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Array Designs for Long-Distance Wireless Power Transmission: State
INVITED PAPER Array Designs for Long-Distance Wireless Power Transmission: State-of-the-Art and Innovative Solutions A review of long-range WPT array techniques is provided with recent advances and future trends. Design techniques for transmitting antennas are developed for optimized array architectures, and synthesis issues of rectenna arrays are detailed with examples and discussions. By Andrea Massa, Member IEEE, Giacomo Oliveri, Member IEEE, Federico Viani, Member IEEE,andPaoloRocca,Member IEEE ABSTRACT | The concept of long-range wireless power trans- the state of the art for long-range wireless power transmis- mission (WPT) has been formulated shortly after the invention sion, highlighting the latest advances and innovative solutions of high power microwave amplifiers. The promise of WPT, as well as envisaging possible future trends of the research in energy transfer over large distances without the need to deploy this area. a wired electrical network, led to the development of landmark successful experiments, and provided the incentive for further KEYWORDS | Array antennas; solar power satellites; wireless research to increase the performances, efficiency, and robust- power transmission (WPT) ness of these technological solutions. In this framework, the key-role and challenges in designing transmitting and receiving antenna arrays able to guarantee high-efficiency power trans- I. INTRODUCTION fer and cost-effective deployment for the WPT system has been Long-range wireless power transmission (WPT) systems soon acknowledged. Nevertheless, owing to its intrinsic com- working in the radio-frequency (RF) range [1]–[5] are plexity, the design of WPT arrays is still an open research field currently gathering a considerable interest (Fig. -
FOX Hunting Basics FOX Hunting Basics
FOX Hunting Basics FOX Hunting Basics Steps in a transmiter hunt •Signal acquisiton •Triangulaton –Plot bearings on map to get an estmated directon of the transmiter •Homing –“follow your nose” •Snifng –Up close and personal FOX Hunting Basics Following Clues •Finding the transmiter is a process of following clues to the source of the signal. Important clues include: –Directon –Signal Strength –Rate of change in directon –Rate of change in signal strength –Terrain shadowing –Non-radio clues: keep your eyes open! FOX Hunting Basics Tools for Determining Directon •Antenna with directonal patern •Some way to measure signal strength •Some way to reduce signal strength as you get close to avoid receiver overload –“Atenuator” Bearings Bearings Waldo ©DreamWorks Distribution Limited.All rights reserved. Imagery §>2018 Google, Msg data ©2Q1S Google United States Terms Send feel Bearings Equipment Used for DF’ing Equipment Used for DF’ing Equipment Used for DF’ing Radio Attenuator Directional Antenna Equipment Used for DF’ing The attenuator is used to reduce signals so the S meter is in the middle of the scale in the presence of a strong signal Attenuator Strong Signal Equipment Used for DF’ing The attenuator is used to reduce signals so the S meter is in the middle of the scale in the presence of a strong signal Attenuator Strong Signal Equipment Used for DF’ing Time Difference of Arrival TDOA Equipment Used for DF’ing Time Difference of Arrival TDOA How it works •Time Difference of Arrival RDF sets work by switching your receiver between two antennas at a rapid rate. -
Model ATH33G50 Antenna, Standard Gain 33Ghz–50Ghz
Model ATH33G50 Antenna, Standard Gain 33GHz–50GHz The Model ATH33G50 is a wide band, high gain, high power microwave horn antenna. With a minimum gain of 20dB over isotropic, the Model ATH33G50 supplies the high intensity fields necessary for RFI/EMI field testing within and beyond the confines of a shielded room. The Model ATH33G50 is extremely compact and light weight for ready mobility, yet is built tough enough for the extra demands of outdoor use and easily mounts on a rigid waveguide by the waveguide flange. Part of a family of microwave frequency antennas, the Model ATH33G50 provides the 33-50GHz response required for many often used test specifications. The Model ATH33G50 standard gain pyramidal horn antenna is electroformed to give precise dimensions and reproducible electrical characteristics. The Model ATH33G50 is used to measure gain for other antennas by comparing the signal level of a test antenna to the signal level of a test antenna to the standard gain horn and adding the difference to the calibrated gain of the standard gain horn at the test frequency. The Model ATH33G50 is also used as a reference source in dual-channel antenna test receivers and can be used as a pickup horn for radiation monitoring. SPECIFICATIONS FREQUENCY RANGE .................................................... 