Uploaded by hrishikesh8113

Antenna fundamentals

advertisement
Antenna and Wave Propagation
Dr. A .Bharathi
Electronics and Communication Engineering Department,
UCE(A), Osmania University.
AM Transmitter Tower
(The tower is the antenn
Antennas in Wireless Communication
Systems
Modulating
Signal
Transmitter
Modulator
Amplifier
Carrier
Signal
Impedance
Matching
Network**
Lossless
Receiver
RF
Amplifier
*BPF
Mixer
IF Filter and
Amplifier
Demod
ulator
LO
Figure 2 Radio Signal Transmission and Reception
Display
device/
speaker
•To understand the various antenna parameters give insight of the radiation
phenomena
•To have thorough understanding of radiation characteristics of different types
of
antennas.
•To study the characteristics of array antennas having directional radiation
characteristics.
•To give insight on aperture antennas and modern antennas.
•To understand the concepts of wave propagation and create awareness about
the
different types of propagation of radio waves at different frequencies.
Outcomes
•The student acquires knowledge about the basic antenna parameters and
radiation
concepts.
•The student learns to analyze wire antennas in detail.
•The student attains engineering fundamentals to analyze and design antenna
arrays.
•The student can classify, analyze and design aperture and modern antennas.
•The student gains ability to identify and explain different modes of
Unit I
Fundamentals of Antenna theory: Principle of radiation, Basic Antenna Parameters
– Patterns, Beam Area, Radiation Intensity, Beam Efficiency, Directivity, Gain,
Antenna Apertures, Effective Height, Illustrative Problems. Retarded Potentials –
Helmholtz Theorem
Thin Linear Wire Antennas – Radiation from Small Electric Dipole, Quarter
wave Monopole and Half Wave Dipole – Current Distributions, Near field and far
field Components, Radiated Power, Radiation Resistance, Beamwidth, Directivity,
Effective Area and Effective Height. Loop Antennas – Introduction, Small Loop,
Comparison of Far Fields of Small Loop and Short Dipole.
Unit II
Antenna Arrays: Basic two element array, N element uniform linear array, Pattern
multiplication, Broadside and End fire array, Planar array, Concept of Phased arrays,
Adaptive array, Basic principle of antenna Synthesis- Binomial array, Tschebysev
array.
Unit III
Practical Antennas: Yagi-uda antenna, V- Antenna, Rhombic antenna, Travelling
wave antennas, Microstrip antennas – Introduction, Features, Advantages and
Limitations, Rectangular Patch Antennas – Geometry, Design equations and
Characteristics.
Unit IV
Aperture and Modern Antennas: Reflector Antennas – Introduction, Flat Sheet
and Corner Reflectors, Paraboloidal Reflectors – Geometry, Pattern
Characteristics, Feed Methods, Reflector Types – Related Features, Illustrative
Problems. Horn Antennas – Types, Fermat’s Principle, Radiation from sectoral
and pyramidal horns, Design Considerations of Pyramidal Horns, Reconfigurable
antenna, Active antenna, Dielectric antennas, Electronic band gap structure and
applications.
Unit V
Wave propagation: Ground wave propagation. Space and surface waves,
Tropospheric refraction and reflection. Sky wave propagation – Virtual height,
Suggested Reading:
Constantine A. Balanis, Modern Antenna Handbook, A John Wiley &
Sons, Inc., Publication, 2008.
John D. Kraus, Ronald J. Marhefka and Ahmed S.Khan, “Antennas
for All Applications” 3rd Edition, Tata McGraw- Hill publishing
company Limited, New Delhi, 2006.
K.D.Prasad, “Antennas and Wave Propagation”, Khanna or Satya
Publications.
Unit I
Fundamentals of Antenna theory: Principle of radiation, Basic
Antenna Parameters – Patterns, Beam Area, Radiation Intensity,
Beam Efficiency, Directivity, Gain, Antenna Apertures,
Effective Height, Illustrative Problems. Retarded Potentials –
Helmholtz Theorem
Thin Linear Wire Antennas – Radiation from Small Electric
Dipole, Quarter wave Monopole and Half Wave Dipole – Current
Distributions, Near field and far field Components,
Radiated Power, Radiation Resistance, Beamwidth, Directivity,
Effective Area and Effective Height. Loop Antennas –
Introduction, Small Loop, Comparison of Far Fields of Small
Basic Types of Antennas
Physical structure of the antenna.
Wire antennas, Aperture antennas, Reflector antennas, Lens antennas, Microstrip
antennas, Array antennas
Frequency of operation
Very Low Frequency (VLF), Low Frequency (LF),Medium Frequency (MF),
High Frequency (HF), Very High Frequency (VHF), Ultra High Frequency (UHF),
Super High Frequency (SHF), Microwave and mm wave
Application
Point-to-point communications, Broadcasting applications, Radar communications,
Satellite communications
Physical structure
Paraboloid
Parabolic cylinder
Shaped
Stacked beam
Convex Lens
Concave Lens
Antennas for Various Applications
 MW Radio – Frequency: 530 to 1620 kHz (use λ/4 monopole antenna)
 Cell Phones – CDMA, GSM900(890-960), GSM1800(1710-1880),
3G(1920-1980,2110-2170), 4G, Wi-Fi/Bluetooth (use monopole, normal
mode helical, microstrip antenna, etc.)
 Cell Towers (use monopole, dipole, microstrip antenna arrays, etc.) Omni or Sectoral coverage
 Satellite and Defense Communications (use microstrip, horn, spiral,
helical, reflector, Yagi-Uda, log-periodic antennas, etc.)
What is an Antenna?
An antenna is a transition device or transducer between a
guided wave and a free space wave, or vice versa.
Reciprocity
• Antenna characteristics are essentially the same regardless of
antenna is sending or receiving electromagnetic energy.
• An antenna ability to transfer energy form the atmosphere to
its receiver with the same efficiency with which it transfers energy
from the transmitter into the atmosphere.
Conditions for Radiation
