1999 EOS Reference Handbook
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GPS Radio Occultation with CHAMP, GRACE-A, Terrasar-X, and COSMIC: Brief Review of Results from GFZ J
GPS radio occultation with CHAMP, GRACE-A, TerraSAR-X, and COSMIC: Brief review of results from GFZ J. Wickert, G. Beyerle, C. Falck, S. Heise, R. König, G. Michalak, D. Pingel*, M. Rothacher, T. Schmidt, and C. Viehweg GeoForschungsZentrum Potsdam, * Deutscher Wetterdienst Overview Current GPS occultation missions During the last decade ground and space based GNSS techniques for atmospheric/ionospheric remote sensing were established. The currently increasing number of receiver platforms (e.g., extension of regional/global ground networks and additional LEO satellites) together with future additional transmitters (GALILEO, reactivated GLONASS, new signal structures for GPS) will extend the potential of these innovative sounding techniques during the next years. Here, we focus to GPS radio CHAMP GRACE TerraSAR-X occultation and present selected examples of recent GFZ results. The activities include orbit and atmospheric /ionospheric occultation data processing for several satellite mission (CHAMP,GRACE-A, SAC-C, and COSMIC), but also various applications. Data sets from CHAMP, GRACE and COSMIC MetOp COSMIC SAC-C Current GPS radio occultation missions: CHAMP (launch July 15, 2000), GRACE (March 17, 2002), TerraSAR-X (June 15, 2007), MetOp (October 18, 2006), COSMIC (April 15, 2006) and SAC-C(November 21, 2000). Number of daily available vertical atmospheric profiles, derived from CHAMP (left), GRACE (middle), and COSMIC (right, UCAR processing) measurements (note the different scale). COSMIC provides significantly more data compared to CHAMP and GRACE-A. The long-term set from CHAMP is unique (300 km orbit altitude expected in Dec. 2008). Validation of CHAMP with MOZAIC aircraft data Near-real time data from CHAMP and GRACE-A (a) (b) (c) GFZ provides near-real time occultation data (bending angle and refractivity profiles) from CHAMP and GRACE-A using it’s operational ground infrastructure including 2 receiving antennas at Ny Ålesund. -
Global Sea-Level Budget 1993–Present
Earth Syst. Sci. Data, 10, 1551–1590, 2018 https://doi.org/10.5194/essd-10-1551-2018 © Author(s) 2018. This work is distributed under the Creative Commons Attribution 4.0 License. Global sea-level budget 1993–present WCRP Global Sea Level Budget Group A full list of authors and their affiliations appears at the end of the paper. Correspondence: Anny Cazenave ([email protected]) Received: 13 April 2018 – Discussion started: 15 May 2018 Revised: 31 July 2018 – Accepted: 1 August 2018 – Published: 28 August 2018 Abstract. Global mean sea level is an integral of changes occurring in the climate system in response to un- forced climate variability as well as natural and anthropogenic forcing factors. Its temporal evolution allows changes (e.g., acceleration) to be detected in one or more components. Study of the sea-level budget provides constraints on missing or poorly known contributions, such as the unsurveyed deep ocean or the still uncertain land water component. In the context of the World Climate Research Programme Grand Challenge entitled “Re- gional Sea Level and Coastal Impacts”, an international effort involving the sea-level community worldwide has been recently initiated with the objective of assessing the various datasets used to estimate components of the sea-level budget during the altimetry era (1993 to present). These datasets are based on the combination of a broad range of space-based and in situ observations, model estimates, and algorithms. Evaluating their quality, quantifying uncertainties and identifying sources of discrepancies between component estimates is extremely useful for various applications in climate research. -
A Survey and Assessment of the Capabilities of Cubesats for Earth Observation
Acta Astronautica 74 (2012) 50–68 Contents lists available at SciVerse ScienceDirect Acta Astronautica journal homepage: www.elsevier.com/locate/actaastro Review A survey and assessment of the capabilities of Cubesats for Earth observation Daniel Selva a,n, David Krejci b a Massachusetts Institute of Technology, Cambridge, MA 02139, USA b Vienna University of Technology, Vienna 1040, Austria article info abstract Article history: In less than a decade, Cubesats have evolved from purely educational tools to a standard Received 2 December 2011 platform for technology demonstration and scientific instrumentation. The use of COTS Accepted 9 December 2011 (Commercial-Off-The-Shelf) components and