NATIONAL ACADEMIES of SCIENCES and ENGINEERING NATIONAL RESEARCH COUNCIL of the UNITED STATES of AMERICA

Total Page:16

File Type:pdf, Size:1020Kb

NATIONAL ACADEMIES of SCIENCES and ENGINEERING NATIONAL RESEARCH COUNCIL of the UNITED STATES of AMERICA NATIONAL ACADEMIES OF SCIENCES AND ENGINEERING NATIONAL RESEARCH COUNCIL of the UNITED STATES OF AMERICA UNITED STATES NATIONAL COMMITTEE International Union of Radio Science National Radio Science Meeting 4-8 January 2000 Sponsored by USNC/URSI University of Colorado Boulder, Colorado U.S.A. United States National Committee INTERNATIONAL UNION OF RADIO SCIENCE PROGRAM AND ABSTRACTS National Radio Science Meeting 4-8 January 2000 Sponsored by USNC/URSI NOTE: Programs and Abstracts of the USNC/URSI Meetings are available from: USNC/URSI National Academy of Sciences 2101 Constitution Avenue, N.W. Washington, DC 20418 at $5 for 1983-1999 meetings. The full papers are not published in any collected format; requests for them should be addressed to the authors who may have them published on their own initiative. Please note that these meetings are national. They are not organized by the International Union, nor are the programs available from the International Secretariat. ii MEMBERSHIP United States National Committee INTERNATIONAL UNION OF RADIO SCIENCE Chair: Gary Brown* Secretary & Chair-Elect: Umran S. !nan* Immediate Past Chair: Susan K. Avery* Members Representing Societies, Groups, and Institutes: American Astronomical Society Thomas G. Phillips American Geophysical Union Donald T. Farley American Meteorological Society vacant IEEE Antennas and Propagation Society Linda P.B. Katehi IEEE Geosciences and Remote Sensing Society Roger Lang IEEE Microwave Theory and Techniques Society Arthur A. Oliner Members-at-Large: Amalia Barrios J. Richard Fisher Melinda Picket-May Ronald Pogorzelski W. Ross Stone Richard Ziolkowski Chairs of the USNC/URSI Commissions: Commission A Moto Kanda Commission B Piergiorgio L. E. Uslenghi Commission C Alfred 0. Hero Commission D Alan Mickelson Commission E Jon Schoenberg Commission F Edgeworth R. Westwater Commission G John C. Foster Commission H Min-Chang Lee Commission J Peter Napier Commission K Frank S. Barnes Officers, Chairs and Vice Chairs of Commissions ofURSI residing in the United States: Past President Thomas B. A. Senior Chair, Commission E Robert L. Gardner Chair, Commission J Jackie N. Hewitt Vice Chair, Commission A Quirino Balzano Vice Chair, Commission H Umran S. Inan * Member ofUSNC/URSI Executive Committee iii DESCRIPTION OF THE INTERNATIONAL UNION OF RADIO SCIENCE The International Union of Radio Science is one of the world scientific unions organized under the International Council of Scientific Unions ([CSU). It is commonly designated as URS! (from its French name, Union Radio Scientifique Internationale). Its aims are (1) to promote the scientific study of radio communications, (2) to aid and organize radio research requiring cooperation on an international scale and to encourage the discussion and publication of the results, (3) to facilitate agreement upon common methods of measurement and the standardization of measuring instruments, and ( 4) to stimulate and to coordinate studies of the scientific aspects of telecommunications using electromagnetic waves, guided and unguided. The International Union itself is an organizational framework to aid in promoting these objectives. The actual technical work is largely done by the National Committee in the various countries. The new officers of the International Union are: President: Hiroshi Matsumoto (Japan) Past President: Thomas B. A. Senior (U.S.A.) Vice Presidents: Kristian Schlegel (Germany) Joseph Shapira (Israel) Andrzej W. Wernik (Poland Paul H. Wittke (Canada) Secretary-General: Paul Lagasse (Belgium) Assistant Secretary-General: Peter Van Daele Administrative Secretary: Inge Heleu The Secretary-General's office and the headquarters of the organi­ zation are located at Avenue Albert Lancaster, 32, B-1180 Brussels, Belgium. The Union is supported by contributions (dues) from 38 member countries. Additional funds for symposia and other scientific activities of the Union are provided by !CSU from contributions received for this purpose from UNESCO. The international Union, as of the XXVth General Assembly held in Kyoto, Japan, August 13-September 2, 1999, has ten bodies called Commissions for centralizing studies in the principal technical fields. Every three years the International