1. Time varying current (or) Acceleration and Deceleration of charge
2. Large separation between conductors
3. It is a high frequency phenomenon and the radiation is always
perpendicular to the direction of current flow
E and H fields in dipole
antenna
Current distribution
Thin wire transmission
line
Linear dipole
Flared transmission
Terminology of Antenna
Input Impedance and VSWR of
Antenna
ZA
Radiation Pattern
Mathematical or graphical representation of radiation properties of
antenna as a function of space coordinates.
E(,) or P(,)
Properties of Radiation Pattern
Plotted with normalized magnitude values
(dB/Linear scale)
Shape is independent of distance r
Depends on antenna polarization
3D Radiation Pattern
Side Lobes
Transmit mode: Wastage of Radiated power
Receive mode : Receive from undesired
directions
The optimum tradeoff between side lobes, gain,
and beam width is an important consideration
for choosing or designing radar antennas
2 D Radiation pattern
Polar Plot
Plot
Rectangular/Linear
Antenna Beamwidth
Beam width of a pattern is the angular separation between two identical points on opposite side of the pattern
maximum
Half-Power Beamwidth (HPBW ) is defined as: “In a plane containing the direction of the maximum of a beam, the
angle between the two directions in which the radiation intensity is one-half value of the beam.”
The angular separation between the first nulls of the pattern is referred to as the First-Null Beamwidth (FNBW )
HPBW Calculations
Example 1
Find the (HPBW) of an antenna having
E() = cos2  for 0o <  < 90o
Solution
E() at half power
0.707 = cos2 
 = 33o
BW = 66o
Example 2
Find the (HPBW) of an antenna having
P() = cos
Example 3
Find the (HPBW) of an antenna having
P() = sin
2 D Radiation pattern
Horizontal Pattern
E()
E()
Horizontal dipole
radiation pattern ????
Vertical
Pattern
3D
Pattern
Principal Plane patterns
E Plane : Plane containing E
field and the direction of
maximum radiation.
H plane : Plane containing H
field and the direction of
maximum radiation.
E plane and H plane Patterns
for a vertical dipole antenna??
3-D Radiation Pa` ttern of
Antenna
Isotropic Radiation
Pattern D = 1 =
0dB
Omni-Directional Radiation
Pattern of λ/2 Dipole
Antenna D = 1.64 = 2.1dB
Directional Radiation
Pattern of Microstrip
Antenna Array D = 500 =
27dB
Field Regions Near Antenna
R1=0.63sqrt(D3/λ)
2
Plane Angle and Solid Angle
One radian is defined as the plane angle with its vertex at the centre of a
circle of radius r that is subtended by an arc whose length is r.
One steradian is defined as the solid angle with its vertex at the centre of a sphere of
radius r that is subtended by a spherical surface area equal to that of a square with
each side of length r.
Radiation Power Density
Power radiated per unit surface area from the antenna surface is
called radiation power density (w/m2).
Instantaneous
Poynting
vector
Average poynting
vector or Average
power density
Real (calculated
over one time
period): Imaginary
part is eliminated
Analogous to Ohm’s law :
P=1/2 VI*
Instantaneous Total Power = Integration of normal component of
poynting vector (power density) over the entire surface
Average (total) radiated
power
Radiation Intensity
Radiation intensity in a given direction is defined as the power
radiated from the antenna per unit solid angle.
Radiated Power Calculations
Beam Solid angle or Beam Area
Asymmetric pattern
Directivity`of Antenna
Directivity of an antenna is the ratio of radiation intensity in the direction of
maximum radiation to the radiation intensity averaged over all the directions.
Um DUo
Uo
Theta in radians
Example: For Infinitesimal
Aperture Concept
Effective Aperture Area, Loss Aperture ,
Aperture
Effective Length
Scattering Aperture,
Collecting
Directivity and G ain of
DirectivityAntenna
of Large Antenna Directivity of Small Antenna
`
D 41253
D  1/
E H
Directivity is proportional to the Effective Aperture Area of
Antenna
Gain = η Directivity
Where η is Radiation Efficiency of Antenna
η = Prad/ Pin
Wave Polarization
At z=0
Equation of the curve which the tip of E field traces at specific point
Case 1: Linear polarization   0 ratio of fields can be anything
Ex0=0 , Ey0=0, Ex0=Ey0
Animation
makes it clear
Slant linear polarization
Case 2: Circular polarization   /2 Both field components have equal amplitude Eo
Case 3 : Elliptical polarization   /2 Both field components have unequal amplitude
LHC
P
LHCP
RHC
P
Clockwis
e
Anti Clockwise
Partial Directivity and Partial
Gain
Calibration may be in dB relative to max. for that antenna, or relative to isotropic
(dBi)
or half wave dipole (dBd).
Gain (dBi) = Gain (dBd) + 2.14 dB
Polarization of Antenna
Orientation of radiated electric field vector in the main beam of the
antenna
Microstrip Antenna in Different
Polarizations
Wave is Linearly Polarized
Wave is Circularly Polarized
Phase shift realized with delay line
Co-Polarization
The desired polarization (the main polarization)
(CO-POL)
Cross-Polarization
The undesired orthogonal polarization
(CROSS-POL).
55
Co-polarized antenna
pattern
Relative Power
Single feed
Phase shift realized with 900 hybrid
(branch line coupler)
XPD
X-polarized patttern
Azimuth Angle
Antenna Bandwidth
Bandwidth: Range of frequencies within which performance of antenna, where the
characteristics (ZA, SLL, G, Polarization, efficiency, beamwidth) conforms to
accepted value.
Notation: fH:fL , (fH-fL )/fo
Impedance Bandwidth, Pattern BW, Axial ratio BW, Gain BW
Axial Ratio of Antenna
, circular
polarization
, elliptical
polarization
, linear polarization
Axial Ratio Bandwidth:
Frequency range over
which AR < 3 dB
Axial Ratio Plot of Circularly Polarized
MSA Bandwidth for AR < 3dB = 380MHz
