Space Agency Response to GCOS Implementation Plan
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Using Earth Observation Data to Improve Health in the United States Accomplishments and Future Challenges
a report of the csis technology and public policy program Using Earth Observation Data to Improve Health in the United States accomplishments and future challenges 1800 K Street, NW | Washington, DC 20006 Tel: (202) 887-0200 | Fax: (202) 775-3199 Author E-mail: [email protected] | Web: www.csis.org Lyn D. Wigbels September 2011 ISBN 978-0-89206-668-1 Ë|xHSKITCy066681zv*:+:!:+:! a report of the csis technology and public policy program Using Earth Observation Data to Improve Health in the United States accomplishments and future challenges Author Lyn D. Wigbels September 2011 About CSIS At a time of new global opportunities and challenges, the Center for Strategic and International Studies (CSIS) provides strategic insights and bipartisan policy solutions to decisionmakers in government, international institutions, the private sector, and civil society. A bipartisan, nonprofit organization headquartered in Washington, D.C., CSIS conducts research and analysis and devel- ops policy initiatives that look into the future and anticipate change. Founded by David M. Abshire and Admiral Arleigh Burke at the height of the Cold War, CSIS was dedicated to finding ways for America to sustain its prominence and prosperity as a force for good in the world. Since 1962, CSIS has grown to become one of the world’s preeminent international policy institutions, with more than 220 full-time staff and a large network of affiliated scholars focused on defense and security, regional stability, and transnational challenges ranging from energy and climate to global development and economic integration. Former U.S. senator Sam Nunn became chairman of the CSIS Board of Trustees in 1999, and John J. -
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. -
GST Responses to “Questions to Inform Development of the National Plan”
GST Responses to “Questions to Inform Development of the National Plan” Name (optional): Dr. Darrel Williams Position (optional): Chief Scientist, (240) 542-1106; [email protected] Institution (optional): Global Science & Technology, Inc. Greenbelt, Maryland 20770 Global Science & Technology, Inc. (GST) is pleased to provide the following answers as a contribution towards OSTP’s effort to develop a national plan for civil Earth observations. In our response we provide information to support three main themes: 1. There is strong science need for high temporal resolution of moderate spatial resolution satellite earth observation that can be achieved with cost effective, innovative new approaches. 2. Operational programs need to be designed to obtain sustained climate data records. Continuity of Earth observations can be achieved through more efficient and economical means. 3. We need programs to address the integration of remotely sensed data with in situ data. GST has carefully considered these important national Earth observation issues over the past few years and has submitted the following RFI responses: The USGS RFI on Landsat Data Continuity Concepts (April 2012), NASA’s Sustainable Land Imaging Architecture RFI (September 2013), and This USGEO RFI (November 2013) relative to OSTP’s efforts to develop a national plan for civil Earth observations. In addition to the above RFI responses, GST led the development of a mature, fully compliant flight mission concept in response to NASA’s Earth Venture-2 RFP in September 2011. Our capacity to address these critical national issues resides in GST’s considerable bench strength in Earth science understanding (Drs. Darrel Williams, DeWayne Cecil, Samuel Goward, and Dixon Butler) and in NASA systems engineering and senior management oversight (Drs. -
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. -
Carbon Earth Observatory for Carbon Dioxide Reduction Robert D
Carbon Earth Observatory for Carbon Dioxide Reduction Robert D. Cormia Foothill College GHG Emissions / NET Strategies Terrestrial Options for Negative Emissions Earth System Observation Data Platform Technology (NET) The messaging from IPCC is clear; without significant and sustained • Argo • OCO-2/OCO-3 Carbon Dioxide Reduction (CDR) strategies, there is no realistic • Afforestation and reforestation, stop deforestation, • Aqua • GOSAT 2 chance of avoiding potentially disastrous climate change. increase biomass of forest and soils for decades In addition to emission reduction, “drawdown” of atmospheric • Terra • ECOSTRESS carbon dioxide must begin soon and remain in place through the • Monitor and enhance grassland productivity and • CloudSat • GEDI end of the century. There are carbon sinks in the terrestrial carbon