Union holds a meeting called the General Assembly. The next is the XXV!th, to be held in August, 2002, in Maastricht, the Netherlands. The Secretariat prepares and distributes the Proceedings of the General Assemblies. The International Union V arranges international symposia on specific subjects pertaining to the work of one or several Commissions and also cooperates with other Unions in international symposia on subjects of joint interest. Radio is unique among the fields of scientific work in having a specific adaptability to large-scale international research programs, since many of the phenomena that must be studied are worldwide in extent and yet are in a measure subject to control by experimenters. Exploration of space and the extension of scientific observations to the space environment are dependent on radio for their research. One branch, radio astronomy, involves cosmic phenomena. URS! thus has a distinct field of usefulness in furnishing a meeting ground for the numerous workers in the manifold aspects of radio research; its meetings and committee activities furnish valuable means of promoting research through exchange of ideas. Steering Committee: D. Cook P. L. Jensen D. Thorsen R. Frehlich J. McKie Technical Program Committee: G.S. Brown, Chairperson S.K. Avery U. !nan M. Picket-May D. Wilton E Barnes M. Kanda L. Scharf R. Frehlich M.-C. Lee J. Schoenberg A. Gasiewski P. Napier D. Thorsen vi Wednesday Morning, January 5, 2000 Session Al, 08:55 AM, Wed., Room 151 METROLOGY FOR DETECTION OF BURIED OBJECTS Chairpersons: LS. Riggs, Auburn Univ ([email protected]) J. Harvey, Army Research Office ([email protected]) Al-1 UXOCOE MASTER PLAN FOR QUANTITATNE TESTING OF UXO 09:00 SENSOR TECHNOLOGIES Richard Weaver, Director Joint Unexploded Ordnance Coordinating Office Attn: AMSEL-RD-UXO-CO 10221 Burbeck Road Ft. Belvoir, VA 22060-5806 Denis M. Reidy E-OIR Measurements, Inc. P.O. Box 1240 Spotsylvania, VA 22553-1240 Fairly comparing the detection and discrimination performance of sensors or systems is always difficult. A useful comparison is nearly impossible in uncontrolled test situations. The Unexploded Ordnance Center of Excellence (UXOCOE) proposes measuring performance using a set of standard test locations, targets, and protocols that are administered by an impartial entity. This paper briefly outlines a master plan to establish standard test sites, protocols, and procedures for Unexploded Ordnance (UXO) sensors. Since the 1990's, significant investments by both the government and private industry have produced an exciting array of promising developments in sensors for detection of buried munitions, both ordnance and mines. Technologies such as ground penetrating radar (GPR), magnetometry, electro-magnetic induction (EMI) and synthetic aperture radar (SAR) are just a few examples that form the basis for many UXO detection sensors under development. Within each of these technology categories of UXO sensors, there are a number of different technical approaches being sold as the "best" way to exploit the respective technology. In addition, sensor fusion concepts (i.e. using more than one sensor technology) are being explored in an effort to bring the best of each technology to bear in solving the UXO problem. The UXO industry (both military and civilian) cannot reasonably equally support every technology and sensor type being explored and promoted today. Rather, a tradeoff must occur in which only those technologies that are the most superior (both technically and economically) will become the de facto industry standards. Since it is unclear at this point which technotogies and sensors types are superior, deciding how to wisely invest scarce R&D funds in this environment is complex. Al We-AM Al-2 SPLITTING OF DEGERATE NATURAL MODES FOR 09:20 BURIED TARGETS WITH ALMOST-02 SYMMETRY Carl E. Baum Air Force Research Laboratory DEHP 3550 Aberdeen Ave. SE Kirtland AFB, NM 87117-5776 A recent paper [C.E. Baum, Interaction Note 523, 1996] has introduced a target signature based on continuous two-dimensional rotational symmetry with axial symmetry planes (C,,a =02 symmetry). For wavelengths on the order of the target dimensions, this is sufficient to give zero backscattering cross polarization in the usual radar h, v coordinates ---> where the axis of rotation is perpendicular to the 1 h direction: Furthermore this property remains as the radar is moved around the target. For targets on or under the ground surface, this also allows for