Development of Conical Horn Feed for Reflector Antenna
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Corrugated Feed-Horn Arrays for Future CMB Polarization Experiments Settore Scientifico Disciplinare FIS/01
UNIVERSITA` DEGLI STUDI DI MILANO FACOLTA` DI SCIENZE MATEMATICHE, FISICHE E NATURALI DOTTORATO DI RICERCA IN FISICA, ASTROFISICA E FISICA APPLICATA Corrugated feed-horn arrays for future CMB polarization experiments Settore Scientifico disciplinare FIS/01 Coordinatore: Prof. Marco BERSANELLI Tutore: Prof. Marco BERSANELLI Co-Tutore: Dott. Fabrizio VILLA Tesi di dottorato di: Francesco DEL TORTO Ciclo XXIV Anno Accademico 2011-2012 To my parents Introduction The actual most corroborated model of modern cosmology is the “Hot Big Bang Model”, that results in agree with the cosmological scientific discov- eries of the last 50 years. The main observational pillars that support the model are: the discovery by Edwin Hubble of the expansion of the Universe, the abundances of the primordial elements and the discovery of the Cosmic Microwave Background (CMB) radiation. In 1929 Edwin Hubble discovered the linear relationship in distant galax- ies between their distance and recession velocity: v = Hd. The current value for the Hubble constant is known with very high precision as 72 8 Km/sec/Mpc [1], from the measurements obtained by the Hubble Space Tele-± scope on even far distant galaxies w.r.t. to the Hubble measurements. According to the Hot Big Bang Model, in the first era of its life, the Universe was constituted by photons, electrons and protons. During this time the firsts primordial elements were produced, i.e. Helium, Deuterium, and Beryllium. The abundances of the primordial elements can be calculated with precision by the Hot Big Bang Model, resulting in good agreement with the measured abundances [2], [3]. In 1965 Arno Penzias and Robert Wilson discovered the CMB, already predicted in 1948 by George Gamow in the framework of an Hot Big Bang Model. -
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 ................................................................ -
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. -
Progress Toward Corrugated Feed Horn Arrays in Silicon Abstract
Progress Toward Corrugated Feed Horn Arrays in Silicon J. Britton,∗ K. W. Yoon, J. A. Beall, D. Becker, H. M. Cho, G. C. Hilton, M. D. Niemack, and K. D. Irwin Quantum Sensors Group, NIST, Boulder, CO 80305, USA Abstract We are developing monolithic arrays of corrugated feed horns fabricated in silicon for dual-polarization single-mode operation at 90, 145 and 220 GHz. The arrays consist of hundreds of platelet feed horns assembled from gold-coated stacks of micro- machined silicon wafers. As a first step, Au-coated Si waveguides with a circular, corrugated cross section were fabricated; their attenuation was measured to be less than 0.15 dB/cm from 80 to 110 GHz at room temperature. To ease the manufacture of horn arrays, electrolytic deposition of Au on degenerate Si without a metal seed layer was demonstrated. An apparatus for measuring the radiation pattern, optical efficiency, and spectral band-pass of prototype horns is described. Feed horn arrays made of silicon may find use in measurements of the polarization anisotropy of the cosmic microwave background radiation. Imaging detectors at millimeter wavelengths can now be built with hundreds of pixels.[1] However, parallel gains in free-space coupling optics have lagged. At NIST we are pursuing monolithic arrays of corru- gated platelet feed horns made with Si. Each layer in the stack is a Si wafer with photolithographically de- fined apertures. Once assembled and coated with Au, these horn arrays are expected to feature the same low loss, wide bandwidth, minimal side lobes and low cross- correlation as electroformed horns.[2, 3] Moreover, rel- ative to metal corrugated arrays [4], Si horn arrays are expected to have the following benefits: (a) a thermal ex- pansion matched to Si detectors, (b) lower thermal mass, and (c) a straightforward development to arrays of thou- sands of horns. -
Resolving Interference Issues at Satellite Ground Stations
