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A Weather Vane Antenna for 2 Meters VHF Incognito! Here’S a 2 Meter Antenna Figure 1—The Completed Weather Vane Your Neighbors Won’T Recognize
John Portune, W6NBC, and Fred Adams, WD6ACJ A Weather Vane Antenna for 2 Meters VHF incognito! Here’s a 2 meter antenna Figure 1—The completed weather vane your neighbors won’t recognize. antenna. Can you find the loop? eeping a homeowners’ association happy isn’t easy. criminate than a dipole or J-pole. [While horizontal loops do bet- Many hams burdened with CC&Rs often live with ter in noisy situations because that local noise tends to be mainly Kbadly compromised antennas. Why not combine a com- E-field oriented, the perceived SNR improvement of a narrow- pact magnetic loop with a functional weather vane and put band antenna is principally due to the reduction in out-of-band high-performance right out in full view? A neighbor even asked signals that cause IMD, rather than any reduction of the receiver me where I got mine, so she could get one, too. noise floor.—Ed.] They also tend to work better close to the ground Compact loops, often called magnetic loops, have been or near other objects. around for years. They’re tiny open-ended ring radiators, al- 1 ways less than roughly /10th wavelength in diameter. Recently Construction we’ve seen them mostly on HF where their small size is of All materials (Figures 3A and 3B) are common hardware store great appeal. But they work very well on other bands too; here items. I recommend a tubing cutter for cutting the pipe, copper on 2 meters. Remarkably, this VHF ver- and PVC. Also, a different brand of copper sion achieves an efficiency of 93%, yet fittings may require slight adjustments to radiates as if it were a full-sized dipole the cutting dimensions shown. -
High Frequency Communications – an Introductory Overview
High Frequency Communications – An Introductory Overview - Who, What, and Why? 13 August, 2012 Abstract: Over the past 60+ years the use and interest in the High Frequency (HF -> covers 1.8 – 30 MHz) band as a means to provide reliable global communications has come and gone based on the wide availability of the Internet, SATCOM communications, as well as various physical factors that impact HF propagation. As such, many people have forgotten that the HF band can be used to support point to point or even networked connectivity over 10’s to 1000’s of miles using a minimal set of infrastructure. This presentation provides a brief overview of HF, HF Communications, introduces its primary capabilities and potential applications, discusses tools which can be used to predict HF system performance, discusses key challenges when implementing HF systems, introduces Automatic Link Establishment (ALE) as a means of automating many HF systems, and lastly, where HF standards and capabilities are headed. Course Level: Entry Level with some medium complexity topics Agenda • HF Communications – Quick Summary • How does HF Propagation work? • HF - Who uses it? • HF Comms Standards – ALE and Others • HF Equipment - Who Makes it? • HF Comms System Design Considerations – General HF Radio System Block Diagram – HF Noise and Link Budgets – HF Propagation Prediction Tools – HF Antennas • Communications and Other Problems with HF Solutions • Summary and Conclusion • I‟d like to learn more = “Critical Point” 15-Aug-12 I Love HF, just about On the other hand… anybody can operate it! ? ? ? ? 15-Aug-12 HF Communications – Quick pretest • How does HF Communications work? a. -
Rcosmo: R Package for Analysis of Spherical, Healpix and Cosmological Data Arxiv:1907.05648V1 [Stat.CO] 12 Jul 2019
