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General Assembly Distr.: General 29 January 2001
United Nations A/AC.105/751/Add.1 General Assembly Distr.: General 29 January 2001 Original: English Committee on the Peaceful Uses of Outer Space National research on space debris, safety of space objects with nuclear power sources on board and problems of their collisions with space debris Note by the Secretariat* Addendum Contents Chapter Paragraphs Page I. Introduction........................................................... 1-2 2 Replies received from Member States and international organizations .................... 2 United States of America ......................................................... 2 European Space Agency.......................................................... 7 __________________ * The present document contains replies received from Member States and international organizations between 25 November 2000 and 25 January 2001. V.01-80520 (E) 020201 050201 A/AC.105/751/Add.1 I. Introduction 1. At its forty-third session, the Committee on the Peaceful Uses of Outer Space agreed that Member States should continue to be invited to report to the Secretary- General on a regular basis with regard to national and international research concerning the safety of space objects with nuclear power sources, that further studies should be conducted on the issue of collision of orbiting space objects with nuclear power sources on board with space debris and that the Committee’s Scientific and Technical Subcommittee should be kept informed of the results of such studies.1 The Committee also took note of the agreement of the Subcommittee that national research on space debris should continue and that Member States and international organizations should make available to all interested parties the results of that research, including information on practices adopted that had proved effective in minimizing the creation of space debris (A/AC.105/736, para. -
The Early Explorers by Andrew J
The Early Explorers by Andrew J. LePage August 8, 1999 Among these programs were the next generation of Introduction Explorer satellites the ABMA was planning. In the chaos that swept the United States after the launching of the first Soviet Sputniks, a variety of The First New Explorers satellite programs was sponsored by the Department The first of the new series of larger Explorer satellites of Defense (DoD) to supplement (and in some cases was the 39.7 kilogram (87.5 pound) satellite NASA supplant) the country's flagging "official" satellite designated as S-1. Built by JPL, the spin stabilized program, Vanguard. One of the stronger programs S-1 consisted of a pair of fiberglass cones joined at was sponsored by the ABMA (Army Ballistic Missile their bases with a diameter and height of 76 Agency) with its engineering team lead by the centimeters each. The scientific payload consisted of German rocket expert, Wernher von Braun. Using instruments to study cosmic rays, solar X-ray and the Juno I launch vehicle, the ABMA team launched ultraviolet emissions, micrometeorites, as well as the America's first satellite, Explorer 1, which was built globe's heat balance. This was all powered by a bank by Caltech's Jet Propulsion Laboratory (JPL) (see of 15 nickel-cadmium batteries recharged by 3,000 Explorer: America's First Satellite in the February solar cells mounted on the satellite's exterior. This 1998 issue of SpaceViews). advanced payload was equipped with a timer to turn itself off after a year in orbit. While these first satellites returned a wealth of new data, they were limited by the tiny 11 kilogram (25 Explorer S-1 was launched from Cape Canaveral on pound) payload capability of the Juno I. -
AAS Worldwide Telescope: Seamless, Cross-Platform Data Visualization Engine for Astronomy Research, Education, and Democratizing Data
