Programmes in Progress
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
Potential of Polarization/Raman Lidar to Separate Fine Dust, Coarse Dust
Atmos. Meas. Tech., 10, 3403–3427, 2017 https://doi.org/10.5194/amt-10-3403-2017 © Author(s) 2017. This work is distributed under the Creative Commons Attribution 3.0 License. Potential of polarization/Raman lidar to separate fine dust, coarse dust, maritime, and anthropogenic aerosol profiles Rodanthi-Elisavet Mamouri1,2 and Albert Ansmann3 1Cyprus University of Technology, Dep. of Civil Engineering and Geomatics, Limassol, Cyprus 2The Cyprus Institute, Energy, Environment, and Water Research Center, Nicosia, Cyprus 3Leibniz Institute for Tropospheric Research, Leipzig, Germany Correspondence to: Rodanthi-Elisavet Mamouri ([email protected]) Received: 26 April 2017 – Discussion started: 4 May 2017 Revised: 28 July 2017 – Accepted: 2 August 2017 – Published: 19 September 2017 Abstract. We applied the recently introduced polarization advantages in comparison to 355 and 1064 nm polarization lidar–photometer networking (POLIPHON) technique for lidar approaches and leads to the most robust and accurate the first time to triple-wavelength polarization lidar measure- POLIPHON products. ments at 355, 532, and 1064 nm. The lidar observations were performed at Barbados during the Saharan Aerosol Long- Range Transport and Aerosol-Cloud-Interaction Experiment (SALTRACE) in the summer of 2014. The POLIPHON 1 Introduction method comprises the traditional lidar technique to separate mineral dust and non-dust backscatter contributions and the Polarization lidar is a very powerful remote sensing tool for new, extended approach to separate even the fine and coarse aerosol and cloud research. The technique has been used for dust backscatter fractions. We show that the traditional and a long time to monitor and investigate cirrus cloud systems the advanced method are compatible and lead to a consis- (e.g., Sassen, 1991, 2005; Reichardt et al., 2002, 2008) and tent set of dust and non-dust profiles at simplified, less com- polar stratospheric cloud evolution (see, e.g., Browell et al., plex aerosol layering and mixing conditions as is the case 1990; Achtert and Tesche, 2014). -
Secretariat Distr.: General 25 November 2014
United Nations ST/SG/SER.E/733 Secretariat Distr.: General 25 November 2014 Original: English Committee on the Peaceful Uses of Outer Space Information furnished in conformity with the Convention on Registration of Objects Launched into Outer Space Letter dated 30 October 2014 from the Legal Services Department of the European Space Agency addressed to the Secretary-General In conformity with the Convention on Registration of Objects Launched into Outer Space (General Assembly resolution 3235 (XXIX), annex), the rights and obligations of which the European Space Agency (ESA) has declared its acceptance of, the Agency has the honour to transmit information on space objects Sentinel-1A and ATV-5, which were put into orbit within the past seven months (see annex). The Agency has the further honour to note that with effect from 28 October 2014, the date of signature of the Agreement between the European Union, Represented by the European Commission, and the European Space Agency on the Implementation of the Copernicus Programme, Including the Transfer of Ownership of Sentinels, the Agency has transferred the ownership of Sentinel-1A to the European Union. (Signed) Marco Ferrazzani ESA Legal Counsel and Head of the Legal Services Department V.14-07991 (E) 031214 041214 *1407991* ST/SG/SER.E/733 Annex Registration data on space objects launched by the European Space Agency* Sentinel-1A Information provided in conformity with the Convention on Registration of Objects Launched into Outer Space Committee on Space Research 2014-016A international -
Laser Retroreflectors for Insight and an International Mars Geophysical Network (MGN)