33-50GHz POWER INPUT (maximum) ............................................ 240 watts CW 2000 watts Peak POWER GAIN (over isotropic) ........................................ 20 ± 2dB VSWR Average ................................................................ -
AND CLOSED- RING MICROSTRIP ANTENNAS Redacted for Privacy Abstract Approved: Dr
AN ABSTRACT OF THE THESIS OF MohammedAshrafSultan for the degree of Doctor of Philosophy in Electrical and Computer Engineering presen- ted on Alril 28, 1986 Title: THE RADIATION CHARACTERISTICS OF OPEN-AND CLOSED- RING MICROSTRIP ANTENNAS Redacted for privacy Abstract approved: Dr. Vijai°K. Tripath1- The purpose of this study is toinvestigate the radiation characteristics of open- andclosed-ring micro- strip structures for applications asmicrowave antenna elements. The expressions for the radiationfields of these structures are obtained from the aperturefields of the ideal cavity model associatedwith the microstrip structure.The expressions for theradiation fields are then used to calculate the radiationcharacteristics of these microstrip structures. The radiation fields of theideal gap structure(gap angle 0) are derived in Chapter 3. For this case the aperture fields can be expressedeither in terms of the spherical Bessel functions (odd-modes) orin terms of the Bessel functions of integer order(even-modes) which is shown to result in a convergentseries or closed form expressions respectively for theradiation fields. study of the radiation patterns for thevarious modes of the ideal gap open-ring structuresreveals that the first radial TM12 mode can potentially be an efficient useful mode for applications of this structure as aradiating element. The radiation fields of the general annularand cir- cular sectors are numerically examinedin the following chapter in terms of the various physical parametersof these structures. The derived expressions forthe radia- tion fields are used to study the radiation patterns, radiation:peak in the broadside direction andthe beam- width of these structures for various sectorangles, widths and the modes of excitation. -
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. -
Analysis and Measurement of Horn Antennas for CMB Experiments
Analysis and Measurement of Horn Antennas for CMB Experiments Ian Mc Auley (M.Sc. B.Sc.) A thesis submitted for the Degree of Doctor of Philosophy Maynooth University Department of Experimental Physics, Maynooth University, National University of Ireland Maynooth, Maynooth, Co. Kildare, Ireland. October 2015 Head of Department Professor J.A. Murphy Research Supervisor Professor J.A. Murphy Abstract In this thesis the author's work on the computational modelling and the experimental measurement of millimetre and sub-millimetre wave horn antennas for Cosmic Microwave Background (CMB) experiments is presented. This computational work particularly concerns the analysis of the multimode channels of the High Frequency Instrument (HFI) of the European Space Agency (ESA) Planck satellite using mode matching techniques to model their farfield beam patterns. To undertake this analysis the existing in-house software was upgraded to address issues associated with the stability of the simulations and to introduce additional functionality through the application of Single Value Decomposition in order to recover the true hybrid eigenfields for complex corrugated waveguide and horn structures. The farfield beam patterns of the two highest frequency channels of HFI (857 GHz and 545 GHz) were computed at a large number of spot frequencies across their operational bands in order to extract the broadband beams. The attributes of the multimode nature of these channels are discussed including the number of propagating modes as a function of frequency. A detailed analysis of the possible effects of manufacturing tolerances of the long corrugated triple horn structures on the farfield beam patterns of the 857 GHz horn antennas is described in the context of the higher than expected sidelobe levels detected in some of the 857 GHz channels during flight. -
