NASA's Earth Science Data Systems Program
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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. -
Funding and Strategic Alignment Guidance for Infusing Small
https://ntrs.nasa.gov/search.jsp?R=20160013708 2019-08-29T17:18:43+00:00Z NASA/TM—2016-219161 Funding and Strategic Alignment Guidance for Infusing Small Business Innovation Research Technology Into Science Mission Directorate Projects at Glenn Research Center for 2015 Hung D. Nguyen and Gynelle C. Steele Glenn Research Center, Cleveland, Ohio November 2016 NASA STI Program . in Profile Since its founding, NASA has been dedicated • CONTRACTOR REPORT. Scientific and to the advancement of aeronautics and space science. technical findings by NASA-sponsored The NASA Scientific and Technical Information (STI) contractors and grantees. Program plays a key part in helping NASA maintain this important role. • CONFERENCE PUBLICATION. Collected papers from scientific and technical conferences, symposia, seminars, or other The NASA STI Program operates under the auspices meetings sponsored or co-sponsored by NASA. of the Agency Chief Information Officer. It collects, organizes, provides for archiving, and disseminates • SPECIAL PUBLICATION. Scientific, NASA’s STI. The NASA STI Program provides access technical, or historical information from to the NASA Technical Report Server—Registered NASA programs, projects, and missions, often (NTRS Reg) and NASA Technical Report Server— concerned with subjects having substantial Public (NTRS) thus providing one of the largest public interest. collections of aeronautical and space science STI in the world. Results are published in both non-NASA • TECHNICAL TRANSLATION. English- channels and by NASA in the NASA STI Report language translations of foreign scientific and Series, which includes the following report types: technical material pertinent to NASA’s mission. • TECHNICAL PUBLICATION. Reports of For more information about the NASA STI completed research or a major significant phase program, see the following: of research that present the results of NASA programs and include extensive data or theoretical • Access the NASA STI program home page at analysis. -
Airborne Science Program 2014 ANNUAL REPORT (Front Cover: View from C-130 During ARISE) NASA Airborne Science Program 2014 ANNUAL REPORT
NASA Airborne Science Program 2014 ANNUAL REPORT (Front Cover: View from C-130 during ARISE) NASA Airborne Science Program 2014 ANNUAL REPORT National Aeronautics and Space Administration Table of Contents Leadership Comments 1 Program Overview 3 Structure of the Program 3 New Program Capabilities 4 Flight Request System 5 Fiscal Year 2014 Flight Requests 5 Funded Flight Hours (Flown) 7 Science 9 Major Mission highlights 10 Operation Ice Bridge 10 ARISE 13 Earth Venture Suborbital - 1 15 SABOR 22 UAVSAR 24 Support to ESD Satellite Missions, including Decadal Survey Missions 25 Integrated Precipitation and Hydrology Experiment (IPHEX) 26 HyspIRI Preparatory Airborne Studies 27 MABEL Alaska 2014 Campaign 28 Support to Instrument Development 29 ASCENDS 30 Geostationary Trace gas and Aerosol Sensor Optimiztion (GEO-TASO) instrument 30 CarbonHawk 31 Upcoming Activities 32 Aircraft 33 ASP-Supported Aircraft 34 Other NASA Earth Science Aircraft 41 The NASA ASP Small Unmanned Systems Projects 47 SIERRA UAS 47 DragonEye UAS 48 Viking-400 49 Aircraft Cross-Cutting Support and IT Infrastructure 50 ASP Facility Science Infrastructure 50 Facility Instrumentation 50 Sensor Network IT Infrastructure 50 NASA Airborne science Data and Telemetry (NASDAT) System 52 Satellite Communications Systems 50 Payload Management 52 Mission Tool Suite 53 Advanced Planning 56 Requirements update 56 5-yr plan 57 Education, Training, Outreach and Partnerships 58 Student Airborne Research Program 2014 58 Mission Tools Suite for Education (MTSE) 60 Partnerships 62 Appendices 63 Appendix A: Historical Perspective, Jeffrey Myers 63 Appendix B: Five-Year Plan 68 Appendix C: Acronyms 72 LEADERSHIP COMMENTS Bruce Tagg Program Manager, Airborne Science Program Welcome to the 2014 edition of the The program’s Mission Tool Suite for Education Airborne Science Program (ASP) (MTSE) had another very busy year as well. -
The Space-Based Global Observing System in 2010 (GOS-2010)
