E PO Contact List August2013f.Pdf

Total Page:16

File Type:pdf, Size:1020Kb

E PO Contact List August2013f.Pdf Earth Science Mission Description Website E/PO Lead First Name E/PO Lead Last Name Organization Email The ACRIMSAT mission is measuring Total Solar Irradiance (TSI). The ACRIMSAT spacecraft carries the Active Cavity ACRIMSAT http://acrim.jpl.nasa.gov Karen Yuen JPL [email protected] Radiometer Irradiance Monitor (ACRIM) III instrument, the third in a series of long-term solar monitoring tools. The Airborne Science Program within the Earth Science Airborne Science Program Division is responsible for providing aircraft systems that http://airbornescience.nasa.gov Cheryl Yuhas NASA HQ [email protected] further science and advance the use of satellite data. To improve our understanding of the role of North American ecosystems in the global carbon cycle, the Airborne Microwave Observatory of Subcanopy and Subsurface is AirMOSS http://airmoss.jpl.nasa.gov Annie Richardson JPL [email protected] providing new continental-scale estimates of periodic changes in the amount of carbon dioxide exchanged between these ecosystems and the atmosphere. Aqua is obtaining a set of precise atmosphere and ocean measurements to understand their role in Earth's climate and its variations. Aqua carries six state-of-the-art instruments to observe Earth's ocean, atmosphere, land, ice and snow covers, and vegetation, providing high measurement accuracy, spatial detail, and temporal frequencey. It is gathering data on Earth's water cycle, in particular Aqua http://aqua.nasa.gov Steve Graham GSFC [email protected] information on water vapor and clouds, precipitation from the atmosphere, soil wetness on land, ice on both land and sea, and snow cover. It also provides information on vegetation cover, temperatures of the air, land and water, and radiation from both the sun and the Earth. Aqua is a joint project of the United States, Japan and Brazil. The Atmospheric Infrared Sounder (AIRS) is one of six instruments aboard the Aqua satellite. Together with the Advanced Microwave Sounding Unit (AMSU-A), these instruments observe the global water and energy cycles, climate variation and trends, and the response of the climate Aqua / AIRS http://airs.jpl.nasa.gov Sharon Ray JPL [email protected] system to increased greenhouse gases. AIRS creates 3-D maps of air and surface water temperature, water vapor and cloud properties. AIRS can also measure trace greenhouse gases such as ozone, carbon monoxide, carbon dioxide, and methane. NASA Earth Science Missions E/PO Contact List 1 Updated August 2013 Earth Science Mission Description Website E/PO Lead First Name E/PO Lead Last Name Organization Email Aquarius measures the salinity, or saltiness, of the ocean surface. Throughout the history of Earth, the weathering of rocks has delivered mineral salts into the ocean. Over decades, the amount of salt in ocean basins has been relatively stable. The water cycle operates on much faster time scales, however, causing changes in salinity patterns. Aquarius Freshwater input from rivers, melting ice, rain and snow http://aquarius.nasa.gov Annette deCharon University of Maine [email protected] makes the ocean less salty. Processes that cause freshwater to exit the ocean—such as evaporation and formation of sea ice—make the ocean saltier. Differences in salinity can play a major role in moving seawater—and the heat it carries— around the globe. Thus salinity is crucial to keeping Earth’s climate in balance. Recent studies suggest that even small changes in stratospheric humidity may have significant climate impacts. The Airborne Tropical TRopopause EXperiment uses the long- ATTREX http://espo.nasa.gov/missions/attrex/ Jhony Zavaleta ARC [email protected] range NASA Global Hawk uninhabited aircraft systems to understand changes in stratospheric humidity and ozone concentrations to support climate studies. The Aura mission studies Earth's ozone, air quality and climate. It is designed exclusively to conduct research on the composition, chemistry and dynamics of Earth's atmosphere. Aura's objective is to study the chemistry and dynamics of Sigma Space Aura Earth's atmosphere with emphasis on the upper troposphere http://aura.gsfc.nasa.gov Ginger Butcher [email protected] Corp/GSFC and lower stratosphere by employing multiple instruments on a single satellite. The satellite's measurements enable scientists to investigate questions about ozone trends, air quality changes, and their linkage to climate change. The Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observation (CALIPSO) satellite is providing new insight into the role that clouds and atmospheric aerosols (airborne particles) play in regulating Earth's weather, climate, and air CALIPSO quality. CALIPSO and CloudSat are highly complementary and http://www-calipso.larc.nasa.gov/outreach/ Jessica Taylor LaRC [email protected] together provide 3-D perspectives of how clouds and aerosols form, evolve, and affect weather and climate. CALIPSO is a joint preject between NASA and Centre