Space Weather Effects Effects from Solar Storms
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Multiple Polar Cap Arcs: Akebono &Lpar;Exos D&Rpar; Observations
Radio Science,Volume 31, Number 3, Pages645-653, May-June 1996 Multiple polar cap arcs: Akebono (Exos D) observations T. Obara, T. Mukai, H. Hayakawa, K. Tsuruda, A. Matsuoka, and A. Nishida Institute of Spaceand AstronauticalScience, Kanagawa, Japan H. Fukunishi Department of Geophysicsand Astrophysics,Tohoku University,Sendai, Japan Center for Atmosphericand SpaceSciences, Utah State University,Logan Abstract. Akebono (Exos D) observationsdemonstrate that polar cap arcssometimes have a fine structure,that is, multiple (doubleor triple) arcswith spacingof a few tens of kilometers.The multiplepolar cap arcsare dominantlyobserved in the nightsidepolar cap region, suggestingthat low backgroundconductance favors the appearanceof the structuredarcs. A relationshipbetween the spacingand the averageenergy of the precipitatingelectrons is investigated.Results show that a higher energyleads to a wider spacing.Akebono observationsalso showthe existenceof a downwardcurrent region embeddedbetween upward current regions (arcs). Comparison of the observationswith resultsfrom a coupledmagnetosphere-ionosphere Sun-aligned arc model is made, which showsgood qualitativeagreement between the modelingand observationalresults on the spacing-energydependence and the effect of backgroundionospheric conductance. Introduction dawn-to-duskcomponent of the electric field is the major contributorto the negativedivE. These results The electronsreaching low altitudes in the polar suggestthat localized electron precipitation in the cap region were categorized as "polar -
Doc.10100.Space Weather Manual FINAL DRAFT Version
Doc 10100 Manual on Space Weather Information in Support of International Air Navigation Approved by the Secretary General and published under his authority First Edition – 2018 International Civil Aviation Organization TABLE OF CONTENTS Page Chapter 1. Introduction ..................................................................................................................................... 1-1 1.1 General ............................................................................................................................................... 1-1 1.2 Space weather indicators .................................................................................................................... 1-1 1.3 The hazards ........................................................................................................................................ 1-2 1.4 Space weather mitigation aspects ....................................................................................................... 1-3 1.5 Coordinating the response to a space weather event ......................................................................... 1-3 Chapter 2. Space Weather Phenomena and Aviation Operations ................................................................. 2-1 2.1 General ............................................................................................................................................... 2-1 2.2 Geomagnetic storms .......................................................................................................................... -
Space UK Earth’S Surface Water
Issue #49 IN THIS ISSUE: Staring at the Sun MYSTERIOUS Helpline from Space Weightless in the Clouds MERCURY Contents News Cornwall Calling Space Weather Watcher Mapping the Route to Mars Honour for UK Astronaut New Satellite Tracks Pollution UK-France Space Deal In Pictures The Sun Features Mysterious Mercury Zero-G Science Helpline from Space Education Resources UK Space History Skylark Made in the UK Earth-i Info News Cornwall Calling The first Moon landing Cornwall Calling Credit: NASA Cornwall could soon be Antennas at Goonhilly beamed communicating with the Moon and images of the 1969 Moon landing Mars, following the announcement and, shortly after it was built in that the world’s first commercial deep 1985, the 32-metre Goonhilly-6 space communication base will be at antenna carried the historic Live Aid the Goonhilly Earth Station. concert broadcast to TV viewers An £8.4 million investment will see a around the world. two-year upgrade of the Goonhilly-6 A Space Industry Bill, announced antenna so it can communicate as part of the Queen’s speech in One of the large dishes at Goonhilly with future robotic and crewed 2017, will introduce new powers missions to the Moon and Mars. The to allow rocket and spaceplane Credit: Goonhilly Cornwall and Isles of Scilly Local launches from UK soil. Goonhilly is Enterprise Partnership’s Growth Deal also offering spacecraft tracking and the European Space Agency and communications facilities as (ESA) – which the UK Space Agency part of the Spaceport Cornwall contributes to – funded the contract, funding bid. which will allow Goonhilly to support “We see huge opportunities for ESA’s worldwide network of spacecraft the developing space sector in monitoring ground stations. -