a vertically stratified earth which maintains the above symmetry. Note that it is the lack of something (the h, v backscattering) which is the signature. As such this can be referred to as a vampire signature, a vampire not seeing its reflection in a mirror (in this case the h, v mirror), at least according to legend. This signature has now been experimentally observed [L. Carin, R. Kapoor, and C.E. Baum, IEEE Trans. Geoscience and Remote Sensing, pp. 1985-1988, 1998]. Note that for SAR ( synthetic aperture radar) measurements the 0 2 symmetry is important since measurements are made from many azimuthal angles around the target. For buried targets and associated lossy dielectric half space with 0 2 symmetry (vertical rotation axis and axial symmetry planes, infinite in number) there is a two-fold degeneracy
Recommended publications
  • Users' Guide for Hand-Held and Walk-Through Metal Detectors
    U.S. Department of Justice Office of Justice Programs National Institute of Justice National Institute of Justice Users’ Guide for Hand-Held and Walk-Through Metal Detectors NIJ Guide 600–00 ABOUT THE LAW ENFORCEMENT AND CORRECTIONS STANDARDS AND TESTING PROGRAM The Law Enforcement and Corrections Standards and Testing Program is sponsored by the Office of Science and Technology of the National Institute of Justice (NIJ), U.S. Department of Justice. The program responds to the mandate of the Justice System Improvement Act of 1979, which directed NIJ to encourage research and development to improve the criminal justice system and to disseminate the results to Federal, State, and local agencies. The Law Enforcement and Corrections Standards and Testing Program is an applied research effort that determines the technological needs of justice system agencies, sets minimum performance standards for specific devices, tests commercially available equipment against those standards, and disseminates the standards and the test results to criminal justice agencies nationally and internationally. The program operates through: The Law Enforcement and Corrections Technology Advisory Council (LECTAC), consisting of nationally recognized criminal justice practitioners from Federal, State, and local agencies, which assesses technological needs and sets priorities for research programs and items to be evaluated and tested. The Office of Law Enforcement Standards (OLES) at the National Institute of Standards and Technology, which develops voluntary national performance standards for compliance testing to ensure that individual items of equipment are suitable for use by criminal justice agencies. The standards are based upon laboratory testing and evaluation of representative samples of each item of equipment to determine the key attributes, develop test methods, and establish minimum performance requirements for each essential attribute.
    [Show full text]
  • Together We Can Do Great Things Gyda'n Gilydd, Gallwn Wneud
    Together we can do great things Gyda’n gilydd, gallwn wneud pethau mawr Headteacher/Prifathro Mrs S Parry Headteachers Blog Number 136 Blog Prifathro Rhif 5th March 2021 Dear Parents, Guardians and Students/Annwyl Rieni,Gwarchodwyr a Myfyrwyr LHS - the return This week, we received the wonderful news that infection rates in Wales have reduced to a rate that Welsh Government consider it safe for us to formally plan for the staggered return of all students from 15th March. On Monday 8th March I will send our comprehensive plans to all stakeholders to allow everyone to get ready to return. We are reviewing all risk assessments and health and safety processes around the school. As part of this, we will be sending out guidance and resources for the optional use of lateral flow testing for staff and students. Rest assured that we will temper our enthusiasm to get back with our commitment to health and safety. There will be significant additional measures in place. We are preparing all details in preparation to update you on Monday. Patagonia bound on our 100 Heroes Charity and Fitness Event! In the meantime, please do follow the link below to view a very special video message that has been made by the staff of City Hospice to talk about the impact that our 100 Heroes campaign can have on the work that they do. We are really touched to hear from the amazing staff who work at City Hospice. We are making the journey of 12,000km to Patagonia because City Hospice has provided love and care for many members of our community and is close to our heart.
