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Multi-Instrument Space-Borne Observations and Validation of the Physical Model of the Lithosphere-Atmosphere-Ionosphere-Magnetosphere Coupling
Multi-instrument space-borne observations and validation of the physical model of the Lithosphere-Atmosphere-Ionosphere-Magnetosphere Coupling Abstract We propose an investigation of the near-Earth space plasma dynamics and electromagnetic environment by multiparameter analysis from variety of space-based missions and creation of physical model of the coupling between lithosphere, atmosphere, ionosphere and magnetosphere which are linked by the chain of processes initiated by atmospheric boundary layer modification by air pollution (dust aerosols, nuclear disaster) and modification of boundary layer by major natural disasters: earthquakes, tsunamis, hurricanes/typhoons and volcanoes. Our intention is to find from experimental data and their detailed analysis the key processes in atmosphere, which modify the Earth plasma environment system under various geophysical conditions including natural and anthropogenic disasters. As input for analysis and modeling we will use the data products about atmosphere, ionosphere and magnetosphere from different satellites, including NASA EOS (TERRA, AQUA), NOAA/POES, and ESA/ EUMETSAT (METEOSAT, ENVISAT, SWARM), DEMETER/CNES, FORMOSAT-3/COSMIC, as well as ground observations of GPS/TEC, ground electromagnetic (EM) fields meteorological monitoring data, geochemistry, etc. Statistical studies that use these data sets individually have already proven the complex nature of the interconnection between lithosphere and atmosphere events and earth space environment through the Global Electric Circuit. Just recently the members of this team came independently to same conclusion that many processes in atmosphere of different origin create the similar variations in the space plasma environment what implies the existence of common physical mechanism of their generation. One of the main drivers for such coupling is the change of the boundary layer conductivity through the air pollution, Ion Induced Nucleation triggered by natural and anthropogenic radioactivity, and mesoscale atmospheric systems such as tropical hurricanes/typhoons. -
Space in Central and Eastern Europe
EU 4+ SPACE IN CENTRAL AND EASTERN EUROPE OPPORTUNITIES AND CHALLENGES FOR THE EUROPEAN SPACE ENDEAVOUR Report 5, September 2007 Charlotte Mathieu, ESPI European Space Policy Institute Report 5, September 2007 1 Short Title: ESPI Report 5, September 2007 Editor, Publisher: ESPI European Space Policy Institute A-1030 Vienna, Schwarzenbergplatz 6 Austria http://www.espi.or.at Tel.: +43 1 718 11 18 - 0 Fax - 99 Copyright: ESPI, September 2007 This report was funded, in part, through a contract with the EUROPEAN SPACE AGENCY (ESA). Rights reserved - No part of this report may be reproduced or transmitted in any form or for any purpose without permission from ESPI. Citations and extracts to be published by other means are subject to mentioning “source: ESPI Report 5, September 2007. All rights reserved” and sample transmission to ESPI before publishing. Price: 11,00 EUR Printed by ESA/ESTEC Compilation, Layout and Design: M. A. Jakob/ESPI and Panthera.cc Report 5, September 2007 2 EU 4+ Executive Summary ....................................................................................... 5 Introduction…………………………………………………………………………………………7 Part I - The New EU Member States Introduction................................................................................................... 9 1. What is really at stake for Europe? ....................................................... 10 1.1. The European space community could benefit from a further cooperation with the ECS ................................................................. 10 1.2. However, their economic weight remains small in the European landscape and they still suffer from organisatorial and funding issues .... 11 1.2.1. Economic weight of the ECS in Europe ........................................... 11 1.2.2. Reality of their impact on competition ............................................ 11 1.2.3. Foreign policy issues ................................................................... 12 1.2.4. Internal challenges ..................................................................... 12 1.3. -
