GST Responses to “Questions to Inform Development of the National 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. -
New Millennium Program
NASA Facts National Aeronautics and Space Administration Jet Propulsion Laboratory California Institute of Technology Pasadena, CA 91109 New Millennium Program NASA's New Millennium program, a series of discerning trends, examining planetary climates and missions to test cutting-edge technologies never atmospheres, or landing to study such surface phe- before flown, will pave the way for a 21st century nomena as seismic and meteorological activity. Other fleet of affordable, frequently launched spacecraft sets of spacecraft could form a constellation uniquely perhaps 10 to suited to study 15 per year solar systems with highly beyond our own. focused sci- These goals ence objec- require significant tives. changes in almost New all aspects of Millennium spacecraft design will develop and deployment. and validate New Millennium the essential experimental tech- technologies nology flights will and capabilities validate key tech- required for nologies required these new to move toward. types of mis- Testing these sions. The pro- technologies in gram is flight will speed designed to ini- up their infusion tiate a revolu- New Millenniums Deep Space 1 will test ion propulsion and other technologies into the market- tionary new when the spacecraft flies by an asteroid and later possibly a comet (above). place. Some of way of explor- the space instru- ing Earth, the solar system and astrophysical events in ments of tomorrow may become as small and light- and far beyond the Milky Way galaxy. These new weight as a pocket wallet. missions will ensure NASA's technological readiness Drawing on diverse sectors of the country's sci- for post-2000 space and Earth science missions. -
Statement by Lynn Cline, United States Representative on Agenda
Statement by Kevin Conole, United States Representative, on Agenda Item 7, “Matters Related to Remote Sensing of the Earth by Satellite, Including Applications for Developing Countries and Monitoring of the Earth’s Environment” -- February 12, 2020 Thank you, Madame Chair and distinguished delegates. The United States is committed to maintaining space as a stable and productive environment for the peaceful uses of all nations, including the uses of space-based observation and monitoring of the Earth’s environment. The U.S. civil space agencies partner to achieve this goal. NASA continues to operate numerous satellites focused on the science of Earth’s surface and interior, water and energy cycles, and climate. The National Oceanic and Atmospheric Administration (or NOAA) operates polar- orbiting, geostationary, and deep space terrestrial and space weather satellites. The U.S. Geological Survey (or USGS) operates the Landsat series of land-imaging satellites, extending the nearly forty-eight year global land record and serving a variety of public uses. This constellation of research and operational satellites provides the world with high-resolution, high-accuracy, and sustained Earth observation. Madame Chair, I will now briefly update the subcommittee on a few of our most recent accomplishments under this agenda item. After a very productive year of satellite launches in 2018, in 2019 NASA brought the following capabilities on- line for research and application users. The ECOsystem Spaceborne Thermal Radiometer Experiment on the International Space Station (ISS) has been used to generate three high-level products: evapotranspiration, water use efficiency, and the evaporative stress index — all focusing on how plants use water. -
High-Temporal-Resolution Water Level and Storage Change Data Sets for Lakes on the Tibetan Plateau During 2000–2017 Using Mult
