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China's Touch on the Moon
commentary China’s touch on the Moon Long Xiao As well as being a milestone in technology, the Chang’e lunar exploration programme establishes China as a contributor to space science. With much still to learn about the Moon, fieldwork beyond Earth’s orbit must be an international effort. hen China’s Chang’e 3 spacecraft geological history of the landing site. touched down on the lunar High-resolution images have shown rocky Wsurface on 14 December 2013, terrain with outcrops of porphyritic basalt, it was the first soft landing on the Moon such as Loong Rock (Fig. 2). Analysis since the Soviet Union’s Luna 24 mission of data collected by the penetrating in 1976. Following on from the decades- Chang’e 3 radar should lead to identification of the old triumphs of the Luna missions and underlying layers of regolith, impact breccia NASA’s Apollo programme, the Chang’e and basalt. lunar exploration programme is leading the China’s robotic field geologist Yutu has charge of a new generation of exploration Basalt outcrop Yutu rover stalled in its traverse of the lunar surface, on the lunar surface. Much like the earlier but plans for the Chang’e 5 sample-return space programmes, the China National mission are moving forward. The primary Space Administration (CNSA) has been objective of the mission will be to return developing its capabilities and technologies 100 m 2 kg of samples from the surface and depths step by step in a series of Chang’e missions UNIVERSITY STATE © NASA/GSFC/ARIZONA of up to 2 m, probably also in the relatively of increasing ambition: orbiting and Figure 1 | The Chinese Chang’e 3 spacecraft and smooth northern Mare Imbrium. -
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). -
Planetary Science Division Status Report
Planetary Science Division Status Report Jim Green NASA, Planetary Science Division January 26, 2017 Astronomy and Astrophysics Advisory CommiBee Outline • Planetary Science ObjecFves • Missions and Events Overview • Flight Programs: – Discovery – New FronFers – Mars Programs – Outer Planets • Planetary Defense AcFviFes • R&A Overview • Educaon and Outreach AcFviFes • PSD Budget Overview New Horizons exploresPlanetary Science Pluto and the Kuiper Belt Ascertain the content, origin, and evoluFon of the Solar System and the potenFal for life elsewhere! 01/08/2016 As the highest resolution images continue to beam back from New Horizons, the mission is onto exploring Kuiper Belt Objects with the Long Range Reconnaissance Imager (LORRI) camera from unique viewing angles not visible from Earth. New Horizons is also beginning maneuvers to be able to swing close by a Kuiper Belt Object in the next year. Giant IcebergsObjecve 1.5.1 (water blocks) floatingObjecve 1.5.2 in glaciers of Objecve 1.5.3 Objecve 1.5.4 Objecve 1.5.5 hydrogen, mDemonstrate ethane, and other frozenDemonstrate progress gasses on the Demonstrate Sublimation pitsDemonstrate from the surface ofDemonstrate progress Pluto, potentially surface of Pluto.progress in in exploring and progress in showing a geologicallyprogress in improving active surface.in idenFfying and advancing the observing the objects exploring and understanding of the characterizing objects The Newunderstanding of Horizons missionin the Solar System to and the finding locaons origin and evoluFon in the Solar System explorationhow the chemical of Pluto wereunderstand how they voted the where life could of life on Earth to that pose threats to and physical formed and evolve have existed or guide the search for Earth or offer People’sprocesses in the Choice for Breakthrough of thecould exist today life elsewhere resources for human Year forSolar System 2015 by Science Magazine as exploraon operate, interact well as theand evolve top story of 2015 by Discover Magazine. -
