GEOS 657 - Lecture 10
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Pre-Flight SAOCOM-1A SAR Performance Assessment by Outdoor Campaign
remote sensing Technical Note Pre-Flight SAOCOM-1A SAR Performance Assessment by Outdoor Campaign Davide Giudici 1, Andrea Monti Guarnieri 2 ID and Juan Pablo Cuesta Gonzalez 3,* 1 ARESYS srl, Via Flumendosa 16, 20132 Milan, Italy; [email protected] 2 Politecnico di Milano, Piazza Leonardo da Vinci 32, 20133 Milan, Italy; [email protected] 3 CONAE, Avda. Paseo Colon 751, 1063 Buenos Aires, Argentina * Correspondence: [email protected]; Tel.: +39-02-8724-4809 Academic Editors: Timo Balz, Uwe Soergel, Mattia Crespi, Batuhan Osmanoglu, Daniele Riccio and Prasad S. Thenkabail Received: 23 May 2017; Accepted: 12 July 2017; Published: 14 July 2017 Abstract: In the present paper, we describe the design, execution, and the results of an outdoor experimental campaign involving the Engineering Model of the first of the two Argentinean L-band Synthetic Aperture Radars (SARs) of the Satélite Argentino de Observación con Microondas (SAOCOM) mission, SAOCOM-1A. The experiment’s main objectives were to test the end-to-end SAR operation and to assess the instrument amplitude and phase stability as well as the far-field antenna pattern, through the illumination of a moving target placed several kilometers away from the SAR. The campaign was carried out in Bariloche, Argentina, during June 2016. The experiment was successful, demonstrating an end-to-end readiness of the SAOCOM-SAR functionality in realistic conditions. The results showed an excellent SAR signal quality in terms of amplitude and phase stability. Keywords: SAR; pre-flight testing; SAR performance 1. Introduction The forthcoming Argentinean mission Satélite Argentino de Observación con Microondas (SAOCOM) [1] is constituted by two identical Low-Earth-Orbit (LEO) satellites, SAOCOM-1A and -1B, carrying as the main payload an L-band Synthetic Aperture Radar (SAR). -
Appendix C: Insar
Dirty Little Secrets about InSAR [EarthScope 2009] C-band interferograms are decorrelated over most of the SAF and Cascadia except urban areas. Envisat is almost out of fuel and the C-band replacement is a few years away. L-band ALOS has almost no data on descending tracks. L-band ALOS has ionospheric phase variations are +/- 10 cm on some interferograms. L-band ALOS has poor orbit control (but excellent orbit occuracy). Less than 2% of the 17 Tbytes of GeoEarthScope data has been downloaded. DESDYNI the US InSAR mission will launch in 2019 (40 years after Seasat). Open source InSAR software is not of “geodetic” quality. Dirty Little Secrets about InSAR [Today] C-band interferograms are decorrelated over most of the SAF and Cascadia except urban areas. Sentinel-1A and B are both functioning. They operate in TOPS mode which is a nightmare! < 10 cm accuracy orbits are essential. L-band ALOS-1 has almost no data on descending tracks. L-band ALOS-/2 has ionospheric phase variations are +/- 100 cm on some interferograms. L-band ALOS has poor orbit control (but excellent orbit occuracy). ALOS-2 data ree morerestricted than ALOS-1 NISAR the US InSAR mission will launch in 2021 (43 years after Seasat). NISAR is only a 3-year mission! Open source InSAR software is getting better but contains some ugly code. Need a programmer to remove the deadwood and streamline the installation and testing. X-band 3 cm TerraSAR COSMO-SkyMed interferogram using data from 19 February 2009 and 9 April 2009. Perpendicular baseline is 480 m, and the satellite’s right-looking angle is 37 degrees. -
European Space Surveillance and Tracking
