Radio Frequency Interference (Rfi) Mapping for Radio Astronomy in Peninsular Malaysia
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
2010 NCJ Jan Feb Cover.Pmd
$4 WWW.RADiOSCAMATORUL.Hi2.RO ■ Adapting the Ameritron RCS-4 for Remote-SiteWWW.GiURUMELE.Hi2.RO Antenna Switching ■ NCJ Reviews: Up the Tower by Steve Morris, K7LXC ■ Results: Summer 2009 NAQP (CW, SSB, RTTY) ■ Results: Fall 2009 NA Sprint (CW, SSB, RTTY) Top Photo: Rick, K6VVA, chronicles his lessons learned while building a remote contesting station at “Locust Peak.” Bottom Photo: NCJ remembers the four members of the C6APR team, who died tragically while en route to the Bahamas for the 2009 CQ WW SSB: (L-R) Ed, K3IXD; Randy, K4QO; Pete, W2GJ, and Dallas, W3PP. 225 Main Street • Newington, CT 06111-1494 CT Newington, • Street Main 225 American Radio Relay League Relay Radio American NCJ : The National Contest Journal Contest National The : Array Solutions Your Source for Outstanding Radio Products Count on us for sound, reliable, effi cient and effective equipment. It’s been our passion for over 18 years. Make sure to visit our website to see all that we have to offer. WWW.RADiOSCAMATORUL.Hi2.ROFeaturing... Antenna Switches EightPak 8X2 RF Matrix Antenna Switch ■ 8 antennas can switch between 2 radios to cover more bands and antennas. ■ High isolation between all ports means safe reliable operation without risk to New! radio front ends. ■ CoverC MOREMORE Single 4-wire control cable, makes wiring easy and economical. Bands and Antennas! ■ Multiple EightPaks can use the same control cable simplifying wiring of large installations. ■ Can be used with the manual controller or via RS-232 or USB interface. WWW.GiURUMELE.Hi2.ROIncludes an application to allow full-confi guration of multiple switches and antenna selection assignments. -
Radio Astronomy
Theme 8: Beyond the Visible I: radio astronomy Until the turn of the 17th century, astronomical observations relied on the naked eye. For 250 years after this, although astronomical instrumentation made great strides, the radiation being detected was still essentially confined to visible light (Herschel discovered infrared radiation in 1800, and the advent of photography opened up the near ultraviolet, but these had little practical significance). This changed dramatically in the mid-20th century with the advent of radio astronomy. 8.1 Early work: Jansky and Reber The atmosphere is transparent to visible light, but opaque to many other wavelengths. The only other clear “window” of transparency lies in the radio region, between 1 mm and 30 m wavelength. One might expect that the astronomical community would deliberately plan to explore this region, but in fact radio astronomy was born almost accidentally, with little if any involvement of professional astronomers. Karl Jansky (1905−50) was a radio engineer at Bell Telephone. In 1932, while studying the cause of interference on the transatlantic radio-telephone link, he discovered that part of the interference had a periodicity of one sidereal day (23h 56m), and must therefore be coming from an extraterrestrial source. By considering the time at which the interference occurred, Jansky identified the source as the Milky Way. This interesting finding was completely ignored by professional astronomers, and was followed up only by the radio engineer and amateur astronomer Grote Reber (1911−2002). Reber built a modern-looking paraboloid antenna and constructed maps of the radio sky, which also failed to attract significant professional attention. -
Silicon Flatirons Leadership 8-9
