0418 Space Cluster Brochure FINAL
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Russia's Posture in Space
Russia’s Posture in Space: Prospects for Europe Executive Summary Prepared by the European Space Policy Institute Marco ALIBERTI Ksenia LISITSYNA May 2018 Table of Contents Background and Research Objectives ........................................................................................ 1 Domestic Developments in Russia’s Space Programme ............................................................ 2 Russia’s International Space Posture ......................................................................................... 4 Prospects for Europe .................................................................................................................. 5 Background and Research Objectives For the 50th anniversary of the launch of Sputnik-1, in 2007, the rebirth of Russian space activities appeared well on its way. After the decade-long crisis of the 1990s, the country’s political leadership guided by President Putin gave new impetus to the development of national space activities and put the sector back among the top priorities of Moscow’s domestic and foreign policy agenda. Supported by the progressive recovery of Russia’s economy, renewed political stability, and an improving external environment, Russia re-asserted strong ambitions and the resolve to regain its original position on the international scene. Towards this, several major space programmes were adopted, including the Federal Space Programme 2006-2015, the Federal Target Programme on the development of Russian cosmodromes, and the Federal Target Programme on the redeployment of GLONASS. This renewed commitment to the development of space activities was duly reflected in a sharp increase in the country’s launch rate and space budget throughout the decade. Thanks to the funds made available by flourishing energy exports, Russia’s space expenditure continued to grow even in the midst of the global financial crisis. Besides new programmes and increased funding, the spectrum of activities was also widened to encompass a new focus on space applications and commercial products. -
Template: 10Th Anniversary Powerpoint
Science and Technology Facilities Council One of Europe’s largest multi-disciplinary scientific research organisations Dr Ling Xu How we’re funded Taxpayers HM Government (and HM Treasury) STFC science and technology delivers real benefits to peoples’ lives, and contributes to the prosperity and security of the UK Delivering Economic Growth through Innovation STFC’s Asset Base Innovation Resilient Economy Knowledge Skills Technology Inspiration What we spend £530m from government in 2015-16* • International Subscriptions (CERN, ESO, ILL, ESRF, FAIR) £155m • Domestic Facilities (ISIS, Diamond, CLF) £156m • Core (academic grants, lab operations, support services) £218m • Supplemented by project-based external revenue around £60m p.a. International Facilities Core Revenue What we do World Class Research, Innovation and Skills • Broad range of physical, life and computational sciences • Around 1,700 scientists in particle and nuclear physics, and astronomy mainly in the University Sector • Access for 7,500 scientists to world-leading, large-scale facilities • Science and Innovation Campuses at Daresbury and Harwell • Globally-recognised capabilities and expertise in technology R&D • Inspiring young people to undertake STEM What we are Boulby Underground UK Astronomy Technology Centre Laboratory Edinburgh, Scotland North Yorkshire Polaris House Daresbury Laboratory Swindon, Wiltshire Sci-Tech Daresbury Warrington, Cheshire Chilbolton Observatory Rutherford Appleton Laboratory Stockbridge, Hampshire Harwell Didcot, Oxfordshire …and internationally Our facilities drive research Neutron Sources • Providing powerful insights into key areas of energy, biomedical research, climate, environment and security. High Power Lasers • Providing applications on bioscience and nanotechnology and demonstrating laser driven fusion as a future source of sustainable, clean energy. Light Sources • Providing new breakthroughs in medicine, environmental and materials science, engineering, electronics and cultural heritage. -
