The only thing changing with time is the B-field so , dE = -dz . DB/dt = -dB/dt .

If this were done with total mathematical rigor the derivatives are actually partial derivatives.

So the relationship between E and B form Faraday’s Law is

∂E/ ∂z = ∂ B / ∂t

Now consider a rectangular path in the y-z plane of length l and width dz as shown. Apply Ampere’s law

. d = μo d/dt

The path integral only has contributions along portions parallel to the y-axis

. d = B l – (B+ dB ) l = -l dB

The flux integral can be done because the E-field is nearly constant over the rectangle

= El dz

Putting these results into Ampere’s Law ,

-l dB = = μo d/dt (Eldz) - dB/dz = μo dE/dt . Because only the E-field is changing with time. Again these are actually partial derivatives. So the relationship E and B from Ampere’s law is ∂ B / ∂ z = - μo ∂ E/∂ t .

In summary

∂ E / ∂ z = - ∂ E/∂ t

Is ∂ B / ∂ z = - μo ∂ E/∂ t .

Taking the derivative with respect to z of the first equation and the derivative with respect to the second equation gives

∂ 2 E / ∂ z 2 = - ∂ B / ∂ z ∂ t and ∂ 2 B / ∂ z ∂t = - μo ∂ 2 E/∂ t 2

Combining the results produces ∂ 2 E / ∂ z 2 = μo ∂ 2 E/∂ t 2

This is called Wave Equation.

7.2 Uniform Plane waves

Waves with constant phase fronts whose amplitude (Eo) is uniform.

x = -jwμo H

Where E field of a uniform plane is given by

The magnetic field is then

E field is in direction

H field is in direction

Wave is propagating in direction

Or in time-domain

E(z,t) = Re { E e jwt } = Eo cos (wt – kz)

Similarly

H(z,t) = Re { E e jwt / o } = Eo / o cos (wt -kz)

7.3 Maxwell’s equation in Phasor form

Maxwell’s equations is considered for time-harmonic fields. These fields whose only time dependence is sinusoidal which may be represented in phasor domain just like scalar time-harmonic functions.

For example, we write the relationship between time-harmonic field ( , t) and its phasor field ( as

( , t) = Real { ( exp(j2)}

Where f is the frequency of radiation. The phasor representation simplifies the analysis of electromagnetic waves since it completes removes the time dependency from all field components.

Maxwell’s equations in phasor form

7.4 Wave Equation in Phasor form

It is possible to express any wave as a superposition of harmonics with different frequencies. Then for each harmonic the wave equation

2 - μ ∂ 2 / ∂ t 2 = 0

Can be written in the form of equation for the phasor

2 + w 2 μ = 0 – Helmholtz equation

We omitted here the underline symbol in the phasor that represents the sinusoidal function of time ( , t) . Solution for every component of the phasor can be obtained by using the procedure of separation of variables.

In rectangular (Cartesian) coordinates

Ei(x,y,z) = Xi (x) Yi(y) Zi(z) (i=x,y,z)

From Helmholtz equation we obtain

∂ 2 Xi / ∂ x 2 . 1/(Xi(x)) + ∂ 2 Yi / ∂ y 2 . 1/(Yi(y)) + ∂ 2 Zi / ∂ z 2 . 1/(Zi(z) + w 2 μ =0

It follows that each of the first three terms must be constant

∂ 2 Xi / ∂ x 2 . 1/ 1/(Xi(x))= -k 2 x ( k 2 x = constant >0)

∂ 2 Yi / ∂ y 2 . 1/(Yi(y)) = -k 2 y ( k 2 y = constant >0)

∂ 2 Zi / ∂ y 2 . 1/(Zi(z)) = -k 2 z ( k 2 z = constant >0)

Where k 2 x, k 2 y, k 2 z satisfy the so-called dispersion equation.

k 2 = k 2 x+ k 2 y+ k 2 z = w 2 μ

Xi(x) = Ai e -ikx + Bi eikx

If only first term is retained in phasor the sinusoidal in time domain solution for the field will have the form

Xi(x,t) = Re { Ai e –i(kx-wt)} = Ai cos(kx -wt)

It corresponds to the wave travelling in positive x-direction.

