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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. -
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. -
Electronic Spectroscopy of Free Base Porphyrins and Metalloporphyrins
Absorption and Fluorescence Spectroscopy of Tetraphenylporphyrin§ and Metallo-Tetraphenylporphyrin Introduction The word porphyrin is derived from the Greek porphura meaning purple, and all porphyrins are intensely coloured1. Porphyrins comprise an important class of molecules that serve nature in a variety of ways. The Metalloporphyrin ring is found in a variety of important biological system where it is the active component of the system or in some ways intimately connected with the activity of the system. Many of these porphyrins synthesized are the basic structure of biological porphyrins which are the active sites of numerous proteins, whose functions range from oxygen transfer and storage (hemoglobin and myoglobin) to electron transfer (cytochrome c, cytochrome oxidase) to energy conversion (chlorophyll). They also have been proven to be efficient sensitizers and catalyst in a number of chemical and photochemical processes especially photodynamic therapy (PDT). The diversity of their functions is due in part to the variety of metals that bind in the “pocket” of the porphyrin ring system (Fig. 1). Figure 1. Metallated Tetraphenylporphyrin Upon metalation the porphyrin ring system deprotonates, forming a dianionic ligand (Fig. 2). The metal ions behave as Lewis acids, accepting lone pairs of electrons ________________________________ § We all need to thank Jay Stephens for synthesizing the H2TPP 2 from the dianionic porphyrin ligand. Unlike most transition metal complexes, their color is due to absorption(s) within the porphyrin ligand involving the excitation of electrons from π to π* porphyrin ring orbitals. Figure 2. Synthesis of Zn(TPP) The electronic absorption spectrum of a typical porphyrin consists of a strong transition to the second excited state (S0 S2) at about 400 nm (the Soret or B band) and a weak transition to the first excited state (S0 S1) at about 550 nm (the Q band). -
Supplemental Information for an Amateur Radio Facility
COMMONWEALTH O F MASSACHUSETTS C I T Y O F NEWTON SUPPLEMENTAL INFORMA TION FOR AN AMATEUR RADIO FACILITY ACCOMPANYING APPLICA TION FOR A BUILDING PERMI T, U N D E R § 6 . 9 . 4 . B. (“EQUIPMENT OWNED AND OPERATED BY AN AMATEUR RADIO OPERAT OR LICENSED BY THE FCC”) P A R C E L I D # 820070001900 ZON E S R 2 SUBMITTED ON BEHALF OF: A LEX ANDER KOPP, MD 106 H A R TM A N ROAD N EWTON, MA 02459 C ELL TELEPHONE : 617.584.0833 E- MAIL : AKOPP @ DRKOPPMD. COM BY: FRED HOPENGARTEN, ESQ. SIX WILLARCH ROAD LINCOLN, MA 01773 781/259-0088; FAX 419/858-2421 E-MAIL: [email protected] M A R C H 13, 2020 APPLICATION FOR A BUILDING PERMIT SUBMITTED BY ALEXANDER KOPP, MD TABLE OF CONTENTS Table of Contents .............................................................................................................................................. 2 Preamble ............................................................................................................................................................. 4 Executive Summary ........................................................................................................................................... 5 The Telecommunications Act of 1996 (47 USC § 332 et seq.) Does Not Apply ....................................... 5 The Station Antenna Structure Complies with Newton’s Zoning Ordinance .......................................... 6 Amateur Radio is Not a Commercial Use ............................................................................................... 6 Permitted by -
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. -
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. -
Spectrum and the Technological Transformation of the Satellite Industry Prepared by Strand Consulting on Behalf of the Satellite Industry Association1
Spectrum & the Technological Transformation of the Satellite Industry Spectrum and the Technological Transformation of the Satellite Industry Prepared by Strand Consulting on behalf of the Satellite Industry Association1 1 AT&T, a member of SIA, does not necessarily endorse all conclusions of this study. Page 1 of 75 Spectrum & the Technological Transformation of the Satellite Industry 1. Table of Contents 1. Table of Contents ................................................................................................ 1 2. Executive Summary ............................................................................................. 4 2.1. What the satellite industry does for the U.S. today ............................................... 4 2.2. What the satellite industry offers going forward ................................................... 4 2.3. Innovation in the satellite industry ........................................................................ 5 3. Introduction ......................................................................................................... 7 3.1. Overview .................................................................................................................. 7 3.2. Spectrum Basics ...................................................................................................... 8 3.3. Satellite Industry Segments .................................................................................... 9 3.3.1. Satellite Communications .............................................................................. -
