MDL ANNUAL REPORT Is Devoted to JPL Chief Technologist Dr
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Ka-Band Satellite Consumer Triple-Play and Professional Video Services
Ka-Band Satellite Consumer Triple-Play and Professional Video Services Guillaume Benoit, Hector Fenech, Stefano Pezzana, and Alessia Tomatis Eutelsat, 70 rue Balard, 75015 Paris, France +33 1 53 98 47 47 {gbenoit,hfenech,spezzana,atomatis}@eutelsat.fr Abstract. This article presents Eutelsat European Ka-band implementation of the broadband ToowayTM service and its evolution through a dedicated Ka-band exclusive satellite (KA-SAT). It also explains Eutelsat’s choice in se- lecting the Ka-band for interactive services, broadcast video and IPTV ser- vices, demonstrating the optimal consumer service synergy between existing Ku-band and new Ka-band services. KA-SAT satellite is not focusing only on consumer triple-play services. In- deed, Eutelsat strategy consists in offering also professional video and data services in Ka-band (video distribution, video contribution, e-cinema, file transport) sharing the same transparent satellite bandwidth and the same ground segment infrastructure. For those professional video applications the last content processing (SVC) and satellite transport (DVB-S2 ACM) techniques are under deployment and this paper will present simulation results and link budgets estimations for a large number of future commercial applications. 1 Introduction Eutelsat operates 25 satellites in the geostationary arc from 15°W to 70.5°E offering a variety of services from corporate networks to broadcasting. The HOT BIRD™ con- stellation at 13°E constitutes the prime position for DTH (Direct to Home) and cable broadcasting, utilizing the full Ku-band spectrum from 10.70 GHz to 12.75 GHz. There are 102 transponders delivering about 1400 TV channels. The HOT BIRD™ service area reaches some 120 million satellite and cable households. -
James A. Sinclair
James A. Sinclair MS 183-601, Jet Propulsion Laboratory Research Scientist 4800 Oak Grove Dr, Pasadena, CA 91109 Jet Propulsion Laboratory/Caltech E-mail: [email protected] Tel: +1 (818) 354-4853 Education 2010 - 2014 DPhil Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, United Kingdom. Thesis title: “Seasonal and interannual variability in Saturn’s stratosphere” Advisor: Prof. Patrick Irwin 2006 - 2010 MPhys Astrophysics (1st class), University of St. Andrews, St. Andrews, United Kingdom Thesis title: “Impact of stellar model spectra on disc detection” Advisor: Dr. Christiane Helling Research Experience 2018-Present Research Scientist, Jet Propulsion Laboratory/Caltech, Pasadena, CA, United States. • Auroral forcing of Jupiter’s stratospheric thermal structure and chemistry from mid-infrared spectroscopy. • Mid-infrared measurements and analysis of Jupiter’s dynamic weather layer to support the Juno mission. • Non-LTE radiative-transfer modelling of Jupiter’s atmosphere. • Seasonal variability in Saturn’s atmosphere. • Coupling of Neptune’s troposphere and stratosphere. • Influence of comet/asteroid impacts on Jupiter’s atmosphere. • Science collaborator for development of next-generation planetary-science instruments. 2015-2018 NASA Postdoctoral Fellow, Jet Propulsion Laboratory/Caltech, Pasadena, CA, United States Mentor: Dr. Glenn Orton • Auroral forcing of Jupiter’s stratospheric thermal structure and chemistry from mid-infrared spectroscopy. • Mid-infrared measurements and analysis of Jupiter’s dynamic weather layer to support the Juno mission. • Retrieval analyses of Voyager and Cassini spectra to derive atmospheric information at Jupiter’s poles. 2014-2015 Postdoctoral Research Assistant, Atmospheric, Oceanic & Planetary Physics, University of Oxford, Oxford, United Kingdom. Supervisors: Prof. Patrick Irwin, Dr. Simon Calcutt • Forward-model spectra simulations of the Martian atmosphere in nadir, limb and occultation sounding. -