2013 ANNUAL REPORT Silicon Flatirons A Center for Law, Technology, and Entrepreneurship at the University of Colorado TABLE OF CONTENTS Letter from the Executive Director 4-5 About Silicon Flatirons 6-7 Silicon Flatirons Leadership 8-9 Mission Elevate the Debate Surrounding Technology Policy Issues 10-11 Support and Enable Entrepreneurship in the Technology Community 12-15 Inspire, Prepare, and Place Students in Technology and Entrepreneurial Law 16-19 Output Calendar of Events 20-21 Silicon Flatirons Reports and Faculty Publications 22 People Silicon Flatirons Fellows 23 Affiliated Faculty 24-25 Advisory Boards 26-27 Supporters 28-29 www.silicon-flatirons.org 3 LEttER FROM THE EXECUTIVE DIRECTOR Federal Trade Commission to direct our IP/IT Initiative. Paul is through two summer programs we now host—(1) the placement tremendous such opportunity. The Silicon Flatirons’ engagement recently brought this experience to bear at our January 17th of Colorado students in technology law and policy summer in the community is also evident from our range of research conference on Privacy Harm. We also brought back Blake Reid internships in Washington, D.C. (including those supported by the reports related to entrepreneurship and innovation—ranging from (’10) as the Director of our Samuelson-Glushko Technology Dale Hatfield Scholars Program); and (2) a new Colorado-based the Denver Startup Scene to University Outreach to Health Care Law and Policy Clinic. In addition to directing the TLPC, Blake program that places students with technology companies after Innovation. assumed the lead role for the Silicon Flatirons Technology Policy completing a rigorous boot camp. If you are interested in getting DC Internship program. -
Hnh ENGINEERING
HnHENGINEERING OVERVIEW 1991 has been a productive and rewarding year for Engineers throughout the Corporation. Important projects that have come to fruition include the Broadcasting Centre at Southampton, the Blackstaff development in Belfast, the Millbank parliamentary broadcasting facility, the new Manchester vehicle maintenance base, Television Centre Stage V, Skelton C HF station, and many more, as detailed in the following pages. The year will also be remembered for notable progress on the digital front. The new D3 digital video recorder is rapidly becoming established as the main post production machine, and high quality digital stereo television sound is now available to more than 70% of the BBC's audience via NlCAM 728. However the most notable 'digital event' of 1991 could turn out to be the Digital Audio Broadcasting (DAB) demon- strations that we mounted in Birmingham in July. These demonstrations showed that DAB can deliver CD-quality digital sound to fixed, portable, or car receivers, even in inhospitable reception areas. Some difficulties remain to be overcome, including the need to get agreement on a frequency assignment for new DAB radio services. Nevertheless, most of those attending the demonstrations were convinced that they had witnessed a major technical advance in sound broad- casting, whose introduction cannot long be delayed. TRANSMISSIO TRANSMISSION OPERATIONS As a result of the Broadcasting Act, the transmission responsibilities previously discharged by the IBA United Kingdom have been taken over by a private company, National Skelton C, opened in May 1991 by Mark Transcommunications Limited (NTL). In order to deal Lennox-Boyd, Under Secretary for with the consequent mutual charging for site faci- Foreign and Commonwealth Affairs, is fully lities a computer database has been established, automated and is the UK's first high-power HF which deals with the complicated charging system transmitting station to be operated as a remote and maintains records of NTLfacilities on BBC sites. -
Micro-Level Econometric and Water-Quality Modeling: Simulation of Nutrient Management Policy Effects Christopher Sean Burkart Iowa State University
Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 2006 Micro-level econometric and water-quality modeling: simulation of nutrient management policy effects Christopher Sean Burkart Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Part of the Agricultural Economics Commons, and the Economics Commons Recommended Citation Burkart, Christopher Sean, "Micro-level econometric and water-quality modeling: simulation of nutrient management policy effects " (2006). Retrospective Theses and Dissertations. 1804. https://lib.dr.iastate.edu/rtd/1804 This Dissertation is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Micro-level econometric and water-quality modeling: simulation of nutrient management policy effects by Christopher Sean Burkart A dissertation submitted to the graduate faculty in partial fulfillment of the requirements for the degree of DOCTOR OF PHILOSOPHY Major: Economics Program of Study Committee: Catherine L. Kling, Major Professor Bruce Babcock Roy Gu Joseph Herriges Jinhua Zhao Iowa State University Ames, Iowa 2006 Copyright © Christopher Sean Burkart, 2006. All rights reserved. UMI Number: 3217259 INFORMATION TO USERS The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleed-through, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send a complete manuscript and there are missing pages, these will be noted. -
