0830-Zvedre RUSSIA in SPACE 2008
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GLONASS System As a Tool for Space Weather Monitoring
GLONASS System as a tool for space weather monitoring V.V. Alpatov, S.N. Karutin, А.Yu. Repin Institute of Applied Geophysics, Roshydromet TSNIIMASH, Roscosmos BAKU-2018 PLAN OF PRESENTATION General information about GLONASS Goals Organization and Management Technical information about GLONASS Space Weather Effects On Space Systems On Ground based Systems Possible Opportunities of GLONASS for Monitoring Space Weather Effects Russian Monitoring System for Monitoring Space Weather Effects with Use Opportunities of GLONASS 2 GENERAL INFORMATION ABOUT GLONASS NATIONAL SATELLITE NAVIGATION POLICY AND ORGANIZATION Presidential Decree of May 17, 2007 No. 638 On Use of GLONASS (Global Navigation Satellite System) for the Benefit of Social and Economic Development of the Russian Federation Federal Program on GLONASS Sustainment, Development and Use for 2012-2020 – planning and budgeting instrument for GLONASS development and use Budget planning for the forthcoming decade – up to 2030 GLONASS Program governance: Roscosmos State Space Corporation Government Contracting Authority – Program Coordinator Government Contracting Authorities Program Scientific and Coordination Board GLONASS Program Goals: Improving GLONASS performance – its accuracy and integrity Ensuring positioning, navigation and timing solutions in restricted visibility of satellites, interference and jamming conditions Enhancing current application efficiency and broadening application domains 3 CHARACTERISTICS IMPROVEMENT PLAN Accuracy Improvement by means of: . Ground Segment -
GLONASS Interface Control Document Specifies Parameters of Interface Between GLONASS Space Segment and User Equipment
GLOBALNAVIGATION SATELLITE SYSTEM GLONASS TION CENTER INTERFACE CONTROL DOCUMENT COORDINATION SCIENTIFIC INFORMA MOSCOW 1998ã. Version 4.0 1998 GLONASS ICD COORDINATION SCIENTIFIC INFORMATION CENTER TABLE OF CONTENTS FIGURES................................................................................................................................................................... 2 TABLES .................................................................................................................................................................... 3 ABBREVIATIONS.................................................................................................................................................... 4 1. INTRODUCTION ................................................................................................................................................. 5 1.1 GLONASS PURPOSE.......................................................................................................................................... 5 1.2 GLONASS COMPONENTS .................................................................................................................................. 5 1.3 NAVIGATION DETERMINATION CONCEPT ............................................................................................................. 5 2. GENERAL............................................................................................................................................................. 6 2.1 ICD DEFINITION ............................................................................................................................................... -
Report of the Commission on the Scientific Case for Human Space Exploration
