S-lOO 44 Stockholm, Sweden
|
|
- Joel Marshall
- 8 years ago
- Views:
Transcription
1 LIST OF PARTICIPANTS Akasofu, S-I Alfven, H Andersson, L E d'angelo, N Ashour-Abda11a, M Axford, W I Block, L Borg, H Bostrom, R Brunberg, E-l\. Bryant, D A Christophersen, P Derblom, H Dungey, J W Dysthe, K Egeland, A Eliasson, L Evans, D S Fahleson, D U Fiil thammar, C-G Galeev, A A Gendrin, R Gustafsson, G Geophysical Institute, Fairbanks, Alaska 99701, USA S-lOO 44 Stockholm 70, Danish Space Research Institute, Lundtoftevej 7, DK-2800 Lyngby, Denmark Centre National d'etudes des Telecommunications, F Issy-1es-Moulineauz, France Max-Planck-Institut fur Aeronomie, Postfach 60, D-3411 Lindau/Harz, Germany Inst. for mekanik, Kungl. Tekniska Hogskolan, S-lOO 44 Stockholm 70, S-lOO 44 Stockholm 70, S-lOO 44 Stockholm 70, Appleton Laboratory, Ditton Park, Slough SL3 9 JX, England Uppsala Jonosfarobservatorium, S Uppsala, Imperial College, Department of Physics, Prince Consort Road, London S W 7. England Tromso Universitet, N-9001 Det Norske Institutt for Kosmisk Fysikk, Postboks 1048, Blindern, Oslo 3, Norway Inst. for geokosmofysik, Umea universitet, Kiruna geofysiska institut, Umea, Space Environment Lab., NOAA Environment Res. Lab., Boulder, Colorado 80302, USA S-lOO 44 Stockholm 70, S-lOO 44 Stockholm, Space Research Institute, Academy of Sciences of USSR, Moscow Region, USSR Groupe Recherches Ionospherique, CNET 3 Av de la Republique, 92-Issy-les-Moulineaux, France T r o m s ~ N o r w a J 363
2 364 Haerendel, G Heikkila, W J Holmgren, L-A Holt, 0 Hones Jr, E W Hultqvist, B Johnson, R G Juren, C Kennel, C F Lundin, R Maehlum., B McIlwain, C E Mozer, F S Riedler, W Rossberg, L Ronrunark, K Sagdeev, R Z Scarf, F L Smith, P Stenflo, L S raas, F PARTICIPANTS Max-Planck-Institut fur Physik und Astrophysik, Institut fur Extraterrestrische Physik, D-8046 Garching b MUnchen, Germany University of Texas at Dallas, POBox 688, Richardson, Texas 75080, USA Tromso Universitet, POBox 387, N-9001 Tromso, Norway Los Alamos Scientific Lab., Los Alamos, New Mexico 87544, USA Lockheed Palo Alto Research Lab., Palo Alto, California 94304, USA Plasma Physics Group, Department of Physics, University of California, Los Angeles, California 90025, USA Forsvarets Forskingsinstitutt, Avd for elektronikk, Postboks 25, 2007 Kjeller, Norway Physics Dept, Univ. of Calif., San Diego, La Jolla, California 92037, USA Physics Dept. and Space Science Lab., Univ. of Calif., Berkley, California 94820, USA Institut fur Nachrichtentechnik, Technische Hochschule Graz, Inffeldgasse 12, A-8010 Graz, Austria Max-Planck-Institut fur Aeronomie, Postfach 60, D-3411 Lindau/Harz, Germany Avd. for teoretisk plasmafysik, Umea universitet, Kiruna geofysiska institut, S Umea, Space Research Institute, Academy of Sciences of USSR, Moscow Region, USSR Space Sciences Department, TRW System Group, Redondo Beach, California 90278, USA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA Avd. for teoretisk plasmafysik, Umea universitet, S Umea, Fysisk Institutt avd A, Universitetet i Bergen, Allegaten 53/55, N-5014 Bergen U, Norway
