DOCSLIB.ORG

Of * SPACE Sôletstôé £K

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
Of * SPACE Sôletstôé £K v-% • •;• ESA SP -.1032' • • ' > " • A' •tL- •• ;• % •• .- . • i*-V'..;' • '-. '*•' 7 " • - - •Jr y ' * » •^ ••'• m, • • ..' *" * «-* V " »• •?*'.- - • • •3 - 1 •• l . • • * • •4 •• ) ..'.•, %.:" - / Report on thê açtiyitie« of * SPACE SÔlEtstôÉ £K •. :, .v f^gloo 2,85" esa SP-1032 September 1980 Report on the activities of Space Science Department in 1978/1979 Compiled by DE Page BFitton APedersen B G Taylor &K-PWenzel from inputs received from SSD staff european space agency / agence spatiale européenne 8-10, rue Mario-Nikis, 75738 PARIS CEDEX 15, France Documents in the ESA SP four-digit series contain information of value to or derived from the Agency's programmes (other than the proceedings of ESA- sponsored conferences or symposia), are published by the ESA Scientific and Technical Publications Branch. ESTEC. and are printed in The Netherlands by ESTEC Reproduction Services. Approved for publication: 18 July 1980 Edited by: W.R. Burke with the assistance of J. Mort. Job no.: 802645 Price code: El Copyright C 1980 by European Space Agency ISSN 0379-6566 Contents Introduction I Summary of Department budget and manpower 4 Cosmic Ray Division 5 Space Plasma Physics Division 21 Astronomy Division 33 High Energy» Astrophysics Division S3 Annex I - Considerations and recommendations of the SSD Advisory Committee 65 Annex II — List of Seminars 69 ( ! Introduction The 22 scientific staff in Space Science Department The Department aims through its structure, working support studies of potential ESA missions, act as project methods and continuous reorientation of its research scientists during the development and data-exploitation priorities to be in a position at any time to provide phases of chosen missions and carry out some research. scientific support to studies or projects over a majority of the scientific disciplines in or likely to come into the ESA The study scientist supports studies through the various scientific programme. It is unrealistic to attempt to cover phases leading up to selection of the Agency's projects. all areas and. given the constraints of a lowering <:tafT He feeds in at an early stage experience gained by SSD in ceiling and fixed budget, re-direction has to be slow former projects and attempts to bridge the gap between because of the long time constants ofspace projects. In the desires of the European scientists and the technical deciding how best to proceed. SSD has from time lo time and financial realities of project execution. sought advice from senior scientists outside ESA. The most recent report on SSD. which resulted from the The project scientist provides the liaison between the meeting of Professors J Geiss. J Hieblol. C de Jager. national experimenters and the ESA project engineers R Lust and Sir Harric Massey in July (978. is attached as and sorts out conflicts between scientists participating in an Annex to this report (rcf. ESA.SPC(7K}30). the same project. During project execution he tries lo ensure that the original scientific aims of the mission are SSD is at present structured in four Divisions The as far as possible maintained within the constraints Cosmic Ray. Space Plasma Physics. Astronomy and properly imposed by the available technology, the cost High Energy Astrophysics Divisions. Figure 1 illustrates and the schedule. Together with participating scientists this structure, names the scientists and visitors working he draws up plans for operating the satellite in orbit and in each Division and briefly lists the scientific topics for distributing the data. These plans require continuing being dealt with. The way in which SSD has evolved revision after launch in the light of scientific discoveries over the years in response lo the needs of the ESA and unexpected behaviour of spacecraft and programme is more fully described in the last SSD report experiments. The project scientist encourages the (Ref. ESA/SPCf7S)/l ), One change recently made (others exchange and intercomparison of data and frequently can be found in the body of the report) has been the organises symposia for these purposes. strengthening of the ultraviolet expertise in the Astronomy Division so that the Space Telescope project All SSD scientists participate in a research programme and allied photon-detector developments could be better which is carried out jointly with colleagues in other supported. This change was achieved at the expense of European laboratories. The time which any individual the infrared programme, since although SSD has had lo can give to his research varies markedly from year to allocate considerable feasibility-study effort to this area. year depending on the demands of the projects which ESA has not yet had an IR project approved. Although must be supported. On average, research occupies less the Department has no Division devoted to atmospheric then 50 percent of the working hours of an SSD scientist. physics, it has expertise in infrared techniques which are well suited to the study