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1
CHAPTER 1
INTRODUCTION
Microstrip patch antennas are widely used in wireless communications
due to their inherent advantages of low profile, less weight, low cost, and ease
of integration with microstrip circuits. However, the main disadvantage of
microstrip antennas is the small bandwidth. Improvement of broader bandwidth
becomes an important need for many applications such as for high speed
networks. Many methods have been proposed to improve the bandwidth. One of
the methods is introducing slots. To improve bandwidth in our project we
introduced 2 slots in microstrip patch and formed E-shaped antenna. Recently,
high-speed wireless computer networks have attracted the attention of
researchers, especially in the 5-6 GHz band .It finds applications in WiMax and
Indoor and Outdoor WLAN. WiMax frequency band ranging from 2 to 11 GHz
and the standard is IEEE802.16. Current 5 GHz wireless computer network
systems operate in the 5.15-5.35 GHz band, future systems may make use of the
5.72-5.85 GHz band in addition to the 5.15-5.35 GHz band, for even faster data
rates. Our resonant frequency is 5.8GHz. So we are choosing IEEE802.11a/g
network standard. Such networks have the ability to provide high- speed
connectivity (>50 Mb/s) between notebook computers, PCs, personal organizers
and other wireless digital appliances. Many novel antenna designs have been
proposed to suit the standard for high-speed wireless computer networks. The
Ansoft’s HFSS which is the industry standard simulation tool for 3D full-wave
electromagnetic field simulation based on Finite Element Method (FEM) has
been used for simulation. To improve the gain we made (1*2) array and it gives
better gain and better directivity.
2
CHAPTER 2
LITERATURE REVIEW
[1].Microstrip Antenna Array for WiMAX & WLAN Applications
This paper presents the design of microstrip rectangular patch antenna
with center frequency at 2.4 GHz for WiMAX and WLAN application. The
array of four by one (4x1) patch array with microstrip line feeding technique
was designed and simulated.The antenna array designed on Roger5880 substrate
with overall size of 200 x 100 x 1.59 mm3 and dielectric substrate with 𝜀𝑟 = 2.2.
Quarter-wave transformer is used to match the feeding line to the antennas. The
simulation return loss is equal to -32 dB & -30 dB at the freq. of 1.8 GHz & 2.4
GHz respectively. The dimension of the microstrip antenna also has an impact
on the antenna performance because the current is mainly distributed along the
edge on the radiator. The ground plane of the antenna design perform operation
as an impedance matching circuit, and it tunes the input impedance and hence
changes the operating bandwidth with variation of antenna feed size. The
performance was measured and it shows that the array antenna outperform the
single antenna in terms of directivity, bandwidth and gain.
[2].Coax-Fed E-Shaped Microstrip Patch Antenna with Triple Bands
This paper presents a method of designing the millimeter-wave E-Shaped
microstrip antenna which is very suitable for integration with wireless local area
network (WLAN) applications, widely used in the areas of mobile radio and
wireless communication applications, also found very useful in the field of
global navigation satellite systems(GNSS), global positioning system (GPS).
High Frequency Structure Simulator (HFSS) is a high- frequency simulation
software which is based on a finite element method and its accuracy and
powerful features makes it a common tool for antenna designers. The patch was
designed as rectangular shaped resonating on FR4_epoxy substrate with relative
permittivity dielectric constant of 4.4 and height (H) of 1.6mm. The length (L)
of the patch is 27.99mm and width (W) is 37.2 mm. The area of the ground
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plane sets 74.4 × 55.98 mm2 . To obtain the desired optimum performance in
terms of VSWR and radiation pattern, two rectangular slots with dimension of
19.1mm x 8mm were cut out from both the upper and lower side of the
rectangular patch thus forming the E-shaped patch shape which in turn yields a
significant improvement in terms of the VSWR that became less than two
(VSWR <2) for all the three frequency bands. The two slots were separated by a
distance of 8mm.The designed antenna can achieve triple band performance to
simultaneously cover the 1.18GHz, 2.42GHz and 4.05GHz frequency with
return loss of -12.50dB, -12.60dB and -15.50dB respectively. Good return loss
and radiation pattern characteristics were all obtained in the frequency band of
interest.
[3].Microstrip Patch Antenna for WiMax/WLAN Applications
This paper contains microstrip patch antenna designed with Inset feed
technique. The antenna is mainly intended to be used for WiMAX (2.2-3.4
GHz) & WLAN (2.40–2.48 GHz) wireless applications. The ground plane
dimensions have given as 100×100 mm and patch dimension 35.4×45.6 mm.
The di-electric material of the substrate (εr) selected for this design is glass
epoxy which has a dielectric constant of 4.4 and loss tangent equal to 0.001. The
proposed antenna resonates at 1.65 GHz frequency and has frequency range
from 1.01 to 2.62 GHz giving a wide band width of 88.57%, and maximum
radiating efficiency of about 99%.
[4].Slotted Rectangular Microstrip Antenna for Bandwidth Enhancement
In this paper the bandwidth enhancement of microstrip antennas is
demonstrated by the loading of a pair of right-angle slots and a modified U-
shaped slot in a rectangular microstrip patch. The rectangular patch has
dimensions of 37.3 mm 24.87 mm and is printed on a grounded FR4 substrate of
thickness 1.6 mm, relative permittivity ) 4.4, and size 60 mm 50 mm. In the
proposed antenna, the longer arm of the right-angle slots is in parallel to the
nonradiating edges and its arm length needs to be about 90% of the patch
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length; the shorter arm is perpendicular to the nonradiating edges and its arm
length should be greater than 40% of the patch width. t the fundamental
resonant frequency of the unslotted rectangular patch antenna is at about 1.9
GHz, with an operating bandwidth of 1.9%. Since the obtained antenna
bandwidths are as large as 4.3–4.6%, the proposed antennas show a much
greater operating bandwidth, more than 2.2 times that of an unslotted
rectangular patch antenna.
5
CHAPTER 3
ANTENNA PARAMETERS
An antenna is an electrical conductor or system of conductors Transmitter
- Radiates electromagnetic energy into space Receiver - Collects
electromagnetic energy from spaceThe IEEE definition of an antenna as given
by Stutzman and Thiele is, “That part of a transmitting or receiving system that
is designed to radiate or receive electromagnetic waves”. The major parameters
associated with an antenna are defined in the following sections.
3.1.ANTENNA GAIN
Gain is a measure of the ability of the antenna to direct the input power
into radiation in a particular direction and is measured at the peak radiation
intensity. Consider the power density radiated by an isotropic antenna with input
power P0
at a distance R which is given by S = P0/4πR
2. An isotropic antenna
radiates equally in all directions, and it’s radiated power density S is found by
dividing the radiated power by the area of the sphere 4πR2.An isotropic radiator
is considered to be 100% efficient. The gain of an actual antenna increases the
power density in the direction of the peak radiation:
Equation 3.1
Gain is achieved by directing the radiation away from other parts of the
radiation sphere. In general, gain is defined as the gain-biased pattern of the
antenna.