    [Show full text]
  • Use of Metal Detectors Tahoe National Forest
    Use of Metal Detectors Tahoe National Forest Metal Detector Use Definitions Metal detectors are used by both hobbyists and professionals to look for hidden coins, pipes, and other metallic objects. Due to the need to protect Treasure Trove archaeological sites, we’ve prepared this guide for the Treasure trove includes money, gems, precious metal use of metal detectors on Tahoe National Forest lands. coins, plate, or bullion that has been deliberately hidden If you have questions, contact information is listed on the with the intention of recovering it later. The search for back of this document. buried treasure can involve methods that are damaging to natural and cultural resources, thus a special-use permit from the Forest Service is required. Each permit Help Protect History request is evaluated before such permits are granted. Archaeological sites throughout California provide important insights and knowledge about the past that Archaeological Sites can be gained nowhere else. They are the repositories The use of metal detectors to locate objects of historical for people and cultures not represented in history books. or archaeological value is permitted subject to the Removing artifacts from sites destroys the context of the provisions of the Archaeological Resource Protection Act site, much like tearing pages from a book. Professional of 1979 and the Secretary of Agriculture’s Regulations. archaeologists depend on finding artifacts in their This activity requires a special-use permit. Permits are original location and association to other objects, so they only issued for legitimate research conducted by can accurately understand and interpret the story of that qualified professional archaeologists.
    [Show full text]
  • Istituto Di Radioastronomia Inaf
    ISTITUTO DI RADIOASTRONOMIA INAF STATUS REPORT October 2007 http://www.ira.inaf.it/ Chapter 1. STRUCTURE AND ORGANIZATION The Istituto di Radioastronomia (IRA) is presently the only INAF structure with divisions distributed over the national territory. Such an organization came about because IRA was originally a part of the National Council of Research (CNR), which imposed the first of its own reforms in 2001. The transition from CNR to INAF began in 2004 and was completed on January 1st , 2005. The Institute has its headquarters in Bologna in the CNR campus area, and two divisions in Firenze and Noto. The Medicina station belongs to the Bologna headquarters. A fourth division is foreseen in Cagliari at the Sardinia Radiotelescope site. The IRA operates 3 radio telescopes: the Northern Cross Radio Telescope (Medicina), and two 32-m dishes (Medicina and Noto), which are used primarily for Very Long Baseline Interferometry (VLBI) observations. The IRA leads the construction of the Sardinia Radio Telescope (SRT), a 64-m dish of new design. This is one of the INAF large projects nowadays. The aims of the Institute comprise: - the pursuit of excellence in many research areas ranging from observational radio astronomy, both galactic and extragalactic, to cosmology, to geodesy and Earth studies; - the design and management of the Italian radio astronomical facilities; - the design and fabrication of instrumentation operating in bands from radio to infrared and visible. Main activities of the various sites include: Bologna: The headquarters are responsible for the institute management and act as interface with the INAF central headquarters in Roma. Much of the astronomical research is done in Bologna, with major areas in cosmology, extragalactic astrophysics, star formation and geodesy.
    [Show full text]
  • How to Find GOLD
    FIND GOLD TO HOW “Whether you hunt for gold How to Find in the field and stream or in old mines, mine dumps or dredge piles, this book will guide you on your quest to GOLD recover more gold.” Metal Detecting and Panning GARRETT/L Learn effective use of a metal detector and gold pan for: AGAL • Dry panning • Wet panning • Nugget hunting • Field searching Ram Publishing Company A subsidiary of Garrett Metal Detectors ISBN-13: 978-0-915920-98-3 ISBN-10: 0-915920-98-0 $3.95 R 1881 West State Street 50395 Garland, TX 75042 AM PN 1509400 ISBN 0-915920-98-0 9 780915 920983 Charles Garrett / Roy Lagal How to Find GOLD Metal Detecting and Panning Charles Garrett/Roy Lagal HOW TO FIND GOLD © Charles L. Garrett/Roy Lagal 2007 Manufactured in the United States of America. All rights reserved. No part of this book may be reproduced or transmitted in any form or by any means, electronic or mechanical, including photocopying, recording or by any information storage or retrieval system, except in the case of brief quotations embodied in critical articles and reviews. For information, address all inquiries to Editor, Ram Publishing Company. First printing: July 2007 2 www.garrett.com CONTENTS About the Author ...................................................5 Introduction ............................................................9 Basic Tools.............................................................11 Additional Tools ...............................................12 Using a Pan to Find Gold ....................................13 Wet Panning .....................................................14