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. -
Choosing a Ham Radio
Choosing a Ham Radio Your guide to selecting the right equipment Lead Author—Ward Silver, NØAX; Co-authors—Greg Widin, KØGW and David Haycock, KI6AWR • About This Publication • Types of Operation • VHF/UHF Equipment WHO NEEDS THIS PUBLICATION AND WHY? • HF Equipment Hello and welcome to this handy guide to selecting a radio. Choos- ing just one from the variety of radio models is a challenge! The • Manufacturer’s Directory good news is that most commercially manufactured Amateur Radio equipment performs the basics very well, so you shouldn’t be overly concerned about a “wrong” choice of brands or models. This guide is intended to help you make sense of common features and decide which are most important to you. We provide explanations and defini- tions, along with what a particular feature might mean to you on the air. This publication is aimed at the new Technician licensee ready to acquire a first radio, a licensee recently upgraded to General Class and wanting to explore HF, or someone getting back into ham radio after a period of inactivity. A technical background is not needed to understand the material. ABOUT THIS PUBLICATION After this introduction and a “Quick Start” guide, there are two main sections; one cov- ering gear for the VHF and UHF bands and one for HF band equipment. You’ll encounter a number of terms and abbreviations--watch for italicized words—so two glossaries are provided; one for the VHF/UHF section and one for the HF section. You’ll be comfortable with these terms by the time you’ve finished reading! We assume that you’ll be buying commercial equipment and accessories as new gear. -
Infrared Astronomy Break: Sara and Rebeka
Astro 121, Spring 2014 Week 13 (April 24) Topic: Infrared astronomy Break: Sara and Rebeka Reading for this week: As we switch to looking at observing at wavelengths other than visible light, we’re moving beyond what Chromey covers. For this week, I’ve suggested reading from two sources. Glass gives a good introduction to the infrared and covers much of the practical material about filter systems, etc. McLean then fills in more details of practicalities of instrumentation for the infrared and how it is different from the optical. • Chromey briefly discusses the main broadband IR filter system in Section 10.4.3. • Glass, Handbook of Infrared Astronomy. In the same series as the book by Howell, this is a relatively new book with excellent coverage of infrared astronomy. Reading: Chapter 2 (The Infrared Sky); Chapter 3 (Photometry) through 3.2; and Chapter 6 (Instrumentation). You may also want to skim the rest of Chapter 3 and all of Chapter 4; they concentrate on applications of infrared photometry and spectroscopy, respectively. • McLean, Electronic Imaging in Astronomy (second edition). Ian McLean was one of the people most closely involved in the development and use of the early infrared arrays, and this is an area where this book stands out. Read Chapter 11, skipping pp. 400–404 (and in general reading the chapter for understanding of concepts rather than lots of details). One bit of physics that is worth reviewing for this week is the concept from thermodynamics that good absorbers are also good emitters, and correspondingly that the reflectivity R of some object is related to its emissivity ε by ε = 1 – R. -
Custom Products
Back to MiMixxerer Home Page CUSTOM PRODUCTS Table of Contents Introduction Detailed Data Sheets Questions & Answers 100 Davids Drive • Hauppauge, NY 11788 • 631-436-7400 • Fax: 631-436-7430 • www.miteq.com TABLETABLE OF CONTENTS OF CONTENTS (CONT.) CONTENTS CONTENTS MULTIPLIERS (CONT.) CUSTOM PRODUCTS Detailed Data Sheets Detailed Data Sheets (Cont.) Passive Frequency Doublers Low-Noise Block Downconverter Octave Bandwidth Four-Channel Downconverter Module Millimeter Five-Channel Downconverter Module CONTENTSMultioctave Bandwidth with Input RF Switch/Limiter CUSTOMDrop-In PRODUCTS and LO Amplifier/Divider ActiveCONTENTS Frequency Doublers Block Diagram of MITEQ 5-Channel Gain GeneralNarrow and Octave Bandwidth and Phase-Matched Front-End QuickIntDrop-InTION Reference Applications of Five-Channel Front Ends Millimeter Four-Channel 1 to 18 GHz TypicalMultioctaveCorporate Subsystem Bandwidth Overview Worksheet Image Rejection Downconverter Millimeter Three-Channel Mixer Amplifier UsefulActiveTechnology Multiplier System Assemblies Formulas Overview Direct Microwave Digital I/Q DetailedX2Specification Data Sheets Definitions Modulator System Millimeter Integrated Upconverter and Three-ChannelX3Quality Assurance LNA Downconverter Module Power Amplifier Low-NoiseMTBFMillimeter Calculations Block Downconverter Block Downconverter X4 Low-Noise Block Converter Four-ChannelManufacturingMillimeter Downconverter Flow Diagrams Module X-Band Low-Noise Block Converter Five-ChannelX5Device 883 DownconverterScreening Module Switched Power Amplifier Assembly