the ongoing miniaturization of several technologies have already led to scattered instances of missions with promising Keywords: scientific value. Furthermore, advantages in terms of development cost and develop- Cubesats ment time with respect to larger satellites, as well as the possibility of launching several Earth observation satellites dozens of Cubesats with a single rocket launch, have brought forth the potential for University satellites radically new mission architectures consisting of very large constellations or clusters of Systems engineering Cubesats. These architectures promise to combine the temporal resolution of GEO Remote sensing missions with the spatial resolution of LEO missions, thus breaking a traditional trade- Nanosatellites Picosatellites off in Earth observation mission design. This paper assesses the current capabilities of Cubesats with respect to potential employment in Earth observation missions. A thorough review of Cubesat bus technology capabilities is performed, identifying potential limitations and their implications on 17 different Earth observation payload technologies. These results are matched to an exhaustive review of scientific require- ments in the field of Earth observation, assessing the possibilities of Cubesats to cope with the requirements set for each one of 21 measurement categories. -
OSTM/Jason-2 Products Handbook
OSTM/Jason-2 Products Handbook References: CNES : SALP-MU-M-OP-15815-CN EUMETSAT : EUM/OPS-JAS/MAN/08/0041 JPL: OSTM-29-1237 NOAA : Issue: 1 rev 0 Date: 17 June 2008 OSTM/Jason-2 Products Handbook Iss :1.0 - date : 17 June 2008 i.1 Chronology Issues: Issue: Date: Reason for change: 1rev0 June 17, 2008 Initial Issue People involved in this issue: Written by (*) : Date J.P. DUMONT CLS V. ROSMORDUC CLS N. PICOT CNES S. DESAI NASA/JPL H. BONEKAMP EUMETSAT J. FIGA EUMETSAT J. LILLIBRIDGE NOAA R. SHARROO ALTIMETRICS Index Sheet : Context: Keywords: Hyperlink: OSTM/Jason-2 Products Handbook Iss :1.0 - date : 17 June 2008 i.2 List of tables and figures List of tables: Table 1 : Differences between Auxiliary Data for O/I/GDR Products 1 Table 2 : Summary of error budget at the end of the verification phase 9 Table 3 : Main features of the OSTM/Jason-2 satellite 11 Table 4 : Mean classical orbit elements 16 Table 5 : Orbit auxiliary data 16 Table 6 : Equator Crossing Longitudes (in order of Pass Number) 18 Table 7 : Equator Crossing Longitudes (in order of Longitude) 19 Table 8 : Models and standards 21 Table 9 : CLS01 MSS model characteristics 22 Table 10 : CLS Rio 05 MDT model characteristics 23 Table 11 : Recommended editing criteria 26 Table 12 : Recommended filtering criteria 26 Table 13 : Recommended additional empirical tests 26 Table 14 : Main characteristics of (O)(I)GDR products 40 Table 15 - Dimensions used in the OSTM/Jason-2 data sets 42 Table 16 - netCDF variable type 42 Table 17 - Variable’s attributes 43 List of figures: Figure 1 -
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. -
The Journey to Mars: How Donna Shirley Broke Barriers for Women in Space Engineering
The Journey to Mars: How Donna Shirley Broke Barriers for Women in Space Engineering Laurel Mossman, Kate Schein, and Amelia Peoples Senior Division Group Documentary Word Count: 499 Our group chose the topic, Donna Shirley and her Mars rover, because of our connections and our interest level in not only science but strong, determined women. One of our group member’s mothers worked for a man under Ms. Shirley when she was developing the Mars rover. This provided us with a connection to Ms. Shirley, which then gave us the amazing opportunity to interview her. In addition, our group is interested in the philosophy of equality and we have continuously created documentaries that revolve around this idea. Every member of our group is a female, so we understand the struggles and discrimination that women face in an everyday setting and wanted to share the story of a female that faced these struggles but overcame them. Thus after conducting a great amount of research, we fell in love with Donna Shirley’s story. Lastly, it was an added benefit that Ms. Shirley is from Oklahoma, making her story important to our state. All of these components made this topic extremely appealing to us. We conducted our research using online articles, Donna Shirley’s autobiography, “Managing Martians”, news coverage from the launch day, and our interview with Donna Shirley. We started our research process by reading Shirley’s autobiography. This gave us insight into her college life, her time working at the Jet Propulsion Laboratory, and what it was like being in charge of such a barrier-breaking mission. -