7.5 Plane waves in free space and in homogeneous material

. d S = μo ꙴ o dɸ E / dt

In empty space where Q=0 and I=0

The following are the differential equations relating E and B . The subscripts on the components Ey and Bz

∂ E / ∂ x = - ∂ B / ∂ t

∂ B / ∂ x = - μo ∂E/dt

For example when we evaluate ∂ E/ ∂ x we assume that t is constant . Likewise when we evaluate ∂ B / ∂ t x is held constant

∂ 2 E/ ∂ x 2 = ∂/∂x (∂B/∂t) = - ∂/∂t(∂B/∂x) = - ∂/∂t(-μoꙴ o ∂E/∂t)

∂ 2 E/ ∂ x 2 = μoꙴ o ∂ 2E/∂t 2

∂2B/∂x 2 = μoꙴ o ∂ 2B/∂t 2

The wave speed v replaced by c where

c = 1/ ꙴ o

7.6 Wave equation for conducting medium

A so-called Ohmic conductor is a medium that satisfies Ohm's law, which can be written in the form

$\displaystyle {\bf j} = \sigma {\bf E},$

(1)

Where ${\bf j}$ is the current density (i.e., the current per unit area), ${\bf E}$ the electric field-strength, and $\sigma$ a constant known as the electrical conductivity of the medium in question.

The $ z$ -directed propagation of a plane electromagnetic wave, linearly polarized in the $ x$ -direction, through an Ohmic conductor of conductivity $\sigma$ is governed by

$\displaystyle \frac{\partial E_x}{\partial t} +\frac{\sigma}{\epsilon_0} E_x$

$\displaystyle =-\frac{1}{\epsilon_0}\, \frac{\partial H_y}{\partial z},$

(2)

$\displaystyle \frac{\partial H_y}{\partial t}$

$\displaystyle = - \frac{1}{\mu_0} \frac{\partial E_x}{\partial z},$

(3)

For a so-called good conductor, which satisfies the inequality $\sigma\gg \epsilon_0\,\omega$ , the first term on the left-hand side of Equation (3) is negligible with respect to the second term, and the previous two equations reduce to

$\displaystyle E_x$

$\displaystyle \simeq- \frac{1}{\sigma}\,\frac{\partial H_y}{\partial z},$

(4)

$\displaystyle \frac{\partial H_y}{\partial t}$

$\displaystyle = -\frac{1}{\mu_0} \frac{\partial E_x}{\partial z}.$

(5)

These equations can be solved to give

$\displaystyle E_x(z,t)$

$\displaystyle = E_0 {\rm e}^{-z/d} \cos(\omega t-z/d),$

(6)

$\displaystyle H_y(z,t)$

$\displaystyle = E_0 Z^{ -1} {\rm e}^{-z/d} \cos(\omega t-z/d-\pi/4),$

(7)

Where

$\displaystyle d = \left(\frac{2}{\mu_0 \sigma \omega}\right)^{1/2},$

(8)

And

$\displaystyle Z = \left(\frac{\mu_0 \omega}{\sigma}\right)^{1/2} = \left(\frac{\epsilon_0 \omega}{\sigma}\right)^{1/2} Z_0.$

(9)

Equations (7) and (9) indicate that the amplitude of an electromagnetic wave propagating through a conductor decays exponentially on a characteristic length scale, $ d$ , that is known as the skin-depth.

Consequently, an electromagnetic wave cannot penetrate more than a few skin-depths into a conducting medium.

The skin-depth is smaller at higher frequencies. This implies that high frequency waves penetrate a shorter distance into a conductor than low frequency waves.