6
Equation 3.2
3.2.ANTENNA EFFICIENCY
The surface integral of the radiation intensity over the radiation sphere
divided by the input power P0
is a measure of the relative power radiated by the
antenna, or the antenna efficiency.
Equation 3.3
Where Pr is the radiated power. Material losses in the antenna or reflected
power due to poor impedance match reduce the radiated power.
3.3.EFFECTIVE AREA
Antennas capture power from passing waves and deliver some of it to the
terminals. Given the power density of the incident wave and the effective area
of the antenna, the power delivered to the terminals is the product.
Equation 3.4
For an aperture antenna such as a horn, parabolic reflector, or flat-plate
array, effective area is physical area multiplied by aperture efficiency. In
general, losses due to material, distribution, and mismatch reduce the ratio of
the effective area to the physical area. Typical estimated aperture efficiency for
a parabolic reflector is 55%. Even antennas with infinitesimal physical areas,
such as dipoles, have effective areas because they remove power from passing
waves.
7
3.4.DIRECTIVITY
Directivity is a measure of the concentration of radiation in the direction
of the maximum.
Equation 3.5
Directivity and gain differ only by the efficiency, but directivity is easily
estimated from patterns. Gain—directivity times efficiency—must be measured.
The average radiation intensity can be found from a surface integral over the
radiation sphere of the radiation intensity divided by 4π, the area of the sphere
in steradians:
Equation 3.6
This is the radiated power divided by the area of a unit sphere. The
radiation intensity U(θ,φ) separates into a sum of co- and cross-polarization
components:
Equation 3.7
Both co- and cross-polarization directivities can be defined:
8
Equation 3.8
Directivity can also be defined for an arbitrary direction D(θ,φ) as
radiation intensity divided by the average radiation intensity, but when the
coordinate angles are not specified, we calculate directivity at Umax
3.5.PATH LOSS
We combine the gain of the transmitting antenna with the effective area of
the receiving antenna to determine delivered power and path loss. The power
density at the receiving antenna is given by equation 3.2 and the received power
is given by equation 3.4. By combining the two, we obtain the path loss as given
below.
Equation3.9
Antenna 1 transmits, and antenna 2 receives. If the materials in the
antennas are linear and isotropic, the transmitting and receiving patterns are
identical . When we consider antenna 2 as the transmitting antenna and antenna
1 as the receiving antenna, the path loss is
Equation 3.10
We make quick evaluations of path loss for various units of distance R
and for frequency f in megahertz using the formula
Equation 3.11
where KU
depends on the length units as shown below
9
3.6.INPUT IMPEDANCE
The input impedance of an antenna is defined as “the impedance
presented by an antenna at its terminals or the ratio of the voltage to the current
at the pair of terminals or the ratio of the appropriate components of the electric
to magnetic fields at a point”. Hence the impedance of the antenna can be
written as given below.
Equation 3.12
where Zin
is the antenna impedance at the terminals
Rin
is the antenna resistance at the terminals
Xin
is the antenna reactance at the terminals
The imaginary part, Xin
of the input impedance represents the power stored
in the near field of the antenna. The resistive part, Rin
of the input impedance
consists of two components, the radiation resistance Rrand the loss resistance
RL. The power associated with the radiation resistance is the power actually
radiated by the antenna, while the power dissipated in the loss resistance is lost
as heat in the antenna itself due to dielectric or conducting losses.
10
3.7.ANTENNA FACTOR
The engineering community uses an antenna connected to a receiver such
as a spectrum analyzer, a network analyzer, or an RF voltmeter to measure field
strength E. Most of the time these devices have a load resistor ZL that matches
the antenna impedance. The incident field strength Ei equals antenna factor AF
times the received voltage Vrec
.
We relate this to the antenna effective height:
Equation 3.13
AF has units meter−1
but is often given as dB(m−1
). Sometimes, antenna
factor is referred to the open-circuit voltage and it would be one-half the value
given by equation 3.13. We assume that the antenna is aligned with the electric
field; in other words, the antenna polarization is the electric field component
measured:
Equation 3.14
This measurement may be corrupted by a poor impedance match to the
receiver and any cable loss between the antenna and receiver that reduces the
voltage and reduces the calculated field strength.
3.8.RETURN LOSS
It is a parameter which indicates the amount of power that is “lost” to the
load and does not return as a reflection. Hence the RL is a parameter to indicate
how well the matching between the transmitter and antenna has taken place.
Simply put it is the S11 of an antenna. A graph of s11 of an antenna vs
11
frequency is called its return loss curve. For optimum working such a graph
must show a dip at the operating frequency and have a minimum dB value at
this frequency. This parameter was found to be of crucial importance to our
project as we sought to adjust the antenna dimensions for a fixed operating
frequency. A simple RL curve is shown in figure 3.1.
Figure 3.1: RL curve of an antenna
3.9.RADIATION PATTERN
The radiation pattern of an antenna is a plot of the far-field radiation
properties of an antenna as a function of the spatial co-ordinates which are
specified by the elevation angle (θ) and the azimuth angle (φ). More specifically
it is a plot of the power radiated from an antenna per unit solid angle which is
nothing but the radiation intensity. It can be plotted as a 3D graph or as a 3D
polar or Cartesian slice of this 3D graph. It is an extremely parameter as it
shows the antenna’s directivity as well as gain at various points in space. It
serves as the signature of an antenna and one look at it is often enough to realize
the antenna that produced it. Because this parameter was so important to our
software simulations we needed to understand it completely.
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3.10.BEAMWIDTH
Beamwidth of an antenna is easily determined from its 2D radiation
pattern and is also a very important parameter. Beamwidth is the angular
separation of the half-power points of the radiated pattern. The way in which
beamwidth is determined is shown in figure 3.2.
Figure 3.2: Determination of HPBW from radiation pattern
3.11.VSWR
The parameter VSWR is a measure that numerically describes how well
the antenna is impedance matched to the transmission line it is connected to.
