Satellites & Sensors
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												  GEO and GEOSS……GEO - GEOSS Support of the CBD 2010 Targets CBD - SBSTTA Paris, 4 July 2007 Douglas Muchoney, GEO Secretariat © GEO Secretariat The Earth is a complex system of systems © GEO Secretariat Any Single Problem Requires Many Data Sets A Single Data Set Will Serve Many Communities © GEO Secretariat Solar Energy © GEO Secretariat GEOSS Implementation is a Non- binding, Voluntary Process • Relies on the Goodwill of Members and Participating Organizations • Efficient for Contribution of Components • Not a Funding Mechanism • GEO implements GEOSS © GEO Secretariat GEO Goal Improve and Coordinate Observation Systems Provide Easier & More Open Data Access Foster Use (Science, Applications, Capacity Bldg) … to answer Society’s need for informed decision making © GEO Secretariat GEOSS: A Global, Coordinated, Comprehensive and Sustained System of Observing Systems © GEO Secretariat GEOSS will Address Nine Societal Benefit Areas 1. Reduction and Prevention of Disasters 2. Human Health and Epidemiology 3. Energy Management 4. Climate Variability & Change 5. Water Management 6. Weather Forecasting 7. Ecosystems 8. Agriculture 9. Biodiversity © GEO Secretariat GEOSS achievement through 5 Transverse Areas 1. Architecture 2. Data Management 3. User Engagement 4. Capacity Building 5. Outreach © GEO Secretariat Envisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 SPIN-2 SeaWinds Orbview 2, 3 TRMM DMC ACRIMSAT EROS A1 ERBS Radarsat ALOS Toms-EP QuickBird Grace Landsat 7 Jason UARS Space Observation© GEO Secretariat Systems In Situ Observation Systems © GEO Secretariat GEO Societal Benefit Areas 1. Reduction and Prevention of Disasters 2. Human Health 3. Energy Management 4. Climate Change 5. Water Management 6. Weather Forecasting 7. Ecosystems 8. Agriculture 9.
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												  Overview of Sensors for ApplicationsOVERVIEW OF SENSORS FOR APPLICATIONS Deepak Putrevu Head, MTDD/AMHTDG EM SPECTRUM Visible 0.4-0.7μm Near infrared (NIR) 0.7-1.5μm Optical Infrared Shortwave infrared (SWIR) 1.5-3.0μm Mid-wave infrared (MWIR) 3.0-8.0μm (OIR) Region Longwave IR(LWIR)/Thermal IR(TIR) 8.0-15μm Far infrared (FIR) Beyond15μm Gamma Rays X Rays UV Visible NIR SWIR Thermal IR Microwave P-band: ~0.25 – 1 GHz Microwave Region L-band: 1 -2 GHz S-band: 2-4 GHz •Sensors are 24x365 C-band: 4-8 GHz •Signal data characteristics X-band: 8-12 GHz unique to the microwave region of the EM spectrum Ku-band: 12-18 GHz K-band: 18-26 GHz •Response is primarily governed by geometric Ka-band: 26-40 GHz structures and hence V-band: 40 - 75 GHz complementary to optical W-band: 75-110 GHz imaging mm-wave: 110 – 300GHz Basic Interactions between Electromagnetic Energy and the Earth’s Surface Incident Power reflected, ρP Reflectivity: The fractional part of the radiation, P incident radiation that is reflected by the surface. Power absorbed, αP Absorptivity: the fractional part of the = Power emitted, εP incident radiation that is absorbed by the surface. Power transmitted, τP Emissivity: The ratio of the observed flux emitted by a body or surface to that of a P= Pr + Pt + Pa blackbody under the same condition. 푃 푃 푃 푟 + 푡 + 푎 = 1 푃 푃 푃 Transmissivity: The fractional part of the ρ + τ + α =1 radiation transmitted through the medium. At thermal equilibrium, absorption and emission are the same.