sequestration, including hydrology • CALIPSO • LandSat biosphere that have the potential to remove gigatons of carbon Improve soil microbial activity, carbon uptake in soils, dioxide each year, for decades or more. An earth observatory • • SMAP • TROPOMI system, for analysis of carbon cycle processes throughout the userecommended management practices • ICESat-2 • GeoCARB (2022) biosphere, could help measure, inform, and optimize terrestrial • Restore wetlands and connect to ocean inlet to increase carbon sequestration projects. salinity and decrease methane emissions NASA Earth Observing System (EOS) • Enhance Net Primary Productivity (NPP) of oceans Integrated toolset to help achieve CDR Goals NASA’s Earth Observatory tools are designed for accurate and precise measurements of atmospheric gases, geometric aspects of land and biomass, and can sense biochemical changes in plants and biomass that may result from climate change. If we are to be effective in optimizing carbon dioxide reduction projects, we need an integrated data platform with both spatial and temporal resolution. -
Complete List of Contents
Complete List of Contents Volume 1 Cape Canaveral and the Kennedy Space Center ......213 Publisher’s Note ......................................................... vii Chandra X-Ray Observatory ....................................223 Introduction ................................................................. ix Clementine Mission to the Moon .............................229 Preface to the Third Edition ..................................... xiii Commercial Crewed vehicles ..................................235 Contributors ............................................................. xvii Compton Gamma Ray Observatory .........................240 List of Abbreviations ................................................. xxi Cooperation in Space: U.S. and Russian .................247 Complete List of Contents .................................... xxxiii Dawn Mission ..........................................................254 Deep Impact .............................................................259 Air Traffic Control Satellites ........................................1 Deep Space Network ................................................264 Amateur Radio Satellites .............................................6 Delta Launch Vehicles .............................................271 Ames Research Center ...............................................12 Dynamics Explorers .................................................279 Ansari X Prize ............................................................19 Early-Warning Satellites ..........................................284 -
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. -
An Overview of the Seawifs Project and Strategies for Producing a Climate Research Quality Global Ocean Bio-Optical Time Series
ARTICLE IN PRESS Deep-Sea Research II 51 (2004) 5–42 An overview of the SeaWiFS project andstrategies for producing a climate research quality global ocean bio-optical time series Charles R. McClain*, Gene C. Feldman, Stanford B. Hooker Code 970.2, Office for Global Carbon Studies, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA Received1 April 2003; accepted19 November 2003 Abstract The Sea-viewing Wide Field-of-view Sensor (SeaWiFS) Project Office was formally initiated at the NASA Goddard Space Flight Center in 1990. Seven years later, the sensor was launched by Orbital Sciences Corporation under a data- buy contract to provide 5 years of science quality data for global ocean biogeochemistry research. To date, the SeaWiFS program has greatly exceeded the mission goals established over a decade ago in terms of data quality, data accessibility andusability, ocean community infrastructure development,cost efficiency, andcommunity service. The SeaWiFS Project Office andits collaborators in the scientific community have madesubstantial contributions in the areas of satellite calibration, product validation, near-real time data access, field data collection, protocol development, in situ instrumentation technology, operational data system development, and desktop level-0 to level-3 processing software. One important aspect of the SeaWiFS program is the high level of science community cooperation andparticipation. This article summarizes the key activities andapproaches the SeaWiFS Project Office pursuedto define,achieve, and maintain the mission objectives. These achievements have enabledthe user community to publish a large andgrowing volume of research such as those contributedto this special volume of Deep-Sea Research. Finally, some examples of major geophysical events (oceanic, atmospheric, andterrestrial) capturedby SeaWiFS are presentedto demonstratethe versatility of the sensor.