VSWR stands for Voltage Standing Wave Ratio and is also referred to Standing
Wave Ratio. VSWR is a function of reflection coefficient which describes the
power reflected from the antenna . If the reflection coefficient is given by ,then
VSWR is defined by
VSWR=1+|| / 1+|| Equation 3.15
13
VSWR is always a real number. Smaller VSWR better the antenna is
matched to transmission line and more power is delivered to antenna. The
minimum VSWR is 1. In this case no power is reflected from the antenna which
is ideal. The voltage would have a constant magnitude along the transmission
line. Practically VSWR under 2 is accepted. VSWR measures the potential to
radiate VSWR alone is not sufficient to determine an antenna is functioning
properly
3.12.BANDWIDTH
The bandwidth of the patch is defined as the frequency range over which
it is matched with that of the feed line within specified limits . In other words,
the frequency range over which the antenna will perform satisfactorily. This
means the channels have larger usable frequency range and thus results in
increased transmission. The bandwidth of an antenna is usually defined by the
acceptable standing wave ratio (SWR) value over the concerned frequency
range.
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CHAPTER 4
TYPES OF ANTENNAS
Antennas can be classified in several ways. One way is the frequency
band of operation. Others include physical structure and
electrical/electromagnetic design. Most simple, non-directional antennas are
basic dipoles or monopoles. More complex, directional antennas consist of
arrays of elements, such as dipoles, or use one active and several passive
elements, as in the Yagi antenna. New antenna technologies are being
developed that allow an antenna to rapidly change its pattern in response to
changes in direction of arrival of the received signal. These antennas and the
supporting technology are called adaptive or “smart” antennas and may be used
for the higher frequency bands in the future. A few commonly used antennas are
described in the following sections.
4.1.YAGI-UDA ANTENNA
Yagi-uda or simply Yagi antennas are the most high gain antennas and
are known after the names of professor S.Uda and Yagi. This antenna consists
of a driven element, a reflector and one or more directors. The driven element is
a resonant half wave dipole usually of metallic rod at the frequency of
operation. The parasitic elements of continuous metallic rods are arranged
parallel to the driven element and at the same line of sight level. The parasitic
elements receive their excitation from the voltages induced by the current flow
in the driver element. The phase and currents flowing due to induced voltage
depend on the spacing between the elements and the reactance of the element.
Fig 4.1:Yagi-UdaAntenna
15
4.2.FOLDED DIPOLE ANTENNA
A dipole antenna consists of two conductors extending in opposite
directions, with a total length that is often, but not always, a half of a
wavelength long. Dipoles are typically oriented horizontally in which case they
are weakly directional: signals are reasonably well radiated toward or received
from all directions with the exception of the direction along the conductor itself;
this region is called the antenna blind cone or null.
Figure 4.2: Dipole antenna
4.3. HELICAL ANTENNA
Helical antenna is the another type of radiator and perhaps it is the
simplest antenna to provide the circularly polarized waves or nearly so which
are used in extra terrestrial communications in which satellite relays are
involved. Helical antenna is broad band VHF and UHF antenna to provide
circular polarization characteristics. It consists of a helix of thicker copper wire
or tubing wound in the shape of a screw thread and used as an antenna with a
flat metal plate called a ground plate.
4.4. Corner Reflector An antenna comprised of one or more dipole elements in front of a
corner reflector, called the corner-reflector antenna, is illustrated in figure 4.3
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Figure 4.3: Corner-reflector antennas
This antenna has moderately high gain, but its most important pattern
feature is that the forward (main beam) gain is much higher than the gain in the
opposite direction. This is called the front-to-back ratio.
4.5.Microstrip( Patch ) Antennas In spacecraft or aircraft applications, where size, weight, cost,
performance, ease of installation and aerodynamic profile are constraints, low
profile antennas are required. In order to meet these specifications Microstrip or
patch antennas are used. Microstrip patch antennas are popular for low profile
applications at frequencies above 100 MHz. They usually consists of a very thin
metallic strip or patch on a dielectric –coated ground plane (circuit board).
17
CHAPTER 5
MICROSTRIP PATCH ANTENNA In its basic form, a Microstrip Patch antenna consists of a radiating patch
on one side of a dielectric substrate which has a ground plane on the other side
as shown in Figure.5.1.
Figure 5.1:Microstrip patch antenna
The patch is normally made of conducting material such as copper or gold
and can take any possible shape. The radiating patch and the feed lines are
usually photo etched on the dielectric substrate.
In order to simplify analysis and performance estimation, generally
square, rectangular, circular, triangular, and elliptical or some other common
shape patches are used for designing a microstrip antenna.
For a rectangular patch, the length L of the patch is usually 0.3333λo<L <
0.5 λo, where λo is the free-space wavelength. The patch is selected to be very
thin such that t<<λo (where t is the patch thickness). The height h of the
dielectric substrate is usually 0.003λo≤h≤0.05 λo. The dielectric constant of the
substrate (εr) is typically in the range 2.2 ≤ εr≤12.
Microstrip patch antennas radiate primarily because of the fringing fields
between the patch edge and the ground plane. For good performance of antenna,
a thick dielectric substrate having a low dielectric constant is necessary since it
18
provides larger bandwidth, better radiation and better efficiency. However, such
a typical configuration leads to a larger antenna size. In order to reduce the size
of the Microstrip patch antenna, substrates with higher dielectric constants must
be used which are less efficient and result in narrow bandwidth. Hence a trade-
off must be realized between the antenna performance antenna and dimensions.
Figure 5.2: Typical patch shapes
5.1. PROPERTIES OF A BASIC MICROSTRIP PATCH A microstrip or patch antenna is a low profile antenna that has a number
of advantages over other antennas it is lightweight, low cost, and easy to
integrate with accompanying electronics. While the antenna can be 3D in
structure (wrapped around an object, for example), the elements are usually flat;
Hence their other name, planar antennas. The figure 5.3 shows a patch antenna
in its basic form: a flat plate on a ground plane. The center conductor of a coax
serves as the feed probe to couple electromagnetic energy in and/or out of the
patch. The electric field distribution of a rectangular patch in its fundamental
mode is also shown.
Figure 5.3: Basic microstrip patch antenna with probe feeding
19
The electric field is zero at the center of the patch, maximum (positive) at
one side, and minimum (negative) on the opposite side. It should be mentioned
that the minimum and maximum continuously change side according to the
instantaneous phase of the applied signal. The electric field does not stop
abruptly at the patch's periphery as in a cavity rather the fields extend the outer
periphery to some degree. These field extensions are known as fringing fields
and cause the patch to radiate. Some popular analytic modeling techniques for
patch antennas are based on this leaky cavity concept. Therefore, the
fundamental mode of a rectangular patch is often denoted using cavity theory as
the TM10 mode.
Since this notation frequently causes confusion, we will briefly explain it.
TM stands for transversal magnetic field distribution. This means that only three
field components are considered instead of six. The field components of interest
are: the electric field in the z direction, and the magnetic field components in x
and y direction using a Cartesian coordinate system, where the x and y axes are
parallel with the ground plane and the z axis is perpendicular.
In general, the modes are designated as TMnmz. The z value is mostly
omitted since the electric field variation is considered negligible in the z axis.
