The Interoperable Global Navigation Satellite Systems Space Service Volume
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Amateur-Satellite Service
Amateur-Satellite Service 1 26/11/2012 Some facts about the amateur-satellite service • Began in 1961 • Pioneered low-cost satellite technology • First privately funded space satellites • First satellite search & rescue (OSCAR 6 & 7) • First inter-satellite transmissions • Early tele-medicine transmissions • Pioneered distributed engineering 2 26/11/2012 Amateur-satellite organizations (by country) • Argentina AMSAT-LU • Australia AMSAT-Australia • Austria AMSAT-OE • Bermuda AMSAT-BDA • Brazil BRAMSAT • Chile AMSAT-CE • Denmark AMSAT-OZ • Germany AMSAT-DL • Finland AMSAT-OH • France AMSAT-France • Israel AMSAT-Israel • Italy AMSAT-Italia 3 26/11/2012 Amateur-satellite organizations (by country)…continued • Korea KITSAT Project • Mexico AMSAT-Mexico • New Zealand AMSAT-ZL • Qatar AMSAT-Qatar • Japan JAMSAT • North America AMSAT-NA • Russia AMSAT-R • South Africa AMSAT-SA • Spain AMSAT-URE • Sweden AMSAT-Sweden • United Kingdom AMSAT-UK • USA, Canada AMSAT-NA 4 26/11/2012 Co-operation with universities to develop & construct amateur-satellites Amateur satellites have been designed and constructed by university students with the help of local amateurs and amateur-satellite organizations. Some examples: ◊ Stellenbosch University (South Africa) ◊ University of Surrey (UK) ◊ University of Mexico ◊ Weber State University (USA) 5 26/11/2012 Student satellite project 6 26/11/2012 Orbiting Satellite Carrying Amateur Radio (OSCARs) Early satellite projects • April 1959 Concept of a satellite built by and for amateurs • OSCAR I Dec 1961 - Jan 1962, -
50 Satellite Formation-Flying and Rendezvous
Parkinson, et al.: Global Positioning System: Theory and Applications — Chap. 50 — 2017/11/26 — 19:03 — page 1 1 50 Satellite Formation-Flying and Rendezvous Simone D’Amico1) and J. Russell Carpenter2) 50.1 Introduction to Relative Navigation GNSS has come to play an increasingly important role in satellite formation-flying and rendezvous applications. In the last decades, the use of GNSS measurements has provided the primary method for determining the relative position of cooperative satellites in low Earth orbit. More recently, GNSS data have been successfully used to perform formation-flying in highly elliptical orbits with apogees at tens of Earth radii well above the GNSS constellations. Current research aims at dis- tributed precise relative navigation between tens of swarming nano- and micro-satellites based on GNSS. Similar to terrestrial applications, GNSS relative navigation benefits from a high level of common error cancellation. Furthermore, the integer nature of carrier phase ambiguities can be exploited in carrier phase differential GNSS (CDGNSS). Both aspects enable a substantially higher accuracy in the estimation of the relative motion than can be achieved in single-spacecraft navigation. Following historical remarks and an overview of the state-of-the-art, this chapter addresses the technology and main techniques used for spaceborne relative navigation both for real-time and offline applications. Flight results from missions such as the Space Shuttle, PRISMA, TanDEM-X, and MMS are pre- sented to demonstrate the versatility and broad range of applicability of GNSS relative navigation, from precise baseline determination on-ground (mm-level accuracy), to coarse real-time estimation on-board (m- to cm-level accuracy). -
Peter Gülzow, DB2OS 2020-06-05 © AMSAT-DL OSCAR-10 (P3-B) OSCAR-13 (P3-C) OSCAR-40 (P3-D)
Peter Gülzow, DB2OS 2020-06-05 © AMSAT-DL OSCAR-10 (P3-B) OSCAR-13 (P3-C) OSCAR-40 (P3-D) OSCAR-100 (P4-A) AMSAT Phase 4 = GEO The meaning of Es'hail “The story behind the name Es’hail (Canopus) is the name of a star which becomes visible in the night sky of the Middle East as summer turns to autumn. Traditionally, the sighting of Es’hail brings happiness as it means that winter is coming and that good weather will soon be with us. We hope that the arrival of Es’hailSat will equally be beneficial for the satellite community.” (from Es’hailSat: Follow the star) Canopus /kəˈnoʊpəs is the brightest star in the southern constellation of Carina, and is located near the western edge of the constellation around 310 light-years from the Sun. Its proper name is generally considered to originate from the mythological Canopus, who was a navigator for Menelaus, king of Sparta. H E Abdullah bin Hamad Al Attiyah, A71AU, Chairman of the Administrative Control and Time line Transparency Authority, who is also the Chairman of the Qatar Amateur Radio 1001+ arabian nights… Society (QARS) during the Qatar international amateur radio festival in December 2012. 2012 AMSAT-DL meets QARS | (DB2OS @ International Amateur Radio Festival in Qatar) | 2013 Es’hailSat - | Qatar Satellite Company | (idea, concept, design requirements, RFI, meetings with potential | suppliers, RFP, finalisiation of requirements) | 2016 Kick-Off at MELCO Japan | (Technical presentations, Requirements review, Critical Design Review, | Design Validation) | 2018 November 15th launch with SpaceX Falcon 9 2012 Qatar Ham Radio Festival Executives from Qatar’s Es’hailSat and Japan’s Mitsubishi Electric Space Systems (MELCO) in Kamakura, outside of Tokyo, Japan, to observe the vacuum chamber test of Es'hail-2. -