AAS WorldWide Telescope: Seamless, Cross-Platform Data Visualization Engine for Astronomy Research, Education, and Democratizing Data The Harvard community has made this article openly available. Please share how this access benefits you. Your story matters Citation Rosenfield, Philip, Jonathan Fay, Ronald K Gilchrist, Chenzhou Cui, A. David Weigel, Thomas Robitaille, Oderah Justin Otor, and Alyssa Goodman. 2018. AAS WorldWide Telescope: Seamless, Cross-Platform Data Visualization Engine for Astronomy Research, Education, and Democratizing Data. The Astrophysical Journal: Supplement Series 236, no. 1. Published Version https://iopscience-iop-org.ezp-prod1.hul.harvard.edu/ article/10.3847/1538-4365/aab776 Citable link http://nrs.harvard.edu/urn-3:HUL.InstRepos:41504669 Terms of Use This article was downloaded from Harvard University’s DASH repository, and is made available under the terms and conditions applicable to Open Access Policy Articles, as set forth at http:// nrs.harvard.edu/urn-3:HUL.InstRepos:dash.current.terms-of- use#OAP Draft version January 30, 2018 Typeset using LATEX twocolumn style in AASTeX62 AAS WorldWide Telescope: Seamless, Cross-Platform Data Visualization Engine for Astronomy Research, Education, and Democratizing Data Philip Rosenfield,1 Jonathan Fay,1 Ronald K Gilchrist,1 Chenzhou Cui,2 A. David Weigel,3 Thomas Robitaille,4 Oderah Justin Otor,1 and Alyssa Goodman5 1American Astronomical Society 1667 K St NW Suite 800 Washington, DC 20006, USA 2National Astronomical Observatories, Chinese Academy of Sciences 20A Datun Road, Chaoyang District Beijing, 100012, China 3Christenberry Planetarium, Samford University 800 Lakeshore Drive Birmingham, AL 35229, USA 4Aperio Software Ltd. Headingley Enterprise and Arts Centre, Bennett Road Leeds, LS6 3HN, United Kingdom 5Harvard Smithsonian Center for Astrophysics 60 Garden St. -
University of Iowa Instruments in Space
University of Iowa Instruments in Space A-D13-089-5 Wind Van Allen Probes Cluster Mercury Earth Venus Mars Express HaloSat MMS Geotail Mars Voyager 2 Neptune Uranus Juno Pluto Jupiter Saturn Voyager 1 Spaceflight instruments designed and built at the University of Iowa in the Department of Physics & Astronomy (1958-2019) Explorer 1 1958 Feb. 1 OGO 4 1967 July 28 Juno * 2011 Aug. 5 Launch Date Launch Date Launch Date Spacecraft Spacecraft Spacecraft Explorer 3 (U1T9)58 Mar. 26 Injun 5 1(U9T68) Aug. 8 (UT) ExpEloxrpelro r1e r 4 1915985 8F eJbu.l y1 26 OEGxOpl o4rer 41 (IMP-5) 19697 Juunlye 2 281 Juno * 2011 Aug. 5 Explorer 2 (launch failure) 1958 Mar. 5 OGO 5 1968 Mar. 4 Van Allen Probe A * 2012 Aug. 30 ExpPloiorenre 3er 1 1915985 8M Oarc. t2. 611 InEjuxnp lo5rer 45 (SSS) 197618 NAouvg.. 186 Van Allen Probe B * 2012 Aug. 30 ExpPloiorenre 4er 2 1915985 8Ju Nlyo 2v.6 8 EUxpKlo 4r e(rA 4ri1el -(4IM) P-5) 197619 DJuenc.e 1 211 Magnetospheric Multiscale Mission / 1 * 2015 Mar. 12 ExpPloiorenre 5e r 3 (launch failure) 1915985 8A uDge.c 2. 46 EPxpiolonreeerr 4130 (IMP- 6) 19721 Maarr.. 313 HMEaRgCnIe CtousbpeShaetr i(cF oMxu-1ltDis scaatelell itMe)i ssion / 2 * 2021081 J5a nM. a1r2. 12 PionPeioenr e1er 4 1915985 9O cMt.a 1r.1 3 EExpxlpolorerer r4 457 ( S(IMSSP)-7) 19721 SNeopvt.. 1263 HMaalogSnaett oCsupbhee Sriact eMlluitlet i*scale Mission / 3 * 2021081 M5a My a2r1. 12 Pioneer 2 1958 Nov. 8 UK 4 (Ariel-4) 1971 Dec. 11 Magnetospheric Multiscale Mission / 4 * 2015 Mar. -
Smiths 0 N U N Ins Ti Tu Tion Astrophysical Observatory
SMITHS0 NUN INS TITU TION ASTROPHYSICAL OBSERVATORY OPTICAL SATELLITE- TRACKING PROGRAM Grant Number NGR 09-015-002 Semiannual Progress Report No. 20 1 January 1969 to 30 June 1969 Project Director: Fred L. Whipple Prepared for National Aeronautics and Space Administration Washington, D. C. 20546 Smithsonian Institution Astrophysical Observatory Cambridge, Massachusetts 021 38 SMITHSONIAN INS TITU TION ASTROPHYSICAL OBSERVATORY OPTICAL SATELLITE- TRACKING PROGRAM Grant Number NGR 09-015-002 Semiannual Progress Report No. 20 1 January 1969 to 30 June 1969 Project Director: Fred L. Whipple Prepared for National Ae r onauti cs and Space Administration Washington, D. C. 20546 Smithsonian Institution A s t r o phy s i cal Ob s e rvatory Cambridge, Massachusetts 021 38 908-2 TABLE OF CONTENTS Page INTRODUCTION .................................. 1 RESEARCHPROGRAMS ............................. .2 GEODETIC INVESTIGATIONS ...................... 3 ATMOSPHERIC INVESTIGATIONS ................... 6 DATAACQUISITION ............................... 8 SATELLITE- TRACKING AND DATA-ACQUISITION DEPARTMENT ................................ 9 COMMUNICATIONS ............................. 21 DATAPROCESSING ................................ 23 DATA PROCESSING ............................. 24 PHOTOREDUCTION DIVISION ...................... 27 PROGRAMMING DIVISION. ........................ 29 EDITORIAL AND PUBLICATIONS. ...................... 31 ii INTRODUCTION In support of the scientific and operational requirements under the Satellite- Tracking Program grant, the -
