ANTENNA and WAVE PROPAGATION Lecture Notes B.TECH (III YEAR – II SEM) (2019-20)

Total Page:16

File Type:pdf, Size:1020Kb

ANTENNA and WAVE PROPAGATION Lecture Notes B.TECH (III YEAR – II SEM) (2019-20) ANTENNA AND WAVE PROPAGATION Lecture Notes B.TECH (III YEAR – II SEM) (2019-20) Prepared by: Mr. M. SREEDHAR REDDY, Associate Professor Mrs.RENJU PANICKER, Assistant Professor Department of Electronics and Communication Engineering MALLA REDDY COLLEGE OF ENGINEERING & TECHNOLOGY (Autonomous Institution – UGC, Govt. of India) Recognized under 2(f) and 12 (B) of UGC ACT 1956 (Affiliated to JNTUH, Hyderabad, Approved by AICTE - Accredited by NBA & NAAC – ‘A’ Grade - ISO 9001:2015 Certified) Maisammaguda, Dhulapally (Post Via. Kompally), Secunderabad – 500100, Telangana State, India MALLA REDDY COLLEGE OF ENGINEERING AND TECHNOLOGY III Year B.Tech. ECE-II Sem L T/P/D C 4 1/ - /- 3 (R17A0416) ANTENNAS AND WAVE PROPAGATION OBJECTIVES Understand basic terminology and concepts of Antennas. To attain knowledge on the basic parameters those are considered in the antenna design process and the analysis while designing that. Analyze the electric and magnetic field emission from various basic antennas and mathematical Formulation of the analysis. To have knowledge on antenna operation and types as well as their usage in real time filed. Aware of the wave spectrum and respective band based antenna usage and also to know the propagation of the waves at different frequencies through different layers in the existing layered free space environment structure. UNIT -I: Antenna Basics: Introduction, Basic Antenna Parameters – Patterns, Beam Area, Radiation Intensity, Beam Efficiency, Directivity-Gain-Resolution, Antenna Apertures, Illustrative Problems. Fields from Oscillating Dipole, Field Zones, Front - to-back Ratio, Antenna Theorems, Radiation, Retarded Potentials – Helmholtz Theorem. Thin Linear Wire Antennas – Radiation from Small Electric Dipole, Quarter Wave Monopole and Half Wave Dipole – Current Distributions, Field Components, Radiated Power, Radiation Resistance, Beam Width, Directivity, Effective Area, Effective Height, Natural Current Distributions, Far Fields and Patterns of Thin Linear Centre-fed Antennas of Different Lengths, Illustrative Problems. UNIT –II: VHF, UHF and Microwave Antennas - I : Arrays with Parasitic Elements, Yagi-Uda Array, Folded Dipoles and their Characteristics, Helical Antennas – Helical Geometry, Helix Modes, Practical Design Considerations for Monofilar Helical Antenna in Axial and Normal Modes, Horn Antennas – Types, Optimum Horns, Design Considerations of Pyramidal Horns, Illustrative Problems. VHF, UHF and Microwave Antennas - II: Microstrip Antennas – Introduction, Features, Advantages and Limitations, Rectangular Patch Antennas – Geometry and Parameters, Characteristics of Microstrip Antennas. Impact of Different Parameters on Characteristics, Reflector Antennas – Introduction, Flar Sheet and Corner Reflectors, Paraboloidal Reflectors – Geometry, Pattern Characteristics, Feed Methods, Reflector Types – Related Features, Illustrative Problems. Lens Antennas – Introduction, Geometry of Non-metallic Dielectric Lenses, Zoning, Applications. UNIT -III: Antenna Arrays: Point Sources – Definition, Patterns, arrays of 2 Isotropic Sources - Different Cases, Principle of Pattern Multiplication, Uniform Linear Arrays – Broadside Arrays, Endfire Arrays, EFA with Increased Directivity, Derivation of their Characteristics and Comparison, BSAs with Non-uniform Amplitude Distributions – General Considerations and Binomial Arrays, Illustrative Problems. Antenna Measurements: Introduction, Concepts - Reciprocity, Near and Far Fields, Coordinate System Patterns to be Measured, Pattern Measurement Arrangement, Directivity Measurement, Gain Measurements (by Comparison, Absolute and 3- Antenna Methods) UNIT -IV: Wave Propagation – I: Introduction, Definitions, Categorizations and General Classifications, Different Modes of Wave Propagation, Ray/Mode Concepts, Ground Wave Propagation (Qualitative Treatment) – Introduction, Plane Earth Reflections, Space and Surface Waves, Wave Tilt, Curved Earth Reflections. Space Wave Propagation – Introduction, Field Strength Variation with Distance and Height, Effect of Earth‘s Curvature, Absorption, Super Refraction, M-Curves and Duct Propagation, Scattering Phenomena, Tropospheric Propagation. UNIT -V: Wave Propagation – II: Sky Wave Propagation – Introduction, Structure of Ionosphere, Refraction and Reflection of Sky Waves by Ionosphere, Ray Path, Critical Frequency, MUF, LUF, OF, Virtual Height and Skip Distance, Relation between MUF and Skip Distance, Multihop Propagation. TEXT BOOKS: 1. Antennas and Wave Propagation – J.D. Kraus, R.J. Marhefka and Ahmad S. Khan, TMH, New Delhi, 4th ed., (Special Indian Edition), 2010. 