Earth Syst. Sci. Data, 11, 1603–1627, 2019 https://doi.org/10.5194/essd-11-1603-2019 © Author(s) 2019. This work is distributed under the Creative Commons Attribution 4.0 License. High-temporal-resolution water level and storage change data sets for lakes on the Tibetan Plateau during 2000–2017 using multiple altimetric missions and Landsat-derived lake shoreline positions Xingdong Li1, Di Long1, Qi Huang1, Pengfei Han1, Fanyu Zhao1, and Yoshihide Wada2 1State Key Laboratory of Hydroscience and Engineering, Department of Hydraulic Engineering, Tsinghua University, Beijing, China 2International Institute for Applied Systems Analysis (IIASA), 2361 Laxenburg, Austria Correspondence: Di Long ([email protected]) Received: 21 February 2019 – Discussion started: 15 March 2019 Revised: 4 September 2019 – Accepted: 22 September 2019 – Published: 28 October 2019 Abstract. The Tibetan Plateau (TP), known as Asia’s water tower, is quite sensitive to climate change, which is reflected by changes in hydrologic state variables such as lake water storage. Given the extremely limited ground observations on the TP due to the harsh environment and complex terrain, we exploited multiple altimetric mis- sions and Landsat satellite data to create high-temporal-resolution lake water level and storage change time series at weekly to monthly timescales for 52 large lakes (50 lakes larger than 150 km2 and 2 lakes larger than 100 km2) on the TP during 2000–2017. The data sets are available online at https://doi.org/10.1594/PANGAEA.898411 (Li et al., 2019). With Landsat archives and altimetry data, we developed water levels from lake shoreline posi- tions (i.e., Landsat-derived water levels) that cover the study period and serve as an ideal reference for merging multisource lake water levels with systematic biases being removed. -
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. -
NASA Earth Science Research Missions NASA Observing System INNOVATIONS
NASA’s Earth Science Division Research Flight Applied Sciences Technology NASA Earth Science Division Overview AMS Washington Forum 2 Mayl 4, 2017 FY18 President’s Budget Blueprint 3/2017 (Pre)FormulationFormulation FY17 Program of Record (Pre)FormulationFormulation Implementation MAIA (~2021) Implementation MAIA (~2021) Landsat 9 Landsat 9 Primary Ops Primary Ops TROPICS (~2021) (2020) TROPICS (~2021) (2020) Extended Ops PACE (2022) Extended Ops XXPACE (2022) geoCARB (~2021) NISAR (2022) geoCARB (~2021) NISAR (2022) SWOT (2021) SWOT (2021) TEMPO (2018) TEMPO (2018) JPSS-2 (NOAA) JPSS-2 (NOAA) InVEST/Cubesats InVEST/Cubesats Sentinel-6A/B (2020, 2025) RBI, OMPS-Limb (2018) Sentinel-6A/B (2020, 2025) RBI, OMPS-Limb (2018) GRACE-FO (2) (2018) GRACE-FO (2) (2018) MiRaTA (2017) MiRaTA (2017) Earth Science Instruments on ISS: ICESat-2 (2018) Earth Science Instruments on ISS: ICESat-2 (2018) CATS, (2020) RAVAN (2016) CATS, (2020) RAVAN (2016) CYGNSS (>2018) CYGNSS (>2018) LIS, (2020) IceCube (2017) LIS, (2020) IceCube (2017) SAGE III, (2020) ISS HARP (2017) SAGE III, (2020) ISS HARP (2017) SORCE, (2017)NISTAR, EPIC (2019) TEMPEST-D (2018) SORCE, (2017)NISTAR, EPIC (2019) TEMPEST-D (2018) TSIS-1, (2018) TSIS-1, (2018) TCTE (NOAA) (NOAA’S DSCOVR) TCTE (NOAA) (NOAA’SXX DSCOVR) ECOSTRESS, (2017) ECOSTRESS, (2017) QuikSCAT (2017) RainCube (2018*) QuikSCAT (2017) RainCube (2018*) GEDI, (2018) CubeRRT (2018*) GEDI, (2018) CubeRRT (2018*) OCO-3, (2018) CIRiS (2018*) OCOXX-3, (2018) CIRiS (2018*) CLARREO-PF, (2020) EOXX-1 CLARREOXX XX-PF, (2020) EOXX-1 -
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 -
Spaceborne Remote Sensing Ϩ ROBERT E
DECEMBER 2008 DAVISETAL. 1427 NASA Cold Land Processes Experiment (CLPX 2002/03): Spaceborne Remote Sensing ϩ ROBERT E. DAVIS,* THOMAS H. PAINTER, DON CLINE,# RICHARD ARMSTRONG,@ TERRY HARAN,@ ϩ KYLE MCDONALD,& RICK FORSTER, AND KELLY ELDER** * Cold Regions Research and Engineering Laboratory, U.S. Army Corps of Engineers, Hanover, New Hampshire ϩ Department of Geography, University of Utah, Salt Lake City, Utah #National Operational Remote Sensing Hydrology Center, National Weather Service, Chanhassen, Minnesota @ National Snow and Ice Data Center, University of Colorado, Boulder, Colorado & Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California ** Rocky Mountain Research Station, USDA Forest Service, Fort Collins, Colorado (Manuscript received 26 April 2007, in final form 15 January 2008) ABSTRACT This paper describes satellite data