Hence TMnm remains with n and m the field variations in x and y direction.
The field variation in the y direction (impedance width direction) is negligible;
thus m is 0. And the field has one minimum to maximum variation in the x
direction (resonance length direction); thus n is1 in the case of the fundamental.
5.2.DIMENSIONS
The resonant length determines the resonant frequency and is about l/2
for a rectangular patch excited in its fundamental mode. The patch is, in fact,
electrically a bit larger than its physical dimensions due to the fringing fields.
The deviation between electrical and physical size is mainly dependent on the
PC board thickness and dielectric constant.
20
A better approximation for the resonant length is:
Equation 5.1 This formula includes a first order correction for the edge extension due to the
fringing fields, with:
L = resonant length
λd = wavelength in PC board
λo = wavelength in free space
εr = dielectric constant of the PC board material
Other parameters that will influence the resonant frequency:
Ground plane size
Metal (copper) thickness
Patch (impedance) width
5.3.METHODS TO ENHANCE GAIN IN MICROSTRIP PATCH
ANTENNA
Most compact microstrip antenna designs show decreased antenna gain
owing to the antenna size reduction. To overcome this disadvantage and obtain
an enhanced antenna gain, several designs for gain-enhanced compact
microstrip antennas with the loading of a high permittivity dielectric superstrate
or the inclusion of an amplifier-type active circuitry have been demonstrated.
Use of a high-permittivity superstrate loading technique gives an increase in
antenna gain of about 10dBi with a smaller radiating patch. An amplifier-type
active microstrip antenna as a transmitting antenna with enhanced gain and
bandwidth has also been implemented.
5.4.APPLICATIONS OF MICROSTRIP PATCH ANTENNAS
Microstrip patch antennas are increasing in popularity for use in wireless
applications due to their low-profile structure. Therefore they are extremely
21
compatible for embedded antennas in handheld wireless devices such as cellular
phones, pagers etc. The telemetry and communication antennas on missiles need
to be thin and conformal and are often microstrip patch antennas. Another area
where they have been used successfully is in satellite communication.
5.5.ADVANTAGES AND DISADVANTAGES OF PATCH ANTENNAS
Some of their principal advantages of microstrip patch antennas are given
below:
• Light weight and low volume.
• Low profile planar configuration which can be easily made conformal to
host surface
• Low fabrication cost, hence can be manufactured in large quantities.
• Supports both, linear as well as circular polarization.
• Can be easily integrated with microwave integrated circuits (MICs).
• Capable of dual and triple frequency operations.
• Mechanically robust when mounted on rigid surfaces.
Microstrip patch antennas suffer from a number of disadvantages as
compared to conventional antennas. Some of their major disadvantages are
given below:
• Narrow bandwidth
• Low efficiency
• Low Gain
• Extraneous radiation from feeds and junctions
• Poor end fire radiator except tapered slot antennas
• Low power handling capacity.
• Surface wave excitation
Microstrip patch antennas have a very high antenna quality factor (Q). Q
represents the losses associated with the antenna and a large Q leads to narrow
bandwidth and low efficiency. Q can be reduced by increasing the thickness of
the dielectric substrate. But as the thickness increases, an increasing fraction of
the total power delivered by the source goes into a surface wave. This surface
22
wave contribution can be counted as an unwanted power loss since it is
ultimately scattered at the dielectric bends and causes degradation of the antenna
characteristics. However, surface waves can be minimized by use of photonic
bandgap structure. Other problems such as low gain and low power handling
capacity can be overcome by using an array configuration for the elements.
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CHAPTER 6
FEED TECHNIQUES
Microstrip patch antennas can be fed by a variety of methods. These
methods can be classified into two categories- contacting and non-contacting. In
the contacting method, the RF power is fed directly to the radiating patch using
a connecting element such as a microstrip line. In the non-contacting scheme,
electromagnetic field coupling is done to transfer power between the microstrip
line and the radiating patch. The four most popular feed techniques used are the
microstrip line, coaxial probe (both contacting schemes), aperture coupling and
proximity coupling (both non-contacting schemes).
6.1.MICROSTRIP LINE FEED
In this type of feed technique, a conducting strip is connected directly to
the edge of the microstrip patch as shown in Figure 3.4. The conducting strip is
smaller in width as compared to the patch and this kind of feed arrangement has
the advantage that the feed can be etched on the same substrate to provide a
planar structure.
Figure 5.1: Microstrip Line Feed
24
The purpose of the inset cut in the patch is to match the impedance of the
feed line to the patch without the need for any additional matching element.
This is achieved by properly controlling the inset position. Hence this is an easy
feeding scheme, since it provides ease of fabrication and simplicity in modeling
as well as impedance matching. However as the thickness of the dielectric
substrate being used, increases, surface waves and spurious feed radiation also
increases, which hampers the bandwidth of the antenna. The feed radiation also
leads to undesired cross polarized radiation. The performance analysis of
different feeding techniques are given below. Since microstrip feed has better
performance characteristics we have chosen microstrip feeding technique.
Table6.1:Performance characteristics of feeding techniques
25
CHAPTER 7
SUBSTRATE
The dielectric constant plays a major role in the overall performance of
the antenna. It affects both the width, in turn the characteristic impedance and
the length resulting in an altered resonant frequency and reduced transmission
efficiency. we are using the FR4 substrate with the permittivity 4.4.
7.1.FR4 SUBSTRATE
"FR" stands for flame retardant.FR-4 (or FR4) is a grade designation
assigned to glass-reinforced epoxy laminate sheets, tubes, rods and printed
circuit boards (PCB).
FR-4 glass epoxy is a popular and versatile high-pressure thermoset
plastic laminate grade with good strength to weight ratios. With near zero water
absorption, FR-4 is most commonly used as an electrical insulator possessing
considerable mechanical strength. The material is known to retain its high
mechanical values and electrical insulating qualities in both dry and humid
conditions. These attributes, along with good fabrication characteristics, lend
utility to this grade for a wide variety of electrical and mechanical applications.
26
CHAPTER 8
HFSS SOFTWARE
8.1. INTRODUCTION
HFSS is antenna simulation software. Besides that it can be used in the
design of an integrated circuit, a high speed interconnect or any other type of
electronic component, HFSS often is used during the design stage, and is an
integral part of the design process.
8.2.THE MATHEMATICAL METHOD USED BY HFSS HFSS™ uses a numerical technique called the Finite Element Method
(FEM). This is a procedure where a structure is subdivided into many smaller
subsections called finite elements. The finite elements used by HFSS are
tetrahedral, and the entire collection of tetrahedral is called a mesh. A solution is
found for the fields within the finite elements, and these fields are interrelated so
that Maxwell’s equations are satisfied across inter-element boundaries. Yielding
a field solution for the entire, original, structure. Once the field solution has
been found, the generalized S-matrix solution is determined.