Mp-Ist-056-32
UNCLASSIFIED/UNLIMITED The International Reference Ionosphere – Climatological Standard for the Ionosphere Dieter Bilitza Raytheon IS, Space Physics Data Facility GSFC, Code 612.4 Greenbelt, MD 20771 U.S.A. [email protected] ABSTRACT The International Reference Ionosphere (IRI) a joint project of URSI and COSPAR is the defacto standard for a climatological specification of ionospheric parameters. IRI is based on a wide range of ground and space data and has been steadily improved since its inception in 1969 with the ever-increasing volume of ionospheric data and with better mathematical descriptions of the observed global and temporal variation patterns. The IRI model has been validated with a large amount of data including data from the most recent ionospheric satellites (KOMPSAT, ROCSAT and TIMED) and data from global network of ionosondes. Several IRI teams are working on specific aspects of the IRI modeling effort including an improved representation of the topside ionosphere with a seamless transition to the plasmasphere, a new effort to represent the global variation of F2 peak parameters using the Neural Network (NN) technique, and the inclusion of several additional parameters in IRI, e.g., spread-F probability and ionospheric variability. Annual IRI workshops are the forum for discussions of these efforts and for all science activities related to IRI as well as applications of the IRI model in engineering and education. In this paper I will present a status report about the IRI effort with special emphasis on the presentations and results from the most recent IRI Workshops (Paris, 2004; Tortosa, 2005) and on the most important ongoing IRI activities. -
UC Irvine UC Irvine Previously Published Works
UC Irvine UC Irvine Previously Published Works Title Astrophysics in 2006 Permalink https://escholarship.org/uc/item/5760h9v8 Journal Space Science Reviews, 132(1) ISSN 0038-6308 Authors Trimble, V Aschwanden, MJ Hansen, CJ Publication Date 2007-09-01 DOI 10.1007/s11214-007-9224-0 License https://creativecommons.org/licenses/by/4.0/ 4.0 Peer reviewed eScholarship.org Powered by the California Digital Library University of California Space Sci Rev (2007) 132: 1–182 DOI 10.1007/s11214-007-9224-0 Astrophysics in 2006 Virginia Trimble · Markus J. Aschwanden · Carl J. Hansen Received: 11 May 2007 / Accepted: 24 May 2007 / Published online: 23 October 2007 © Springer Science+Business Media B.V. 2007 Abstract The fastest pulsar and the slowest nova; the oldest galaxies and the youngest stars; the weirdest life forms and the commonest dwarfs; the highest energy particles and the lowest energy photons. These were some of the extremes of Astrophysics 2006. We attempt also to bring you updates on things of which there is currently only one (habitable planets, the Sun, and the Universe) and others of which there are always many, like meteors and molecules, black holes and binaries. Keywords Cosmology: general · Galaxies: general · ISM: general · Stars: general · Sun: general · Planets and satellites: general · Astrobiology · Star clusters · Binary stars · Clusters of galaxies · Gamma-ray bursts · Milky Way · Earth · Active galaxies · Supernovae 1 Introduction Astrophysics in 2006 modifies a long tradition by moving to a new journal, which you hold in your (real or virtual) hands. The fifteen previous articles in the series are referenced oc- casionally as Ap91 to Ap05 below and appeared in volumes 104–118 of Publications of V. -
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. -
Jaxa Today 10.Pdf
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 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. We examine the H3’s unique features and the development program’s pinned by this philosophy, JAXA pursues a broad range of pro- objectives. -
Committee on Space Research (COSPAR)
