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8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 1
Radiation from Infinitesimal
(Elementary) Source
Radiation from Infinitesimal (Electric) Dipole
Duality in Maxwells Equations
Radiation from Infinitesimal Magnetic Dipole(Electric Current Loop)
Radiation Zones
TE4109 Antennas 2
Radiation from Infinitesimal Dipole (1)
Infinitesimal dipole very short current element
A very short piece of infinitesimally thin wire with constant currentdistribution
, /50l l
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TE4109 Antennas 3
Radiation from Infinitesimal Dipole (2)
Magnetic vector potential (VP) of a current element
( ) ( )4
PQj R
Q
PQL
eA P I Q dl
R
=
Recall that P is the observation point and Q is the source pointwhere integration takes place
( ) ( ) ( ) ( )4 4
PQ PQ
Q
j R j R
Q z
PQ PQL l
e eA P I Q dl A P Ia dl
R R
= =
The dipole is infinitesimally small, so the following approximation ishold
PQR r
TE4109 Antennas 4
Radiation from Infinitesimal Dipole (3)
Finally, Magnetic VP is given by
/ 2
/ 2( )
4
j rl
zl
I eA P a dl
r
=
4
j r
z eA a I lr
=
The above result is used in applications of the superpositionprinciple
4
j re
dA I dlr
=
The field radiated by any complex antenna in a linear medium canbe represented as a superposition of the fields due to currentelements.
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TE4109 Antennas 5
Radiation from Infinitesimal Dipole (4)
In antenna theory, the preferred coordinate system is the sphericalsystem.
cos( ) ( ) cos( )4
sin( ) ( ) sin( )4
0
j r
r z
j r
z
eA A I l
r
eA A I l
r
A
= =
= =
=
( , , ) ( , , ) ( , , ) ( , , )r rA r a A r a A r a A r = + +
Angular dependence is separable fromradial dependence.
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
TE4109 Antennas 6
Radiation from Infinitesimal Dipole (5)
Field vectors of a current element (see note for derivation)
They are vectors at a point in free space, specified by
1H A
=
( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , )r r
r r
H r a H r a H r a H rE r a E r a E r a E r
= + += + +
1( )sin( ) 1
4
0
j r
r
eH j I l
j r r
H H
= +
= =
( , , )r
The magnetic field
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TE4109 Antennas 7
Radiation from Infinitesimal Dipole (6)
The electric field
1( )
J jE A j A A
j j
= =
2
2
1 12 ( )cos( )
4
1 1( )sin( ) 1
( ) 4
0
j r
r
j r
eE I l
r j r r
eE j I l
j r r r
E
= +
= +
=
TE4109 Antennas 8
Radiation from Infinitesimal Dipole (7)
EM fields generated by the current element is rather complicatedunlike the VP.
The use of VP instead of the field vectors is usually advantageous inantenna studies
Features of the field vectors of a current element
Longitudinal components decrease with distance as 1/r2 or faster
Transverse component have a 1/r term dominant at large distances
Transverse electric and magnetic field components are orthogonal toeach other
In the far zone,
andE H
| | | | | | | |E H E H = =
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TE4109 Antennas 9
Radiated Power from Infinitesimal Dipole (1)
Power density (Poynting vector) of a current element
( ) ( )
( )
* *
* *
1 1 ( )
2 2
1
2
r r
r r r r
W E H a E a E a H
a E H a E H a W a W
= = +
= = +
2 2
2 2 3
2
2 3 2
( ) sin ( )1
8 ( )
( ) sin( )cos( ) 1116 ( )
0
r
I l jW
r r
I lW jr r
W
=
= +
=
TE4109 Antennas 10
Radiated Power from Infinitesimal Dipole (2)
Total power of a current element is calculated over surface of asphere
S
P W ds=
Surface vector is described by its normal vector and its area
2
sin( )s
r
ds a ds
a r d d
=
=
2 ( ) ( sin( ) )r r rS
P a W a W a r d d = +
Thus,
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
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TE4109 Antennas 11
Radiated Power from Infinitesimal Dipole (3)
Only the radial component of the Poynting vector contributes to theoverall power.
2
31 , W
3 ( )
I l jP
r
=
Radiated power is equal to the real part of the complex power.
2
, W3
rad
I lP
=
Radiation resistance of a current element (ideal dipole)
221 22
r r PP R I RI
= =
22
,3
id
r
lR
=
120 =
2
80 ,idr
lR
=
TE4109 Antennas 12
Duality in Maxwells Equations (1)Substituting the quantities from one set of EM equations with therespective quantities from the dual set produces a valid equation(the dual of the given one).