27
Figure 8.1: Mathematical method used by HFSS
Mathematically, HFSS solves for the electric field E using equation 8.1 subject
to excitations and boundary conditions.
Equation 8.1 Where HFSS calculates the magnetic field H using equation:
Equation 8.2 The remaining electromagnetic quantities are derived using the
constitutive relations. In practice, to calculate the fields and S-matrix associated
with a structure with ports, HFSS derives a finite element matrix using the
above field equations. The following shows, in principle, the procedure that
HFSS follows:
1. Divide the structure into a finite element mesh using tetrahedral elements.
2. Define testing functions Wn, for each tetrahedron, resulting in thousands
of basis functions.
3. Multiply field equation 8.1 by a Wn and integrate over the solution
volume.
Equation 8.3 This procedure yields thousands of equations for n=1,2,…,N
28
Manipulating the N equations, using Green’s theorem and the divergence
theorem yields:
Equation 8.3a For n=1,2,…,N ,
Equation 8.4 rewrites (8.3a) as
Equation 8.5 For n=1,2,…,N Equation (6.5) then has the form
Equation 8.6 Or
Equation 8.7 In the matrix equation, A is a known NxN matrix that includes any
applied boundary condition terms, while b contains the port excitations, voltage
and current sources and incident waves. Once you have solved for x, from equation 8.4, you know E. The above
process is performed automatically by HFSS and is fully independent of user
interaction. HFSS uses the above process repeatedly, changing the mesh in a
very deliberate manner, until the correct field solution is found. This repetitive
process is known as the adaptive iterative solution process and is a key to the
highly accurate results that HFSS provides.
8.3. THE ADAPTIVE SOLUTION PROCESS IMPORTANCE TO HFSS
The adaptive solution process is the method by which HFSS
guarantees that a final answer to a given EM problem is the correct answer.
It is a necessary part of the overall solution process and is the key reason
why a user can have extreme confidence in HFSS’s accuracy.
29
Figure 8.2.Adaptive solution process
8.4.THE SIX GENERAL STEPS IN AN HFSS SIMULATION There are six main steps to creating and solving a proper
HFSS simulation. They are:
1.Create model/geometry
2.Assign boundaries
3.Assign excitations
4. Set up the solution
5.Solve 6.Post-process the results
30
Fig 8.3: General steps in HFSS simulation
Every HFSS simulation will involve, to some degree, all six of the
above steps. While it is not necessary to follow these steps in exact order, it is
good modeling practice to follow them in a consistent model-to-model manner. Step one: The initial task in creating an HFSS model consists of the creation of
the physical model that a user wishes to analyze. This model creation can be
done within HFSS using the3D modeler. The 3D modeler is fully parametric
and will allow a user to create a structure that is variable with regard to
geometric dimensions and material properties. A parametric structure, therefore,
is very useful when final dimensions are not known or design is to be “tuned.”
Alternatively, a user can import 3D structures from mechanical drawing
packages, such as SolidWorks®, Pro/E® or AutoCAD®. Geometry, once
imported into HFSS, can be modified within the 3D modeling environment.
This will then create geometry that can be parameterized. Step two: The assignment of “boundaries” generally is done next. Boundaries
are applied to specifically created 2D (sheet) objects or specific surfaces of 3D
objects. Boundaries have a direct impact on the solutions that HFSS provides;
therefore, users are encouraged to closely review the section on Boundaries in
this document. Step Three: After the boundaries have been assigned, the excitations (or
ports)should be applied. As with boundaries, the excitations have a direct
impact on the quality of the results that HFSS will yield for a given model.
31
Because of this, users are again encouraged to closely review the section on
excitations in this document. While the proper creation and use of excitations is
important to obtaining the most accurate HFSS results, there are several
convenient rules of thumb that a user can follow. These rules are described in
the excitations section.
Step Four: Once boundaries and excitations have been created, the next step is
to create a solution setup. During this step, a user will select a solution
frequency, the desired convergence criteria, the maximum number of adaptive
steps to perform, a frequency band over which solutions are desired, and what
particular solution and frequency sweep methodology to use. Step Five: When the initial four steps have been completed by an HFSS user,
the model is now ready to be analyzed. The time required for an analysis is
highly dependent upon the model geometry, the solution frequency, and
available computer resources. A solution can take from a few seconds, to the
time needed to get a coffee, to an overnight run. It is often beneficial to use the
remote solve capability of HFSS to send a particular simulation run to another
computer that is local to the user’s site. This will free up the user’s PC so it can
be used to perform other work. Step six: Once the solution has finished, a user can post-process the results.
Post processing of results can be as simple as examining the S-parameters of the
device modeled or plotting the fields in and around the structure. Users can also
examine the far fields created by an antenna. In essence, any field quantity or
S,Y,Z parameter can be plotted in the post-processor. Additionally, if a
parameterized model has been analyzed, families of curves can be created.
8.5.SOLUTION TYPES
HFSS has three solution types. The Driven Modal solution type is used
for most HFSS simulations, especially those that include passive, high-
frequency structures such as microstrips, waveguides, and transmission lines.
For simulations that deal with Signal Integrity issues, the Driven
Terminal Mode, is used. These simulations generally include models that have
32
multi-conductor transmission lines.
The Eigen mode solver will provide results in terms of Eigenmodes or
resonances of a given structure. This solver will provide the frequency of the
resonances as well as the fields at a particular resonance
8.6. BOUNDARIES IN HFSS
Within the context of HFSS, boundaries exist for two main purposes:
a. To either create an open or a closed electromagnetic model or,
b. To simplify the electromagnetic or geometric complexity of the
electromagnetic model.
While the concept of boundaries can be confusing to an HFSS user, they
can be simply thought of serving two main purposes. The first of these is to
create either an open or a closed model.
A closed model simply represents a structure, or a solution volume,
where no energy can escape except through an applied port. For an Eigen mode
simulation, this could be a cavity resonator. For a driven modal or terminal
solution, this could be a waveguide or some other fully enclosed structure.
An open model represents an electromagnetic model that allows
electromagnetic energy to emanate or radiate away. Common examples would
be an antenna, a PCB, or any structure that is not enclosed within a closed
cavity. While most HFSS simulations deal with models that are open, by
default, HFSS initially assumes that any given model is closed. HFSS assumes
all outer surfaces of the solution space are covered, or coated, by a perfect
electric conductor boundary. In order to create an open model, a user will need
to specify a boundary on the outer surfaces that will overwrite the default
perfect electric conductor boundary.
