Austria from Space

Total Page:16

File Type:pdf, Size:1020Kb

Austria from Space « Why do we invest in Space » Dr. Volker Liebig Director of Earth Observation Programmes, ESA SPACE DAY Vienna 27th March 2007 http://www.esa.int 10/2006 - 1 Austria from space http://www.esa.int 10/2006 - 2 1 The European Space Agency The idea of an independent European space agency dates back to the early 1960’s. ESA was formed in 1975, replacing the satellite and launcher organisations ESRO and ELDO. Today ESA has 17 Member States. http://www.esa.int 10/2006 - 3 ESA Member States ESA has 17 Member States : • Austria, Belgium, Denmark, Finland, France, Germany, Greece, Ireland, Italy, Luxembourg, Norway, the Netherlands, Portugal, Spain, Sweden, Switzerland and the United Kingdom • Hungary, the Czech Republic and Romania are European Cooperating States • Canada takes part in some projects under a cooperation agreement 1987 http://www.esa.int 10/2006 - 4 2 An inter-governmental organisation The purpose with a mission to provide and promote - for exclusively peaceful purposes - of ESA the exploitation of: • Space science, research & technology • Space applications. ESA achieves this through: • Space activities and programmes • Long term space policy • A specific industrial policy • Coordinating European with national space programmes. http://www.esa.int 10/2006 - 5 All Member States participate in activities and a common set of programmes related to Space Science (mandatory programmes). In addition, members chose the level of participation in so called optional programmes: Human space flight Microgravity research Earth observation Telecommunications Satellite navigation Launcher development http://www.esa.int 10/200610/2004 - 4- 6 3 ESTEC - Noordwijk, the European Space Research and ESA headquarters Technology Centre and establishments Staff - 1074 EAC - Cologne, Germany HEADQUARTERS - Paris, France European Astronaut Centre ESA headquarters houses the Director Staff - 16 General’s office, general administration and the main programme directorates. ESOC -Darmstadt, Germany Staff - 367 (including Brussels, Kourou European Space Operations liaison, Moscow, Toulouse, Washington Centre offices). Staff – 251 (including Houston Office) ESRIN - Frascati, European Space Research Institute Staff - 174 ESAC - Villafranca, European Staff in post at 28/02/07, total: 1894 Space Astronomy Centre Staff - 12 http://www.esa.int 10/2006 - 7 ESA is responsible for research The birth of and development of space projects. commercial operators • On completion of qualification, these projects are handed over to outside bodies for the production/exploitation phase. Operational systems are transferred to new or specially established organisations: • Launchers: Arianespace - launcher production phase and launch operations • Telecommunications: Eutelsat & Inmarsat - international communications services via ECS/MARECS • Meteorology: Eumetsat - Meteosat weather satellites, Metop • Satellite Navigation: Galileo Supervisory Authority – GSA (E.U. Agency) http://www.esa.int 10/2006 - 8 4 For over 30 years ESA's space science Space projects have shown the scientific Science benefits of multi-nation cooperation. Areas covered by ESA: • Space environment of the Earth • Solar-terrestrial interaction • Interplanetary medium • Moon, planets and other objects • Stars and the universe • Fundamental Physics http://www.esa.int 10/2006 - 9 Science missions of today (excerpt) • Ulysses (1990-...) - (with NASA) heliospheric studies • Cassini-Huygens (1997-2005-...) to Saturn & Titan • Newton (XMM) (1999-...) Multi Mirror mission • Cluster 2 (2000-...) Earth’s magnetosphere • Mars Express (2003-...) to Mars • SMART-1 (2003-2006) to the Moon • Rosetta (2004-...) to comet First image of Titan’s surface Churyumov-Gerasimenko • Venus Express (2005-...) to Venus http://www.esa.int 10/2006 - 10 5 Hubble Cluster 2 Cassini / Ulysses Huygens Soho Newton (XMM) http://www.esa.int 10/2006 - 11 Planet Mars (Mars Express) Titan (Cassini-Huygens) http://www.esa.int 10/2006 - 12 6 Spacecraft / Satellites Examples of Austrian competences Austrian Aerospace, SIEMENS, Magna Steyr: development of space-qualified hardware and software, technology transfer ¾ e.g. satellite on-board electronics & mechanics, thermal hardware, ground support equipment ¾ mission control S/W, sat communication, etc. Aerosol Collector and Pyrolyser (APC) experiment onboard Huygens