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												  Indian Payload Capabilities for Space MissionsINDIAN PAYLOAD CAPABILITIES FOR 13, Bangalore - SPACE MISSIONS July 11 A.S. Kiran Kumar Director Space Applications Centre International ASTROD Symposium, Ahmedabad th 5 Application-specific EO payloads IMS-1(2008) RISAT-1 (2012) MX/ HySI-T C-band SAR CARTOSAT-2/2A/2B RESOURCESAT-2 (2011) (2007/2009/2010) LISS 3/ LISS 4/AWiFS PAN RESOURCESAT-1 (2003) LISS 3/ LISS 4 AWiFS CARTOSAT-1 (2005) (Operational) STEREOPAN Megha-Tropiques (2011) TES(2001) MADRAS/SAPHIR/ScARaB/ Step& Stare ROSA PAN OCEANSAT-2 (2009) OCM/ SCAT/ROSA YOUTHSAT(2011) LiV HySI/RaBIT INSAT-3A (2003) KALPANA-1 (2002) VHRR, CCD VHRR Application-specific EO payloads GISAT MXVNIR/SWIR/TIR/HySI RISAT-3 RESOURCESAT-3A/3B/3C L-band SAR CARTOSAT-3 RESOURCESAT-2A LISS 3/LISS 4/AWiFS PAN LISS3/LISS4/AWiFS RESOURCESAT-3 LISS 3/LISS 4/ CARTOSAT-2C/2D AWiFS (Planned) PAN RISAT-1R C-band SAR SARAL Altimeter/ARGOS OCEANSAT-3 OCM , TIR GISAT MXVNIR/SWIR/ INSAT- 3D TIR/HySI Imager/Sounder EARTH OBSERVATION (LAND AND WATER) RESOURCESAT-1 IMS-1 RESOURCESAT-2 RISAT-1 RESOURCESAT-2A RESOURCESAT-3 RESOURCESAT-3A/3B/3C RISAT-3 GISAT RISAT-1R EARTH OBSERVATION (CARTOGRAPHY) TES CARTOSAT-1 CARTOSAT-2/2A/2B RISAT-1 CARTOSAT-2C/2D CARTOSAT-3 RISAT-3 RISAT-1R EARTH OBSERVATION (ATMOSPHERE & OCEAN) KALPANA-1 INSAT- 3A OCEANSAT-1 INSAT-3D OCEANSAT-2 YOUTHSAT GISAT MEGHA–TROPIQUES OCEANSAT-3 SARAL Current observation capabilities : Optical Payload Sensors in Spatial Res. Swath/ Radiometry Spectral bands Repetivity/ operation Coverage (km) revisit CCD 1 1 Km India & 10 bits 3 (B3, B4, B5) 4 times/ day surround.
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												  History of the Indian Remote Sensing ProgrammeHistory of the Indian Remote Sensing Programme Ranganath Navalgund Vikram Sarabhai Distinguished Professor Indian Space Research Organisation Bangalore, India Workshop on Small Satellites & Sensor Technology for Disaster Management, Indo-US S&T Forum CANEUSMarch SSTDM 31, 2014 2014 BEGINNING Stared with the pioneering experiment of detecting Coconut Root Wilt Disease using Color Infrared Film in 1970s by Prof. P. R. Pisharoty. Jun 07,1979 Bhaskara-I (1979) and Bhaskara-II (1981) – Experimental Remote Sensing Satellites provided the Aerial view of Grove Area foundation for the operational Indian Remote Sensing Programme. Nov 20, 1981 (Coconut Root Wilt Disease Study) The Result is operational Indian Remote Sensing Programme with the launch of IRS-1A on March 17, 1988 CANEUS SSTDM 2014 DURING 1980s NRSA established Earth Station Complex at Annaram Village, Shadnagar, 59 km from Balanagar in 1979 to receive Landsat Data TERMINAL-1 (10M DIA) L & S Band 15 Mbps 1980-83: Landsat 2,3 & NOAA- 2, 3 1983-88: Landsat 5, ERS, SPOT & NOAA Today: Multimission ScenarioCANEUS - 4 SSTDMTerminals 2014 (7.5m) - upto 960Mbps EVOLUTION OF (Microwave RISAT-1 (2012) Capability) INDIAN EO SYSTEMS C Band SAR (5.35 GHz) IMS-1 (2008) (Hyperspectral HySI Sensor (64 bands, 506 m) Capability) TWSAT-MX (4 bands, 37 m) TES, Cartosat-1, 2/2A/2B (1999, (High Spatial Resolution 2005, 2007, 2008, 2010) & Stereo Capability) PAN : 2.5 m, 1m Fore +26o Aft: -5o Resourcesat-1/2 (2003, 2011) (Multi resolution, Frequent LISS-3: 23 m, 4 XS, observations, Better LISS-4: 5.8
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												  Highlights in Space 2010International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no.
