Das GMES-Weltraumsegment & Relevante Earth Explorer Missionen

Total Page:16

File Type:pdf, Size:1020Kb

Das GMES-Weltraumsegment & Relevante Earth Explorer Missionen Das GMES-Weltraumsegment & relevante Earth Explorer Missionen A. Ginati, ESA © ESA 2003 DLR & DWD Nationaler Nutzerworkshop “Operationelle Satellitensysteme der Erdüberwachung” 7-9 November 2005, Walberberg Table of Content ¾ESAESA’’ss LiLivingving PlanetPlanet PrograProgrammemme ¾GMESGMES ¾EarthEarth Watch/EUMETSATWatch/EUMETSAT ¾EarthEarth ObservationObservation EnvelopeEnvelope ProgrammeProgramme Living Planet Programme • ESA dual-mission approach: –Earth Explorermissions, research oriented, also demonstration of techniques • Core and Opportunity Missions • Cooperation with JAXA, NASA etc – Implemented in Earth Observation Envelope Programme: • End-to-end implementation of Earth Explorer missions and preparation Earth Watch missions • 5 year slices, current EOEP-2, EOEP-3 proposed – Earth Watch missions, operational service oriented, implemented with partners • EUMETSAT, GEO and LEO operational meteorological missions • GMES Missions for the Global Monitoring for Environment and Security with the EC, EUMETSAT, MS others – Implemented in Dedicated EUMETSAT/GMES programmes: • Coordinate/parallel with programmes of partners (EUMETSAT, EC,MS) which cover also operational phase GMES European independence in critical data sources for environmental monitoring & security European contribution to the Global EO System of Systems (GEOSS) Established in 1998, gained political momentum 2001 ( GMES Service Element has been approved, MC Nov. 2001) • Initially, GMES investments focused on service developments • 100 Meuro by ESA, 100 Meuro by EC, plus MS projects (funded by CNES, DLR etc.) • Large number GMES user organisations across Europe Space segment preparation by ESA in 2004 • GMES system architecture, Phase A of GMES space missions EU declared GMES the next flagship for Europe in space, after Galileo GMES Service Element – initial services Coastal Real-time Ocean Ice Monitoring Northern View Risk fire & flood Forest Monitoring Soil & Water Land Motion Risks Urban Services Humanitarian Aid Food Security Atmosphere The overall GMES Space Component Gap analysis leads to 7 types of instruments 10-30 m SAR for interferometry, ocean, ice, land applications 0.5-10 m SAR for detailed land mapping 10-30 m multispectral instruments for land mapping 0.5-10 m optical instrument for detailed land mapping 100-1000 m wide-swath thermal infrared instruments for sea surface and land temperature measurements 100-1000 m wide-swath multi-spectral instruments for ocean colour and global land monitoring radar altimeters for ocean current measurements at high inclination orbit radar altimeters for ocean current measurements at low inclination orbit radar scatterometers for sea surface wind speed and direction atmospheric chemistry instruments for trace gas composition, pollution and climate change monitoring (leo and geo) 100-500 m infrared instruments for fire monitoring GMES – Space component 1. SAR imaging All weather, day/night applications, interferometry 2. Superspectral imaging, vegetation. forestry, security 3. Ocean monitoring Wide-swath ocean color and surface temperature sensors, altimeter 4. GEO- atmospheric composition monitoring, trans-boundary pollution 5. LEO- atmospheric composition monitoring IR-element, 3-band sensor for hot spot detection GMES : Sentinels and IR-element GPS Antenna S-Band TMA Antenna Star Instrument Tracker X-Band Antenna Sentinel –1 Sentinel –2 Sentinel –3 C-band SAR, wide swath, Multi-spectral imaging, Multi-spectral imaging medium resolution 8 bands 443 - 1 375 nm, VNIR-SWIR-TIR, 250–1000 m 10-30 m res. res, Altimeter, Sentinel –4 Sentinel –5 IR-element Atmospheric composition Atmospheric composition 