Telecommunikation Satellites: the Actual Situation and Potential Future Developments
Telecommunikation Satellites: The Actual Situation and Potential Future Developments Dr. Manfred Wittig Head of Multimedia Systems Section D-APP/TSM ESTEC NL 2200 AG Noordwijk [email protected] March 2003 Commercial Satellite Contracts 25 20 15 Europe US 10 5 0 1995 1996 1997 1998 1999 2000 2001 2002 2003 European Average 5 Satellites/Year US Average 18 Satellites/Year Estimation of cumulative value chain for the Global commercial market 1998-2007 in BEuro 35 27 100% 135 90% 80% 225 Spacecraft Manufacturing 70% Launch 60% Operations Ground Segment 50% Services 40% 365 30% 20% 10% 0% 1 Consolidated Turnover of European Industry Commercial Telecom Satellite Orders 2000 30 2001 25 2002 3 (7) Firm Commercial Telecom Satellite Orders in 2002 Manufacturer Customer Satellite Astrium Hispasat SA Amazonas (Spain) Boeing Thuraya Satellite Thuraya 3 Telecommunications Co (U.A.E.) Orbital Science PT Telekommunikasi Telkom-2 Indonesia Hangar Queens or White Tails Orders in 2002 for Bargain Prices of already contracted Satellites Manufacturer Customer Satellite Alcatel Space New Indian Operator Agrani (India) Alcatel Space Eutelsat W5 (France) (1998 completed) Astrium Hellas-Sat Hellas Sat Consortium Ltd. (Greece-Cyprus) Commercial Telecom Satellite Orders in 2003 Manufacturer Customer Satellite Astrium Telesat Anik F1R 4.2.2003 (Canada) Planned Commercial Telecom Satellite Orders in 2003 SES GLOBAL Three RFQ’s: SES Americom ASTRA 1L ASTRA 1K cancelled four orders with Alcatel Space in 2001 INTELSAT Launched five satellites in the last 13 month average fleet age: 11 Years of remaining life PanAmSat No orders expected Concentration on cash flow generation Eutelsat HB 7A HB 8 expected at the end of 2003 Telesat Ordered Anik F1R from Astrium Planned Commercial Telecom Satellite Orders in 2003 Arabsat & are expected to replace Spacebus 300 Shin Satellite (solar-array steering problems) Korea Telecom Negotiation with Alcatel Space for Koreasat Binariang Sat. -
Eutelsat S.A. €300,000,000 3.125% Bonds Due 2022 Issue Price: 99.148 Per Cent
EUTELSAT S.A. €300,000,000 3.125% BONDS DUE 2022 ISSUE PRICE: 99.148 PER CENT The €300,000,000 aggregate principal amount 3.125% per cent. bonds due 10 October 2022 (the Bonds) of Eutelsat S.A. (the Issuer) will be issued outside the Republic of France on 9 October 2012 (the Bond Issue). Each Bond will bear interest on its principal amount at a fixed rate of 3.125 percent. per annum from (and including) 9 October 2012 (the Issue Date) to (but excluding) 10 October 2022, payable in Euro annually in arrears on 10 October in each year and commencing on 10 October 2013, as further described in "Terms and Conditions of the Bonds - Interest"). Unless previously redeemed or purchased and cancelled in accordance with the terms and conditions of the Bonds, the Bonds will be redeemed at their principal amount on 10 October 2022 (the Maturity Date). The Issuer may at its option, and in certain circumstances shall, redeem all (but not part) of the Bonds at par plus any accrued and unpaid interest upon the occurrence of certain tax changes as further described in the section "Terms and Conditions of the Bonds - Redemption and Purchase - Redemption for tax reasons". The Bondholders may under certain conditions request the Issuer to redeem all or part of the Bonds following the occurrence of certain events triggering a downgrading of the Bonds as further described in the Section "Terms and Conditions of the Bonds — Redemption and Purchase - Redemption following a Change of Control". The obligations of the Issuer in respect of principal and interest payable under the Bonds constitute direct, unconditional, unsecured and unsubordinated obligations of the Issuer and shall at all times rank pari passu among themselves and pari passu with all other present or future direct, unconditional, unsecured and unsubordinated obligations of the Issuer, as further described in "Terms and Conditions of the Bonds - Status". -
