Space Weather: Storm from the Sun Booklet
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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 .......................................................................................................................... -
Analysis of Geomagnetic Storms in South Atlantic Magnetic Anomaly (SAMA)
Analysis of geomagnetic storms in South Atlantic Magnetic Anomaly (SAMA) Júlia Maria Soja Sampaio, Elder Yokoyama, Luciana Figueiredo Prado Copyright 2019, SBGf - Sociedade Brasileira de Geofísica Moreover, Dst and AE indices may vary according to the This paper was prepared for presentation during the 16th International Congress of the geomagnetic field geometry, such as polar to intermediate Brazilian Geophysical Society held in Rio de Janeiro, Brazil, 19-22 August 2019. latitudinal field variations. In this framework, fluctuations Contents of this paper were reviewed by the Technical Committee of the 16th in the geomagnetic field can occur under the influence of International Congress of the Brazilian Geophysical Society and do not necessarily represent any position of the SBGf, its officers or members. Electronic reproduction or the South Atlantic Magnetic Anomaly (SAMA). The SAMA storage of any part of this paper for commercial purposes without the written consent is a region of minimum geomagnetic field intensity values of the Brazilian Geophysical Society is prohibited. ____________________________________________________________________ at the Earth’s surface (Figure 1), and its dipole intensity is decreasing along the past 1000 years (Terra-Nova et. al., Abstract 2017). Geomagnetic storm is a major disturbance of Earth’s In this study we will compare the behavior of the types of magnetosphere resulted from the interaction of solar wind geomagnetic storms basis on AE and Dst indices. and the Earth’s magnetic field. This disturbance depends of the Earth magnetic field geometry, and varies in terms of intensity from the Poles to the Equator. This disturbance is quantified through geomagnetic indices, such as the Dst and the AE indices. -
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. -
Observations of Solar Wind Penetration Into the Earth's Magnetosphere: the Plasma Mantle
ENNIO R. SANCHEZ, CHING-I. MENG, and PATRICK T. NEWELL OBSERVATIONS OF SOLAR WIND PENETRATION INTO THE EARTH'S MAGNETOSPHERE: THE PLASMA MANTLE The large database provided by the continuous coverage of the Defense Meteorological Satellite Pro gram polar orbiting satellites constitutes an important source of information on particle precipitation in the ionosphere. This information can be used to monitor and map the Earth's magnetosphere (the cavity around the Earth that forms as the stream of particles and magnetic field ejected from the Sun, known as the solar wind, encounters the Earth's magnetic field) and for a large variety of statistical studies of its morphology and dynamics. The boundary between the magnetosphere and the solar wind is pre sumably open in some places and at some times, thus allowing the direct entry of solar-wind plasma into the magnetosphere through a boundary layer known as the plasma mantle. The preliminary results of a statistical study of the plasma-mantle precipitation in the ionosphere are presented. The first quan titative mapping of the ionospheric region where the plasma-mantle particles precipitate is obtained. INTRODUCTION Polar orbiting satellites are very useful platforms for studying the properties of the environment surrounding the Earth at distances well above the ionosphere. This article focuses on a description of the enormous poten tial of those platforms, especially when they are com bined with other means of measurement, such as ground-based stations and other satellites. We describe in some detail the first results of the kind of study for which the polar orbiting satellites are ideal instruments. -
The Van Allen Probes' Contribution to the Space Weather System