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 1492.pdf Laser Retroreflectors for InSight and an International Mars Geophysical Network (MGN). S. Dell’Agnello1, G.O. Delle Monache1, L. Porcelli1,2, M. Tibuzzi1, L. Salvatori1, C. Mondaini1, M. Muccino1, L. Ioppi1, O. Luongo1, M. Petrassi1, G. Bianco1,3, R. Vittori1,4, W.B. Banerdt5, J.F. Grinblat5, C. Benedetto3, F. Pasquali3, R. Mugnuolo3, D.C. Gruel5, J.L.Vago6 and P. Baglioni6. 1Istituto Nazionale di Fisica Nucleare–Laboratori Nazionali di Frascati (INFN–LNF), Via E. Fermi 40, 00044, Frascati, Italy ([email protected]); 2Dipartimento di Fisica, Università della Calabria (UniCal), Via P. Bucci, 87036, Arcavacata di Rende, Italy; 3Agenzia Spaziale Italiana– Centro di Geodesia Spaziale “Giuseppe Colombo” (ASI–CGS), Località, Terlecchia 75100, Matera, Italy; 4Italian Air Force, Rome, Italy, ASI and Embassy of Italy in Washington DC; 5NASA–Jet Propulsion Laboratory (JPL), California Institute of Technology, Pasadena, CA 91109, USA; 6ESA–ESTEC, Noordwijk, The Netherlands. Abstract. There are laser retroreflectors on the Moon, of the INFN-ASI Affiliation-Association to NASA- but there were no laser retroreflectors on Mars until the SSERVI sservi.nasa.gov) is shown in the figure below. NASA InSight mission [1][2] landed and started oper- ating successfully on the surface of the red planet on Nov. 26, 2018. The ESA ExoMars Schiaparelli mis- sion, which unfortunately failed Mars landing in 2016, was carrying a laser retroreflector like InSight [3]. These instruments are positioned by measuring the time-of-flight of short laser pulses, the so-called “laser ranging” technique (for details on satellite/lunar laser ranging and altimetry see https://ilrs.gsfc.nasa.gov). -
AMA 2009 UNE ANNÉE « BIG BANG » IYA09 - Behind the Big Bang
LE MAGAZINE D’INFORMATION DU CENTRE NATIONAL D’ÉTUDES SPATIALES cnescnesmag N° 41 04/2009 AMA 2009 UNE ANNÉE « BIG BANG » IYA09 - Behind the Big Bang L’oiseau et le satellite Birds under satellite scrutiny JEAN-MICHEL JARRE Un ambassadeur pour l’astronomie Astronomy’s ambassador sommaire ERATJ contents N°41 - 04/2009 06 04 / 15 news Smos, Des mesures disponibles à l’automne SMOS: data coming soon Soyouz, dernière ligne droite avant le lancement Soyuz in Guiana: first launch in sight 11 100 ans pour le salon du Bourget Paris Air Show centenary 16 / 29 politique Business & politics 16 Interview Fadela Amara, secrétaire d’État en charge de la Politique de la ville, à l’occasion du démarrage de l’opération « Espace dans ma ville » 2009. IInterview with Fadela Amara, Junior Minister for Urban Affairs, for the kick-off of Space in my City 2009. Séminaire de prospective Space science seminar Histoire d’espace: La France moteur de l’Europe spatiale Space History: France as Europe’s engine room in space 30 / 37 société Society L’oiseau et le satellite 30 Birds under satellite scrutiny Une expertise pour l’écotaxe poids lourds CNES expertise applied to truck eco-tax 38 / 59 dossier Special report 2009, une année « Big Bang » 2009 - Behind the Big Bang 60 / 68 Monde World États-Unis : la Nasa attend une nouvelle impulsion United States: NASA awaiting new momentum Europe : cap sur l’Espace européen de la recherche Europe: European Research Area in sight 69 / 75 culture Arts & living L’espace s’invite à La Nuit des musées Space in the spotlight on museum night Un espace dédié aux enseignants Dedicated site for teachers Des fusées expérimentales à Biscarosse Experimental rockets and more 60 CNESMAG journal trimestriel de communication externe du Centre national d’études spatiales.2 place Maurice-Quentin. -
The EXOD Search for Faint Transients in XMM-Newton Observations
UvA-DARE (Digital Academic Repository) The EXOD search for faint transients in XMM-Newton observations Method and discovery of four extragalactic Type I X-ray bursters Pastor-Marazuela, I.; Webb, N.A.; Wojtowicz, D.T.; van Leeuwen, J. DOI 10.1051/0004-6361/201936869 Publication date 2020 Document Version Final published version Published in Astronomy & Astrophysics Link to publication Citation for published version (APA): Pastor-Marazuela, I., Webb, N. A., Wojtowicz, D. T., & van Leeuwen, J. (2020). The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters. Astronomy & Astrophysics, 640, [A124]. https://doi.org/10.1051/0004-6361/201936869 General rights It is not permitted to download or to forward/distribute the text or part of it without the consent of the author(s) and/or copyright holder(s), other than for strictly personal, individual use, unless the work is under an open