of the atmosphere and indeed In addition SSD has had on average during 1978/79 six joint proposals have been submitted for such studies. In visiting scientists, each of whom may be expected lo stay addition the Cosmic Ray Division has pursued, together for two years. This visitor programme is financed from with atmospheric scientists in Belgium, its interest in the General (Education) Budget of ESA and is not Sun/Earth relations by developing detectors to measure therefore a burden to the Scientific Programme. the solar constant, and plans are now being made to Although visitors, unlike other SSD staff, are not obliged devote the 1980 ESLAB symposium lo just this topic. to give priority to project work, SSD has found them helpful in all aspects of the work. Their presence has The Department has continued to adhere to its policy of helped to maintain a scientific atmosphere within SSD. carrying out research in co-operation with outside especially at times when the demands of project work scientific groups and of looking for arrangements which have threatened to extinguish the research programme, could benefit countries and institutes having little space and has helped to strengthen links with outside scientific experience. A recent example is the preparation by the groups. Cosmic Ray Division and Dublin Institute for Advanced Studies of a cosmic-ray experiment to be flown on the Long Duration Exposure Facility (Shuttle Test Flight). Head of department Assi./sec. Dr D E Page Miss A M van den Eijkel Divisions Cosmic Ray Space Plasma Physics Astroromy High energy astrophysics Division Head Dr K-P Wenzel Dr A Pedersen Dr B Fitton Dr BG Taylor Scientists Dr V Domingo Dr A Gonfalone Dr R Emery Dr RD Andresen Dr AC Durney Dr R Grard Dr Th de Graauw Dr K Bennett Dr R Reinhard Dr K Knott Dr B Feuerbacher Dr A Peacock Dr.TR Sanderson Dr V Formisano Dr F Macchetto Dr RD Wills Dr R Zobl Project ISPM Geos Lidar Cos-B scientist ISEE FSLP IUE Exosat support HEOS-2. HEOS-1. ST Exosat payload ESRO-IV FSLP management Studies 1978/79 Comets POLO Hipparcos EXUV Asteroids Eiscatsat Infrared space GRIST SEOCS Geos-3 observatory X-fay spectroscopy X-ray transients Research Cosmic rays + solar Magnetospheric fields + Opt. + UV astronomy X and gamma astronomy areas particles waves IR astronomy detection techniques Magnetosphere Surface charging Laboratory astrophysics Sun-climate relations Laboratory plasmas Visiting Dr R Kamermans Dr D Andersson DrSLidholm Dr J Davelaar scientists Dr JP Lebreton Dr D Naylor Dr G Manzo Dr F Becckmans (+five IUE Fellows at ( + Dr G Lichti Villafranca) (Cos-B. ESOC» Figure ! Posilion at end of 1979 In the chapters which follow each of the four Divisions provided by each Division. A dramatic increase appears has described its work in the sequence: 'Support given to in the chapter prepared by the Astronomy Division and projects', 'Support given to studies', and 'Research this is explained almost entirely by the success of IUE activities'. The effort and time devoted to each area of and the involvement of SSD staff at ESTEC together work is by no means proportional to the length of text with visiting scientists based at Villafranca in the IUE appearing in each area. Any attempt to fully describe spacecraft operations. support given to a project tends to result in what is merely a diary of meetings, tests, failures, re-scheduling SSD encouragement of other scientists to co-ordinate efforts, repair of experiments, re-tests, compromise data has continued and several symposia and workshops negotiation, inter-experimenter refereeing etc.. and such have been convened within the framework of the diaries, although instructive, seemed inappropriate in International Magnelospheric Study. The 1978 annual this report Reports on projects and studies therefore in symposium was held in cooperation with COSPAR at general simply describe the project and say that it was Innsbruck and was called: 'Advances in Magnetospheric supported. It should be mentioned, however, that major Physics with Geos-1 and ISEE-1 and 2'. The 1979 efforts, outside the normal role ofSSD, have gone into symposium on 'Magnetospheric Boundary Layers' was the IUE and Exosat projects. Tbe scientific operations of jointly sponsored by the Max Planck Institute at IUE were planned and are directed from the Astronomy Carching, Space Science Department the American Division to which the visiting scientists at Villafranca Geophysical Union, the European Geophysical Society report. The design and production of the Exosat payload and the Austrian Solar and Space Agency. For the is being managed from the High Energy Astrophysics twelfth time SSD compiled the report describing results Division and plans are now being made for the operation from ESA's scientific projects which is issued each year of the Exosat Observatory and the distribution of the at the time of the COSPAR meeting. A brief text written data. in more popular style (SP-1013) was also prepared in order to describe the 'Achievements of ESA Scientific During 1978/79 the rate of publications has remained at Satellites'.