2. Electromagnetic Waves and Radiating Systems – E.C. Jordan and K.G. Balmain, PHI, 2nd ed., 2000. REFERENCE BOOKS: 1. Antenna Theory - C.A. Balanis, John Wiley & Sons, 3rd Ed., 2005. 2. Antennas and Wave Propagation – K.D. Prasad, Satya Prakashan, Tech India Publications, New Delhi, 2001. 3. Transmission and Propagation – E.V.D. Glazier and H.R.L. Lamont, The Services Text Book of Radio, vol. 5, Standard Publishers Distributors, Delhi. 4. Antennas – John D. Kraus, McGraw-Hill (International Edition), 2nd Ed. 1988. 5. Electronic and Radio Engineering – F.E. Terman, McGraw-Hill, 4th edition, 1955 . OUTCOMES Student will be able to Aware of antenna parameter considerations Capable to analyze the designed antenna and field evaluation under various conditions and formulate the electric as well as magnetic fields equation set for far field and near field conditions Understand the array system of different antennas and field analysis under application of different currents to the individual antenna elements Understand the design issues, operation of fundamental antennas and their operation methodology in practice. Design a lens structure and also the bench set up for antenna parameter measurement of testing for their effectiveness Knowledge about the means of propagation of electromagnetic waves ANTENNA AND WAVE PROPAGATIONS LECTURE NOTES UNIT – I: ANTENNA BASICS HISTORY OF AN ANTENNAS: The first radio antennas were built by Heinrich Hertz, a professor at the Technical Institute in Karlsruhe , Germany. Heinrich Hertz‘s end-loaded half-wave dipole transmitting antenna and resonant half-wave receiving loop operating at λ = 8 m in 1886. Hertz was the pioneer and father of radio, his invention remained a laboratory uriosity until 20-year-old Guglielmo Marconi of Bologna, Italy, went on to add tuning circuits, big antenna and ground systems for longer wavelengths, and was able to signal over large distances. In mid-December 1901 he startled the world by receiving signals at St. Johns, Newfoundland, from a transmitting station he had constructed at Poldhu in Cornwall, England. Guglielmo Marconi‘s square conical antenna at Poldhu, England, in 1905 for sending transatlantic signals at wavelengths of 1000s of meters. Shown in fig. below. Rarely has an invention captured the public imagination as Marconi‘s wireless did at the beginning of the 20th century. With the advent of radar during World War II, centimeter wavelengths became popular and the entire radio spectrum opened up to wide usage. Thousands of communication satellites bristling with antennas now circle the earth in low, medium, and geostationary orbits. The geostationary satellites form a ring around the earth similar to the rings around Saturn. Your hand-held Global Position Satellite (GPS) receiver gives your latitude, longitude and elevation to centimeter accuracy anywhere on or above the earth day or night, cloudy or clear. Very Large Array (VLA) of 27 steerable parabolic dish antennas each 25 m in diameter operating at centimeter wavelengths for observing radio sources at distances of billions of light-years. The array is located at the National Radio Astronomy Observatory near Socorro, New Mexico in 1980 . Shown in fig. below. Our probes with their arrays of antennas have visited the planets of the solar system and beyond, responding to our commands and sending back photographs and data at centimeter wavelengths even though it may take over 5 hours for the signals to travel one way. And our radio telescope antennas operating at millimeter to kilometer wavelengths receive signals from objects so distant that it has taken more than 10 billion years for the signals to arrive. Helix antenna array on one of 24 Global Position Satellites (GPS) in Medium Earth Orbit (MEO) at 20,000km. Operating at λ = 20 cm, these satellites provide you on or above the earth with your position (latitude, longitude and elevation) to an accuracy of better than 1 meter in 1985 . Shown in fig. below. In the above image, the