Estimating Gale to Hurricane Force Winds Using the Satellite Altimeter
VOLUME 28 JOURNAL OF ATMOSPHERIC AND OCEANIC TECHNOLOGY APRIL 2011 Estimating Gale to Hurricane Force Winds Using the Satellite Altimeter YVES QUILFEN Space Oceanography Laboratory, IFREMER, Plouzane´, France DOUG VANDEMARK Ocean Process Analysis Laboratory, University of New Hampshire, Durham, New Hampshire BERTRAND CHAPRON Space Oceanography Laboratory, IFREMER, Plouzane´, France HUI FENG Ocean Process Analysis Laboratory, University of New Hampshire, Durham, New Hampshire JOE SIENKIEWICZ Ocean Prediction Center, NCEP/NOAA, Camp Springs, Maryland (Manuscript received 21 September 2010, in final form 29 November 2010) ABSTRACT A new model is provided for estimating maritime near-surface wind speeds (U10) from satellite altimeter backscatter data during high wind conditions. The model is built using coincident satellite scatterometer and altimeter observations obtained from QuikSCAT and Jason satellite orbit crossovers in 2008 and 2009. The new wind measurements are linear with inverse radar backscatter levels, a result close to the earlier altimeter high wind speed model of Young (1993). By design, the model only applies for wind speeds above 18 m s21. Above this level, standard altimeter wind speed algorithms are not reliable and typically underestimate the true value. Simple rules for applying the new model to the present-day suite of satellite altimeters (Jason-1, Jason-2, and Envisat RA-2) are provided, with a key objective being provision of enhanced data for near-real- time forecast and warning applications surrounding gale to hurricane force wind events. Model limitations and strengths are discussed and highlight the valuable 5-km spatial resolution sea state and wind speed al- timeter information that can complement other data sources included in forecast guidance and air–sea in- teraction studies. -
Solar Aircraft Design
Cumhuriyet Üniversitesi Fen Fakültesi Cumhuriyet University Faculty of Science Fen Bilimleri Dergisi (CFD), Cilt:36, No: 3 Özel Sayı (2015) Science Journal (CSJ), Vol. 36, No: 3 Special Issue (2015) ISSN: 1300-1949 ISSN: 1300-1949 SOLAR AIRCRAFT DESIGN Sadegh RAHMATI1,*, Amir GHASED2 1,2Department of Mechanical Engineering, Majlesi Branch, Islamic Azad University, Isfahan, Iran Received: 01.02.2015; Accepted: 05.05.2015 ______________________________________________________________________________________________ Abstract. Generally domain Aircraft uses conventional fuel. These fuel having limited life, high cost and pollutant. Also nowadays price of petrol and other fuels are going to be higher, because of scarcity of those fuels. So there is great demand of use of non-exhaustible unlimited source of energy like solar energy. Solar aircraft is one of the ways to utilize solar energy. Solar aircraft uses solar panel to collect the solar radiation for immediate use but it also store the remaining part for the night flight. This paper intended to stimulate research on renewable energy sources for aviation. In future solar powered air planes could be used for different types of aerial momitoring and unmanned flights. This review paper brietly shows history, application and use of solar aircraft. We are focusing on design and fabrication of solar aircraft which is unmanned prototype. Keywords: Solar energy, Reynolds number, Bernoulli’s principle 1. INTRODUCTION Energy comes in different forms. Light is a form of energy. Sun is source of energy called “sunlight”. Sunshine is free and never gets used up Also. There is a lot of it. The sunlight that heats the Earth in an hour has more energy than the people of the world use in a year. -
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. -
SEASAT Geoid Anomalies and the Macquarie Ridge Complex Larry Ruff *
Physics of the Earth and Planetary Interiors, 38 (1985) 59-69 59 Elsevier Science Publishers B.V., Amsterdam - Printed in The Netherlands SEASAT geoid anomalies and the Macquarie Ridge complex Larry Ruff * Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109 (U.S.A.) Anny Cazenave CNES-GRGS, 18Ave. Edouard Belin, Toulouse, 31055 (France) (Received August 10, 1984; revision accepted September 5, 1984) Ruff, L. and Cazenave, A., 1985. SEASAT geoid anomalies and the Macquarie Ridge complex. Phys. Earth Planet. Inter., 38: 59-69. The seismically active Macquarie Ridge complex forms the Pacific-India plate boundary between New Zealand and the Pacific-Antarctic spreading center. The Late Cenozoic deformation of New Zealand and focal mechanisms of recent large