CONTRIBUTED RESEARCH ARTICLE 1 rcosmo: R Package for Analysis of Spherical, HEALPix and Cosmological Data Daniel Fryer, Ming Li, Andriy Olenko Abstract The analysis of spatial observations on a sphere is important in areas such as geosciences, physics and embryo research, just to name a few. The purpose of the package rcosmo is to conduct efficient information processing, visualisation, manipulation and spatial statistical analysis of Cosmic Microwave Background (CMB) radiation and other spherical data. The package was developed for spherical data stored in the Hierarchical Equal Area isoLatitude Pixelation (Healpix) representation. rcosmo has more than 100 different functions. Most of them initially were developed for CMB, but also can be used for other spherical data as rcosmo contains tools for transforming spherical data in cartesian and geographic coordinates into the HEALPix representation. We give a general description of the package and illustrate some important functionalities and benchmarks. Introduction Directional statistics deals with data observed at a set of spatial directions, which are usually positioned on the surface of the unit sphere or star-shaped random particles. Spherical methods are important research tools in geospatial, biological, palaeomagnetic and astrostatistical analysis, just to name a few. The books (Fisher et al., 1987; Mardia and Jupp, 2009) provide comprehensive overviews of classical practical spherical statistical methods. Various stochastic and statistical inference modelling issues are covered in (Yadrenko, 1983; Marinucci and Peccati, 2011). The CRAN Task View Spatial shows several packages for Earth-referenced data mapping and analysis. All currently available R packages for spherical data can be classified in three broad groups. The first group provides various functions for working with geographic and spherical coordinate systems and their visualizations. -
From Stargazing to Space Travel Our Brief History Into Space
From Stargazing to Space Travel Our brief history into space Science in the News Elaine Garcia Angela She November 4th, 2015 Why do we care? Gives us perspective • What did our forefathers think of the Heavens? • Why did they think that? • How did theories change throughout time? Gives us purpose • Mystery drives inquiry and discovery. Important Lessons were Learned and will Continue to be Discovered! Keywords Astrologyl – The study and interpretation of the movements and positions of celestial bodies in relation to Earth and Earthly affairs. Astronomy – The study of physical objects in space: gas, dust, stars, planets, moons, comets, and other non-Earthly mass and phenomena. • Astrophysics – The study of the physical nature and energy of cosmic mass. • Cosmology – A branch of study that theorizes about the origin and nature of the universe. Outline 1. Star Gazing • Theories about why, where, and how 2. Star Studying • Technology to study the unknown 3. Star Reaching • Demo on space exploration Outline 1. Star Gazing • Theories about why, where, and how 2. Star Studying • Technology to study the unknown 3. Star Reaching • Demo on space exploration What are stars’ purpose? Are they the actions, moods, or warnings of celestial beings? Star Worship Is their existence independent and separated from Earth’s existence and purpose? Star Navigation and Measurement Millennia of Lessons 570 BC 384 BC 276 BC 1600 O 1750+ BC 427 BC 310 BC 90 1700 Millennia of Lessons The earliest records of astronomical observations and mathematics. 1750+ BC Greek Rule Zeus King of Gods Hera Queen of Gods Poseidon God of the Sea Hades God of the Underworld Helios The Sun God Ares God of War Aphrodite Goddess of Love Eros God of Love Athena Goddess of Wisdom Hephaestus God of Fire/Forge Wikicommons.com What season is it? Zodiac surrounds the Earth, noting the Seasons Wikicommons.com Millennia of Lessons The earliest records of astronomical observations and mathematics. -
50 Years of the Lovell Telescope Transcript
50 years of the Lovell telescope Transcript Date: Wednesday, 5 December 2007 - 12:00AM 50 YEARS OF THE LOVELL TELESCOPE Professor Ian Morison The Early days at Jodrell Bank In late 1945 Dr Bernard Lovell (as he then was) returned to Manchester University after working on the development of radar during the war years. His aim was to continue his researches into cosmic rays - highly energetic particles that enter the Earth's atmosphere from outer space. He had the idea that sporadic echoes sometimes received by military radars might be the result of cosmic rays entering the atmosphere and thus radar observations might provide a new way to continue his researches. Radar observations were not practical in the centre of Manchester so he took his ex-army radar system out to the University's Botanical Grounds at Jodrell Bank, some 20 miles to the south. By the middle of December 1945, the