The second reason why boundaries are used within HFSS is to decrease
the geometric/electromagnetic complexity of a given structure or model. These
boundaries should only be used internally to a model or possibly on a symmetry
plane. They should be applied to specifically created 2D sheet objects or to
specific surfaces of3D objects. While boundaries can be very useful, a user
should exercise caution when using them as they can create unintended results if
33
applied incorrectly.
Every HFSS model a user creates will use boundaries on the outer
surfaces of the solution space. This is a direct result of the fact that a user must
specify whether a given model is open or closed. As a result, any given HFSS
model will always either have Conducting, Radiation, or Perfectly Matched
Layer Boundary on all outer surfaces.
Conducting boundaries are the perfect electric conductor, finite
conductivity, or impedance boundary. Not every HFSS model, however, will
use simplifying boundaries. When using boundaries to create simpler models,
users should take care to not create a model that has unreasonable or
inappropriate boundaries applied.
There are twelve boundaries within HFSS. Boundaries are applied to
specifically create 2Dsheet objects, or surfaces of 3D objects. The twelve
boundaries are:
1. Perfect Electric Conductor (PEC): default HFSS boundary fully
encloses the solution space and creates a closed model.
2. Radiation: used to create an open model.
3. Perfectly Matched layer (PML): used to create an open model and.
preferred for antenna simulations.
4. Finite Conductivity: allows creation of single layer conductor.
5. Layered Impedance: allows creation of multilayer conductors and thin
dielectrics.
6. Impedance: allows creation of ohm per square material layers.
7. Lumped RLC: allows creation of ideal lumped components.
8. Symmetry: used to enforce a symmetry boundary.
9. Master: used in conjunction with Slave Boundary to model infinitely
large repeating array structures.
10. Slave: used in conjunction with Master Boundary to model large
infinitely repeating array structures.
11. Screening Impedance: allows creation of large screens or grids.
12. Perfect H: allows creation of a symmetry plane.
34
8.6.1. Perfect Electric Conductor
The Perfect Electric Conductor or PEC Boundary is the HFSS default
boundary that is applied to all outer faces of the solution space. It represents a
lossless perfect conductor. This default boundary creates a closed model. This
boundary can also be used to create a symmetry plane if it is placed on an outer
face of the solution space.
Figure 8.4: Cavity resonator showing the default Perfect Electric
Boundary on all outer solution space surfaces
8.6.2. Radiation Boundary
The Radiation Boundary is used to create an open model in HFSS. It
should only be appliedto outer faces of the solution space. If simulating an
antenna, the radiation boundary shouldbe placed a quarter wavelength away
from any radiating surface.
35
Figure 8.5: Radiation boundry
8.7. APPLYING BOUNDARIES
Boundaries are applied either to specifically created 2D sheet objects or
to and individual face or faces of one or more 3D objects. Boundaries are
applied in the HFSS modeling window by selecting a face of a 3Dobject or a 2D
sheet object and selecting the boundaries command. The subsequent menu will
allow a user to select which boundary to apply to the selected face(s) or
surface(s). If additional information is needed, a user will have to specify the
appropriate information in the wizard dialogs that appear.
Figure 8.6 Applying boundary
36
8.8. ASSIGNING EXCITATIONS
There are seven types of excitations in HFSS: Wave Ports, Lumped Ports,
Floquet Ports, Incident Fields, Current Sources, Voltage Sources and Magnetic
Bias Source. All excitation types provide field information, but only the Wave
port, Lumped Port, and Floquet port provide S parameters. The use of the
Magnetic Bias Source allows a user model a magnetic bias acting on a ferrite
material.
Figure 8.7: Excitation in HFSS In HFSS, it is with the various excitations that a user can specify the
sources of fields, voltages, charges or currents for a given simulation. The most
commonly used excitation types, or ports, are the wave port and the lumped
port. These ports provide field information as well as S, Y, Z parameters and, in
the case of the wave port, a port wave impedance and gamma, the propagation
constant. The wave impedance and gamma values are related to the
37
transmission line structure that is represented by the wave port.
For models where a magnetic bias is present, such as a circulator, the
magnetic bias source can be used in conjunction with wave or lumped ports to
create a model.
For simulations of large planar and periodic structures such as infinite
antenna arrays, frequency selective surfaces or photonic band gap structures, the
Floquet port can be used.
If an ideal current or voltage source is desired, the current and voltage
sources can be used. However, these sources will only provide field information
and therefore are of limited use in an RF design environment. Only the wave
port and the lumped port types will be discussed in detail in the following
sections.
Both the Wave Port and Lumped Port are available for use in both the
Driven Modal Solution type and the Driven Terminal Solution Type. There is,
however, a small difference in how the ports are set up.
8.8.1. Lumped Port
Lumped Ports are the other commonly used excitation type in HFSS. This
port type is analogous to a current sheet source and can also be used to excite
commonly used transmission lines. Lumped ports are also useful to excite
voltage gaps or other instances where wave ports are not applicable. They
should only be applied internally to the solution space. Shown below are examples of commonly used wave ports with proper size
dimensions.
Fig 8.8: Microstrip model showing a Lumped Port applied between the
signal trace and ground plane
38
Lumped ports are ports that can be used in simulations where energy
needs to be sourced internally to a model. Lumped ports are simpler to create
than wave ports but do not yield as much information as a wave port. Lumped
ports yield S,Y,Z parameters and fields, but they do not yield any gamma or
wave impedance information. The results of a lumped port cannot be de-
embedded but can be renormalized.
Unlike wave ports, lumped ports can support only a single mode. A
lumped port can be defined on any 2D object that has edges which contact two
conducting objects. The boundary that is applied to all edges that do not touch a
conductor is a perfect H, which ensures that the normal electric field is equal to
zero on those edges.
When creating a lumped port, it is necessary that a user draw an
integration line for each port. This integration line should be drawn between the
center points of the edges that contact metal objects. For an example of this, see
the graphic at the end of this section.
The complex impedance Zs, defined when the port was created, serves as
the reference impedance of the S-matrix of the lumped port. The impedance Zs,
has the characteristics of a wave impedance; it is used to determine the strength
of a source, such as the modal voltage V and modal current I, through complex
power normalization.
Figure 8.9: Microstrip lumped port showing integration line (in red). Line
is drawn between along the centre line of the port between the edges that
contact metal objects.
39
It should also be noted that when the reference impedance is a complex
value, the magnitude of the S-matrix is not always less than or equal to 1, even
for a passive device.
Table 8.1: The difference between lumped ports and wave ports
8.9. THE SOLUTION FREQUENCY SETTING
The solution frequency is used by HFSS to determine the maximum
initial tetrahedral size and is the frequency at which HFSS explicitly solves the
given model. The solution frequency is the frequency at which HFSS explicitly
solves a given simulation. It is also at this frequency that the adaptive solution
operates, and it is the fields at this frequency that are used to determine whether
a model has converged or not. The solution frequency should be set to the operating frequency of the
device being simulated. If a frequency sweep result is desired in a simulation,
the solution frequency should be set to a frequency that is 50 percent of the
maximum frequency desired. On a practical note, for most antenna simulations, the solution frequency
should be set to the operating frequency of the antenna. For simulations of
filters, the solution frequency should be set to the center of the band pass
frequency.