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. -
Lunar Life Sciences Payload Assessment
Lunar Surface Science Workshop 2020 (LPI Contrib. No. 2241) 5077.pdf LUNAR LIFE SCIENCES PAYLOAD ASSESSMENT. S. C. Sun1, F. Karouia2, M. P. Lera3, M. P. Parra1, H. E. Ray4, A. J. Ricco1, S. M. Spremo1. 1NASA Ames Research Center, 2Blue Marble Space Institute of Science, 3KBR, 4ASRC Federal Space and Defense, Inc. Introduction: The Moon provides a unique site to ISS, including systems that integrate into EXPRESS study living organisms. The fractional gravity and (EXpedite the PRocessing of ExperimentS for Space) unique radiation environment have similarities to Mars Racks or are external space exposure research facilities. and will help us understand how life will respond to These same systems can be the basis for future payload conditions on the red planet. Martian and lunar envi- systems for experiments to be performed beyond Low ronments can be simulated on the ground but not to high Earth Orbit. Such facilities would need to be adapted to fidelity. Altered gravity and increased radiation are dif- be compatible with the new research platforms and ficult to replicate simultaneously, which makes study- function in the harsher radiation environment found out- ing their combined effect difficult. The International side the magnetosphere. If Gateway and a lunar based- Space Station, and previously, the Space Shuttle, pro- lab could provide EXPRESS-compatible interfaces, lev- vided a microgravity environment, and could simulate eraging hardware developed for ISS would be more fea- fractional-g only via an onboard centrifuge. Because sible. the ISS and Space Shuttle orbits were within the Earth’s Gaps in Capabilities: Many of the payload systems magnetosphere, experiments on those platforms have that have been developed require human tending. -
Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards
Utah State University DigitalCommons@USU Presentations Materials Physics 5-8-2017 Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards JR Dennison Utah State Univesity Follow this and additional works at: https://digitalcommons.usu.edu/mp_presentations Part of the Condensed Matter Physics Commons Recommended Citation Dennison, JR, "Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards" (2017). Utah NASA Space Grant Consortium Annual Meeting. Presentations. Paper 168. https://digitalcommons.usu.edu/mp_presentations/168 This Presentation is brought to you for free and open access by the Materials Physics at DigitalCommons@USU. It has been accepted for inclusion in Presentations by an authorized administrator of DigitalCommons@USU. For more information, please contact [email protected]. Of Mice and Materials: Payoffs of UNSGC Research Infrastructure Awards J.R. Dennison Materials Physics Group Physics Department, Utah State University Utah NASA Space Grant Consortium Annual Meeting Weber State University May 8, 2017 To paraphrase Douglas Adams, “Space is [harsh]. You just won’t believe how vastly, hugely, mind-bogglingly [harsh] it is.” Interactions with this harsh space environment can modify materials and cause unforeseen and detrimental effects to spacecraft. The Poster Child for Space Environment Effects Ag coated Mylar with micrometeoroid impact USU MISSIE SUSpECS Logan, UT II Sample Tray Before After Complex dynamic interplay between space environment, satellite motion, and materials properties Facilities & Capabilities • Four ultrahigh vacuum chambers for electron emission tests equipped with electron, ion, and photon sources, detectors, and surface analysis capabilities. Sample Characterization & Preparation • Two high vacuum chambers for resistivity tests. • Bulk composition (AA, IPC). • High vacuum chamber for electrostatic breakdown tests. -
18Th EANA Conference European Astrobiology Network Association