earthquakes in the Macquarie Ridge complex appear consistent with the current plate tectonic models. These models predict a combination of strike-slip and convergent motion in the northern Macquarie Ridge, and strike-slip motion in the southern part. The Hjort trench is the southernmost expression of the Macquarie Ridge complex. Regional considerations of the magnetic lineations imply that some oceanic crust may have been consumed at the Hjort trench. Although this arcuate trench seems inconsistent with the predicted strike-slip setting, a deep trough also occurs in the Romanche fracture zone. Geoid anomalies observed over spreading ridges, subduction zones, and fracture zones are different. Therefore, geoid anomalies may be diagnostic of plate boundary type. We use SEASAT data to examine the Maequarie Ridge complex and find that the geoid anomalies for the northern Hjort trench region are different from the geoid anomalies for the Romanche trough. -
Earth Science Data and Information System (ESDIS) Project Update
Earth Science Data and Information System (ESDIS) Project Update October 15-16, 2008 National Snow and Ice Data Center & Physical Oceanography DAAC User Working Group Meeting Pasadena, CA [email protected] ESDIS Project Code 423 NASA GSFC Topics •• ESDISESDIS OrganizationOrganization •• SystemSystem ContextContext •• KeyKey MetricsMetrics •• DataData ArchitectureArchitecture •• KeyKey ActivitiesActivities – Data Discovery – Customer Satisfaction & Metrics – Operations Management 2 Earth Science Data and Information System (ESDIS) Project • The ESDIS Project is responsible for the Earth Observing System Data and Information System (EOSDIS), one of the largest civilian Science Information System in the world • The EOSDIS: – Ingests, archives, processes, and distributes an unprecedented volume of science data for NASA’s flagship Earth science missions (e.g., Terra, Aqua, Aura, ICESat) – Supports unique requirements of a variety of Earth science disciplines (e.g., land, atmosphere, snow/ice, and ocean) as well as inter- disciplinary researchers, climate This Jason sea-surface height image shows modelers, and application users sea surface height anomalies with the seasonal cycle (the effects of summer, fall, (e.g., U.S. Forest Service) winter, and spring) removed. Each image is a 10-day average of data, centered on the date – Employs state-of-the-art hardware indicated. and software technology to achieve Courtesy: NASA EOSDIS Physical 3 Oceanography DAAC required data throughput EOSDIS Manages Data For All 24 EOS Measurements Aqua (5/02) -
Sea Level Change 13SM Supplementary Material
Sea Level Change 13SM Supplementary Material Coordinating Lead Authors: John A. Church (Australia), Peter U. Clark (USA) Lead Authors: Anny Cazenave (France), Jonathan M. Gregory (UK), Svetlana Jevrejeva (UK), Anders Levermann (Germany), Mark A. Merrifield (USA), Glenn A. Milne (Canada), R. Steven Nerem (USA), Patrick D. Nunn (Australia), Antony J. Payne (UK), W. Tad Pfeffer (USA), Detlef Stammer (Germany), Alakkat S. Unnikrishnan (India) Contributing Authors: David Bahr (USA), Jason E. Box (Denmark/USA), David H. Bromwich (USA), Mark Carson (Germany), William Collins (UK), Xavier Fettweis (Belgium), Piers Forster (UK), Alex Gardner (USA), W. Roland Gehrels (UK), Rianne Giesen (Netherlands), Peter J. Gleckler (USA), Peter Good (UK), Rune Grand Graversen (Sweden), Ralf Greve (Japan), Stephen Griffies (USA), Edward Hanna (UK), Mark Hemer (Australia), Regine Hock (USA), Simon J. Holgate (UK), John Hunter (Australia), Philippe Huybrechts (Belgium), Gregory Johnson (USA), Ian Joughin (USA), Georg Kaser (Austria), Caroline Katsman (Netherlands), Leonard Konikow (USA), Gerhard Krinner (France), Anne Le Brocq (UK), Jan Lenaerts (Netherlands), Stefan Ligtenberg (Netherlands), Christopher M. Little (USA), Ben Marzeion (Austria), Kathleen L. McInnes (Australia), Sebastian H. Mernild (USA), Didier Monselesan (Australia), Ruth Mottram (Denmark), Tavi Murray (UK), Gunnar Myhre (Norway), J.P. Nicholas (USA), Faezeh Nick (Norway), Mahé Perrette (Germany), David Pollard (USA), Valentina Radić (Canada), Jamie Rae (UK), Markku Rummukainen (Sweden), Christian Schoof (Canada), Aimée Slangen (Australia/Netherlands), Jan H. van Angelen (Netherlands), Willem Jan van de Berg (Netherlands), Michiel van den Broeke (Netherlands), Miren Vizcaíno (Netherlands), Yoshihide Wada (Netherlands), Neil J. White (Australia), Ricarda Winkelmann (Germany), Jianjun Yin (USA), Masakazu Yoshimori (Japan), Kirsten Zickfeld (Canada) Review Editors: Jean Jouzel (France), Roderik van de Wal (Netherlands), Philip L.