7.7 Plane waves in lossy dielectrics

A dielectric material can be lossy that is exhibit a nonzero conductivity

In this situation a conduction current must be added to the displacement current when considering Ampere’s law.

x E (r) = -jw μ H ( r )

x H (r) = j ( r ) + j w E(r) = ( + j w ) E( r )

2 E (r ) – j w μ ( + j w ) E (r ) =0

Assuming as previously that the electric field is linearly polarized in the y direction and the wave propagates in the z direction

Where the propagation constant

2 = j w μ ( j w ) = (jw) 2 μ ( 1 + / j w )

The propagation constant is complex

= α + j β

In a vacuum α = 0 and β = k. In general case the real and imaginary parts are non- linear functions of the frequency

α (w) = / 2 [ 1 + 1 + ( / w ) 2

= w 2[ 1 + 1 + ( / w ) 2

As a result the phase velocity may depend on the waves frequency. This phenoma is called dispersion and the medium in which wave is propagating called a dispersive medium.

7.8 Propagation in good conductors

Consider the propagation of an electromagnetic wave through a conducting medium which obeys Ohm's law:

$\begin{displaymath} {\bf j} = \sigma {\bf E}. \end{displaymath}$

(1)

Here, $\sigma$ is the conductivity of the medium in question. Maxwell's equations for the wave take the form:

$\displaystyle \nabla\cdot{\bf E}$

$\textstyle =$

$\displaystyle 0,$

(2)

$\displaystyle \nabla\cdot{\bf B}$

$\textstyle =$

$\displaystyle 0,$

(3)

$\displaystyle \nabla\times{\bf E}$

$\textstyle =$

$\displaystyle - \frac{\partial {\bf B}}{\partial t} ,$

(4)

$\displaystyle \nabla\times{\bf B}$

$\textstyle =$

$\displaystyle \mu_0 {\bf j} + \epsilon \epsilon_0\mu_0 \frac{\partial {\bf E}}{\partial t},$

(5)

Where $\epsilon$ is the dielectric constant of the medium. It follows, from the above equations, that

$\begin{displaymath} \nabla\times\nabla\times{\bf E} = -\nabla^2{\bf E} = -\frac{... ... \epsilon_0\mu_0 \frac{\partial {\bf E}}{\partial t}\right]. \end{displaymath}$

(6)

Looking for a wave-like solution of the form

$\begin{displaymath} {\bf E} = {\bf E}_0 {\rm e}^{ {\rm i} (k z-\omega t)}, \end{displaymath}$

(7)

We obtain the dispersion relation

$\begin{displaymath} k^2 = \mu_0 \omega (\epsilon \epsilon_0 \omega + {\rm i} \sigma). \end{displaymath}$

(8)

Consider a poor'' conductor for which $\sigma\ll \epsilon \epsilon_0 \omega$ . In this limit, the dispersion relation (8) yields

$\begin{displaymath} k\simeq n \frac{\omega}{c} + {\rm i} \frac{\sigma}{2}\sqrt{\frac{\mu_0} {\epsilon \epsilon_0}}, \end{displaymath}$

(9)

Where $n=\sqrt{\epsilon}$ is the refractive index. Substitution into Eq. (8) gives

$\begin{displaymath} {\bf E} = {\bf E}_0 {\rm e}^{-z/d} {\rm e}^{ {\rm i} (k_r z-\omega t)}, \end{displaymath}$

(10)

Where

$\begin{displaymath} d = \frac{2}{\sigma}\sqrt{\frac{\epsilon \epsilon_0}{\mu_0}}, \end{displaymath}$

(11)

And $k_r = n \omega/c$ . Thus, we conclude that the amplitude of an electromagnetic wave propagating through a conductor decays exponentially on some length-scale, $d$ , which is termed the skin-depth.

Note, from Eq. (11), that the skin-depth for a poor conductor is independent of the frequency of the wave.