3-band sensor for monitoring from GEO monitoring from LEO enhanced fire monitoring and detection Sentinel-1 requirements User Requirements are derived from GMES Services. Three services have reached a level of maturity such that firm information requirements can be established. Others will follow. – Monitoring the European Marine Environment – Monitoring the Arctic Environment and Sea-Ice Zones – Monitoring and Assessing Land Surface-Motion Risks across Europe Sentinel-1 Concept • Alternative satellite configurations under consideration •C band SAR Main modes are: – Stripmap 5 m swath 80 km – Scan SAR Interferometric wide swath 20X 5 m swath 240 km – Scan SAR Extra wideswath 80X25 m swath 400 km –Wave mode • S/C: ~2500 kg and 5 KW • Instrument duty cycle 15-20 min per orbit • Downlink data rate ~ 550 Mb/s. The definition study is being performed by EADS Astrium UK and subcontractors Sentinel-2 requirements • User requirements: from ESA GMES Service Elements, Forest, Soil/Aqua-SAGE, GUS (Urban Services), Risk-EOS, DUP Kyoto Inventory, Globwetland, and EC Geoland Project •Translated intomission/system requirements: – Coverage: global land (EU+worldwide), except polar caps – Spatial sampling distance (SSD): 10 m (goal) - 30 m (threshold) – Revisit time: 7 days to guarantee “seasonal” cloud-free product – Spectral bands: 3 sets of bands defined to allow room for trade-off at mission level • Minimum set of bands: 6 broad bands (Landsat-5 TM) •Nominalset of bands: 8 bands (LDCM), including 6 broad bands similar to Landsat-5 TM (band position and width optimised to minimise sensitivity to atmospheric water vapour) & two narrow bands at 443 nm (aerosol correction) and 1375 nm (cirrus cloud contamination detection and correction) •Extendedset of bands: 18 narrow bands encompassing LDCM spectral bands, with better sensitivity to bio-geophysical parameters & additional bands in the red edge (vegetation health) and SWIR (plant water content, vegetation structure, live/dead vegetation/soil discrimination) •Optionalpanchromatic channel at 5 m SSD (goal) Sentinel-2: Concepts Optical multi-spectral wide swath, medium resolution for mainly land applications. - to provide continuity to services developed with SPOT-5 and Landsat data. - Complementary to OLI / LDCM possibly on NPOESS C1/C4 - Building on studies on super- hyper- spectral missions Proposed sensor concept included: 10 bands in the VNIR and 2 bands in the SWIR Wide swath 320 km (700 km, SSO), 20 m spatial resolution The estimates for resources were 135 kg, 120 W and 800 Mbps GPS Antenna S-Band TMA Antenna Star Instrument Tracker X-Band Antenna The Definition Study aims for tuning of requirements and for the identification of efficient system concepts. Work performed by EADS Astrium and subcontractors. Contract started in early September. Sentinel-3: Requirements • User requirements from ESA GMES Service Elements: ROSES (ocean), Coastwatch (coastal zones) and GMFS (Food Security), Risk-EOS, and EC Geoland and Mersea Projects, and are consistent with Eumetsat (strawman missions Ocean Imaging / Ocean Topography) •Translated intomission/system requirements: – Coverage: global open ocean and land areas (except polar caps), coastal waters of Europe, the Mediterranean Sea, and the North Atlantic – Spatial sampling distance at SSP: 1 km (open ocean) - 250 m (coastal zones/land) – Revisit time: 1-3 days – Spectral bands: 21 spectral channels in VNIR/SWIR/TIR providing continuity to MERIS, Vegetation and AATSR – Radar altimeter with 3 cm RMS range noise level • With the support of encompassing studies involving numerous related operational, research and technical organisations Sentinel-3: Concepts Altimeter, high resolution ALT Doppler, no interferometry ACT 800 Km, SSO, 06:00 – 18:00 600 kg, 700 W, 20 Gb Implementation of optical and altimeter