ENE 429 Antenna and Transmission Lines

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Transcript ENE 429 Antenna and Transmission Lines

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ENE 428 Microwave Engineering

Lecture 1

Introduction, Maxwell’s equations, fields in media, and boundary conditions 1

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Syllabus

•Asst. Prof. Dr. Rardchawadee Silapunt, [email protected]

•Lecture: 9:30pm-12:20pm Tuesday, CB41004 12:30pm-3:20pm Wednesday, CB41002 •Office hours : By appointment •Textbook: Microwave Engineering by David M. Pozar (3 rd edition Wiley, 2005) • Recommended additional textbook: Applied Electromagnetics by Stuart M.Wentworth (2 nd edition Wiley, 2007) 2

Grading

Homework 10% Quiz 10% Midterm exam 40% Final exam 40%

Vision

Providing opportunities for intellectual growth in the context of an engineering discipline for the attainment of professional competence, and for the development of a sense of the social context of technology.

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Course overview

• Maxwell’s equations and boundary conditions for electromagnetic fields • Uniform plane wave propagation • Waveguides • Antennas • Microwave communication systems RS 10-11/06/51 4

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Introduction

http://www.phy.ntnu.edu.tw/ntnujava/viewtopic.php?t=52 • Microwave frequency range (300 MHz – 300 GHz) • Microwave components are distributed components.

• Lumped circuit elements approximations are invalid.

• Maxwell’s equations are used to explain

H

and ) 5

Introduction (2)

• From Maxwell’s equations, if the electric field

E

is changing with time, then the magnetic field

H

varies spatially in a direction normal to its orientation direction • Knowledge of fields in media and boundary conditions allows useful applications of material properties to microwave components • A

uniform plane wave

, both electric and magnetic fields lie in the

transverse plane

, the plane whose normal is the direction of propagation 6 RS

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Maxwell’s equations

 

H

 

D

 

v B

 0  

t B

 

D

t M

(1) (2) (3) (4) 7

Maxwell’s equations in free space •  = 0, 

r

= 1, 

r

= 1 

H

  0  0 

E

t

H

t

Amp ère’s law Faraday’s law 

0

0

= 4  x10 -7 Henrys/m = 8.854x10

-12 farad/m 8 RS

RS Integral forms of Maxwell’s equations 

C

S

C

S

   

t

S

  

t

S

V

 

dv

Q

I

 0 (1) (2) (3) (4) 9

Fields are assumed to be sinusoidal or harmonic, and time dependence with steady-state conditions • Time dependence form:

E

 )

a x

• Phasor form:

E s

j

A x y z e a x

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Maxwell’s equations in phasor form 

E S

  

H S

 

D

 

v B

 0 

M

(1) (2) (3) (4) 11 RS

Fields in dielectric media (1)

atoms or molecules of the material to create electric flux,

D

  0

E

P e

/ 2

P e

where is the electric polarization. • In the linear medium, it can be shown that

P e

   0

e E

.

D

  0 (1  

e

)

E

   0

r E

 

E

.

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Fields in dielectric media (2)

•  may be complex then

e

expressed as  can be complex and can be  

j

 '' • Imaginary part is counted for loss in the medium due to damping of the vibrating dipole moments. • The loss of dielectric material may be considered as an equivalent conductor loss if the material has a conductivity  . Loss tangent is defined as tan   ''   ' .

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Anisotropic dielectrics

• The most general linear relation of anisotropic dielectrics can be expressed in the form of a tensor which can be written in matrix form as    

D x D y D z

           

xx yx zx

xy

yy

zy

xz

yz

zz

   

E E

E E

.

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Analogous situations for magnetic media (1) polarization of by aligned magnetic dipole moments

B

  0 (

H

P m

) / 2

P

• In the linear medium, it can be shown that

P m

 

m H

.

• Then we can write

B

  0 (1  

m

)

H

   0

r H

 

H

.

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Analogous situations for magnetic • media (2)  may be complex then

m

 expressed as  

j

 can be complex and can be '' • Imaginary part is counted for loss in the medium due to damping of the vibrating dipole moments. 16 RS

Anisotropic magnetic material

• The most general linear relation of anisotropic material can be expressed in the form of a tensor which can be written in matrix form as  

z

     

xx

yx

zx

xy

yy

zy

xz

yz

zz

       

H H H x y z

        

H H H x y z

    .

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Boundary conditions between two media

B n2 H t2 D n2 E t2 n

 2 

D

1   

S

2   1

B n1 H t1 D n1 E t1

E

2

n

  

H E

1 2  

H

1  

M S J S

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Fields at a dielectric interface

• Boundary conditions at an interface between two lossless dielectric materials with no charge or current densities can be shown as 2   1 2   1 1 1 2 2 .

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Fields at the interface with a perfect conductor • Boundary conditions at the interface between a dielectric with the perfect conductor can be shown as 0 0  0.

M S

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General plane wave equations (1) • Consider medium free of charge • For linear, isotropic, homogeneous, and time invariant medium, assuming no free magnetic current, 

E

   

t E

  

H t

(1) (2) 21 RS

General plane wave equations (2) Take curl of (2), we yield   ( 

E

  

t

 

t H

)  

E t

)    

E

t

   2

E

t

2 From

A A

2

A

then 2

E

   

E

t

   2

E

t

2 For charge free medium 0 RS 22

Helmholtz wave equation

For electric field  2

E

  

E

t

   2

E

t

2 For magnetic field  2

H

  

H

t

   2

H

t

2 RS 23

Time-harmonic wave equations

• Transformation from time to frequency domain  

t

j

 Therefore  2

E s

j

  

j

 )

E s

 2

E s

j

  

j

 )

E s

 0  2

E s

  2

E s

 0 24 RS

Time-harmonic wave equations

or  2

H s

  2

H s

 0 where  

j

  

j

 ) This  term is called

propagation constant

or we can write 

=

+j

 RS where   = attenuation constant (Np/m)

=

phase constant (rad/m) 25

Solutions of Helmholtz equations • Assuming the electric field is in x-direction and the wave is propagating in z- direction • The instantaneous form of the solutions

E

E e

0 

z

cos(  

x

E e

0   

z

cos(  

x

• Consider only the forward-propagating wave, we have

E

E e

0  

z

cos(  

x

• Use Maxwell’s equation, we get

H

H e

 

z

cos(   RS

y

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Solutions of Helmholtz equations in phasor form • Showing the forward-propagating fields without time harmonic terms.

E s

  

z e

a x H s

  

z e

a y

• Conversion between instantaneous and phasor form Instantaneous field = Re(e j  t  phasor field) RS 27

Intrinsic impedance

• For any medium,  

E x H y

 

j

 

j

 • For free space  

E x H y

E

0

H

0   0  0  120   RS 28

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Propagating fields relation

H s

 1 

a

 

E s E s

  

a

 

H s a

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