Introduction to the Special Issue on Scientific Balloon Capabilities and Instrumentation
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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. -
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. -
Airships Over Lincolnshire
Airships over Lincolnshire AIRSHIPS Over Lincolnshire explore • discover • experience explore Cranwell Aviation Heritage Museum 2 Airships over Lincolnshire INTRODUCTION This file contains material and images which are intended to complement the displays and presentations in Cranwell Aviation Heritage Museum’s exhibition areas. This file looks at the history of military and civilian balloons and airships, in Lincolnshire and elsewhere, and how those balloons developed from a smoke filled bag to the high-tech hybrid airship of today. This file could not have been created without the help and guidance of a number of organisations and subject matter experts. Three individuals undoubtedly deserve special mention: Mr Mike Credland and Mr Mike Hodgson who have both contributed information and images for you, the visitor to enjoy. Last, but certainly not least, is Mr Brian J. Turpin whose enduring support has added flesh to what were the bare bones of the story we are endeavouring to tell. These gentlemen and all those who have assisted with ‘Airships over Lincolnshire’ have the grateful thanks of the staff and volunteers of Cranwell Aviation Heritage Museum. Airships over Lincolnshire 3 CONTENTS Early History of Ballooning 4 Balloons – Early Military Usage 6 Airship Types 7 Cranwell’s Lighter than Air section 8 Cranwell’s Airships 11 Balloons and Airships at Cranwell 16 Airship Pioneer – CM Waterlow 27 Airship Crews 30 Attack from the Air 32 Zeppelin Raids on Lincolnshire 34 The Zeppelin Raid on Cleethorpes 35 Airships during the inter-war years -
The EBEX Balloon Borne Experiment-Optics, Receiver, and Polarimetry
The EBEX Balloon Borne Experiment - Optics, Receiver, and Polarimetry The EBEX Collaboration: Asad M. Aboobaker1, Peter Ade2, Derek Araujo3, Fran¸cois Aubin4, Carlo Baccigalupi5;6, Chaoyun Bao4, Daniel Chapman3, Joy Didier3, Matt Dobbs7;8, Christopher Geach4, Will Grainger9, Shaul Hanany4;∗, Kyle Helson10, Seth Hillbrand3, Johannes Hubmayr11, Andrew Jaffe12, Bradley Johnson3, Terry Jones4, Jeff Klein4, Andrei Korotkov10, Adrian Lee13, Lorne Levinson14, Michele Limon3, Kevin MacDermid7, Tomotake Matsumura4;15, Amber D. Miller3, Michael Milligan4, Kate Raach4, Britt Reichborn-Kjennerud3, Ilan Sagiv14, Giorgio Savini16, Locke Spencer2;17, Carole Tucker2, Gregory S. Tucker10, Benjamin Westbrook11, Karl Young4, Kyle Zilic4 ABSTRACT The E and B Experiment (EBEX) was a long-duration balloon-borne cosmic mi- crowave background polarimeter that flew over Antarctica in 2013. We describe the experiment's optical system, receiver, and polarimetric approach, and report on their in-flight performance. EBEX had three frequency bands centered on 150, 250, and 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109 2School of Physics and Astronomy, Cardiff University, Cardiff, CF24 3AA, United Kingdom 3Physics Department, Columbia University, New York, NY 10027 4University of Minnesota School of Physics and Astronomy, Minneapolis, MN 55455 5Astrophysics Sector, SISSA, Trieste, 34014, Italy 6INFN, Sezione di Trieste, Via Valerio 2, I-34127 Trieste, Italy 7McGill University, Montreal, Quebec, H3A 2T8, Canada 8Canadian Institute for -
Telescope Design Considerations
CMB S-4: Telescope Design Considerations September 12, 2016 T. Essinger-Hileman, N. Halverson, S. Hanany, M. D. Niemack, S. Padin, S. Parshley, C. Pryke, T. Suzuki, E. Switzer, K. Thompson, et al. Institutions DRAFT Contents 1 Introduction 1 1.1 Optics benchmarks . .2 2 Current CMB telescope designs and maturity 3 2.1 Current small aperture telescope designs . .4 2.2 Current large aperture telescope designs . .5 2.3 Concept for high throughput large aperture telescope design . .6 3 Telescope engineering to improve systematics 9 3.1 Monolithic mirrors . .9 3.2 Boresight rotation . 10 3.3 Shields and baffles . 10 4 Potential future studies and development areas 13 A Optics designs for current projects 16 A.1 Advanced ACTPol . 16 A.2 BICEP3 . 17 A.3 CLASS . 18 A.4 EBEX . 19 A.5 Keck/Spider . 20 A.6 Piper . 21 A.7 Simons Array . 22 A.8 SPT-3G . 23 B Projects using crossed-Dragone telescopes 24 B.1 ABS . 24 B.2 QUIET . 25 B.3 CCAT-prime . 26 DRAFT i 1 Introduction CHARGE: Summarize the current state of the technology and identify R&D efforts neces- sary to advance it for possible use in CMB-S4. CMB-S4 will likely require a scale-up in number of elements, frequency coverage, and bandwidth relative to current instruments. Because it is searching for lower magnitude signals, it will also require stronger control of systematic uncertainties. Current landscape • Existing CMB experiments have a range of telescope sizes (∼ 0:3 to 10 m) and styles (cold refractors and offset Gregory and crossed Dragone reflectors). -