National d'Etudes Spatiales (CNES) of France. The Carbon in Arctic Reservoirs Vulnerability Experiment aircraft mission will collect detailed measurements of CARVE important greenhouse gases on local to regional scale in the http://science.jpl.nasa.gov/projects/CARVE/ Karen Yuen JPL [email protected] Alaskan Arctic and demonstrate new capabilities to quantify Arctic carbon changes and carbon cycle-climate processes. CloudSat is among the first satellites to study clouds on a global basis. Its key observations are the vertical profiles of Todd Ellis SUNY-Oneonta [email protected] cloud liquid water and ice water contents, and related cloud physical and radiative properties. CloudSat flies in a tight Colorado State CloudSat formation with the CALIPSO satellite, and both follow behind http://cloudsat.atmos.colostate.edu Deanna TeBockhorst [email protected] University the Aqua satellite in a looser formation. The combination of these satellites provide a rich source of information that can be used to assess the role of clouds in Peter Falcon JPL [email protected] both weather and climate. NASA Earth Science Missions E/PO Contact List 2 Updated August 2013 Earth Science Mission Description Website E/PO Lead First Name E/PO Lead Last Name Organization Email To understand how to better diagnose air pollution, NASA scientists have planned a series of airborne field campaigns—called DISCOVER-AQ—that fly over selected U.S. cities taking air quality measurements. Scientists are coordinating these measurements with satellite- and ground- based measurements to see where the differences are. One http://www.nasa.gov/mission_pages/discover- DISCOVER-AQ Lin Chambers LaRC [email protected] airplane carries remote sensing instruments to make aq/ measurements looking down from about 26,000 feet, simulating what a satellite would see, while a second plane flies beneath the first, spiraling up and down at selected points to measure pollution in the different layers of the atmosphere. The Global Precipitation Measurement Mission is an international satellite mission to provide next-generation observations of rain and snow worldwide every three hours. NASA and the Japan Aerospace Exploration Agency (JAXA) will launch a “Core” satellite carrying advanced instruments that will set a new standard for precipitation measurements from GPM space. The data they provide will be used to unify http://www.nasa.gov/gpm Dalia Kirschbaum GSFC [email protected] precipitation measurements made by an international network of partner satellites to quantify when, where, and how much it rains or snows around the world. This will help advance our understanding of Earth’s water and energy cycles, improve weather forecasting, and deliver other societal benefits. The Earth System Science Pathfinder (ESSP) Program is a science-driven Program designed to provide an innovative Earth System Science http://science.nasa.gov/about-us/smd- approach to Earth science research by providing periodic, Kimberly Land LaRC [email protected] Pathfinder Program programs/earth-system-science-pathfinder/ competitively selected opportunities to accommodate new and emergent scientific priorities. The New Millennium Program Earth Observing-1 (EO-1) program completed its baseline mission requirements successfully after one year of operations on Nov. 20, 2001. In Dec. 2001, NASA HQ approved a plan to permit the EO-1 EO-1 Program to embark on an Extended Mission operations phase. http://eo1.gsfc.nasa.gov Nancy Leon JPL [email protected] The objectives of the Extended Mission are to maximize the infusion of EO-1 technology by simultaneously increasing utilization of the on-orbit resource and to reduce the cost of operations through a Continuous Improvement Program. The primary goal of the Gravity Recovery and Climate Experiment (GRACE) mission is to accurately map variations in Earth's gravity field. Another goal of the mission is to create a http://www.nasa.gov/mission_pages/Grace/ind University of Texas - GRACE better profile of the Earth's atmosphere. The results are Margaret Baguio [email protected] ex.html Austin contributing to global climate change studies. GRACE is a joint project between NASA and Deutsche Forschungsanstalt fur Luft und Raumfahrt (DLR) in Germany. NASA Earth Science Missions E/PO Contact List 3 Updated August 2013 Earth Science Mission Description Website E/PO Lead First Name E/PO Lead Last Name Organization Email GRACE Follow-on The GRACE Follow-on mission is scheduled for launch in 2017. http://grace.jpl.nasa.gov Tom Nolan JPL [email protected] Since 2012, the Hurricane and Severe Storm Sentinel mission has been using two NASA Global Hawk aircraft to help http://www.nasa.gov/mission_pages/hurricane HS3 Bernadette Luna ARC [email protected] understand and better predict hurricane intensity in the s/missions/hs3/index.html Atlantic Ocean basin. The Ice, Cloud, and land Elevation Satellite studied the ice sheets and sea ice that blanket the North and South Pole regions, as well as global measurements of aerosol, cloud, and vegetation height.