content license (like Creative Commons). Disclaimer/Complaints regulations If you believe that digital publication of certain material infringes any of your rights or (privacy) interests, please let the Library know, stating your reasons. In case of a legitimate complaint, the Library will make the material inaccessible and/or remove it from the website. Please Ask the Library: https://uba.uva.nl/en/contact, or a letter to: Library of the University of Amsterdam, Secretariat, Singel 425, 1012 WP Amsterdam, The Netherlands. You will be contacted as soon as possible. UvA-DARE is a service provided by the library of the University of Amsterdam (https://dare.uva.nl) Download date:02 Oct 2021 A&A 640, A124 (2020) Astronomy https://doi.org/10.1051/0004-6361/201936869 & c ESO 2020 Astrophysics The EXOD search for faint transients in XMM-Newton observations: Method and discovery of four extragalactic Type I X-ray bursters I. -
Church of the Brethren May Meet Hrre In
' ' , s i * Take inventory of your printed” sup One word can tell the Btory of con plies; If you need anything, the - tinued business activity in the com - j ■ ' Times stands ready to give munity—Advertising. vi:;/ you Bervice, • . AND THE SJIOUE TIMES FOUR CENTS /,-;t VOL. LX . No. 33 OCEAN GROVE, NEW JERSEY, FRIDAY, AUGUST 16, 1935 - / ' : $ THOMSON GETS ‘MARTHA" IS BIBLE LESSON HOTEL MEN WANT CHURCH 7,500 HEAR BISHOP MOUZON Mrs. Gertrude Brown To Teach At OF THE BRETHREN RARE SOUVENIRS St; Paul’s MORE PUBLICITY in Au ditoriu m sermons “Martha” is the Bible class les MAY MEET HRRE IN 1936 THREE ANNIVERSARY: MEMOS son for .the coming Sundny. Text, WILL REQUEST LARGER BUD “Jesus loved! Martha and her sister ARE PRESENTED and! Lazarus,” John,: 11:5: Read GET APPROPRIATION. Preacher Sees Chance For Uniting of Three Luke, 10\38-42 and John, VI '.17-28. National Convention Would Bring Eight Thou Sixth Founders’ Day, Stokes Gold Dr, Francis Harvey Green will be Appoint Nominating Committee Branches of Methodist Church—Prays For en Wedding and Dr. Ballard’s the teacher 'at the|. Auditorium For Report at September Meet sand Delegates for Eight Days—Dr. Hen Bible Class,, at" 2.30. .Written Ques Birthday Arc Noted In Special ing of Ocean Grove Hotel As Kingdom of God and Revival of Hope, tions will be answered at the begin son Offers Buildings for Sessions—Ar Announcements. ning of theperiod. sociation. Endorse Play-Ground Faith and Love— Gives His Definition of Three precious documents have The Assembly BiblejClhss, which D rive/ rangements Committee Decides Today. -
We Help Earth Benefit from Space in Summary 2019 Contents
WE HELP EARTH BENEFIT FROM SPACE IN SUMMARY 2019 CONTENTS About this report 2019 HIGHLIGHTS This is an English summary of Swedish 3 Space Corporation’s (SSC) 2019 Annual and Sustainability Report. CEO STATEMENT The Swedish report, available at our web- 4 site, is the legally binding annual report. THIS IS SSC The report summarizes the 2019 fiscal 6 year and covers performance on issues most important to SSC's ability to deliver SSC GLOBAL PRESENCE value to stakeholders in a changing and complex business environment. This 8 summary serves as our United Nations Global Compact (UNGC) Communi- EVOLVING SPACE LANDSCAPE 9 cations on Progress. Visit: STRATEGIC APPROACH https://www.sscspace.com/about-ssc/finances/reports-archive/ 10 Copyright: Unless otherwise indicated, SSC has the copyright to images in this publication. FOCUS AREAS FOR PROFITABLE SUSTAINABLE GROWTH 12 EMPLOYEES - OUR GREATEST ASSET 14 MEET OUR PEOPLE 15 2019 HIGHLIGHTS 2019 HIGHLIGHTS 2019 was another year of exciting space missions and projects for the space sector as a whole, but also for SSC. The rapid development has allowed us to grow and take new steps to prepare for the future. MASER 14 and inauguration of SubOrbital Express as a service Our MASER 14 sounding rocket reached an altitude of approximately 250 kilometers and spent over six minutes in microgravity. The mission inaugurated SubOrbital Express, a service to enable research into microgravity applications, atmospheric physics or other scientific disciplines. In this microgravity environment, we conducted experiments on fluid drainage, X-ray radio graphy and dust formation. Read more: https://www.suborbitalexpress.com Inauguration of exciting antenna art in Inuvik The two SSC antennas at the Inuvik site are painted by the local artists Anick Jenks and Ron English. -