AIRLIFT RODEO a Brief History of Airlift Competitions, 1961-1989
"- - ·· - - ( AIRLIFT RODEO A Brief History of Airlift Competitions, 1961-1989 Office of MAC History Monograph by JefferyS. Underwood Military Airlift Command United States Air Force Scott Air Force Base, Illinois March 1990 TABLE OF CONTENTS Foreword . iii Introduction . 1 CARP Rodeo: First Airdrop Competitions .............. 1 New Airplanes, New Competitions ....... .. .. ... ... 10 Return of the Rodeo . 16 A New Name and a New Orientation ..... ........... 24 The Future of AIRLIFT RODEO . ... .. .. ..... .. .... 25 Appendix I .. .... ................. .. .. .. ... ... 27 Appendix II ... ...... ........... .. ..... ..... .. 28 Appendix III .. .. ................... ... .. 29 ii FOREWORD Not long after the Military Air Transport Service received its air drop mission in the mid-1950s, MATS senior commanders speculated that the importance of the new airdrop mission might be enhanced through a tactical training competition conducted on a recurring basis. Their idea came to fruition in 1962 when MATS held its first airdrop training competition. For the next several years the competition remained an annual event, but it fell by the wayside during the years of the United States' most intense participation in the Southeast Asia conflict. The airdrop competitions were reinstated in 1969 but were halted again in 1973, because of budget cuts and the reduced emphasis being given to airdrop operations. However, the esprit de corps engendered among the troops and the training benefits derived from the earlier events were not forgotten and prompted the competition's renewal in 1979 in its present form. Since 1979 the Rodeos have remained an important training event and tactical evaluation exercise for the Military Airlift Command. The following historical study deals with the origins, evolution, and results of the tactical airlift competitions in MATS and MAC. -
The Future of Amateur Radio Satellites in the Cubesat
The Future of Amateur Radio Satellites in the CubeSat Era The Radio Amateur Satellite Corporation (AMSAT) seeks to place an ongoing series of 3U or 6U satellites into highly elliptical orbits to provide long duration communications service to the worldwide amateur radio community. AMSAT's technical challenges in preparing a HEO satellite mission are very similar to what is required for Lunar or Interplanetary CubeSat missions, including harsh thermal and radiation environments, little or no magnetic field to torque against, and challenging communications links, which make this mission very different from the many LEO CubeSats that have been built and launched by other organizations. AMSAT is seeking partnerships with other organizations to demonstrate new technologies in High Earth Orbit, to carry low cost scientific instruments into HEO and to qualify for NASA sponsored launches into Geosynchronous Transfer Orbit or other high altitude orbits whenever such an opportunity occurs. Radio Amateurs have been building and launching small satellites for over 50 years. OSCAR-1 was launched on December 12, 1961 as a secondary payload on the Thor- Agena rocket that launched the US Air Force Discoverer-36 mission. OSCAR-1 was the first satellite to be deployed as a secondary payload from a launch vehicle. The bureaucratic efforts required to secure permission to launch OSCAR-1 greatly exceeded the effort required to build the satellite and established a precedent for all subsequent secondary payload launches of the past five decades. OSCAR stands for “Orbiting Satellite Carrying Amateur Radio”. Today many agencies, laboratories, universities and high schools are building and launching dozens of small satellites every year, but it all started with OSCAR-1 in 1961. -
Galileo FOC-M7 SAT 19-20-21-22
LAUNCH KIT December 2017 VA240 Galileo FOC-M7 SAT 19-20-21-22 VA240 Galileo FOC-M7 SAT 19-20-21-22 ARIANESPACE’S SECOND ARIANE 5 LAUNCH FOR THE GALILEO CONSTELLATION AND EUROPE For its 11th launch of the year, and the sixth Ariane 5 liftoff from the Guiana Space Center (CSG) in French Guiana during 2017, Arianespace will orbit four more satellites for the Galileo constellation. This mission is being performed on behalf of the European Commission under a contract with the European Space Agency (ESA). For the second time, an Ariane 5 ES version will be used to orbit satellites in Europe’s own satellite navigation system. At the completion of this flight, designated Flight VA240 in Arianespace’s launcher family numbering system, 22 Galileo spacecraft will have been launched by Arianespace. Arianespace is proud to deploy its entire family of launch vehicles to address Europe’s needs and guarantee its independent access to space. Galileo, an iconic European program Galileo is Europe’s own global navigation satellite system. Under civilian control, Galileo offers guaranteed high-precision positioning around the world. Its initial services began in December CONTENTS 2016, allowing users equipped with Galileo-enabled devices to combine Galileo and GPS data for better positioning accuracy. The complete Galileo constellation will comprise a total of 24 operational satellites (along with > THE LAUNCH spares); 18 of these satellites already have been orbited by Arianespace. ESA transferred formal responsibility for oversight of Galileo in-orbit operations to the GSA VA240 mission (European GNSS Agency) in July 2017. Page 3 Therefore, as of this launch, the GSA will be in charge of the operation of the Galileo satellite Galileo FOC-M7 satellites navigation systems on behalf of the European Union. -