COSPAR 2020 AWARDS Press Release (for immediate release) Committee on Space Research (COSPAR) To be presented on 30 January during the 43rd COSPAR Scientific Assembly 28 January – 4 February 2021, Sydney, Australia See below for complete citations and a brief description of COSPAR. - COSPAR Space Science Award for outstanding contributions to space science: William J. Borucki (USA), Astrobiology and Space Research Directorate, NASA Ames Research Center, Moffett Field, California Ken McCracken (Australia), CSIRO and Jellore Technologies, retired, New South Wales - COSPAR International Cooperation Medal for distinguished contributions to space science and work that has contributed significantly to the promotion of international scientific cooperation: John Kiss (USA) and Francisco Javer Medina Díaz (Spain), College of Arts & Sciences, University of North Carolina—Greensboro, Greensboro, North Carolina and PCNPµG Lab (Plant Cell Nucleolus, Proliferation & Microgravity), Centro de Investigaciones Biológicas – CSIC, Madrid - COSPAR William Nordberg Medal commemorating the late William Nordberg and for distinguished contributions to the application of space science in a field covered by COSPAR: Daniel J. McCleese (USA), Jet Propulsion Laboratory, California Institute of Technology, Pasadena, California - COSPAR Harrie Massey Award honoring the memory of Sir Harrie Massey, FRS, for outstanding contributions to the development of space research in which a leadership role is of particular importance: Alexander Held (Australia), CSIRO Centre of -
Modeling Seasonal Variations of Auroral Particle Precipitation in a Global-Scale Magnetosphere-Ionosphere Simulation M
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114, A01204, doi:10.1029/2008JA013108, 2009 Modeling seasonal variations of auroral particle precipitation in a global-scale magnetosphere-ionosphere simulation M. Wiltberger,1 R. S. Weigel,2 W. Lotko,3 and J. A. Fedder4 Received 20 February 2008; revised 8 September 2008; accepted 6 November 2008; published 14 January 2009. [1] A variety of observations have shown strong seasonal variations in a vast array of magnetosphere-ionosphere parameters, including field-aligned currents, cross polar cap potential, and precipitating electron energy flux. In this paper we examine how these variations are modeled in the Lyon-Fedder-Mobarry (LFM) global-scale magnetohydrodynamic simulation of the coupled solar wind-magnetosphere-ionosphere system. In order to account for changes in the solar wind conditions caused by the seasonal variation of the Earth’s dipole tilt we carefully select the solar wind parameters so that the effective driving conditions are the same across the March, June, and December intervals examined. The seasonal variation of the field-aligned current strengths is in good agreement with observations, with the sunlit hemisphere having more current than the dark hemisphere in the June and December intervals. However, in order to bring the modeled precipitating electron energy flux into better agreement with the observations we need to utilize a modified current-voltage relationship which includes a proxy for illumination effects. We provide a detailed description of the LFM’s magnetosphere-ionosphere coupling interface including how illumination effects are incorporated into the model. This methodology for including these effects does not allow for determining if changes in conductance or ionospheric density are responsible for the changes. -
Associations Between Space Weather Events and the Incidence of Acute Myocardial Infarction and Deaths from Ischemic Heart Disease
atmosphere Article Associations between Space Weather Events and the Incidence of Acute Myocardial Infarction and Deaths from Ischemic Heart Disease Vidmantas Vaiˇciulis 1,2,*, Jone˙ Vencloviene˙ 3,4, Abdonas Tamošiunas¯ 5,6, Deivydas Kiznys 3, Dalia Lukšiene˙ 1,5, Daina Kranˇciukaite-Butylkinien˙ e˙ 5,7 and RiˇcardasRadišauskas 1,5 1 Department of Environmental and Occupational Medicine, Lithuanian University of Health Sciences, LT-47181 Kaunas, Lithuania; [email protected] (D.L.); [email protected] (R.R.) 2 Health Research Institute, Lithuanian University of Health Sciences, LT-47181 Kaunas, Lithuania 3 Department of Environmental Sciences, Vytautas Magnus University, LT-44248 Kaunas, Lithuania; [email protected] (J.V.); [email protected] (D.K.) 4 Laboratory of Clinical Cardiology, Institute of Cardiology, Lithuanian University of Health Sciences, LT-50103 Kaunas, Lithuania 5 Laboratory of Population Studies, Institute of Cardiology, Lithuanian University of Health Sciences, LT-50103 Kaunas, Lithuania; [email protected] (A.T.); [email protected] (D.K.