Load more

Recommended publications
  • ESA Missions AO Analysis
    ESA Announcements of Opportunity Outcome Analysis Arvind Parmar Head, Science Support Office ESA Directorate of Science With thanks to Kate Isaak, Erik Kuulkers, Göran Pilbratt and Norbert Schartel (Project Scientists) ESA UNCLASSIFIED - For Official Use The ESA Fleet for Astrophysics ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 2 ESA Announcement of Observing Opportunities Ø Observing time AOs are normally only used for ESA’s observatory missions – the targets/observing strategies for the other missions are generally the responsibility of the Science Teams. Ø ESA does not provide funding to successful proposers. Ø Results for ESA-led missions with recent AOs presented: • XMM-Newton • INTEGRAL • Herschel Ø Gender information was not requested in the AOs. It has been ”manually” derived by the project scientists and SOC staff. ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 3 XMM-Newton – ESA’s Large X-ray Observatory ESA UNCLASSIFIED - For Official Use Dual-Anonymous Proposal Reviews | STScI | 25/09/2019 | Slide 4 XMM-Newton Ø ESA’s second X-ray observatory. Launched in 1999 with annual calls for observing proposals. Operational. Ø Typically 500 proposals per XMM-Newton Call with an over-subscription in observing time of 5-7. Total of 9233 proposals. Ø The TAC typically consists of 70 scientists divided into 13 panels with an overall TAC chair. Ø Output is >6000 refereed papers in total, >300 per year ESA UNCLASSIFIED - For Official Use
    [Show full text]
  • 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).
    [Show full text]
  • Naming the Extrasolar Planets
    Naming the extrasolar planets W. Lyra Max Planck Institute for Astronomy, K¨onigstuhl 17, 69177, Heidelberg, Germany [email protected] Abstract and OGLE-TR-182 b, which does not help educators convey the message that these planets are quite similar to Jupiter. Extrasolar planets are not named and are referred to only In stark contrast, the sentence“planet Apollo is a gas giant by their assigned scientific designation. The reason given like Jupiter” is heavily - yet invisibly - coated with Coper- by the IAU to not name the planets is that it is consid- nicanism. ered impractical as planets are expected to be common. I One reason given by the IAU for not considering naming advance some reasons as to why this logic is flawed, and sug- the extrasolar planets is that it is a task deemed impractical. gest names for the 403 extrasolar planet candidates known One source is quoted as having said “if planets are found to as of Oct 2009. The names follow a scheme of association occur very frequently in the Universe, a system of individual with the constellation that the host star pertains to, and names for planets might well rapidly be found equally im- therefore are mostly drawn from Roman-Greek mythology. practicable as it is for stars, as planet discoveries progress.” Other mythologies may also be used given that a suitable 1. This leads to a second argument. It is indeed impractical association is established. to name all stars. But some stars are named nonetheless. In fact, all other classes of astronomical bodies are named.
    [Show full text]
  • 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.
    [Show full text]
  • The High Energy Astrophysics Division Newsletter
    SPRING 2017 The High Energy Astrophysics Division Newsletter In this Issue: View from the Chair — special advertising section — hidden black holes revealed, and others — second running — finding a path through spacetime — announcing mysteries under the ice — performance enhancements for Chandra — milestones for XMM — the hunt continues for Swift — ULXNS — on the trail of the wild neutrino with INTEGRAL — searching at home with Fermi — energetic electrons seen at the ISS — news from the cosmos — of scientific interest — a Universe of learning — NICER launch prep — SRG progress — the wisdom of Athena — the slant on IXPE — the XARM — building CTA — all-seeing Lynx — in memoriam From the Chair for the discovery of merging black hole binaries, and for beginning the new era of gravitational-wave astronomy. CHRIS REYNOLDS (U. MD) Prof. González will give the Rossi Prize Lecture at the All systems are go for our 16th Divisional meeting to 231st AAS meeting to be held at National Harbor, MD be held in Sun Valley, Idaho, 20-24 August 2017! Regis- in January 2018. Please join me in congratulating all of tration and abstract submission is now open and we’re this year’s HEAD prize winners. looking forward to an exciting scientific program cover- ing all aspects of high-energy astrophysics, kicked off by The past few months has been eventful in the world a total solar eclipse! of high-energy astrophysics missions. NICER and ISS- CREAM are at the Kennedy Space Center and ready for One of the most important aspects of these meet- launch to the International Space Station. Further in the ings is the chance to honor a new batch of HEAD future, NASA has formally selected the Imaging X-ray Po- prize winners.