elements on separate satellites Optical sensor: OC, SST by Visible Infrared Imager (VIRI), ocean /land colour, sea /land surface temp., or separated optical sensors 800 Km, SSO, 00:00– 12:00 830 kg, 950W, 150 Gb The Definition Study aims for tuning of requirements and for the identification of efficient system concepts. Work performed by AAS and subcontractors. Contract started in early September. Preliminary considerations: Sentinels 4 and 5 Area Mission Characteristics Sentinels Ozone and Complement MetOp and NPOESS with limb- S-5 UV sounders operating in the MIR or mw range, radiation possibly UV-VIS (ACECHEM concept shown) Air Quality Frequent temporal coverage, 2 h (0.5 h goal), S-4 candidate for GEO, 50 km ( 5 km goal) UV-VIS: 290 – 310; 310 – 400; 400 – 600; 750 – (example 780; SWIR: 2310 – 2390; MIR: 2100 – 2200 cm-1, desired, TIR: 800 – 1200 cm-1, desired MTG) Climate CH4, CO and aerosol measurements, preferably S-5 with sensitivity to planetary boundary layer (Sciamachy, IASI, Mopitt heritage) The user requirements call for two elements: Sentinel-4 in GEO and Sentinel-5 in LEO Being studied in coordination with EUMETSAT MTG and Post-EPS Sentinels 4 & 5 : CAPACITY study to define user requirements Pre-phase A industrial studies 4th Q. 2005 Relations EUMETSAT and GMES missions • Sentinel–3 – Related to Post-EPS Ocean Imaging and Ocean Topography Strawman Missions • Sentinel-4 – Related to MTG UVS (and IRS) mission • Sentinel-5 – Related to Post-EPS Atmospheric Chemistry Mission Strawman Mission – Current Sentinel-5 concept assumes tandem flight with MetOp for coincidence of limb sounding m-wave and / or IR observations with MetOp’s GOME-2 and IASI – also UV-VNIR-SWIR nadir looking “SCIAMACHY-follow-on” • Sentinel-4, 5 concept under refinement: GEO or multi-LEO • ESA – EUMETSAT staff coordinating definition of EUMETSAT and GMES missions supported respectively by EUMETSAT Application Expert Groups and GMES User Groups GMES Space Component - Implementation Approach GMES Space Component 2005 2006 2007 2008 2009 2010 2011
Recommended publications
  • The Early Explorers by Andrew J
    The Early Explorers by Andrew J. LePage August 8, 1999 Among these programs were the next generation of Introduction Explorer satellites the ABMA was planning. In the chaos that swept the United States after the launching of the first Soviet Sputniks, a variety of The First New Explorers satellite programs was sponsored by the Department The first of the new series of larger Explorer satellites of Defense (DoD) to supplement (and in some cases was the 39.7 kilogram (87.5 pound) satellite NASA supplant) the country's flagging "official" satellite designated as S-1. Built by JPL, the spin stabilized program, Vanguard. One of the stronger programs S-1 consisted of a pair of fiberglass cones joined at was sponsored by the ABMA (Army Ballistic Missile their bases with a diameter and height of 76 Agency) with its engineering team lead by the centimeters each. The scientific payload consisted of German rocket expert, Wernher von Braun. Using instruments to study cosmic rays, solar X-ray and the Juno I launch vehicle, the ABMA team launched ultraviolet emissions, micrometeorites, as well as the America's first satellite, Explorer 1, which was built globe's heat balance. This was all powered by a bank by Caltech's Jet Propulsion Laboratory (JPL) (see of 15 nickel-cadmium batteries recharged by 3,000 Explorer: America's First Satellite in the February solar cells mounted on the satellite's exterior. This 1998 issue of SpaceViews). advanced payload was equipped with a timer to turn itself off after a year in orbit. While these first satellites returned a wealth of new data, they were limited by the tiny 11 kilogram (25 Explorer S-1 was launched from Cape Canaveral on pound) payload capability of the Juno I.