2 2
0
4
Electric Source ( 0, 0)
1
( )
j r
V
E j H
H j E J
DB
J j
A A J
eA J dv
r
H A
jE j A
M
A
J
=
= +
= =
=
+ =
=
=
=
=
2 2
0
4
Magnetic Source ( 0,
(
1
0)
)
m
m
j r
V
H j E
E j H M
BD
M j
F F M
eF M dv
r
E
J
j
M
F
jH F F
=
=
= =
=
+ =
=
=
=
=
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TE4109 Antennas 13
Duality in Maxwells Equations (2)
Dual Quantities
Given 1/
Dual 1/
E H J M A F
H E M J F A
TE4109 Antennas 14
Radiation from Infinitesimal Magnetic Dipole (1)
Infinitesimal magnetic dipole very short magnetic currentelement (exists in the text book only)
Magnetic current is assumed to be constant along the element
It is the duality of the infinitesimal electric dipole
Magnetic current is in the unit of V (volts)
Magnetic current is related to the magnetic current density by
mS
I M ds=
Electric vector potential
( ) ( )4
PQ
Q
j R
Q
PQv
eF P M Q dv
R
=
( ) ( ) , C/m4
PQ
Q
j R
m QL
PQ
eF P I Q dl
R
=
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 15
Radiation from Infinitesimal Magnetic Dipole (2)
In antenna theory, the preferred coordinate system is the sphericalsystem.
cos( ) ( ) cos( )4
sin( ) ( ) sin( )4
0
j r
r z m
j r
z m
eF F I l
r
eF F I l
r
F
= =
= =
=
( , , ) ( , , ) ( , , ) ( , , )r rF r a F r a F r a F r = + +
Angular dependence is separable fromradial dependence.
TE4109 Antennas 16
Radiation from Infinitesimal Magnetic Dipole (5)
Field vectors of a magnetic current element
They are vectors at a point in free space, specified by
1E F
=
( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , ) ( , , )
r r
r r
H r a H r a H r a H rE r a E r a E r a E r
= + += + +
1( )sin( ) 1
4
0
j r
m
r
eE j I l
j r r
E E
= +
= =
( , , )r
The electric field
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 17
Radiation from Infinitesimal Magnetic Dipole (6)
The magnetic field
1( )
M jH F j F F
j j
= =
2
2
2( )cos( ) 1 1
4
( )sin( ) 1 11
( ) 4
0
j r
mr
j r
m
I l eH
r j r r
j I l eH
j r r r
H
= +
= +
=
TE4109 Antennas 18
Magnetic Dipole and Electric-Current Loop (1)
Equivalence of the field excited by a magnetic dipole and anelectric-current loop
Since the magnetic current Im does not exist, we need to find its
physically-realizable equivalence in terms of electric current I
Considering two sets of Maxwells equations
1 1
1 1
21 1
Electric Current
E j H
H j E J
E E j J
=
= +
=
2 2
2 2
22 2
Magnetic Current
H j E
E j H M
E E M
=
=
=
1 2 1 2If , then andj J M E E H H = = =
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TE4109 Antennas 19
Magnetic Dipole and Electric-Current Loop (2)
This result relates the magnetic dipole to the electric-current loop
j J M =
Considering the surface S, enclosed by the closed path C
[ ] [ ]
( )C CS S
j J ds M ds =
Applying Stokes theorem
Cj I M dc =
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
TE4109 Antennas 20
Magnetic Dipole and Electric-Current Loop (3)
Magnetic current density is assumed nonzero and constant only at
the section l.
Cj I M dc =
j I M l =
[ ] m LI MA= [ ]L mj IA I l =
Small loop of electric current I and of area A[L] creates EM fieldequivalent to that of a small magnetic dipole (magnetic current
element) (Il)
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
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TE4109 Antennas 21
Fields of Infinitesimal Current Loop (1)
Fields of a small electric-current loop
[ ]L mj IA I l =
2
2
2
2
1( ) sin( ) 1 ,
4
1 12 ( )cos( ) ,
4
1 1( )sin( ) 1 ,
( ) 4
0.