Application Note Resolving Interference Issues at Satellite Ground Stations Introduction RF interference represents the single largest impact to robust satellite operation performance. Interference issues result in significant costs for the satellite operator due to loss of income when the signal is interrupted. Additional costs are also encountered to debug and fix communications problems. These issues also exert a price in terms of reputation for the satellite operator. According to an earlier survey by the Satellite Interference Reduction Group (SIRG), 93% of satellite operator respondents suffer from satellite interference at least once a year. More than half experience interference at least once per month, while 17% see interference continuously in their day-to-day operations. Over 500 satellite operators responded to this survey. Satellite Communications Overview Satellite earth stations form the ground segment of satellite communications. They contain one or more satellite antennas tuned to various frequency bands. Satellites are used for telephony, data, backhaul, broadcast, community antenna television (CATV), internet, and other services. Depending on the application, each satellite system may be receive only or constructed for both transmit and receive operations. A typical earth station is shown in figure 1. Figure 1. Satellite Earth Station Each satellite antenna system is composed of the antenna itself (parabola dish) along with various RF components for signal processing. The RF components comprise the satellite feed system. The feed system receives/transmits the signal from the dish to a horn antenna located on the feed network. The location of the receiver feed system can be seen in figure 2. The satellite signal is reflected from the parabolic surface and concentrated at the focus position. -
POWER MICROWAVE FEED HORN C. Chang Department of Engineering
Progress In Electromagnetics Research, PIER 101, 157{171, 2010 DESIGN AND EXPERIMENTS OF THE GW HIGH- POWER MICROWAVE FEED HORN C. Chang Department of Engineering Physics Tsinghua University Beijing, China X. X. Zhu, G. Z. Liu, J. Y. Fang, R. Z. Xiao, C. H. Chen H. Shao, J. W. Li, H. J. Huang, and Q. Y. Zhang Northwest Institute of Nuclear Technology Xi'an, Shannxi, China Z. Q. Zhang National Key Laboratory of Antennas and Microwave Technology Xidian University Xi'an, Shannxi, China Abstract|Design and optimization of high-power microwave (HPM) feed horn by combining the aperture ¯eld with radiation patterns are presented in the paper. The optimized feed horn in C band satis¯es relatively uniform aperture ¯eld, power capacity higher than 3 GW, symmetric radiation patterns, low sidelobes, and compact length. Cold tests and HPM experiments were conducted to investigate the radiation patterns and power capacity of the horn. The theoretical radiation patterns are consistent with the cold test and HPM experimental results. The power capacity of the compact HPM horn has been demonstrated by HPM experiments to be higher than 3 GW. 1. INTRODUCTION The maximum power produced by S-band resonant BWO has attained 5 GW with 100 J energy pulses [1]. With the development of narrowband multi-giga-watt HPM sources operated under vacuum, the power capacity of the HPM horn has become the major factor of Corresponding author: C. Chang ([email protected]). 158 Chang et al. limiting HPM transmission and radiation [2{5]. When the electric ¯eld amplitude at the aperture of the horn is higher than the breakdown threshold, secondary electron multipactor and plasma discharge happen at the vacuum side of the dielectric radome, leading to HPM breakdown and pulse shortening [2{5]. -
PARABOLIC DISH ANTENNAS Paul Wade N1BWT © 1994,1998
Chapter 4 PARABOLIC DISH ANTENNAS Paul Wade N1BWT © 1994,1998 Introduction Parabolic dish antennas can provide extremely high gains at microwave frequencies. A 2- foot dish at 10 GHz can provide more than 30 dB of gain. The gain is only limited by the size of the parabolic reflector; a number of hams have dishes larger than 20 feet, and occasionally a much larger commercial dish is made available for amateur operation, like the 150-foot one at the Algonquin Radio Observatory in Ontario, used by VE3ONT for the 1993 EME Contest. These high gains are only achievable if the antennas are properly implemented, and dishes have more critical dimensions than horns and lenses. I will try to explain the fundamentals using pictures and graphics as an aid to understanding the critical areas and how to deal with them. In addition, a computer program, HDL_ANT is available for the difficult calculations and details, and to draw templates for small dishes in order to check the accuracy of the parabolic surface. Background In September 1993, I finished my 10 GHz transverter at 2 PM on the Saturday of the VHF QSO Party. After a quick checkout, I drove up Mt. Wachusett and worked four grids using a small horn antenna. However, for the 10 GHz Contest the following weekend, I wanted to have a better antenna ready. Several moderate-sized parabolic dish reflectors were available in my garage, but lacked feeds and support structures. I had thought this would be no problem, since lots of people, both amateur and commercial, use dish antennas. -