system was operating and his team was soon able to prove that the echoes were coming not from cosmic rays but from ionized meteor trails left behind when small particles, released from comets, are burnt up in the upper atmosphere of the Earth. Radar Antenna in the Botany Grounds. The Jodrell Bank Experimental Station. The observations continued and, to house the expanding staff and equipment, the Jodrell Bank Experimental Station was built in the field next to the Botanic Grounds. Lovell realised that a much more sensitive radio telescope would be required to detect cosmic rays and so, in 1947, the researchers built a large parabolic reflector, 66-m across, pointing upwards to observe the sky passing overhead. -
The Lovell Telescope … Through Its Surfaces Simon Garrington, JBO/University of Manchester
The Lovell Telescope … through its surfaces Simon Garrington, JBO/University of Manchester • Original design & redesign: 1950-1957 • Radical modification & new surface: 1971 • Replacement of surface: 2001 • Replacement of original Picture A. Holloway surface: 2018 • Other consequences: foundations O1 Original MkI proposal and changes • Concept & proposals: 1950-1 • Lovell-Husband Sep 1949 • Radio Astronomy Cttee 1950 • rail track; towers, cradle, 4-inch mesh • 2-inch mesh/5-in profile by 20 Mar 1951 submission • Design changes • 21cm line discovered (Ewen 25 Mar 1951) • Inner 100’ mesh 1x2-in ‘at no cost’ ? Sep 1952 • Interest from Air Ministry: 10cm radar • March 1954: 3/4-in mesh -> stronger cradle … but Air Ministry step back O2 Original MkI proposal and changes • Concept & proposals: 1950-1 • Lovell-Husband Sep 1949 • Radio Astronomy Cttee 1950 • rail track; towers, cradle, 4-inch mesh • 2-inch mesh/5-in profile by 20 Mar 1951 submission • Design changes • 21cm line discovered (Ewen 25 Mar 1951) • Inner 100’ mesh 1x2-in ‘at no cost’ ? Sep 1952 • Interest from Air Ministry: 10cm radar • March 1954: 3/4-in mesh -> stronger cradle … but Air Ministry step back O3 Original MkI proposal and changes • Concept & proposals: 1950-1 • Lovell-Husband Sep 1949 • Radio Astronomy Cttee 1950 • rail track; towers, cradle, 4-inch mesh • 2-inch mesh/5-in profile by 20 Mar 1951 submission • Design changes • 21cm line discovered (Ewen 25 Mar 1951) • Inner 100’ mesh 1x2-in ‘at no cost’ ? Sep 1952 • Interest from Air Ministry: 10cm radar • March 1954: 3/4-in -
Rhodri Evans
Rhodri Evans The Cosmic Microwave Background How It Changed Our Understanding of the Universe Astronomers’ Universe More information about this series at http://www.springer.com/series/6960 Rhodri Evans The Cosmic Microwave Background How It Changed Our Understanding of the Universe 123 Rhodri Evans School of Physics & Astronomy Cardiff University Cardiff United Kingdom ISSN 1614-659X ISSN 2197-6651 (electronic) ISBN 978-3-319-09927-9 ISBN 978-3-319-09928-6 (eBook) DOI 10.1007/978-3-319-09928-6 Springer Cham Heidelberg New York Dordrecht London Library of Congress Control Number: : 2014957530 © Springer International Publishing Switzerland 2015 This work is subject to copyright. All rights are reserved by the Publisher, whether the whole or part of the material is concerned, specifically the rights of translation, reprinting, reuse of illustrations, recitation, broadcasting, reproduction on microfilms or in any other physical way, and transmission or information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed. Exempted from this legal reservation are brief excerpts in connection with reviews or scholarly analysis or material supplied specifically for the purpose of being entered and executed on a computer system, for exclusive use by the purchaser of the work. Duplication of this publication or parts thereof is permitted only under the provisions of the Copyright Law of the Publisher’s location, in its current version, and permission for use must always be obtained from Springer. Permissions for use may be obtained through RightsLink at the Copyright Clearance Center. Violations are liable to prosecution under the respective Copyright Law. -
Adventures in Radio Astronomy Instrumentation and Signal Processing