j r
j r
r
j r
r
eE IA
j r r
eH j IA
r j r r
eH IA
j r r r
E E H
= +
= +
= +
= = =
In the far-field region the radial components have no far-field terms
E H
| | | | | | | |E H E H = =
TE4109 Antennas 22
Radiated Power from Infinitesimal Current Loop (1)
Power density (Poynting vector) of a small electric-current loop
( ) ( )
( )
* * *
* *
1 1 ( )
2 2
1
2
r r
r r r r
W E H a E a H a H
a E H a E H a W a W
= = +
= + = +
24 2
2 3
sin ( ) 1( ) 1
2 (4 ) ( )rW IA
r j r
=
Total power of a current loop is calculated over surface of a sphere
Only radial component of the Poynting vector contributes to theradiated power
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TE4109 Antennas 23
Radiated Power from Infinitesimal Current Loop (2)
Total power of a current element is calculated over surface of asphere
2 ( ) ( sin( ) )r r rS
P a W a W a r d d = +
4 2
3
1( ) 1 , W
12 ( )P IA
j r
=
Radiated power is equal to the real part of the complex power.
4 2( ) , W
12radP IA
=
Radiation resistance of a small electric-current loop
2
2
1 2
2 r r
PP R I R
I= = 4 2 ,
6md
radR A
=
TE4109 Antennas 24
Radiation Zones (1)
Space surrounding an antenna is divided into three regions
Reactive near-field region
Region immediately surrounding the antenna
Reactive field predominates
Radiating near-field (Fresnel) region
Radiation field is more significant but the angular field distribution isstill dependent on the distance from the antenna
Far-field (Fraunhofer) region
Angular field distribution does not depend on the distance from theantenna Spherical wave front
The field is a transverse EM wave
3
0.62 D
r
Largest dimension
of the antenna
D=
3 220.62
D Dr
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TE4109 Antennas 25
Radiation Zones (2)Amplitude pattern changes in
shape as the distance is variedfrom the reactive near field to the
far field due to variations of fieldmagnitude and phase
In the reactive near-field region,pattern is nearly uniform
In the far-field region, pattern iswell formed
Constantine A. Balanis, Antenna Theory, Analysis and Design, 3rd Ed., 2005
Constantine A. Balanis, Antenna Theory, Analysis and Design, 3rd Ed., 2005
TE4109 Antennas 26
Radiation Zones (3)
Study the general field behavior of the infinitesimal electric dipole.
2
2
1 12 ( )cos( )
4
1 1( )sin( ) 1
( ) 40
r r
j r
r
j r
E a E a E a E
eE I l
r j r r
eE j I l
j r r r
E
= + +
= +
= +
=
1( )sin( ) 1
4
0
r r
j r
r
H a H a H a H
eH j I l
j r r
H H
= + +
= +
= =
2 2
2 2 3
2
2 3 2
Complex Poynting Vector
( ) sin ( )1
8 ( )
( ) sin( )cos( ) 11
16 ( )
0
r r
r
W a W a W a W
I l jW
r r
I lW j
r r
W
= + +
=
= +
=
{ } { }2
3
Overall Power
Re Im
1 , W3 ( )
P P j P
I l jP
r
= +
=
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TE4109 Antennas 27
Reactive Near-Field Region
It is the region within the sphere having the radius of3
0.62 1D
r r
2
2
1( )sin( ) 1
4
1 12 ( )cos( )
4
1 1( )sin( ) 1
( ) 4
0
j r
j r
r
j r
r
eH j I l
j r r
eE I l
r j r r
eE j I l
j r r r
H H E
= +
= +
= +
= = =
2
3
3
( )sin( )
4
( )cos( )
4
( )sin( )
4
0
j r
j r
r
j r
r
I l eH
r
I l eE j
r
I l eE j
r
H H E
= = =
Electric field and magnetic field are in phase quadrature Field isreactive (ejr can be neglected)
{ } { }2 2
3
1Im Re
3 ( ) 3 rad
I l I lP P P
r
= = =
TE4109 Antennas 28
Radiating Near-Field (Fresnel) Region
Intermediate region between the reactive near-field region and thefar-field region
Radiation field is more significant but the angular field distributionstill depends is the distance from the antenna
3 220.62 1
D Dr r
Fields can be founded by ignoring the higher-order (1/r)n
-terms
2
( )sin( )
4
( )cos( )
2
( )sin( )
4
0
j r
j r
r
j r
r
I l eH j
r