Design and Analysis of Pyramidal Horn Antenna
www.ijcrt.org © 2020 IJCRT | Volume 8, Issue 3 March 2020 | ISSN: 2320-2882 Design and analysis of pyramidal Horn antenna 1 Mrs. Rikita Gohil, 2 Mrs. Niti P. Gupta Electronics and Communication Engineering Department S.V.I.T. Vasad, Gujarat, India Abstract: This paper discusses the design of a pyramidal horn antenna with high gain, suppressed side lobes. The horn antenna is widely used in the transmission and reception of RF microwave signals. Horn antennas are extensively used in the fields of T.V. broadcasting, microwave devices and satellite communication. It is usually an assembly of flaring metal, waveguide and antenna. The physical dimensions of pyramidal horn that determine the performance of the antenna. The length, flare angle, aperture diameter of the pyramidal antenna is observed. These dimensions determine the required characteristics such as impedance matching, radiation pattern of the antenna. The antenna gives gain of about 25.5 dB over operating range while delivering 10 GHz bandwidth. Ansoft HFSS 13 software is used to simulate the designed antenna. Pyramidal horn can be designed in a variety of shapes in order to obtain enhanced gain and bandwidth. The designed Pyramidal Horn Antenna is functional for each X-Band application. The horn is supported by a rectangular wave guide. Index Terms - Gain, Horn, Impedance, RF, Rectangular Waveguide, Return loss, Radiation pattern. INTRODUCTION Pyramidal horn is one type of aperture antenna flared in both directions, a combination of E-plane and H-plane horns. 3D figure is shown as Figure 1.Horn antennas are commonly used as a standard gain antenna for calibration purpose of other antennas. -
A Flexible 2.45 Ghz Rectenna Using Electrically Small Loop Antenna
A Flexible 2.45 GHz Rectenna Using Electrically Small Loop Antenna Khaled Aljaloud1,2, Kin-Fai Tong1 1Electronic and Electrical Engineering Department, University College London, London, UK, [email protected] 2Electrical Engineering Department, King Saud University, Riyadh, Saudi Arabia Abstract—We present the concept and design of a compact schlocky diode connected in series to one of the two feed flexible electromagnetic energy-harvesting system using electri- terminals of the antenna and to the coplanar transmission line, cally small loop antenna. In order to make the integration of the a capacitor to minimize the ripple level. The reported system system with other devices simpler, it is designed as an integrated system in such a way that the collector element and the rectifier in this letter is sufficiently capable of reusing low microwave circuit are mounted on the same side of the substrate. The energy for both flat and curved configurations. rectenna is designed and fabricated on flexible substrate, and its performance is verified through measurement for both flat and curved configurations. The DC output power and the efficiency II. DESIGN AND RESULT are investigated with respect to power density and frequency. It is observed through measurements that the proposed system The two main parts of rectenna system are largely designed can achieve 72% conversion efficiency for low input power level, individually and unified through the matching network. In this -11 dBm (corresponding power density 0.2 W=m2), while at the work, the proposed rectenna is built as an integral system, and same time occupying a smaller footprint area compared to the thus the rectifier circuit is matched to the collector to maximize existing work. -
Characteristics of Naval Fire . Control Radar
COPY~ CO NFI oP 1895· CHARACTERISTICS OF ,. NAVAL FIRE .CONTROL RADAR • ~ r' -i8Nfi6ENtiAt• ABUREAU OF ORDNANCE PUBLICATION ~ OP 1895 CHARACTERISTICS OF NAVAL FIRE CONTROL RADAR 12 NOVEMBER 1954 DEPARTMENT OF THE NAVY BUREAU OF ORDNANCE WASHINGTON 25, D. C. 12 November 1954 ORDNANCE PAMPHLET 1895 CHARACTERISTICS OF NAVAL FIRE CONTROL RADAR 1. Ordnance Pamphlet 1895 describes both the fundamental principles of operation of radar equipment in general and the characteristics of specific United States Naval fire control radar equipment. 2. This publication is intended for use by all personnel concerned with radar operation in general, and with the application of basic radar principles to fire control radar. 