Essential Radio Astronomy
February 2, 2016 Time: 09:25am chapter1.tex © Copyright, Princeton University Press. No part of this book may be distributed, posted, or reproduced in any form by digital or mechanical means without prior written permission of the publisher. 1 Introduction 1.1 AN INTRODUCTION TO RADIO ASTRONOMY 1.1.1 What Is Radio Astronomy? Radio astronomy is the study of natural radio emission from celestial sources. The range of radio frequencies or wavelengths is loosely defined by atmospheric opacity and by quantum noise in coherent amplifiers. Together they place the boundary be- tween radio and far-infrared astronomy at frequency ν ∼ 1 THz (1 THz ≡ 1012 Hz) or wavelength λ = c/ν ∼ 0.3 mm, where c ≈ 3 × 1010 cm s−1 is the vacuum speed of light. The Earth’s ionosphere sets a low-frequency limit to ground-based radio astronomy by reflecting extraterrestrial radio waves with frequencies below ν ∼ 10 MHz (λ ∼ 30 m), and the ionized interstellar medium of our own Galaxy absorbs extragalactic radio signals below ν ∼ 2 MHz. The radio band is very broad logarithmically: it spans the five decades between 10 MHz and 1 THz at the low-frequency end of the electromagnetic spectrum. Nearly everything emits radio waves at some level, via a wide variety of emission mechanisms. Few astronomical radio sources are obscured because radio waves can penetrate interstellar dust clouds and Compton-thick layers of neutral gas. Because only optical and radio observations can be made from the ground, pioneering radio astronomers had the first opportunity to explore a “parallel universe” containing unexpected new objects such as radio galaxies, quasars, and pulsars, plus very cold sources such as interstellar molecular clouds and the cosmic microwave background radiation from the big bang itself. -
Wide-Band, Low-Frequency Pulse Profiles of 100 Radio Pulsars With
A&A 586, A92 (2016) Astronomy DOI: 10.1051/0004-6361/201425196 & c ESO 2016 Astrophysics Wide-band, low-frequency pulse profiles of 100 radio pulsars with LOFAR M. Pilia1,2, J. W. T. Hessels1,3,B.W.Stappers4, V. I. Kondratiev1,5,M.Kramer6,4, J. van Leeuwen1,3, P. Weltevrede4, A. G. Lyne4,K.Zagkouris7, T. E. Hassall8,A.V.Bilous9,R.P.Breton8,H.Falcke9,1, J.-M. Grießmeier10,11, E. Keane12,13, A. Karastergiou7 , M. Kuniyoshi14, A. Noutsos6, S. Osłowski15,6, M. Serylak16, C. Sobey1, S. ter Veen9, A. Alexov17, J. Anderson18, A. Asgekar1,19,I.M.Avruch20,21,M.E.Bell22,M.J.Bentum1,23,G.Bernardi24, L. Bîrzan25, A. Bonafede26, F. Breitling27,J.W.Broderick7,8, M. Brüggen26,B.Ciardi28,S.Corbel29,11,E.deGeus1,30, A. de Jong1,A.Deller1,S.Duscha1,J.Eislöffel31,R.A.Fallows1, R. Fender7, C. Ferrari32, W. Frieswijk1, M. A. Garrett1,25,A.W.Gunst1, J. P. Hamaker1, G. Heald1, A. Horneffer6, P. Jonker20, E. Juette33, G. Kuper1, P. Maat1, G. Mann27,S.Markoff3, R. McFadden1, D. McKay-Bukowski34,35, J. C. A. Miller-Jones36, A. Nelles9, H. Paas37, M. Pandey-Pommier38, M. Pietka7,R.Pizzo1,A.G.Polatidis1,W.Reich6, H. Röttgering25, A. Rowlinson22, D. Schwarz15,O.Smirnov39,40, M. Steinmetz27,A.Stewart7, J. D. Swinbank41,M.Tagger10,Y.Tang1, C. Tasse42, S. Thoudam9,M.C.Toribio1,A.J.vanderHorst3,R.Vermeulen1,C.Vocks27, R. J. van Weeren24, R. A. M. J. Wijers3, R. Wijnands3, S. J. Wijnholds1,O.Wucknitz6,andP.Zarka42 (Affiliations can be found after the references) Received 20 October 2014 / Accepted 18 September 2015 ABSTRACT Context. -
Great Discoveries Made by Radio Astronomers During the Last Six Decades and Key Questions Today
