Preparations for the Geostationary Imaging Fourier Transform
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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. -
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. -
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 -
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. -
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. -
Interference EESS NASA
National Aeronautics and Space Administration ITU International Satellite Symposium 2019 Bariloche, Argentina 25‐27 September 2019 Science Services and Harmful Interference Coralí Roura Senior Spectrum Regulatory and Policy Advisor NASA Headquarters 26 September 2019 James T. Higgins Arctic Slope Technical Services NASA Office Support www.nasa.gov Overview 1 Harmful Interference to Science Services 3 Worldwide Science Services Passive • What is “Harmful Interference”? Sensing Frequencies • Typical sources of interference to science 4 Worldwide Science Services Passive services Sensing Bands 2 Radio Frequency Interference to Science 5 Importance of Passive Sensing Services 6 Summary • Aqua Mission & AMSR‐E Instrument 7 Science Services: Passive and Active • Frequency bands affected by RFI on AMSR‐E Remote Sensing and AMSR2 • Video: NASA | Getting the Big Picture − RFI from Ground‐based 8 References − RFI from GSO satellite surface reflections, and direct broadcast satellites • General Impact to Measurements & Consequences of Interference • Radio Frequency Interference Mitigations 2 Harmful Interference to Science Services What is “Harmful Interference”? Typical sources of interference to science services • ITU‐R Radio Regulations Sec. 1.169 ‐ harmful • Authorized transmitters operating in shared bands interference: Interference which endangers the functioning of a radionavigation service • Unauthorized transmitters operating in the band or of other safety services or seriously • Unwanted emissions from systems operating in adjacent bands -
Aquarius User Guide
AQUARIUS USER GUIDE Aquarius Dataset Version 3.0 Guide Version: 6.0 June 2, 2014 Revision: 19 Document #s: JPL D-70012 AQ-010-UG-0008 JPL URS CL#: 14-0748 National Aeronautics and Space Administration Physical Oceanography Distributed Active Archive Center (PO.DAAC) Jet Propulsion Laboratory 4800 Oak Grove Drive Pasadena, California 91109-8099 California Institute of Technology © 2014 California Institute of Technology. Government sponsorship acknowledged. Document Change Record Author Reason for Change Pages/paragraphs changed Date of revision Gregg Foti 1. Original Draft All 11 Aug. 2011 Chris Finch 2. Clean up section 4.2, other minor edits All 16 Sep. 2011 3. Changed footprint sizes of radiometer J. Vazquez 6,7 20 Oct 2011 and scatterometer J. Vazquez 4. Updated table on Level 3 metadata 25 Jan 2012 V. Tsontos 5. Editorial review 26 Jan 2012 6. Update of Level 2 metadata variables V. Tsontos associated with the release of version 29 16 Mar. 2012 1.2.2 of the Aquarius dataset 7. Update of Level 2 metadata variables V. Tsontos associated with the release of version 29 16 Mar. 2012 1.2.3 of the Aquarius dataset V. Tsontos 8. Added copyright information to title page 1 22 Mar. 2012 9. Updated Level 2 & 3 metadata for V. Tsontos version 1.2.3 of the Aquarius dataset. Various 29 Mar. 2012 Formatting improvements. 10. Updated Level 2 & 3 metadata for V. Tsontos Various 20 Apr. 2012 version 1.3 of the Aquarius dataset. 11. Updated Level 2 scatterometer-related descriptions based on information from Section 4.2 & associated tables V. -
Earth Observing System, Volume Iia: Data and Information System, Report of the EOS Data Panel
Publications 1986 Earth Observing System, volume IIa: Data and Information System, Report of the EOS Data Panel Raymond Arvidson Washington University Frederick Billingsley Jet Propulsion Labortory Robert Chase Woods Hole Oceanographic Institution Pat Chavez Jr. United States Geological Service Michael Devirian NASA Headquarters See next page for additional authors Follow this and additional works at: https://commons.erau.edu/publication Part of the Atmospheric Sciences Commons, and the Meteorology Commons Scholarly Commons Citation Arvidson, R., Billingsley, F., Chase, R., Chavez, P., Devirian, M., Mosher, F., & et al. (1986). Earth Observing System, volume IIa: Data and Information System, Report of the EOS Data Panel. , (). Retrieved from https://commons.erau.edu/publication/551 