Second Quarter 2003 Quarterly Launch Report 1
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EOOS Posters Abstracts
Posters Submissions – EOOS Conference 21 23 November 2018 1. Sylvie Pouliquen Ifremer [email protected] Authors: "Gille Reverdin CNRS/INSU email: [email protected] , Pierre-Yves Le Traon Ifremer & Mercator-Ocean email: [email protected]) and the Coriolis 2014-2020 steering committee." Theme: From standalone to integrated ocean and coastal observing platforms Title: Coriolis: an integrated in-situ ocean observation infrastructure for operational oceanography and ocean/climate research "The Coriolis (www.coriolis.eu.org) structure gathers efforts of seven French institutes (CNES, CNRS, IFREMER, IPEV, IRD, Météo-France, SHOM, CEREMA) to organize the in-situ component of the French operational oceanography infrastructure. The objective is to organize the data acquisition and real- time/delayed mode data processing of in-situ measurements required for operational oceanography and ocean/climate research. Coriolis is focused on a limited number of physical and biogeochemical parameters that are acquired systematically and in real time or slightly delayed mode. Coriolis follows a fully open data policy. The framework of collaboration for Coriolis was renewed in 2014 and now covers the time period of 2014 up to 2020. By signing this new agreement, the eight directors of French institutes have clearly stated their willingness to sustain and consolidate further the Coriolis in-situ infrastructure. The new framework agreement strengthens the links between research and operational oceanography. The scope is also extended to integrate the main French contributions to the global and regional in-situ observing systems: Argo, gliders, research vessels, ship of opportunities, drifting buoys, marine mammals, tidal networks and high frequency coastal observatories. -
Kaluza-Klein Gravity, Concentrating on the General Rel- Ativity, Rather Than Particle Physics Side of the Subject
Kaluza-Klein Gravity J. M. Overduin Department of Physics and Astronomy, University of Victoria, P.O. Box 3055, Victoria, British Columbia, Canada, V8W 3P6 and P. S. Wesson Department of Physics, University of Waterloo, Ontario, Canada N2L 3G1 and Gravity Probe-B, Hansen Physics Laboratories, Stanford University, Stanford, California, U.S.A. 94305 Abstract We review higher-dimensional unified theories from the general relativity, rather than the particle physics side. Three distinct approaches to the subject are identi- fied and contrasted: compactified, projective and noncompactified. We discuss the cosmological and astrophysical implications of extra dimensions, and conclude that none of the three approaches can be ruled out on observational grounds at the present time. arXiv:gr-qc/9805018v1 7 May 1998 Preprint submitted to Elsevier Preprint 3 February 2008 1 Introduction Kaluza’s [1] achievement was to show that five-dimensional general relativity contains both Einstein’s four-dimensional theory of gravity and Maxwell’s the- ory of electromagnetism. He however imposed a somewhat artificial restriction (the cylinder condition) on the coordinates, essentially barring the fifth one a priori from making a direct appearance in the laws of physics. Klein’s [2] con- tribution was to make this restriction less artificial by suggesting a plausible physical basis for it in compactification of the fifth dimension. This idea was enthusiastically received by unified-field theorists, and when the time came to include the strong and weak forces by extending Kaluza’s mechanism to higher dimensions, it was assumed that these too would be compact. This line of thinking has led through eleven-dimensional supergravity theories in the 1980s to the current favorite contenders for a possible “theory of everything,” ten-dimensional superstrings. -
To All the Craft We've Known Before