The EXOD Search for Faint Transients in XMM-Newton Observations
UvA-DARE (Digital Academic Repository) The EXOD search for faint transients in XMM-Newton observations Method and discovery of four extragalactic Type I X-ray bursters Pastor-Marazuela, I.; Webb, N.A.; Wojtowicz, D.T.; van Leeuwen, J. DOI 10.1051/0004-6361/201936869 Publication date 2020 Document Version Final published version Published in Astronomy & Astrophysics Link to publication Citation for published version (APA): Pastor-Marazuela, I., Webb, N. A., Wojtowicz, D. T., & van Leeuwen, J. (2020). The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters. Astronomy & Astrophysics, 640, [A124]. https://doi.org/10.1051/0004-6361/201936869 General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:02 Oct 2021 A&A 640, A124 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936869 & c ESO 2020 Astrophysics The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters I. -
Sentinel-2 and Sentinel-3 Mission Overview and Status
Sentinel-2 and Sentinel-3 Mission Overview and Status Craig Donlon – Sentinel-3 Mission Scientist and Ferran Gascon – Sentinel-2 QC manager and others @ESA IOCCG-21, Santa Monica, USA 1-3rd March 2016 Overview – What is Copernicus? – Sentinel-2 mission and status – Sentinel-3 mission and status Sentinel-3A OLCI first light Svalbard: 29 Feb 14:07:45-14:09:45 UTC Bands 4, 6 and 7 (of 21) at 490, 560, 620 nm Spain and Gibraltar 1 March 10:32:48-10:34:48 UTC California USA 29 Feb 17:44:54-17:46:54 UTC What is Copernicus? Space Component In-Situ Services A European Data Component response to global needs 6 What is Copernicus? – Space in Action for You! • A source of information for policymakers, industry, scientists, business and the public • A European response to global issues: • manage the environment; • understand and to mitigate the effects of climate change; • ensure civil security • A user-driven programme of services for environment and security • An integrated Earth Observation system (combining space-based and in-situ data with Earth System Models) Components & Competences Coordinators: Partners: Private Space Industries companies Component National Space Agencies Overall Programme EMCWF EMSA Mercator snd Ocean Coordination FRONTEX Service Services operators Component EUSC EEA JRC In-situ data are supporting the Space and Services Components Copernicus Funding Funding for Development Funding for Operational Phase until 2013 (c.e.c.): Phase as from 2014 (c.e.c.): ~€ 3.7 B (from ESA and € 4.3 B for the EU) whole programme (from EU) -
The Navy Navigation Satellite System (Transit)
ROBERT J. DANCHIK THE NAVY NAVIGATION SATELLITE SYSTEM (TRANSIT) This article provides an update on the status of the Navy Navigation Satellite System (TRANSIT). Some insights are provided on the evolution of the system into its current configuration, as well as a discussion of future plans. BACKGROUND sign goal was never achieved for long in those early In 1958, research scientists at APL solved the orbit days because the satellites had short operational life of the first Russian satellite, Sputnik-I, by analysis of times. The failures largely resulted from inadequate the observed Doppler shift of its transmitted signal. component quality and the large number of wiring in This led immediately to the concept of satellite navi terconnections. However, after OSCAR 2 10 and OS gation and the development of the U.S. Navy Navi CAR 12 were launched in 1966 and 1967, respectively, gation Satellite System (TRANSIT) by APL, under the enough data on the failure mechanisms became avail sponsorship of the Navy's Special Projects Office, to able to APL to achieve the desired advances in reli provide position fixes for the Fleet Ballistic Missile ability. The integrated circuit introduced in OSCAR Weapon System submarines. (The articles in Ref. 1, 10 significantly extended the satellite lifetime by im a previous issue of the fohns Hopkins APL Techni proving component reliability and reducing the num cal Digest devoted to TRANSIT, give the principles ber of interconnections. Subsequently, the last major of operation and early history of the system.) Now, design change made to the solar cell interconnections, 26 years after its conception, the system is mature. -
Ground Truth: Corona Landmarks Ground Truth: Corona Landmarks an Introduction