collected as part of the 2002/03 Cold Land Processes Experiment (CLPX). These data include multispectral and hyperspectral optical imaging, and passive and active mi- crowave observations of the test areas. The CLPX multispectral optical data include the Advanced Very High Resolution Radiometer (AVHRR), the Landsat Thematic Mapper/Enhanced Thematic Mapper Plus (TM/ETMϩ), the Moderate Resolution Imaging Spectroradiometer (MODIS), and the Multi-angle Imag- ing Spectroradiometer (MISR). The spaceborne hyperspectral optical data consist of measurements ac- quired with the NASA Earth Observing-1 (EO-1) Hyperion imaging spectrometer. The passive microwave data include observations from the Special Sensor Microwave Imager (SSM/I) and the Advanced Micro- wave Scanning Radiometer (AMSR) for Earth Observing System (EOS; AMSR-E). Observations from the Radarsat synthetic aperture radar and the SeaWinds scatterometer flown on QuikSCAT make up the active microwave data. 1. Introduction erties, land cover, and terrain. -
Statement by Lynn Cline, United States Representative on Agenda
Statement by Kevin Conole, United States Representative, on Agenda Item 6, “Matters Related to Remote Sensing of the Earth by Satellite, Including Applications for Developing Countries and Monitoring of the Earth’s Environment” -- April 27, 2021 Thank you, Madame Chair. The United States is committed to maintaining space as a stable and productive environment for the peaceful uses of all nations, including the uses of space-based observation and monitoring of the Earth’s environment. The U.S. civil space agencies partner together to achieve this goal. NASA continues to operate numerous satellites focused on the science of Earth’s surface and interior, water and energy cycles, and climate. NOAA operates polar- orbiting, geostationary, and deep space terrestrial and space weather satellites. USGS operates the Landsat series of land imaging satellites, extending Landsat’s nearly 50-year history of –recording the Earth’s surface and serving a variety of public uses. This constellation of research and operational satellites provides the world with high quality, sustained observations of our Earth’s, lands, interior, oceans, and atmosphere. Madame Chair, throughout the last year, NASA expanded the use of Earth observations of basic and applied research. 2020 culminated with the launch of the Sentinel-6 Michael Freilich spacecraft on November 10th. As a historic U.S.- European partnership, the Sentinel-6 Michael Freilich spacecraft will begin a five- and-a-half-year prime mission to collect the most accurate data yet on global sea levels and on how our oceans are rising in response to climate change. The mission will also collect precise data of atmospheric temperature and humidity that will help improve weather forecasts and climate models. -
Artificial Intelligence at the Jet Propulsion Laboratory
AI Magazine Volume 18 Number 1 (1997) (© AAAI) Articles Making an Impact Artificial Intelligence at the Jet Propulsion Laboratory Steve Chien, Dennis DeCoste, Richard Doyle, and Paul Stolorz ■ The National Aeronautics and Space Administra- described here is in the context of the remote- tion (NASA) is being challenged to perform more agent autonomy technology experiment that frequent and intensive space-exploration mis- will fly on the New Millennium Deep Space sions at greatly reduced cost. Nowhere is this One Mission in 1998 (a collaborative effort challenge more acute than among robotic plane- involving JPL and NASA Ames). Many of the tary exploration missions that the Jet Propulsion AI technologists who work at NASA expected Laboratory (JPL) conducts for NASA. This article describes recent and ongoing work on spacecraft to have the opportunity to build an intelli- autonomy and ground systems that builds on a gent spacecraft at some point in their careers; legacy of existing success at JPL applying AI tech- we are surprised and delighted that it has niques to challenging computational problems in come this early. planning and scheduling, real-time monitoring By the year 2000, we expect to demonstrate and control, scientific data analysis, and design NASA spacecraft possessing on-board automat- automation. ed goal-level closed-loop control in the plan- ning and scheduling of activities to achieve mission goals, maneuvering and pointing to execute these activities, and detecting and I research and technology development resolving of faults to continue the mission reached critical mass at the Jet Propul- without requiring ground support. At this Asion Laboratory (JPL) about five years point, mission accomplishment can begin to ago. -