Note, also, that $k_r d\gg 1$ for a poor conductor, indicating that the wave penetrates many wave-lengths into the conductor before decaying away.

Consider a good'' conductor for which $\sigma\gg \epsilon \epsilon_0 \omega$ . In this limit, the dispersion relation (11) yields

$\begin{displaymath} k\simeq \sqrt{{\rm i} \mu_0 \sigma \omega}. \end{displaymath}$

(12)

Substitution we get

$\begin{displaymath} d = \frac{1}{k_r} = \sqrt{\frac{2}{\mu_0 \sigma \omega}}. \end{displaymath}$

(13)

It can be seen that the skin-depth for a good conductor decreases with increasing wave frequency. The fact that $k_r d= 1$ indicates that the wave only penetrates a few wave-lengths into the conductor before decaying away.

7.9 Skin effect

We derived the equation

2 E = μ ꙴ ∂ 2 E / t2 + μ E / t ------------------------(1)

Where σ is the conductivity.

Substituting a plane wave

---------------------------------------(2)

Yields

2 = w 2 + I μ w --------------------------------------------(3)

To solve this we have to take a complex wavenumber

˜k = k + iκ-------------------------------------------------------------- (4)

Equating the real and imaginary parts in (3) yields

k 2 − κ 2 = w 2 ---------------------------------------------------------- (5)

2kκ = µσω -----------------------------------------------------------------------------------. (6)

The second equation can be solved for κ = µσω /2k then eliminating κ from (5) yields

k 4 – (µσω /2) 2 = µσω 2 k 2

This is a quadratic in k 2 with solution

Then we can use (5) to obtain

Now the complex wavenumber (4) implies

The first exponential decays with z and causes attenuation of the wave.

The characteristic distance over which the wave decays is known as the skin depth and is given by

δ = 1/k

Thus, the skin depth is the typical distance a wave penetrates into a conductor.

7.10 Poynting theorem

Poynting theorem states that the net power flowing out of a given volume V is equal to the time rate of decrease of stored electromagnetic energy in that volume decreased by the conduction losses is the total power leaving the volume = rate of decrease of stored electromagnetic energy ohmic power dissipated due to motion of charge.

Proof:

The energy density carried by the electromagnetic wave can be calculated using Maxwell's equations

Div = 0 -----------------------------(i)

Div = 0 ---------------------------------(ii)

Curl = - ∂ B / ∂t -----------------------------------(iii)

And curl = + ∂ / ∂t

Taking scalar product of (iii) with H and (iv) with

That is curl = - . ∂ / ∂t --------------------------------------(iv)

curl = . + . ∂ / ∂t ----------------------------------------(v)

So div ( x ) = - [ ∂ / ∂ t + ∂ / ∂ t] - .

But = μ and =

So ∂ / ∂ t = ∂ )/ ∂ t = ½ μ ∂/∂t (H 2)

= ∂/∂t [ ½ . ]

And ∂ / ∂ t = ∂ / ∂ t ( μ ) = ½ μ ∂ / ∂ t (H 2 )

= ∂ / ∂ t (1/2 . . )

And ∂ / ∂ t = ∂ / ∂ t ( ) = ½ ∂ / ∂ t (E 2 ) = ∂ / ∂ t [ ½ . ]

So from equation div ( x ) = - ∂ / ∂ t [ ½ . . ] - .

. = - ∂ / ∂ t [ ½ . . ] – div ( x )

Integrating equation over a volume V enclosed by a surface S

dV = - |∂ / ∂ t [ ½ . . | dV - (( x ) dV

Or dV = - H 2 + ½ E 2 ] dV - (( x ) ds

As = μ = and Ucm / ∂t dV - x .ds

Or - x .dV = - ∂/∂t ½[ μ H 2 + ½ E 2] dV - ds

Or ds = - Ucm / ∂t dV - x .dV

Or ds = - - Ucm / ∂t dV - x .dV

That is the Total power leaving the volume = rate of decrease of stored e.m.f energy - ohmic power dissipated due to charge motion

This equation represents the poynting theorem according to which the net power flowing out of a given volume is equal to the rate of decrease of stored electromagnetic energy in that volume minus the conduction losses.