400,000 Visitors to Mars…and Counting Liftoff! A Fly’s-Eye View “Spacers”Are Doing it for Themselves September/October/November 2003 $4.95 to all the craft we’ve known before... 23rd International Space Development Conference ISDC 2004 “Settling the Space Frontier” Presented by the National Space Society May 27-31, 2004 Oklahoma City, Oklahoma Location: Clarion Meridian Hotel & Convention Center 737 S. Meridian, Oklahoma City, OK 73108 (405) 942-8511 Room rate: $65 + tax, 1-4 people Planned Programming Tracks Include: Spaceport Issues Symposium • Space Education Symposium • “Space 101” Advanced Propulsion & Technology • Space Health & Biology • Commercial Space/Financing Space Space & National Defense • Frontier America & the Space Frontier • Solar System Resources Space Advocacy & Chapter Projects • Space Law and Policy Planned Tours include: Cosmosphere Space Museum, Hutchinson, KS (all day Thursday, May 27), with Max Ary Oklahoma Spaceport, courtesy of Oklahoma Space Industry Development Authority Oklahoma City National Memorial (Murrah Building bombing memorial) Omniplex Museum Complex (includes planetarium, space & science museums) Look for updates on line at www.nss.org or www.nsschapters.org starting in the fall of 2003. detach here ISDC 2004 Advance Registration Form Return this form with your payment to: National Space Society-ISDC 2004, 600 Pennsylvania Ave. S.E., Suite 201, Washington DC 20003 Adults: #______ x $______.___ Seniors/Students: #______ x $______.___ Voluntary contribution to help fund 2004 awards $______.___ Adult rates (one banquet included): $90 by 12/31/03; $125 by 5/1/04; $150 at the door. Seniors(65+)/Students (one banquet included): $80 by 12/31/03; $100 by 5/1/04; $125 at the door. -
Dod Space Technology Guide
Foreword Space-based capabilities are integral to the U.S.’s national security operational doctrines and processes. Such capa- bilities as reliable, real-time high-bandwidth communica- tions can provide an invaluable combat advantage in terms of clarity of command intentions and flexibility in the face of operational changes. Satellite-generated knowledge of enemy dispositions and movements can be and has been exploited by U.S. and allied commanders to achieve deci- sive victories. Precision navigation and weather data from space permit optimal force disposition, maneuver, decision- making, and responsiveness. At the same time, space systems focused on strategic nuclear assets have enabled the National Command Authorities to act with confidence during times of crisis, secure in their understanding of the strategic force postures. Access to space and the advantages deriving from operat- ing in space are being affected by technological progress If our Armed Forces are to be throughout the world. As in other areas of technology, the faster, more lethal, and more precise in 2020 advantages our military derives from its uses of space are than they are today, we must continue to dynamic. Current space capabilities derive from prior invest in and develop new military capabilities. decades of technology development and application. Joint Vision 2020 Future capabilities will depend on space technology programs of today. Thus, continuing investment in space technologies is needed to maintain the “full spectrum dominance” called for by Joint Vision 2010 and 2020, and to protect freedom of access to space by all law-abiding nations. Trends in the availability and directions of technology clearly suggest that the U.S. -
Guía De Instrumentos Y Métodos De Observación : Volumen IV
Guía de Instrumentos y Métodos de Observación Volumen IV – Observaciones desde el espacio Edición de 2018 TIEMPO CLIMA AGUA OMM-N° 8 Guía de Instrumentos y Métodos de Observación Volumen IV – Observaciones desde el espacio Edición de 2018 OMM-N° 8 NOTA DE LA EDICIÓN METEOTERM, base terminológica de la OMM, está disponible en la página web: http://public. wmo.int/es/recursos/meteoterm. Conviene informar al lector de que cuando copie un hipervínculo seleccionándolo del texto podrán aparecer espacios adicionales inmediatamente después de http://, https://, ftp://, mailto:, y después de las barras (/), los guiones (-), los puntos (.) y las secuencias ininterrumpidas de caracteres (letras y números). Es necesario suprimir esos espacios de la dirección URL copiada. La dirección URL correcta aparece cuando se pone el cursor sobre el enlace o cuando se hace clic en el enlace y luego se copia en el navegador. OMM-N° 8 © Organización Meteorológica Mundial, 2018 La OMM se reserva el derecho de publicación en forma impresa, electrónica o de otro tipo y en cualquier idioma. Pueden reproducirse pasajes breves de las publicaciones de la OMM sin autorización siempre que se indique claramente la fuente completa. La correspondencia editorial, así como todas las solicitudes para publicar, reproducir o traducir la presente publicación parcial o totalmente deberán dirigirse al: Presidente de la Junta de Publicaciones Organización Meteorológica Mundial (OMM) 7 bis, avenue de la Paix Tel.: +41 (0) 22 730 84 03 Case postale No 2300 Fax: +41 (0) 22 730 81 17 CH-1211 Genève 2, Suiza Correo electrónico: [email protected] ISBN 978-92-63-30008-9 NOTA Las denominaciones empleadas en las publicaciones de la OMM y la forma en que aparecen presentados los datos que contienen no entrañan, de parte de la Organización, juicio alguno sobre la condición jurídica de ninguno de los países, territorios, ciudades o zonas citados o de sus autoridades, ni respecto de la delimitación de sus fronteras o límites. -