-B.) 6 Department of Preventive Medicine, Lithuanian University of Health Sciences, LT-47181 Kaunas, Lithuania 7 Department of Family Medicine, Lithuanian University of Health Sciences, LT-50009 Kaunas, Lithuania * Correspondence: [email protected]; Tel.: +370-678-34506 Abstract: The effects of charged solar particles hitting the Earth’s magnetosphere are often harmful Citation: Vaiˇciulis,V.; Vencloviene,˙ J.; and can be dangerous to the human organism. The aim of this study was to analyze the associations Tamošiunas,¯ A.; Kiznys, D.; Lukšiene,˙ of geomagnetic storms (GSs) and other space weather events (solar proton events (SPEs), solar flares D.; Kranˇciukaite-Butylkinien˙ e,˙ D.; (SFs), high-speed solar wind (HSSW), interplanetary coronal mass ejections (ICMEs) and stream Radišauskas, R. -
Anti-Aging Effects of Long-Term Space Missions, Estimated by Heart Rate
www.nature.com/scientificreports OPEN Anti-aging efects of long-term space missions, estimated by heart rate variability Received: 10 January 2019 Kuniaki Otsuka1,2, Germaine Cornelissen2, Yutaka Kubo3, Koichi Shibata3, Koh Mizuno4,5, Accepted: 5 June 2019 Hiroshi Ohshima5, Satoshi Furukawa5 & Chiaki Mukai5 Published: xx xx xxxx Reports that aging slows down in space prompted this investigation of anti-aging efects in humans by analyzing astronauts’ heart rate variability (HRV). Ambulatory 48-hour electrocardiograms from 7 astronauts (42.1 ± 6.8 years; 6 men) 20.6 ± 2.7 days (ISS01) and 138.6 ± 21.8 days (ISS02) after launch were divided into 24-hour spans of relative lower or higher magnetic disturbance, based on geomagnetic measures in Tromso, Norway. Magnetic disturbances were signifcantly higher on disturbed than on quiet days (ISS01: 72.01 ± 33.82 versus 33.96 ± 17.90 nT, P = 0.0307; ISS02: 71.06 ± 51.52 versus 32.53 ± 27.27 nT, P = 0.0308). SDNNIDX was increased on disturbed days (by 5.5% during ISS01, P = 0.0110), as were other HRV indices during ISS02 (SDANN, 12.5%, P = 0.0243; Triangular Index, 8.4%, P = 0.0469; and TF-component, 17.2%, P = 0.0054), suggesting the action of an anti-aging or longevity efect. The efect on TF was stronger during light (12:00–17:00) than during darkness (0:00–05:00) (P = 0.0268). The brain default mode network (DMN) was activated, gauged by increases in the LF-band (9.7%, P = 0.0730) and MF1-band (9.9%, P = 0.0281). -
The Economic Impact of Critical National Infrastructure Failure Due to Space Weather
Natural Hazard Science, Oxford Research Encyclopaedia (ORE) The Economic Impact of Critical National Infrastructure Failure Due to Space Weather Edward J. Oughton1 1Centre for Risk Studies, Judge Business School, University of Cambridge, Cambridge, UK Corresponding author: Edward Oughton ([email protected]) 1 Natural Hazard Science, Oxford Research Encyclopaedia (ORE) Summary and key words Space weather is a collective term for different solar or space phenomena that can detrimentally affect technology. However, current understanding of space weather hazards is still relatively embryonic in comparison to terrestrial natural hazards such as hurricanes, earthquakes or tsunamis. Indeed, certain types of space weather such as large Coronal Mass Ejections (CMEs) are an archetypal example of a low probability, high severity hazard. Few major events, short time-series data and a lack of consensus regarding the potential impacts on critical infrastructure have hampered the economic impact assessment of space weather. Yet, space weather has the potential to disrupt a wide range of Critical National Infrastructure (CNI) systems including electricity transmission, satellite communications and positioning, aviation and rail transportation. Recently there has been growing interest in these potential economic and societal impacts. Estimates range from millions of dollars of equipment damage from the Quebec 1989 event, to some analysts reporting billions of lost dollars in the wider economy from potential future disaster scenarios. Hence, this provides motivation for this article which tracks the origin and development of the socio-economic evaluation of space weather, from 1989 to 2017, and articulates future research directions for the field. Since 1989, many economic analyses of space weather hazards have often completely overlooked the physical impacts on infrastructure assets and the topology of different infrastructure networks.