    [Show full text]
  • 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.
    [Show full text]
  • 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 .
    [Show full text]
  • Cygnus X-3 and the Case for Simultaneous Multifrequency
    by France Anne-Dominic Cordova lthough the visible radiation of Cygnus A X-3 is absorbed in a dusty spiral arm of our gal- axy, its radiation in other spectral regions is observed to be extraordinary. In a recent effort to better understand the causes of that radiation, a group of astrophysicists, including the author, carried 39 Cygnus X-3 out an unprecedented experiment. For two days in October 1985 they directed toward the source a variety of instru- ments, located in the United States, Europe, and space, hoping to observe, for the first time simultaneously, its emissions 9 18 Gamma Rays at frequencies ranging from 10 to 10 Radiation hertz. The battery of detectors included a very-long-baseline interferometer consist- ing of six radio telescopes scattered across the United States and Europe; the Na- tional Radio Astronomy Observatory’s Very Large Array in New Mexico; Caltech’s millimeter-wavelength inter- ferometer at the Owens Valley Radio Ob- servatory in California; NASA’s 3-meter infrared telescope on Mauna Kea in Ha- waii; and the x-ray monitor aboard the European Space Agency’s EXOSAT, a sat- ellite in a highly elliptical, nearly polar orbit, whose apogee is halfway between the earth and the moon. In addition, gamma- Wavelength (m) ray detectors on Mount Hopkins in Ari- zona, on the rim of Haleakala Crater in Fig. 1. The energy flux at the earth due to electromagnetic radiation from Cygnus X-3 as a Hawaii, and near Leeds, England, covered function of the frequency and, equivalently, energy and wavelength of the radiation.
    [Show full text]
  • Espinsights the Global Space Activity Monitor
    ESPInsights The Global Space Activity Monitor Issue 2 May–June 2019 CONTENTS FOCUS ..................................................................................................................... 1 European industrial leadership at stake ............................................................................ 1 SPACE POLICY AND PROGRAMMES .................................................................................... 2 EUROPE ................................................................................................................. 2 9th EU-ESA Space Council .......................................................................................... 2 Europe’s Martian ambitions take shape ......................................................................... 2 ESA’s advancements on Planetary Defence Systems ........................................................... 2 ESA prepares for rescuing Humans on Moon .................................................................... 3 ESA’s private partnerships ......................................................................................... 3 ESA’s international cooperation with Japan .................................................................... 3 New EU Parliament, new EU European Space Policy? ......................................................... 3 France reflects on its competitiveness and defence posture in space ...................................... 3 Germany joins consortium to support a European reusable rocket.........................................
    [Show full text]
  • Esrange Launching Programme
    ESRANGE SPACE CENTER EASP LAUNCHING PROGRAMME 16 AUGUST 2021 Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Rx/Bx TW SSC Cust Conf 2020 HEMERA SB 2020-2 Student balloon 1 balloon 1 balloon Mini-BOOSTER HEMERA SB 2020-1 3 balloons 2020 1 balloons SPIDER 2 1 IM rocket EOSTRE 1 balloon STERN 2020-2 LEONIS 1 rocket CNES 2021 BEXUS 30/31 STORT SF3 LTU IWC 16 MAPHEUS-11 4 balloons 2 balloons 1 Imp. Orion 1 Balloon 1 IM/IM rocket STORT SF1&2 TEXUS 57 BOLT-1 2Imp. Orion 1 VSB-30 rocket 1 S-31/IO rocket NO parachute test 2021 3-6 drops BROR test HADT 2021 REXUS 27/28 2 balloons STORT TF1 2 Imp. Orion rockets LTU IWC 17 1 IO rocket 1 Balloon HEMERA-2 MAPHEUS-9/10 CNES Pre-campaign 1 balloon 2 IM/IM rockets NASA summer 2022 / SUNRISE-3 REXUS 29/30 4 balloons BEXUS 32/33 2 Imp. Orion rockets SERA 4 2 balloons 1 rocket HADT 2022 TEXUS 58/59 (ESA) 2 balloons 2 VSB-30 rockets MIRIAM-2 MAIUS 2 HEMERA LSB-1 2022 1 IM/IO rocket 1 VSB-30 rocket 1 balloon BROR HIFLIER 1 1 IM/IO rocket 1 S-31/IO rocket S1X-M15 DLR ESBO STUDIO MAPHEUS-12 1 VSB-30 rocket 1 balloon 1 VSB-30 rocket STERN 2022-1 HyEnd 25th ESA-PAC symposium HEMERA-3 1 rocket Biarritz, France 1 balloon PERFORMED DECIDED TENTATIVE SCHEDULE UNDER CONSIDERATION NON-ESC LAUNCH PRE-TEST/OTHER EASTER ESRANGE SPACE CENTER EASP LAUNCHING PROGRAMME 16 AUGUST 2021 Jan Feb Mar Apr May Jun Jul Aug Sep Oct Nov Dec Rx/Bx TW 26th ESA-PAC symposium HEMERA2-1 BEXUS 34/35 Switzerland 1 balloon 2 balloons REXUS 31/32 2 Imp.