2ndEuropean EU SST Webinar: Space Operations in Space Surveillance and Tracking 16Surveillance November 2020 –and14h CETTracking The EU SST activities received funding from the European Union programmes, notably from the Horizon 2020 research and innovation programme under grant agreements No 760459, No 785257, No 713630, No 713762 and No 634943, and the Copernicus and Galileo programme under grant agreements No 299/G/GRO/COPE/19/11109, No 237/GRO/COPE/16/8935 and No 203/G/GRO/COPE/15/7987. This Portal reflects only the SST Cooperation’s actions and the European Commission and the Research Executive Agency are not responsible for any use that may be made of the information it contains. 2nd EU SST Webinar Operations in Space Surveillance and Tracking Speakers Pascal María Antonia Cristina Florian João FAUCHER (CNES) RAMOS (CDTI) PÉREZ (CDTI) DELMAS (CNES) ALVES (EU SatCen) Pier Luigi Lt. Moreno Juan Christophe Rodolphe RIGHETTI PERONI (IT MoD) ESCALANTE MORAND (EEAS) MUÑOZ (EUMETSAT) (EC – DG ECHO) (EC-DG DEFIS) 2nd EU SST Webinar: Operations in Space Surveillance and Tracking 16 November 2020 3 Agenda (1/2) 14h00-14h10: Welcome to the 2nd EU SST Webinar [Moderator: Mr Oliver Rajan (EU SatCen)] 14h10-14h50: SST Support Framework: Safeguarding European space infrastructure • Overview, governance model, security relevance and future perspectives [SST Cooperation Chair: Dr Pascal Faucher (CNES)] EU SST Architecture & Service Provision Model • Sensors network • Database and Catalogue precursor • Services [Chair of the SST Technical Committee: -
NASA's Earth Science Data Systems Program
NASA's Earth Science Data Systems Program Program Executive for Earth Science Data Systems Earth Science Division (DK) Science Mission Directorate, NASA Headquarters February 16, 2016 5/25/2016 1 NASA Strategic Plan 2014 • Objective 2.2: Advance knowledge of Earth as a system to meet the challenges of environmental change, and to improve life on our planet. – How is the global Earth system changing? What causes these changes in the Earth system? How will Earth’s systems change in the future? How can Earth system science provide societal benefits? – NASA’s Earth science programs shape an interdisciplinary view of Earth, exploring the interaction among the atmosphere, oceans, ice sheets, land surface interior, and life itself, which enables scientists to measure global climate changes and to inform decisions by Government, organizations, and people in the United States and around the world. We make the data collected and results generated by our missions accessible to other agencies and organizations to improve the products and services they provide… 5/25/2016 2 Major Components of the Earth Science Data Systems Program • Earth Observing System Data and Information System (EOSDIS) – Core systems for processing, ingesting and archiving data for the Earth Science Division • Competitively Selected Programs – Making Earth System Data Records for Use in Research Environments (MEaSUREs) – Advancing Collaborative Connections for Earth System Science (ACCESS) • International and Interagency Coordination and Development – CEOS Working Group on Information -
The Space-Based Global Observing System in 2010 (GOS-2010)
WMO Space Programme SP-7 The Space-based Global Observing For more information, please contact: System in 2010 (GOS-2010) World Meteorological Organization 7 bis, avenue de la Paix – P.O. Box 2300 – CH 1211 Geneva 2 – Switzerland www.wmo.int WMO Space Programme Office Tel.: +41 (0) 22 730 85 19 – Fax: +41 (0) 22 730 84 74 E-mail: [email protected] Website: www.wmo.int/pages/prog/sat/ WMO-TD No. 1513 WMO Space Programme SP-7 The Space-based Global Observing System in 2010 (GOS-2010) WMO/TD-No. 1513 2010 © World Meteorological Organization, 2010 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate these publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0)22 730 84 03 P.O. Box No. 2300 Fax: +41 (0)22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] FOREWORD The launching of the world's first artificial satellite on 4 October 1957 ushered a new era of unprecedented scientific and technological achievements. And it was indeed a fortunate coincidence that the ninth session of the WMO Executive Committee – known today as the WMO Executive Council (EC) – was in progress precisely at this moment, for the EC members were very quick to realize that satellite technology held the promise to expand the volume of meteorological data and to fill the notable gaps where land-based observations were not readily available. -