18th EANA Conference European Astrobiology Network Association Abstract book 24-28 September 2018 Freie Universität Berlin, Germany Sponsors: Detectability of biosignatures in martian sedimentary systems A. H. Stevens1, A. McDonald2, and C. S. Cockell1 (1) UK Centre for Astrobiology, University of Edinburgh, UK ([email protected]) (2) Bioimaging Facility, School of Engineering, University of Edinburgh, UK Presentation: Tuesday 12:45-13:00 Session: Traces of life, biosignatures, life detection Abstract: Some of the most promising potential sampling sites for astrobiology are the numerous sedimentary areas on Mars such as those explored by MSL. As sedimentary systems have a high relative likelihood to have been habitable in the past and are known on Earth to preserve biosignatures well, the remains of martian sedimentary systems are an attractive target for exploration, for example by sample return caching rovers [1]. To learn how best to look for evidence of life in these environments, we must carefully understand their context. While recent measurements have raised the upper limit for organic carbon measured in martian sediments [2], our exploration to date shows no evidence for a terrestrial-like biosphere on Mars. We used an analogue of a martian mudstone (Y-Mars[3]) to investigate how best to look for biosignatures in martian sedimentary environments. The mudstone was inoculated with a relevant microbial community and cultured over several months under martian conditions to select for the most Mars-relevant microbes. We sequenced the microbial community over a number of transfers to try and understand what types microbes might be expected to exist in these environments and assess whether they might leave behind any specific biosignatures. -
LOFAR-UK a Science Case for UK Involvement in LOFAR
LOFAR-UK A science case for UK involvement in LOFAR Assembled and edited on behalf of the LOFAR-UK consortium by Philip Best December 2007 Contributors: Paul Alexander (Cambridge), David Bacon (Edinburgh/Portsmouth), David Bersier (Liverpool JMU), Philip Best (Edinburgh), Rob Beswick (Manchester), Andy Breen (Aberyst- wyth), Elias Brinks (Hertfordshire), Catherine Brocksopp (UCL/MSSL), Sandra Chapman (War- wick), Michele Cirasuolo (Edinburgh), Judith Croston (Hertfordshire), Owain Davies (RAL), Tom Dwelly (Southampton), Steve Eales (Cardiff), Alastair Edge (Durham), Brian Ellison (RAL), Rob Fender (Southampton), Lyndsay Fletcher (Glasgow), Martin F¨ullekrug (Bath), Simon Garrington (Manchester), Dave Green (Cambridge), Martin Haehnelt (Cambridge), Martin Hardcastle (Hert- fordshire), Richard Harrison (RAL), Faridey Honary (Lancaster), Rob Ivison (ATC), Neal Jackson (Manchester), Matt Jarvis (Hertfordshire), Christian Kaiser (Southampton), Joe Khan (Glasgow), Hans-Rainer Kl¨ockner (Oxford), Eduard Kontar (Glasgow), Michael Kramer (Manchester), Cedric Lacey (Durham), Mark Lancaster (UCL), Tom Maccarone (Southampton), Alec MacKinnon (Glas- gow), Ross McLure (Edinburgh), Avery Meiksin (Edinburgh), Cathryn Mitchell (Bath), Bob Nichol (Portsmouth), Will Percival (Portsmouth), Robert Priddey (Hertfordshire), Steve Rawlings (Ox- ford), Chris Simpson (Liverpool JMU), Ian Stevens (Birmingham), Tom Theuns (Durham), Phil Uttley (Southampton), Peter Wilkinson (Manchester), Graham Woan (Glasgow) Contents 1 Executive Summary 1 2 Introduction 3 2.1 International extensions of LOFAR . .......... 4 2.2 Thisdocument .................................... ... 6 3 LOFAR in the context of UK radio astronomy 7 3.1 The University of Manchester and Jodrell Bank Observatory ............. 7 3.2 The University of Cambridge and the Mullard Radio Astronomy Observatory . 8 3.3 LOFAR-UK as a stepping-stone to the SKA . ...... 9 4 LOFAR-UK and the Epoch of Reionisation 10 4.1 Introduction: The Epoch of Reionisation . -
Space Biology Research and Biosensor Technologies: Past, Present, and Future †