1 ROYAL ASTRONOMICAL SOCIETY Burlington House, Piccadilly London W1J 0BQ, UK T: 020 7734 4582/ 3307 F: 020 7494 0166 [email protected] www.ras.org.uk Registered Charity 226545 Report of the Commission on the Scientific Case for Human Space Exploration Professor Frank Close, OBE Dr John Dudeney, OBE Professor Ken Pounds, CBE FRS 2 Contents (A) Executive Summary 3 (B) The Formation and Membership of the Commission 6 (C) The Terms of Reference 7 (D) Summary of the activities/meetings of the Commission 8 (E) The need for a wider context 8 (E1) The Wider Science Context (E2) Public inspiration, outreach and educational Context (E3) The Commercial/Industrial context (E4) The Political and International context. (F) Planetary Science on the Moon & Mars 13 (G) Astronomy from the Moon 15 (H) Human or Robotic Explorers 15 (I) Costs and Funding issues 19 (J) The Technological Challenge 20 (J1) Launcher Capabilities (J2) Radiation (K) Summary 23 (L) Acknowledgements 23 (M) Appendices: Appendix 1 Expert witnesses consulted & contributions received 24 Appendix 2 Poll of UK Astronomers 25 Appendix 3 Poll of Public Attitudes 26 Appendix 4 Selected Web Sites 27 3 (A) Executive Summary 1. Scientific missions to the Moon and Mars will address questions of profound interest to the human race. These include: the origins and history of the solar system; whether life is unique to Earth; and how life on Earth began. If our close neighbour, Mars, is found to be devoid of life, important lessons may be learned regarding the future of our own planet. 2. While the exploration of the Moon and Mars can and is being addressed by unmanned missions we have concluded that the capabilities of robotic spacecraft will fall well short of those of human explorers for the foreseeable future. -
Forthcoming Changes in the Global Satellite Observing Systems Mitch Goldberg, NOAA Outline
Forthcoming changes in the Global Satellite Observing Systems Mitch Goldberg, NOAA Outline Overview of CGMS and CEOS. Overview of the key satellite observations for NWP Discuss satellite agencies plans for these key observations Short overview emerging observations or technology which we need to pay attention to. Summary Members: CMA CNES CNSA ESA EUMETSAT IMD IOC/UNESCO JAXA JMA KMA NASA ROSCOSMOS ROSHYRDOMET WMO Observers: CSA EC ISRO KARI KORDI SOA Strategy for addressing key satellite data Begin with WIGOS 5th Workshop of the Impact of Various Observing Systems on NWP (Sedona Report). UKMO impact report: Impact of Metop and other satellite data within the Met Office global NWP system using a forecast adjoint-based sensitivity method- Feb 2012, tech repot #562 and MWR October 2013 paper Recall key observation types for NWP Compare with what space agencies are planning to provide continuity and enhancements to these observing types. Make use of the WMO OSCAR database Time scale between now and 2030. Sedona Report Observations contributing to the largest reduction of forecast errors are those observations with vertical information (temperature, water vapor). The single instrument with the largest impact is hyperspectral IR Microwave dominates because of the number of satellites and ability to view thru low water content clouds. However, there is now no single, dominating satellite sensor. GPSRO shows good impact, and largest impact per observation Atmospheric Motion Vector Winds and Scatterometers are single level data and have modest impacts Concerns about the declining number of observations into the future – mostly due to the replacement of 2 year life satellites with 7 years (e.g. -
Russia's Posture in Space
Russia’s Posture in Space: Prospects for Europe Executive Summary Prepared by the European Space Policy Institute Marco ALIBERTI Ksenia LISITSYNA May 2018 Table of Contents Background and Research Objectives ........................................................................................ 1 Domestic Developments in Russia’s Space Programme ............................................................ 2 Russia’s International Space Posture ......................................................................................... 4 Prospects for Europe .................................................................................................................. 