    [Show full text]
  • 18. ESLAB Symposium on X-Ray Astronomy C Cheveningen, W Ha*>E (Netherlands) 5-9 Nov 1984 EA-CONF—7714 X-RAY and OPTICAL
    18. ESLAB symposium on X-ray astronomy ccheveningen, W Ha*>e (Netherlands) 5-9 Nov 1984 CEEA-CONF—771A 4 X-RAY AND OPTICAL VARIABILITY AT THE HOUR TIMESCALE FOR IE 0630+178 (GEMINGA) AND ITS PROPOSED OPTICAL COUTERPART L. vigroux1, J. A. Paul Service d'Astrophysique, Centre d'Etudes Nucléaires de Saclay 91191 Gif-sur-Yvette CEDEX, France P. Delâche Observatoire de Nice, BP 139, 06003 Nice CEDEX, France G. F. Bignami, P. A. Caraveo Istituto di Fisica Cosmica del CNR Via Bassini 15, 20133 Kilano, Italy L. Salotti Dipartimento di Fisica, Université di Milano via Celoria 16, 20133 Milano, Italy ABSTRACT. Einttem and EXOSAT data on the soft X-ray source IE 0630+173, the proposed counterpart of the -r-ray source GEMINGA, are analyzed for variability on the time scale of one to three hours. The EXOSAT September 1983 data, with an uninterrupted strech of over 10 he-.-s offer the most interesting case. In parallel, a similar analysis is presented for the first time, for the optical data of the m ~2i proposed counterpart. About 30 CCD exposures, of 15 min. each, taken over two consecutive nights at the 3.6 m CFH telescope, yield evidence of variability, when compared to the data of similar nearby objects in the field. 1. INTRODUCTION The high-energy (£50 Mev) 7-ray source 2CG 195+04 (GEMINGA), discovered by the $AS-2 satellite and accurately measured by the COS-B mission, has recently been identified with an Eimtatn/EXOSAT soft X-ray source through its periodic emission at -59 s, Which had been seen in the SAS-2 data, subsequently confirmed and later retracted by the COS-B team as non significant (see Bignami, Caraveo, and Paul 1984, and references therein).
    [Show full text]
  • Japan's Technical Prowess International Cooperation
    Japan Aerospace Exploration Agency April 2016 No. 10 Special Features Japan’s Technical Prowess Technical excellence and team spirit are manifested in such activities as the space station capture of the HTV5 spacecraft, development of the H3 Launch Vehicle, and reduction of sonic boom in supersonic transport International Cooperation JAXA plays a central role in international society and contributes through diverse joint programs, including planetary exploration, and the utilization of Earth observation satellites in the environmental and disaster management fields Japan’s Technical Prowess Contents No. 10 Japan Aerospace Exploration Agency Special Feature 1: Japan’s Technical Prowess 1−3 Welcome to JAXA TODAY Activities of “Team Japan” Connecting the Earth and Space The Japan Aerospace Exploration Agency (JAXA) is positioned as We review some of the activities of “Team the pivotal organization supporting the Japanese government’s Japan,” including the successful capture of H-II Transfer Vehicle 5 (HTV5), which brought overall space development and utilization program with world- together JAXA, NASA and the International Space Station (ISS). leading technology. JAXA undertakes a full spectrum of activities, from basic research through development and utilization. 4–7 In 2013, to coincide with the 10th anniversary of its estab- 2020: The H3 Launch Vehicle Vision JAXA is currently pursuing the development lishment, JAXA defined its management philosophy as “utilizing of the H3 Launch Vehicle, which is expected space and the sky to achieve a safe and affluent society” and to become the backbone of Japan’s space development program and build strong adopted the new corporate slogan “Explore to Realize.” Under- international competitiveness.
    [Show full text]