Recommended publications
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • SMD Technology Program – Community Update
    SMD Technology Program – Community Update Presentation to the 2010 Annual LEAG Meeting Gordon Johnston, NASA HQ/SMD/PSD September 14, 2010 1 09/10/2010 1 Outline • SMD Technology – Investment Areas and OCT Coordination • Planetary Science Technology Review (PSTR) Panel – Purpose – Team – PSTR Activities and Planned Products – Current Status – Major Observations – Near Term Plans Planetary Science Technology Review--Purpose, Status, and Plans 09/10/2010 2 SMD Technology Investments • NASA Science Mission Directorate invests over $500M in technology development. • Technology investments are made via four major avenues: – Mission-specific technology developments with flight projects – Individual PI-led research investigations – Suborbital research programs – Earth science technology program • SMD is mission focused – Technology investments through the SMD Science Divisions • SMD covers all TRL levels – Low to mid (R+A, instrument incubators, EST) – Mid to late (suborbital, EST, mission focused tech) • SMD is coordinating with and supporting the OCT effort to improve the overall Agency capabilities in Science and Technology development. – Dr. Michael Moore is the SMD point of contact. 09/10/2010 3 SMD Integration with OCT Direct Communications Chief Technologist (CT) AA Science Deputy CT Mission Directorate Partnerships, Innovation & Technology Financial Management Commercial Space Coordinator Communications Strategic Integration Astrophysics and PhysicsHeliophysics Division Early‐Stage Game Changing Crosscutting Capability Innovation Technology
    [Show full text]
  • Deep Space One Telecommunication Development M.I
    • • SSC98-IV-l • Deep Space One Telecommunication Development M.I. Herman, S. Valas, W. Hatch, C.C. Chen, S. H. Zingales, R. P. Scaramastra, L.R. Amaro, • and M. D. Rayman Jet Propulsion Laboratory • California Institute of Technology 4800 Oak Grove Drive • Pasadena, CA 91109 m1s 161-213 818-354-8541 • [email protected] • Abstract. Deep Space One (DS1) is the first of the New Millennium Program deep space technology validation missions, to be launched October 1998. This paper focuses on the • Telecommunication Subsystem architecture, technology developments, as well as the test results. Technical factors that influenced the subsystem architecture were the ability to command the • spacecraft and downlink telemetry data in cruise and emergency situations, and the need to provide radiometric data. Additional challenges included the requirement to demonstrate new • telecommunication technology, enable the validation of other system technologies (for example solar electric propulsion, autonomous navigation, and beacon monitor operation), and at the same time utilize a single string system design. From a programmatic perspective we had to accomplish • these goals within a budget and workforce load that was at least a factor 2 less than the Mars • Pathfinder Project. The Small Deep Space Transponder (SDST), a new technology developed by Motorola, is the • heart of the Telecommunication Subsystem and is a result of a JPL multimission sponsored competitive award. The SDST provides the functionality normally associated with 4-5 individual • subassemblies at less than half the mass (2.95 kg). Another new technology to be validated on DS1 is a 2.5W Ka-band solid state amplifier developed by Lockheed Martin (under their own funding).