EUTELSAT's HOT BIRD™ 9 SATELLITE GOES LIVE Paris, 17
PR/10/09 EUTELSAT’s HOT BIRD™ 9 SATELLITE GOES LIVE Paris, 17 February 2009 Eutelsat Communications (Euronext Paris: ETL) announces the full entry into commercial service of its HOT BIRD™ 9 satellite at 13 degrees East. Built by EADS Astrium and launched on 20 December 2008 by Arianespace, Eutelsat’s new high-capacity broadcast satellite has a projected in-orbit life of more than 15 years. The smooth transfer of television and radio channels onto HOT BIRD™ 9 was completed this morning at 4am GMT by Eutelsat’s control centre, working in close collaboration with broadcast clients and providers of uplink services. With the entry into service of HOT BIRD™ 9, copositioned with Eutelsat’s HOT BIRD™ 6 and HOT BIRD™ 8 satellites, HOT BIRD™ 7A can now be redeployed to 9 degrees East. Rebranded EUROBIRD™ 9A, the satellite will assume all broadcasts currently carried by the 20 transponders on EUROBIRD™ 9 and introduce 18 additional transponders at the 9 degrees East neighbourhood, which has seen the number of channels more than double in one year to almost 150. Released from this position, EUROBIRD™ 9 will continue its useful life in orbit at another location. HOT BIRD™ 9 has a payload of up to 64 Ku-band transponders and is the second in Eutelsat’s new generation of HOT BIRD™ broadcast satellites, following HOT BIRD™ 8 which was launched in 2006. These high-capacity spacecraft have the dual mission of renewing Eutelsat’s resource at its premium video neighbourhood at 13 degrees East and elevating in-orbit security to industry-leading levels. -
Redalyc.Búsqueda General Con La Cámara Mosaico CCD Del
Revista Mexicana de Física ISSN: 0035-001X [email protected] Sociedad Mexicana de Física A.C. México Ferrín, I.; Leal, C.; Hernandez, J. Búsqueda general con la cámara mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela Revista Mexicana de Física, vol. 52, núm. 3, mayo, 2006, pp. 9-11 Sociedad Mexicana de Física A.C. Distrito Federal, México Disponible en: http://www.redalyc.org/articulo.oa?id=57020393003 Cómo citar el artículo Número completo Sistema de Información Científica Más información del artículo Red de Revistas Científicas de América Latina, el Caribe, España y Portugal Página de la revista en redalyc.org Proyecto académico sin fines de lucro, desarrollado bajo la iniciativa de acceso abierto ASTROFISICA´ REVISTA MEXICANA DE FISICA´ S 52 (3) 9–11 MAYO 2006 Busqueda´ general con la camara´ mosaico CCD del telescopio Schmidt de 1m del Observatorio Nacional de Venezuela I. Ferr´ın y C. Leal Facultad de Ciencias, Departamento de F´ısica, Centro de Astrof´ısica Teorica,´ Universidad de Los Andes Merida,´ Venezuela J. Hernandez Centro de investigaciones de astronom´ıa, CIDA, Merida,´ Venezuela Recibido el 25 de noviembre de 2003; aceptado el 12 de octubre de 2004 En el presente trabajo se muestran los resultados del programa de busqueda´ y seguimiento de diversos objetos astronomicos:´ estrellas variables, supernovas y objetos en movimiento dentro del Sistema Solar. Para ello estamos utilizando el telescopio Schmidt de 1m de diametro´ del Observatorio Nacional de Venezuela, el cual tiene acoplado una camara´ mosaico CCD de 67 Megap´ıxeles, en un arreglo de 4 £ 4 CCDs, cada uno de 2048 £ 2048 p´ıxeles. -
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. -
Discovery of Remarkable Opposition Surges on Pluto and Charon