References:

Faraday, Maxwell, and the Electromagnetic Field:by Basil Mahon and Nancy Forbes.
ELECTROMAGNETISM: Theory and Applications Book by ASHUTOSH PRAMANIK
Field and wave electromagnetics Textbook by David K. Cheng

Unit 7

Electromagnetic Waves

Unit 7

Electromagnetic Waves

Unit 7

Electromagnetic Waves

7.1 Derivation of wave equation

Maxwell’s equations in empty space (free of charges and currents) are :

Gauss’s Law for electricity . d =0

Gauss’s Law for magnetism . d =0

Faraday’s law of induction . d = d ɸB/dt

Ampere’s law . d = μo dɸꙴ / dt

Consider a rectangular path in the x-z plane of height h and width dz as shown.

Apply Faraday’s Law . d = d ɸB/dt  . d = -d/dt

The path integral only has contributions along vertical portions of the path

. d = (E + dE) h – Eh = hdE

The flux integral can be done because the B-field is nearly constant over the rectangle.

= Bhdz

Putting these results in Faraday’s law hdE = -d/dt (Bhdz)

The only thing changing with time is the B-field so , dE = -dz . DB/dt = -dB/dt .

If this were done with total mathematical rigor the derivatives are actually partial derivatives.

So the relationship between E and B form Faraday’s Law is

∂E/ ∂z = ∂ B / ∂t

Now consider a rectangular path in the y-z plane of length l and width dz as shown. Apply Ampere’s law

. d = μo d/dt

The path integral only has contributions along portions parallel to the y-axis

. d = B l – (B+ dB ) l = -l dB

The flux integral can be done because the E-field is nearly constant over the rectangle

= El dz

Putting these results into Ampere’s Law ,

In summary

∂ E / ∂ z = - ∂ E/∂ t

Is ∂ B / ∂ z = - μo ∂ E/∂ t .

Taking the derivative with respect to z of the first equation and the derivative with respect to the second equation gives

∂ 2 E / ∂ z 2 = - ∂ B / ∂ z ∂ t and ∂ 2 B / ∂ z ∂t = - μo ∂ 2 E/∂ t 2

Combining the results produces ∂ 2 E / ∂ z 2 = μo ∂ 2 E/∂ t 2

This is called Wave Equation.

7.2 Uniform Plane waves

Waves with constant phase fronts whose amplitude (Eo) is uniform.

x = -jwμo H

Where E field of a uniform plane is given by

The magnetic field is then

E field is in direction

H field is in direction

Wave is propagating in direction

Or in time-domain

E(z,t) = Re { E e jwt } = Eo cos (wt – kz)

Similarly

H(z,t) = Re { E e jwt / o } = Eo / o cos (wt -kz)

7.3 Maxwell’s equation in Phasor form

Maxwell’s equations is considered for time-harmonic fields. These fields whose only time dependence is sinusoidal which may be represented in phasor domain just like scalar time-harmonic functions.

For example, we write the relationship between time-harmonic field ( , t) and its phasor field ( as

( , t) = Real { ( exp(j2)}

Where f is the frequency of radiation. The phasor representation simplifies the analysis of electromagnetic waves since it completes removes the time dependency from all field components.