GCS, Plansee, Joanneum Research, Austrian Research Centres Seibersdorf: aerospace technologies, space propulsion, space applications, communication & navigation http://www.esa.int 10/2006 - 13 Space Science & Exploration Examples of Austrian involvement The Cassini-Huygens mission as example of Austrian High-Tech: electronics for the ACP instrument, swivel mechanism, thermal insulation, electric and mechanic ground equipment Institut für Weltraumforschung, Austrian Academy of Sciences: experimental space research, extraterrestrial physics, satellite geodesy – involvement i.a. with Cluster, BepiColombo, Venus Express, Huygens, Rosetta, GOCE, Mars Express, etc. http://www.esa.int 10/2006 - 14 7 International Elements of European contribution • Development & operation of flight elements Space Station and associated ground infrastructure: - Columbus Laboratory - Automated Transport Vehicle (ATV) • Development and delivery of hardware and software to partners: Node 2, Node 3, Data Management System for the Russian Service Module (Zvezda), European Robotic Arm, Cupola, and other elements • Development of multi-user experiment facilities on ISS, in the framework of the Microgravity Facilities for Columbus programme • Preparation for the operation & utilisation of ISS; Preparation for astronaut activities on ISS http://www.esa.int 10/2006 - 15 http://www.esa.int 10/2006 - 16 8 AURORA: human & robotic exploration A long-term plan for exploration activities: • Preparation of enabling technologies and infrastructures as well as preparation / demonstration of core capabilities needed for next step in space exploration • European participation in a human space transportation programme (CSTS – Crew Space Transportation System) • Participation to moon orbit and/or moon surface infrastructure or other exploration missions • A new mission to Mars with a launch planned in 2020 http://www.esa.int 10/2006 - 17 Earth Observation: from understanding planet Earth to operational services T h e c h a l l e n g e o f G l o b a l C h a n g e IPCC Report 2007 (1st part): Global temperature increase between + 1.8 and 4.0 deg. until 2100 Arctic: ice-free as of 2nd half of the century Sea level rise: up to 48cm until 2100 Permafrost: up to 90% melting until 2100, freeing high amounts of Methane gas Precipitation: decrease in arid regions and increase in wet areas Storms and surges: less in number but significantly stronger in intensity Gulf Stream: significantly weakened http://www.esa.int 10/2006 - 18 9 Envisat Envisat celebrated 5th year in space on 28 February, fulfilling its expected lifetime, and expected to operate until 2010 280 GB of data products generated per day, 78 types of data products available, more than 1200 projects currently served http://www.esa.int 10/2006 - 19 Major scientific results of ENVISAT and ERS Climate change: Global sea level rise of ~3mm/year and sea surface temperature increase of ~0.1 deg. C since 1992 (Envisat + ERS). Atmosphere: Worldwide monitoring of air pollution, with evidence of fast growing air pollution in China since 1995 (Envisat + ERS-2). Polar areas: Daily monitoring of sea ice motion and observation of Antarctica ice-shelves collapse. Ozone hole Oceanography: Quantification of global chlorophyll concentration, an index of the oceanic phytoplankton biomass. Tectonics: Identification of the blind tectonic fault at the origin of the Bam earthquake in December 2003. NO2 / SCIAMACHY (Jan. 2003 - June 2004) http://www.esa.int 10/2006 - 20 10 GOCE 7th EE SMOS EARTH CARE ADM AEOLUS SWARM CRYOSAT 2 http://www.esa.int 10/2006 - 21 Long-term operational Earth monitoring Cooperation with EUMETSAT: Meteosat and Metop Meteosat / MSG Metop Since 1978, ESA has Europe’s first polar developed 9 orbiting satellite for Meteosat satellites op. meteorology Launch of Metop-A: 19.10.2006 MSG-2 21.12.2005 http://www.esa.int 10/2006 - 22 11 Global Monitoring European independence in critical data sources for environmental monitoring and security for Environment and the European contribution to the Global Earth Observation System of Systems (GEOSS) Security (GMES) ESA is in charge of the implementation of the GMES Space Component (GSC) The GSC comprises: Development, launch and IOV of the Sentinels Ground Segment Access to EO data for ESA, Eumetsat, Member States’ missions and TPM for GMES services (Fast Track) Development of Sentinel Ground Segment 2007: decision for transition to Phase 2 