What Is Gravity Probe B? a Quest for Experimental Truth the GP-B Flight
What is Gravity Probe B? than Gravity Probe B. It’s just a star, a telescope, and a spinning sphere.” However, it took the exceptional collaboration of Stanford, Gravity Probe B (GP-B) is a NASA physics mission to experimentally MSFC, Lockheed Martin and a host of others more than four decades investigate Einstein’s 1916 general theory of relativity—his theory of gravity. to develop the ultra-precise gyroscopes and the other cutting- GP-B uses four spherical gyroscopes and a telescope, housed in a satellite edge technologies necessary to carry out this “simple” experiment. orbiting 642 km (400 mi) above the Earth, to measure, with unprecedented accuracy, two extraordinary effects predicted by the general theory of rela- The GP-B Flight Mission & Data Analysis tivity: 1) the geodetic effect—the amount by which the Earth warps the local spacetime in which it resides; and 2) the frame-dragging effect—the amount On April 20, 2004 at 9:57:24 AM PDT, a crowd of over 2,000 current and by which the rotating Earth drags its local spacetime around with it. GP-B former GP-B team members and supporters watched and cheered as the tests these two effects by precisely measuring the precession (displacement) GP-B spacecraft lifted off from Vandenberg Air Force Base. That emotionally angles of the spin axes of the four gyros over the course of a year and com- overwhelming day, culminating with the extraordinary live video of paring these experimental results with predictions from Einstein’s theory. the spacecraft separating from the second stage booster meant, as GP-B Program Manager Gaylord Green put it, “that 10,000 things went right.” A Quest for Experimental Truth Once in orbit, the spacecraft first underwent a four-month Initialization The idea of testing general relativity with orbiting gyroscopes was sug- and Orbit Checkout (IOC), in which all systems and instruments were gested independently by two physicists, George Pugh and Leonard Schiff, initialized, tested, and optimized for the data collection to follow. -
Cosmic Origins Newsletter, September 2016, Vol. 5, No. 2
National Aeronautics and Space Administration Cosmic Origins Newsletter September 2016 Volume 5 Number 2 Summer 2016 Cosmic Origins Program Inside this Issue Update Summer 2016 Cosmic Origins Program Update ............................1 Mansoor Ahmed, COR Program Manager Hubble Reveals Stellar Fireworks in ‘Skyrocket’ Galaxy ................2 Message from the Astrophysics Division Director .........................2 Susan Neff, COR Program Chief Scientist Light Echoes Give Clues to Protoplanetary Disk ............................3 Far-IR Surveyor Study Status .............................................................5 Welcome to the September 2016 Cosmic Origins (COR) newslet- LUVOIR Study Status .........................................................................5 ter. In this issue, we provide updates on several activities relevant to Strategic Astrophysics Technology (SAT) Selections the COR Program objectives. Some of these activities are not under for ROSES-2015 ...................................................................................6 the direct purview of the program, but are relevant to COR goals, Technology Solicitations to Enable Astrophysics Discoveries ......6 therefore we try to keep you informed about their progress. Cosmic Origins Suborbital Program: Balloon Program – BETTII ................................................................7 In January 2016, Paul Hertz (Director, NASA Astrophysics) News from SOFIA ...............................................................................8 presented his -
SEER for Hardware's Cost Model for Future Orbital Concepts (“FAR OUT”)
Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com SEER for Hardware’s Cost Model for Future Orbital Concepts (“FAR OUT”) Lee Fischman ISPA/SCEA Industry Hills 2008 Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Introduction A model for predicting the cost of long term unmanned orbital spacecraft (Far Out) has been developed at the request of AFRL. Far Out has been integrated into SEER for Hardware. This presentation discusses the Far Out project and resulting model. © 2008 Galorath Incorporated Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Goals • Estimate space satellites in any earth orbit. Deep space exploration missions may be considered as data is available, or may be an area for further research in Phase 3. • Estimate concepts to be launched 10-20 years into the future. • Cost missions ranging from exploratory to strategic, with a specific range decided based on estimating reliability. The most reliable estimates are likely to be in the middle of this range. • Estimates will include hardware, software, systems engineering, and production. • Handle either government or commercial missions, either “one-of-a-kind” or constellations. • Be used in a “top-down” manner using relatively less specific mission resumes, similar to those available from sources such as the Earth Observation Portal or Janes Space Directory. © 2008 Galorath Incorporated Presented at the 2008 SCEA-ISPA Joint Annual Conference and Training Workshop - www.iceaaonline.com Challenge: Technology Change Over Time Evolution in bus technologies Evolution in payload technologies and performance 1. -
UHD with Asiasat
UHD with AsiaSat Alan WONG Manager, Sales Solutions 23 Jun 2016 AsiaSat Proprietary & Confidential AsiaSat Proprietary & Confidential Contents • Brief Introduction of AsiaSat • Hands-on Satellite Transmission • Our Engagement with UHD • How we see UHD? • AsiaSat UHD Platform • Next Step AsiaSat Proprietary & Confidential UHD with AsiaSat 2 Brief Introduction of AsiaSat Our Background Our Satellite Fleet Our Facilities Our People AsiaSat Proprietary & Confidential AsiaSat Corporate Video AsiaSat Proprietary & Confidential UHD with AsiaSat 4 Our Background Head-quartered in Hong Kong Established in 1988 Listing in Hong Kong Stock Exchange Regional Satellite Operator • Asia’s leading satellite operator, aiming to provide highest quality satellite communications services in the region Coverage • Across 50 countries in Asia-Pacific • Reaching 2/3 of world's population Customer Profile • International and Regional TV Broadcasters • Telecommunications Service Providers • News Agencies • Corporations and Governments AsiaSat Proprietary & Confidential UHD with AsiaSat 5 Our Satellite Fleet C-band Ku-band For more details of our satellite fleet, please visit our web site (http://www.asiasat.com/technology/satellite-fleet). AsiaSat Proprietary & Confidential UHD with AsiaSat 6 Our Earth Stations Tai Po Earth Station Stanley Earth Station For more details of our facilities, please visit our web site (http://www.asiasat.com/aboutus/facilities). AsiaSat Proprietary & Confidential UHD with AsiaSat 7 Tai Po Earth Station AsiaSat Tai Po Earth Station is Antennas Services • 1x 1.3m (C) • Uplink Service located at the Tai Po Industrial • 2x 9.0m (C) • Downlink Service Estate in the New Territories, • 3x 7.3m (C) • Occasional Service Hong Kong. • 2x 6.3m (C) • Conditional Access • 1x 6.1m (C) Service • 4x 7.3m (Ku) • Compression Service • 2x 6.3m (Ku) • Playout Service The Station is a two level building • 1x 4.9m (Ku) • Monitoring Service of 5,551 sq.m. -
Design by Contract: the Lessons of Ariane
. Editor: Bertrand Meyer, EiffelSoft, 270 Storke Rd., Ste. 7, Goleta, CA 93117; voice (805) 685-6869; [email protected] several hours (at least in earlier versions of Ariane), it was better to let the computa- tion proceed than to stop it and then have Design by to restart it if liftoff was delayed. So the SRI computation continues for 50 seconds after the start of flight mode—well into the flight period. After takeoff, of course, this com- Contract: putation is useless. In the Ariane 5 flight, Object Technology however, it caused an exception, which was not caught and—boom. The exception was due to a floating- point error during a conversion from a 64- The Lessons bit floating-point value, representing the flight’s “horizontal bias,” to