antennas help the communication to be established in the whole area, including the valleys and mountains. This process would obviously be easier than laying a wiring system throughout the area. The ubiquitous, hand-held cellphone with half-wave antenna operating at λ = 30 cm, which connects you to everybody. Antennas are the essential communication link for aircraft and ships. Antennas for cellular phones and all types of wireless devices link us to everyone and every thing. With mankind‘s activities expanding into space, the need for antennas will grow to an unprecedented degree. Antennas will provide the vital links to and from everything out there. The future of antennas reaches to the stars. INTRODUCTION: Antennas are our electronic eyes and ears on the world. They are our links with space. They are an essential, integral part of our civilization. An antenna (or aerial) is an electrical device which converts electric
Recommended publications
  • A Technical Assessment of Aperture-Coupled Antenna Technology
    Running head: APERTURE-COUPLED ANTENNA TECHNOLOGY 1 A Technical Assessment of Aperture-coupled Antenna Technology Justin Obenchain A Senior Thesis submitted in partial fulfillment of the requirements for graduation in the Honors Program Liberty University Spring 2014 APERTURE-COUPLED ANTENNA TECHNOLOGY 2 Acceptance of Senior Honors Thesis This Senior Honors Thesis is accepted in partial fulfillment of the requirements for graduation from the Honors Program of Liberty University. ______________________________ Carl Pettiford, Ph.D. Thesis Chair ______________________________ Kyung K. Bae, Ph.D. Committee Member ______________________________ James Cook, Ph.D. Committee Member ______________________________ Brenda Ayres, Ph.D. Honors Director ______________________________ Date APERTURE-COUPLED ANTENNA TECHNOLOGY 3 Abstract Aperture coupling refers to a method of construction for patch antennas, which are specific types of microstrip antennas. These antennas are used in a variety of applications including cellular telephones, military radios, and other communications devices. The purpose of this thesis is to assess the benefits and drawbacks of aperture- coupled antenna technology. To develop a successful analysis of the patch antenna construction technique known as aperture coupling, this assessment begins by examining basic antenna theory and patch antenna design. After uncovering some of the fundamental principles that govern aperture-coupled antenna technology, a hypothesis is created and assessed based on the positive and negative aspects
    [Show full text]
  • Radiometry and the Friis Transmission Equation Joseph A
    Radiometry and the Friis transmission equation Joseph A. Shaw Citation: Am. J. Phys. 81, 33 (2013); doi: 10.1119/1.4755780 View online: http://dx.doi.org/10.1119/1.4755780 View Table of Contents: http://ajp.aapt.org/resource/1/AJPIAS/v81/i1 Published by the American Association of Physics Teachers Related Articles The reciprocal relation of mutual inductance in a coupled circuit system Am. J. Phys. 80, 840 (2012) Teaching solar cell I-V characteristics using SPICE Am. J. Phys. 79, 1232 (2011) A digital oscilloscope setup for the measurement of a transistor’s characteristic curves Am. J. Phys. 78, 1425 (2010) A low cost, modular, and physiologically inspired electronic neuron Am. J. Phys. 78, 1297 (2010) Spreadsheet lock-in amplifier Am. J. Phys. 78, 1227 (2010) Additional information on Am. J. Phys. Journal Homepage: http://ajp.aapt.org/ Journal Information: http://ajp.aapt.org/about/about_the_journal Top downloads: http://ajp.aapt.org/most_downloaded Information for Authors: http://ajp.dickinson.edu/Contributors/contGenInfo.html Downloaded 07 Jan 2013 to 153.90.120.11. Redistribution subject to AAPT license or copyright; see http://ajp.aapt.org/authors/copyright_permission Radiometry and the Friis transmission equation Joseph A. Shaw Department of Electrical & Computer Engineering, Montana State University, Bozeman, Montana 59717 (Received 1 July 2011; accepted 13 September 2012) To more effectively tailor courses involving antennas, wireless communications, optics, and applied electromagnetics to a mixed audience of engineering and physics students, the Friis transmission equation—which quantifies the power received in a free-space communication link—is developed from principles of optical radiometry and scalar diffraction.