Maxwell’s equations in phasor form

7.4 Wave Equation in Phasor form

It is possible to express any wave as a superposition of harmonics with different frequencies. Then for each harmonic the wave equation

2 - μ ∂ 2 / ∂ t 2 = 0

Can be written in the form of equation for the phasor

2 + w 2 μ = 0 – Helmholtz equation

In rectangular (Cartesian) coordinates

Ei(x,y,z) = Xi (x) Yi(y) Zi(z) (i=x,y,z)

From Helmholtz equation we obtain

∂ 2 Xi / ∂ x 2 . 1/(Xi(x)) + ∂ 2 Yi / ∂ y 2 . 1/(Yi(y)) + ∂ 2 Zi / ∂ z 2 . 1/(Zi(z) + w 2 μ =0

It follows that each of the first three terms must be constant

∂ 2 Xi / ∂ x 2 . 1/ 1/(Xi(x))= -k 2 x ( k 2 x = constant >0)

∂ 2 Yi / ∂ y 2 . 1/(Yi(y)) = -k 2 y ( k 2 y = constant >0)

∂ 2 Zi / ∂ y 2 . 1/(Zi(z)) = -k 2 z ( k 2 z = constant >0)

Where k 2 x, k 2 y, k 2 z satisfy the so-called dispersion equation.

k 2 = k 2 x+ k 2 y+ k 2 z = w 2 μ

Xi(x) = Ai e -ikx + Bi eikx

If only first term is retained in phasor the sinusoidal in time domain solution for the field will have the form

Xi(x,t) = Re { Ai e –i(kx-wt)} = Ai cos(kx -wt)

It corresponds to the wave travelling in positive x-direction.

7.5 Plane waves in free space and in homogeneous material

. d S = μo ꙴ o dɸ E / dt

In empty space where Q=0 and I=0

The following are the differential equations relating E and B . The subscripts on the components Ey and Bz

∂ E / ∂ x = - ∂ B / ∂ t

∂ B / ∂ x = - μo ∂E/dt

For example when we evaluate ∂ E/ ∂ x we assume that t is constant . Likewise when we evaluate ∂ B / ∂ t x is held constant

∂ 2 E/ ∂ x 2 = ∂/∂x (∂B/∂t) = - ∂/∂t(∂B/∂x) = - ∂/∂t(-μoꙴ o ∂E/∂t)

∂ 2 E/ ∂ x 2 = μoꙴ o ∂ 2E/∂t 2

∂2B/∂x 2 = μoꙴ o ∂ 2B/∂t 2

The wave speed v replaced by c where

c = 1/ ꙴ o

7.6 Wave equation for conducting medium

A so-called Ohmic conductor is a medium that satisfies Ohm's law, which can be written in the form

$\displaystyle {\bf j} = \sigma {\bf E},$

(1)

The $ z$ -directed propagation of a plane electromagnetic wave, linearly polarized in the $ x$ -direction, through an Ohmic conductor of conductivity $\sigma$ is governed by

$\displaystyle \frac{\partial E_x}{\partial t} +\frac{\sigma}{\epsilon_0} E_x$

$\displaystyle =-\frac{1}{\epsilon_0}\, \frac{\partial H_y}{\partial z},$

(2)

$\displaystyle \frac{\partial H_y}{\partial t}$

$\displaystyle = - \frac{1}{\mu_0} \frac{\partial E_x}{\partial z},$

(3)

$\displaystyle E_x$

$\displaystyle \simeq- \frac{1}{\sigma}\,\frac{\partial H_y}{\partial z},$

(4)

$\displaystyle \frac{\partial H_y}{\partial t}$

$\displaystyle = -\frac{1}{\mu_0} \frac{\partial E_x}{\partial z}.$

(5)

These equations can be solved to give

$\displaystyle E_x(z,t)$

$\displaystyle = E_0 {\rm e}^{-z/d} \cos(\omega t-z/d),$

(6)

$\displaystyle H_y(z,t)$

$\displaystyle = E_0 Z^{ -1} {\rm e}^{-z/d} \cos(\omega t-z/d-\pi/4),$

(7)

Where

$\displaystyle d = \left(\frac{2}{\mu_0 \sigma \omega}\right)^{1/2},$

(8)

And

$\displaystyle Z = \left(\frac{\mu_0 \omega}{\sigma}\right)^{1/2} = \left(\frac{\epsilon_0 \omega}{\sigma}\right)^{1/2} Z_0.$

(9)

Consequently, an electromagnetic wave cannot penetrate more than a few skin-depths into a conducting medium.