biosensors Perspective Space Biology Research and Biosensor Technologies: Past, Present, and Future † Ada Kanapskyte 1,2, Elizabeth M. Hawkins 1,3,4, Lauren C. Liddell 5,6, Shilpa R. Bhardwaj 5,7, Diana Gentry 5 and Sergio R. Santa Maria 5,8,* 1 Space Life Sciences Training Program, NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (A.K.); [email protected] (E.M.H.) 2 Biomedical Engineering Department, The Ohio State University, Columbus, OH 43210, USA 3 KBR Wyle, Moffett Field, CA 94035, USA 4 Mammoth Biosciences, Inc., South San Francisco, CA 94080, USA 5 NASA Ames Research Center, Moffett Field, CA 94035, USA; [email protected] (L.C.L.); [email protected] (S.R.B.); [email protected] (D.G.) 6 Logyx, LLC, Mountain View, CA 94043, USA 7 The Bionetics Corporation, Yorktown, VA 23693, USA 8 COSMIAC Research Institute, University of New Mexico, Albuquerque, NM 87131, USA * Correspondence: [email protected]; Tel.: +1-650-604-1411 † Presented at the 1st International Electronic Conference on Biosensors, 2–17 November 2020; Available online: https://iecb2020.sciforum.net/. Abstract: In light of future missions beyond low Earth orbit (LEO) and the potential establishment of bases on the Moon and Mars, the effects of the deep space environment on biology need to be examined in order to develop protective countermeasures. Although many biological experiments have been performed in space since the 1960s, most have occurred in LEO and for only short periods of time. These LEO missions have studied many biological phenomena in a variety of model organisms, and have utilized a broad range of technologies. -
An Initial Assessment of the Robust and Compact Hybrid Environmental Lidar (RACHEL)
An initial assessment of the Robust And Compact Hybrid Environmental Lidar (RACHEL) A.C. Povey1, D.M. Peters1, R.G. Grainger1, D. Rees2, and J.L. Agnew3 1University of Oxford, Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, Parks Road, Oxford, OX1 3PU, United Kingdom, [email protected] 2Hovemere Ltd., Tonbridge, TN9 1RF, United Kingdom 3STFC Rutherford Appleton Laboratory, HSIC, Didcot, OX11 0QX, United Kingdom ABSTRACT The Robust And Compact Hybrid Environmental Lidar (RACHEL) is a 355nm, 4-channel Raman lidar system that has been developed for unattended, continuous measurement of the distributions of particulates, wa- ter vapour, and other pollutants in the boundary layer and troposphere, including the capacity for scanning the full hemisphere. The system has been designed to be portable and low-cost, providing the potential to investigate a wide range of environments with a single instrument. Deployment at the beginning of 2010 at the STFC Chilbolton Observatory has provided a unique oppor- tunity to cross-compare the instrument against the nu- merous lidar and radar systems stationed at the obser- vatory and to evaluate the implementation of various measurements into the data evaluation, such as ra- diosondes, radiometers, and aircraft observations. The system was deployed during the Eyjafjallajökull erup- Figure 1. RACHEL deployed at the Chilbolton Observatory in tion of April 2010, observing the appearance and evo- southern England. Reflective insulation has been applied to lution of the ash plume over southern England. the surfaces exposed to direct sunlight to improve tempera- ture stability. 1. INTRODUCTION beam is expanded by a factor five to a diameter of Aerosols present the greatest source of uncertainty in 35 mm with divergence < 0.3 mrad and is transmitted global climate models [1]. -
NASA Ames to Establish Nationwide Lunar Science Institute
November 2007 Worden gives upbeat message about future work for Ames BY JOHN BLUCK "We have switched material to In an upbeat talk to a crowd that phenolic impregnated carbon abla- filled the Ames main auditorium, tor (PICA), a (heat shield) material Ames Center Director S. Pete Worden developed here," Worden noted. His outlined an exciting future at Ames projected slide also listed Ames as that includes new work in exploration, leading PICA development and test- science and aeronautics -- each about a ing both for the Crew Exploration Ve- third of the center's efforts, he said. "I hicle, now called Orion, and the Mars have a gazillion charts to go through," Science Laboratory (MSL), which has photo by Eric James NASA he said. a planned launch date in fall 2009. His wide-ranging presentation Worden said that Ames' arc jets about Ames touched on moon explo- facility "a unique facility in the world." ration, a lunar institute, moon dust re- He added, "We want to upgrade search, heat shield work for spacecraft them." destined for the moon and Mars, a Mars sample "cache box" assignment, Life Sciences rising supercomputer capability, small "We are getting additional life Ames Center Director S. Pete Worden responds satellite work with a potential for support tasks assigned by Johnson to a question during the recent upbeat talk he many missions, increased astrobiology (and Marshall)," Worden said. "This is gave to the center about the future of Ames. work, growing cooperation among significant." continued on page 5 academia, and commercial partners and Ames and much more. -