3 PARTICIPANTS Vasyliunas, V M Westerlund, S Westin, H Whalen, B A Williams, D Department of Physics and Center for Space Research,Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA Division of Physics, National Research Council of Canada, Ottawa, Ontario, Canada Space Environment Lab. NOAA Environment Research Lab. R43, Boulder, Colorado 80302, USA 36S
4 SUBJECT INDEX Acceleration, 187, 229, 251, 271, 291, 305, 319, 320, 325 Adiabatic processes, 170, 251 Anomalous resistivity, 1, 65, 76, 187, 196, 202, 233, 240, 252, 271, 284, 360 ATS-6 satellite, 92, 273 Auroral currents, 13, 14 Auroral electrojets, 2, 113, 129 Auroral particles, 92, 319 Barium ions, 148 Birkeland currents, 2, 229, 240, 341,359 Bohm condition, 235 Boundaries, 69, 79, 85, 341 Charge exchange, 168 Collapse, 263 Conductivity, 5, 81, 243, 342, 361 Convection, 13, 39, 148, 149, 251, 352 Cosmogonic problem, 16 Coulomb scattering, 176 Current disruption, 1 Diffuse auroras, 127 Diffusion coefficient, 174 Dipole field, 8, 352 Discrete auroras, 127 Dispersion relations, 206, 214, 265 Dissipation, 76, 251 DMSP-2 satellite, 113 Double layer, 1, 5, 76, 229, Dungey's model, 69, 74, 137, 139 Electric field, 5, 46, 75,81, 187, 234, 247, 271, 320, 325, 334, 342 Electron beams, 91, 100, 241, 252, 333 Electrostatic waves, 201, 205, 277 Energy spectrogram, 97, Energy transfer, 9, 13, 259 Entry layer, 38 Equivalent circuit, 16 Explorer 45(53) satellite, 159, 252 Fermi acceleration, 326 Field aligned currents, 132, 238, 284, 334 Field aligned fluxes, 94, 326, 331,342 Filaments, 5 Frozen-in fields, 12, 71 Geomagnetic storm, 159, 180, 271 Group velocity, 201, 218 Growth phase, 123, 141 Guiding center, 70 Hel iosphere, 17 Helium ions, 45, 48 HEOS 2 experiments, 24 Ins tab i 1 i tie s, 5, 201, 206, 218, 229, 237, 271, 277, 306, 310 Interconnection,
5 368 INDEX Interglanetary magnetic field, , 13 7 Ion beams, 333 Ion cyclotron waves, 64, 163, 202, 252, 273, 304, 310 Ionic components, 45 Ionospheric current, 134 ISIS-2 satellite, 113 Jovian magnetosphere, 19, 287 Kelvin-Helmholtz instability, 38 Laboratory experiments, 6, 229 Laminar flow, 233 Landau resonance, 174, 256, 326 Langmuir condition, 235 Langmuir waves, 262 Lifetimes, 176 Lorentz transformation, 75 Loss cone, 105, 201, 223, 251, 291 Magnetic equator, 91 Magnetic field line reconnection, 5, 9, 75 Magnetic field topology, 74 Parametric interactions, 262, 286 Phase space density, 35, 166 Pitch angle, 98-99, 101, ,163, ,203,271, 291, 294, 298, 315, 331, 344 Plasma cavity, 263 Plasma flow, 28, 33,143,147 Plasma heating, 251, 261, 271 Plasma interactions, 163 Plasma layer, 25 Plasma pause, 252, 302 Plasma sheet, 79, 137, 139, 141, 145, 152, 187 Plasmon condensate, 262 Polar cusp, 23-24, 39 Polar rain, 84 Polar shower, 84 Polar squall, 85 Poynting vector, 81 Precipitating electrons, 261, 291, 299, 328 Precipitating ions, 55, 259, 294, 299, 312 Protons, 26, 46, 47, 143, 160, 252, 294 Pseudo-plasma, 1, 3, 6 Magneto-hydrodynamic dynamo, 113, Quasi-linear diffusion, 38, 203, 243, 354, , 291 Magnetopause, 25, 37, 69, 72 Magnetosheet plasma, 69, 71 Magnetospheric cleft, 148 Magnetospheric disturbances, 115 Magnetotail, 14, 137, 355 Maxwell-s equations, 7, 359 Mode coupling, 262, 286 Moving plasma, 10 Narrow band emissions, 213, 223, Neutral line, 74, 137, 145, 156, 187,319 Neutral point, 75 Neutral sheet, 12, 17, 187, 190 Non-Maxwellian distribution functions, 5, 207, 252, , 311 Ohm-s law, 81 Oxygen ions, 51, 336 Radiation belt electrons, 174 Reconnection, 75, 148 Recovery phase, 164 Resonant particles, 253, 273, 321 Ring current, 2, 16, 165, 252, 259, 302 SAR arcs, 170,261,273 Shock waves, 71, 115, 281 Solar wind, 9, 14, 23, 71, 137 Substorm, 118, , 146, 187, 271 Trajectories, 191 Trapped particles, 233 Turbulence spectrum, 266, 271, 291, 306