Information Summaries
TIROS 8 12/21/63 Delta-22 TIROS-H (A-53) 17B S National Aeronautics and TIROS 9 1/22/65 Delta-28 TIROS-I (A-54) 17A S Space Administration TIROS Operational 2TIROS 10 7/1/65 Delta-32 OT-1 17B S John F. Kennedy Space Center 2ESSA 1 2/3/66 Delta-36 OT-3 (TOS) 17A S Information Summaries 2 2 ESSA 2 2/28/66 Delta-37 OT-2 (TOS) 17B S 2ESSA 3 10/2/66 2Delta-41 TOS-A 1SLC-2E S PMS 031 (KSC) OSO (Orbiting Solar Observatories) Lunar and Planetary 2ESSA 4 1/26/67 2Delta-45 TOS-B 1SLC-2E S June 1999 OSO 1 3/7/62 Delta-8 OSO-A (S-16) 17A S 2ESSA 5 4/20/67 2Delta-48 TOS-C 1SLC-2E S OSO 2 2/3/65 Delta-29 OSO-B2 (S-17) 17B S Mission Launch Launch Payload Launch 2ESSA 6 11/10/67 2Delta-54 TOS-D 1SLC-2E S OSO 8/25/65 Delta-33 OSO-C 17B U Name Date Vehicle Code Pad Results 2ESSA 7 8/16/68 2Delta-58 TOS-E 1SLC-2E S OSO 3 3/8/67 Delta-46 OSO-E1 17A S 2ESSA 8 12/15/68 2Delta-62 TOS-F 1SLC-2E S OSO 4 10/18/67 Delta-53 OSO-D 17B S PIONEER (Lunar) 2ESSA 9 2/26/69 2Delta-67 TOS-G 17B S OSO 5 1/22/69 Delta-64 OSO-F 17B S Pioneer 1 10/11/58 Thor-Able-1 –– 17A U Major NASA 2 1 OSO 6/PAC 8/9/69 Delta-72 OSO-G/PAC 17A S Pioneer 2 11/8/58 Thor-Able-2 –– 17A U IMPROVED TIROS OPERATIONAL 2 1 OSO 7/TETR 3 9/29/71 Delta-85 OSO-H/TETR-D 17A S Pioneer 3 12/6/58 Juno II AM-11 –– 5 U 3ITOS 1/OSCAR 5 1/23/70 2Delta-76 1TIROS-M/OSCAR 1SLC-2W S 2 OSO 8 6/21/75 Delta-112 OSO-1 17B S Pioneer 4 3/3/59 Juno II AM-14 –– 5 S 3NOAA 1 12/11/70 2Delta-81 ITOS-A 1SLC-2W S Launches Pioneer 11/26/59 Atlas-Able-1 –– 14 U 3ITOS 10/21/71 2Delta-86 ITOS-B 1SLC-2E U OGO (Orbiting Geophysical -
Centaur Dl-A Systems in a Nutshell
NASA Technical Memorandum 88880 '5 t I Centaur Dl-A Systems in a Nutshell (NASA-TM-8888o) CElTAUR D1-A SYSTEBS IN A N87- 159 96 tiljTSBELL (NASA) 29 p CSCL 22D Andrew L. Gordan Lewis Research Center Cleveland, Ohio January 1987 . CENTAUR D1-A SYSTEMS IN A NUTSHELL Andrew L. Gordan National Aeronautics and Space Administration Lewis Research Center Cleveland, Ohio 44135 SUMMARY This report identifies the unique aspects of the Centaur D1-A systems and subsystems. Centaur performance is described in terms of optimality (pro- pellant usage), flexibility, and airborne computer requirements. Major I-. systems are described narratively with some numerical data given where it may 03 CJ be useful. v, I W INTRODUCT ION The Centaur D1-A launch vehicle continues to be a key element in the Nation's space program. The Atlas/Centaur and Titan/Centaur combinations have boosted into orbit a variety of spacecraft on scientific, lunar, and planetary exploration missions and Earth orbit missions. These versatile, reliable, and accurate space booster systems will contribute to many significant space pro- grams well into the shuttle era. Centaur D1-A is the latest version of the Nation's first high-energy cryogenic launch vehicle. Major improvements in avionics and payload struc- ture have enhanced mission flexibility and mission success reliability. The liquid hydrogen and liquid oxygen propellants and the pressurized stainless steel structure provide a top-performance vehicle. Centaur's primary thrust comes from two Pratt 8, Whitney constant- thrust, turbopump-fed, regeneratively cooled, liquid-fueled rocket engines. Each RL10A-3-3a engine can generate 16 500 lb of thrust, for a total thrust of 33 000 lb. -
Novell® Platespin® Recon 3.7.4 User Guide 5.6.4 Printing and Exporting Reports