The solution frequency is also the frequency that should be used for any
calculations the user performs when creating a model that depend on a
40
frequency. Examples of these types of calculations are air region size for
antenna problems, skin depth calculations, PML wizard input, etc.
Figure 8.10: Solution frequency setting
8.10.THE DELTA- S SETTING The Delta-S parameter is the main convergence criterion used HFSS
when determining whether a model has converged or not.
41
Figure 8.11: Delta- S setting
As mentioned, the adaptive process is a key element to ensuring that
HFSS yields the correct answer. Because of the direct relationship between the
electric fields in a simulation and the calculated S- matrix for that simulation,
the convergence of the simulation is presented to a user via the delta-S value.
The value of delta-S is the change in the magnitude of the S-parameters
between two consecutive passes.
Or, in electric field terms, the change in the electric field distribution
between successive solutions. Once the magnitude and phases of all S-
parameters change by less than the user-specified delta-S value, the analysis
stops and is considered converged. Or conversely, again in electric field terms,
once the electric fields are no longer changing in the given model, the field
solution has converged and is correct.
If the desired delta-S parameter is never reached, HFSS will
continue until the requested number of passes is completed. The maximum delta-S is defined as
Equation 8.8 where:
• i and j cover all matrix entries.
• N represents the pass number.
42
The delta-S number should be set between 0.005 and 0.01 for the
majority of HFSS simulations.
8.11.THE MAXIMUM REFINEMENT PER PASS AND MAXIMUM NUMBER OF PASSES AND SETTINGS
The Maximum number of passes is the maximum number of adaptive
iterations HFSS performs in order to reach convergence. The Maximum
refinement per pass is the percentage of tetrahedral elements that are subdivided
with each adaptive pass.
Figure 8.12: Plot showing number of tetrahedral increase versus adaptive
pass. (Maximum refinement per pass set to 30 %.) Refinement percentage and number of adaptive passes are both used in
the adaptive solution process. The refinement percentage specifies the largest
number of tetrahedral that can be subdivided per adaptive pass. The maximum
number of adaptive passes is the maximum number of times HFSS will refine
the mesh in order to try and converge.
The adaptive solution process uses the delta-S, maximum refinement per
pass, and maximum number of passes to converge to the correct answer. The
delta-S and maximum number of passes determine when HFSS will stop the
adaptive solution process. If convergence is reached before the maximum
number of passes has been performed, the solution process will stop. HFSS will
43
stop if convergence is not reached, but the maximum number of passes has been
reached. In such cases, it is recommended to increase the number of passes so
that HFSS can reach convergence.
8.12.THE DIFFERENT FREQUENCY SWEEPS
HFSS has three distinct sweep types: the discrete sweep, the fast sweep,
and the interpolating sweep. Depending on the needs of a user, a particular
sweep type may be preferred. Generally, the solution times required for a
frequency sweep type increase in the following order: fast, interpolating, and
discrete. But, for solutions that require field information at only a few (less than
five)discrete frequency points, the discrete sweep can be faster than either of the
other two. The fast sweep is useful when many frequency points are desired
over a limited frequency range. The interpolating sweep is most useful when
solving problems from DC to a high frequency.
For both the interpolating and fast sweeps, the number of desired
frequency points is not related to the time it takes to generate the frequency
sweep results. Both of these sweeps, in essence, generate a pole-zero transfer
function, and it is the generation of this function that requires the majority of the
solution time. Once the “transfer” function has been generated, S-parameter data
is rapidly.
Figure 8.13: Applying frequency sweep
44
HFSS has three sweep types available: discrete, fast, and interpolating.
The fast sweep generates a full-field solution within the specified frequency
range. The fast sweep is best suited for simulations that have a number of sharp
resonances. A fast sweep is highly accurate in determining the behavior of a
structure near a resonance. The fast sweep works by using the center frequency
of the sweep to create an Eigen value problem that will be used in an Adaptive
Lanczos-Padé Sweep (ALPS) procedure to determine all the field solutions in
the requested frequency range.
Because the fast sweep uses the results of the adaptive process to
generate the Eigen value problem, it is efficient to set the solution frequency to
be equal to the center sweep frequency when using the fast sweep. A key
benefit of the fast sweep is that it allows a user to post-process and display
fields at any frequency and at any location within the frequency sweep. The
interpolating sweep estimates a solution for the S-matrix over an entire
frequency range. HFSS does this by choosing appropriate frequency points at
which to solve for the field solution. HFSS continues to choose frequency
points until the full sweep solution lies within a given error tolerance. The
interpolating sweep is best suited for very broadband frequency sweeps. The
interpolating sweep uses less RAM than a fast sweep. A key benefit of the
interpolating sweep is that it can easily determine the frequency sweep response
from DC to any desired high frequency.
The interpolating sweep, however, only has the solution frequency field
data available for post-processing. Field data for other frequencies within the
interpolating sweep range are therefore not available. The discrete sweep
generates explicit field solutions at specific frequency points in the desired
frequency sweep. The discrete sweep solution time is directly dependent on the
number of frequency points desired. The more frequency steps a user requests,
the longer HFSS will need to complete the frequency sweep. The explicit field
solution is obtained by substituting the desired frequencies into the matrix
45
equation that was created during the adaptive solution process. Each frequency
solution is therefore explicitly based on the adaptive solution, and not
interpolated via a numerical method like the fast and interpolating sweeps.
Arguably, therefore, the discrete sweep is the most accurate sweep
available. It, however, is also the sweep that requires the most time to generate
frequency sweep results when many frequency steps are desired.
8.13.PLOTTING ANTENNA RESULTS
Far field antenna patterns are easily generated by HFSS by again using
the Reports Editor. The procedure is similar to plotting the standard circuit
parameters. But the model should have included either Radiation or PML
boundaries, and a Far Field Setup must be defined before Far Field quantities
can be plotted.
Figure 8.14: Insertion of Far Field Setup
46
Figure 8.15: Plotting antenna results While the plotting of far fields is straight forward, there are some key items a user
should know regarding how HFSS generates far field data. When HFSS generates far field
data, the field values on the radiation surface(s)are used to compute the fields in the space
surrounding
The modeled structure, outside of the solution volume. This space is broken down
into the near field and far field regions, where the near field is the region close to the solution
volume. In general, the electric field in this external region can be written as Equation 8.9 Where S represents the radiation boundary surfaces. J is the imaginary unit. ω is the angular frequency, 2πf. μ0 is the relative permeability of free space.