a 16-bit signed integer: In other words, the value that was converted was greater than what of Ariane can be represented as a 16-bit signed inte- ger. There was no explicit exception han- dler to catch the exception, so it followed the usual fate of uncaught exceptions and crashed the entire software, hence the onboard computers, hence the mission. This is the kind of trivial error that we Jean-Marc Jézéquel, IRISA/CNRS are all familiar with (raise your hand if you Bertrand Meyer, EiffelSoft have never done anything of this sort), although fortunately the consequences are usually less expensive. How in the world everal contributions to this made up of respected experts from major department have emphasized the European countries, which produced a How in the world could importance of design by contract report in hardly more than a month. -
GLONASS Spacecraft
INNO V AT IO N The task of designing and developing the GLONASS GLONASS spacecraft fell to the Scientific Production Association of Applied Mechan ics (Nauchno Proizvodstvennoe Ob"edinenie Spacecraft Prikladnoi Mekaniki or NPO PM) , located near Krasnoyarsk in Siberia. This major aero Nicholas L. Johnson space industrial complex was established in 1959 as a division of Sergei Korolev 's Kaman Sciences Corporation Expe1imental Design Bureau (Opytno Kon struktorskoe Byuro or OKB). (Korolev , among other notable achievements , led the Fourteen years after the launch of the effort to develop the Soviet Union's first first test spacecraft, the Russian Global Nav launch vehicle - the A launcher - which igation Satellite System (Global 'naya Navi placed Sputnik 1 into orbit.) The founding gatsionnaya Sputnikovaya Sistema or and current general director and chief GLONASS) program remains viable and designer is Mikhail Fyodorovich Reshetnev, essentially on schedule despite the economic one of only two still-active chief designers and political turmoil surrounding the final from Russia's fledgling 1950s-era space years of the Soviet Union and the emergence program. of the Commonwealth of Independent States A closed facility until the early 1990s, (CIS). By the summer of 1994, a total of 53 NPO PM has been responsible for all major GLONASS spacecraft had been successfully Russian operational communications, navi Despite the significant economic hardships deployed in nearly semisynchronous orbits; gation, and geodetic satellite systems to associated with the breakup of the Soviet Union of the 53 , nearly 12 had been normally oper date. Serial (or assembly-line) production of and the transition to a modern market economy, ational since the establishment of the Phase I some spacecraft, including Tsikada and Russia continues to develop its space programs, constellation in 1990. -
The Evolving Launch Vehicle Market Supply and the Effect on Future NASA Missions
Presented at the 2007 ISPA/SCEA Joint Annual International Conference and Workshop - www.iceaaonline.com The Evolving Launch Vehicle Market Supply and the Effect on Future NASA Missions Presented at the 2007 ISPA/SCEA Joint International Conference & Workshop June 12-15, New Orleans, LA Bob Bitten, Debra Emmons, Claude Freaner 1 Presented at the 2007 ISPA/SCEA Joint Annual International Conference and Workshop - www.iceaaonline.com Abstract • The upcoming retirement of the Delta II family of launch vehicles leaves a performance gap between small expendable launch vehicles, such as the Pegasus and Taurus, and large vehicles, such as the Delta IV and Atlas V families • This performance gap may lead to a variety of progressions including – large satellites that utilize the full capability of the larger launch vehicles, – medium size satellites that would require dual manifesting on the larger vehicles or – smaller satellites missions that would require a large number of smaller launch vehicles • This paper offers some comparative costs of co-manifesting single- instrument missions on a Delta IV/Atlas V, versus placing several instruments on a larger bus and using a Delta IV/Atlas V, as well as considering smaller, single instrument missions launched on a Minotaur or Taurus • This paper presents the results of a parametric study investigating the cost- effectiveness of different alternatives and their effect on future NASA missions that fall into the Small Explorer (SMEX), Medium Explorer (MIDEX), Earth System Science Pathfinder (ESSP), Discovery,