http://www.esa.int 10/2006 - 23 Earth observation Examples of Austrian involvement GeoVille: market leader for Earth observation applications in spatial planning; Austrian lead organisation in GMES Land GeoSpace: Earth observation applications, public outreach gcs: development of the ENVISAT data dissemination system http://www.esa.int 10/2006 - 24 12 Telecommunications: a commercial success Telecommunications Satellites represent the largest worldwide commercial space market. Key areas of interest to ESA are: • Fixed services • Broadcasting • Mobile communications • Navigation • Data relay • Multimedia http://www.esa.int 10/2006 - 25 • A complete civil satellite navigation system Galileo: satellite developed by ESA and the EU
Recommended publications
  • Meteosat Third Generation (MTG) Lightning Imager (LI) Calibration and 0-1B Data Processing
    Meteosat Third Generation (MTG) Lightning Imager (LI) calibration and 0-1b data processing Marcel Dobber EUMETSAT EUMETSAT-Allee 1, 64295 Darmstadt, Germany; +49-6151-807 7209 [email protected] Stephan Kox EUMETSAT EUMETSAT-Allee 1, 64295 Darmstadt, Germany; +49-6151-807 7248 [email protected] ABSTRACT The European Meteosat Third Generation (MTG) Lightning Imager (LI) is an instrument on the geostationary MTG Imager satellite series, for which the first satellite is scheduled for launch in 2021. The MTG series consists of six satellites in total: Four imager satellites, equipped with the Flexible Combined Imager (FCI) and Lightning Imager (LI) instruments, and two sounding satellites, with the Infrared Sounder (IRS) and Sentinel-4 UVN instruments. EUMETSAT will operate the satellites, instruments and ground facilities for MTG, including LI. The Lightning Imager will continuously provide lightning group and flashes information for almost the complete visible Earth disc from a geostationary orbit around zero degrees longitude in the time period 2021 to 2041. The instrument will measure day and night and will provide detected transient data from lightning optical pulses in the near-infrared at a spatial resolution that corresponds to 4.5 km x 4.5 km at the subsatellite point. The instrument also measures and provides background radiance images every 30 seconds. In this paper the Lightning Imager mission objectives and basic instrument detection principles will be described. In addition, the calibration (on ground and in orbit) and 0-1b data processing will be presented and discussed. at sub-satellite longitude of about 0 degrees, for a 1. SUMMARY geographical coverage area that covers almost the complete visible Earth disc.
    [Show full text]
  • Laser Retroreflectors for Insight and an International Mars Geophysical Network (MGN)
    50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 1492.pdf Laser Retroreflectors for InSight and an International Mars Geophysical Network (MGN). S. Dell’Agnello1, G.O. Delle Monache1, L. Porcelli1,2, M. Tibuzzi1, L. Salvatori1, C. Mondaini1, M. Muccino1, L. Ioppi1, O. Luongo1, M. Petrassi1, G. Bianco1,3, R. Vittori1,4, W.B. Banerdt5, J.F. Grinblat5, C. Benedetto3, F. Pasquali3, R. Mugnuolo3, D.C. Gruel5, J.L.Vago6 and P. Baglioni6. 1Istituto Nazionale di Fisica Nucleare–Laboratori Nazionali di Frascati (INFN–LNF), Via E. Fermi 40, 00044, Frascati, Italy ([email protected]); 2Dipartimento di Fisica, Università della Calabria (UniCal), Via P. Bucci, 87036, Arcavacata di Rende, Italy; 3Agenzia Spaziale Italiana– Centro di Geodesia Spaziale “Giuseppe Colombo” (ASI–CGS), Località, Terlecchia 75100, Matera, Italy; 4Italian Air Force, Rome, Italy, ASI and Embassy of Italy in Washington DC; 5NASA–Jet Propulsion Laboratory (JPL), California Institute of Technology, Pasadena, CA 91109, USA; 6ESA–ESTEC, Noordwijk, The Netherlands. Abstract. There are laser retroreflectors on the Moon, of the INFN-ASI Affiliation-Association to NASA- but there were no laser retroreflectors on Mars until the SSERVI sservi.nasa.gov) is shown in the figure below. NASA InSight mission [1][2] landed and started oper- ating successfully on the surface of the red planet on Nov. 26, 2018. The ESA ExoMars Schiaparelli mis- sion, which unfortunately failed Mars landing in 2016, was carrying a laser retroreflector like InSight [3]. These instruments are positioned by measuring the time-of-flight of short laser pulses, the so-called “laser ranging” technique (for details on satellite/lunar laser ranging and altimetry see https://ilrs.gsfc.nasa.gov).