6 FOTON RETRIEVABLE CAPSULES This Section Is Aimed at Providing New and Experienced Users with Basic Utilisation Information Regarding Foton Retrievable Capsules
6 FOTON RETRIEVABLE CAPSULES This section is aimed at providing new and experienced users with basic utilisation information regarding Foton retrievable capsules. It begins with an introduction to the Foton capsule. 6.1 Introduction to Foton Capsules 6.1.1 What Are Foton Capsules? Foton capsules (Figure 6-1 and Figure 6-2) are unmanned, retrievable capsules, derived from the design of the 1960’s Soviet Vostok manned spacecraft and the Zenit military reconnaissance satellite. These capsules are very similar to the Bion and Resurs-F satellites introduced by the Soviets in the 1970’s, for biological research and Earth natural resources investigation, respectively. The first Foton capsule was launched in 1985 as Cosmos 1645 and only with the fourth launch in 1988 was the spacecraft officially designated Foton (Foton-4). These capsules are launched into near-circular, low-earth orbits by a Soyuz-U rocket, providing researchers with gravity levels less than 10 -5 g, for missions lasting approximately 2 weeks. The earlier Foton missions were conceived primarily for materials science research, but later missions also began to include experiments in the fields of fluid physics, biology and radiation dosimetry. ESA’s participation in the Foton programme began in 1991 with a protein crystallisation experiment on-board Foton-7, followed by a further 35 experiments up to and including the Foton- 12 mission in 1999. In 2002, ESA provided a large number of experiments for the Foton-M1 mission (the first flight of an upgraded version of the Foton spacecraft). This mission ended in disaster when the Soyuz launcher rocket exploded shortly after lift-off due to a malfunction in one of its engines. -
Genesat (Launched Dec 2006), – Pre-Sat/Nanosail-D (Aug 2008) – Pharmasat (Launched May 2009), – O/OREOS (Planned May
National Aeronautics and Space Administration Free Flyer Utilization for Biology Research John W. Hines Chief Technologist, Engineering Directorate Technical Director, Nanosatellite Missions NASA-Ames Research Center NASA Applications of BioScience/BioTechnology HumanHuman ExplorationExploration EmphasisEmphasis FundamentalFundamental ExploratiExploratioonn Subsystems BiologyBiology Subsystems EmphasisEmphasis HumansHumans SmallSmall OrganismsOrganisms (Mice,(Mice, Rats) Rats) TiTissussue,e, O Orrgansgans MammalianMammalian CellsCells Human Health Emphasis ModelModel Organisms, BioMolecules Organisms, BioMolecules MicrobesMicrobes 2 4 Free-Flyer Utilization Free Flyer Features • Advantage: Relatively inexpensive means to increase number of flight opportunities • Capabilities: – Returnable capsule to small secondary non-recoverable satellites, and/or – In-situ measurement and control with autonomous sample management • Command and Control: Fully automated or uplinked command driven investigations. • Research data: Downlink and/or receipt of the samples • Collaborations: Interagency, academic, commercial and international Russian Free Flyers Early Free Flyers NASA Biosatellite I, II, 1966-67 NASA Biosatellite III, 1969 Nominal 3d flights Nominal 20d flight • Response to microgravity & • Spaceflight responses of non-human radiation: various biological species primates • Onboard radiation source Timeline of Russian-NASA Biology Spaceflights Collaborations Bion* Characteristics Bion Rationale • Increases access to space • Proven Platforms