17_SWARUP (G-L)chiuso_074-092.QXD_Layout 1 01/08/11 10:06 Pagina 74 The Scientific Legacy of the 20th Century Pontifical Academy of Sciences, Acta 21, Vatican City 2011 www.pas.va/content/dam/accademia/pdf/acta21/acta21-swarup.pdf Great Discoveries Made by Radio Astronomers During the Last Six Decades and Key Questions Today Govind Swarup 1. Introduction An important window to the Universe was opened in 1933 when Karl Jansky discovered serendipitously at the Bell Telephone Laboratories that radio waves were being emitted towards the direction of our Galaxy [1]. Jansky could not pursue investigations concerning this discovery, as the Lab- oratory was devoted to work primarily in the field of communications. This discovery was also not followed by any astronomical institute, although a few astronomers did make proposals. However, a young electronics engi- neer, Grote Reber, after reading Jansky’s papers, decided to build an inno- vative parabolic dish of 30 ft. diameter in his backyard in 1935 and made the first radio map of the Galaxy in 1940 [2]. The rapid developments of radars during World War II led to the dis- covery of radio waves from the Sun by Hey in 1942 at metre wavelengths in UK and independently by Southworth in 1942 at cm wavelengths in USA. Due to the secrecy of the radar equipment during the War, those re- sults were published by Southworth only in 1945 [3] and by Hey in 1946 [4]. Reber reported detection of radio waves from the Sun in 1944 [5]. These results were noted by several groups soon after the War and led to intensive developments in the new field of radio astronomy. -
University of Groningen the Logistic Design of the LOFAR Radio Telescope Schakel, L.P
University of Groningen The logistic design of the LOFAR radio telescope Schakel, L.P. IMPORTANT NOTE: You are advised to consult the publisher's version (publisher's PDF) if you wish to cite from it. Please check the document version below. Document Version Publisher's PDF, also known as Version of record Publication date: 2009 Link to publication in University of Groningen/UMCG research database Citation for published version (APA): Schakel, L. P. (2009). The logistic design of the LOFAR radio telescope: an operations Research Approach to optimize imaging performance and construction costs. PrintPartners Ipskamp B.V., Enschede, The Netherlands. Copyright Other than for strictly personal use, it is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), unless the work is under an open content license (like Creative Commons). Take-down policy If you believe that this document breaches copyright please contact us providing details, and we will remove access to the work immediately and investigate your claim. Downloaded from the University of Groningen/UMCG research database (Pure): http://www.rug.nl/research/portal. For technical reasons the number of authors shown on this cover page is limited to 10 maximum. Download date: 26-09-2021 Chapter 2 Radio Telescopes 2.1 Introduction This chapter explains the basics of radio telescopes, the types of radio telescopes that exist, and what they can observe in the universe. It is included to provide the reader background information on radio telescopes and to introduce concepts which will be used in later chapters. -
Recovery Plan for the Cook Inlet Beluga Whale (Delphinapterus Leucas)
Recovery Plan for the Cook Inlet Beluga Whale (Delphinapterus leucas) National Marine Fisheries Service National Oceanic and Atmospheric Administration December 2016 Cover photo is a composite of two photographs and was created specifically for this document. Use by permission only: Anchorage photo: Michael Benson Beluga photo: T. McGuire, LGL Alaska Research Associates, Inc., under MMPA/ESA Research permit # 14210 Cook Inlet Beluga Whale DISCLAIMER Recovery Plan DISCLAIMER Recovery plans delineate such reasonable actions as may be necessary, based upon the best scientific and commercial data available, for the conservation and survival of listed species. Plans are published by the National Marine Fisheries Service (NMFS), sometimes prepared with the assistance of recovery teams, contractors, State agencies, and others. Recovery plans do not necessarily represent the views, official