    [Show full text]
  • The Birth of Nasa - 1958
    THE BIRTH OF NASA - 1958 Jonathan McDowell Harvard-Smithsonian Center for Astrophysics [email protected] http://www.planet4589.org “In this decade...” May 25, 1961: JFK starts the Moon race. But the Space Age was already in full flow NASA was formed in 1958 The US space effort began long before that Cue the space race... October 1942: First into space America in orbit 1957-1961 Early program run by military and CIA: − US Army (ABMA/Huntsville): Explorer, Pioneer (with JPL) − US Navy (NRL/Washington): Vanguard − US Navy (NOTS/China Lake): “NOTSNIK” − US Air Force (WDD/Los Angeles): Able, Samos, Midas − CIA (Langley): CORONA (Discoverer) NASA formed 1958 for civilian space programs NRO formed 1961 for reconnaissance programs THE ROCKET'S RED GLARE ABMA/JPL Explorer Werner von Braun's stretched V-2 with spinning upper stages from JPL and tiny 4 kg payload Redstone reached apogee, spinning stages fired horizontally to get orbital velocity NRL's Vanguard NRL's Vanguard Bad rep - but stage 2 and 3 used for Delta with success Early launches used 2 kg test satellite - success on 3rd try Standard “Vanguard sphere” was 51cm - 2 of 8 made orbit Some of the Vanguard team went to Goddard to do science satellites, but some stayed at NRL Now we know: the Vanguard 51-cm sphere satellite had a later, secret history NOTSnik - Jul/Aug 1958 NOTS project First air-launched satellite attempt, off California coast Six tries, no confirmed successes 2 types of payload: radiation diagnostics for Argus artificial radiation belts, and infrared scanner instrument.
    [Show full text]
  • AAS Explorer Issue #8
    lookingback: Mexico City | 15 AMERICAN ASTRONAUTICAL SOCIETY Newsletter of the AAS History Committee | www.astronautical.org | Editor: Tim Chamberlin ([email protected]) Anxiously awaiting results INSIDE from Augustine Commission he Lovin’ Spoonful probably JULY 2009 | ISSUE 8 had it right in 1966 — “Hot T town, summer in the city!” Many of us who work in the space industry are anxiously awaiting the results of the Augustine Commission (part deux). I can’t help By Michael L. Ciancone, Chair, AAS History Committee but reflect on the various commis- sions of which NASA has been the (program startups) and graduations subject over the past few decades, as (launches!) as signs of a healthy and RELIVE HISTORIC discussed in several articles circulat- vital spaceflight program. APOLLO MISSION ing in cyberspace. Reports of individual HistComm These commissions offered member activities, plans and accom- ® Web sites mark historic lunar landing 40 years ago / 2 recommendations that met with vary- plishments are provided in this ing degrees of acceptance and imple- newsletter. As you can see, we’ve ® NASA seeking ideas from public mentation. In the immortal words of been a busy and productive lot! about Wernher Yogi Berra, “It’s like déjà vu all over Although it seems like a long way von Braun again.” off yet, the AAS Annual Conference collection / 3 I’ve noticed that along with and National Meeting is just around ® On book- announcements for space-related the corner — scheduled for Dec. 2-3 shelves: Is space a ‘wild west’ or global anniversaries are a number of obitu- at the Gilruth Center at Johnson commons? / 4 aries saluting folks who left their Space Center in Houston.