    [Show full text]
  • Radio Astronomy
    Edition of 2013 HANDBOOK ON RADIO ASTRONOMY International Telecommunication Union Sales and Marketing Division Place des Nations *38650* CH-1211 Geneva 20 Switzerland Fax: +41 22 730 5194 Printed in Switzerland Tel.: +41 22 730 6141 Geneva, 2013 E-mail: [email protected] ISBN: 978-92-61-14481-4 Edition of 2013 Web: www.itu.int/publications Photo credit: ATCA David Smyth HANDBOOK ON RADIO ASTRONOMY Radiocommunication Bureau Handbook on Radio Astronomy Third Edition EDITION OF 2013 RADIOCOMMUNICATION BUREAU Cover photo: Six identical 22-m antennas make up CSIRO's Australia Telescope Compact Array, an earth-rotation synthesis telescope located at the Paul Wild Observatory. Credit: David Smyth. ITU 2013 All rights reserved. No part of this publication may be reproduced, by any means whatsoever, without the prior written permission of ITU. - iii - Introduction to the third edition by the Chairman of ITU-R Working Party 7D (Radio Astronomy) It is an honour and privilege to present the third edition of the Handbook – Radio Astronomy, and I do so with great pleasure. The Handbook is not intended as a source book on radio astronomy, but is concerned principally with those aspects of radio astronomy that are relevant to frequency coordination, that is, the management of radio spectrum usage in order to minimize interference between radiocommunication services. Radio astronomy does not involve the transmission of radiowaves in the frequency bands allocated for its operation, and cannot cause harmful interference to other services. On the other hand, the received cosmic signals are usually extremely weak, and transmissions of other services can interfere with such signals.
    [Show full text]
  • B.Signatures-And-Pho
    Signature Identifications & Photographs Pier by Pier — Miller Goss (March 2018) The names are given as (1) Surname, (2) Exact form of the signauture in brackets [], location (e.g. E1-1 for pier E1 and side 1), and notes. Many individuals are still not known to us (marked by a ?). If you have notes for individuals (e.g. full name, affiliation, connection to Ron Bracewell, etc) please contact Goss ([email protected]). The list below gives the signatures on each of the nine sundial piers, from 8 am through 4 pm. The tenth pier introduces the Sundial Plaza and is adjacent to the sole Stanford dish that we have. All photos are March 2018. 8am — Side 1 faces the center of the sundial. N4 (off the pad to the west); N4 is the Stanford designation, meaning the 4th telescope on the north arm. 9am — side 4 to the center – N1. 10am – side 4 to the center – E2 11am — side 4 to the center – E3 NOON — side 1 to the center – E1 1pm— side 4 to the center (our dish was mounted on this pier) – W1 2pm— side 3 to the center — S1 3pm— side 4 to the center — W2 4pm — side 3 to the center — N2 (off the pad to the east) The 10th pier (not part of the sundial; near the dish) — W1 --------------------------------------------------------------------------------------------------------------------------------------- 8 AM Pier N4 (off the pad). side 1 to center Side 1 8am Frater [Bob Frater] N4-1. Roberts H. Frater . University of Sydney, CSIRO, Resmed. 1 Side 2 8am Watkinson [Arthur Watkinson] N4-2. RPL colleague of Ron’s and later Sydney Univer , Fleurs.
    [Show full text]
  • Wikipedia, the Free Encyclopedia
    SKA newsletter Volume 21 - April 2011 The Square Kilometre Array Exploring the Universe with the world’s largest radio telescope www.skatelescope.org Please click the relevant section title to skip to that section 03 Project news 04 From the SPDO 05 SKA science 08 Engineering update 10 Site characterisation 12 Outreach update 14 Industry participation 17 News from around the world 18 Africa 20 Australia and New Zealand 23 Canada 25 China 28 Europe 31 India 33 US 35 Future meetings and events Project news Project news 04 From the SPDO Crucial steps for the SKA project were At its first meeting on 2 April, the Founding taken in the last week of March 2011. A Board decided that the location of the SKA Founding Board was created with the Project Office (SPO) will be at the Jodrell aim of establishing a legal entity for the Bank Observatory near Manchester in the project by the time of the SKA Forum in UK. This decision followed a competitive Canada in early July, as well as agreeing bidding process in which a number of the resourcing of the Project Execution excellent proposals were evaluated in an Plan for the Pre-construction Phase international review process. The SPO, which from 2012 to 2015. The Founding Board is hoped to grow to 60 people over the next replaces the Agencies SKA Group with four years, will supersede the SPDO currently immediate effect. Prof John Womersley based at the University of Manchester. The from the UK’s Science and Technology physical move to a new building at Jodrell Facilities Council (STFC) was elected Bank Observatory is scheduled for mid-2012.