3. This publication does not supersede any existing publication. 4. This publication is El8N¥'1!HU! AitL and shall be safeguarded in ac cordance with the security provisions of U. S. Navy Regulations. It is for bidden to make extracts from or to copy this classified document, except as provided for in Article 0910 of the United States Navy Security Manual for Classified Matter. M. F. ScHoEFFEL Rear Admiral, U. S. Navy Ohief, Bureau of Ordnance .tONFIDENTIAL- 'i!Qt 'FilEt 'IJ,ll CONTENTS Chapter Page Chapte1· Page FOREWORD vi 2. Close-in Targets ............. 28 (cont) Merging Targets ............. 28 PART I-GENERAL Propeller Modulation ......... 28 1. PRINCIPLES OF THE RADAR ART 1 Geographical and Atmospheric The Echo Principle ............. 1 Conditions ................ 28 The Radio Echo at Work ......... 1 Low-flying Targets ........... 29 Radar Measurements ........... 2 Land Echoes ................ 29 Factors Affecting Radar Radar Countermeasures ...... 31 Measurements ............... 6 Spotting Surface Gun Fire ...... 32 Power and Range ............ 6 Range Spotting ............. -
Highlights of Antenna History
~~ IEEE COMMUNICATIONS MAGAZINE HlOHLlOHTS OF ANTENNA HISTORY JACK RAMSAY A look at the major events in the development of antennas. wires. Antenna systems similar to Edison’s were used by A. E. Dolbear in 1882 when he successfully and somewhat mysteriously succeeded in transmitting code and even speech to significant ranges, allegedly by groundconduction. NINETEENTH CENTURY WIRE ANTENNAS However, in one experiment he actually flew the first kite T is not surprising that wire antennas were inaugurated antenna.About the same time, the Irish professor, in 1842 by theinventor of wire telegraphy,Joseph C. F. Fitzgerald, calculated that a loop would radiate and that Henry, Professor’ of Natural Philosophy at Princeton, a capacitance connected to a resistor would radiate at VHF NJ. By “throwing a spark” to a circuit of wire in an (undoubtedly due to radiation from the wire connecting leads). Iupper room,Henry found that thecurrent received in a In Hertz launched,processed, and received radio 1887 H. parallel circuit in a cellar 30 ft below codd.magnetize needies. waves systematically. He used a balanced or dipole antenna With a vertical wire from his study to the roof of his house, he attachedto ’ an induction coilas a transmitter, and a detected lightning flashes 7-8 mi distant. Henry also sparked one-turn loop (rectangular) containing a sparkgap as a to a telegraph wire running from his laboratory to his house, receiver. He obtained “sympathetic resonance” by tuning the and magnetized needles in a coil attached to a parailel wire dipole with sliding spheres, and the loop by adding series 220 ft away. -
Day 2 Session 3
Day 2 Session 3 VSAT installation 1 1- VSAT Installation IDU Satellite receivers and routers are versatile and powerful networking platforms that receive and manage content at the network edge Modern IDUs incorporate many functions: • Routing • Encryption • Compression • Acceleration • QoS • Modem • NMS 2 1- VSAT Installation Satellite Modems Satellite modems have several options that must be considered: • 70/140 MHz or L-band IF • BUC power supply • Voltage of BUC power supply (24 or 48) 3 1- VSAT Installation Router Routers are available from a variety of manufacturers but most modern satellite modems and IDU’s incorporate this functionality internally. Modem based routers provide features not generally found in terrestrial routers: • Compatibility with encapsulators • TCP spoofing (to reduce latency and improve speed) 4 1- VSAT Installation Firewall Firewalls provide proactive threat defense that stops attacks before they spread through the network. 5 1- VSAT Installation Typical configuration 6 1- VSAT Installation Sample Hardware list The VSAT system consists of the following hardware: • The Indoor unit • The Outdoor unit assembly 7 1- VSAT Installation Sample Hardware list The outdoor unit assembly consists of: TRF FEED OMT • OMT (Orthomode Transducer) separates the transmit signal from the received signal, taking advantage of their different polarization. • TRF (Transmit Reject Filter) prevents the high power transmit signal from entering (and overloading) the receive chain. 8 1- VSAT Installation Sample Hardware list The outdoor unit assembly consists of: LNB BUC • LNB (for the receiving signal). The LNB converts the C/Ku band signal received from the satellite into an L band signal. • BUC. The BUC converts the L band signal from the IDU into a C/Ku band signal for transmission.