    [Show full text]
  • 2006-449: Industrial Engineering Application in Space Mission
    2006-449: INDUSTRIAL ENGINEERING APPLICATION IN SPACE MISSION Douglas McLennan, Goddard Space Flight Center Dr. Douglas McLennan is the Project Manager of the Space Technology - 5 (ST-5) at the Goddard Space flight Center (GSFC) in Greenbelt, Maryland. Dr. McLennan received his B.Sc. in Physics in 1978 from Carleton University, Ottawa, Ontario Canada. He received his M.S. in 1980 and Ph.D. in 1983 from Georgetown University, Washington D.C. Guangming Chen, Morgan State University Dr. Guangming Chen is an Associate Professor in Industrial Engineering at Morgan State University. He joined Morgan State faculty in 1990 as an Assistant Professor. Since September 2002, he has worked with ST-5 project at Goddard Space Flight Center, under the NASA Administrator?s Fellowship Program and his NASA Faculty Award for Research (FAR) grant. He also worked at NASA Goddard Space Flight Center under NASA/ASEE Summer Faculty Fellowship in 1999 and 2000. He also worked as Guest Scientist at Brookhaven National Lab, Long Island, NY in 1994 Summer and he was a Reliability Engineer at A-Line Plastics, Inc., Plymouth, Michigan before he came to Morgan. He received his Ph.D. from Wayne State University, Detroit, Michigan in 1990 and a B.S. in 1982 and a M.S. in 1984 from Shanghai Jiao Tong University. Ricky Whittington, Morgan State University Mr. Whittington is a graduate student in Industrial Engineering at Morgan State University and a research assistant in the NASA project. He received a B.S. in Industrial Engineering from Morgan State University in May 2005. Page 11.752.1 Page © American Society for Engineering Education, 2006 INDUSTRIAL ENGINEERING COLLABORATION WITH NASA ST-5 PROJECT Ricky Whittington*, Guangming Chen** Morgan State University School of Engineering Department of Industrial, Manufacturing and Information Engineering Baltimore, Maryland 21251 (*Graduate Student; **NAFP Fellow and Contact Person) And Douglas D.
    [Show full text]
  • Mission Operations of Earth Observing-1 with Onboard Autonomy
    Mission Operations of Earth Observing-1 with Onboard Autonomy Gregg Rabideau, Daniel Tran, Steve Chien, Benjamin Cichy, Rob Sherwood Jet Propulsion Laboratory, California Institute of Technology Dan Mandl, Stuart Frye1, Seth Shulman2, Joseph Szwaczkowski2 Goddard Space Flight Center Darrell Boyer, Jim Van Gaasbeck Interface & Control Systems future spacecraft activities that is consistent with the Abstract extensive list of spacecraft and mission constraints. Space mission operations are extremely labor and Finally, when an activity is imminent, CASPER submits a knowledge-intensive and are driven by the ground and request for execution by the onboard executive, SCL. flight systems. Inclusion of an autonomy capability can SCL initiates a set of scripts that perform the complete have dramatic effects on mission operations. We describe sequence of commands for the spacecraft and its the prior, labor and knowledge intensive mission payloads. Prior to executing each command, constraints operations flow for the Earth Observing-1 (EO-1) spacecraft as well as the new autonomous operations as are checked again to confirm the validity of the command part of the Autonomous Sciencecraft Experiment (ASE). as well as to ensure the safety of the spacecraft. After the command is sent, the executive checks for a successful initiation and completion of the command. W hen a full 1. Introduction sequence for a data collection is complete, one or more of the science processing algorithms are triggered and the EO-1 is the first satellite of the Earth observing series of entire process repeats. NASA‘s New Millennium Program (NMP). Since its launch on November 21, 2000, under management of the The ASE software provides many benefits to the science Goddard Space Flight Center (GSFC), EO-1 has and engineering teams involved in operations.
    [Show full text]
  • Preparations for the Geostationary Imaging Fourier Transform
    PREPARATIONS FOR THE GEOSYNCHRONOUS IMAGING FOURIER TRANSFORM SPECTROMETER J.F. Le Marshall1, W.L. Smith2, R.G. Seecamp1, A. Rea1, L.M. Leslie3, M. Dunn4 and B. Choi5 1 Bureau of Meteorology, Melbourne, Australia, 2 NASA Langley Research Center, Hampton, VA, 23681, USA, 3 University of Oklahoma, Norman, Oklahoma, USA, 4 Latrobe University, Melbourne, Australia, 5 Latrobe University, Bendigo, Australia INTRODUCTION The Geosynchronous Imaging Fourier Transform Spectrometer (GIFTS) will be completed in late 2005, to support a 2006 or later launch. The GIFTS will be orbited as part of NASA’s New Millennium Program Earth Observing-3 (EO-3) Mission and will serve as a prototype of sounding systems to fly on future operational geostationary satellites. The first year of operation of GIFTS will support the infusion of new technologies and data processing techniques into future geostationary operational satellite systems and ensure their timely exploitation in numerical weather prediction (NWP). The mission will validate the GIFTS measurement concept for altitude-resolved (water vapour observation based) winds. The GIFTS will result in high temporal and spatial resolution soundings of the atmosphere for temperature and absorbing species such as water vapour and ozone, and demonstrate new technologies for future research and operational systems. We note some of the development activity in support the application of GIFTS data over continental USA and also note preparation for the collection and utilisation of this data when the GIFTS is stationed over its permanent position which is dependent upon the satellite mission of which GIFTS is part. The development activity includes preparation for providing; radiance products for NWP, altitude resolved, error characterised winds, temperature and moisture profiles, product imagery (stability fields, water vapour fields, etc.), sea and land surface temperatures with attendant emissivities, ozone and CO amounts and cloud properties.
