Spacewire Datasheet
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Spacewire Links Routers and Networks ECSS-E50-12A
SpaceWire Links Routers and Networks ECSS-E50-12A Presented by Ph. Armbruster ESA/ESTEC/TOS-ED Data Systems Division [email protected] Credit – University of Dundee - European Space Agency Contents Part 1 Contents Part 2 § Introduction § SpaceWire Packets § Physical Level § Routing Switch Concepts § Signal Level – Worm-hole routing § Character Level – Header deletion – Path addressing § Exchange Level – Logical addressing § Packet Level – Priority – Arbitration – Group adaptive routing – Fault tolerance § Networks § Time Codes SpaceWire § SpaceWire is a standard for spacecraft onboard data-handling – ESA ECSS-E-50-12A § SpaceWire based on two commercial standards – IEEE-1355 – LVDS (Low Voltage Differential Signalling) § SpaceWire is the result of work by many people in ESA, NASA, the space industry and academia. SpaceWire Key Features § High data rate ( > 100 Mbps) § Distance of 10m + § Scalable § Low error rate § Good EMC performance § Low-power § Fault tolerance support § Radiation tolerant components Purpose § SpaceWire provides a unified high-speed data- handling infrastructure for connecting together – sensors, – processing elements, – mass-memory units, – downlink telemetry sub-systems, and – EGSE equipment. Purpose § The purpose of the SpaceWire standard is – to facilitate the construction of high-performance onboard data-handling systems – to help reduce system integration costs – to promote compatibility between data-handling equipment and sub-systems – to encourage re-use of data handling equipment across several different missions. Scope § SpaceWire links are – full-duplex, point-to-point, serial data communication links. § The scope of the SpaceWire standard is the – physical connectors and cables, – electrical properties, and – logical protocols. Scope § The SpaceWire standard covers the following normative protocol levels – Physical Level: Connectors, cables, cable assemblies and PCB tracks – Signal Level: Signal encoding, voltage levels, noise margins, and data rates. -
Bepicolombo - a Mission to Mercury
BEPICOLOMBO - A MISSION TO MERCURY ∗ R. Jehn , J. Schoenmaekers, D. Garc´ıa and P. Ferri European Space Operations Centre, ESA/ESOC, Darmstadt, Germany ABSTRACT BepiColombo is a cornerstone mission of the ESA Science Programme, to be launched towards Mercury in July 2014. After a journey of nearly 6 years two probes, the Magneto- spheric Orbiter (JAXA) and the Planetary Orbiter (ESA) will be separated and injected into their target orbits. The interplanetary trajectory includes flybys at the Earth, Venus (twice) and Mercury (four times), as well as several thrust arcs provided by the solar electric propulsion module. At the end of the transfer a gravitational capture at the weak stability boundary is performed exploiting the Sun gravity. In case of a failure of the orbit insertion burn, the spacecraft will stay for a few revolutions in the weakly captured orbit. The arrival conditions are chosen such that backup orbit insertion manoeuvres can be performed one, four or five orbits later with trajectory correction manoeuvres of less than 15 m/s to compensate the Sun perturbations. Only in case that no manoeuvre can be performed within 64 days (5 orbits) after the nominal orbit insertion the spacecraft will leave Mercury and the mission will be lost. The baseline trajectory has been designed taking into account all operational constraints: 90-day commissioning phase without any thrust; 30-day coast arcs before each flyby (to allow for precise navigation); 7-day coast arcs after each flyby; 60-day coast arc before orbit insertion; Solar aspect angle constraints and minimum flyby altitudes (300 km at Earth and Venus, 200 km at Mercury). -
ESA & ESOC Overview
NASA PM Challenge 2010 Developing the International Program/Project Management Community 9/10 February 2010 Dr. Bettina Böhm Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 1 Used with Permission PURPOSE OF ESA / ACTIVITIES “To provide for and promote, for exclusively Space science peaceful purposes, cooperation among Human spaceflight European states in space research and Exploration technology and their space applications.” Earth observation Launchers [Article 2 of ESA Convention] Navigation ESA is one of the few space agencies Telecommunications in the world to combine responsibility Technology in all areas of space activity. Operations Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 2 ESA FACTS AND FIGURES Over 30 years of experience 18 Member States 2080 staff, thereof 880 in Program Directorates, 790 in Operations and Technical Support and 410 in other Support Directorates 3 500 million Euros budget Over 60 satellites designed and tested Over 60 satellites operated in-flight and 8 missions rescued 16 scientific satellites in operation Five types of launcher developed More than 180 launches made Program & Project Manager Career at ESA | Bettina Böhm | ESA/HQ | 23/11/09 | Page 3 ESA Locations EAC (Cologne) Salmijaervi ESTEC Astronaut training (Noordwijk) Satellite technology development and testing Harwell ESOC ESA HQ (Darmstadt) (Paris) Brussels Satellite operations and ground system technology development ESAC (Villanueva de la Cañada Oberpfaffenhofen -
Spacewire Protocol ID: What Does It Means to You?