I l eE
r
I l eE j
r
H H E
= = =
2
2
1( )sin( ) 1
4
1 12 ( )cos( )
4
1 1( )sin( ) 1
( ) 4
0
j r
j r
r
j r
r
eH j I l
j r r
eE I l
r j r r
eE j I l
j r r r
H H E
= +
= +
= +
= = =
Er is still not negligible, but the transverse components E and Hare dominant
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 29
Far-Field (Fraunhofer) Region (1)
Only terms 1/r are considered22
1D
r r
The field is transverse EM wave
( )sin( )
4
0( )
sin( )4
0
j r
r
j r
r
I l eH j
r
E
I l eE j
r
H H E
= = =
2
2
1( )sin( ) 1
4
1 12 ( )cos( )
4
1 1( )sin( ) 1
( ) 4
0
j r
j r
r
j r
r
eH j I l
j r r
eE I l
r j r r
eE j I l
j r r r
H H E
= +
= +
= +
= = =
TE4109 Antennas 30
Far-Field (Fraunhofer) Region (2)
Complex Poynting vector is in the radial direction
2 2
2 2 3
2
2 3 2
Complex Poynting Vector
( ) sin ( )
18 ( )
( ) sin( )cos( ) 11
16 ( )
0
r r
r
W a W a W a W
I l jW
r r
I lW j
r r
W
= + +
=
= +
=
2 2
2 2
Complex Poynting Vector
( ) sin ( )8
0
0
r r
r
W a W a W a W
I lW
r
W
W
= + +
=
=
0
EZ
H
= =2
21 1
2 2r r
EW a a H
= =
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 31
Radiation Separation (1)
Consider the VP integral for a linear current source
( )4
j R
L
eA I l dl
R
=
2 2 2( ) ( ) ( )R x x y y z z = + +
Size of an infinitesimalantenna is very small.
Distance between theintegration point and theobservation point isconsidered constant.
2 2 2R r x y z = + +http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
TE4109 Antennas 32
Radiation Separation (2)
As the maximum dimension of the antenna becomes comparable to
the wavelength, the error, especially in the phase term R,
increases.
1 1Amplitude Factor:
Phase Factor: Error in / 8 22.5
j R R r
e
R
r
< =
For an infinitesimally thin wire
2 2 2
2 2 2 2 2 2
0 ( )
( 2 ) 2 cos( )
x y R x y z z
R x y z z zz r z rz
= = = + +
= + + + = +
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TE4109 Antennas 33
Radiation Separation (3)
Using the binomial expansion and ignoring high-order terms
1 2 2 3 3( 1) ( 1)( 2)( ) ...2! 3!
n n n n nn n n n na b a na b a b a b
+ = + + + +
2 2 3 2
2
1 1cos( ) sin ( ) cos( )sin ( )
2 2R r z z z
r r + +
Only the first twoterms are taken into
account
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
TE4109 Antennas 34
Far-Field Approximation (1)
At the distance very far from the source
Only the first twoterms are taken intoaccount
z r
2 2 3 2
2
1 1cos( ) sin ( ) cos( )sin ( )
2 2
cos( )
R r z z zr r
R r z
+ +
http://www.ece.mcmaster.ca/faculty/nikolova/antenna_dload/current_lectures/L03_RadIS.pdf
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 35
Far-Field Approximation (2)
The minimum distance, at which the phase error is acceptable
32 2 2
2
1cos( ) cos( )sin ( )
2
The mo
1sin ( )
st significant error ter
2
m
zr
R r z zr
+ +
22 22 max
max
( )1 ( ) ( / 2)( ) sin ( ) ( )
2 2 2
zz De r e r
r r r
= = =
2( / 2) 2 8
D
r
2
2Dr
In addition, andr D r
TE4109 Antennas 36
Radiating Near-Field Approximation (1)
This region is adjacent to the Fraunhofer region, so its upperboundary is given by
22Dr
2 2 3 2
2
2 2
1 1cos( ) sin ( ) cos( )sin ( )
2 2
1cos( ) sin ( )
2
R r z z zr r
R r z zr
+ +
+
When the observation point is in this region, the approximation of Ris given by
8/10/2019 TE4109 Lecture06-07-Radiation From Infinitesimal (Elementary) Source
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TE4109 Antennas 37
Radiating Near-Field Approximation (2)
The minimum distance, at which the phase error is acceptable
2
2 3 221cos( ) sin ( )2
T
1cos( )sin ( )
he most significant error term
2R r zz z
r r + +
32
2
1 ( )( ) cos( )sin ( ) Maximum at arctan( 2) 54.7
2
ze r
r
= =
3
2
( / 2) 1 2
2 3 83
D
r
3 320.62
3 3
D Dr
=
2
1
3