In 1938-39. the ·Meteorological Depar~Ment
DGO. 28. 89 620 - Report on the Administration of the Meteorological Department of the Government of India in 1938-39. the ·Meteorological Depar~ment_ . ~ . of the · Government : of India • in 1938-39. , PUBLISIIB:D B1' 'I'D MANAGD or PtriiLicATJONS) Du.a1. PamuD Jl'l' I'D lbNACu, Govmx~Dm' w hmu Puss~ Nrw DELHI. 1939. List of Agenca 111 India from whom Government ol India Publications are available. (II) PnoVIKCIAL GOVU..'QlBXT BOOK DIIPO'l'S. Alan: :-supertntenclea~ Allam SeeRtarlDt Press, 8hlllonc. Bm&& :-BuperlnteDdeat, Go¥erament Prtntfna:, P. 0. Gnl&arb&Rll, Patna. Bo• ...Y :-Bnpadotendent, Government Prlnti.DI and StaUonery, Qnceo'a Road, BombQ'. Ol!fTB&L PIIO'nlfOIB :-Superintendent, Oovnm:nont Prlntlq, Central Provinces, Nagpar Ka.ollAB :-Snperlotendeot, Government PreA, Mount Itoad, lladru. Ro&TII•WMI' homn PBovtlfOB :-Manager, Government Pr1nUng Gnd StatlonorJ', Peshawar.. OIU8U. :-PRW OBlctr, Secretariat, Cutt«k. PUKIAB :-superlateodtnt, Oovtmmrnt Printing, PunJab, Lahore. 81110 :-lfanacer, B!acl Government Boqlc Depot and l!Ccord Qmce, Karacld (S&dar), UIIITID PROYI!fOBS :-superintendent, Printing and Stationery, tJ, P., Allahabad. (b) PRIVATE DoOE.•IEU.US. Advanl & co~ The Mall, oawupore. r.ya11 Book nepot, Lynnpote. - Aero StorDI!!. 1\.ara.chl.• Malhn:ra ..t Co., Post !'ox No. O.t, l.Ahnre;l'tc:~sll!. U. P, Army Unaketry StorOI, l[t)~:'l (PUnJib).t l~Mhur & Co.. Mesua. B. &. Chaf.ur-VUu hote., Civil lbnthlya & Co. Ltd. S&al.lut• ltoad, Almer. Lines, J'odhpur (B4Jprttanr.). Bonq.::Ll flyhut 6tu~J. 'Dum Duro Caolt.• Mlnen-:t Book. Shop, Aon.rkull Street, Labore. Blunvn!l.nl ,t Sor1,, New Delhi. -
Extreme Space Weather Events of Colaba: Estimation of Interplanetary Conditions
Extreme Space Weather events of Colaba: Estimation of interplanetary conditions. B. Veenadhari Sandeep Kumar, S.Tulasiram, Selvakumaran S. Mukherjee, Rajesh Singh, B. D. Kadam Indian Institute of Geomagnetism, Navi Mumbai, India. SCOSTEP-WDS Workshop, 27-30 October, 2015 Tokyo, Japan Out line WDC- Mumbai : Activities Colaba - Bombay old magnetic records Extreme Space weather events – Geomagnetic storms Solar and Interplanetary drivers, estimation of interplanetary conditions. Some characteristics of Severe magnetic storms of solar cycle 23 summary Colaba observatory, Bombay 1846‐1904 Indian magnetic observatory at Alibag, established in 1904…. History of Geomagnetism in India The Indian Institute of Geomagnetism (IIG) is a premier research Institute actively engaged in basic and applied Colaba Observatory research in Geomagnetism and allied fields, is the successor to COLABA-ALIBAG observatories. The Colaba observatory was built at one of the original islands of Mumbai, to support British navigation and shipping interest at its thriving port. The Observatory was set up in 1826; though the regular Geomagnetism and Meteorological measurements were started here in 1841. The Colaba-Alibag observatory has the distinction of having an uninterrupted record of magnetic data since 1841, and the only such observatory in the world. During (1846-1872) only eye observations were taken and recorded at Colaba whereas photographic recordings of the variations in magnetic elements and absolute observations started between 1872 -1906. World Data Center- Geomagnetism, Mumbai The World Data Centre for Geomagnetism (WDCG), Mumbai was the first World Data Centre in India during 1971 as WDC-C2 (India and Japan) in Asian region as part of World Data Centre system (WDC System) by ICSU. -
Index of Astronomia Nova