(13%)
Procedure for Antenna Analysis
1.
2.
3.
4.
Knowledge of current distribution
Find A
Find H using H= 1/(∇xA)
Find E using Maxwell’s curl equation jE= ∇x H
Retarded Vector
I = I oej  t
Potential
I = Io e j (t-td)
td = r/c
j( t-  r) Since r/c = r
I
=
I
e
o
If I is considered
in the expression of vector potential it is called retarded vector
Step 2: Find A
Infinitesimal small
dipole
Step 3: Find H using H= 1/(∇xA)
Step 4 Find E using Maxwell’s curl equation jE=
∇x H
Fields in the far field region
1. What is the phase difference
between fields and current
2. What is the ratio between E
and H
3. Does the fields radiated by
antenna has identical properties
as uniform plane wave (TEM wave)
4. What is the polarization of the
antenna.
5. What is power radiated by antenna
Power radiated by Hertizian dipole
Directivity
Effective Aperture Area and Effective
length
Analysis of Short Dipole
R=r
CALCULATE POWER, RADIATION RESISTANCE. DIRECTIVITY AND
Analysis of Half wave Dipole
Step 1 :
Current
Distribution
Step 3: Find H using H= 1/(∇xA)
Far field term
Step 4: Find E using E/
H
Power radiated by half wavelength dipole
antenna
CALCULATE RADIATION RESISTANCE, DIRECTIVITY,
EFFECTIVE
APERTURE AREA AND EFFECTIVE LENGTH
D= 1.64 (2.15dB)
0.62l
Ae = 0.13λ2
le =
MONOPOLE ANTENNA
All practical antenna at low frequency are monopole antenna
Fields radiated by monopole antenna are same as dipole antenna.
It radiates only in hemisphere.
Image Theory
Image
Theory
Same current distribution as half wavelength
dipole
CALCULATE POWER RADIATED, RADIATION RESISTANCE,
DIRECTIVITY, EFFECTIVE APERTURE AREA AND EFFECTIVE
Unit II
Antenna Arrays
Basic two element array, N element
uniform linear array, Pattern
multiplication, Broadside and End fire
array, Planar array, Concept of
Phased arrays, Adaptive array, Basic
principle of antenna Synthesis Binomial array, Tschebysev array.
Array of Point Sources
Usually the radiation pattern of a single element is relatively wide, and provides
low values of relative gain.
In many applications it is necessary to design antennas with very directive
characteristics (very high gain) to meet the demands of long-distance
communication.
This can only be accomplished by increasing the electrical size of the antenna.
Another way is to form an assembly of radiating elements in an electrical and
geometrical configuration: ARRAY.
In an array of identical elements there are five factors that can be used to shape
the overall pattern of the antenna, viz.:
Five factors that can be used to shape the overall pattern of the antenna
1.
2.
3.
4.
5.
The geometrical configuration of the overall array (linear, circular, rectangular, spherical etc.
)
The relative displacement between the elements
The excitation amplitude of the individual elements
The excitation phase of the individual elements
The relative pattern of the individual elements
In most cases, the elements of an array are identical (though this is not necessary).
The elements may be of any form e.g. wires, apertures etc.
The total field of the array is determined by the vector addition of the fields radiated
by the individual elements.
This assumes that the current in each element is the same as that of the isolated
elements.
To provide very directive patterns, it is necessary that the fields from individual
elements interfere constructively (add) in the desired direction and interfere
destructively (cancel each other) in the remaining space.
The simplest and most practical array is formed by placing the elements along a
line:
Two-Element Array
Electric field of horizontal dipole in the far-zone
Let us represent the electric fields in the far-zone of the array elements in the
form
The far-field approximation of the two-element array problem:
Assumptions: The array elements are
• Identical, i.e.,
• Oriented in the same way in space (they have identical
polarization), i.e.,
• excitation is of the same amplitude, i.e.,
Therefore for two element array of horizontal hertz
antennas the total field is
Then, the total field is:
The normalized AF,
The normalized field pattern of the array is
expressed as:
PATTERN MULTIPLICATION
Since, the array factor does not depend on the directional characteristics of the individual
elements, it can be formulated by replacing the actual elements with isotropic (point)
sources assuming that each point source has amplitude, phase and location of the
corresponding element it is replacing.
The field pattern of an array of non-isotropic but similar point sources is the product of the
pattern of the individual source and the pattern of an array of isotropic point sources having the
same locations, relative amplitudes and phase as the non-isotropic sources.
Example 1: An array consists of two horizontal infinitesimal dipoles located at a distance d = λ
/ 4 from each other. Find the nulls of the total field, if the excitation magnitudes are the same
and the phase difference is:
a) β = 0;
b) β =/2;
c) β = −/2
The element factor En(θ,φ) does not depend on β, and it produces the same null in all three cases. Since En(θ,φ)
=|cosθ|, the null is at θ1 = / 2.
The AF depends on β and produces different results in the 3 cases:
a) β = 0
Array factor for various values of d (0):
d = λ/2
A solution with a real-valued angle does not exist.
In this case, the total field pattern has only 1 null at θ =90°.
d=λ
b) β = /2
The equation
does not have a solution.
The total field pattern has 2 nulls: θ1 = 90° and θ2 = 0°
c) β = −/2
The total field pattern has 2 nulls: θ1 = 90° and at θ2
=180°.
N-Element Linear Array: Uniform Amplitude and Spacing
• An array of identical elements all of identical magnitude and each with a progressive phase