5 Background and Research Objectives For the 50th anniversary of the launch of Sputnik-1, in 2007, the rebirth of Russian space activities appeared well on its way. After the decade-long crisis of the 1990s, the country’s political leadership guided by President Putin gave new impetus to the development of national space activities and put the sector back among the top priorities of Moscow’s domestic and foreign policy agenda. Supported by the progressive recovery of Russia’s economy, renewed political stability, and an improving external environment, Russia re-asserted strong ambitions and the resolve to regain its original position on the international scene. Towards this, several major space programmes were adopted, including the Federal Space Programme 2006-2015, the Federal Target Programme on the development of Russian cosmodromes, and the Federal Target Programme on the redeployment of GLONASS. This renewed commitment to the development of space activities was duly reflected in a sharp increase in the country’s launch rate and space budget throughout the decade. Thanks to the funds made available by flourishing energy exports, Russia’s space expenditure continued to grow even in the midst of the global financial crisis. Besides new programmes and increased funding, the spectrum of activities was also widened to encompass a new focus on space applications and commercial products. -
Venona Special Studies
- 1 - Venona Project Special Studies Transcribed by Students of the Mercyhurst College Institute for Intelligence Studies Arranged by John Earl Haynes, Library of Congress, 2010 COVER NAMES IN NEW YORK TRAFFIC p. 2 UNIDENTIFIED COVER NAMES IN NEW YORK TRAFFIC p. 86 COVER NAMES IN SAN FRANCISCO TRAFFIC p. 92 COVER NAMES IN WASHINGTON TRAFFIC p. 123 ADDITIONAL COVERNAMES AND RELATED INFORMATION IN DIPLOMATIC TRAFFIC p. 127 REVISED TRANSLATION OF MESSAGE ON ANTENNA-LIBERAL'S WIFE ETHEL p. 135 THE COVERNAMES "ANTENNA" AND "LIBERAL" IN . MESSAGES p. 139 ESSAGES IN . INVOLVING THE COVERNAME"ENORMOZ" AND THE NAMES OF NUCLEAR PHYSICISTS, ETC. p. 147 UNDATED REPORT OF MEREDITH GARDNER p. 155 DEVELOPMENT OF THE “G--“HOMER” [“GOMER”] CASE p. 158 THE KOMAR (KRAVCHENKO) AFFAIR IN . MESSAGES p. 161 REVISED TRANSLATION OF TWO . MESSAGES ON CHANGES IN COVERNAMES p. 170 THE COVERNAME "KARAS" IN. TRAFFIC p. 178 THE COVERNAMES "TÉNOR", "BAS", AND "CHETÁ" (? IN . TRAFFIC p. 181 - 2 - Special Study Cover Names in New York Traffic - 3 - cover-name Message number Date Publication reference S/ or 3/NBF/ 19 N.Y. to M. 812 29053 JKI 06 T1022 1B-1910 0027A ABRAM N.Y. to M. 992 24063 JKR 14 T872√ 1B-7518 0005A JACK SOBLE 1086 06073 JKV 48 T873√ 2A-0011 1957 29113 NNNNNN T939√ 625 04054 JHD 48 T916√ 851 15064 JIJ 40 T10.1√ 1146 10084 JHM 41 T123√ 1251 02094 JHN 12 T301√ (to ChEKh) 0005B 1353 23094 JHO 42 T289√ 1449 12104 JIL 37 T106√ 1754 14124 JHZ 49 T6√ 48 11015 JHV 37 (NSA)T1941 AVGUR 2A-0013 1638 (AUGUR) N.Y. -
Fred Mistichelli NESDIS Spectrum Manager Rich Kelley Alion Science
WRC-19 Fred Mistichelli Geneva NESDIS Spectrum Manager 28 October to 22 November 2019 Rich Kelley Alion Science for NESDIS 29 Nov – 5 Dec 2017 o discusses spectrum concerns faced by ITSC membership between now and 2019. o covers WRC- 19 agenda items of concern in passive bands and one major new active downlink o describes rfi detection and suppression methods Satellites and agencies possibly affected by WRC-19 decisions Satellite agency Satellite agency Aqua NASA Meteor-M N2 RosHydroMet Coriolis DoD Meteor-M N2-1 RosHydroMet DWSS-1 DoD Meteor-M N2-2 RosHydroMet DWSS-2 DoD Meteor-M N2-3 RosHydroMet FY-3B CMA Meteor-M N2-4 RosHydroMet FY-3C CMA Meteor-M N2-5 RosHydroMet FY-3D CMA Meteor-MP N1 RosHydroMet FY-3E CMA Meteor-MP N2 RosHydroMet FY-3F CMA Metop-A EUMETSAT FY-3G CMA Metop-B EUMETSAT FY-3H CMA Metop-C EUMETSAT FY-3RM-1 CMA Metop-SG-A1 EUMETSAT FY-3RM-2 CMA Metop-SG-A2 EUMETSAT GCOM-W1 JAXA Metop-SG-A3 EUMETSAT GPM Core Observatory NASA Metop-SG-B1 EUMETSAT HY-2A NSOAS Metop-SG-B2 EUMETSAT JPSS-1 NOAA Metop-SG-B3 EUMETSAT JPSS-2 NOAA NOAA-15 NOAA JPSS-3 