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 1723.pdf Discovery of Remarkable Opposition Surges on Pluto and Charon. B. J. Buratti1, M. D. Hicks1, E. Kramer1, J. Bauer2. 1Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109; bon- [email protected]; 2University of Maryland Department of Astronomy, College Park, MD 20742 Introduction: The July 2015 encounter of the New Observations: Our full request of four nights was Horizons spacecraft with Pluto brought a large Kuiper assigned to this project in 2018 and observations in Belt Object into sharp focus for the first time [1]. Pluto JHK wavelengths (1.2, 1.6 and 2.2 µm) were obtained is a dynamic body with the first-ever active glaciers on all nights. One night was slightly cirussy, and fur- observed outside the Earth, possible clouds, snow, sea- ther data analysis beyond the usual pipeline processing sonal volatile transport, and at least two types of the [2] is required to fully reduce this data. Luckily, this dark, elusive material that is ubiquitous in the outer night was the least critical, being slightly smaller in Solar System and that may be tied to the origin of life solar phase angle than our fourth night, which was ob- on Earth. But as spectacular as this flyby was, it repre- tained at our maximum phase angle. sented an instant in time, leaving out the long temporal baseline that is required to capture, understand, and Table 1-2018 JHK data obtained at opposition model the seasonal events and the types of geologic Time (civil) Solar phase angle (°) Longitude (°) processes that were observed on Pluto – and that hap- July 11 0.008 35 pen on 100-year time scales, at least. -
Site Preservation at Palomar Observatory Robert J
SITE PRESERVATION AT PALOMAR OBSERVATORY ROBERT J. BRUCATO Palomar Observatory, California Institute of Technology, Pasadena, CA 91125 ABSTRACT Palomar Mountain was selected as the site of the 200-inch Hale Telescope in 1934. Since then, and especially over the past decade, the population growth of southern California has had a growing adverse impact on the observatory's environment. In 1981, a very active program was initiated to work with the local governmental agencies to prevent further deterioration of the conditions as the area continues to become increasingly urbanized. The character and scope of the program are described in the paper, as well as more general observations relating to the site preservations process. INTRODUCTION The Palomar Observatory, like many of the major optical observatories in the world, is faced with the prospect of increased man-made interference. The most obvious form of this interference is sky glow, or light pollution, from artificial lighting, but the effects of air pollution, aircraft operations and radio frequency interference are also important. To meet these threats, Gerry Neugebauer (the Director of Palomar Observatory) and I have had to expend a greater fraction of our resources to protect our facilities. The aim of this paper is to describe the situation at Palomar and to share our experience. To be sure, the different local conditions make the situation at each observatory a unique case, but there certainly are elements of this issue that are common to all. HISTORICAL BACKGROUND Palomar Mountain is located in the northern part of San Diego County, about 70 km (about 45 miles) from the city of San Diego and about 160 km (about 100 miles) from the Los Angeles basin to the west-northwest. -
The Sitian Project
An Acad Bras Cienc (2021) 93(Suppl. 1): e20200628 DOI 10.1590/0001-3765202120200628 Anais da Academia Brasileira de Ciências | Annals of the Brazilian Academy of Sciences Printed ISSN 0001-3765 I Online ISSN 1678-2690 www.scielo.br/aabc | www.fb.com/aabcjournal PHYSICAL SCIENCES The SiTian Project JIFENG LIU, ROBERTO SORIA, XUE-FENG WU, HONG WU & ZHAOHUI SHANG Abstract: SiTian is an ambitious ground-based all-sky optical monitoring project, developed by the Chinese Academy of Sciences. The concept is an integrated network of dozens of 1-m-class telescopes deployed partly in China and partly at various other sites around the world. The main science goals are