L. J. Zanetti et al. The Van Allen Probes’ Contribution to the Space Weather System Lawrence J. Zanetti, Ramona L. Kessel, Barry H. Mauk, Aleksandr Y. Ukhorskiy, Nicola J. Fox, Robin J. Barnes, Michele Weiss, Thomas S. Sotirelis, and NourEddine Raouafi ABSTRACT The Van Allen Probes mission, formerly the Radiation Belt Storm Probes mission, was renamed soon after launch to honor the late James Van Allen, who discovered Earth’s radiation belts at the beginning of the space age. While most of the science data are telemetered to the ground using a store-and-then-dump schedule, some of the space weather data are broadcast continu- ously when the Probes are not sending down the science data (approximately 90% of the time). This space weather data set is captured by contributed ground stations around the world (pres- ently Korea Astronomy and Space Science Institute and the Institute of Atmospheric Physics, Czech Republic), automatically sent to the ground facility at the Johns Hopkins University Applied Phys- ics Laboratory, converted to scientific units, and published online in the form of digital data and plots—all within less than 15 minutes from the time that the data are accumulated onboard the Probes. The real-time Van Allen Probes space weather information is publicly accessible via the Van Allen Probes Gateway web interface. INTRODUCTION The overarching goal of the study of space weather ing radiation, were the impetus for implementing a space is to understand and address the issues caused by solar weather broadcast capability on NASA’s Van Allen disturbances and the effects of those issues on humans Probes’ twin pair of satellites, which were launched in and technological systems. -
Transmittal of Geotail Prelaunch Mission Operation Report
National Aeronautics and Space Administration Washington, D.C. 20546 ss Reply to Attn of: TO: DISTRIBUTION FROM: S/Associate Administrator for Space Science and Applications SUBJECT: Transmittal of Geotail Prelaunch Mission Operation Report I am pleased to forward with this memorandum the Prelaunch Mission Operation Report for Geotail, a joint project of the Institute of Space and Astronautical Science (ISAS) of Japan and NASA to investigate the geomagnetic tail region of the magnetosphere. The satellite was designed and developed by ISAS and will carry two ISAS, two NASA, and three joint ISAS/NASA instruments. The launch, on a Delta II expendable launch vehicle (ELV), will take place no earlier than July 14, 1992, from Cape Canaveral Air Force Station. This launch is the first under NASA’s Medium ELV launch service contract with the McDonnell Douglas Corporation. Geotail is an element in the International Solar Terrestrial Physics (ISTP) Program. The overall goal of the ISTP Program is to employ simultaneous and closely coordinated remote observations of the sun and in situ observations both in the undisturbed heliosphere near Earth and in Earth’s magnetosphere to measure, model, and quantitatively assess the processes in the sun/Earth interaction chain. In the early phase of the Program, simultaneous measurements in the key regions of geospace from Geotail and the two U.S. satellites of the Global Geospace Science (GGS) Program, Wind and Polar, along with equatorial measurements, will be used to characterize global energy transfer. The current schedule includes, in addition to the July launch of Geotail, launches of Wind in August 1993 and Polar in May 1994. -
National Space Weather Program Implementation Plan, 2Nd Edition, July 2000
National Space Weather Program Implementation Plan, 2nd Edition, July 2000 http://www.ofcm.gov/ The National Space Weather Program The Implementation Plan 2nd Edition July 2000 National Space Weather Program Implementation Plan, 2nd Edition, July 2000 http://www.ofcm.gov/ NATIONAL SPACE WEATHER PROGRAM COUNCIL Mr. Samuel P. Williamson, Chairman Federal Coordinator Dr. David L. Evans Department of Commerce Colonel Michael A. Neyland, USAF Department of Defense Mr. Robert E. Waldron Department of Energy Mr. James F. Devine Department of the Interior Mr. David Whatley Department of Transportation Dr. Edward J. Weiler National Aeronautics and Space Administration Dr. Margaret S. Leinen National Science Foundation Lt Col Michael R. Babcock, USAF, Executive Secretary Office of the Federal Coordinator for Meteorological Services and Supporting Research National Space Weather Program Implementation Plan, 2nd Edition, July 2000 http://www.ofcm.gov/ NATIONAL SPACE WEATHER PROGRAM Implementation Plan 2nd Edition Prepared by the Committee for Space Weather for the National Space Weather Program Council Office of the Federal Coordinator for Meteorology FCM-P31-2000 Washington, DC July 2000 National Space Weather Program Implementation Plan, 2nd Edition, July 2000 http://www.ofcm.gov/ National Space Weather Program Implementation Plan, 2nd Edition, July 2000 http://www.ofcm.gov/ FOREWORD We are pleased to present this Second Edition of the National Space Weather Program Implementation Plan. We published the program's Strategic Plan in 1995 and the first Implementation Plan in 1997. In the intervening period, we have made tremendous progress toward our goals but much work remains to be accomplished to achieve our ultimate goal of providing the space weather observations, forecasts, and warnings needed by our Nation. -