    [Show full text]
  • NASA's Earth Science National Aeronautics and Space
    DOCUMENT RESUME ED 432 453 SE 062 500 TITLE Understanding Our Changing Planet: NASA's Earth Science Enterprise. 1998 Fact Book. INSTITUTION National Aeronautics and Space Administration, Greenbelt, MD. Goddard Space Flight Center. REPORT NO NP-1998(02)-009-GSFC PUB DATE 1998-00-00 NOTE 25p. PUB TYPE Guides Classroom - Teacher (052) EDRS PRICE MF01/PC01 Plus Postage. DESCRIPTORS Climate Change; *Earth Science; *Ecology; Elementary Secondary Education; Energy Conservation; Natural Sciences; *Science Education; *Scientific Concepts; *Space Sciences; Water IDENTIFIERS National Aeronautics and Space Administration ABSTRACT This document describes NASA's Earth Science Enterprise, a comprehensive program to study the earth as an environmental system. The Earth Science Enterprise has three main components:(1) a series of earth-observing satellites;(2) an advanced data system; and (3) teams of scientists who will study the data. Contents include:(1) "The Earth Science Enterprise," an overview of the program; (2) "Questions and Answers," key questions about how NASA studies the earth; (3) "NASA Facts," information on related science issues; (4) "Earth Science Enterprise Accomplishments," accomplishments from the past to the future; (5) "Earth Science Enterprise Researchers," information about the people who are part of the program; (6) "Earth Science Enterprise Facts," specific information about missions and recent changes; and (7)"Where Do I Get More Information?" a listing of Earth Science Enterprise education contacts. (CCM) ******************************************************************************** Reproductions supplied by EDRS are the best that can be made from the original document. ******************************************************************************** UN 2TANDIING `NG:ING 1=1 4-1 NASA'S EARTH SCIENCE ENTERPRISE U.S. DEPARTMENT OF EDUCATION Office of Educational Research and Improvement EDUCATIONAL RESOURCES INFORMATION CENTER (ERIC) y...T.trt"s document has been reproduced as received from the person or organization originating it.
    [Show full text]
  • NASA Advisory Council Science Committee, April 20-21, 2010
    NASA Advisory Council Science Committee, April 20‐21, 2010 Table of Contents Welcome and Introduction 3 Goddard Space Flight Center (GSFC) Welcome 3 NASA SMD Science Plan 6 Lunch talk 7 PSS Update 8 PSD Science Highlights 8 Status of Pu‐238 9 ESS Update 9 ESD Update 9 Operating missions 10 NASA Technology Initiative 10 Q&A with SMD AA 11 APD/APS Update 12 APD Science Highlights 12 Kepler Data Release Policy 13 HPS Update 13 HPD Status 14 NMP Lessons Learned 14 ISS Utilization 15 Discussion 16 Public Comments 17 Findings and Recommendations 17 Appendix A‐ Attendees Appendix B‐ Membership roster Appendix C‐ Presentations Appendix D‐ Agenda Prepared by Joan M. Zimmermann Harris Corp. 2 NASA Advisory Council Science Committee, April 20‐21, 2010 Welcome and Introduction Dr. Wesley T. Huntress, Chair of the NASA Advisory Council (NAC) Science Committee, opened the proceedings, thanking the director of the Goddard Space Flight Center (GSFC) for hosting the meeting. T. Jens Feeley, Executive Secretary made some brief logistical announcements. Dr. Huntress alluded to President Obama’s April 15, 2010, visit to the Kennedy Center, welcomed the new NASA funding contained in the FY11 budget request, as well as a clear plan with timeframes for destinations. He briefly reviewed three recommendations that had been transmitted to NASA Administrator Charles Bolden, namely strong NAC Science Committee support for the development of a new technology program, a proposed re-initiation of Pu-238 production in the U.S., and the establishment of various new NAC Science Subcommittee analysis groups. Goddard Space Flight Center (GSFC) Welcome Dr.
    [Show full text]