Spacewire Protocol ID: What Does It Means To You? Glenn Rakow Richard Schnurr Daniel Gilley Steve Parkes NASA GSFC NASA GSFC Lockheed Martin University of Dundee Code 561 Code 561 Greenbelt, MD Greenbelt, MD Sunnyvale, CA Dundee, Scotland, UK 301-286-5993 301-2864 852 00441382345194 [email protected] [email protected] daniel.nilley6dlmco.com sparkes@,computing.dundee.ac.uk Abstract- Spacewire is becoming a popular solution for standard but with one restriction. The restriction is that the satellite high-speed data buses because it is a simple first byte seen at the destination by the user needs to be a standard that provides great flexibility for a wide range of logical address, independent of the addressing scheme used. system requirements. It is simple in packet format and The second field is defined as the Protocol ID, which is protocol, allowing users to easily tailor their implementation usually one byte in length. The packet cargo (user defined) for their specific application. Some of the attractive aspects follows the Protocol ID. After the packet cargo is the EOP, of Spacewire that make it easy to implement also make it which defines the end of packet. The value of the Protocol hard for future reuse. Protocol reuse is difticult because ID is assigned by the Spacewire working group and the Spacewire does not have a defined mechanism to protocol description published for others to use. communicate with the higher layers of the protocol stack. This has forced users of Spacewire to define unique packet The development of Protocols for Spacewire is currently formats and define how these packets are to be processed. -
Annu Al R Ep Or T 2016–2017
ANNUAL REPORT 2016–2017 ANNUAL Goddard Earth Sciences Technology and Research Studies and Investigations GESTAR Staff Hanson, Heather Miller, Kevin Wen, Guoyong Achuthavarier, Deepthi Holdaway, Dan Mohammed, Priscilla Wiessinger, Scott Ahamed, Aakash Humberson, Winnie Monroe, Brian Wright, Ernie Amatya, Pukar Hurwitz, Margaret Moran, Amy Yang, Weidong Andrew, Andrea Ibrahim, Amir Ng, Joy Yang, Yuekui Anyamba, Assaf Jackson, Katrina Norris, Peter Yao, Tian Aquila, Valentina Jentoft-Nilsen, Marit Nowottnick, Ed Zhang, Cheng Armstrong, Amanda Jepsen, Rikke Oda, Tom Zhang, Qingyuan Arnold, Nathan Jethva, Hiren Olsen, Mark Zhou, Yaping Barker, Ryan Jin, Daeho Orbe, Clara Ziemke, Jerald Beck, Jefferson Jin, Jianjun Patadia, Falguni Bell, Benita Ju, Junchang Patel, Kiran GESTAR Integrated Belvedere, Debbie Keating, Shane Paynter, Ian Project Team (IPT) Bensusen, Sally Kekesi, Alex Pelc, Joanna Ball, Carol Bollian, Tobias Keller, Christoph Peng, Jinzheng Corso, Bill Bridgman, Tom Khan, Maudood Poje, Lisa Espiritu, Angie Brucker, Ludovic Kim, Dongchul Potter, Gerald Gardner, Jeanette Buchard, Virginie Kim, Dongjae Prescott, Ishon Houghton, Amy Carvalho, David Kim, Hyokyung Prive, Nikki Morgan, Dagmar Radcliff, Matthew Samuel, Elamae ACKNOWLEDGEMENTS Castellanos, Patricia Kim, Min-Jeong Cede, Alexander Knowland, Emma Reale, Oreste Celarier, Ed Kolassa, Jana Rousseaux, Cecile Technical Editor Cetinic, Ivona Korkin, Sergey Sayer, Andy Amy Houghton Chang, Yehui Kostis, Helen-Nicole Schiffer, Robert Chatterjee, Abhishek Kowalewski, Matthew Schindler, -
Securing Japan an Assessment of Japan´S Strategy for Space