INSTRONICS 12.Pdf
2011 INSTRONICS Nov www.measurers.yolasite.com YEAR: 2011 ISSUE:3 VOL:12 NOV CONTENTS 1. BASICS Convenor Terms & Definitions- - - - - - - - - - - - - -1 Prof.M.Muruganandam, HOD/EIE. 2.PERSONALITY Chief Editor Jacques Charles - - - - - - - - - - - - - - - - - 2 Prof.C.Venkatesh, 3. CIRCUIT IDEA Asst.Prof./EIE. Mini Tracker- - - - - - - - - - - - - - - - - - - 4 Student Editors 4. NEW PRODUCTS- - - - - - - - - - - - - - - - - - 5 Ms.A.Priyanga, Mr.N.Yuvaraj. 5. SENSOR Sub-Editors Wired Glove- - - - - - - - - - - - - - - - - - - -6 6.KNOW HOW?- - - - - - - - - - - - - - - - - - - - - 8 Mr.C.S.Muraleedharan, Ms.S.A.Diana Mary, 7.CROSS WORD - - - - - - - - - - - - - - - - - - - -10 Ms.J.Nivedhitha. 8. TECHNO FOCUS- - - - - - - - - - - - - - - - - -11 Graphics & 9.DEEP FOCUS - - - - - - - - - - - - - - - - - - - - -12 Designing 10.COMPANY PROFILE - - - - - - - - - - - - - -14 Mr.C.Vijay. Mr.S.Vignesh Kumar. EDITORS: The Editors and Publishers of this magazine do their best to verify the information published, but do not take responsibili ty for the absolute accuracy of the information. Your commends are welcomed and you can send your and newsletters through email to the mail-ID [email protected] 2011 INSTRONICS Nov www.measurers.yolasite.com “Our life is what our thought makes of it Great thought comes from the heart” We thank Our Beloved Principal Dr.M.Madheswaran For his valuable guidance and encouragement in bringing up this magazine “INSTRONICS” successfully. - EIE ASSOCIATION 2011 INSTRONICS Nov www.measurers.yolasite.com TERMS &DEFINITIONS: INTERCHANGEABILITY ERROR: ICON: A measurement error that can occur if two or more probes are used to A graphic functional symbol make the same measurement. It is display. Graphic representation of a caused by a slight variation in functions to be performed by the characteristics of different probes. computer. INTERPRETER: IPTS-68: A system program that converts International Practical and executes each instruction of a Temperature Scale of 1968. -
Philosophy and Ethics of Aerospace Engineering
UNIVERSIDADE DA BEIRA INTERIOR Engenharia Philosophy and Ethics of Aerospace Engineering António Luis Martins Mendes Tese para obtenção do Grau de Doutor em Aeronautical Engineering (3º ciclo de estudos) Orientador: Prof. Doutor Jorge Manuel Martins Barata Covilhã, Dezembro de 2016 ii Dedicatória Gostaria de dedicar esta tese a minha Avó Rosa e aos meus Pais por acreditarem em mim e pelo apoio estes anos todos desde a primeira classe até agora. Obrigado por tudo! ii Acknowledgments My deepest gratitude to Professor Jorge Barata for the continuous support throughout college since I was invited to become a member of his Research and Development team until the present days. His patience, motivation, knowledge, individual and family values have been a mark on my own professional and personal life. His teaching and guidance allowed me to succeed in life to extents I never thought it could have happened. I could have not imagined having a better advisor and mentor for my PhD study. Beside my mentor, I would like to say thank you to Professor André Silva and my colleague and friend Fernando Neves for all the good and bad moments throughout college and life events. I would like to recognize some other professors that made a difference in my studies and career paths – Professor Koumana Bousson, Professor Jorge Silva, Professor Pedro Gamboa, Professor Miguel Silvestre, Professor Aomar Abdesselam, Professor Sarychev and my colleague Maria Baltazar. Last but not least, I would like to thank my family: my wife Kristie, my kids (AJ and Bela) and my neighbor Fred LaCount for the spiritual support throughout this study and phase of my life. -
Task Force on Cosmic Microwave Background Research