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												  Type Here Your TitleEnvisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 GEO-GLAM SPIN-2 SeaWinds GLOBAL AGRICULTURALOrbview 2, 3 MONITORINGTRMM DMC ACRIMSAT EROS A1 ERBS Radarsat Jai Singh PariharALOS for the GEOGLAM group and GEO Agriculture CommunityToms-EP of Practice QuickBird Grace Landsat 7 Jason UARS © GEO Secretariat Cereal grain production per hectare (Source: SAGE, Univ. of Wisconsin, Madison, Wisc., USA) 5th GEOSS-Asia Pacific Symposium, Tokyo, April 2-4, 2012 1. The GEO-GLAM Initiative : Objectives To reinforce the international community’s capacity to produce and disseminate relevant, timely and accurate forecasts of agricultural production at national, regional and global scales. Envisat SORCE Aura/Aqua/Terra Sage QuikScat IKONOS CBERS SeaWiFS SPOT 4, 5 SPIN-2 SeaWinds Orbview 2, 3 TRMM DMC ACRIMSAT EROS A1 ERBS Radarsat ALOS Toms-EP QuickBird Grace Landsat 7 Jason UARS © GEO Secretariat Agronomy Earth Observation Agro-economy Cultivated area / crop type area Meteorology Cereal grain production per hectare (Source: SAGE, Univ. of Wisconsin, Madison, Wisc., USA) Crop yield forecast 2 1. The GEO-GLAM Initiative : Background (G20 2011) 3 1. The GEO-GLAM Initiative : Background (G20 2011) G20 Final Declaration (Nov. 2011) 44. We commit to improve market information and transparency in order to make international markets for agricultural commodities more effective. To that end, we launched: • The "Agricultural Market Information System" (AMIS) in Rome on September 15, 2011, to improve information on markets ...; • The "Global Agricultural Geo-monitoring Initiative" (GEOGLAM) in Geneva on September 22-23, 2011, to coordinate satellite monitoring observation systems … to enhance crop production projections ... 4 2.
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												  Precision Optics and AssembliesPRECISION OPTICS AND ASSEMBLIES Image: NASA Wide Field Infrared Survey Telescope (WFIRST) High-performance, reliable optics for ground and space-based observation Dazzling details of Earth and insights into the mysteries of the universe BENEFITS have one thing in common — L3Harris precision optics. High-perfor- > Meet the most demanding mance optical components and assemblies have been integral to the requirements for spatial world’s most sophisticated ground- and space-based telescopes and frequency, mounting and satellites for more than 50 years. application-specific needs > Provide end-to-end capabilities with cost-effective fabrication SPECIALIZING IN CUSTOM, L3Harris provides solutions for high- LARGE-SCALE OPTICS performance systems, including: > Create surface finish to less than two-nanometer root mean > Ground- and space-based telescopes L3Harris provides optomechanical design, square (RMS) on glass and glass optical fabrication, test and assembly > Solid and lightweight optics for ceramic materials capabilities for precision optics solutions autocollimating systems and systems. The company manufactures > Lightweight fast-steering mirrors large optical components, including lightweight and solid mirrors in most > High-energy laser optics geometric shapes, to meet low surface > Optical test systems microroughness and tight surface figure error specifications. This experience, > Relay mirrors along with a rigorous metrology and > Observation and vacuum testing program and state-of-the-art compatible viewing windows in-house facilities,
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												  India's Early Satellites – Spin-Stabilized and Bias MomentumIndia’s Early Satellites – Spin-Stabilized and Bias Momentum ISRO Aryabhata – for Space Science (Launch date 19 April 1975) Aryabhata was India's first satellite It was launched by the Soviet Union from Kapustin Yar Mission type Astrophysics Satellite of Earth Aryabhata was built by the ISRO Launch date 19 April 1975 engineers to conduct Carrier rocket Cosmos-3M experiments related to X-ray astronomy, solar physics, and Mass 360.0 kg Power 46 W from solar panels aeronomy. Orbital elements Regime LEO The satellite reentered the Inclination 50.7º Orbital period 96 minutes Earth's atmosphere on 11 Apoapsis 619 km February 1992. Periapsis 563 km *National Space Science Data Center, NASA Goddard Space Flight Center Bhaskara (Earth Observation) Satellites (launched in 1979-1981)* Bhaskara-I and II Satellites were built by the ISRO, and they were India's first low orbit Earth Observation Satellite.They collected data on telemetry, oceanography, hydrology. Bhaskara-I, weighing 444 kg at launch, was launched on June 7, 1979 from Kapustin Yar aboard the Intercosmos launch vehicle. It was placed in an orbital Perigee of 394 km and Apogee of 399 km at an inclination of 50.7°. The satellite consisted of- Two television cameras operating in visible (0.6 micrometre) and near-infrared (0.8 micrometre) and collected data related to hydrology, forestry and geology. Satellite microwave radiometer (SAMIR) operating at 19 GHz and 22 GHz for study of ocean-state, water vapor, liquid water content in the atmosphere, etc. The satellite provided ocean and land surface data. Housekeeping telemetry was received until re-entry on 17 February 1989.