Index of Astronomia Nova Index of Astronomia Nova. M. Capderou, Handbook of Satellite Orbits: From Kepler to GPS, 883 DOI 10.1007/978-3-319-03416-4, © Springer International Publishing Switzerland 2014 Bibliography Books are classified in sections according to the main themes covered in this work, and arranged chronologically within each section. General Mechanics and Geodesy 1. H. Goldstein. Classical Mechanics, Addison-Wesley, Cambridge, Mass., 1956 2. L. Landau & E. Lifchitz. Mechanics (Course of Theoretical Physics),Vol.1, Mir, Moscow, 1966, Butterworth–Heinemann 3rd edn., 1976 3. W.M. Kaula. Theory of Satellite Geodesy, Blaisdell Publ., Waltham, Mass., 1966 4. J.-J. Levallois. G´eod´esie g´en´erale, Vols. 1, 2, 3, Eyrolles, Paris, 1969, 1970 5. J.-J. Levallois & J. Kovalevsky. G´eod´esie g´en´erale,Vol.4:G´eod´esie spatiale, Eyrolles, Paris, 1970 6. G. Bomford. Geodesy, 4th edn., Clarendon Press, Oxford, 1980 7. J.-C. Husson, A. Cazenave, J.-F. Minster (Eds.). Internal Geophysics and Space, CNES/Cepadues-Editions, Toulouse, 1985 8. V.I. Arnold. Mathematical Methods of Classical Mechanics, Graduate Texts in Mathematics (60), Springer-Verlag, Berlin, 1989 9. W. Torge. Geodesy, Walter de Gruyter, Berlin, 1991 10. G. Seeber. Satellite Geodesy, Walter de Gruyter, Berlin, 1993 11. E.W. Grafarend, F.W. Krumm, V.S. Schwarze (Eds.). Geodesy: The Challenge of the 3rd Millennium, Springer, Berlin, 2003 12. H. Stephani. Relativity: An Introduction to Special and General Relativity,Cam- bridge University Press, Cambridge, 2004 13. G. Schubert (Ed.). Treatise on Geodephysics,Vol.3:Geodesy, Elsevier, Oxford, 2007 14. D.D. McCarthy, P.K. -
The History and Future of Space Weather Forecasting
The History and Future of Space Weather Dr. Thomas Berger NOAA Space Weather Prediction Center HAO 75th Anniversary September 2, 2015 18th and 19th Century The Subject: Aurora Borealis Geodetic Expedition to Lapland Pierre Maupertuis, 1736 A Treatise on Meteorology Elias Loomis, 1868 1580 Augsburg, Germany 17-March-2015 ©Joe McCabe 22-January-2012 Aurorae are linked to terrestrial “Magnetic Storms” Kew Observatory, London, 1859 1852: Edward Sabine asserts that magnetic storms are correlated with sunspots... ...but there was no physical mechanism to explain a magnetic storm on Earth originating at the Sun. Then on the morning of September 1st, 1859... Redhill, Surrey, England Richard Carrington records the first known “white light flare” 1826 — 1875 September 1st, 1859 11:20 am local time A sudden magnetic jump was later found at exactly the same time… Kew Observatory, London, September 1st 1859 ...and approximately 17.5 hrs later, a HUGE magnetic storm commenced: Kew Observatory, London, September 2nd 1859 The storm was detected all over the world... Colaba Observatory, Bombay, India September 1—3 1859 …and auroral displays were observed as far south as Honolulu and Venezuela. “The red light was so vivid that the roofs of the houses and the leaves of the trees appeared as if covered with “The red light was so vivid that the roofs of the houses and the leaves of the trees appeared as if covered with blood” Report of the aurora seen in San Salvador, September 2, 1859 1861: Balfour Stewart proposes a link between Carrington’s observation and the geomagnetic storm. If no connexion had been known to subsist between these two classes of phenomena, it would, perhaps, be wrong to consider this “.. -
Ukrainian-Presentation.Pdf
AERONAUTICSAERONAUTICS ANDAND AEROSPACEAEROSPACE ACHIEVEMENTSACHIEVEMENTS ANDAND RESEARCHESRESEARCHES ININ UKRAINEUKRAINE AIR TRANSPORT NETWORK Conference on International Aerospace London, 13 – 14 March, 2008 Prof. A. Zbrutsky Dean of Aerospace Systems Faculty NTUU “Kyiv Polytechnic Institute ” STRUCTURESTRUCTURE ► 1. Space industry ► 2. Aeronautics ► 3. Universities SpaceSpace industryindustry ofof UkraineUkraine History During 40 years of space era: developed 5 types of launch vehicles (Kosmos, Interkosmos,Cyclone-2, Cyclone-3, Zenit) developed and launched more than 400 satellites for astrophysical and global research and the Earth remote sensing developed four generations of combat strategic missile systems produced more than 10 000 ballistic missiles that ensured parity in cold war Participated almost in every most important space projects of the USSR: Launch of the first Earth satellite First human flight to space Programs of flights to the Moon and Solar system planets Interkosmos international program Launch of Salut and Mir orbital stations Development of Energiya-Buran Space Launch System Organization of Ukrainian Space Industry National Space Agency of Ukraine Manufacturing enterprises Research institutes and design offices Specialized Enterprises • PA Makarov “Yuzhmash” Plant • Yuzhnoye State Design Office • National Space Facilities • Arsenal Plant, State Enterprise • Arsenal Central Design Office, State Control and Test Center • Khartron Public Company; Enterprise • National Youth Aerospace • PA Komunar • Ukrainian Engineering -