Adventures in Radio Astronomy Instrumentation and Signal Processing by Peter Leonard McMahon Submitted to the Department of Electrical Engineering in partial fulfillment of the requirements for the degree of Master of Science in Electrical Engineering at the University of Cape Town July 2008 Supervisor: Professor Michael Inggs Co-supervisors: Dr Dan Werthimer, CASPER1, University of California, Berkeley Dr Alan Langman, Karoo Array Telescope arXiv:1109.0416v1 [astro-ph.IM] 2 Sep 2011 1Center for Astronomy Signal Processing and Electronics Research Abstract This thesis describes the design and implementation of several instruments for digi- tizing and processing analogue astronomical signals collected using radio telescopes. Modern radio telescopes have significant digital signal processing demands that are typically best met using custom processing engines implemented in Field Pro- grammable Gate Arrays. These demands essentially stem from the ever-larger ana- logue bandwidths that astronomers wish to observe, resulting in large data volumes that need to be processed in real time. We focused on the development of spectrometers for enabling improved pulsar2 sci- ence on the Allen Telescope Array, the Hartebeesthoek Radio Observatory telescope, the Nan¸cay Radio Telescope, and the Parkes Radio Telescope. We also present work that we conducted on the development of real-time pulsar timing instrumentation. All the work described in this thesis was carried out using generic astronomy pro- cessing tools and hardware developed by the Center for Astronomy Signal Processing and Electronics Research (CASPER) at the University of California, Berkeley. We successfully deployed to several telescopes instruments that were built solely with CASPER technology, which has helped to validate the approach to developing radio astronomy instruments that CASPER advocates. -
High Resolution Radio Astronomy Using Very Long Baseline Interferometry
IOP PUBLISHING REPORTS ON PROGRESS IN PHYSICS Rep. Prog. Phys. 71 (2008) 066901 (32pp) doi:10.1088/0034-4885/71/6/066901 High resolution radio astronomy using very long baseline interferometry Enno Middelberg1 and Uwe Bach2 1 Astronomisches Institut, Universitat¨ Bochum, 44801 Bochum, Germany 2 Max-Planck-Institut fur¨ Radioastronomie, Auf dem Hugel¨ 69, 53121 Bonn, Germany E-mail: [email protected] and [email protected] Received 3 December 2007, in final form 11 March 2008 Published 2 May 2008 Online at stacks.iop.org/RoPP/71/066901 Abstract Very long baseline interferometry, or VLBI, is the observing technique yielding the highest-resolution images today. Whilst a traditionally large fraction of VLBI observations is concentrating on active galactic nuclei, the number of observations concerned with other astronomical objects such as stars and masers, and with astrometric applications, is significant. In the last decade, much progress has been made in all of these fields. We give a brief introduction to the technique of radio interferometry, focusing on the particularities of VLBI observations, and review recent results which would not have been possible without VLBI observations. This article was invited by Professor J Silk. Contents 1. Introduction 1 2.9. The future of VLBI: eVLBI, VLBI in space and 2. The theory of interferometry and aperture the SKA 10 synthesis 2 2.10. VLBI arrays around the world and their 2.1. Fundamentals 2 capabilities 10 2.2. Sources of error in VLBI observations 7 3. Astrophysical applications 11 2.3. The problem of phase calibration: 3.1. Active galactic nuclei and their jets 12 self-calibration 7 2.4. -
2016 in the United States Wikipedia 2016 in the United States from Wikipedia, the Free Encyclopedia
4/30/2017 2016 in the United States Wikipedia 2016 in the United States From Wikipedia, the free encyclopedia Events in the year 2016 in the United States. Contents 1 Incumbents 1.1 Federal government 1.2 Governors 1.3 Lieutenant governors 2 Events 2.1 January 2.2 February 2.3 March 2.4 April 2.5 May 2.6 June 2.7 July 2.8 August 2.9 September 2.10 October 2.11 November 2.12 December 3 Deaths 3.1 January 3.2 February 3.3 March 3.4 April 3.5 May 3.6 June 3.7 July 3.8 August 3.9 September 3.10 October 3.11 November 3.12 December 4 See also 5 References Incumbents Federal government President: Barack Obama (DIllinois) Vice President: Joe Biden (DDelaware) Chief Justice: John Roberts (New York) https://en.wikipedia.org/wiki/2016_in_the_United_States 