THEMIS Telescope Images Analysed for Space Weather Traces
EPSC Abstracts Vol. 14, EPSC2020-1022, 2020 https://doi.org/10.5194/epsc2020-1022 Europlanet Science Congress 2020 © Author(s) 2021. This work is distributed under the Creative Commons Attribution 4.0 License. THEMIS telescope images analysed for space weather traces Melinda Dósa1, Valeria Mangano2, Zsofia Bebesi1, Stefano Massetti2, Anna Milillo2, and Anna Görgei3 1Wigner Research Centre for Physics, Space Physics and Space Technology, Budapest, Hungary ([email protected]) 2INAF/IAPS, Istituto Nazionale di Astrofisica, Roma, Italy 3Eötvös Loránd University, Institute of Physics The THEMIS solar telescope operating on Tenerife (Canary islands) has observed Mercury’s Na exosphere along several campaigns since 2007. A dataset of images taken between 2009 and 2013 are analysed here in relation with propagated solar wind data. A small subset of the images shows a low level of correlation between Na-emission and solar wind dynamic pressure. The amount of data at present is not sufficient to make a clear statement on whether the correlation is a coincidence or can be explained by other factors (position of Mercury and Earth, solar activity, etc.). Nevertheless, the authors present a comprehensive study taking into account all possible factors. Sodium plays a special role in Mercury’s exosphere: due to its strong resonance line it has been observed and monitored by Earth-based telescopes for decades. Different and highly variable patterns of Na-emission have been identified, the most common and recurrent being the high latitude double-peak pattern [1]. It is clear that the exosphere is linked to the surface and influenced by the interstellar medium and the solar wind deviated by the magnetosphere, but the role and weight of the single processes are still under discussion [2]. -
On Magnetic Storms and Substorms
ILWS WORKSHOP 2006, GOA, FEBRUARY 19-24, 2006 On magnetic storms and substorms G. S. Lakhina, S. Alex, S. Mukherjee and G. Vichare Indian Institute of Geomagnetism, New Panvel (W), Navi Mumbai-410218, India Abstract. Magnetospheric substorms and storms are indicators of geomagnetic activity. Whereas the geomagnetic index AE (auroral electrojet) is used to study substorms, it is common to characterize the magnetic storms by the Dst (disturbance storm time) index of geomagnetic activity. This talk discusses briefly the storm-substorms relationship, and highlights some of the characteristics of intense magnetic storms, including the events of 29-31 October and 20-21 November 2003. The adverse effects of these intense geomagnetic storms on telecommunication, navigation, and on spacecraft functioning will be discussed. Index Terms. Geomagnetic activity, geomagnetic storms, space weather, substorms. _____________________________________________________________________________________________________ 1. Introduction latitude magnetic fields are significantly depressed over a Magnetospheric storms and substorms are indicators of time span of one to a few hours followed by its recovery geomagnetic activity. Where as the magnetic storms are which may extend over several days (Rostoker, 1997). driven directly by solar drivers like Coronal mass ejections, solar flares, fast streams etc., the substorms, in simplest terms, are the disturbances occurring within the magnetosphere that are ultimately caused by the solar wind. The magnetic storms are characterized by the Dst (disturbance storm time) index of geomagnetic activity. The substorms, on the other hand, are characterized by geomagnetic AE (auroral electrojet) index. Magnetic reconnection plays an important role in energy transfer from solar wind to the magnetosphere. Magnetic reconnection is very effective when the interplanetary magnetic field is directed southwards leading to strong plasma injection from the tail towards the inner magnetosphere causing intense auroras at high-latitude nightside regions. -
Cmes, Solar Wind and Sun-Earth Connections: Unresolved Issues