referred to as a Uniform Array
The Array Factor (AF) is given by:

AF  1  e

j  kd co s    
N
 AF 

e
 e

j 2  kd co s    
j  n 1  kd co s    
N

n 1

 
j  n 1 
e

j N
1  kd
co s
  
  kd co s   
n 1
N

e

is
AF 

e
j  n 1 
…..(1)
n 1
  kd co s   

Multiply both sides of (1) bye j , subtract the original equation from
the

resulting equation ,
 e j N  1 
 AF  

j
e

1




j  N 1 
 AF  e 
2


 N
si
n



 2

 si n  1 


 2





 

 

…..(2)
• The phase factor exp[ j(N −1)ψ / 2] represents the phase shift of the array’s phase centre
relative to the origin, and it would be one if the origin coincides with the array centre.
• Neglecting the phase factor gives

 N
si
n



 2
AF  
 1

si n 


 2

For small values
of
,:




 
 
 
…..(3)

 N

si
n




 2


AF  









 2 


…..(4)
To normalize equation (3) or (4), we need the
maximum of the AF. Re-write equation (3) as:
 A F  m ax  N
f  x 
Equations 3 and 4 are written in normalized form as:

 N
si n 

1 
 2

 A F n 
N 
 1
si n 


 2

si n  N x 
N si n  x 
The function f(x) has its maximum at x = 0, ,
…, and the value of this maximum is fmax =1.




 

 

…..(5)

 N

si
n



1 
 2



 A F n 
N 
 





 2 


…..(6)
Nulls of the Array: Equations 5 and 6 are set equal to zero. That is,
 N
si n 
 2

N

2
   0
   n
 
2n


…..(7)
 n  co s 1 




n  1, 2 , 3, ....


N

 2 d 
n  N , 2 N , 3 N , .... because for these values of n, equation 5 attains its maximum value as

it reduces
si n  0  0
to
form.
n determine the order of the nulls (first, second, etc.).
The values of
For a zero to exist, the argument of arccosine must be between –1 and +1. nulls depend on d and
.The maximum of equation 5 occurs when,

2


1
2
 kd co s     |    m
m
 

 m  co s 1 
    2 m  
 2 d

AF has only one maximum and occurs when,
m  0
  0
That is, the observation angle that makes

…..(8)
m  0 , 1, 2 , 

 m  co s 1 

 2


d 
…..(9)
Secondary maxima/ Side lobe
maxima
Maxima of first sidelobe
The 3-dB point for the array factor of equation 6:
N
2

 
N
2
 kd co s     |    1 .3 9 1
h
 h  co s

1 

 2

 
d 

2 .7 8 2  


N

which can also be written as
h 

2
 si n
1 


 2

 
d 

2 .7 8 2  


N

For large values of d it reduces to:
…..(10)
The half power beamwidth is:
h  2
m h
…..(11)
Broadside Array
• Maximum radiation of an array directed normal to the axis of the array.
  90
• Maximum of the array factor occurs when (equations 5 and 6):
• For broadside array,
  kd co s     0
  kd co s    | 9 0   0
   0
• For broadside pattern, all elements should have same phase and amplitude excitation.
• To ensure that there are no maxima in other directions, which are referred to as grating lobes, the
separation between the elements should not be equal to multiples of a wavelength
  0 when
d=/4,N10
d=,N10
End-Fire Array
• An end-fire array is an array, which has its maximum radiation along the axis of the array (θ =0°, 180°).
• To direct the maximum toward θ =0°:
  kd co s    | 0      kd
• To direct the maximum toward θ =180°:
  kd co s    | 1 8 0     kd
If the element separation is a multiple of a wavelength
(d=n, n1,2,3,…), then there exists a maxima in the
broadside directions.
Phased (Scanning) Array
The 0th order maximum (m=0) of AFn occurs when
  kd co s     0
• This gives the relation between the direction of the main beam θ0 and the phase difference β .
The direction of the main beam can be controlled by the phase shift β . This is the basic
principle of electronic scanning for phased arrays.
• The scanning must be continuous. That is why the feeding system should be capable of
continuously varying the progressive phase β between the elements. This is accomplished by
ferrite or diode shifters (varactors).
Example:
Values of the progressive phase shift β as dependent on the direction of the main beam θ0
for a uniform linear array with d = λ/4.
   kd co s  0  

2
co s  0
0
0
60
120

-90
-45
45
180
90
The HPBW of a scanning array is obtained with β = −kdcosθ0:
 