    [Show full text]
  • Church of the Brethren May Meet Hrre In
    ' ' , s i * Take inventory of your printed” sup­ One word can tell the Btory of con­ plies; If you need anything, the - tinued business activity in the com­ - j ■ ' Times stands ready to give munity—Advertising. vi:;/ you Bervice, • . AND THE SJIOUE TIMES FOUR CENTS /,-;t VOL. LX . No. 33 OCEAN GROVE, NEW JERSEY, FRIDAY, AUGUST 16, 1935 - / ' : $ THOMSON GETS ‘MARTHA" IS BIBLE LESSON HOTEL MEN WANT CHURCH 7,500 HEAR BISHOP MOUZON Mrs. Gertrude Brown To Teach At OF THE BRETHREN RARE SOUVENIRS St; Paul’s MORE PUBLICITY in Au ditoriu m sermons “Martha” is the Bible class les­ MAY MEET HRRE IN 1936 THREE ANNIVERSARY: MEMOS son for .the coming Sundny. Text, WILL REQUEST LARGER BUD­ “Jesus loved! Martha and her sister ARE PRESENTED and! Lazarus,” John,: 11:5: Read GET APPROPRIATION. Preacher Sees Chance For Uniting of Three Luke, 10\38-42 and John, VI '.17-28. National Convention Would Bring Eight Thou­ Sixth Founders’ Day, Stokes Gold­ Dr, Francis Harvey Green will be Appoint Nominating Committee Branches of Methodist Church—Prays For en Wedding and Dr. Ballard’s the teacher 'at the|. Auditorium For Report at September Meet­ sand Delegates for Eight Days—Dr. Hen­ Bible Class,, at" 2.30. .Written Ques­ Birthday Arc Noted In Special ing of Ocean Grove Hotel As­ Kingdom of God and Revival of Hope, tions will be answered at the begin­ son Offers Buildings for Sessions—Ar­ Announcements. ning of theperiod. sociation. Endorse Play-Ground Faith and Love— Gives His Definition of Three precious documents have The Assembly BiblejClhss, which D rive/ rangements Committee Decides Today.
    [Show full text]
  • FAME-C: Cloud Property Retrieval Using Synergistic AATSR and MERIS Observations
    Atmos. Meas. Tech., 7, 3873–3890, 2014 www.atmos-meas-tech.net/7/3873/2014/ doi:10.5194/amt-7-3873-2014 © Author(s) 2014. CC Attribution 3.0 License. FAME-C: cloud property retrieval using synergistic AATSR and MERIS observations C. K. Carbajal Henken, R. Lindstrot, R. Preusker, and J. Fischer Institute for Space Sciences, Freie Universität Berlin (FUB), Berlin, Germany Correspondence to: C. K. Carbajal Henken ([email protected]) Received: 29 April 2014 – Published in Atmos. Meas. Tech. Discuss.: 19 May 2014 Revised: 17 September 2014 – Accepted: 11 October 2014 – Published: 25 November 2014 Abstract. A newly developed daytime cloud property re- trievals. Biases are generally smallest for marine stratocu- trieval algorithm, FAME-C (Freie Universität Berlin AATSR mulus clouds: −0.28, 0.41 µm and −0.18 g m−2 for cloud MERIS Cloud), is presented. Synergistic observations from optical thickness, effective radius and cloud water path, re- the Advanced Along-Track Scanning Radiometer (AATSR) spectively. This is also true for the root-mean-square devia- and the Medium Resolution Imaging Spectrometer (MERIS), tion. Furthermore, both cloud top height products are com- both mounted on the polar-orbiting Environmental Satellite pared to cloud top heights derived from ground-based cloud (Envisat), are used for cloud screening. For cloudy pixels radars located at several Atmospheric Radiation Measure- two main steps are carried out in a sequential form. First, ment (ARM) sites. FAME-C mostly shows an underestima- a cloud optical and microphysical property retrieval is per- tion of cloud top heights when compared to radar observa- formed using an AATSR near-infrared and visible channel.