www.novell.com/documentation User Guide Novell® PlateSpin® Recon 3.7.4 September 2012 Legal Notices Novell, Inc., makes no representations or warranties with respect to the contents or use of this documentation, and specifically disclaims any express or implied warranties of merchantability or fitness for any particular purpose. Further, Novell, Inc., reserves the right to revise this publication and to make changes to its content, at any time, without obligation to notify any person or entity of such revisions or changes. Further, Novell, Inc., makes no representations or warranties with respect to any software, and specifically disclaims any express or implied warranties of merchantability or fitness for any particular purpose. Further, Novell, Inc., reserves the right to make changes to any and all parts of Novell software, at any time, without any obligation to notify any person or entity of such changes. Any products or technical information provided under this Agreement may be subject to U.S. export controls and the trade laws of other countries. You agree to comply with all export control regulations and to obtain any required licenses or classification to export, re-export or import deliverables. You agree not to export or re-export to entities on the current U.S. export exclusion lists or to any embargoed or terrorist countries as specified in the U.S. export laws. You agree to not use deliverables for prohibited nuclear, missile, or chemical biological weaponry end uses. See the Novell International Trade Services Web page (http://www.novell.com/info/exports/) for more information on exporting Novell software. -
A New Polarimeter to Study the Curl Component of the Cosmic Microwave Background Polarization
UNIVERSITA` DEGLI STUDI DI ROMA \LA SAPIENZA" Facolt`adi Scienze Matematiche Fisiche e Naturali A new polarimeter to study the curl component of the Cosmic Microwave Background polarization Tesi di Laurea Specialistica in Astronomia ed Astro¯sica Anno Accademico 2005/2006 Author Supervisor Lorenzo Moncelsi Prof. Paolo de Bernardis Register: 1071681 Co-supervisor Dott. Federico Nati Contents Introduzione 6 Introduction 10 1 The Hot Big Bang Model and the Inflation add-on 11 1.1 Introduction . 11 1.2 The Standard Cosmological Model . 11 1.3 The Unsolved Problems . 17 1.3.1 The flatness problem . 17 1.3.2 The horizons problem . 18 1.3.3 The absence of magnetic monopoles . 19 1.4 The Solution: Inflation . 20 1.5 The Physics of Inflation . 22 1.5.1 Scalar Fields . 22 1.5.2 Slow-Roll Approximation . 25 1.5.3 Exact Solutions . 26 1.5.4 Hamilton-Jacobi Formulation . 28 1.5.5 Reheating . 29 1.5.6 Scalar Fluctuations . 30 1.5.7 Tensor Fluctuations . 34 2 The Cosmic Microwave Background 37 2.1 Introduction . 37 2.2 Earth's Absolute Motion: The Dipole Anisotropy . 39 2.3 The Last Scattering Surface . 42 2.4 The Temperature Power Spectrum . 44 2.4.1 Physical E®ects at Recombination . 44 2.4.2 Statistical Treatment . 47 2.4.3 The Shape of the Spectrum . 49 2.5 Polarization . 54 2.5.1 Thomson Scattering at Recombination . 54 2.5.2 Statistical Treatment . 56 2.5.3 Quadrupole Anisotropy From Scalar Perturbations . 65 I 2.5.4 Quadrupole Anisotropy From Tensor Perturbations . -
The Hot and Energetic Universe
The Hot And Energetic Universe The Universe was always the final frontier of the Human quest for knowledge Through all its history, humanity has observed the sky trying to understand the Cosmos outside the limits of our planet Today, this effort has yielded significant results. Now we know that our sun is a typical star, which does not differ significantly from the other stars of the starry sky. We have discovered the planets of our Solar System and we have studied the conditions prevailing in them. We studied asteroids and comets and found their important role in the formation of planets. We understand the basic principles of the formation, the life and the death of stars. We have also discovered thousands of exoplanets orbiting other stars. We studied giant star clusters. We have discovered dense clouds of interstellar dust and gas where new stars are born continuously. We have managed to describe the gigantic complex of stars to which we belong. Our Galaxy. We realized that our Galaxy is not alone in the universe and that there are hundreds of billions of galaxies. We discovered that the universe of galaxies is extremely violent and in constant motion. Finally we found that the whole universe is in accelerating expansion and we are searching urgently for its origin. This quest is an epic journey towards knowledge, which abolish superstitions and defines human existence. Vehicles for the journey of humanity in the universe are scientific instruments called telescopes, which are installed at various observatories. Telescopes collect light. Their performance depends on the diameter of the lens or mirror used. -