2 .7 8 2  

 h 1, 2  co s 1 





2

d
N



The total beamwidth is
H PBW
H PBW

co s
1
  
 2  d  kd

  h1   h 2
co s
0 
2 .7 8 2
N

1   

co
s

 2  d  kd


co s
0 
2 .7 8 2
N



k  2
H P B W  co s
1 


co s  0

2 .7 8 2 
2 .7 8 2 
1 

 co s
co s  0 

N kd 
N kd 

If L is length of the array:
N 
H P B W  co s
1 
 co s  0

L  d
d






1 
 0 .4 4 3 
   co s

 co s  0  0 .4 4 3 
L

d


 L  d 

These equations can be used to calculate the HPBW of a broadside array, too (θ0 =90°=const ). However,
they are not valid for end-fire arrays.
N-Element Linear Array: Directivity
1. Broadside Array:
  0
The radiation intensity can be written as:
U      A F  
n 

2

 N

si
n
kd
co
s




2


 

  N kd co s  






  2

Z 

The directivity is
D
0

4 U
m ax
Pr a d

U
N
2
2
 si n  Z  
 

Z


kd co s 
m ax
U
0

Since the array factor is normalized, the numerator is unity and occurs
 at9 0
.
2

The Average Radiation Intensity can be written as:
U
0


1
Pr a d 
4
1
2


0
1
2

U 


4
0 0

 N

si
n
kd
co
s




 2



  N kd co s  






  2

 si n  d  d 
2
si n  d 
changing the variable
Z 
N
2
dZ  
U
0

1
N kd
N kd 2
  N kd
2
kd co s 
N
2
kd si n  d 
 si n Z 


Z


2
dZ
U
0

for a large array N kd
infinity.
1
N kd
N kd 2
  N kd
2
2  L ar g e 
 si n Z 


Z


2
dZ
the above equation can be approximated by extending the limits to
since
  si n Z 
   Z 
2
dZ  
The directivity is then,
For End fire array Do = ?
overall length of the array
L   N  1 d
For large L ( L much larger than d )
N-Element Linear Array: Uniform Spacing, Non-uniform Amplitude
•
The most often used Broad-Side Arrays (BSAs), are classified according to the type of their excitation
amplitude:
1. The uniform BSA – relatively high directivity, but the side-lobe levels are high;
2. Dolph–Tschebyscheff BSA – for a given number of elements maximum directivity is next after
that of the uniform BSA; side-lobe levels are the lowest in comparison with the other two types of
arrays for a given directivity;
3. Binomial BSA – does not have good directivity but has very low side-lobe levels (when d = λ/2,
there are no side lobes at all).
Even number (2M) of elements, located symmetrically along the z-axis, with excitation symmetrical
with respect to z = 0.
For a broadside array (β =0),
Odd number (2M+1) of elements, located symmetrically along the z-axis,
For a broadside array (β =0),
Binomial Array
1  x 
m 1
 1   m  1 x 
 m  1  m  2 
2!
x
2

 m  1  m  2   m  3 
3!
The positive coefficients of the series expansion:
1
m=1
1
m=2
1
m=3
1
m=4
1
m=5
m=6
1
2
3
4
5
1
1
3
6
10
1
4
10
Binomial BSA – when d = λ/2, there are no side lobes at all
1
5
1
x
3
 ...
An approximate closed-form expression for the HPBW with d = λ/2:
H PBW 
1 .0 6
N 1

1 .0 6
2L


1 .7 5
L 
The directivity with spacing d = λ/2 is
D
0
 1 .7 7
N  1 .7 7
2L    1
For a 10 element binomial array with a spacing of λ/2
between elements, determine the half power beam width
and the maximum directivity(in dB).
Dolph-Tschebyscheff Array
A compromise between uniform and binomial arrays.
Excitations coefficients are related to Tschebyscheff polynomials.
A Dolph-Tschebyscheff array with no sidelobes reduces to the binomial design. The excitation
coefficients for this case, as obtained by both methods would be identical.
Array Factor for symmetric amplitude excitation:
• Summation of M or (M+1) cosine terms.
• Largest harmonic of the cosine terms is one less than the total no. of elements of the
array.
• Each cosine term, whose argument is an integer times a fundamental frequency, can be
rewritten as a series of cosine functions with the fundamental frequency as the
argument.
If we let
z  co s uabove equations can be rewritten as:
And each is related to a Tschebyscheff (Chebyshev) polynomial
Tm  z 
T m  z   2 zT m 1  z   T m  2  z 
124
These relations between cosine functions and Tschebyscheff polynomials are valid only in the
range:
1  z  1

co s  m u   1
 Tm  z   1

for
1  z  1
The recursion formula for Tschebyscheff polynomials is:
T m  z   2 zT m 1  z   T m  2  z 

The polynomials can also be computed using:
T m  z   co s  m co s
1
 z  
T m  z   co sh  m co sh
1
 z  
 1  z  1
z   1, z   1

The first seven Tschebyscheff polynomials have
been plotted below:
Properties
• All polynomials pass through
• For
(1, 1)
1  z  1
 1  Tm  z    1
• All roots occur within
1  z  1
• All maxima and minima within this range have
values
1
126
PLANAR ARRAYS
• Planar arrays provide directional beams, symmetrical patterns with low side lobes, much higher
directivity (narrow main beam) than that of their individual element.
• In principle, they can point the main beam toward any direction. Can scan the beam in both the
planes.
• Applications – tracking radars, remote sensing, communications, etc.
If the axis of array has arbitrary orientation then array
factor is given by
If the axis of
array is along z
axis
The AF of a linear array of M elements along the x-axis is
M
A F x1 