Task Force On Cosmic Microwave Background Research Final Report July 11, 2005 -1- MEMBERS OF THE CMB TASK FORCE James Bock Caltech/JPL Sarah Church Stanford University Mark Devlin University of Pennsylvania Gary Hinshaw NASA/GSFC Andrew Lange Caltech Adrian Lee University of California at Berkeley/LBNL Lyman Page Princeton University Bruce Partridge Haverford College John Ruhl Case Western Reserve University Max Tegmark Massachusetts Institute of Technology Peter Timbie University of Wisconsin Rainer Weiss (chair) Massachusetts Institute of Technology Bruce Winstein University of Chicago Matias Zaldarriaga Harvard University AGENCY OBSERVERS Beverly Berger National Science Foundation Vladimir Papitashvili National Science Foundation Michael Salamon NASA/HDQTS Nigel Sharp National Science Foundation Kathy Turner US Department of Energy -2- Table of Contents Executive Summary ...........................................................................................4 1 Outline of Report ................................................................................................8 sidebar “Some History and Perspective..............................................................10 2 Cosmology and Inflation ..................................................................................11 sidebar “Direct Measurement of Primeval Gravitational Waves” ....................18 3 Theory of CMB Polarization and Gravitational Waves ....................................19 4 Astrophysical Disturbances in Measuring the CMB Polarization: Gravitational -
NASA Stratospheric Balloons Science at the Edge of Space
National Aeronautics and Space Administration NASA Stratospheric Balloons Science at the edge of Space REPORT OF THE SCIENTIFIC BALLOONING ASSESSMENT GROUP The Scientific Ballooning Assessment Group Martin Israel Washington University in St. Louis, Chair Steven Boggs University of California, Berkeley Michael Cherry Louisiana State University Mark Devlin University of Pennsylvania Jonathan Grindlay Harvard University Bruce Lites National Center for Astrophysics Research James Margitan Jet Propulsion Laboratory Jonathan Ormes University of Denver Carol Raymond Jet Propulsion Laboratory Eun-Suk Seo University of Maryland, College Park Eliot Young Southwest Research Institute, Boulder Vernon Jones NASA Headquarters, Executive Secretary Ex Officio: Vladimir Papitashvili NSF, Office of Polar Programs David Pierce NASA, GSFC/WFF Balloon Program Office, Chief Debora Fairbrother NASA, GSFC/WFF Balloon Program Office, Technologist Jack Tueller NASA GSFC, Balloon Program Project Scientist John Mitchell NASA GSFC, Balloon Program Deputy Project Scientist Cover Photo: The Balloon-borne Experiment with Superconducting Spectrometer, BESS Polar II at Williams Field, McMurdo, Antarctica. Facing Page Photo: The International ocusingF Optics Collaboration for micro-Crab Sensitivity (InFOCmS), a hard x-ray telescope with CdZnTe pixel detector as a focal plane imager. NASA Stratospheric Balloons Science at the edge of Space Report of the Scientific Ballooning Assessment Group January 2010 Table of Contents Executive Summary 3 Scientific Ballooning has Made Important Contributions to NASA’s Program 9 Balloon-borne Instruments Will Continue to Contribute to NASA’s Objectives 15 Many Scientists with Leading Roles in NASA were Trained in the Balloon Program 35 The Balloon Program has Substantial Capability for Achieving Quality Science 37 Findings 41 Acronyms 46 References 49 The Cosmic Ray Energetics And Mass instrument (CREAM) hangs on the launch vehicle at Williams Field near McMurdo base Antarctica. -
The Rise and Fall of Lighter-Than-Air Aircraft, 1783 – 1937 Marc Mercado Southern Illinois University Carbondale
Legacy Volume 17 | Issue 1 Article 7 2017 The Rise and Fall of Lighter-Than-Air Aircraft, 1783 – 1937 Marc Mercado Southern Illinois University Carbondale Follow this and additional works at: https://opensiuc.lib.siu.edu/legacy Recommended Citation Mercado, Marc (2017) "The Rise and Fall of Lighter-Than-Air Aircraft, 1783 – 1937," Legacy: Vol. 17 : Iss. 1 , Article 7. Available at: https://opensiuc.lib.siu.edu/legacy/vol17/iss1/7 This Article is brought to you for free and open access by OpenSIUC. It has been accepted for inclusion in Legacy by an authorized administrator of OpenSIUC. For more information, please contact [email protected]. 