3794 Series Granger Wideband Conical Monopole Antennas
3794 Series Granger Wideband Conical Monopole Antennas ● 2-30 MHz Bandwidth permits Frequency change without antenna tuning ● Up to 25 KW average power rating ● 50 Ohm input provides 2.0:1 nominal VSWR without impedance transformers ● Single tower ● Short, medium, long-range communications General Description The Model 3794 series antenna is a vertically polarized, omnidirectional broadband antenna for transmitting or receiving applications. It is designed for high power area coverage. The 3794 Wideband Conical Monopole Antenna is an inverted cone- like structure with it’s apex pointing downwards. The array is supported by a 17 inch (431 mm) face steel guyed tower and consists of a number of evenly spaced radiator wires. The radiators spread out from the tower top to an outer guyed catenary then converge back down at the tower base. The antenna is fed at the apex of the cone through a 50 ohm coaxial connector. A ground screen is laid over the area below the antenna and consists of a radial pattern of wire laid on the ground with it’s centre at the apex of the antenna. The radiating elements of the array are prefabricated to facilitate installation. All radiators are manufactured from aluminum clad steel wire for maximum conductivity and corrosion resistance. The mechanical arrangement provides high strength while keeping both manufacturing and installation costs to a minimum. Application The 3794 Wideband Conical Monopole Antenna Series provides a cost effective solution for the vertical omnidirectional antenna if the reduced ground area offered by the 1794 Monocone is not required. The broad frequency range permits use of the optimum frequency for any distance. -
1- Consider an Array of Six Elements with Element Spacing D = 3Λ/8. A
1- Consider an array of six elements with element spacing d = 3 λ/8. a) Assuming all elements are driven uniformly (same phase and amplitude), calculate the null beamwidth. b) If the direction of maximum radiation is desired to be at 30 o from the array broadside direction, specify the phase distribution. c) Specify the phase distribution for achieving an end-fire radiation and calculate the null beamwidth in this case. 5- Four isotropic sources are placed along the z-axis as shown below. Assuming that the amplitudes of elements #1 and #2 are +1, and the amplitudes of #3 and #4 are -1, find: a) the array factor in simplified form b) the nulls when d = λ 2 . a) b) 1- Give the array factor for the following identical isotropic antennas with N and d. 3- Design a 7-element array along the x-axis. Specifically, determine the interelement phase shift α and the element center-to-center spacing d to point the main beam at θ =25 ° , φ =10 ° and provide the widest possible beamwidth. Ψ=x kdsincosθφα +⇒= 0 kd sin25cos10 ° °+⇒=− αα 0.4162 kd nulls at 7Ψ nnπ2 nn π 2 =±, = 1,2, ⋅⋅⋅⇒Ψnull =±7 , = 1,2,3,4,5,6 α kd2π n kd d λ α −=−7 ( =⇒= 1) 0.634 ⇒= 0.1 ⇒=− 0.264 2- Two-element uniform array of isotropic sources, positioned along the z-axis λ 4 apart is seen in the figure below. Give the array factor for this array. Find the interelement phase shift, α , so that the maximum of the array factor occurs along θ =0 ° (end-fire array). -
Development of Conical Horn Feed for Reflector Antenna
International Journal of Engineering and Technology Vol. 1, No. 1, April, 2009 1793-8236 Development of Conical Horn Feed For Reflector Antenna Jagdish. M. Rathod, Member, IACSIT and Y.P.Kosta, Senior Member IEEE waveguide that provides the impedance transformation Abstract—We have designed a antenna feed with prime between the waveguide impedance and the free-space concerned that with the growing conjunctions in the mobile impedance. Horn radiators are used both as antennas in their networks, the parabolic antenna are evolving as an useful device own right, and as illuminators for reflector antennas. Horn for point to point communications where the need for high antennas are not a perfect match to the waveguide, although directivity and high power density is at the prime importance. With these needs we have designed the unusual type of feed standing wave ratios of 1.5:1 or less are achievable. The gain antenna for parabolic dish that is used for both reception and of a horn radiator is proportional to the area A of the flared transmission purpose. This different frequency band open flange), and inversely proportional to the square of the performance having horn feed, works for the parabolic wavelength [8].Following Fig.1 gives types of Horn reflector antenna. We have worked on frequency band between radiators. 