California State University, Northridge Low Earth Orbit
CALIFORNIA STATE UNIVERSITY, NORTHRIDGE LOW EARTH ORBIT BUSINESS CENTER A Project submitted in partial satisfaction of the requirements for the degree of Master of Science in Engineering by Dallas Gene Bienhoff May 1985 The Proj'ectof Dallas Gene Bienhoff is approved: Dr. B. J. Bluth Professor T1mothy Wm. Fox - Chair California State University, Northridge ii iii ACKNOWLEDGEHENTS I wish to express my gratitude to those who have helped me over the years to complete this thesis by providing encouragement, prodding and understanding: my advisor, Tim Fox, Chair of Mechanical and Chemical Engineering; Dr. B. J. Bluth for her excellent comments on human factors; Dr. B. J. Campbell for improving the clarity; Richard Swaim, design engineer at Rocketdyne Division of Rockwell International for providing excellent engineering drawings of LEOBC; Mike Morrow, of the Advanced Engineering Department at Rockwell International who provided the Low Earth Orbit Business Center panel figures; Bob Bovill, a commercial artist, who did all the artistic drawings because of his interest in space commercialization; Linda Martin for her word processing skills; my wife, Yolanda, for egging me on without nagging; and finally Erik and Danielle for putting up with the excuse, "I have to v10rk on my paper," for too many years. iv 0 ' PREFACE The Low Earth Orbit Business Center (LEOBC) was initially conceived as a modular structure to be launched aboard the Space Shuttle, it evolved to its present configuration as a result of research, discussions and the desire to increase the efficiency of space utilization. Although the idea of placing space stations into Earth orbit is not new, as is discussed in the first chapter, and the configuration offers nothing new, LEOBC is unique in its application. -
Ionospheric Cusp Flows Pulsed by Solar Wind Alfvén Waves
c Annales Geophysicae (2002) 20: 161–174 European Geophysical Society 2002 Annales Geophysicae Ionospheric cusp flows pulsed by solar wind Alfven´ waves P. Prikryl1, G. Provan2, K. A. McWilliams2, and T. K. Yeoman2 1Communications Research Centre, Ottawa, Ontario K2H 8S2, Canada 2Department of Physics and Astronomy, University of Leicester, UK Received: 7 February 2001 – Revised: 24 August 2001 – Accepted: 10 September 2001 Abstract. Pulsed ionospheric flows (PIFs) in the cusp foot- bow shock were the source of magnetopause surface waves print have been observed by the SuperDARN radars with inducing reconnection. periods between a few minutes and several tens of minutes. Key words. Interplanetary physics (MHD waves and PIFs are believed to be a consequence of the interplanetary turbulence) – Magnetospheric physics (magnetosphere- magnetic field (IMF) reconnection with the magnetospheric ionosphere interactions; solar wind-magnetosphere interac- magnetic field on the dayside magnetopause, ionospheric tions) signatures of flux transfer events (FTEs). The quasiperiodic PIFs are correlated with Alfvenic´ fluctuations observed in the upstream solar wind. It is concluded that on these occasions, the FTEs were driven by Alfven´ waves coupling to the day- 1 Introduction side magnetosphere. Case studies are presented in which the dawn-dusk component of the Alfven´ wave electric field mod- Ionospheric dynamics near the cusp footprint attest to pro- ulates the reconnection rate as evidenced by the radar obser- cesses at the dayside magnetopause and in particular, to vations of the ionospheric cusp flows. The arrival of the IMF pulsed magnetic reconnection (Cowley et al., 1991; Lock- southward turning at the magnetopause is determined from wood et al., 1993).