WMO Space Programme SP-7 The Space-based Global Observing For more information, please contact: System in 2010 (GOS-2010) World Meteorological Organization 7 bis, avenue de la Paix – P.O. Box 2300 – CH 1211 Geneva 2 – Switzerland www.wmo.int WMO Space Programme Office Tel.: +41 (0) 22 730 85 19 – Fax: +41 (0) 22 730 84 74 E-mail: [email protected] Website: www.wmo.int/pages/prog/sat/ WMO-TD No. 1513 WMO Space Programme SP-7 The Space-based Global Observing System in 2010 (GOS-2010) WMO/TD-No. 1513 2010 © World Meteorological Organization, 2010 The right of publication in print, electronic and any other form and in any language is reserved by WMO. Short extracts from WMO publications may be reproduced without authorization, provided that the complete source is clearly indicated. Editorial correspondence and requests to publish, reproduce or translate these publication in part or in whole should be addressed to: Chairperson, Publications Board World Meteorological Organization (WMO) 7 bis, avenue de la Paix Tel.: +41 (0)22 730 84 03 P.O. Box No. 2300 Fax: +41 (0)22 730 80 40 CH-1211 Geneva 2, Switzerland E-mail: [email protected] FOREWORD The launching of the world's first artificial satellite on 4 October 1957 ushered a new era of unprecedented scientific and technological achievements. And it was indeed a fortunate coincidence that the ninth session of the WMO Executive Committee – known today as the WMO Executive Council (EC) – was in progress precisely at this moment, for the EC members were very quick to realize that satellite technology held the promise to expand the volume of meteorological data and to fill the notable gaps where land-based observations were not readily available. -
Improved Quality Control for Quikscat Near Real-Time Data
JP4.6 Improved Quality Control for QuikSCAT Near Real-time Data S. Mark Leidner, Ross N. Hoffman, and Mark C. Cerniglia Atmospheric and Environmental Research Inc., Lexington, Massachusetts Abstract errors. We will illustrate the types of errors that occur due to rain contamination and ambiguity removal. SeaWinds on QuikSCAT, launched in June 1999, We will also give examples of how the quality of the provides a new source of surface wind information retrieved winds varies across the satellite track, and over the world’s oceans. This new window on global varies with wind speed. surface vector winds has been a great aid to real- SeaWinds is an active, Ku-band microwave radar time operational users, especially in remote areas operating near ¢¤£¦¥¨§ © and is sensitive to centimeter- of the world. As with in situ observations, the qual- scale or capillary waves on the ocean surface. ity of remotely-sensed geophysical data is closely These waves are usually in equilibrium with the wind. tied to the characteristics of the instrument. But Each radar backscatter observation samples a patch remotely-sensed scatterometer winds also have a of ocean about . The vector wind is re- whole range of additional quality control concerns trieved by combining several backscatter observa- different from those of in situ observation systems. tions made from multiple viewing geometries as the The retrieval of geophysical information from the raw scatterometer passes overhead. The resolution of satellite measurements introduces uncertainties but the retrieved winds is . also produces diagnostics about the reliability of the Backscatter from capillary waves on the ocean retrieved quantities. -
Watching the Winds Where Sea Meets Sky 14 August 2014, by Rosalie Murphy
Watching the winds where sea meets sky 14 August 2014, by Rosalie Murphy the speed and direction of wind at the ocean's surface. "Before scatterometers, we could only measure ocean winds on ships, and sampling from ships is very limited," said Timothy Liu of NASA's Jet Propulsion Laboratory in Pasadena, California, who led the science team for NASA's QuikScat mission. Scatterometry began to emerge during World War II, when scientists realized wind disturbing the ocean's surface caused noise in their radar signals. NASA included an experimental scatterometer in its The SeaWinds scatterometer on NASA's QuikScat first space station in 1973 and again when it satellite stares into the eye of 1999's Hurricane Floyd as launched its SeaSat satellite in 1978. During its it hits the U.S. coast. The arrows indicate wind direction, three-month life, SeaSat's scatterometer provided while the colors represent wind speed, with orange and scientists with more individual wind observations yellow being the fastest. Credit: NASA/JPL-Caltech than ships had collected in the previous century. The ocean covers 71 percent of Earth's surface and affects weather over the entire globe. Hurricanes and storms that begin far out over the ocean affect people on land and interfere with shipping at sea. And the ocean stores carbon and heat, which are transported from the ocean to the air and back, allowing for photosynthesis and affecting Earth's climate. To understand all these processes, scientists need information about winds A JPL team then designed a mission called near the ocean's surface. -