PALSAR-FBS L-HH Mode and Landsat-TM Data Fusion for Geological Mapping
Advances in Remote Sensing, 2016, 5, 246-268 http://www.scirp.org/journal/ars ISSN Online: 2169-2688 ISSN Print: 2169-267X PALSAR-FBS L-HH Mode and Landsat-TM Data Fusion for Geological Mapping Abderrazak Bannari1, Ali El-Battay1, Ali Saquaque2, Abdelhafid Miri2 1Department of Geoinformatics, Arabian Gulf University, Manama, Kingdom of Bahrain 2Managem Mineral ONA Group, Twin Center, Casablanca, Kingdom of Morocco How to cite this paper: Bannari, A., El- Abstract Battay, A., Saquaque, A. and Miri, A. (2016) PALSAR-FBS L-HH Mode and Landsat-TM Characterized by lithological diversity and rich mineral resources, Benshangul-Gu- Data Fusion for Geological Mapping. Ad- muz National Regional State located in Asosa Zones, Western Ethiopia has been in- vances in Remote Sensing, 5, 246-268. vestigated for geological mapping and morpho-structural lineaments extraction us- http://dx.doi.org/10.4236/ars.2016.54020 ing PALSAR (Phased Array type L-band Synthetic Aperture Radar) Fine Beam Single Received: October 12, 2016 (FBS) L-HH polarization and Landsat-5 TM (Thematic Mapper) datasets. These data Accepted: November 18, 2016 were preprocessed to retrieve ground surface reflectance and backscatter coefficients. Published: November 21, 2016 To overcome the geometry acquisition between the two sensors, they were geometri- cally and topographically rectified using ASTER-V2 DEM. Intensity-Hue-Saturation, Copyright © 2016 by authors and directional filters and automatic lineaments extraction were applied on the datasets Scientific Research Publishing Inc. This work is licensed under the Creative for lithological units’ discrimination and structural delimitation for potential mineral Commons Attribution International exploration. The obtained results showed good relationship among the topographic License (CC BY 4.0). -
ISSUE 134, AUGUST 2013 2 Imperative: Venus Continued
Imperative: Venus — Virgil L. Sharpton, Lunar and Planetary Institute Venus and Earth began as twins. Their sizes and densities are nearly identical and they stand out as being considerably more massive than other terrestrial planetary bodies. Formed so close to Earth in the solar nebula, Venus likely has Earth-like proportions of volatiles, refractory elements, and heat-generating radionuclides. Yet the Venus that has been revealed through exploration missions to date is hellishly hot, devoid of oceans, lacking plate tectonics, and bathed in a thick, reactive atmosphere. A less Earth-like environment is hard to imagine. Venus, Earth, and Mars to scale. Which L of our planetary neighbors is most similar to Earth? Hint: It isn’t Mars. PWhy and when did Earth’s and Venus’ evolutionary paths diverge? This fundamental and unresolved question drives the need for vigorous new exploration of Venus. The answer is central to understanding Venus in the context of terrestrial planets and their evolutionary processes. In addition, however, and unlike virtually any other planetary body, Venus could hold important clues to understanding our own planet — how it has maintained a habitable environment for so long and how long it can continue to do so. Precisely because it began so like Earth, yet evolved to be so different, Venus is the planet most likely to cast new light on the conditions that determine whether or not a planet evolves habitable environments. NASA’s Kepler mission and other concurrent efforts to explore beyond our star system are likely to find Earth-sized planets around Sun-sized stars within a few years.