1 Marc Mercado The Rise and Fall of Lighter-Than-Air Aircraft, 1783 – 1937 When one thinks about military aircraft, they rarely think about anything other than jets or helicopters, both of which are heavier-than-air aircraft. From the perspective of the twenty- first century, it is almost humorous to imagine a fragile, slow paced, and highly flammable gas- filled balloon gliding over a battlefield and a hailstorm of bullets. However, hot air balloons and zeppelins, which are both lighter-than-air aircraft, saw a great deal of military use until the end of the First World War. It is perhaps even stranger to think that experts considered lighter-than-air aircraft, which in retrospect seem little more than flying fire hazards, the safest and most effective form of military and commercial air travel. Though lighter-than-air aircraft have existed over twice as long as their currently more widely used heavier-than-air counterparts, due to a perceived lack of usefulness and safety, they saw a sharp decline in both military and commercial use in the early twentieth century. -
A Balloon-Borne Cosmic Microwave Background Anisotropy Probe
The E and B EXperiment: A balloon-borne cosmic microwave background anisotropy probe Seth Hillbrand Submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in the Graduate School of Arts and Sciences COLUMBIA UNIVERSITY 2014 c 2014 Seth Hillbrand All Rights Reserved ABSTRACT The E and B EXperiment: A balloon-borne cosmic microwave background anisotropy probe Seth Hillbrand The E and B Experiment (EBEX), is a balloon-borne sub-orbital cosmic microwave background polarimeter, designed to measure polarization levels in the microwave spectrum. EBEX recently completed an 11-day Antarctic long duration balloon (LDB) science flight in January, 2013. 1000 transition edge sensor bolometric detectors in ∼ three frequency bands centered at 150, 250 and 410 GHz sampled a large segment of the southern sky. Over 1.5TB of data were collected during the LDB flight. In this thesis, we describe the design and performance of the EBEX software components monitoring and controlling the system during the flight, including automation, telemetry, data storage and readout array management. We also describe the design and development of a novel attitude reconstruction system for a balloon-borne pointed observation platform based on a daytime star camera and 3-axis gyroscopes. The data gathered during the LDB flight are analyzed and the results presented showing attitude reconstruction error at less than 2000 RMS for an 80 second interval. Table of Contents 1 Introduction1 2 EBEX Science4 2.1 Concordance Cosmology.........................4 2.1.1 Expanding Universe.......................6 2.1.2 Flat Universe...........................9 2.1.3 Hot, Dense Early Universe....................9 2.1.4 Dark Matter Universe..................... -
Bruce Comstock
FÉDÉRATION AÉRONAUTIQUE INTERNATIONALE Ballooning Commission Hall of Fame ROBERT BROTHERS, FRANCE Inducted 2000 Photo and plaque published with permission of the Anderson/Abruzzo International Balloon Museum in Albuquerque, New Mexico, USA 1 Anne-Jean Robert, (aîné, the elder). 1758-1820. Marie-Noël Robert, (cadet, the younger). 1760-1820. The Robert brothers were skilled mechanical constructors. They helped professor Jacques Alexandre César Charles build the first usable hydrogen balloons. Charles knew about the work of Cavendish, Black and Cavallo, and realised that hydrogen would make a suitable lifting agent. The problem was to find a airtight and light gas container. The brothers had found a method to dissolve rubber in turpentine. This mixture was used to varnish the silk used to construct the envelopes of the balloons (The silk was red and white but when rubberised, the white parts changed to light yellow). August 27, 1783 Professor Charles and the Robert brothers publicly demonstrated a 35 m3 hydrogen balloon - a rubberised silk sphere. This was the first free flight by a gas balloon. The balloon was launched from Champ de Mars, Paris. It quickly rose to high altitude and landed in Gonesse (15 km NE Paris) where scared villagers attacked the "monster from space". December 1st, 1783. The younger brother, Marie-Noël Robert, accompanied professor Charles on the first human flight in a gas balloon. The "charlière" contained 380 m3 hydrogen and was launched from "Le jardin des Tuileries" in Paris at 13.45. They landed in Nesle-La-Vallée after a 2 hour 5 minute flight covering 36 km. July 15th, 1784.