m 1
I
me
j  m 1  kd x si n  co s    x 
si n  co s   co s 
x
directional cosine with respect to x-axis.
• All elements are equispaced with an interval of dx and a progressive shift βx.
• Im denotes the excitation amplitude of the element at the point with coordinates: x=(m-1)dx,
y=0.
•• This
is thearrays
element
the mnext
-th row
and the
1stincolumn
of the array
matrix. array is
If N such
are of
placed
to each
other
the y direction,
a rectangular
formed.
• We assume again that they are equispaced at a distance dy and there is a progressive
phase shift along each row of βy.
Then, the AF of the entire M×N array is
• The pattern of a rectangular array is the product of the array factors of the linear arrays in
the x and y directions.
• In the case of a uniform planar (rectangular) array, all elements have the same excitation
I m 1  I 1n  I 0
amplitudes:
M
AF  I 0 

e
j  m 1  kd x si n  co s    x 
N

m 1

e
j  n 1   kd
n 1
• The normalized array factor is obtained as:
A F n  , 

 1
  
 M


 M
si n 
 2

 1
si n 

2

 
 N
si
n


x   
1
2


 
   N
 1
si
n


x 


2
  


x
 kd x si n  co s  

y
 kd
y
si n  si n

x
  
y

y  


 
y 
 

y si n
 si n    y 
3-D PATTERN OF A 5-ELEMENT SQUARE PLANAR UNIFORM ARRAY WITHOUT GRATING LOBES (d=λ/4, βx=
βy=0 )
3-D PATTERN OF A 5-ELEMENT SQUARE PLANAR UNIFORM ARRAY WITHOUT GRATING LOBES (d=λ/2, βx=
βy=0 ):
Unit III
Practical Antennas
Yagi-uda antenna, Travelling wave antennas, V- Antenna,
Rhombic antenna, Microstrip antennas – Introduction,
Features, Advantages and Limitations, Rectangular
Patch Antennas – Geometry, Design equation and
Characteristics.
YAGI UDA ANTENNA
It is HF, VHF, UHF Antenna
It overcomes the drawback of non uniform array antenna.
1. Driven Element
Active element
A resonant half wave dipole’
Power supplied from source through transmission line
2. Reflector
Passive element
Not directly fed. Derives power by EM coupling
 Adds up fields of driven element in the direction from reflector towards the driven elemen
Length 5% more than driven element
3. Director
Passive element
Not directly fed. Derives power by EM coupling
 Adds up fields of driven element in the direction away from driven element past the director
Length 5% less than driven element
3 Element Yagi Uda Antenna
Endfire Array
Current lags
Current leads
One reflector and many driven elements
Z = 73+ j45 ohms
Space adjustment
Balun
Stubs
Quarter wave transformer
Folded dipole
PH = Id2RH
Pf=If2Rf
Id=I If=I/2
Increased impedance, Large bandwidth
Current flowing is unequal
Zin =73x r
Zin =73x (1+d2/d1)2
Long Wire Antenna/ Travelling wave Antenna/Harmonic
Antenna
K determines the orientation of main
beam
Two types of Long wire antenna
Non Resonant antenna
Resonant
antenna
EFA radiation pattern with a sharp null
V Antenna
Apex angle controls the
direction of main beam.
I
I /180
V antenna array
EFA
Distance between two elements is λ/4.
The phase difference in currents is 90 deg.
The fields cancel in backward direction and reinforce in forward direction.
Do not need a reflector to cancel in back radiation.
Gain doubles or triples depending on no. of elemetns.
V antenna array
BSA
Distance between two elements is λ/4.
Maximum radiation is in the direction of termination.
Rhombic Antenna
Each leg is made of two or three wires to achieve constant current along the
line.
Only P/8 power is wasted.
Microstrip Antenna
Microstrip antenna--G. A. Deschamps. In 1950s
Radiating patch on grounded
substrate
Geometry of Microstrip Patch
Photograph of Microstrip patch
Microstrip line Feed
 Fed by quarter wavelength transmission line
Different factors to be
 Inset feed
 Offset feed
feeding techniques:
Co-axial Probe feed
Proximity Coupled microstrip feed
 Aperture Coupled microstrip feed
considered for selecting
 Impedance matching
 Radiating structure and feed structure
 Minimization of spurious radiation
 Suitability of feed for array applications
Advantages:
 Simple
 Allows for planar feeding
 Easy to obtain input match
Disadvantages:
 Significant feedline radiation for thicker substrates
 For deep notches, pattern may show distortion.
Advantages:
 Feed can be placed in desired location
 Easy to locate
 Low spurious radiation
Disadvantages:
 Narrow bandwidth
 Easy to model
 Inner conductor causes impedance mismatch problems.
Disadvantages:
 Requires multilayer fabrication
 Alignment is important for input match
Advantages:
 Allows for planar feeding
 Feed-line radiation is isolated from patch radiation
 Higher bandwidth, since probe inductance restriction is eliminated for the substrate thickness, and
a double-resonance can be created.
 Allows for use of different substrates to optimize antenna and feed-circuit performance
Proximity (EMC) Coupling
Advantages:
 Allows for planar feeding
 Less spurious radiation compared to
microstrip feed
 The proximity coupling has the largest
bandwidth (as high as 13 %),
Disadvantages:
 Requires multilayer fabrication
 Alignment is important for input match
Microstrip Antenna Analysis
Analytical techniques
· The transmission line model
· The cavity model
· The MNM
Numerical techniques
· The method of moments (MoM)
. The finite-element method (FEM)
· The spectral domain technique (SDT)
· The finite-difference time domain (FDTD) method
Transmission-Line Model
It is the easiest of all available models
It yields the least accurate results
It gives good physical insight
Basically the transmission-line model represents the
microstrip antenna by two slots, separated by
transmission line of length L.
The discontinuity introduced by the rapid change in the line width at the junction
between the feed line and patch radiates.
No field
variation