40 Ans De Coopération Spatiale Franco-Russe
#4 - octobre 2008 DOSSIER : 40 ANS DE COOPERATION FRANCO-RUSSE ESPACE & TEMPS Le mot du président IFHE Institut Français d’Histoire de l’Espace adresse de correspondance : 2, place Maurice Quentin Voici le quatrième numéro de notre bulletin avec, comme cela est 75039 Paris Cedex 01 le cas depuis deux ans, il a pris de l’embonpoint en passant de Tél : 01 40 39 04 77 22 à 32 pages. Dans le numéro précédent de février 2008, nous avions traité du L’institut Français d’Histoire de l’Espace (IFHE) est une 50e anniversaire du premier satellite américain et du 30e anni - association selon la Loi de 1901 créée le 22 mars 1999 qui versaire du satellite Météosat. Cette fois, nous avons consacré s’est fixée pour obiectifs de valoriser l’histoire de l’espace l’essentiel du numéro au 40e anniversaire de la coopération et de participer à la sauvegarde et à la préservation du franco-russe qui avait fait l’objet d’un important colloque à Moscou en octobre 2006. J’avais été invité par le Cnes à cet patrimoine documentaire. Il est administré par un Conseil, évènement historique. A l’époque, l’IFHE n’avait pas eu la pos - et il s’est doté d’un Conseil Scientifique. sibilité de le traiter sous la forme d’une conférence ou d’un col - loque comme ce fut la cas pour la coopération franco-améri - Conseil d’administration caine en décembre 2005. Il m’a donc semblé naturel publier ce Président d’honneur....... Michel Bignier dossier qui présente le contenu de la plupart des interventions Président................... -
5 Orbit and Ground Track of a Satellite
5 Orbit and Ground Track of a Satellite 5.1 Position of the Satellite on its Orbit Let (O; x, y, z) be the Galilean reference frame already defined. The satellite S is in an elliptical orbit around the centre of attraction O. The orbital plane P makes a constant angle i with the equatorial plane E. However, although this plane P is considered as fixed relative to in the Keplerian motion, in a real (perturbed) motion, it will in fact rotate about the polar axis. This is precessional motion,1 occurring with angular speed Ω˙ , as calculated in the last two chapters. A schematic representation of this motion is given in Fig. 5.1. We shall describe the position of S in using the Euler angles. 5.1.1 Position of the Satellite The three Euler angles ψ, θ and χ were introduced in Sect. 2.3.2 to specify the orbit and its perigee in space. In the present case, we wish to specify S. We obtain the correspondence between the Euler angles and the orbital elements using Fig. 2.1: ψ = Ω, (5.1) θ = i, (5.2) χ = ω + v. (5.3) Although they are fixed for the Keplerian orbit, the angles Ω, ω and M − nt vary in time for a real orbit. The inclination i remains constant, however. The distance from S to the centre of attraction O is given by (1.41), expressed in terms of the true anomaly v : a(1 − e2) r = . (5.4) 1+e cos v 1 The word ‘precession’, meaning ‘the action of preceding’, was coined by Coper- nicus around 1530 (præcessio in Latin) to speak about the precession of the equinoxes, i.e., the retrograde motion of the equinoctial points. -
A Small Biography of Alshashtri Jambhekar
A Small Biography of R.M. Khaladkar 17/5, Shindenagar, Bavdhan (Khurd), Alshashtri Jambhekar NDA Road, Pune – The First Indian who Headed E-mail: [email protected] the Colaba Observatory The Colaba observatory was established by the below in order that it would provide information and East India Company in 1826 for astronomical inspiration to many of our colleagues of the present observations and time keeping services for and the coming generations. Bombay (Mumbai) port. The geomagnetism and meteorological measurements started in 1841 Early life th by Prof. Orlebar who was then the Professor of He was born on 6 January 1812 in a remote natural philosophy (science) at the Elphinstone village- Pombhurle in Sindhudurg district of Konkan college. However, in 1842 he had to go on the