    [Show full text]
  • 25. Antennas II
    25. Antennas II Radiation patterns Beyond the Hertzian dipole - superposition Directivity and antenna gain More complicated antennas Impedance matching Reminder: Hertzian dipole The Hertzian dipole is a linear d << antenna which is much shorter than the free-space wavelength: V(t) Far field: jk0 r j t 00Id e ˆ Er,, t j sin 4 r Radiation resistance: 2 d 2 RZ rad 3 0 2 where Z 000 377 is the impedance of free space. R Radiation efficiency: rad (typically is small because d << ) RRrad Ohmic Radiation patterns Antennas do not radiate power equally in all directions. For a linear dipole, no power is radiated along the antenna’s axis ( = 0). 222 2 I 00Idsin 0 ˆ 330 30 Sr, 22 32 cr 0 300 60 We’ve seen this picture before… 270 90 Such polar plots of far-field power vs. angle 240 120 210 150 are known as ‘radiation patterns’. 180 Note that this picture is only a 2D slice of a 3D pattern. E-plane pattern: the 2D slice displaying the plane which contains the electric field vectors. H-plane pattern: the 2D slice displaying the plane which contains the magnetic field vectors. Radiation patterns – Hertzian dipole z y E-plane radiation pattern y x 3D cutaway view H-plane radiation pattern Beyond the Hertzian dipole: longer antennas All of the results we’ve derived so far apply only in the situation where the antenna is short, i.e., d << . That assumption allowed us to say that the current in the antenna was independent of position along the antenna, depending only on time: I(t) = I0 cos(t) no z dependence! For longer antennas, this is no longer true.
    [Show full text]
  • Path Loss and Shadowing 2017
    Path-loss and Shadowing (Large-scale Fading) PROF. MICHAEL TSAI 2017/10/23 Friis Formula TX Antenna RX Antenna �"�"�- × � ⇒ � = � - 0 4��+ EIRP=�"�" % Power spatial density &' 1 × 4��+ 2 � � � � = � � - Antenna Aperture � 4��+ • Antenna Aperture=Effective Area �� • Isotropic Antenna’s effective area � ≐ �,��� �� • Isotropic Antenna’s Gain=1 �� • � = � �� � � � � �� � � � • Friis Formula becomes: � = � � � = � � � � ��� � ���� 3 � � � �� Friis Formula � = � � � � ��� � �� • is often referred as “Free-Space Path Loss” (FSPL) ��� � • Only valid when d is in the “far-field” of the transmitting antenna • Far-field: when � > ��, Fraunhofer distance ��� • � = , and it must satisfies � ≫ � and � ≫ � � � � � • D: Largest physical linear dimension of the antenna • �: Wavelength • We often choose a �� in the far-field region, and smaller than any practical distance used in the system � � • Then we have � � = � � � � � � � 4 Received Signal after Free-Space Path Loss phase difference due to propagation distance ���� � ������� − � � � = �� �N � ��� ���� � ��� � Free-Space Path Loss Carrier (sinusoid) Complex envelope 5 Example: Far-field Distance • Find the far-field distance of an antenna with maximum dimension of 1m and operating freQuency of 900 MHz (GSM 900) • Ans: • Largest dimension of antenna: D=1m • Operating FreQuency: f=900 MHz � �×��� • Wavelength: � = = = �. �� � ���×��� ��� � • � = = = �. �� (m) � � �.�� 6 Example: FSPL • If a transmitter produces 50 watts of power, express the transmit power in units of (a) dBm and (b) dBW. • If 50 watts
    [Show full text]
  • Antenna Theory and Matching
    Antenna Theory and Matching Farrukh Inam Applications Engineer LPRF TI 1 Agenda • Antenna Basics • Antenna Parameters • Radio Range and Communication Link • Antenna Matching Example 2 What is an Antenna • Converts guided EM waves from a transmission line to spherical wave in free space or vice versa. • Matches the transmission line impedance to that of free space for maximum radiated power. • An important design consideration is matching the antenna to the transmission line (TL) and the RF source. The quality of match is specified in terms of VSWR or S11. • Standing waves are produced when RF power is not completely delivered to the antenna. In high power RF systems this might even cause arching or discharge in the transmission lines. • Resistive/dielectric losses are also undesirable as they decrease the efficiency of the antenna. 3 When does radiation occur • EM radiation occurs when charge is accelerated or decelerated (time-varying current element). • Stationary charge means zero current ⇒ no radiation. • If charge is moving with a uniform velocity ⇒ no radiation. • If charge is accelerated due to EMF or due to discontinuities, such as termination, bend, curvature ⇒ radiation occurs. 4 Commonly Used Antennas • PCB antennas – No extra cost – Size can be demanding at sub 433 MHz (but we have a good solution!) – Good performance at > 868 MHz • Whip antennas – Expensive solutions for high volume – Good performance – Hard to fit in many applications • Chip antennas – Medium cost – Good performance at 2.4 GHz – OK performance at 868-955