    [Show full text]
  • Astronomy 2009 Index
    Astronomy Magazine 2009 Index Subject Index 1RXS J160929.1-210524 (star), 1:24 4C 60.07 (galaxy pair), 2:24 6dFGS (Six Degree Field Galaxy Survey), 8:18 21-centimeter (neutral hydrogen) tomography, 12:10 93 Minerva (asteroid), 12:18 2008 TC3 (asteroid), 1:24 2009 FH (asteroid), 7:19 A Abell 21 (Medusa Nebula), 3:70 Abell 1656 (Coma galaxy cluster), 3:8–9, 6:16 Allen Telescope Array (ATA) radio telescope, 12:10 ALMA (Atacama Large Millimeter/sub-millimeter Array), 4:21, 9:19 Alpha (α) Canis Majoris (Sirius) (star), 2:68, 10:77 Alpha (α) Orionis (star). See Betelgeuse (Alpha [α] Orionis) (star) Alpha Centauri (star), 2:78 amateur astronomy, 10:18, 11:48–53, 12:19, 56 Andromeda Galaxy (M31) merging with Milky Way, 3:51 midpoint between Milky Way Galaxy and, 1:62–63 ultraviolet images of, 12:22 Antarctic Neumayer Station III, 6:19 Anthe (moon of Saturn), 1:21 Aperture Spherical Telescope (FAST), 4:24 APEX (Atacama Pathfinder Experiment) radio telescope, 3:19 Apollo missions, 8:19 AR11005 (sunspot group), 11:79 Arches Cluster, 10:22 Ares launch system, 1:37, 3:19, 9:19 Ariane 5 rocket, 4:21 Arianespace SA, 4:21 Armstrong, Neil A., 2:20 Arp 147 (galaxy pair), 2:20 Arp 194 (galaxy group), 8:21 art, cosmology-inspired, 5:10 ASPERA (Astroparticle European Research Area), 1:26 asteroids. See also names of specific asteroids binary, 1:32–33 close approach to Earth, 6:22, 7:19 collision with Jupiter, 11:20 collisions with Earth, 1:24 composition of, 10:55 discovery of, 5:21 effect of environment on surface of, 8:22 measuring distant, 6:23 moons orbiting,
    [Show full text]
  • Trimble Business Center User Guide
    User Guide Trimble® Business Center Version 2.00 Corporate Office Trimble Navigation Limited Engineering and Construction Division 5475 Kellenburger Road Dayton, Ohio 45424-1099 U.S.A. Phone: +1-937-233-8921 Toll free (in USA): +1-800-538-7800 Fax: +1-937-233-9441 www.trimble.com Copyright and Trademarks © 2005-2008, Trimble Navigation Limited. All rights reserved. The Globe & Triangle logo and Trimble are trademarks of Trimble Navigation Limited. All other trademarks are the property of their respective owners. Release Notice This is the help for version 2.00 of Trimble Business Center software. Trimble® Business Center User Guide ii Contents Contents Welcome To Trimble Business Center 1 Get Started 2 Register This Software ......................................................................................................................................2 Retaining User Settings When Upgrading.......................................................................................................4 Get Familiar with the Interface........................................................................................................................5 Project Explorer.................................................................................................................................................6 Selection Explorer .............................................................................................................................................7 View Filter Manager .........................................................................................................................................8
    [Show full text]
  • Index of Astronomia Nova