Improved Quality Control for Quikscat Near Real-Time Data
JP4.6 Improved Quality Control for QuikSCAT Near Real-time Data S. Mark Leidner, Ross N. Hoffman, and Mark C. Cerniglia Atmospheric and Environmental Research Inc., Lexington, Massachusetts Abstract errors. We will illustrate the types of errors that occur due to rain contamination and ambiguity removal. SeaWinds on QuikSCAT, launched in June 1999, We will also give examples of how the quality of the provides a new source of surface wind information retrieved winds varies across the satellite track, and over the world’s oceans. This new window on global varies with wind speed. surface vector winds has been a great aid to real- SeaWinds is an active, Ku-band microwave radar time operational users, especially in remote areas operating near ¢¤£¦¥¨§ © and is sensitive to centimeter- of the world. As with in situ observations, the qual- scale or capillary waves on the ocean surface. ity of remotely-sensed geophysical data is closely These waves are usually in equilibrium with the wind. tied to the characteristics of the instrument. But Each radar backscatter observation samples a patch remotely-sensed scatterometer winds also have a of ocean about . The vector wind is re- whole range of additional quality control concerns trieved by combining several backscatter observa- different from those of in situ observation systems. tions made from multiple viewing geometries as the The retrieval of geophysical information from the raw scatterometer passes overhead. The resolution of satellite measurements introduces uncertainties but the retrieved winds is . also produces diagnostics about the reliability of the Backscatter from capillary waves on the ocean retrieved quantities. -
Watching the Winds Where Sea Meets Sky 14 August 2014, by Rosalie Murphy
Watching the winds where sea meets sky 14 August 2014, by Rosalie Murphy the speed and direction of wind at the ocean's surface. "Before scatterometers, we could only measure ocean winds on ships, and sampling from ships is very limited," said Timothy Liu of NASA's Jet Propulsion Laboratory in Pasadena, California, who led the science team for NASA's QuikScat mission. Scatterometry began to emerge during World War II, when scientists realized wind disturbing the ocean's surface caused noise in their radar signals. NASA included an experimental scatterometer in its The SeaWinds scatterometer on NASA's QuikScat first space station in 1973 and again when it satellite stares into the eye of 1999's Hurricane Floyd as launched its SeaSat satellite in 1978. During its it hits the U.S. coast. The arrows indicate wind direction, three-month life, SeaSat's scatterometer provided while the colors represent wind speed, with orange and scientists with more individual wind observations yellow being the fastest. Credit: NASA/JPL-Caltech than ships had collected in the previous century. The ocean covers 71 percent of Earth's surface and affects weather over the entire globe. Hurricanes and storms that begin far out over the ocean affect people on land and interfere with shipping at sea. And the ocean stores carbon and heat, which are transported from the ocean to the air and back, allowing for photosynthesis and affecting Earth's climate. To understand all these processes, scientists need information about winds A JPL team then designed a mission called near the ocean's surface. -
Seasat—A 25-Year Legacy of Success
Remote Sensing of Environment 94 (2005) 384–404 www.elsevier.com/locate/rse Seasat—A 25-year legacy of success Diane L. Evansa,*, Werner Alpersb, Anny Cazenavec, Charles Elachia, Tom Farra, David Glackind, Benjamin Holta, Linwood Jonese, W. Timothy Liua, Walt McCandlessf, Yves Menardg, Richard Mooreh, Eni Njokua aJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, United States bUniversitaet Hamburg, Institut fuer Meereskunde, D-22529 Hamburg, Germany cLaboratoire d´Etudes en Geophysique et Oceanographie Spatiales, Centre National d´Etudes Spatiales, Toulouse 31401, France dThe Aerospace Corporation, Los Angeles, CA 90009, United