    [Show full text]
  • Exp-1: Understand the Pathloss Prediction Formula
    Exp-1: Understand the pathloss prediction formula. Aim To understand the pathloss prediction formula Objectives 1. Calculation of received signal strength as a function of distance of separation between transmitter and receiver. 2. To understand the impact of the following parameters on received signal strength. (a) Transmitter Power (b) Path loss exponent, (c) Carrier frequency, (d) Receiver antenna height, (e) Transmitter antenna height. 1 Theory for Experiment 1:-Understand the pathloss prediction formula. The design of a communication system involves selection of values for several parameters. One of the important parameter is the transmit power. Higher transmit power ensures large allowable separation distance between the transmitter (Tx) and receiver(Rx). Of course the loss in signal power per unit distance depends on the properties of the medium. In case of wireless communication on one hand it is desired to have a very large coverage (large allowable separation between Txand Rx) on the other hand it is also desired that co-channel interference be as low as possible.An understanding of the large scale propagation effects is very important for design of suitable communication system. In terrestrial mobile communication system, electro-magnetic wave propagation is affected by reflection, diffraction and scattering. These lead to dynamic variation of signal strength as a function of time, frequency, distance of separation, antenna height, antenna configuration, local scattering environment etc. Propagation models are necessary in order to predict the received signal strength for a given set of parameters as mentioned above. These models can be broadly considered under:- • Large scale Fading Model. • Small Scale Fading Model.
    [Show full text]
  • Low-Profile Wideband Antennas Based on Tightly Coupled Dipole
    Low-Profile Wideband Antennas Based on Tightly Coupled Dipole and Patch Elements Dissertation Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Erdinc Irci, B.S., M.S. Graduate Program in Electrical and Computer Engineering The Ohio State University 2011 Dissertation Committee: John L. Volakis, Advisor Kubilay Sertel, Co-advisor Robert J. Burkholder Fernando L. Teixeira c Copyright by Erdinc Irci 2011 Abstract There is strong interest to combine many antenna functionalities within a single, wideband aperture. However, size restrictions and conformal installation requirements are major obstacles to this goal (in terms of gain and bandwidth). Of particular importance is bandwidth; which, as is well known, decreases when the antenna is placed closer to the ground plane. Hence, recent efforts on EBG and AMC ground planes were aimed at mitigating this deterioration for low-profile antennas. In this dissertation, we propose a new class of tightly coupled arrays (TCAs) which exhibit substantially broader bandwidth than a single patch antenna of the same size. The enhancement is due to the cancellation of the ground plane inductance by the capacitance of the TCA aperture. This concept of reactive impedance cancellation was motivated by the ultrawideband (UWB) current sheet array (CSA) introduced by Munk in 2003. We demonstrate that as broad as 7:1 UWB operation can be achieved for an aperture as thin as λ/17 at the lowest frequency. This is a 40% larger wideband performance and 35% thinner profile as compared to the CSA. Much of the dissertation’s focus is on adapting the conformal TCA concept to small and very low-profile finite arrays.