Seasat—A 25-Year Legacy of Success
Remote Sensing of Environment 94 (2005) 384–404 www.elsevier.com/locate/rse Seasat—A 25-year legacy of success Diane L. Evansa,*, Werner Alpersb, Anny Cazenavec, Charles Elachia, Tom Farra, David Glackind, Benjamin Holta, Linwood Jonese, W. Timothy Liua, Walt McCandlessf, Yves Menardg, Richard Mooreh, Eni Njokua aJet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, United States bUniversitaet Hamburg, Institut fuer Meereskunde, D-22529 Hamburg, Germany cLaboratoire d´Etudes en Geophysique et Oceanographie Spatiales, Centre National d´Etudes Spatiales, Toulouse 31401, France dThe Aerospace Corporation, Los Angeles, CA 90009, United States eCentral Florida Remote Sensing Laboratory, University of Central Florida, Orlando, FL 32816, United States fUser Systems Enterprises, Denver, CO 80220, United States gCentre National d´Etudes Spatiales, Toulouse 31401, France hThe University of Kansas, Lawrence, KS 66047-1840, United States Received 10 June 2004; received in revised form 13 September 2004; accepted 16 September 2004 Abstract Thousands of scientific publications and dozens of textbooks include data from instruments derived from NASA’s Seasat. The Seasat mission was launched on June 26, 1978, on an Atlas-Agena rocket from Vandenberg Air Force Base. It was the first Earth-orbiting satellite to carry four complementary microwave experiments—the Radar Altimeter (ALT) to measure ocean surface topography by measuring spacecraft altitude above the ocean surface; the Seasat-A Satellite Scatterometer (SASS), to measure wind speed and direction over the ocean; the Scanning Multichannel Microwave Radiometer (SMMR) to measure surface wind speed, ocean surface temperature, atmospheric water vapor content, rain rate, and ice coverage; and the Synthetic Aperture Radar (SAR), to image the ocean surface, polar ice caps, and coastal regions. -
Aqua Summary (As of May 31, 2019) • Spacecraft Bus – Nominal Operations (Excellent Health) ‒ All Components Remain on Primary Hardware
Aqua Summary (as of May 31, 2019) • Spacecraft Bus – Nominal Operations (Excellent Health) ‒ All components remain on primary hardware. ‒ 18 of 132 Solar Array Strings appear to have failed. See slide 2. Similar failures have occurred on Aura. ‒ Significant power generation margin remains. • MODIS – Nominal Operations (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ All components remain on primary hardware except 10W Lamps used for calibration. • AIRS – Nominal Operations (<10% of Channels degraded) – (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ ~200 of 2378 channels are degraded due to radiation, however they are still useful. ‒ Cooler-A Telemetry, frozen since a 3/28/2014 Anomaly, was restored during recovery activities performed on 9/27/2016. • AMSU-A – Nominal Operations for 9 of 15 Channels (Fair Health) ‒ All voltages, currents, and temperatures are as expected. ‒ 3 of 15 channels have been removed from Level 2 processing. 2 channels (#1 & #2) are unavailable. ‒ AMSU-A2 Anomaly on 9/24/2016 caused loss of Channels 1 and 2. The initial recovery attempts were unsuccessful. The instrument manufacturer recommends not switching to the A-side to attempt to recover AMSU-A2. ‒ AMSU-A1 Anomaly on 6/21/2018 caused unexplained shift in Channel 14. Channel 14 data have now been removed from processing, and the anomaly is considered closed. • CERES-AFT (FM-3) – Nominal Operations (Excellent Health) ‒ All voltages, currents, and temperatures are as expected. ‒ Cross-Track and Biaxial Modes are fully functioning. ‒ All channels remain operational. • CERES-FORE (FM-4) – Nominal Operations (Good Health) ‒ All voltages, currents, and temperatures are as expected. -
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. -
SMEX05 Quikscat/Seawinds Backscatter Data: Iowa
Notice to Data Users: The documentation for this data set was provided solely by the Principal Investigator(s) and was not further developed, thoroughly reviewed, or edited by NSIDC. Thus, support for this data set may be limited. SMEX05 QuikSCAT/SeaWinds Backscatter Data: Iowa Summary This data set includes radar backscatter data collected over the Soil Moisture Experiment 2005 (SMEX05) area of Iowa, USA from 01 May 2005 through 31 July 2005. The SeaWinds scatterometer on the NASA Quick Scatterometer (QuikSCAT) satellite collected backscatter data. The total volume of this data set is approximately 18 megabytes. Data are provided in gzip compressed Brigham Young University - Microwave Earth Remote Sensing (BYU-MERS) Scatterometer Image Reconstruction (SIR) images and Graphics Interchange Format (GIF) images, and are available via FTP. The Advanced Microwave Scanning Radiometer - Earth Observing System (AMSR-E) is a mission instrument launched aboard NASA's Aqua satellite on 04 May 2002. AMSR-E validation studies linked to SMEX are designed to evaluate the accuracy of AMSR-E soil moisture data. Specific validation objectives include: assessing and refining soil moisture algorithm performance; verifying soil moisture estimation accuracy; investigating the effects of vegetation, surface temperature, topography, and soil texture on soil moisture accuracy; and determining the regions that are useful for AMSR-E soil moisture measurements. Citing These Data: Long, David G. 2010. SMEX05 QuikSCAT/SeaWinds Backscatter Data: Iowa. Boulder, Colorado USA: NASA DAAC at the National Snow and Ice Data Center. Overview Table Category Description gzip compressed SIR Data format GIF Spatial coverage 41.5º to 42.5º N, 93º to 95º W Temporal coverage 01 May 2005 to 31 July 2005 queh-a-NAm05-121-124.sir.SME.gz File naming convention queh-a-NAm05-121-124.sir.SM.gif .gz files range in size from 7 to 32 KB File size .gif files range in size from 3 KB to 14 KB Procedures for obtaining data Data are available via FTP. -
Synthetic Aperture Radar in Europe: ERS, Envisat, and Beyond
SYNTHETIC APERTURE RADAR IN EUROPE Synthetic Aperture Radar in Europe: ERS, Envisat, and Beyond Evert Attema, Yves-Louis Desnos, and Guy Duchossois Following the successful Seasat project in 1978, the European Space Agency used advanced microwave radar techniques on the European Remote Sensing satellites ERS-1 (1991) and ERS-2 (1995) to provide global and repetitive observations, irrespective of cloud or sunlight conditions, for the scientific study of the Earth’s environment. The ERS synthetic aperture radars (SARs) demonstrated for the first time the feasibility of a highly stable SAR instrument in orbit and the significance of a long-term, reliable mission. The ERS program has created opportunities for scientific discovery, has revolutionized many Earth science disciplines, and has initiated commercial applica- tions. Another European SAR, the Advanced SAR (ASAR), is expected to be launched on Envisat in late 2000, thus ensuring the continuation of SAR data provision in C band but with important new capabilities. To maximize the use of the data, a new data policy for ERS and Envisat has been adopted. In addition, a new Earth observation program, The Living Planet, will follow Envisat, offering opportunities for SAR science and applications well into the future. (Keywords: European Remote Sensing satellite, Living Planet, Synthetic aperture radar.) INTRODUCTION In Europe, synthetic aperture radar (SAR) technol- Earth Watch component of the new Earth observation ogy for polar-orbiting satellites has been developed in program, The Living Planet, and possibly the scientific the framework of the Earth observation programs of Earth Explorer component will include future SAR the European Space Agency (ESA). -
US FGGE Project Office NOAA 6010 Executive Blvd
U.S. FGGE Project Office NOAA 6010 Executive Blvd. Rockville, Maryland 20852 Phone: 301-443-8861 THE GLOBAL WEATHER EXPERIMENT N o . 12____________________________________________________________________ December 1978 D-DAY "In The Beginning," there was nothing but planning, much discussing, and more pondering over something called FGGE. Now, we are off and running I The FGGE Operational Year commences December 1 and January 5 opens the First Special Observing Period. As the Holiday Season approaches, the FGGE Project Office would like to thank all those who have already contributed to the Experiment and express best wishes to all for the New Year. SATELLITE UPDATE TIROS-N Introduction: The first TIROS-N advanced weather satellite was launched from the Western Test Range in California by an Atlas F Launch Vehicle on October 13, 1978. TIROS-N is the first of the third generation weather satellites. The remaining seven satellites in this series, called collectively the TIROS-N series, will be designated NOAA A-G before launch, and as NOAA 6-12 once in orbit. NOAA-A is planned to be launched during the spring of 1979 with the remaining three pairs of spacecraft to be launched roughly at the rate of one pair every two years. The TIROS-N satellites series replaces the ITOS series of meteorological satellites and have a design lifetime of 2 years. The initial TIROS-N satellite, also called TIROS-N, was placed into a near- polar, sun-synchronous orbit with an inclination of 98.9° and at an average altitude of 854 kilometers (km) in contrast to 1511 km for NOAA-5.