States eCentral Florida Remote Sensing Laboratory, University of Central Florida, Orlando, FL 32816, United States fUser Systems Enterprises, Denver, CO 80220, United States gCentre National d´Etudes Spatiales, Toulouse 31401, France hThe University of Kansas, Lawrence, KS 66047-1840, United States Received 10 June 2004; received in revised form 13 September 2004; accepted 16 September 2004 Abstract Thousands of scientific publications and dozens of textbooks include data from instruments derived from NASA’s Seasat. The Seasat mission was launched on June 26, 1978, on an Atlas-Agena rocket from Vandenberg Air Force Base. It was the first Earth-orbiting satellite to carry four complementary microwave experiments—the Radar Altimeter (ALT) to measure ocean surface topography by measuring spacecraft altitude above the ocean surface; the Seasat-A Satellite Scatterometer (SASS), to measure wind speed and direction over the ocean; the Scanning Multichannel Microwave Radiometer (SMMR) to measure surface wind speed, ocean surface temperature, atmospheric water vapor content, rain rate, and ice coverage; and the Synthetic Aperture Radar (SAR), to image the ocean surface, polar ice caps, and coastal regions. -
Aqua Summary (As of May 31, 2019) • Spacecraft Bus – Nominal Operations (Excellent Health) ‒ All Components Remain on Primary Hardware
Aqua Summary (as of May 31, 2019) • Spacecraft Bus – Nominal Operations (Excellent Health) ‒ All components remain on primary hardware. ‒ 18 of 132 Solar Array Strings appear to have failed. See slide 2. Similar failures have occurred on Aura. ‒ Significant power generation margin remains. • MODIS – Nominal Operations (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ All components remain on primary hardware except 10W Lamps used for calibration. • AIRS – Nominal Operations (<10% of Channels degraded) – (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ ~200 of 2378 channels are degraded due to radiation, however they are still useful. ‒ Cooler-A Telemetry, frozen since a 3/28/2014 Anomaly, was restored during recovery activities performed on 9/27/2016. • AMSU-A – Nominal Operations for 9 of 15 Channels (Fair Health) ‒ All voltages, currents, and temperatures are as expected. ‒ 3 of 15 channels have been removed from Level 2 processing. 2 channels (#1 & #2) are unavailable. ‒ AMSU-A2 Anomaly on 9/24/2016 caused loss of Channels 1 and 2. The initial recovery attempts were unsuccessful. The instrument manufacturer recommends not switching to the A-side to attempt to recover AMSU-A2. ‒ AMSU-A1 Anomaly on 6/21/2018 caused unexplained shift in Channel 14. Channel 14 data have now been removed from processing, and the anomaly is considered closed. • CERES-AFT (FM-3) – Nominal Operations (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ Cross-Track and Biaxial Modes are fully functioning. ‒ All channels remain operational. • CERES-FORE (FM-4) – Nominal Operations (Good Health) ‒ All voltages, currents, and temperatures are as expected. -
RAPPORT D'activités ACTIVITÉS SPATIALES Depuis Le Conseil Ministériel De L'esa De Décembre 2014 À Luxembourg Et De Décembre 2016 À Lucerne
RAPPORT D’ACTIVITÉS ACTIVITÉS SPATIALES depuis le Conseil ministériel de l'ESA de décembre 2014 à Luxembourg et de décembre 2016 à Lucerne mars 2018 report 2018_FR_rev 1.doc 2 Table des matières 1 Introduction ................................................................................................................................... 4 2 Stratégie spatiale ............................................................................................................................ 8 3 Résumé des engagements programmatiques et des budgets........................................................... 9 4 Statut des Programmes de l'ESA ................................................................................................... 13 4.1 Activités de base ................................................................................................................... 