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												  ESA Solar System MissionsSmall Missions and the Science Programme of ESA Alvaro Gimenez, Director of Science and Robotic Exploration 26 February 2014 2 2 Astro-H suzaku corot Science Programme building blocks “Large” (Ariane 5-class) missions 1. High innovation content 2. European flagships 3. 1 B€ class 4. 3 per 20 years Herschel XMM-Newton Rosetta BepiColombo L3 L2 JUICE BepiColombo GAIA Herschel Rosetta XMM STSP 1980 1990 2000 2010 2020 2030 2040 H2000 H2000+ CV 2040 2035 2030 2025 2020 2015 2010 2005 2000 1995 1990 0 2 4 6 8 10 Science Programme building blocks “Medium” (Soyuz-class) missions 1. Makes use of current cutting-edge technology 2. Programme workhorse 3. 500 M€ class Planck 4. 3-4 per 10 years Euclid Solar Orbiter Mars Express 2040 2030 2020 2010 2000 1990 1980 0 5 10 15 20 Science Programme building blocks Missions of Opportunity 1. Moderate-size participation of the ESA Science Programme in missions led by partners 2. Format can vary 3. Increase flight and science opportunities for European scientists COROT ASTRO-H Hinode Double Star Science Programme building blocks Small missions a. New Programme element, still “experimental” b. Fast and with ESA CaC = 0.1 yearly budget c. Increase flight opportunities for European scientists d. Example: CHEOPS PLATO EUCLID SOLAR JUICE Astro H ORBITER µSCOPE Cheops ExoMars JWST BEPI LISA PF GAIA COLOMBO Akari Proba 2 Chandrayaan PLANCK Hinode HERSCHEL COROT ROSETTA Double Star SMART INTEGRAL Suzaku 1 SOHO VENUS MARS XMM F 2 CLUSTER → EXPRESS EXPRESS NEWTON CLUSTER HUYGENS ULYSSES ISO Time II HST 2030 2025 2020 2015 2010 2005 2000 1995 1990 1985 0 2 4 6 8 10 12 Small missions a.
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												  Observation of Pc 3/5 Magnetic Pulsations Around the Cusp at Mid Altitude1 OBSERVATION OF PC 3/5 MAGNETIC PULSATIONS AROUND THE CUSP AT MID ALTITUDE Liu Yonghua(1), Liu Ruiyuan(1), B. J. Fraser(2), S. T. Ables(2), Xu Zhonghua(1), Zhang Beichen(1), Shi Jiankui(3), Liu Zhenxing(3), Huang Dehong(1), Hu Zejun(1), Chen Zhuotian(1), Wang Xiao(3), Malcolm Dunlop(4), A. Balogh(5) (1) Polar Research Institute of China, 451 Jinqiao Rd., Shanghai 200136, P. R. CHINA, [email protected] (2) The University of Newcastle, University Drive, Callaghan NSW 2308, AUSTRALIA, [email protected] (3)The Center of Space Science & Applied Research, Chinese Academy of Science, Post Box8701, Beijing 100080, jkshi@@center.cssar.ac.cn (4) The Rutherford Appleton Laboratory, Chilton, DIDCOT, Oxfordshire, OX11 0QX, UK, [email protected] (5)Space and Atmospheric Physics Group, Imperial College, London, [email protected] ABSTRACT transmitted straightforwardly from solar wind to the ionosphere (Bolshakova & Troitskaia, 1984). So far most Since launched in year 2000 the Cluster mission has research work on such topic are on basis of observation passed the region around the cusp at mid-altitude (~6Re) at ground or/and data from satellite located in the for many times, where ULF wave activities are rich in. upstream of solar wind or in the magnetosheath. To my From 0800 to 1300UT on October 30 2002 the Cluster knowledge, few authors take a study based on the spacecrafts ran along an orbit of southern cusp- measurement at the mid-altitude of the cusp. It seems plasmasphere-northern cusp that provides an excellent reasonable to assume that such a measurement be a direct observation of ULF waves in dayside magnetosphere.