    Index of Astronomia Nova Index of Astronomia Nova. M. Capderou, Handbook of Satellite Orbits: From Kepler to GPS, 883 DOI 10.1007/978-3-319-03416-4, © Springer International Publishing Switzerland 2014 Bibliography Books are classified in sections according to the main themes covered in this work, and arranged chronologically within each section. General Mechanics and Geodesy 1. H. Goldstein. Classical Mechanics, Addison-Wesley, Cambridge, Mass., 1956 2. L. Landau & E. Lifchitz. Mechanics (Course of Theoretical Physics),Vol.1, Mir, Moscow, 1966, Butterworth–Heinemann 3rd edn., 1976 3. W.M. Kaula. Theory of Satellite Geodesy, Blaisdell Publ., Waltham, Mass., 1966 4. J.-J. Levallois. G´eod´esie g´en´erale, Vols. 1, 2, 3, Eyrolles, Paris, 1969, 1970 5. J.-J. Levallois & J. Kovalevsky. G´eod´esie g´en´erale,Vol.4:G´eod´esie spatiale, Eyrolles, Paris, 1970 6. G. Bomford. Geodesy, 4th edn., Clarendon Press, Oxford, 1980 7. J.-C. Husson, A. Cazenave, J.-F. Minster (Eds.). Internal Geophysics and Space, CNES/Cepadues-Editions, Toulouse, 1985 8. V.I. Arnold. Mathematical Methods of Classical Mechanics, Graduate Texts in Mathematics (60), Springer-Verlag, Berlin, 1989 9. W. Torge. Geodesy, Walter de Gruyter, Berlin, 1991 10. G. Seeber. Satellite Geodesy, Walter de Gruyter, Berlin, 1993 11. E.W. Grafarend, F.W. Krumm, V.S. Schwarze (Eds.). Geodesy: The Challenge of the 3rd Millennium, Springer, Berlin, 2003 12. H. Stephani. Relativity: An Introduction to Special and General Relativity,Cam- bridge University Press, Cambridge, 2004 13. G. Schubert (Ed.). Treatise on Geodephysics,Vol.3:Geodesy, Elsevier, Oxford, 2007 14. D.D. McCarthy, P.K.
    [Show full text]
  • Construction of an Adaptive E-Learning Environment To
    !PREFACE Construction of an Adaptive E-learning Environment to Address Learning Styles and an Investigation of the Effect of Media Choice Christian Wolf Diplom-Informatiker (FH) Digitale Medien (equivalent to BCompSc(Hons) Digital Media) This exegesis is submitted with the durable record of the project materials on DVD in fulfilment of the requirements for the degree Doctor of Philosophy. School of Education Design and Social Context Portfolio RMIT University January 2007 Certification i Certification I hereby state that a. except where due acknowledgement has been made, the work has been carried out by myself alone; b. the work has not been submitted previously, in whole or in part, to qualify for any other academic award; c. the content of the exegesis is the result of work which has been carried out since the official commencement date of the approved research program; and d. any editorial work, paid or unpaid, carried out by a third party is acknowledged. e. ethics procedures and guidelines have been followed. Christian Wolf Melbourne, January 2007 Acknowledgements ii Acknowledgements This PhD by project was partially funded by a scholarship from the German Academic Exchange Service and a grant from the Telematics Course Development Fund Trust. Thanks to my supervisors Tony Owens, Andrew Seaton, Nicola Yelland, and Robyn Blake for their comments on my work and on earlier versions of this exegesis. Additional thanks for helpful comments on the statistics sections go to John Izard, Cliff DaCosta and Boyka Bratanova. I would also like to express my gratitude to the 63 multimedia students from RMIT University (TAFE division), who participated in the evaluation of iWeaver, as well as to all the ADoM staff members for their support and cooperation.