Rapid Development of Navigation Payloads for Galileo Full Operational Capability
Changing the economics of space RAPID DEVELOPMENT OF NAVIGATION PAYLOADS FOR GALILEO FULL OPERATIONAL CAPABILITY Alex da Silva Curiel Dubai, January 2011 SSTL - the company UK-based satellite manufacturing company owned by EADS Astrium NV (99%) and the University of Surrey (1%) • Formed in 1985, the Company now employs >320 staff and occupies dedicated facilities in Surrey, Kent & Colorado 2 A history of success 34 Satellites completed – c.200 satellite years on-orbit experience 10 Further satellites (35-43) - currently being prepared for launch 18 payloads in progress (4 optical, 14 navigation) HERITAGE: Flight proven - low risk RESULTS: All projects fixed price, delivered on-time and on-budget SUCCESS: Very high mission success – 100% mission success in last 10 years – proven equipment and full redundancy CUSTOMERS: Variety of customers including many “blue chip” operators as well as 15 successful training programmes 3 What is Galileo? Galileo is a joint initiative of the European Commission (EC) and the European Space Agency (ESA). Galileo will be Europe’s own global navigation satellite system, providing a highly accurate, guaranteed global positioning service under civilian control. It will be inter-operable with GPS and GLONASS, the two other global satellite navigation systems 4 Galileo Services • Galileo offers 5 services: – Open signal, dual frequency, mass market use – Commercial signal, better accuracy, service guarantee – authenticated data – Safety-of-Life signal, high integrity service certified for use in safety related -
Highlights in Space 2010
International Astronautical Federation Committee on Space Research International Institute of Space Law 94 bis, Avenue de Suffren c/o CNES 94 bis, Avenue de Suffren UNITED NATIONS 75015 Paris, France 2 place Maurice Quentin 75015 Paris, France Tel: +33 1 45 67 42 60 Fax: +33 1 42 73 21 20 Tel. + 33 1 44 76 75 10 E-mail: : [email protected] E-mail: [email protected] Fax. + 33 1 44 76 74 37 URL: www.iislweb.com OFFICE FOR OUTER SPACE AFFAIRS URL: www.iafastro.com E-mail: [email protected] URL : http://cosparhq.cnes.fr Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law The United Nations Office for Outer Space Affairs is responsible for promoting international cooperation in the peaceful uses of outer space and assisting developing countries in using space science and technology. United Nations Office for Outer Space Affairs P. O. Box 500, 1400 Vienna, Austria Tel: (+43-1) 26060-4950 Fax: (+43-1) 26060-5830 E-mail: [email protected] URL: www.unoosa.org United Nations publication Printed in Austria USD 15 Sales No. E.11.I.3 ISBN 978-92-1-101236-1 ST/SPACE/57 *1180239* V.11-80239—January 2011—775 UNITED NATIONS OFFICE FOR OUTER SPACE AFFAIRS UNITED NATIONS OFFICE AT VIENNA Highlights in Space 2010 Prepared in cooperation with the International Astronautical Federation, the Committee on Space Research and the International Institute of Space Law Progress in space science, technology and applications, international cooperation and space law UNITED NATIONS New York, 2011 UniTEd NationS PUblication Sales no. -
Beyond the Paths of Heaven the Emergence of Space Power Thought
Beyond the Paths of Heaven The Emergence of Space Power Thought A Comprehensive Anthology of Space-Related Master’s Research Produced by the School of Advanced Airpower Studies Edited by Bruce M. DeBlois, Colonel, USAF Professor of Air and Space Technology Air University Press Maxwell Air Force Base, Alabama September 1999 Library of Congress Cataloging-in-Publication Data Beyond the paths of heaven : the emergence of space power thought : a comprehensive anthology of space-related master’s research / edited by Bruce M. DeBlois. p. cm. Includes bibliographical references and index. 1. Astronautics, Military. 2. Astronautics, Military—United States. 3. Space Warfare. 