NOAA NOAA-18 NOAA JPSS-4 NOAA NOAA-19 NOAA Megha-Tropiques ISRO SNPP NOAA [1] National Ocean Satellite Application Center (China) Agenda item spectrum addressed 1.5 17.7-19.7 GHz (space-to-Earth) and 27.5-29.5 GHz (Earth-to-space) 1.6 37.5-39.5 GHz (space-to-Earth), 39.5-42.5 GHz (space-to-Earth), 47.2-50.2 GHz (Earth-to-space) and 50.4-51.4 GHz (Earth-to-space) 1.7 spectrum requirements for telemetry, tracking and command in the space operation service for the growing number of non-GSO satellites with short duration missions (small satellites/microsats/picosats) 1.13 24.25-27.5 GHz (data downlink for JPSS/MetOp) 31.8-33.4 GHz 37-40.5 GHz 47.2-50.2 GHz (passive use only) 50.4-52.6 GHz (passive use only) 81-86 GHz 1.14 regulatory actions for high-altitude platform stations (HAPS), within existing fixed-service allocations Issue 9.1.9 51.4-52.4 GHz n.b.The WMO position paper on WRC 19 agenda items is at (http://wis.wmo.int/file=3379). -
Lunar Life Sciences Payload Assessment
Lunar Surface Science Workshop 2020 (LPI Contrib. No. 2241) 5077.pdf LUNAR LIFE SCIENCES PAYLOAD ASSESSMENT. S. C. Sun1, F. Karouia2, M. P. Lera3, M. P. Parra1, H. E. Ray4, A. J. Ricco1, S. M. Spremo1. 1NASA Ames Research Center, 2Blue Marble Space Institute of Science, 3KBR, 4ASRC Federal Space and Defense, Inc. Introduction: The Moon provides a unique site to ISS, including systems that integrate into EXPRESS study living organisms. The fractional gravity and (EXpedite the PRocessing of ExperimentS for Space) unique radiation environment have similarities to Mars Racks or are external space exposure research facilities. and will help us understand how life will respond to These same systems can be the basis for future payload conditions on the red planet. Martian and lunar envi- systems for experiments to be performed beyond Low ronments can be simulated on the ground but not to high Earth Orbit. Such facilities would need to be adapted to fidelity. Altered gravity and increased radiation are dif- be compatible with the new research platforms and ficult to replicate simultaneously, which makes study- function in the harsher radiation environment found out- ing their combined effect difficult. The International side the magnetosphere. If Gateway and a lunar based- Space Station, and previously, the Space Shuttle, pro- lab could provide EXPRESS-compatible interfaces, lev- vided a microgravity environment, and could simulate eraging hardware developed for ISS would be more fea- fractional-g only via an onboard centrifuge. Because sible. the ISS and Space Shuttle orbits were within the Earth’s Gaps in Capabilities: Many of the payload systems magnetosphere, experiments on those platforms have that have been developed require human tending. -
GLONASS Spacecraft
INNO V AT IO N The task of designing and developing the GLONASS GLONASS spacecraft fell to the Scientific Production Association of Applied Mechan ics (Nauchno Proizvodstvennoe Ob"edinenie Spacecraft Prikladnoi Mekaniki or NPO PM) , located near Krasnoyarsk in Siberia. This major aero Nicholas L. Johnson space industrial complex was established in 1959 as a division of Sergei Korolev 's Kaman Sciences Corporation Expe1imental Design Bureau (Opytno Kon struktorskoe Byuro or OKB). (Korolev , among other notable achievements , led the Fourteen years after the launch of the effort to develop the Soviet Union's first first test spacecraft, the Russian Global Nav launch vehicle - the A launcher - which igation Satellite System (Global 'naya Navi placed Sputnik 1 into orbit.) The founding gatsionnaya Sputnikovaya Sistema or and current general director and chief GLONASS) program remains viable and designer is Mikhail Fyodorovich Reshetnev, essentially on schedule despite the economic one of only two still-active chief designers and political turmoil surrounding the final from Russia's fledgling 1950s-era space years of the Soviet Union and the emergence program. of the Commonwealth of Independent States