    [Show full text]
  • The Meteosat System
    THE METEOSAT SYSTEM EUM TD 05 Published by: EUMETSAT (European Organisation for the Exploitation of Meteorological Satellites) ©1998 EUMETSAT Design: Grigat und Neu THE METEOSAT SYSTEM December 1998 TABLE OF CONTENTS PREFACE .............................................................................. 5 Performance monitoring..............................................21-22 Telecommunications ...........................................................22 System frequencies ..........................................................23 1 OVERVIEW.................................................................. 6 User frequencies ...............................................................23 Introduction .............................................................................. 6 Objectives............................................................................ 7 4 THE GROUND SEGMENT................................. 24 Meteorological satellites ................................................... 7 Future programmes ............................................................ 7 Ground segment facilities ................................................24 Meteosat history ...............................................................11 Primary Ground Station ..................................................... 25 The programmes .............................................................12 Overview ........................................................................... 26 Meteosat services ..............................................................12
    [Show full text]
  • Rapid Development of Navigation Payloads for Galileo Full Operational Capability
    Changing the economics of space RAPID DEVELOPMENT OF NAVIGATION PAYLOADS FOR GALILEO FULL OPERATIONAL CAPABILITY Alex da Silva Curiel Dubai, January 2011 SSTL - the company UK-based satellite manufacturing company owned by EADS Astrium NV (99%) and the University of Surrey (1%) • Formed in 1985, the Company now employs >320 staff and occupies dedicated facilities in Surrey, Kent & Colorado 2 A history of success 34 Satellites completed – c.200 satellite years on-orbit experience 10 Further satellites (35-43) - currently being prepared for launch 18 payloads in progress (4 optical, 14 navigation) HERITAGE: Flight proven - low risk RESULTS: All projects fixed price, delivered on-time and on-budget SUCCESS: Very high mission success – 100% mission success in last 10 years – proven equipment and full redundancy CUSTOMERS: Variety of customers including many “blue chip” operators as well as 15 successful training programmes 3 What is Galileo? Galileo is a joint initiative of the European Commission (EC) and the European Space Agency (ESA). Galileo will be Europe’s own global navigation satellite system, providing a highly accurate, guaranteed global positioning service under civilian control. It will be inter-operable with GPS and GLONASS, the two other global satellite navigation systems 4 Galileo Services • Galileo offers 5 services: – Open signal, dual frequency, mass market use – Commercial signal, better accuracy, service guarantee – authenticated data – Safety-of-Life signal, high integrity service certified for use in safety related
    [Show full text]
  • We Need Your Colouring Skills!
    We need your colouring skills! What do you think the colours of Mercury are? DID YOU KNOW? ercury • Mercury is the smallest planet in our solar system. • It is only slightly larger than the Earth’s Moon. • One day on Mercury is as long as 59 days on Earth. • A year on Mercury is as long as 88 Earth days • Temperatures on Mercury are extreme, reaching 430°C during the day, and -180°C at night. DID YOU KNOW? The Erth Depending on where you are on the globe, you could be spinning through space at just over 1,000 miles per hour. Water covers 70 percent of Earth's surface. 1 million Earths could fit in the Sun. Earth's atmosphere is composed of about 78 percent nitrogen, 21 percent oxygen, 0.9 percent argon, and 0.1 percent other gases. Earth is the only planet not named after a god. We need your colouring skills! What colours will you choose? We need your colouring skills! What do you think the colours of Jupiter are? DID YOU KNOW? Jupiter • Jupiter is the largest planet in the solar system. • Jupiter is as large as 1,300 Earths. • It's the 3rd brightest object in the night sky. • There's a big red spot on Jupiter, which is in fact a storm that has been raging for more than 350 years. DID YOU KNOW? Saturn • Saturn is the 2nd largest planet in the Solar System. • 764 Earths could fit inside Saturn. • Saturn's rings are made of ice and rock. They span 175,000 miles We need your and yet they’re only 20 metres thick.