along W and h
field lines on Microstrip line
Radiates in Broadside direction and Propagates quasi TEM wave.
Example
Design a rectangular microstrip antenna using a substrate (RT/
duroid 5880) with dielectric constant of 2.2, h = 0.1588 cm
(0.0625 inches) so as to resonate at 10 GHz.
Conductance
Rectangular microstrip patch and its equivalent circuit transmission-line model.
where for a slot of finite width W
Since slot #2 is identical to slot #1, its equivalent admittance is
Resonant Input Resistance
The total admittance at slot #1 (input admittance) is
obtained by transferring the admittance of slot #2
from the output terminals to input terminals using the
admittance transformation equation of transmission
lines
If the reduction of the length is properly chosen
(typically 0.48λ < L < 0.49λ), the transformed
admittance of slot #2 becomes
Broadband Techniques of MSA
Modified shaped patches
Planar multi-resonator configurations
Multilayer configurations
Stacked multi-resonator configurations
Impedance matching networks
Log periodic MSA configurations
Ferrite based broad band MSA
Improving Bandwidth
U-Shaped Slot
The introduction of a U-shaped slot can give a significant bandwidth
(10%-40%).
(This is due to a double resonance effect, with two different modes.)
Improving Bandwidth
Double U-Slot
A 44% bandwidth was achieved.
Improving Bandwidth
Parasitic Patches
Radiating Edges Gap Coupled Microstrip
Antennas (REGCOMA).
Non-Radiating Edges Gap Coupled
Microstrip Antennas (NEGCOMA)
Four-Edges Gap Coupled Microstrip
Antennas (FEGCOMA)
Improving Bandwidth
Direct-Coupled Patches
Radiating Edges Direct Coupled Microstrip
Antennas (REDCOMA).
Non-Radiating Edges Direct Coupled
Microstrip Antennas (NEDCOMA)
Four-Edges Direct Coupled Microstrip
Antennas (FEDCOMA)
Microstrip Antennas
Linear array (1-D corporate feed)
22 array
2-D 8X8 corporate-fed array
4  8 corporate-fed / series-fed array
UNIT-V
Concept and benefits of smart antennas,
Types of smart antennas, Beam forming
techniques, Smart antenna methods,
Algorithms.
Unit IV
Aperture and Modern Antennas
Reflector Antennas – Introduction, Flat Sheet and Corner Reflectors,
Paraboloidal Reflectors – Geometry, Pattern Characteristics, Feed
Methods, Reflector Types – Related Features, Illustrative Problems. Horn
Antennas – Types, Fermat’s Principle, Radiation from sectoral and
pyramidal horns, Design Considerations of Pyramidal Horns,
Reconfigurable antenna, Active antenna, Dielectric antennas, Electronic
band gap structure and applications.
Retro reflector
G =2.15dBi for dipole
. Here, shape of wave front is like a sheet of paper.
There is no direct source to generate collimated beam.
How to generate collimated beam ?
What should be shape of reflector?
Parabolic reflector generates collimated beam
Parabolic reflector converts spherical waves originated from
radiator at focus of parabola into a plane wave across the
mouth or aperture of parabola
Rays which do not strike the
reflector appear as
sidelobes. Minimized by
source shield.
Rays parallel to axis
converge
at focus. Others don’t due to
path length difference.
Types of parabolic reflectors
Parabolic cylinder / Cylindrical parabolic reflector
Generated by moving parabolic contour parallel to itself.
Focal line – provide large aperture blockage
Converts cylindrical to plane wavefront
Rectangular aperture
Source- dipole, Linear array BSA
Mechanically simpler
Generates fan beam
Pill box is short parabolic cylinder enclosed by a plate and fed by coaxial feed.
Importance of f/D ratio
Small f/ D ratio ---Deep dish
Feed is closer and can be small
Difficult to support and move mechanically
Spill over is less
Non uniform illumination - low efficiency.
Feeding Techniques
a)
b)
c)
d)
Axial feed
Offset feed
Cassegrain feed
Gregorian feed.
a) Axial feed
Blockage
Increased sidelobes
Impedance mismatch
Transmission line
losses
b) Offset feed
Horn is an antenna that consists of a flaring metal,
shaped like a horn.
What are Reconfigurable Antennas
Traditional Antennas
Designed for single predefined mission - fixed parameters (frequency, radiation pattern,
polarization, and gain).
Reconfigurable Antenna
It is the antenna capable of dynamically modifying its fundamental operating characteristics like
polarization, frequency and radiation pattern, to adapt to changing system requirements and
environmental conditions.
*It becomes most active part of communication link.
NEED FOR RECONFIGURABLE ANTENNAS
 Single Element and Array Scenario
Modern wireless communication systems demand
Multifunctional capabilities
High performance in transmission and reception
Desirable features like minimum weight, low cost, low profile
Traditional antenna
Smart / Adaptable antenna
Reconfigurable Antenna
Reconfiguration mechanism lies in the antenna
Support more than one wireless standard with good isolation
Improves communication link quality and capacity
Needs low front end processing
Classification of Reconfigurable Antennas
Reconfigurable Parameter
Polarization switching
Linear Polarization(LP)
Circular Polarization(CP)
LP, CP combinations
Discrete tuning
Continuous tuning
Single frequency
Multiple frequency
Narrow and Wide band
*Redirect, change or distribute CURRENT
Shape
Direction
Gain
Interesting
RECONFIGURATION TECHNIQUES
Easy to integrate
239
Linear behavior of switch
No switching Elements
Liquid crystal/Ferrite
CHALLENGES
 Needs careful analysis and design - Parameter linkage
 Conceptual design functionality deviates - Modeling complexity
 Single geometry - Multiple operating modes
 Reconfiguration mechanism - Actuation requirements & effects
 Reliability of reconfiguration mechanisms