    [Show full text]
  • Table of Contents - 1 - - 2
    Table of contents - 1 - - 2 - Table of Contents Foreword 5 1. The European Consortium for VLBI 7 2. Scientific highlights on EVN research 9 3. Network Operations 35 4. VLBI technical developments and EVN operations support at member institutes 47 5. Joint Institute for VLBI in Europe (JIVE) 83 6. EVN meetings 105 7. EVN publications in 2007-2008 109 - 3 - - 4 - Foreword by the Chairman of the Consortium The European VLBI Network (EVN) is the result of a collaboration among most major radio observatories in Europe, China, Puerto Rico and South Africa. The large radio telescopes hosted by these observatories are operated in a coordinated way to perform very high angular observations of cosmic radio sources. The data are then correlated by using the EVN correlator at the Joint Institute for VLBI in Europe (JIVE). The EVN, when operating as a single astronomical instrument, is the most sensitive VLBI array and constitutes one of the major scientific facilities in the world. The EVN also co-observes with the Very Long Baseline Array (VLBA) and other radio telescopes in the U.S., Australia, Japan, Russia, and with stations of the NASA Deep Space Network to form a truly global array. In the past, the EVN also operated jointly with the Japanese space antenna HALCA in the frame of the VLBI Space Observatory Programme (VSOP). The EVN plans now to co-observe with the Japanese space 10-m antenna ASTRO-G, to be launched by 2012, within the frame of the VSOP-2 project. With baselines in excess of 25.000 km, the space VLBI observations provide the highest angular resolution ever achieved in Astronomy.
    [Show full text]
  • Issue No. 72, April 2012 ISSN 1323-6326
    CSIRO ASTroNOMY AND SPacE SciENCE www.csiro.au ATNF News Issue No. 72, April 2012 ISSN 1323-6326 CSIRO Astronomy and Space Science — Undertaking world-leading astronomical research and operator of the Australia Telescope National Facility. Editorial Welcome to the April 2012 edition of ATNF forthcoming changes to the ATNF website. News. We review two recent workshops held at ATNF headquarters in Marsfield and we Regular readers will have noticed that this welcome our newest postdoctoral staff. edition has a fresh new appearance. We are in the process of updating the ‘visual Four science articles give a snapshot of identity’ of all CSIRO communications the latest radio astronomy research being including ATNF News, a flagship publication conducted with the ATNF. These include: of CSIRO Astronomy and Space Science An investigation into the neutral gas of (CASS). While the newsletter’s appearance ◆ the blue compact dwarf galaxy NGC 5253 has changed, we will continue to bring you by Ángel R. López-Sánchez and Bärbel news and research results related to CSIRO’s Koribalski Australia Telescope National Facility. A report on constraining the fundamental We start this edition by acknowledging ◆ constants of physics through astronomical Michelle Storey and George Hobbs, two observations of rotational transitions CASS staff members who have recently of methanol by Simon Ellingsen and received external awards for their collaborators contributions to radio astronomy. An ATCA survey of molecular gas in We then feature the recent progress that ◆ high-z radio galaxies by Bjorn Emonts and has been made on the construction of collaborators, and ASKAP and the Murchison Widefield Array, and CSIRO’s contribution to the next phase ◆ Ray Norris’ account of witnessing the of planning for the international Square birth of a quasar.