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												  NISAR Science Workshop – 2014Science Workshop – 2014 NISAR Space Applications Centre NISAR Mission Overview Tapan Misra (ISRO) & Paul Rosen (JPL) Space Applications Centre (SAC) NASA ISRO Synthetic Aperture Radar (NISAR) NISAR Mission Overview Payload / Mission Characteristics Would Enable 1 L-band (24 cm wavelength) Low temporal decorrelation and foliage penetration 2 S-band (12 cm wavelength) Sensitivity to light vegetation 3 SweepSAR technique with Imaging Swath > Global data collection 240 km 4 Polarimetry (Single/Dual/Quad) Surface characterization and biomass estimation 5 12-day exact repeat Rapid Sampling 6 3 – 10 meters mode-dependent SAR resolution Small-scale observations 7 3 years science operations (5 years Time-series analysis consumables) 8 Pointing control < 273 arcseconds Deformation interferometry 9 Orbit control < 500 meters Deformation interferometry 10 > 30% observation duty cycle Complete land/ice coverage 11 Left/Right pointing capability Polar coverage, north and south th th *Mission Concept – Pre-decisional – for Planning and NISAR Science Workshop, SAC Ahmedabad – 17 & 18 Nov. 2014 2 Discussion Purposes Only Key Capabilities for NISAR Repeatable orbits and instrument pointing Swath width sufficient to cover ground-track spacing at equator Polarimetric synthetic aperture radar with “industry-standard” performance parameters valid over the full swath All imaging with the instrument boresight pointed 37 degrees off-nadir and +/- 90 degrees off the body-fixed velocity vector Orbit reconstruction to cm-scale accuracy for efficient interferometric processing and calibration Sufficient duty cycle and mission resources to strobe Earth’s land and ice on ascending and descending orbits each repeat cycle 24-hour turnaround on urgent retargeting and 5-hour latency for data designated as urgent th th *Mission Concept – Pre-decisional – for Planning and NISAR Science Workshop, SAC Ahmedabad – 17 & 18 Nov.