Satellite Situation Report
NASA Office of Public Affairs Satellite Situation Report VOLUME 17 NUMBER 6 DECEMBER 31, 1977 (NASA-TM-793t5) SATELLITE SITUATION~ BEPORT, N8-17131 VOLUME 17, NO. 6 (NASA) 114 F HC A06/mF A01 CSCL 05B Unclas G3/15 05059 Goddard Space Flight Center Greenbelt, Maryland NOTICE .THIS DOCUMENT HAS'BEEN REPRODUCED FROM THE BEST COPY FURNISHED US BY THE SPONSORING AGENCY. ALTHOUGH IT IS RECOGNIZED THAT CERTAIN PORTIONS' ARE ILLEGIBLE, IT IS BEING RELEASED IN THE INTEREST OF MAKING AVAILABLE AS MUCH INFORMATION AS POSSIBLE. OFFICE OF PUBLIC AFFAIRS GCDDARD SPACE FLIGHT CENTER NATIONAL AERONAUTICS AND SPACE ADMINISTRATION VOLUME 17 NO. 6 DECEMBER 31, 1977 SATELLITE SITUATION REPORT THIS REPORT IS PUBLIShED AND DISTRIBUTED BY THE OFFICE OF PUBLIC AFFAIRS, GSFC. GODPH DRgP2 FE I T ERETAO5MUJS E SMITHSONIAN ASTRCPHYSICAL OBSERVATORY. SPACEFLIGHT TRACKING AND DATA NETWORK. NOTE: The Satellite Situation Report dated October 31, 1977, contained an entry in the "Objects Decayed Within the Reporting Period" that 1977 042P, object number 10349, decayed on September 21, 1977. That entry was in error. The object is still in orbit. SPACE OBJECTS BOX SCORE OBJECTS IN ORBIT DECAYED OBJECTS AUSTRALIA I I CANACA 8 0 ESA 4 0 ESRO 1 9 FRANCE 54 26 FRANCE/FRG 2 0 FRG 9 3 INCIA 1 0 INDONESIA 2 0 INTERNATIONAL TELECOM- MUNICATIONS SATELLITE ORGANIZATION (ITSO) 22 0 ITALY 1 4 JAPAN 27 0 NATC 4 0 NETHERLANDS 0 4 PRC 6 14 SPAIN 1 0 UK 11 4 US 2928 1523 USSR 1439 4456 TOTAL 4E21 6044 INTER- CBJECTS IN ORIT NATIONAL CATALOG PERIOD INCLI- APOGEE PERIGEE TQANSMITTTNG DESIGNATION NAME NUMBER SOURCE LAUNCH MINUTES NATION KM. -
Venona Special Studies
- 1 - Venona Project Special Studies Transcribed by Students of the Mercyhurst College Institute for Intelligence Studies Arranged by John Earl Haynes, Library of Congress, 2010 COVER NAMES IN NEW YORK TRAFFIC p. 2 UNIDENTIFIED COVER NAMES IN NEW YORK TRAFFIC p. 86 COVER NAMES IN SAN FRANCISCO TRAFFIC p. 92 COVER NAMES IN WASHINGTON TRAFFIC p. 123 ADDITIONAL COVERNAMES AND RELATED INFORMATION IN DIPLOMATIC TRAFFIC p. 127 REVISED TRANSLATION OF MESSAGE ON ANTENNA-LIBERAL'S WIFE ETHEL p. 135 THE COVERNAMES "ANTENNA" AND "LIBERAL" IN . MESSAGES p. 139 ESSAGES IN . INVOLVING THE COVERNAME"ENORMOZ" AND THE NAMES OF NUCLEAR PHYSICISTS, ETC. p. 147 UNDATED REPORT OF MEREDITH GARDNER p. 155 DEVELOPMENT OF THE “G--“HOMER” [“GOMER”] CASE p. 158 THE KOMAR (KRAVCHENKO) AFFAIR IN . MESSAGES p. 161 REVISED TRANSLATION OF TWO . MESSAGES ON CHANGES IN COVERNAMES p. 170 THE COVERNAME "KARAS" IN. TRAFFIC p. 178 THE COVERNAMES "TÉNOR", "BAS", AND "CHETÁ" (? IN . TRAFFIC p. 181 - 2 - Special Study Cover Names in New York Traffic - 3 - cover-name Message number Date Publication reference S/ or 3/NBF/ 19 N.Y. to M. 812 29053 JKI 06 T1022 1B-1910 0027A ABRAM N.Y. to M. 992 24063 JKR 14 T872√ 1B-7518 0005A JACK SOBLE 1086 06073 JKV 48 T873√ 2A-0011 1957 29113 NNNNNN T939√ 625 04054 JHD 48 T916√ 851 15064 JIJ 40 T10.1√ 1146 10084 JHM 41 T123√ 1251 02094 JHN 12 T301√ (to ChEKh) 0005B 1353 23094 JHO 42 T289√ 1449 12104 JIL 37 T106√ 1754 14124 JHZ 49 T6√ 48 11015 JHV 37 (NSA)T1941 AVGUR 2A-0013 1638 (AUGUR) N.Y. -
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. -
The Hera Mission