1/60 4/30/2017 2016 in the United States Wikipedia Speaker of the House of Representatives: Paul Ryan (RWisconsin) Senate Majority Leader: Mitch McConnell (RKentucky) Congress: 114th https://en.wikipedia.org/wiki/2016_in_the_United_States 2/60 4/30/2017 2016 in the United States Wikipedia Governors and Lieutenant governors Governors Governor of Alabama: Robert J. Bentley Governor of Mississippi: Phil Bryant (Republican) (Republican) Governor of Alaska: Bill Walker Governor of Missouri: Jay Nixon (Independent) (Democratic) Governor of Arizona: Doug Ducey Governor of Montana: Steve Bullock (Republican) (Democratic) Governor of Arkansas: Asa Hutchinson Governor of Nebraska: Pete Ricketts (Republican) (Republican) Governor of California: Jerry Brown Governor of Nevada: Brian Sandoval (Democratic) -
Measuring Inflation with CLASS
Measuring Inflation with CLASS by Dominik Gothe A dissertation submitted to Johns Hopkins University in conformity with the requirements for the degree of Doctor of Philosophy. July 2015 Baltimore, Maryland c Dominik Gothe All rights reserved Abstract Using the Cosmology Large Angular Scale Surveyor (CLASS), we will measure the po- larization of the Cosmic Microwave Background (CMB) to constrain inflationary theory. The gravitational waves generated during the inflationary epoch imprinted specific polar- ization patterns – quantifiable by tensor-to-scalar ratio r – onto the CMB, which CLASS is designed to detect. Furthermore, we will be able to make assertions about the energy scale during inflation by discovering the features of the polarization power spectrum, providing a probe into physics of energy scales not conceivable in particle-accelerator physics. CLASS is a unique ground based experiment with extensive consideration given to mitigating sys- tematic uncertainties. A brief introduction into inflationary cosmology and review of current scientific results will be presented in the light of the upcoming measurements with the newly built CLASS de- tector. I will detail some of my technical contribution to the construction of this telescope. I have conducted my research under the advise of Prof. Bennett. Additionally the thesis was reviewed by Prof. Marriage, Prof. Kamionkowski, Prof. Chuss, and Prof. Strobel. ii Acknowledgments I would like to thank my wife, friends, members of the Johns Hopkins community, my mentors, teachers, supervisors, and dissertation committee. The CLASS project receives support from the National Science Foundation Division of Astronomical Sciences under Grant Numbers 0959349 and 1429236. iii Contents I Physics of the Origin of the Universe 1 1 Introduction to the Big Bang Framework . -
Monitoring Times 2000 INDEX
Monitoring Times 1994 INDEX FEATURES: Air Show: Triumph to Tragedy Season Aug JUNE Duopolies and DXing Broadcast: Atlantic City Aero Monitoring May JULY TROPO Brings in TV & FM A Journey to Morocco May Dayton's Aviation Extravaganza DX Bolivia: Radio Under the Gun June June AUG Low Power TV Stations Broadcasting Battlefield, Colombia Flight Test Communications Jan SEP WOW, Omaha Dec Gathering Comm Intelligence OCT Winterizing Chile: Land of Crazy Geography June NOV Notch filters for good DX April Military Low Band Sep DEC Shopping for DX Receiver Deutsche Welle Aug Monitoring Space Shuttle Comms European DX Council Meeting Mar ANTENNA TOPICS Aug Monitoring the Prez July JAN The Earth’s Effects on First Year Radio Listener May Radio Shows its True Colors Aug Antenna Performance Flavoradio - good emergency radio Nov Scanning the Big Railroads April FEB The Half-Rhombic FM SubCarriers Sep Scanning Garden State Pkwy,NJ MAR Radio Noise—Debunking KNLS Celebrates 10 Years Dec Feb AntennaResonance and Making No Satellite or Cable Needed July Scanner Strategies Feb the Real McCoy Radio Canada International April Scanner Tips & Techniques Dec APRIL More Effects of the Earth on Radio Democracy Sep Spy Catchers: The FBI Jan Antenna Radio France Int'l/ALLISS Ant Topgun - Navy's Fighter School Performance Nov Mar MAY The T2FD Antenna Radio Gambia May Tuning In to a US Customs Chase JUNE Antenna Baluns Radio Nacional do Brasil Feb Nov JULY The VHF/UHF Beam Radio UNTAC - Cambodia Oct Video Scanning Aug Traveler's Beam Restructuring the VOA Sep Waiting