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												  Platforms & SensorsPLATFORMS & SENSORS Platform: the vehicle carrying the remote sensing device Sensor: the remote sensing device recording wavelengths of energy e.g. Aerial photography - the plane and the camera Satellite image example: Platform: Landsat (1, 5, 7 etc..) Sensor: Multispectral Sensor (MSS) or Thematic Mapper (TM) Selected satellite remote sensing systems NASA Visible Earth: long list Wim Bakker's website http://members.home.nl/wim.h.bakker http://earthobservatory.nasa.gov/IOTD/view.php?id=52174 1. Satellite orbits “Sun-synchronous” “Geostationary” Land monitoring Weather satellites ~ 700 km altitude ~ 30,000 km altitude Satellite orbits Geostationary / geosynchronous : 36,000 km above the equator, stays vertically above the same spot, rotates with earth - weather images, e.g. GOES (Geostat. Operational Env. Satellite) Sun-synchronous satellites: 700-900 km altitude, rotates at circa 81-82 degree angle to equator: captures imagery approx the same time each day (10am +/- 30 minutes) - Landsat path: earthnow Sun-synchronous Graphic: http://ccrs.nrcan.gc.ca/resource/tutor/datarecept/c1p2_e.php 700-900 km altitude rotates at ~ 81-82 ° angle to the equator (near polar): captures imagery the same time each day (10.30am +/- 30 minutes) - for earth mapping Orbit every 90-100 minutes produces similar daytime lighting Geostationary satellites capture a (rectangular) scene, sun-synchronous satellites capture a continuous swath, … which is broken into rectangular scenes. 2. Scanner types Whiskbroom (mirror/ cross-track): a small number of sensitive diodes for each band sweep perpendicular to the path or swath, centred directly under the platform, i.e. at 'nadir' e.g. LANDSAT MSS /TM Pushbroom (along-track): an array of diodes (one for each column of pixels) is 'pointed' in a selected direction, nadir or off-nadir, on request, usually 0-30 degrees (max.), e.g.
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												  EDITOR's in This Issuervin bse g S O ys th t r e a m E THE EARTH OBSERVER May/June 2001 Vol. 13 No. 3 In this issue . EDITOR’S SCIENCE MEETINGS Joint Advanced Microwave Scanning Michael King Radiometer (AMSR) Science Team EOS Senior Project Scientist Meeting. 3 Clouds and The Earth’s Radiant Energy I’m pleased to announce that NASA’s Earth Science Enterprise is sponsoring System (CERES) Science Team Meeting a problem for the Odyssey of the Mind competitions during the 2001-2002 . 9 school year. It is a technical problem involving an original performance about environmental preservation. The competitions will involve about The ACRIMSAT/ACRIM3 Experiment — 450,000 students from kindergarten through college worldwide, and will Extending the Precision, Long-Term Total culminate in a World Finals next May in Boulder, CO where the “best of the Solar Irradiance Climate Database . .14 best” will compete for top awards in the international competitions. It is estimated that we reach 1.5 to 2 million students, parents, teachers/ SCIENCE ARTICLES administrators, coaches, etc. internationally through participation in this Summary of the International Workshop on LAI Product Validation. 18 program. An Introduction to the Federation of Earth The Odyssey of the Mind Program fosters creative thinking and problem- Science Information Partners . 19 solving skills among participating students from kindergarten through col- lege. Students solve problems in a variety of areas from building mechanical Tools and Systems for EOS Data . 23 devices such as spring-driven vehicles to giving their own interpretation of literary classics. Through solving problems, students learn lifelong skills Status and Plans for HDF-EOS, NASA’s such as working with others as a team, evaluating ideas, making decisions, Format for EOS Standard Products .
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												  Indian Remote Sensing Satellites (IRS)Topic: Indian Remote Sensing Satellites (IRS) Course: Remote Sensing and GIS (CC-11) M.A. Geography (Sem.-3) By Dr. Md. Nazim Professor, Department of Geography Patna College, Patna University Lecture-5 Concept: India's remote sensing program was developed with the idea of applying space technologies for the benefit of human kind and the development of the country. The program involved the development of three principal capabilities. The first was to design, build and launch satellites to a sun synchronous orbit. The second was to establish and operate ground stations for spacecraft control, data transfer along with data processing and archival. The third was to use the data obtained for various applications on the ground. India demonstrated the ability of remote sensing for societal application by detecting coconut root-wilt disease from a helicopter mounted multispectral camera in 1970. This was followed by flying two experimental satellites, Bhaskara-1 in 1979 and Bhaskara-2 in 1981. These satellites carried optical and microwave payloads. India's remote sensing programme under the Indian Space Research Organization (ISRO) started off in 1988 with the IRS-1A, the first of the series of indigenous state-of-art operating remote sensing satellites, which was successfully launched into a polar sun-synchronous orbit on March 17, 1988 from the Soviet Cosmodrome at Baikonur. It has sensors like LISS-I which had a spatial resolution of 72.5 meters with a swath of 148 km on ground. LISS-II had two separate imaging sensors, LISS-II A and LISS-II B, with spatial resolution of 36.25 meters each and mounted on the spacecraft in such a way to provide a composite swath of 146.98 km on ground.