    [Show full text]
  • Our First Quarter Century of Achievement ... Just the Beginning I
    NASA Press Kit National Aeronautics and 251hAnniversary October 1983 Space Administration 1958-1983 >\ Our First Quarter Century of Achievement ... Just the Beginning i RELEASE ND: 83-132 September 1983 NOTE TO EDITORS : NASA is observing its 25th anniversary. The space agency opened for business on Oct. 1, 1958. The information attached sumnarizes what has been achieved in these 25 years. It was prepared as an aid to broadcasters, writers and editors who need historical, statistical and chronological material. Those needing further information may call or write: NASA Headquarters, Code LFD-10, News and Information Branch, Washington, D. C. 20546; 202/755-8370. Photographs to illustrate any of this material may be obtained by calling or writing: NASA Headquarters, Code LFD-10, Photo and Motion Pictures, Washington, D. C. 20546; 202/755-8366. bQy#qt&*&Mary G. itzpatrick Acting Chief, News and Information Branch Public Affairs Division Cover Art Top row, left to right: ffComnandDestruct Center," 1967, Artist Paul Calle, left; ?'View from Mimas," 1981, features on a Saturnian satellite, by Artist Ron Miller, center; ftP1umes,*tSTS- 4 launch, Artist Chet Jezierski,right; aeronautical research mural, Artist Bob McCall, 1977, on display at the Visitors Center at Dryden Flight Research Facility, Edwards, Calif. iii OUR FIRST QUARTER CENTER OF ACHIEVEMENT A-1 -3 SPACE FLIGHT B-1 - 19 SPACE SCIENCE c-1 - 20 SPACE APPLICATIQNS D-1 - 12 AERONAUTICS E-1 - 10 TRACKING AND DATA ACQUISITION F-1 - 5 INTERNATIONAL PROGRAMS G-1 - 5 TECHNOLOGY UTILIZATION H-1 - 5 NASA INSTALLATIONS 1-1 - 9 NASA LAUNCH RECORD J-1 - 49 ASTRONAUTS K-1 - 13 FINE ARTS PRQGRAM L-1 - 7 S IGN I F ICANT QUOTAT IONS frl-1 - 4 NASA ADvIINISTRATORS N-1 - 7 SELECTED NASA PHOTOGRAPHS 0-1 - 12 National Aeronautics and Space Administration Washington, D.C.
    [Show full text]
  • NASA Is Not Archiving All Potentially Valuable Data
    ‘“L, United States General Acchunting Office \ Report to the Chairman, Committee on Science, Space and Technology, House of Representatives November 1990 SPACE OPERATIONS NASA Is Not Archiving All Potentially Valuable Data GAO/IMTEC-91-3 Information Management and Technology Division B-240427 November 2,199O The Honorable Robert A. Roe Chairman, Committee on Science, Space, and Technology House of Representatives Dear Mr. Chairman: On March 2, 1990, we reported on how well the National Aeronautics and Space Administration (NASA) managed, stored, and archived space science data from past missions. This present report, as agreed with your office, discusses other data management issues, including (1) whether NASA is archiving its most valuable data, and (2) the extent to which a mechanism exists for obtaining input from the scientific community on what types of space science data should be archived. As arranged with your office, unless you publicly announce the contents of this report earlier, we plan no further distribution until 30 days from the date of this letter. We will then give copies to appropriate congressional committees, the Administrator of NASA, and other interested parties upon request. This work was performed under the direction of Samuel W. Howlin, Director for Defense and Security Information Systems, who can be reached at (202) 275-4649. Other major contributors are listed in appendix IX. Sincerely yours, Ralph V. Carlone Assistant Comptroller General Executive Summary The National Aeronautics and Space Administration (NASA) is respon- Purpose sible for space exploration and for managing, archiving, and dissemi- nating space science data. Since 1958, NASA has spent billions on its space science programs and successfully launched over 260 scientific missions.
    [Show full text]
  • Response of Energetic Particles to Magnetospheric Ultra-Low-Frequency Waves
    KAZUE TAKAHASHI RESPONSE OF ENERGETIC PARTICLES TO MAGNETOSPHERIC ULTRA-LOW-FREQUENCY WAVES Ultra-low-frequency (ULF) waves in the space physics context are the lowest-frequency plasma waves propagating in the Earth's magnetosphere. Although the propagation of the waves is explained in mag­ netohydrodynamic (MHD) theory, excitation of the waves involves not only MHD but also kinetic pro­ cesses. In this article, we describe how in situ magnetic field and particle measurements can be used to distinguish the basic properties of ULF waves, including the azimuthal wave number of the standing wave structure and the propagation direction. Examples are taken from observations with the AMPTE/CCE spacecraft. INTRODUCTION A long time ago it was realized that the geomagnetic perimentally determined. This provides a quantitative ba­ field as observed on the ground exhibits small-amplitude sis for testing various theories of plasma instabilities. oscillations with a period of a few minutes. 1 Since then, In this article we describe how energetic particle data the phenomenon has attracted many researchers and has combined with magnetic field data can be used to under­ been called by several different names, including geo­ stand the properties of ULF waves. In some cases, the magnetic micropulsations, magnetic pulsations, ultra­ particles can be treated separately from the bulk of the low-frequency (ULF) pulsations (i.e., frequencies lower plasma, and can be used as test particles probing the spa­ than 3 Hz), or ULF waves. In 1954, Dungey2 predicted tial and temporal structure of ULF pulsations. In that that the oscillations originate in the magnetosphere as case, the type of wave-particle interactions critically de­ magnetohydrodynamic (MHD) waves.