Dr. Patrick Michel Hera Investigation Team PI Université Côte d’Azur Observatoire de la Côte d’Azur CNRS, Lagrange Laboratory Nice, France The Hera Mission ESA UNCLASSIFIED - For Official Use Hera main aspects Role of space missions at ESA in NEO hazard mitigation • Understanding the problem (deflection modeling and simulations) 2001 • Ground versus space solutions analyses • Assessment of space component options 2002- • 6 parallel phase-0 studies (3 space telescopes, 3 rendezvous) Euneos Nero Earthguard 1 2004 • ESA’s NEO Mission Advisory Panel (NEOMAP) established • Kinetic impactor validation ranked highest importance 2004- • Don Quijote mission selected and studied up to phase-A level 2006 • SANCHO / Proba-IP orbiter up to phase A level studies, small deep-space Don Quijote Ishtar Simone 2008- mission to investigate impactor’s result 2009 • AIDA proposed by NASA: USA/impactor + ESA/impact assessment • ESA phase 0 and phase A studies on the observer spacecraft "AIM” (GSP) 2011- Proba-IP 2016 • Phase B1 study and “consolidation phase” for mission definition (GSTP) • HERA: impact observer spacecraft reformulation and optimization AIM 2017- • Phase B1 implementation + payload + technology breadboards (GSTP+SSA) Several concepts 2019 • DART phase-C kick-off on 15 May 2018 Hera iterated AIDA: An International Planetary Defense Mission U.S. National Research Council Committee “Defending Planet Earth: Near-Earth Object Surveys and Hazard Mitigation Strategies” Recommendation: “If [U.S.] Congress chooses to fund mitigation research at an appropriately high level, the first priority for a space mission in the mitigation area is an experimental test of a kinetic impactor along with a characterization, monitoring, and verification system, such as the Don Quixote mission that was previously considered, but not funded, by the European Space Agency. -
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. -
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) -
Thermal Design, Analysis and Test Validation of Turksat-3Usat Satellite
Journal of Thermal Engineering, Vol. 7, No. 3, pp. 468-482, March, 2021 Yildiz Technical University Press, Istanbul, Turkey THERMAL DESIGN, ANALYSIS AND TEST VALIDATION OF TURKSAT-3USAT SATELLITE Murat Bulut1,*, Nedim Sözbir2 ABSTRACT When CubeSat projects are a useful means by which universities can engage their students in space-related activities. TURKSAT-3USAT is a three-unit amateur radio CubeSat jointly developed by the Space Systems Design and Test Laboratory and the Radio Frequency Electronics Laboratory of Istanbul Technical University (ITU), in collaboration with TURKSAT, A.S. company as well as the Turkish Amateur Technology Organization. It was launched on April 26, 2013 as a secondary payload on a CZ-2D rocket from China’s Jiuquan Space Center to an altitude of approximately 680 km. The mission of the satellite has two primary goals: (1) to voice communication at Low Earth Orbit (LEO) and (2) to educate students by providing hands-on experience. TURKSAT-3USAT was designed to sustain a circular, near sun-synchronous LEO, and has dimensions of 10 x 10 x 34 cm3. Within the course of this paper, TURKSAT-3USAT’s thermal control will be addressed. TURKSAT-3USAT’s thermal control model was developed using ThermXL and ESATAN-TMS software. Using this model, temperature distributions of the CubeSat when subjected to various experimental conditions of interest were computed. Using a thermal vacuum chamber (TVAC), thermal cycling and bake-out testing were carried out on the flight model to verify the thermal design performance and check the mathematical model. Based on thermal analysis results, the temperature of equipment was within the allowable temperature range except for the batteries that were between 42.56 oC and -20.31 oC.