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												  China's Space Industry and International CollaborationChina’s Space Industry and International Collaboration Presenter: Ju Jin Title: Minister Counselor,the Embassy of P.R.China Date: Feb 27,2008 Brief History • 52 years since 1956, first space institute established • Learning from Soviet Union until 1960 • U.S.A.’s close door policy until now • China’s self-reliance Policy Major Achievements • 12 series of Long March Launching Rockets • >100 Launches • >80 satellites in remote sensing, telecommunication, GPS, scientific experiment • Manned space flights——Shenzhou 5 (2003) and Shenzhou 6 (2005) • Lunar Exploration Project——Chang’e 1 (2007) LM-2F Launch Vehicle • Stages 1 & 2 & 4 strap-on boosters • 58.3 meters long • Launch Mass: 480 tons • Total Thrust : 600 tons • Reliability & Safety Index: 0.97 & 0.997 • 10 Sub-Systems Manned Space Flight--Shenzhou 6 Manned Space Flight--Shenzhou 6 Lunar Probe Project--Change-1 First Lunar Surface Photos Lunar Probe Project—Change 1 • 3 Years • 17,000 Scientists and Engineers • Young Team averaged in the age of 30s • 100% China-Made • Technology Breakthroughs – All-direction Antenna – Ultra-violet Sensor International Exchange and Cooperation: Main Activities Over the recent years, China has signed cooperation agreements on the peaceful use of outer space and space project cooperation agreements with Argentina, Brazil, Canada, France, Malaysia, Pakistan, Russia, Ukraine, the ESA and the European Commission, and has established space cooperation subcommittee or joint commission mechanisms with Brazil, France, Russia and Ukraine. China and the ESA z Sino-ESA Double Star Satellite Exploration of the Earth's Space Plan. z "Dragon Program," involving cooperation in Earth observation satellites, having so far conducted 16 remote-sensing application projects in the fields of agriculture, forestry, water conservancy, meteorology, oceanography and disasters.
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												  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).
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												  LISA, the Gravitational Wave ObservatoryThe ESA Science Programme Cosmic Vision 2015 – 25 Christian Erd Planetary Exploration Studies, Advanced Studies & Technology Preparations Division 04-10-2010 1 ESAESA spacespace sciencescience timelinetimeline JWSTJWST BepiColomboBepiColombo GaiaGaia LISALISA PathfinderPathfinder Proba-2Proba-2 PlanckPlanck HerschelHerschel CoRoTCoRoT HinodeHinode AkariAkari VenusVenus ExpressExpress SuzakuSuzaku RosettaRosetta DoubleDouble StarStar MarsMars ExpressExpress INTEGRALINTEGRAL ClusterCluster XMM-NewtonXMM-Newton CassiniCassini-H-Huygensuygens SOHOSOHO ImplementationImplementation HubbleHubble OperationalOperational 19901990 19941994 19981998 20022002 20062006 20102010 20142014 20182018 20222022 XMM-Newton • X-ray observatory, launched in Dec 1999 • Fully operational (lost 3 out of 44 X-ray CCD early in mission) • No significant loss of performances expected before 2018 • Ranked #1 at last extension review in 2008 (with HST & SOHO) • 320 refereed articles per year, with 38% in the top 10% most cited • Observing time over- subscribed by factor ~8 • 2,400 registered users • Largest X-ray catalogue (263,000 sources) • Best sensitivity in 0.2-12 keV range • Long uninterrupted obs. • Follow-up of SZ clusters 04-10-2010 3 INTEGRAL • γ-ray observatory, launched in Oct 2002 • Imager + Spectrograph (E/ΔE = 500) + X- ray monitor + Optical camera • Coded mask telescope → 12' resolution • 72 hours elliptical orbit → low background • P/L ~ nominal (lost 4 out 19 SPI detectors) • No serious degradation before 2016 • ~ 90 refereed articles per year • Obs
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												  April 2008 SKYSCRAPERS, INC · Amateur Astronomical Society of Rhode Island · 47 Peeptoad Road North Scituate, RI 02857 · April Meeting with DrThe SkyscraperVol. 35 No. 4 April 2008 SKYSCRAPERS, INC · Amateur Astronomical Society Of Rhode Island · 47 Peeptoad Road North Scituate, RI 02857 · www.theSkyscrapers.org April Meeting with Dr. Alan Guth Friday, April 4 at Seagrave Memorial Observatory Dr. Alan Guth, Professor of Origins, Alan Guth, A Golden Age of Physics at the Massachusetts Insti- Cosmology and other publications. tute of Technology, is best known He will be presenting a talk entitled The Orion Nebula: SBIG 1001E on Meade 16” for the “inflationary” theory of “Inflationary Cosmology.” SCT at Barus and Holley Observatory; L = 12 ex- cosmology in which many features For the April meeting we will be posures x 5 seconds each, binned 1x1; R,G,B = of our universe, including how it returning to Seagrave Observatory. 3 exposures each x 5 seconds each, binned 2x2; came to be so uniform and why it Elections will be held at the April 27 exposures total, total exposure time = 2.25 began so close to the critical density meeting and membership renewals minutes. Images combined and processed using can be explained by. Dr. Guth is the are due. An elections ballot and Maxim DL. Photo by Bob Horton. author of The Inflationary Universe, renewal form are included in the the Quest for a New Theory of Cosmic back of this issue. In This Issue April Meeting with 1 Dr. Alan Guth April 2008 President’s Message 2 Glenn Jackson 4 7:30 pm Annual Meeting with Dr. Alan Guth April Lyrids Meteor 3 Friday Seagrave Memorial Observatory Shower Dave Huestis 5 8:00 pm Public Observing Night Tracking Wildlife
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												  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.