47
Htan is the component of the magnetic field that is tangential to surface.
Enormal is the component of the electric field that is normal to the surface.
Etanis the component of the electric field that is tangential to the surface. G is the free space Green’s function, given by
Equation 8.10
where k0 is the free space wave number, r, r’ represent the field and source points, respectively, ε0 is the permittivity of free space,
μr and εr are the relative permeability and permittivity of a dielectric, respectively. The r dependence seen above is a key far fields characteristic of a spherical wave.
The far field is a spherical TEM wave, which can be described by the following
equation:
Equation8.11 where η is the intrinsic impedance of free space. When calculating the far fields, the previously discussed far-field approximations
are used, and the result is valid only for field points in the far-field region.
48
CHAPTER 9
ANTENNA DESIGN
The top view of the proposed antenna structure has been shown in Fig.9.1. A simple
rectangular microstrip patch antenna has been taken. Size of the antenna is calculated from
the basic patch antenna equations (C. A. Balanis, 2007) and appropriate changes have been
done to make an E shape patch antenna. With a distance of /2 between the patch 1*2 array
antenna is designed to improve the gain. Microstrip feeding is chosen for the excitation of the
proposed antenna. Power is divided equally using the lossless T-junction power divider with
three transmission lines connected at a single junction. Each transmission line is at a distance
of /4 from the patch.
Figure 9.1:Top view of the proposed antenna
In the first step, a ground of (58.222*25.47)mm is constructed. FR4 substrate is
created above the ground with a thickness of 1.6mm.E-shaped patch is created above the
substrate with the specifications given in the table 1. Another patch is created with a distance
of /2 from the previously created patch to form a 1*2 array. Microstrip feeding is chosen for
the excitation of the proposed antenna. Power is divided equally using the lossless T-junction
power divider with three transmission lines connected at a single junction. Each transmission
line is at a distance of /4 from the patch.
49
Figure 9.2:Structure of single E-patch antenna
9.1: PARAMETERS OF E-SHAPED PATCH ANTENNA
PARAMETER DIMENSION(mm)
L 11.5
W 15.5
L1 2.2
W1 1.94
W2 2.5
W3 6.62
GROUND 58.822*25.47
HEIGHT OF SUBSTRATE 1.6
Table 9.1: Parameters of E-shaped patch antenna
50
9.2.DESIGN EQUATIONS
PATCH WIDTH:
𝑊=(co / 2𝑓r )√(2 /𝜖r + 1)
𝑐o𝑖𝑠 𝑠𝑝𝑒𝑒𝑑 𝑜𝑓 𝑙𝑖𝑔ℎt.
PARAMETERS:
𝜖𝑟𝑒𝑓𝑓 = (𝜖𝑟 + 1)/ 2 + ((𝜖𝑟 − 1)/ 2) (1 + 12 (ℎ/ W ))−1 /2 , 𝑊/ ℎ> 1
∆𝐿 /ℎ = (0.412(𝜖𝑟𝑒𝑓𝑓 + 0.3)( 𝑊/ ℎ + 0.264))/ ((𝜖𝑟𝑒𝑓𝑓− 0.258 )(𝑊 /ℎ + 0.8))
PATCH LENGTH:
𝐿=(𝑐𝑜/ 2𝑓𝑟 √𝜖𝑟𝑒𝑓𝑓 )− 2∆𝐿
DISTANCE BETWEEN PATCH & SUBSTRATE IS
3*substrate thickness
51
SIMULATED ANTENNAS IMAGES IN HFSS
Figure 9.3:Base antenna
Figure 9.4: Proposed antenna array
52
CHAPTER 10
RESULTS
The return loss, gain and VSWR of the single and proposed antenna array are plotted
using HFSS. It is observed that the reflection coefficient (S11) is -20.22dB for the desired
frequency band(5.7 to 5.835GHz) with center frequency of 5.8GHz. For the single antenna
the bandwidth obtained is 237.8MHz(-10 dB Bandwidth).The bandwidth is increased to
310.7MHz for the two element array. The obtained return loss, gain and VSWR graph are
shown in figure10.2,figure10.4,figure10.6 respectively. Gain is increased after implementing
array. For the single antenna, gain of 5dB is obtained whereas for the antenna array the gain
is increased to 6.2 dB. The return loss is -16.36dB for single antenna and -20.22dB for array
antenna. The VSWR is obtained as 1.3 for single antenna and 1.13 for array antenna at the
operating frequency 5.8 GHz. Bandwidth and gain are increased by implementing array.
53
SIMULATED RESULTS
Figure 10.1:Return loss of single antenna
Figure 10.2:Return loss of proposed antenna array
54
Figure 10.3: Gain plot of single antenna
Figure 10.4: Gain plot of proposed antenna array
55
3.00 3.50 4.00 4.50 5.00 5.50 6.00 6.50 7.00Freq [GHz]
0.00
5.00
10.00
15.00
20.00
25.00
VS
WR
(1)
HFSSDesign1XY Plot 3 ANSOFT
m1
Curve Info
VSWR(1)Setup1 : Sw eep
Name X Y
m1 5.8000 1.3120
Figure 10.5: VSWR plot of single antenna
Figure 10.6:VSWR plot of proposed antenna array
56
COMPARISON OF BASE ANTENNA AND PROPOSED ANTENNA ARRAY
Table 10.1: comparison of base antenna and proposed antenna array
57
CHAPTER 11
FABRICATION AND TESTING
Our proposed antenna is fabricated and tested at KARUNYA UNIVERSITY,
COIMBATORE.The front view and back view of the fabricated antenna is shown in figure
11.1 and figure 11.2 respectively. The antenna is tested and return loss is measured. The
testing equipment used are shown in figure 11.3 and figure 11.4.
58
Figure11.1:Front view
Figure11.2:Back view
59
Figure11.3:Testing setup
Figure 11.4:MIC holder with antenna
60
RESULT COMPARISION
PARAMETER SIMULATED VALUE MEASURED VALUE
S11 plot -20.2dB -22dB
Table 11.1:Result comparision
61
Testing certificate
62
CHAPTER 12
CONCLUSION
The proposed antenna in this paper is a good solution for wireless application
specially for Wireless Local Area Network (WLAN)&Worldwide Interoperability for
Microwave Access(WiMax) with a special property of smaller in size. This antenna is simple
and compact and having Microstrip feed. This is printed antenna geometry so it is very easy
to integrate with the radio frequency circuit. The proposed antenna has bandwidth of
approximately 302.7MHz and resonance frequency at 5.8GHz. Thus we can conclude that
the proposed antenna suitable for wireless applications in WLAN & Wimax bands being
smaller in size.
63
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