4. Air University (U.S.). Air Command and Staff College. School of Advanced Airpower Studies- -Dissertations. I. Deblois, Bruce M., 1957- UG1520.B48 1999 99-35729 358’ .8—dc21 CIP ISBN 1-58566-067-1 Disclaimer Opinions, conclusions, and recommendations expressed or implied within are solely those of the authors and do not necessarily represent the views of Air University, the United States Air Force, the Department of Defense, or any other US government agency. Cleared for public release: distribution unlimited. ii Contents Chapter Page DISCLAIMER . ii OVERVIEW . ix PART I Space Organization, Doctrine, and Architecture 1 An Aerospace Strategy for an Aerospace Nation . 3 Stephen E. Wright 2 After the Gulf War: Balancing Space Power’s Development . 63 Frank Gallegos 3 Blueprints for the Future: Comparing National Security Space Architectures . 103 Christian C. Daehnick PART II Sanctuary/Survivability Perspectives 4 Safe Heavens: Military Strategy and Space Sanctuary . 185 David W. Ziegler PART III Space Control Perspectives 5 Counterspace Operations for Information Dominance . -
Sentinel-2 and Sentinel-3 Mission Overview and Status
Sentinel-2 and Sentinel-3 Mission Overview and Status Craig Donlon – Sentinel-3 Mission Scientist and Ferran Gascon – Sentinel-2 QC manager and others @ESA IOCCG-21, Santa Monica, USA 1-3rd March 2016 Overview – What is Copernicus? – Sentinel-2 mission and status – Sentinel-3 mission and status Sentinel-3A OLCI first light Svalbard: 29 Feb 14:07:45-14:09:45 UTC Bands 4, 6 and 7 (of 21) at 490, 560, 620 nm Spain and Gibraltar 1 March 10:32:48-10:34:48 UTC California USA 29 Feb 17:44:54-17:46:54 UTC What is Copernicus? Space Component In-Situ Services A European Data Component response to global needs 6 What is Copernicus? – Space in Action for You! • A source of information for policymakers, industry, scientists, business and the public • A European response to global issues: • manage the environment; • understand and to mitigate the effects of climate change; • ensure civil security • A user-driven programme of services for environment and security • An integrated Earth Observation system (combining space-based and in-situ data with Earth System Models) Components & Competences Coordinators: Partners: Private Space Industries companies Component National Space Agencies Overall Programme EMCWF EMSA Mercator snd Ocean Coordination FRONTEX Service Services operators Component EUSC EEA JRC In-situ data are supporting the Space and Services Components Copernicus Funding Funding for Development Funding for Operational Phase until 2013 (c.e.c.): Phase as from 2014 (c.e.c.): ~€ 3.7 B (from ESA and € 4.3 B for the EU) whole programme (from EU) -
Update on PROBA-2 TDM and ALPHASAT TDP8 Flight Data
Update on PROBA-2 TDM and ALPHASAT TDP8 Flight Data Christian POIVEY, Gerard PLANES CONANGLA, Marco d’ALESSIO, Reno HARBOE-SORENSEN ESA ESTEC CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 OUTLINE 1. PROBA-2 TDM 2. Summary of PROBA-2 TDM SEE flight data on memories 3. ALPHASAT TDP8 4. Summary of ALPHASAT TDP8 SEE flight data on memories CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 PROBA-2 Launched on November 2, 2009 LEO orbit: 713-733 km, 98 degrees inclination PROBA-2 - TDM 1. TDM : Memories on board TDM/Proba II a. TID (RADFETs) Atmel AT68166 (4*AT60142) 2M x 8 b. Reference SEU monitor Alliance AS7C34096A-12TI 512K x 8 c. SEL experiment Semi. – SEL Samsung K6R4008V1D 512K x 8 – SEU ISSI IS61LV5128AL-12 512K x 8 d. Flash memory experiment. 2. Period analyzed ISSI IS62WV20488BLL 2M x8 a. March 2010-January 2015 Samsung K9FG08U0M 1G x 8 – (1769 days) CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 PROBA-2 TDM CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 SEL experiment, SEL Data SEL experiment in TDM/Proba-2 Tot SAA Alliance Semi. AS7C34096A-12TI 512K x 8 3 2 Samsung K6R4008V1D-TI10 512K x 8 8 4 ISSI IS61LV5128AL-12 512K x 8 357 293 ISSI IS62WV20488BLL 2M x8 12 5 CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 SEL experiment, SEL Data IS61LV5128AL Differential latchup rate (smoothed in blue) CNES ESA Radiation Effects Final Presentations Days March 9&10, 2015 SEL experiment, SEL Data Comparison with Calculated Rates SEL rate prediction was performed for the 4 SRAMs using OMERE under solar maximum conditions, a sensitive volume thickness of 1 micron and 10 mm of Aluminum shielding.