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												  Rapid Development of Navigation Payloads for Galileo Full Operational CapabilityChanging 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
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												  Territorial Satellite Technologies the NEREUS Network’S Italian Partners’ ExperiencesTerritorial satellite technologies The NEREUS Network’s Italian partners’ experiences December 2011 1 Contents 1. FOREWORD .............................................................................................................. 5 1.1. Reasons behind and object of this document ........................................................... 5 1.2. Activities conducted for the monitoring procedure .................................................. 6 PART I – THE SATELLITE APPLICATIONS CHART ........................................................... 9 2. SUPPLY AND DEMAND RELATING TO SATELLITE SERVICES IN THE CONTEXT OF THE NEREUS NETWORK’S ITALIAN PARTNERS .................................................................................. 10 2.1. Criteria adopted for the survey on the supply of and demand for satellite services 10 2.2. The chart of the Italian NEREUS partners’ satellite applications ............................. 12 PART III – ANALYSES AND PROPOSALS ...................................................................... 70 3. ELEMENTS EMERGING FROM THE SUPPLY AND DEMAND CHART ........................................ 71 3.1. Quantitative outline of the supply and demand chart ............................................ 71 3.2. Schemes identified as a demand needing to be met ............................................... 72 3.3. Projects in the “pre‐operational” stage and close to “end‐user needs” .................. 76 4. CONCLUSIONS ...................................................................................................
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												  NASA Satellite Laser Ranging ProgramNASA 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
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												  EC Workshop February 2013 Export.PptxExoPlanet CDF Study Report: CDF-100(A) April 2010 page 1 of 186 CDF Study Report EXOPLANET Exoplanet Spectroscopy Mission The programs of ESA’s Science and Robo7c Exploraon Directorate F. Favata ExoPlanet CDF Study Report: CDF-100(A) April 2010 page 1 of 186 One Directorate, two programs CDF Study Report • Science Programme EXOPLANET – Mandatory ac7vity Exoplanet Spectroscopy Mission – Science driven – BoFom-up program defini7on – Covers all areas of space science • Robo7c Exploraon Programme – Op7onal program – Technology driven – Top-down program defini7on • Science community consulted – Currently geared to the robo7c exploraon of Mars • Other ac7vi7es may be added ExoPlanet CDF Study Report: CDF-100(A) April 2010 page 1 of 186 Science Programme CDF Study Report • EXOPLANET Mandatory Programme: all Member States Exoplanet Spectroscopy Mission contribute pro-rata to their GNP – The “Agency’s backbone” • Level of Resources decision by unanimity at CMIN – 3-5 yr budget horizon • Content of Programme (which missions?) decided by Science Programme Commiee – Exclusive competence – Simple majority – Each Member State has one vote ExoPlanet CDF Study Report: CDF-100(A) April 2010 page 1 of 186 Science Programme governance CDF Study Report EXOPLANET • BoFom-up, community-driven program Exoplanet Spectroscopy Mission • Missions enter programme through open “Calls” to scien7fic community • Proposals are evaluated by the Space Science Advisory CommiFee (SSAC) • Director of Science makes proposals to SPC • SPC decides ExoPlanet CDF Study Report: CDF-100(A)
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												  First Galileo Satellites Galileo In-Orbit Validation ElementBR-251cover 7/8/06 13:28 Page 1 BR-251 Galileo Joint Undertaking Rue du Luxembourg 3 B-1000 Brussels, Belgium Tel: +32 2 507 80 00 The First Fax: +32 2 507 80 01 Email: [email protected] http://www.galileoju.com European Space Agency Directorate of European Union and Industrial Programmes Galileo Satellites 8-10 rue Mario Nikis F-75738 Paris Cedex 15, France Tel: +33 1 53 69 77 26 Fax: +33 1 53 69 72 86 Email: [email protected] http://www.esa.int/navigation/ European Commission Galileo In-Orbit Validation Element Directorate General for Energy and Transport Unit E.4 Satellite Navigation System (Galileo), Intelligent Transport, DM28 1/64 B-1049 Brussels, Belgium GIOVE Tel: +32 2 29 56040 Fax: +32 2 296 5372 Email: [email protected] http://europa.eu.int/comm/dgs/energy_transport/galileo/ BR-251cover 7/8/06 13:28 Page 2 BR-251 (2nd imprint, August 2006) Published by: ESA Publications Division ESTEC, PO Box 299 2200 AG Noordwijk The Netherlands Editor: Andrew Wilson Design/Layout: Eva Ekstrand Text coordination: Dominique Detain Copyright: ©2006 European Space Agency ISSN: 0250-1589 ISBN: 92-9092-497-7 Photo/image credits: Royal Astronomical Society Library (p.18), C. Beetles/Bridgeman-Giraudon (p.18), Galileo Price: 10 Euros Industries (pp. 7, 11); ESA: P.Carril (front cover, pp. 4, 5, 6, 7), S. Corvaja (front cover, pp. 6, 12), D. Detain (p. 13), J. Huart (pp. 3, 8, 9), A. Le Floch (pp. 4, 10, 16), E. Pedoussaut (p. 13), P.Sebirot (front cover),Trimaran (p.