This Report is brought to you for free and open access by Scholarly Commons. It has been accepted for inclusion in Publications by an authorized administrator of Scholarly Commons. For more information, please contact [email protected]. Authors Raymond Arvidson, Frederick Billingsley, Robert Chase, Pat Chavez Jr., Michael Devirian, Frederick Mosher, and et al. This report is available at Scholarly Commons: https://commons.erau.edu/publication/551 https://ntrs.nasa.gov/search.jsp?R=19860021622 2017-10-09T16:01:38+00:00Z NASA-TM-87777 19860021622 Volumella EliATH []BSEAU~~IJ SYSTEr:1 LIBRARY COpy LANGLEY RESEARCH CENTER LIBRARY, NASA HAMPTON. VIRGINIA REP[]RT []F THE E[]S lJfiTfi Pfi~El NAS/\ National Aeronautics and Space Administration 1986 Technical Memorandum -
Global Precipitation Measurement (Gpm) Mission
GLOBAL PRECIPITATION MEASUREMENT (GPM) MISSION Algorithm Theoretical Basis Document GPROF2017 Version 1 (used in GPM V5 processing) June 1st, 2017 Passive Microwave Algorithm Team Facility TABLE OF CONTENTS 1.0 INTRODUCTION 1.1 OBJECTIVES 1.2 PURPOSE 1.3 SCOPE 1.4 CHANGES FROM PREVIOUS VERSION – GPM V5 RELEASE NOTES 2.0 INSTRUMENTATION 2.1 GPM CORE SATELITE 2.1.1 GPM Microwave Imager 2.1.2 Dual-frequency Precipitation Radar 2.2 GPM CONSTELLATIONS SATELLTES 3.0 ALGORITHM DESCRIPTION 3.1 ANCILLARY DATA 3.1.1 Creating the Surface Class Specification 3.1.2 Global Model Parameters 3.2 SPATIAL RESOLUTION 3.3 THE A-PRIORI DATABASES 3.3.1 Matching Sensor Tbs to the Database Profiles 3.3.2 Ancillary Data Added to the Profile Pixel 3.3.3 Final Clustering of Binned Profiles 3.3.4 Databases for Cross-Track Scanners 3.4 CHANNEL AND CHANNEL UNCERTAINTIES 3.5 PRECIPITATION PROBABILITY THRESHOLD 3.6 PRECIPITATION TYPE (Liquid vs. Frozen) DETERMINATION 4.0 ALGORITHM INFRASTRUCTURE 4.1 ALGORITHM INPUT 4.2 PROCESSING OUTLINE 4.2.1 Model Preparation 4.2.2 Preprocessor 4.2.3 GPM Rainfall Processing Algorithm - GPROF 2017 4.2.4 GPM Post-processor 4.3 PREPROCESSOR OUTPUT 4.3.1 Preprocessor Orbit Header 2 4.3.2 Preprocessor Scan Header 4.3.3 Preprocessor Data Record 4.4 GPM PRECIPITATION ALGORITHM OUTPUT 4.4.1 Orbit Header 4.4.2 Vertical Profile Structure of the Hydrometeors 4.4.3 Scan Header 4.4.4 Pixel Data 4.4.5 Orbit Header Variable Description 4.4.6 Vertical Profile Variable Description 4.4.7 Scan Variable Description 4.4.8 Pixel Data Variable Description -
Small Body Technology Roadmap
DRAFT Small Body Technology Roadmap Executive Summary: The planetary science of small bodies includes ground observations and missions to fly-by, rendezvous, and return samples from a diverse set of targets. Small bodies include asteroids, comets, small satellites, dwarf planets, centaurs, trans-Neptunian objects, and interplanetary dust. These targets offer great diversity over a wide range of heliocentric locations, however; many have similar characteristics that allow for a practical assessment of near-term technology needs. The highest priority needs include a variable focus imager, a high resolution topography instrument, affordable electric propulsion, and a large number of sample return supporting technologies. An initial roadmap of development for small body missions in provided below. I. Introduction his document is to serve as the initial start of an evolving technology development roadmap for small body T mission instruments and systems to allow maximum science return. The missions of interest are for observations, fly-by, rendezvous, landing, and sample return from asteroids, comets, small satellites, dwarf planets, centaurs, and trans-Neptunian objects. Small body missions are diverse both in the type and class of viable missions, but also in the broad range of celestial location. Though the diversity is great, most small body mission instruments and system requirements are broadly applicable over the range of missions without overly cumbersome unique instrument requirements one would expect trying to encompass in-situ environments and science priorities at the larger bodies of planets and moons. The original approach for developing this technology roadmap for small body missions was to develop an all inclusive science traceability matrix for all classes of small body missions, specify the instrument/systems requirements to enable the science return, identify state-of-the-art (SOA) capabilities, and advocate technology development to fill the requirements gap.