    [Show full text]
  • Scientific Problems Addressed by the Spektr-UV Space Project (World Space Observatory—Ultraviolet)
    ISSN 1063-7729, Astronomy Reports, 2016, Vol. 60, No. 1, pp. 1–42. c Pleiades Publishing, Ltd., 2016. Original Russian Text c A.A. Boyarchuk, B.M. Shustov, I.S. Savanov, M.E. Sachkov, D.V. Bisikalo, L.I. Mashonkina, D.Z. Wiebe, V.I. Shematovich, Yu.A. Shchekinov, T.A. Ryabchikova, N.N. Chugai, P.B. Ivanov, N.V. Voshchinnikov, A.I. Gomez de Castro, S.A. Lamzin, N. Piskunov, T. Ayres, K.G. Strassmeier, S. Jeffrey, S.K. Zwintz, D. Shulyak, J.-C. G´erard, B. Hubert, L. Fossati, H. Lammer, K. Werner, A.G. Zhilkin, P.V. Kaigorodov, S.G. Sichevskii, S. Ustamuich, E.N. Kanev, E.Yu. Kil’pio, 2016, published in Astronomicheskii Zhurnal, 2016, Vol. 93, No. 1, pp. 3–48. Scientific Problems Addressed by the Spektr-UV Space Project (World Space Observatory—Ultraviolet) A. A. Boyarchuk1, B.M.Shustov1*, I. S. Savanov1, M.E.Sachkov1, D. V. Bisikalo1, L. I. Mashonkina1, D.Z.Wiebe1,V.I.Shematovich1,Yu.A.Shchekinov2, T. A. Ryabchikova1, N.N.Chugai1, P.B.Ivanov3, N.V.Voshchinnikov4, A. I. Gomez de Castro5,S.A.Lamzin6,N.Piskunov7,T.Ayres8, K. G. Strassmeier9, S. Jeffrey10,S.K.Zwintz11, D. Shulyak12,J.-C.Gerard´ 13,B.Hubert13, L. Fossati14, H. Lammer14,K.Werner15,A.G.Zhilkin1,P.V.Kaigorodov1, S. G. Sichevskii1,S.Ustamuich5,E.N.Kanev1, and E. Yu. Kil’pio1 1Institute of Astronomy, Russian Academy of Sciences, ul. Pyatnitskaya 48, Moscow, 119017 Russia 2Southern Federal University, Rostov-on-Don, 344006 Russia 3Astro Space Center, Lebedev Physical Institute, Russian Academy of Sciences, Moscow, Russia 4St.
    [Show full text]
  • <> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA
    1 SATELITES ARTIFICIALES. Capítulo 5º Subcap. 10 <> CRONOLOGIA DE LOS SATÉLITES ARTIFICIALES DE LA TIERRA. Esta es una relación cronológica de todos los lanzamientos de satélites artificiales de nuestro planeta, con independencia de su éxito o fracaso, tanto en el disparo como en órbita. Significa pues que muchos de ellos no han alcanzado el espacio y fueron destruidos. Se señala en primer lugar (a la izquierda) su nombre, seguido de la fecha del lanzamiento, el país al que pertenece el satélite (que puede ser otro distinto al que lo lanza) y el tipo de satélite; este último aspecto podría no corresponderse en exactitud dado que algunos son de finalidad múltiple. En los lanzamientos múltiples, cada satélite figura separado (salvo en los casos de fracaso, en que no llegan a separarse) pero naturalmente en la misma fecha y juntos. NO ESTÁN incluidos los llevados en vuelos tripulados, si bien se citan en el programa de satélites correspondiente y en el capítulo de “Cronología general de lanzamientos”. .SATÉLITE Fecha País Tipo SPUTNIK F1 15.05.1957 URSS Experimental o tecnológico SPUTNIK F2 21.08.1957 URSS Experimental o tecnológico SPUTNIK 01 04.10.1957 URSS Experimental o tecnológico SPUTNIK 02 03.11.1957 URSS Científico VANGUARD-1A 06.12.1957 USA Experimental o tecnológico EXPLORER 01 31.01.1958 USA Científico VANGUARD-1B 05.02.1958 USA Experimental o tecnológico EXPLORER 02 05.03.1958 USA Científico VANGUARD-1 17.03.1958 USA Experimental o tecnológico EXPLORER 03 26.03.1958 USA Científico SPUTNIK D1 27.04.1958 URSS Geodésico VANGUARD-2A
    [Show full text]