CMEs, solar wind and Sun-Earth connections: unresolved issues Rainer Schwenn Max-Planck-Institut für Sonnensystemforschung, Katlenburg-Lindau, Germany [email protected] In recent years, an unprecedented amount of high-quality data from various spaceprobes (Yohkoh, WIND, SOHO, ACE, TRACE, Ulysses) has been piled up that exhibit the enormous variety of CME properties and their effects on the whole heliosphere. Journals and books abound with new findings on this most exciting subject. However, major problems could still not be solved. In this Reporter Talk I will try to describe these unresolved issues in context with our present knowledge. My very personal Catalog of ignorance, Updated version (see SW8) IAGA Scientific Assembly in Toulouse, 18-29 July 2005 MPRS seminar on January 18, 2006 The definition of a CME "We define a coronal mass ejection (CME) to be an observable change in coronal structure that occurs on a time scale of a few minutes and several hours and involves the appearance (and outward motion, RS) of a new, discrete, bright, white-light feature in the coronagraph field of view." (Hundhausen et al., 1984, similar to the definition of "mass ejection events" by Munro et al., 1979). CME: coronal -------- mass ejection, not: coronal mass -------- ejection! In particular, a CME is NOT an Ejección de Masa Coronal (EMC), Ejectie de Maså Coronalå, Eiezione di Massa Coronale Éjection de Masse Coronale The community has chosen to keep the name “CME”, although the more precise term “solar mass ejection” appears to be more appropriate. An ICME is the interplanetry counterpart of a CME 1 1. -
Radiation Belt Storm Probes Launch
National Aeronautics and Space Administration PRESS KIT | AUGUST 2012 Radiation Belt Storm Probes Launch www.nasa.gov Table of Contents Radiation Belt Storm Probes Launch ....................................................................................................................... 1 Media Contacts ........................................................................................................................................................ 4 Media Services Information ..................................................................................................................................... 5 NASA’s Radiation Belt Storm Probes ...................................................................................................................... 6 Mission Quick Facts ................................................................................................................................................. 7 Spacecraft Quick Facts ............................................................................................................................................ 8 Spacecraft Details ...................................................................................................................................................10 Mission Overview ...................................................................................................................................................11 RBSP General Science Objectives ........................................................................................................................12 -
Polar Observations of Electron Density Distribution in the Earth's
c Annales Geophysicae (2002) 20: 1711–1724 European Geosciences Union 2002 Annales Geophysicae Polar observations of electron density distribution in the Earth’s magnetosphere. 1. Statistical results H. Laakso1, R. Pfaff2, and P. Janhunen3 1ESA Space Science Department, Noordwijk, Netherlands 2NASA Goddard Space Flight Center, Code 696, Greenbelt, MD, USA 3Finnish Meteorological Institute, Geophysics Research, Helsinki, Sweden Received: 3 September 2001 – Revised: 3 July 2002 – Accepted: 10 July 2002 Abstract. Forty-five months of continuous spacecraft poten- Key words. Magnetospheric physics (magnetospheric con- tial measurements from the Polar satellite are used to study figuration and dynamics; plasmasphere; polar cap phenom- the average electron density in the magnetosphere and its de- ena) pendence on geomagnetic activity and season. These mea- surements offer a straightforward, passive method for mon- itoring the total electron density in the magnetosphere, with high time resolution and a density range that covers many 1 Introduction orders of magnitude. Within its polar orbit with geocentric perigee and apogee of 1.8 and 9.0 RE, respectively, Polar en- The total electron number density is a key parameter needed counters a number of key plasma regions of the magneto- for both characterizing and understanding the structure and sphere, such as the polar cap, cusp, plasmapause, and auroral dynamics of the Earth’s magnetosphere. The spatial varia- zone that are clearly identified in the statistical averages pre- tion of the electron density and its temporal evolution dur- sented here. The polar cap density behaves quite systemati- ing different geomagnetic conditions and seasons reveal nu- cally with season. At low distance (∼2 RE), the density is an merous fundamental processes concerning the Earth’s space order of magnitude higher in summer than in winter; at high environment and how it responds to energy and momentum distance (>4 RE), the variation is somewhat smaller.