 Huge computational resources.
Applications of Reconfigurable Antennas
Cognitive Radio System
Primary User - Owns the spectrum
Secondary User – Uses idle spectrum
Key Requirements of Cognitive Radio System
Isolation between ports
Substrate space
Omnidirectional radiation pattern
UWB
Antenna reconfigurability process
 Ultrathin, Light weight Laptop
Mobile Concept PC Utilizing Reconfigurable Antenna and Switching System
Multiband frequency reconfigurable antenna – Cellular and WLAN bands
Diversity board – connects RF modules and antennas
Microcontroller - controls switches on antenna and diversity switch logic
Field Programmable Gate Arrays (FPGAs) or Arduino Boards
Satellite Communication
Requirement – High gain – Deployable antennas
Reconfigurable Deployable Helical Antenna
Deployable reflector Antenna
240MHz to 450MHz
Gold-molybdenum mesh
Dielectric Resonator Antennas
DRAs rely on radiating resonators that can transform guided waves into unguided
waves
Aperture coupling is applicable to DRA of any
shape
Aperture behaves as magnetic current parallel to
slot
It excites magnetic fields in DRA
Feed below ground plane
No spurious radiations
Cancels reactive component of slot
Impedance match
Moving DRA with respect to slot.
Coupling level
Impedance tuning
Slot coupling becomes bulky below L-band
Aperture fed Rectangular
DRA
The probe can also be embedded within DRA
Coupling Adjustment
Probe height
Probe location
Mode of operation - Probe location with respect to DRA
Adjacent TE110
Center- TE011
Advantages:
Provides good coupling and hence efficiency
useful at lower frequency
No external impedance matching network is needed.
Microstrip coupling excites magnetic fields in DRA –
short horizontal magnetic dipole mode
Coupling
 lateral position of ms line wrt DRA
 dielectric constant of DRA
Fabricated DRA
Unit V
Wave propagation
Ground wave propagation. Space and
surface waves, Tropospheric refraction
and reflection. Sky wave propagation –
Virtual height, critical frequency, Maximum
usable frequency – Skip distance, Fading ,
Multi hop propagation.
Wave propagation
Wave propagation is the behavior of the wave when transmitted/
propagated from one point to other on earth through the atmosphere.
In free space wave propagates in TEM mode
Wave polarization is maintained as generated while propagating in free
space.
Ground wave or surface wave mode is used upto 2 MHz.
This mode exists when Tx and Rx antenna are near to earth.
Factors affecting the surface wave are
Frequency of operation
Earth surface(surface irregularities, , conductivity)
Tilt in wavefront of the wave
Frequency of operation
Surface waves follow the contour of the earth becau
Diffraction: Spreading out of waves as they pass through an aperture or
around objects.
Factors affecting Diffraction
Wavelength:
Wavelength of the incident wave plays an important role in determining
the magnitude of diffraction
For the same aperture size: Wave having a longer wavelength will be
diffracted more than shorter wavelength.
Size of aperture:
For same wavelength smaller aperture size diffracts to a much larger
extent as compared to the aperture with a larger size.
Size of Object:
The surface wave curves or bend around object if object size is smaller
than its wavelength.
*High frequencies will not be diffracted by objects but absorbed.
For low frequencies earth appears small and diffraction results in beyond horizon
propagation.
Large distance travel possible with low frequency and high power transmitters.
Earth Surface Irregularities Or Effect Of Earth
As surface travels over ground its induces voltage and it depends on earths  and 
Equivalent circuit of earth.
The induced voltage takes surface wave energy and contributes to attenuation
Attenuation depends on electrical properties of terrain.
Effect of wave polarization.
The best type of surface is one that has good
electrical conductivity.
Tilt in Wavefront
As the wave propagates over the earth, it tilts over more
and more. Eventually, at some distance from Tx, the wave
“lies down and dies.”
wave front which is travelling out from the antenna is
slowed slightly near the ground due to the refractive index
being higher than air. This has the effect of tilting the wave
front forward so that the bottom stays in contact with the
ground.
Maximum range of such a transmitter depends on its
frequency as well as its power. Thus, in the VLF band,
increasing the transmitting power works. This remedy will
not work near the top of the MF range, since propagation is
now definitely limited by tilt.
Field strength at a distance
Radiation from an antenna by means of Ground Wave Propagation gives rise to
a field strength at a distance, which may be calculated by use of Maxwell’s
equations.
The signal received by receiving antenna when placed at this point
**For large d, the reduction of field strength
due to ground and atmospheric
absorption
reduces V.
Space Wave Propagation
Ionospheric Wave Propagation
50
Ionospheric Wave Propagation
Ionosphere acts as a reflecting surface for waves from 2 to 30MHz.
Sky wave of suitable frequency can cover any distance round
earth.
D layer disappears at night.... the E and F layers
bounce the waves back to the earth. This explains
why radio stations adjust their power output at sunset
and sunrise.
A path calculated on the basis of a constant height of the
F2 layer will, if it crosses the terminator, undershoot and
miss the receiving area as shown the F layer over the
target is lower than the F2 layer over the transmitter.
n<1  sinI  sin r  i r
f>fc the wave escapes into atmosphere
fpfc
Secant Law
As i  fmuf 
Depends on N for
Curved Earth Surface????
Download