Full Report Securing Japan An assessment of Japan´s strategy for space Report: Title: “ESPI Report 74 - Securing Japan - Full Report” Published: July 2020 ISSN: 2218-0931 (print) • 2076-6688 (online) Editor and publisher: European Space Policy Institute (ESPI) Schwarzenbergplatz 6 • 1030 Vienna • Austria Phone: +43 1 718 11 18 -0 E-Mail: [email protected] Website: www.espi.or.at Rights reserved - No part of this report may be reproduced or transmitted in any form or for any purpose without permission from ESPI. Citations and extracts to be published by other means are subject to mentioning “ESPI Report 74 - Securing Japan - Full Report, July 2020. All rights reserved” and sample transmission to ESPI before publishing. ESPI is not responsible for any losses, injury or damage caused to any person or property (including under contract, by negligence, product liability or otherwise) whether they may be direct or indirect, special, incidental or consequential, resulting from the information contained in this publication. Design: copylot.at Cover page picture credit: European Space Agency (ESA) TABLE OF CONTENT 1 INTRODUCTION ............................................................................................................................. 1 1.1 Background and rationales ............................................................................................................. 1 1.2 Objectives of the Study ................................................................................................................... 2 1.3 Methodology -
For Sanibel & Captiva
COMMENTARY: RECREATION: ARTS: Sunny, Chelle surveys Terry ventures BIG Arts Craft with some Fort Myers into Octopus's Show features rain 2A Beach...6A garden... 11B fine gifts... 5B 1961-1988 Still first on Sanibel and Captiva VOL. 27, NO. 46 TUESDAY, NOVEMBER 22, 1988 TWO SECTIONS, 64 PAGES 50 CENTS Lorenson becomes mayor fev- Valtin and Klein honored By Barbara Brundage Islander staff writer Councilman Lennart Lorenson's first official act as Sanibel's new mayor was to present plaques to the two outgoing councilmen recognizing their years of ser- vice to the city. Last Tuesday councilmen Mike Klein and Fred Valtin stepped down after completing two terms (eight years) on the council. Both had served as mayor - Valtin three times in 1984,1985 and 1987. Klein, just finishing up his second stint as His Honor, served the first time in 1983. Valtin, who is still convalescing from a heart attack sufferd last June, said he was deeply touched by the honor but he was "confident the city is in good hands." Klein said he was not saying "Goodbye but only So Long." Please see LORENSON, page 26A A Photo by JUDY CORRIGAN Erika Moreira, 13, a Lee County Humane pelican named Seymour. Proceeds from the Society Youth Corps volunteer, with Scruffy, two-day event will benefit Care and Rehabilita- one of the Society's hundreds of dogs and cats tion of Wildlife, Protection of Animals Welfare up for adoption. This weekend's Thanks To The Society and the Humane Society of Lee County f * Animals fundraiser at Periwinkle Place in their efforts to help wild and domestic featured several dogs, cats, raccoons and a animals. -
The Atmospheric Remote-Sensing Infrared Exoplanet Large-Survey
ariel The Atmospheric Remote-Sensing Infrared Exoplanet Large-survey Towards an H-R Diagram for Planets A Candidate for the ESA M4 Mission TABLE OF CONTENTS 1 Executive Summary ....................................................................................................... 1 2 Science Case ................................................................................................................ 3 2.1 The ARIEL Mission as Part of Cosmic Vision .................................................................... 3 2.1.1 Background: highlights & limits of current knowledge of planets ....................................... 3 2.1.2 The way forward: the chemical composition of a large sample of planets .............................. 4 2.1.3 Current observations of exo-atmospheres: strengths & pitfalls .......................................... 