the detection, identification and monitoring of optical transients (such as gravitational wave events, fast radio bursts, supernovae) on the largely unknown timescales of less than 1 day; SiTian will also provide a treasure trove of data for studies of AGN, quasars, variable stars, planets, asteroids, and microlensing events. To achieve those goals, SiTian will scan at least 10,000 square deg of sky every 30 min, down to a detection limit of V ≈ 21 mag. The scans will produce simultaneous light-curves in 3 optical bands. In addition, SiTian will include at least three 4-m telescopes specifically allocated for follow-up spectroscopy of the most interesting targets. We plan to complete the installation of 72 telescopes by 2030 and start full scientific operations in 2032. Key words: surveys, telescopes, transients, relativistic processes. INTRODUCTION a 6.7-m filled aperture) with a 9.6 square deg field of view (Ivezić et al. -
The Big Eye Vol 2 No 1
Friends of Palomar Observatory P.O. Box 200 Palomar Mountain, CA 92060-0200 The Big Eye The Newsletter of the Friends of Palomar Observatory Vol. 2, No. 1 Solar System Now Palomar’s Astronomical Has Eight Planets Bandwidth The International Astronomical Union (IAU) recently downgraded the status of Pluto to that of a “dwarf plan- For the past three years, astronomers at the et,” a designation that will also be applied to the spheri- California Institute of Technology’s Palomar Obser- cal body discovered last year by California Institute of vatory in Southern California have been using the Technology planetary scientist Mike Brown and his col- High Performance Wireless Research and Education leagues. The decision means that only the rocky worlds Network (HPWREN) as the data transfer cyberin- of the inner solar system and the gas giants of the outer frastructure to further our understanding of the uni- system will hereafter be designated as planets. verse. Recent applications include the study of some The ruling effectively settles a year-long controversy of the most cataclysmic explosions in the universe, about whether the spherical body announced last year and the hunt for extrasolar planets, and the discovery informally named “Xena” would rise to planetary status. of our solar system’s tenth planet. The data for all Somewhat larger than Pluto, the body has been informally this research is transferred via HPWREN from the known as Xena since the formal announcement of its remote mountain observatory to college campuses discovery on July 29, 2005, by Brown and his co-discov- hundreds of miles away. -
Hot Bird 2,3,4 & 5
HOT BIRD 2,3,4 & 5 - SuperBeam Page 1 of 1 http://www.eutelsat.org/satellitelhb2to5sb590.htm 5/16/2001 Lyngemark Satellite Chart: Hot Bird 1-5 at 13.0oEl18 CLICK HERE Asia Main I Europe I Europe ~I Europe., Headlines I Live I Free Atlantic 26.0o E <C> 1.0oW 16.0o E <Ku> 10.0o E Hot Bird 1-51 Hot Bird 1 I Hot Bird 2 I Hot Bird 31 Hot Bird 41 Hot Bird 5 Lyngemark Satellite Chart Hot Bird 1-5 at 13.oo E r- Hot Bird 1-5 © Lyngemark Satellite, last updated 2001-05-11 - http://www.lyngsat.com/hotbird.shtml hreq-j--'--IProvider Name Ivideo ~R - FEC INID - TID !source I IB I Tp I iChannel Name i IEnCryption SID - VPID !AudiO I earn Updated r~::~o ~DIGII~~;~~:rd I~J100 '~-id-e--;~-o-R{-~t-~~---i V it"7HiI] ICyfra + - 1318-11000'. I • I--I~~' !British Telecom ~ IMPEG-2 l~;:oo - )318-11100 r I r- I•~ I - r: i! 1201 E ' ,'EWTN Europe 4601i 100111301 Sp j ~ ! 1401G i KNewsLynx feeds) T--"-I [A602[1.OO211202 ICineNova ~~Ptoworks 1460311003 1203 Du 'I i 1204 orig 10723 H Cuccureddu I 1304 E /wide !G tp 111 I ~'" 1010417 IMTA Internatlona.I ,... '1' 4604!I 1004'115041404 GF I I 11604 A I i 1704 Ben IF~ (19~) ~ Sports Europe F,yptow"., rr.:=:.: ox ~ ~towo"" 46051005:~~ . r K;ds Russ;. (00'19) t I Deepam TV [.~ r--Iaccess 4606[1006[1206 Ta 110758 V I (IIJ TPsiAIDIG~rc~~~2 ~J~OO -111176-11200.