    [Show full text]
  • NASA Major Launch Record
    NASA Major Launch Record 1958 MISSION/ LAUNCH LAUNCH PERIOD CURRENT ORBITAL PARAMETERS WEIGHT REMARKS Intl Design VEHICLE DATE (Mins.) Apogee (km) Perigee (km) Incl (deg) (kg) (All Launches from ESMC, unless otherwise noted) 1958 1958 Pioneer I (U) Thor-Able I Oct 11 DOWN OCT 12, 1958 34.2 Measure magnetic fields around Earth or Moon. Error in burnout Eta I 130 (U) velocity and angle; did not reach Moon. Returned 43 hours of data on extent of radiation band, hydromagnetic oscillations of magnetic field, density of micrometeors in interplanetary space, and interplanetary magnetic field. Beacon I (U) Jupiter C Oct 23 DID NOT ACHIEVE ORBIT 4.2 Thin plastic sphere (12-feet in diameter after inflation) to study (U) atmosphere density at various levels. Upper stages and payload separated prior to first-stage burnout. Pioneer II (U) Thor-Able I Nov 8 DID NOT ACHIEVE ORBIT 39.1 Measurement of magnetic fields around Earth or Moon. Third stage 129 (U) failed to ignite. Its brief data provided evidence that equatorial region about Earth has higher flux and higher energy radiation than previously considered. Pioneer III (U) Juno II (U) Dec 6 DOWN DEC 7, 1958 5.9 Measurement of radiation in space. Error in burnout velocity and angle; did not reach Moon. During its flight, discovered second radiation belt around Earth. 1959 1959 Vanguard II (U) Vanguard Feb 17 122.8 3054 557 32.9 9.4 Sphere (20 inches in diameter) to measure cloud cover. First Earth Alpha 1 (SLV-4) (U) photo from satellite. Interpretation of data difficult because satellite developed precessing motion.
    [Show full text]
  • 60 Years of Earth Imaging from Satellites
    50 May-June 2018 60 Years of Earth Imaging from Satellites By Don Hillger and Garry Toth Satellite imagery is a common and integral part of modern life, from the frequent cloud photos used for weather analysis, forecasting and television illustrations to Earth-observing imagery for environmental monitoring. Th is fl ood of imagery is a modern phenomenon. Starting with the fi rst artifi cial satellites in the late 1950s, the ability to view Earth from space has progressed steadily to the point that many terabytes of imagery are now obtained daily from satellites, which have become the main sources of the remote-sensing data that swell the archives of the scientifi c community. Th e topic of satellite imagery and its history could fi ll a large number of volumes. Th e goal of this article is to outline certain aspects of satellite remote- sensing history (hitting the highlights, as it were) and, in particular, to focus on some of the innovative satellite imagery that has recently become available. Th e First Earth Imagery Th e fi rst photo of Earth from space was not taken by a satellite, but rather from a German V-2 missile launched from White Sands Missile Range (WSMR) in New Mexico on Oct. 24, 1946. Th e story of that photo is documented in the Smithsonian Air and Space Magazine (www.airspacemag.com/space/the-fi rst-photo- from-space-13721411/). Th e only postal item known to show this rocket-view image is a 65th anniversary cover for the launch of that V2 rocket.
    [Show full text]