4 2.1.4 The way forward: ARIEL ....................................................................................... 5 2.2 Key Science Questions Addressed by Ariel ....................................................................... 6 2.3 Key Q&A about Ariel ................................................................................................. 6 2.4 Assumptions Needed to Achieve the Science Objectives ..................................................... 10 2.4.1 How do we observe exo-atmospheres? ..................................................................... 10 2.4.2 Targets available for ARIEL .................................................................................. -
Bulletin 132 - November 2007 Node-2 Aloft
B132cover2 11/23/07 11:39 AM Page 1 www.esa.int number 132 - november 2007 Member States Etats membres Austria Allemagne Belgium Autriche Denmark Belgique Finland Danemark France Espagne Germany Finlande Greece France Ireland Grèce Italy Irlande Luxembourg Italie Netherlands Luxembourg Norway Norvège Portugal Pays-Bas SPACE FOR EUROPE Spain Portugal Sweden Royaume-Uni Switzerland Suède United Kingdom Suisse ESA bulletin 132 - november 2007 Node-2 Aloft ESA Communications ESTEC, PO Box 299, 2200 AG Noordwijk, The Netherlands Columbus Next Tel: +31 71 565-3408 Fax: +31 71 565-5433 Visit Publications at http://www.esa.int IFCb132 11/21/07 9:56 AM Page 2 european space agency Editorial/Circulation Office ESA Communications ESTEC, PO Box 299, The European Space Agency was formed out of, and took over the rights and obligations of, the two earlier European space organisations – the 2200 AG Noordwijk European Space Research Organisation (ESRO) and the European Organisation for the Development and Construction of Space Vehicle Launchers The Netherlands (ELDO). The Member States are Austria, Belgium, Denmark, Finland, France, Germany, Greece, Ireland, Italy, Luxembourg, the Netherlands, Norway, Tel: +31 71 565-3408 Portugal, Spain, Sweden, Switzerland and the United Kingdom. Canada is a Cooperating State. Editors Andrew Wilson In the words of its Convention: the purpose of the Agency shall be to provide for and to promote for exclusively peaceful purposes, cooperation among Carl Walker European States in space research and technology and their -
Space Wales Brochure Directory Capability Matrix (Lowres)
WALES A SUSTAINABLE SPACE NATION BROCHURE, DIRECTORY & CAPABILITY MATRIX SPACE WALES Wales - A Sustainable Space Nation 03 Space Wales Leadership Group 08 WASP & Academia 10 Research Centres & Catapults 11 RPAS and T&E in Wales 12 Capability Matrix 14 Company Directory 18 02 SPACE WALES WALES A SUSTAINABLE SPACE NATION Wales, with a population of 3 million people, totals around 5% of the UK populace. In the aerospace sector Wales has around 10% of the overall UK workforce and arguably punches above its weight. When it comes to the space sector Wales has only around 1% of the overall UK personnel and so there is a huge opportunity for growth in a sector which is growing significantly. The UK space sector has set a target of achieving a 10% share of the predicted £400 billion per annum global space market in 2030. A 5% share of this for Wales would equate to £2 billion per year and this is a realisable target which we aim to achieve and will work to exceed. Currently there are around 5000 satellites circling the earth in various orbits. Only 2,000 of these are operational. If OneWeb, Starlink and other potential networks continue with their projected growth that number could increase by a massive 4,500% in the next five years! Demand for data is on the increase, and launching satellites that offer broadband internet service will help to drive down the cost of that data. Reusable rockets and satellites will also help drive down costs and so too will the mass-production of satellites and the development of satellite technology. -