    [Show full text]
  • Meteosat SEVIRI Fire Radiative Power (FRP)
    1 Meteosat SEVIRI Fire Radiative Power (FRP) Products from the 2 Land Surface Analysis Satellite Applications Facility (LSA 3 SAF): Part 1 - Algorithms, Product Contents & Analysis 4 5 Wooster, M.J. 1,2 , Roberts, G. 3, Freeborn, P. H. 1,4 , Xu, W. 1, Govaerts, Y. 5, Beeby, R. 1, 6 He, J. 1, A. Lattanzio 6, Fisher, D. 1,2 , and Mullen, R 1. 7 8 9 1 King’s College London, Environmental Monitoring and Modelling Research Group, 10 Department of Geography , Strand, London, WC2R 2LS, UK. 11 2 NERC National Centre for Earth Observation (NCEO), UK. 12 3 Geography and Environment, University of Southampton, Highfield, Southampton 13 SO17 1BJ, UK . 14 4 Fire Sciences Laboratory, Rocky Mountain Research Station, U.S. Forest Service, 15 Missoula, Montana, USA. 16 5 Rayference, Brussels, Belgium. 17 6 MakaluMedia, Darmstadt, Germany 18 19 20 Abstract 21 Characterising changes in landscape fire activity at better than hourly temporal 22 resolution is achievable using thermal observations of actively burning fires made 23 from geostationary Earth observation (EO) satellites. Over the last decade or more, a 24 series of research and/or operational 'active fire' products have been developed from 25 geostationary EO data, often with the aim of supporting biomass burning fuel 26 consumption and trace gas and aerosol emission calculations. Such "Fire Radiative 27 Power" (FRP) products are generated operationally from Meteosat by the Land 28 Surface Analysis Satellite Applications Facility (LSA SAF), and are available freely 29 every 15 minutes in both near real-time and archived form. These products map the 30 location of actively burning fires and characterise their rates of thermal radiative 31 energy release (fire radiative power; FRP), which is believed proportional to rates of 32 biomass consumption and smoke emission.
    [Show full text]
  • Metop Second Generation Payload
    MetOp Second Generation Payload Marc Loiselet, Ville Kangas, Ilias Manolis, Franco Fois, Salvatore d’Addio European Space Agency, ESA/ESTEC, Keplerlaan 1, 2200 AG Noordwijk, The Netherlands E-mail: [email protected] MetOp-Second Generation Satellite Instruments Instrument Provider The ESA MetOp Second Generation (MetOp-SG) Programme was approved at the ESA Council Meeting at Ministerial level in Naples in Sat-A METimage DLR via EUMETSAT November 2012. IASI-NG CNES via EUMETSAT MetOp-SG is a follow-on to the current, first generation series of MetOp satellites, which is now established as a cornerstone of the global MWS ESA – MetOp-SG network of meteorological satellites. RO ESA – MetOp-SG The MetOp-SG programme is being implemented in collaboration with EUMETSAT. 3MI ESA – MetOp-SG ESA will develop the prototype MetOp-SG satellites (including associated instruments) and procure, on behalf of EUMETSAT, the recurrent Sentinel-5 ESA – GMES satellites (and associated instruments). The overall MetOp-SG space segment architecture consists of two series of satellites (Sat-A, Sat-B), each carrying different suites of instruments and operating in LEO polar orbit. The planned launches of the first of each series of satellites Sat-B SCA ESA – MetOp-SG are at the beginning of 2021 and at end 2022, respectively. MWI ESA – MetOp-SG RO ESA – MetOp-SG More information can be found in the “MetOp Second Generation – Overview” presentation from Graeme Mason, Hubert Barré, Maurizio ICI ESA – MetOp-SG Betto, ESA-ESTEC, The Netherlands. Argos-4 CNES via EUMETSAT Payload ESA is responsible for instrument design of six instruments, namely the MicroWave Sounder (MWS), Scatterometer (SCA), the Radio Occultation (RO), the MicroWave Imaging (MWI), the Ice Cloud Imager (ICI), and the Multi-viewing, Multi-channel, Multi-polarisation imager (3MI).