A closed facility until the early 1990s, (CIS). By the summer of 1994, a total of 53 NPO PM has been responsible for all major GLONASS spacecraft had been successfully Russian operational communications, navi Despite the significant economic hardships deployed in nearly semisynchronous orbits; gation, and geodetic satellite systems to associated with the breakup of the Soviet Union of the 53 , nearly 12 had been normally oper date. Serial (or assembly-line) production of and the transition to a modern market economy, ational since the establishment of the Phase I some spacecraft, including Tsikada and Russia continues to develop its space programs, constellation in 1990. -
2012 BMW Cospas-Sarat Updates Secretariat
2012 Beacon Manufacturers’ Workshop Orlando, Florida 28 September 2012 Cospas-Sarsat Updates Dany St-Pierre Cospas-SSSarsat Secretar iat 0 Source: CNES – D. Ducros Cospas-Sarsat Updates • Intern ati on al Cospas-Sarsat Pr ogr amm e • Space Segment and LUTs status • Saves and Events • MEOSAR System and status • IBRD and Website Updates • Upcoming Events and Activities Cospas-Sarsat Mission and Objective Mission: To provide accurate, timely and reliable distress alert and location data to help SAR authorities assist persons in distress. Objective: To reduce, as far as possible, delays in the provision of distress alerts to SAR and the time to locate a distress and provide assistance. Strategy: To implement, maintain, co-ordinate and operate a satellite system capable of detecting tiitransmissions from radio-beacons tha t complywith C/S specifications. Cospas-Sarsat Participants Netherlands New Algeria Zealand Argentina Nigeria Australia Norway Brazil Pakistan Canada Peru Chile Poland China (P.R.) Russia Cyprus Saudi Denmark Arabia Finland Serbia France Singapore Germany South Africa Greece Spain Hong Kong Sweden India Switzerland Indonesia Thailand Italy Tunisia ITDC Turkey Japan UAE Korea (R. of) UK 4 Founders: Canada, France, Russia and the USA Madagascar USA • 60 % of world land area Vietnam 26 GdStPidGround Segment Providers • 72 % of world population 11 User States 2 Organisations • 84 % of estimated world wealth Cospas-Sarsat System Combined LEO / GEO Operations • LEOSAR: Sarsat (NOAA, MetOp) and Cospas • GEOSAR: GOES (USA), INSAT -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
NASA Ames to Establish Nationwide Lunar Science Institute
November 2007 Worden gives upbeat message about future work for Ames BY JOHN BLUCK "We have switched material to In an upbeat talk to a crowd that phenolic impregnated carbon abla- filled the Ames main auditorium, tor (PICA), a (heat shield) material Ames Center Director S. Pete Worden developed here," Worden noted. His outlined an exciting future at Ames projected slide also listed Ames as that includes new work in exploration, leading PICA development and test- science and aeronautics -- each about a ing both for the Crew Exploration Ve- third of the center's efforts, he said. "I hicle, now called Orion, and the Mars have a gazillion charts to go through," Science Laboratory (MSL), which has photo by Eric James NASA he said. a planned launch date in fall 2009. His wide-ranging presentation Worden said that Ames' arc jets about Ames touched on moon explo- facility "a unique facility in the world." ration, a lunar institute, moon dust re- He added, "We want to upgrade search, heat shield work for spacecraft them." destined for the moon and Mars, a Mars sample "cache box" assignment, Life Sciences rising supercomputer capability, small "We are getting additional life Ames Center Director S. Pete Worden responds satellite work with a potential for support tasks assigned by Johnson to a question during the recent upbeat talk he many missions, increased astrobiology (and Marshall)," Worden said. "This is gave to the center about the future of Ames. work, growing cooperation among significant." continued on page 5 academia, and commercial partners and Ames and much more.