    [Show full text]
  • Radiation Hazard Analysis KVH Industries Carlsbad, CA
    Radiation Hazard Analysis KVH Industries Carlsbad, CA This analysis predicts the radiation levels around a proposed earth station complex, comprised of one (reflector) type antennas. This report is developed in accordance with the prediction methods contained in OET Bulletin No. 65, Evaluating Compliance with FCC Guidelines for Human Exposure to Radio Frequency Electromagnetic Fields, Edition 97-01, pp 26-30. The maximum level of non-ionizing radiation to which employees may be exposed is limited to a power density level of 5 milliwatts per square centimeter (5 mW/cm2) averaged over any 6 minute period in a controlled environment and the maximum level of non-ionizing radiation to which the general public is exposed is limited to a power density level of 1 milliwatt per square centimeter (1 mW/cm2) averaged over any 30 minute period in a uncontrolled environment. Note that the worse-case radiation hazards exist along the beam axis. Under normal circumstances, it is highly unlikely that the antenna axis will be aligned with any occupied area since that would represent a blockage to the desired signals, thus rendering the link unusable. Earth Station Technical Parameter Table Antenna Actual Diameter 1 meters Antenna Surface Area 0.8 sq. meters Antenna Isotropic Gain 34.5 dBi Number of Identical Adjacent Antennas 1 Nominal Antenna Efficiency (ε) 67.50% Nominal Frequency 6.138 GHz Nominal Wavelength (λ) 0.0489 meters Maximum Transmit Power / Carrier 22.0 Watts Number of Carriers 1 Total Transmit Power 22.0 Watts W/G Loss from Transmitter to Feed 1.0 dB Total Feed Input Power 17.48 Watts Near Field Limit Rnf = D²/4λ =5.12 meters Far Field Limit Rff = 0.6 D²/λ = 12.28 meters Transition Region Rnf to Rff In the following sections, the power density in the above regions, as well as other critically important areas will be calculated and evaluated.
    [Show full text]
  • Optical Antennas for Harvesting Solar Radiation Energy Waleed Tariq Sethi
    Optical antennas for harvesting solar radiation energy Waleed Tariq Sethi To cite this version: Waleed Tariq Sethi. Optical antennas for harvesting solar radiation energy. Electronics. Université Rennes 1, 2018. English. NNT : 2018REN1S129. tel-02295386 HAL Id: tel-02295386 https://tel.archives-ouvertes.fr/tel-02295386 Submitted on 24 Sep 2019 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. THÈSE / UNIVERSITÉ DE RENNES 1 sous le sceau de l’Université Bretagne Loire pour le grade de DOCTEUR DE L’UNIVERSITÉ DE RENNES 1 Mention : Traitement de Signal et Télécommunications Ecole doctorale MathSTIC présentée par Waleed Tariq Sethi préparée à l’unité de recherche IETR (UMR 6164) (Institut d’Electronique et de Télécommunications de Rennes UFR Informatique et Electronique Thèse soutenue à Rennes le 16 Février 2018 Optical antennas devant le jury composé de : for harvesting solar Guillaume Ducournau IEMN Université Lille 1 / Polytech'Lille, France / radiation energy rapporteur Paola Russo Università Politecnica delle Marche Ancona, Italy / rapporteur Olivier
    [Show full text]
  • 1.Effective Aperture of Antenna Directivity Bounding and Its
    International Journal of Advanced Trends in Engineering, Science and Technology (IJATEST:2456-1126) Vol.3.Issue.5,September.2018 Effective Aperture of Antenna Directivity Bounding and Its Radiation Aperture MD. Javeed Ahammed 1, Dr. R.P. Singh2, Dr. M. Satya Sai Ram3 1.Research Scholar, ECE Department, Sri Satya Sai University of Technology and Medical Science, Sehore, Bhopal, Madhya Pradesh, India. E-mail: [email protected] 2. Vice- Chancellor, Sri Satya Sai University of Technology and Medical Science, Sehore, Bhopal, Madhya Pradesh, India. 3. HOD, ECE, Chalapathi Institute of Engineering and Technology, Chalapathi Nagar, Guntur, Andhra Pradesh, India. Abstract: In this paper, among the earliest type of antennas in production was aperture type. These antennas were rigid and consisted of a parabolic, paraboloidal, cylindrical, or spherical shape. A major limitation of this type of antenna stems from the fact they could only give one particular radiation pattern, and if one wanted to scan the signal from one point to another, then the whole structure had to be moved which meant the satellite had to be realigned. This major shortcoming led to the development of the more costly phased array technology and other technologies where beam scanning was exploited. The aperture is defined as the area, oriented perpendicular to the direction of an incoming radio wave, which would intercept the same amount of power from that wave as is produced by the antenna receiving it. At any point, a beam of radio waves has an irradiance or power flux density which is the amount of radio power passing through a unit area of one square meter.