    [Show full text]
  • The Role of Italian Industry in Space Exploration
    THE ROLE OF ITALIAN INDUSTRY IN SPACE EXPLORATION Maria Cristina Falvella ASI, Italian Space Agency Head of Strategies and Industrial Policy 53rd Session UN COPUOS Vienna, 17 February 2016 THE ITALIAN SPACE AGENCY (ASI) ASI has been founded in 1988 with the purpose to promote, develop and disseminate the scientific research and technology applied in the Space field. • Specific attention to the competitiveness of the Italian Space Industry, including SMEs • ASI operates in “integrated teams” => industry and research teams under the supervision of ASI ITALY AND EXPLORATION • Since 1964 Italy acts as a pioneer in space • Exploration is a flagship program for Italy, enhancing the competitiveness of the national industrial and scientific community • Participation in successful ESA and NASA programs, with challenging roles for national industries ISS and Mars : the top priorities Italy considers ISS and Mars destinations as part of a single exploration process and works to maximize the technology and system synergies among these destinations as well as to exploit the respective benefits of robotic and human exploration. • Economic and intellectual return out of the investments • Worldwide international relations • Competitiveness of the whole supply chain, from Large System Integrators (LSIs) to Small and Medium Companies (SMEs) • Leader position in international supply chains • Upgrade of technology capabilities and IPR • Benefits in non-space related systems and applications THE ITALIAN SUPPLY CHAIN The strategic effort to encourage the development
    [Show full text]
  • SATELLITE DATA for Weather Forecasting
    VOL. 98 NO. 3 MAR 2017 Mars 2020 Mission Earth Science Jobs: Seven Projections Earth & Space Science News Landsat Archive of Greenland Glaciers SATELLITE DATA for Weather Forecasting Earth & Space Science News Contents MARCH 2017 VOLUME 98, ISSUE 3 PROJECT UPDATE 20 Using LANDSAT to Take the Long View on Greenland Glaciers A new web-based data portal gives scientists access to more than 40 years of satellite imagery, providing seasonal to long-term insights into outflows from Greenland’s ice sheet. PROJECT UPDATE 32 Seeking Signs of Life and More: NASA’s Mars 2020 Mission The next Mars rover will be able to land near rugged terrain, giving scientists access to diverse landscapes. It will also cache core samples, a first step in the quest 26 to return samples to Earth. COVER OPINION Transforming Satellite Data Seven Projections 14 for Earth and Space into Weather Forecasts Science Jobs What do recent political changes mean A NASA project spans the gap between research and operations, for the job market? In the short term, not introducing new composites of satellite imagery to weather much. But long term, expect privatization, forecasters. contract employment, and more. Earth & Space Science News Eos.org // 1 Contents DEPARTMENTS Editor in Chief Barbara T. Richman: AGU, Washington, D. C., USA; eos_ [email protected] Editors Christina M. S. Cohen Wendy S. Gordon Carol A. Stein California Institute Ecologia Consulting, Department of Earth and of Technology, Pasadena, Austin, Texas, USA; Environmental Sciences, Calif., USA; wendy@ecologiaconsulting University of Illinois at cohen@srl .caltech.edu .com Chicago, Chicago, Ill., José D.
    [Show full text]
  • NASA Satellite Laser Ranging Program
    NASA Satellite Laser Ranging Program NASA Goddard Space Flight Center Ron Sebeny MOBLAS 4 Station Manager December 9, 2011 What is Satellite Laser Ranging? Map of International Laser Ranging Service (ILRS) Network Metsahovi PotsdamRiga Mendeleevo Borowiec Komsomolsk Herstmonceux Wettzell Zimmerwald Graz Simiez Changchun Grasse (2) Maidanak Cagliari KtiKatzive lly Beijing Greenbelt San Fernando Matera Keystone (4) Monument Peak Riyadh Wuhan Simosato McDonald Helwan Shanghai Kunming Santiago de Cuba Haleakala Arequipa South Africa Tahiti Yarragadee CiConcepcion Mt. Stromlo Legend: NASA NASA Partner International Cooperating Project: Satellite Laser Ranging (SLR) NASA SLR Network: • Eight Ground Stations • Part of International Laser Ranging Service (ILRS) • Data operations – Data reception, processing, and analysis – Orbit determination – Acquisition generation – Data Archive Laser Ranging Satellite Missions (past/present) : • Geodetic: – Larets, Starlette, Stella, Ajisai, LAGEOS-1, LAGEOS-2, Etalon-1, Etalon-2, BLITS • Earth Sensing/Technology Demonstration: – CHAMP, GRACE-A, GRACE-B, ICESat, Jason-1, Jason-2, Envisat, ERS-2, ETS-8, Beacon-C, TerraSAR-X, SOHLA-1, GOCE, CryoSat-2 • NitiNavigation: – GLONASS-102, GLONASS-115, GLONASS-120, GPS-35, GPS-36, GIOVE-A, GIOVE-B, Compass-M1 4 MOBLAS 4 Monument Peak MOBLAS 4 Monument Peak What is LRO? • Lunar Reconnaissance Orbiter – NASA’s Mission to map the moons surface with highest accuracy to date (highly successful thus far) • Laser ranggging to LRO will imp rove the scientific value of the
    [Show full text]