13 4.2 Le Programme scientifique ................................................................................................... 14 4.3 Observation de la Terre ........................................................................................................ 15 4.4 Télécommunications ............................................................................................................ 19 4.5 Navigation ............................................................................................................................ 23 4.6 Vols habités, Microgravité et Exploration .............................................................................. 24 -
The Annual Compendium of Commercial Space Transportation: 2017
Federal Aviation Administration The Annual Compendium of Commercial Space Transportation: 2017 January 2017 Annual Compendium of Commercial Space Transportation: 2017 i Contents About the FAA Office of Commercial Space Transportation The Federal Aviation Administration’s Office of Commercial Space Transportation (FAA AST) licenses and regulates U.S. commercial space launch and reentry activity, as well as the operation of non-federal launch and reentry sites, as authorized by Executive Order 12465 and Title 51 United States Code, Subtitle V, Chapter 509 (formerly the Commercial Space Launch Act). FAA AST’s mission is to ensure public health and safety and the safety of property while protecting the national security and foreign policy interests of the United States during commercial launch and reentry operations. In addition, FAA AST is directed to encourage, facilitate, and promote commercial space launches and reentries. Additional information concerning commercial space transportation can be found on FAA AST’s website: http://www.faa.gov/go/ast Cover art: Phil Smith, The Tauri Group (2017) Publication produced for FAA AST by The Tauri Group under contract. NOTICE Use of trade names or names of manufacturers in this document does not constitute an official endorsement of such products or manufacturers, either expressed or implied, by the Federal Aviation Administration. ii Annual Compendium of Commercial Space Transportation: 2017 GENERAL CONTENTS Executive Summary 1 Introduction 5 Launch Vehicles 9 Launch and Reentry Sites 21 Payloads 35 2016 Launch Events 39 2017 Annual Commercial Space Transportation Forecast 45 Space Transportation Law and Policy 83 Appendices 89 Orbital Launch Vehicle Fact Sheets 100 iii Contents DETAILED CONTENTS EXECUTIVE SUMMARY . -
2019 Ocean Surface Topography Science Team Meeting Convene
2019 Ocean Surface Topography Science Team Meeting Convene Chicago 16 West Adams Street, Chicago, IL 60603 Monday, October 21 2019 - Friday, October 25 2019 The 2019 Ocean Surface Topography Meeting will occur 21-25 October 2019 and will include a variety of science and technical splinters. These will include a special splinter on the Future of Altimetry (chaired by the Project Scientists), a splinter on Coastal Altimetry, and a splinter on the recently launched CFOSAT. In anticipation of the launch of Jason-CS/Sentinel-6A approximately 1 year after this meeting, abstracts that support this upcoming mission are highly encouraged. Abstracts Book 1 / 259 Abstract list 2 / 259 Keynote/invited OSTST Opening Plenary Session Mon, Oct 21 2019, 09:00 - 12:35 - The Forum 12:00 - 12:20: How accurate is accurate enough?: Benoit Meyssignac 12:20 - 12:35: Engaging the Public in Addressing Climate Change: Patricia Ward Science Keynotes Session Mon, Oct 21 2019, 14:00 - 15:45 - The Forum 14:00 - 14:25: Does the large-scale ocean circulation drive coastal sea level changes in the North Atlantic?: Denis Volkov et al. 14:25 - 14:50: Marine heat waves in eastern boundary upwelling systems: the roles of oceanic advection, wind, and air-sea heat fluxes in the Benguela system, and contrasts to other systems: Melanie R. Fewings et al. 14:50 - 15:15: Surface Films: Is it possible to detect them using Ku/C band sigmaO relationship: Jean Tournadre et al. 15:15 - 15:40: Sea Level Anomaly from a multi-altimeter combination in the ice covered Southern Ocean: Matthis Auger et al.