The skin-depth is smaller at higher frequencies. This implies that high frequency waves penetrate a shorter distance into a conductor than low frequency waves.

7.7 Plane waves in lossy dielectrics

A dielectric material can be lossy that is exhibit a nonzero conductivity

In this situation a conduction current must be added to the displacement current when considering Ampere’s law.

x E (r) = -jw μ H ( r )

x H (r) = j ( r ) + j w E(r) = ( + j w ) E( r )

2 E (r ) – j w μ ( + j w ) E (r ) =0

Assuming as previously that the electric field is linearly polarized in the y direction and the wave propagates in the z direction

Where the propagation constant

2 = j w μ ( j w ) = (jw) 2 μ ( 1 + / j w )

The propagation constant is complex

= α + j β

In a vacuum α = 0 and β = k. In general case the real and imaginary parts are non- linear functions of the frequency

α (w) = / 2 [ 1 + 1 + ( / w ) 2

= w 2[ 1 + 1 + ( / w ) 2

As a result the phase velocity may depend on the waves frequency. This phenoma is called dispersion and the medium in which wave is propagating called a dispersive medium.

7.8 Propagation in good conductors

Consider the propagation of an electromagnetic wave through a conducting medium which obeys Ohm's law:

$\begin{displaymath} {\bf j} = \sigma {\bf E}. \end{displaymath}$

(1)

Here, $\sigma$ is the conductivity of the medium in question. Maxwell's equations for the wave take the form:

$\displaystyle \nabla\cdot{\bf E}$

$\textstyle =$

$\displaystyle 0,$

(2)

$\displaystyle \nabla\cdot{\bf B}$

$\textstyle =$

$\displaystyle 0,$

(3)

$\displaystyle \nabla\times{\bf E}$

$\textstyle =$

$\displaystyle - \frac{\partial {\bf B}}{\partial t} ,$

(4)

$\displaystyle \nabla\times{\bf B}$

$\textstyle =$

$\displaystyle \mu_0 {\bf j} + \epsilon \epsilon_0\mu_0 \frac{\partial {\bf E}}{\partial t},$

(5)

Where $\epsilon$ is the dielectric constant of the medium. It follows, from the above equations, that

$\begin{displaymath} \nabla\times\nabla\times{\bf E} = -\nabla^2{\bf E} = -\frac{... ... \epsilon_0\mu_0 \frac{\partial {\bf E}}{\partial t}\right]. \end{displaymath}$

(6)

Looking for a wave-like solution of the form

$\begin{displaymath} {\bf E} = {\bf E}_0 {\rm e}^{ {\rm i} (k z-\omega t)}, \end{displaymath}$

(7)

We obtain the dispersion relation

$\begin{displaymath} k^2 = \mu_0 \omega (\epsilon \epsilon_0 \omega + {\rm i} \sigma). \end{displaymath}$

(8)

Consider a poor'' conductor for which $\sigma\ll \epsilon \epsilon_0 \omega$ . In this limit, the dispersion relation (8) yields

$\begin{displaymath} k\simeq n \frac{\omega}{c} + {\rm i} \frac{\sigma}{2}\sqrt{\frac{\mu_0} {\epsilon \epsilon_0}}, \end{displaymath}$

(9)

Where $n=\sqrt{\epsilon}$ is the refractive index. Substitution into Eq. (8) gives

$\begin{displaymath} {\bf E} = {\bf E}_0 {\rm e}^{-z/d} {\rm e}^{ {\rm i} (k_r z-\omega t)}, \end{displaymath}$

(10)

Where

$\begin{displaymath} d = \frac{2}{\sigma}\sqrt{\frac{\epsilon \epsilon_0}{\mu_0}}, \end{displaymath}$

(11)

Note, from Eq. (11), that the skin-depth for a poor conductor is independent of the frequency of the wave.