positions, or approval of any individuals or agencies involved in the plan formulation, other than NMFS. They represent the official position of NMFS only after they have been signed by the Assistant Administrator. Recovery plans are guidance and planning documents only; identification of an action to be implemented by any public or private party does not create a legal obligation beyond existing legal requirements. Nothing in this plan should be construed as a commitment or requirement that any Federal agency obligate or pay funds in any one fiscal year in excess of appropriations made by Congress for that fiscal year in contravention of the Anti-Deficiency Act, 31 U.S.C. § 1341, or any other law or regulation. Approved recovery plans are subject to modification as dictated by new findings, changes in species status, and the completion of recovery actions. -
Fundamentals of Radio Astronomy
• 4.85 GHz radio image The Radio Sky at 4.85 GHz • 45 degrees wide • brightest irregular sources are clouds of ionized hydrogen The Radio Universe Dr. Chuck Higgins Middle Tennessee State University • Supernovae remnants appear as faint radio rings • Radio "stars" scattered over the sky - most are luminous radio galaxies 9 (c) National Radio Astronomy Observatory / Associated or quasars (average distance > 5 x 10 ly) Universities, Inc. / National Science Foundation • 4.85 GHz radio image The Radio Sky at 4.85 GHz • 45 degrees wide • brightest irregular sources are clouds of ionized hydrogen Outline 1.The Radio Sky and the EM Spectrum 2.Radio Telescopes 3.What We Learn and Major Discoveries 4.Sources of Radio Emission 5.Examples – Sun, Planets, Stars, Pulsars, Galaxies, etc. 6.Radio JOVE • Supernovae remnants appear as faint radio rings • Radio "stars" scattered over the sky - most are luminous radio galaxies 9 (c) National Radio Astronomy Observatory / Associated or quasars (average distance > 5 x 10 ly) Universities, Inc. / National Science Foundation Radio Astronomy the study of radio waves originating outside Earth’s atmosphere Radio Window 1 THz – 10 MHz 0.3 mm – 30 m Credit: Adapted from STScI/JHU/NASA Radio Telescopes Concept Drawing of the Square Kilometer Array, Australia Green Bank Telescope (NRAO, NSF) Fast Radio Telescope (China) 500 m dish VLA, New Mexico (NRAO, NSF) Itty Bitty Radio Telescope Radio Telescopes Radio Waves Image Credit: Windows to the Universe Radio waves = electromagnetic waves generally caused by moving charged -
ASTRONET ERTRC Report
Radio Astronomy in Europe: Up to, and beyond, 2025 A report by ASTRONET’s European Radio Telescope Review Committee ! 1!! ! ! ! ERTRC report: Final version – June 2015 ! ! ! ! ! ! 2!! ! ! ! Table of Contents List%of%figures%...................................................................................................................................................%7! List%of%tables%....................................................................................................................................................%8! Chapter%1:%Executive%Summary%...............................................................................................................%10! Chapter%2:%Introduction%.............................................................................................................................%13! 2.1%–%Background%and%method%............................................................................................................%13! 2.2%–%New%horizons%in%radio%astronomy%...........................................................................................%13! 2.3%–%Approach%and%mode%of%operation%...........................................................................................%14! 2.4%–%Organization%of%this%report%........................................................................................................%15! Chapter%3:%Review%of%major%European%radio%telescopes%................................................................%16! 3.1%–%Introduction%...................................................................................................................................%16!