CULTURAL An Exhibition by Julie Anand PROGRAMS OF and Damon Sauer THE NATIONAL Sept. 24, 2018 – Feb. 22, 2019 ACADEMY OF NAS Building, Upstairs Gallery SCIENCES 2101 Constitution Ave., N.W. Ground Truth: Corona Landmarks Ground Truth: Corona Landmarks An Introduction In this series of images of what remains of the Corona project, Julie Anand and Damon Sauer investigate our relationship to the vast networks of information that encircle the globe. The Corona project was a CIA and U.S. Air Force surveillance initiative that began in 1959 and ended in 1972. It involved using cameras on satellites to take aerial photographs of the Soviet Union and China. The cameras were calibrated with concrete targets on the ground that are 60 feet in diameter, which provided a reference for scale and ensured images were in focus. Approximately 273 of these concrete targets were placed on a 16-square-mile grid in the Arizona des- ert, spaced a mile apart. Long after Corona’s end and its declassification in 1995, around 180 remain, and Anand and Sauer have spent three years photographing them as part of an ongoing project. In their images, each concrete target is overpowered by an expansive sky, onto which the artists map the paths of orbiting satellites that were present at the Calibration Mark AG49 with Satellites moment the photograph was taken. For Anand and 2016 Sauer, “these markers of space have become archival pigment print markers of time, representing a poignant moment 55 x 44 inches in geopolitical and technologic social history.” A few of the calibration markers like this one are made primarily of rock rather than concrete. -
IAC-18-B2.1.7 Page 1 of 16 a Technical Comparison of Three
A Technical Comparison of Three Low Earth Orbit Satellite Constellation Systems to Provide Global Broadband Inigo del Portilloa,*, Bruce G. Cameronb, Edward F. Crawleyc a Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge 02139, USA, [email protected] b Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge 02139, USA, [email protected] c Department of Aeronautics and Astronautics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge 02139, USA, [email protected] * Corresponding Author Abstract The idea of providing Internet access from space has made a strong comeback in recent years. After a relatively quiet period following the setbacks suffered by the projects proposed in the 90’s, a new wave of proposals for large constellations of low Earth orbit (LEO) satellites to provide global broadband access emerged between 2014 and 2016. Compared to their predecessors, the main differences of these systems are: increased performance that results from the use of digital communication payloads, advanced modulation schemes, multi-beam antennas, and more sophisticated frequency reuse schemes, as well as the cost reductions from advanced manufacturing processes (such as assembly line, highly automated, and continuous testing) and reduced launch costs. This paper compares three such large LEO satellite constellations, namely SpaceX’s 4,425 satellites Ku-Ka-band system, OneWeb’s 720 satellites Ku-Ka-band system, and Telesat’s 117 satellites Ka-band system. First, we present the system architecture of each of the constellations (as described in their respective FCC filings as of September 2018), highlighting the similarities and differences amongst the three systems. -
Corona KH-4B Satellites
Corona KH-4B Satellites The Corona reconnaissance satellites, developed in the immediate aftermath of SPUTNIK, are arguably the most important space vehicles ever flown, and that comparison includes the Apollo spacecraft missions to the moon. The ingenuity and elegance of the Corona satellite design is remarkable even by current standards, and the quality of its panchromatic imagery in 1967 was almost as good as US commercial imaging satellites in 1999. Yet, while the moon missions were highly publicized and praised, the CORONA project was hidden from view; that is until February 1995, when President Clinton issued an executive order declassifying the project, making the design details, the operational description, and the imagery available to the public. The National Reconnaissance Office (NRO) has a web site that describes the project, and the hardware is on display in the National Air and Space Museum. Between 1960 and 1972, Corona satellites flew 94 successful missions providing overhead reconnaissance of the Soviet Union, China and other denied areas. The imagery debunked the bomber and missile gaps, and gave the US a factual basis for strategic assessments. It also provided reliable mapping data. The Soviet Union had previously “doctored” their maps to render them useless as targeting aids and Corona largely solved this problem. The Corona satellites employed film, which was returned to Earth in a capsule. This was not an obvious choice for reconnaissance. Studies first favored television video with magnetic storage of images and radio downlink when over a receiving ground station. Placed in an orbit high enough to minimize the effects of atmospheric drag, a satellite could operate for a year, sending images to Earth on a timely basis.