4.8 GHz to 5.9 GHz for horn type of feed. Here function of the horn is to produce uniform phase front with a larger aperture than that of the waveguide and hence greater directivity. Parabolic dish antenna is the most commonly and widely used antenna in communication field mainly in satellite and radar communication. -
Enhancing the Coverage Area of a WI-FI Access Point Using Cantenna
ISSN 2394-3777 (Print) ISSN 2394-3785 (Online) Available online at www.ijartet.com International Journal of Advanced Research Trends in Engineering and Technology (IJARTET) Vol. 2, Issue 4, April 2015 Enhancing the Coverage Area of a WI-FI Access Point Using Cantenna B.Anandhaprabakaran#1, S.Shanmugam*2,J.Sridhar*3S.Ajaykumar#4 #2-4student #1Assistant Professor, Sri Ramakrishna Engineering College, Coimbatore, Tamilnadu, India Abstract: “The next decade will be the Wireless Era.” – Intel Executive Sean Maloney and other executives framed. Today’s network especially LAN has drastically changed. People expect that they should not be bound to the network. In this scenario, Wireless (WLAN) offers tangible benefits over traditional wired networking. Wi-Fi (Wireless Fidelity) is a generic term that refers to the IEEE 802.11 communications standard for Wireless Local Area Networks (WLANs). Wi-Fi works on three modes namely Ad hoc, Infrastructure and Extended modes. Ad hoc network is P2P mode. Ad hoc does not use any intermediary device such as Access Point. Infra Structure and Extended modes use Access Point as interface between wireless clients. The wireless network is formed by connecting all the wireless clients to the AP. Single access point can support up to 30 users and can function within a range of 100 – 150 feet indoors and up to 300 feet outdoors. The coverage area depends upon the location where the AP is being placed. The AP has the traditional Omni directional antenna The aim of this project is to increase the coverage area of an AP by replacing the traditional Omni directional antenna with Bi-quad antenna with parabolic reflector. -
Improving Fault Tolerance in 802.11 Wireless Long Distance Rural Networks
Improving Fault Tolerance in 802.11 Wireless Long Distance Rural Networks A Thesis Submitted in Partial Fulfillment of the Requirements for the Degree of Master of Technology by Manikantah Kodali under the guidance of Dr. Bhaskaran Raman and co-guidance of Dr. A.R. Harish Department of Computer Science and Engineering Indian Institute of Technology, Kanpur May, 2006 Abstract Wireless technology is a promising solution for providing communication facilities to rural areas. We consider a network deployment with long-distance wireless links between rural locations. One of the network locations consists of a wired connection/communication, to connect the other locations to the Internet. We call this location the central node. Towers and antennae are used for setting up long-distance wireless links in the network. Directional or sector antennae with high directional gain are used which are fixed and static. The network may be multi-hop. Individual village locations can be a few hops (say 2 or 3 hops) from the central node. One of the major issues with these types of networks is fault tolerance. When an intermediate node fails, a part of the network could get disconnected from the central node. This thesis work focuses on improving the fault tolerance of the above type of networks. For improving the fault tolerance we propose and explore three solutions. The basic idea in these solutions is to use another node as a backup node when the intermediate node fails. The first solution termed replication uses multiple directional antennae at the far-away nodes. A programmable RF-Switch is connected between the multiple antennae and the radio, the switch is programmed to select one of the directional antennae for transmission/reception as required. -
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