Japan's Asteroid Missions Hayabusa and Hayabusa2
Japan's Asteroid Missions Hayabusa and Hayabusa2 COPUOS 2013 February 15, 2013, Vienna, Austria Makoto Yoshikawa Hayabusa & Hayabusa2 Project Team, JAXA Lunar and Planetary Missions of Japan ×LUNAR- Hiten A ×Nozom Moon IKAROS 1985 i Moon Sakigake Kaguya 1990 Mars △Akatsuki 1998 Moon Suisei 2003 Hayabusa Venus 2007 BepiColombo 2010 2014 Comet Halley Asteroid Itokawa Hayabusa2 Mercury Asteroid 1999 JU3 February 15, 2013 COPUOS 2013 2 Challenges of Hayabusa and Hayabusa2 Development of the technology for asteroid sample return •Ion engine •Autonomous navigation •Sample collection system •Reentry capsule Impactor system * Study of the origin and evolution of the solar system Molecular cloud Proto solar system disk Solar system Evolution of planets Minerals, H 2O *, Organic matters * (*Hayabusa2) February 15, 2013 COPUOS 2013 3 History of Hayabusa and Hayabusa2 Idea for sample Serious troubles return began in1985 in Hayabusa Now Year 200 01 02 03 04 05 06 07 08 09 10 11 12 13 14 15 0 Sample MUSES-C Hayabusa Analysis ▲ ▲ launch Earth return project Started Hayabusa Mk2 in 1996 Post MUSES-C Post Hayabusa Post Marco Polo Haybusa2 Launch Hyabusa2 Phase-B ▲ Initial proposal in 2006 New proposal in 2009 Copy of Hayabusa but modified Modified Hayabusa adding new challenges Target : C-type asteroid 1999 JU3 Target : C-type asteroid 1999 JU3 Launch: 2010 Launch: 2014 February 15, 2013 COPUOS 2013 4 Starting point of Hayabusa Small Meeting for Asteroid Sample Return Mission ISAS June 29, 1985 Cover of meeting February 15, 2013 COPUOS 2013 5 Mission Scenario of Hayabusa Observations, sampling Earth Swingby Launch 19 May 2004 9 May 2003 Asteroid Arrival 12 Sept. -
Bepicolombo Quick-Look Analysis Interface Status
EPSC Abstracts Vol. 13, EPSC-DPS2019-921-1, 2019 EPSC-DPS Joint Meeting 2019 c Author(s) 2019. CC Attribution 4.0 license. BepiColombo Quick-Look Analysis interface status Thomas Cornet (1), Mark S. Bentley (2), Alan Macfarlane (3), Santa Martínez (4) and the BepiColombo SGS Team. (1) Aurora Technology BV for ESA, (2) HE Space for ESA, (3) Serco Nederland BV for ESA, (4) ESA/ESAC, Villanueva de la Cañada, Madrid, Spain. ([email protected]) Abstract by allowing them to share information in a centralised place. The ESA/JAXA BepiColombo mission to Mercury [1] was launched on the October 20th, 2018. During 2. Development and status its seven years Cruise phase, BepiColombo will perform several flybys of the Earth, Venus and The QLA is the end part of the BepiColombo Science Mercury before its insertion into orbit and start of Operation Control System (BSCS) [2] architecture. science phase at the beginning of 2026. In the harsh The BSCS includes several subsystems retrieving hermean environment, the mission various and processing the spacecraft and instruments instruments will allow studying Mercury as a whole telemetry. Science data are stored according to PDS4 system where the interior, surface and space weather standards in the Planetary Science Archive (PSA) [3]. science will be inter-connected. In this context, the The SGS is responsible of the first step of data ESA Science Ground Segment (SGS) aims at conversion from telemetry to raw data. The providing a support tool for data visualisation and subsequent data levels (partially processed, calibrated) analysis, suited to the specific needs of each are in vast majority produced by the ITs and then instrument team, and facilitating scientific delivered to the SGS.