    [Show full text]
  • Of the Radiation Properties of the Antenna As a Function of Space Coordinates
    LECTURE 4: Fundamental Antenna Parameters (Radiation pattern. Pattern beamwidths. Radiation intensity. Directivity. Gain. Antenna efficiency and radiation efficiency. Frequency bandwidth. Input impedance and radiation resistance. Antenna equivalent area. Relationship between directivity and area.) The antenna parameters describe the antenna performance with respect to space distribution of the radiated energy, power efficiency, matching to the feed circuitry, etc. Many of these parameters are interrelated. There are several parameters not described here, such as antenna temperature and noise characteristics. They will be discussed later in conjunction with radiowave propagation and system performance. 1. Radiation pattern The radiation pattern (RP) (or antenna pattern) is the representation of the radiation properties of the antenna as a function of space coordinates. The RP is measured in the far-field region, where the spatial (angular) distribution of the radiated power does not depend on the distance. One can measure and plot the field intensity, e.g. ∼ E ()θ ,ϕ , or the received power 2 E ()θϕ, 2 ∼ =η H ()θ ,ϕ η The trace of the spatial variation of the received/radiated power at a constant radius from the antenna is called the power pattern. The trace of the spatial variation of the electric (magnetic) field at a constant radius from the antenna is called the amplitude field pattern. Usually, the pattern describes the normalized field (power) values with respect to the maximum value. Note: The power pattern and the amplitude field pattern are the same when computed and plotted in dB. 1 The pattern can be a 3-D plot (both θ and ϕ vary), or a 2-D plot.
    [Show full text]
  • ISOTROPIC RADIATOR in General, Isotropic Radiator Is a Hypothetical
    Lecture 8 Antenna And Wave Propagation Isotropic Antenna ISOTROPIC RADIATOR In general, isotropic radiator is a hypothetical or fictitious radiator. The isotropic radiator is defined as a radiator which radiates energy in all directions uniformly. It is also called isotropic source. As it radiates uniformly in all directions. Basically isotropic radiator is a lossless ideal radiator or antenna. Generally all the practical antennas are compared with the characteristics of the isotropic radiator. The isotropic antenna or radiator is used as reference antenna. Practically all antennas show directional properties i.e. directivity property. That means none of the antennas radiate energy in all directions uniformly. Hence practically isotropic radiator cannot exist. Figure 1: Isotropic radiator Consider that an isotropic radiator is placed at the center of sphere of radius (r). Then all the power radiated by the isotropic radiator passes over the surface area of the sphere given by (4πr) assuming zero absorption of the power. Then at any point on the surface, the Poynting vector W gives the power radiated per unit area in any direction. But radiated power travels in the radial direction. Thus the magnitude of the Poynting vector W will be equal to radial component as the components in θ and ∅ directions are zero i.e. 푊휃=푊∅=0. Type equation here.Hence we can write, Technical College / communication Dept. 1 By: Ghufran M. Hatem Lecture 8 Antenna And Wave Propagation Isotropic Antenna |푊| = 푊푟 The total power radiated is given by, 2 푃푟푎푑 = ∮ 푊 푑푠 = ∮ 푊푟 푑푠 = 푊° ∮ 푑푠 = 4휋푟 푊° Where 푊° = 푃푎푣푔 = Average power density component ∮ 푑푠 = 4휋푟2=surface of sphere 푃 푃 = 푟푎푑 푎푣푔 4휋푟2 Where, P푟푎푑 = Total power radiated in watts r = Radius of sphere in meters 2 푃푎푣푔 =Radial component of average power density in W/m Electric Field of Isotropic Antenna The Point source is located at the origin point O, then the power density at the point Q is given as 푃푟푎푑 2 W 푃 = 4휋푟 … … … … … (1) 푎푣푔 m2 The power density is related to the electric and magnetic field 2 1 ∗ 퐸 1 2 푊 = 푅푒|퐸.
    [Show full text]