region, Maharashtra. After primary education in medical leave for two years. During this period, Marathi and Sanskrit, he shifted to Mumbai at age one Indian luminary - Balshashtri Jambhekar (BJ) 13. There, he excelled in many fields as fast as it was appointed as the Head of this observatory. was almost impossible for any other person, Considering the fact that at that time, most of the especially when the educational institutions, means top positions in India were occupied by the of knowledge like books, newspapers were not Britishers, exceptionally a great honour was available in India as they are today. bestowed upon this young Indian at an age of just Subjects and languages mastered by BJ 31 years. Undoubtedly, it was because of his When most of the population of India was proven merits in the scientific field. -
Solar Physics Research in the Russian Subcontinent - Current Status and Future
Asian Journal of Physics Vol. 29 No. xx (2016) xxx - xxx Solar Physics Research in the Russian Subcontinent - Current Status and Future Alexei A. Pevtsov1, Yury A. Nagovitsyn2, Andrey G. Tlatov3, Mikhail L. Demidov4 1 National Solar Observatory, Sunspot, NM 88349, USA 2 The Main (Pulkovo) Astronomical Observatory, Russian Academy of Sciences, Pulkovskoe sh. 65, St. Petersburg, 196140 Russian Federation 3 Kislovodsk Solar Station of Pulkovo Observatory, PO Box 145, Gagarina Str., 100, Kislovodsk, 357700 Russian Federation 4 Institute of Solar-Terrestrial Physics SB RAS, 664033, Irkutsk, P.O. Box 291, Russian Federation Abstract: Modern research in solar physics in Russia is a multifaceted endeavor, which includes multi-wavelength observations from the ground- and space-based instruments, extensive theoretical and numerical modeling studies, new instrument development, and cross-disciplinary and international research. The research is conducted at the research organizations under the auspices of the Russian Academy of Sciences and to a lesser extent, by the research groups at Universities. Here, we review the history of solar physics research in Russia, and provide an update on recent develop- ments. Qc Anita Publications. All rights reserved 1Introduction The research in solar physics in Russia and countries that until early 1990th were part of Soviet Union has strong historical roots. Thus, for example, there are historical records of naked eyed observations of sunspots through the haze of the forest ¿UHV in 1365 and 1371 (see [1]). The Novgorod Chronicles also contain a description of about 40 solar eclipses between 1064 and 1567 over the what is now a European part of Russia and the Northern Scandinavia. -
Applied Information Systems Research Program (AISRP
NASA-CR-199103 Applied Information Systems Research Program OD ¢_ (AISRP) I N O -.O l'q _ t,n I'o I I I -- c,4 i¢_ I-- i¢_ 1,2 ,,(3 O O Workshop III r_j Meeting Proceedings Laboratory for Atmospheric and Space Physics University of Colorado Boulder, Colorado August 3-6, 1993 Proceedings Issued By: Information Systems Branch Office of Space Science NASA Headquarters APPLIED INFORMATION SYSTEMS RESEARCH PROGRAM WORKSHOP HI FINAL REPORT TABLE OF CONTENTS Executive Summary 5d_ ........ Opening Remarks [Bredekamp] An Overview of the Software Support Laboratory [Davis] 8 ARTIFICIAL INTELLIGENCE TECHNIQUES SESSION Holographic Neural Networks for Space and Commercial Applications [Liu] 9 The SEIDAM (System of Experts for Intelligent Data Management) Project [Goodenough] 10 SIGMA: An Intelligent Model-Building Assistant [Keller] 10 Multivariate Statistical Analysis Software Technologies for Astrophysical Research Involving Large Databases [Djorgovski] 11 SCIENTIFIC VISUALIZATION SESSION The Grid Analysis and Display System (GRADS): A Practical Tool for Earth Science Visualization [Kinter] 13 A Distributed Analysis and Visualization System for Model and Observational Data [Wilhelmson] 13 Handling Intellectual Property at UCAR/NCAR [Buzbee] 14 NCAR Graphics - What's New in 3.2? [Lackman] 15 MclDAS-eXplorer: A Version of MclDAS-X for Planetary Applications [Limaye] 15 Experimenter's Laboratory for Visualized Interactive Science (ELVIS) [Hansen] 16 SAVS: A Space and Atmospheric Visualization Science System [Szuszczewicz] 17 TABLE OF CONTENTS(continued)