Note, also, that $k_r d\gg 1$ for a poor conductor, indicating that the wave penetrates many wave-lengths into the conductor before decaying away.

Consider a good'' conductor for which $\sigma\gg \epsilon \epsilon_0 \omega$ . In this limit, the dispersion relation (11) yields

$\begin{displaymath} k\simeq \sqrt{{\rm i} \mu_0 \sigma \omega}. \end{displaymath}$

(12)

Substitution we get

$\begin{displaymath} d = \frac{1}{k_r} = \sqrt{\frac{2}{\mu_0 \sigma \omega}}. \end{displaymath}$

(13)

7.9 Skin effect

We derived the equation

2 E = μ ꙴ ∂ 2 E / t2 + μ E / t ------------------------(1)

Where σ is the conductivity.

Substituting a plane wave

---------------------------------------(2)

Yields

2 = w 2 + I μ w --------------------------------------------(3)

To solve this we have to take a complex wavenumber

˜k = k + iκ-------------------------------------------------------------- (4)

Equating the real and imaginary parts in (3) yields

k 2 − κ 2 = w 2 ---------------------------------------------------------- (5)

2kκ = µσω -----------------------------------------------------------------------------------. (6)

The second equation can be solved for κ = µσω /2k then eliminating κ from (5) yields

k 4 – (µσω /2) 2 = µσω 2 k 2

This is a quadratic in k 2 with solution

Then we can use (5) to obtain

Now the complex wavenumber (4) implies

The first exponential decays with z and causes attenuation of the wave.

The characteristic distance over which the wave decays is known as the skin depth and is given by

δ = 1/k

Thus, the skin depth is the typical distance a wave penetrates into a conductor.

7.10 Poynting theorem

Proof:

The energy density carried by the electromagnetic wave can be calculated using Maxwell's equations

Div = 0 -----------------------------(i)

Div = 0 ---------------------------------(ii)

Curl = - ∂ B / ∂t -----------------------------------(iii)

And curl = + ∂ / ∂t

Taking scalar product of (iii) with H and (iv) with

That is curl = - . ∂ / ∂t --------------------------------------(iv)

curl = . + . ∂ / ∂t ----------------------------------------(v)

So div ( x ) = - [ ∂ / ∂ t + ∂ / ∂ t] - .

But = μ and =

So ∂ / ∂ t = ∂ )/ ∂ t = ½ μ ∂/∂t (H 2)

= ∂/∂t [ ½ . ]

And ∂ / ∂ t = ∂ / ∂ t ( μ ) = ½ μ ∂ / ∂ t (H 2 )

= ∂ / ∂ t (1/2 . . )

And ∂ / ∂ t = ∂ / ∂ t ( ) = ½ ∂ / ∂ t (E 2 ) = ∂ / ∂ t [ ½ . ]

So from equation div ( x ) = - ∂ / ∂ t [ ½ . . ] - .

. = - ∂ / ∂ t [ ½ . . ] – div ( x )

Integrating equation over a volume V enclosed by a surface S

dV = - |∂ / ∂ t [ ½ . . | dV - (( x ) dV

Or dV = - H 2 + ½ E 2 ] dV - (( x ) ds

As = μ = and Ucm / ∂t dV - x .ds

Or - x .dV = - ∂/∂t ½[ μ H 2 + ½ E 2] dV - ds

Or ds = - Ucm / ∂t dV - x .dV

Or ds = - - Ucm / ∂t dV - x .dV

That is the Total power leaving the volume = rate of decrease of stored e.m.f energy - ohmic power dissipated due to charge motion

References:

Faraday, Maxwell, and the Electromagnetic Field:by Basil Mahon and Nancy Forbes.
ELECTROMAGNETISM: Theory and Applications Book by ASHUTOSH PRAMANIK
Field and wave electromagnetics Textbook by David K. Cheng

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