6 INDEX 369 Turbulent collision frequency, V1asov theory, 195, ,267,284 Turbulent dissipation, 252 Whistler waves, , 273, Turbulent flow, Upper hybrid frequency, 201, 214 X-line, 74, 118,319
The Solar Wind Interaction with the Earth s Magnetosphere: A Tutorial. C. T. Russell
The Solar Wind Interaction with the Earth s Magnetosphere: A Tutorial C. T. Russell Department of Earth and Space Sciences and Institute of Geophysics and Space Physics University of California Los Angeles
More informationProton temperature and Plasma Volatility
The microstate of the solar wind Radial gradients of kinetic temperatures Velocity distribution functions Ion composition and suprathermal electrons Coulomb collisions in the solar wind Waves and plasma
More informationPIXIE/Polar A Success Story! PIXIE (Polar Ionospheric X-ray Imaging Experiment)
PIXIE/Polar A Success Story! PIXIE (Polar Ionospheric X-ray Imaging Experiment) Norsk Romsenter 8 mai 2008 Polars siste runddans Professor Johan Stadsnes ved Universitet i Bergen er vemodig, men mest stolt
More informationKinetic processes and wave-particle interactions in the solar wind
Kinetic processes and wave-particle interactions in the solar wind Eckart Marsch Institute for Experimental and Applied Physics (IEAP), Christian Albrechts University at Kiel, 24118 Kiel, Germany Seminar
More informationWave-particle and wave-wave interactions in the Solar Wind: simulations and observations
Wave-particle and wave-wave interactions in the Solar Wind: simulations and observations Lorenzo Matteini University of Florence, Italy In collaboration with Petr Hellinger, Simone Landi, and Marco Velli
More informationCluster-II: Scientific Objectives and Data Dissemination
r bulletin 102 may 2000 Cluster-II: Scientific Objectives and Data Dissemination C. Ph. Escoubet Space Science Department, ESA Directorate of Scientific Programmes, ESTEC, Noordwijk, The Netherlands Scientific
More informationStatistical Study of Magnetic Reconnection in the Solar Wind
WDS'13 Proceedings of Contributed Papers, Part II, 7 12, 2013. ISBN 978-80-7378-251-1 MATFYZPRESS Statistical Study of Magnetic Reconnection in the Solar Wind J. Enžl, L. Přech, J. Šafránková, and Z. Němeček
More informationCurriculum Vitae: Tuija Inkeri Pulkkinen Aalto University tel: +358-50-591 6013
Curriculum Vitae: Tuija Inkeri Pulkkinen Aalto University tel: +358-50-591 6013 POBox 17800, 00076 AALTO, Finland e-mail: tuija.pulkkinen@aalto.fi Updated May 16, 2015 Research interests Sun-Earth connection
More informationMagnetohydrodynamics. Basic MHD
Magnetohydrodynamics Conservative form of MHD equations Covection and diffusion Frozen-in field lines Magnetohydrostatic equilibrium Magnetic field-aligned currents Alfvén waves Quasi-neutral hybrid approach
More informationTemperature anisotropy in the solar wind
Introduction Observations Simulations Summary in the solar wind Petr Hellinger Institute of Atmospheric Physics & Astronomical Institute AS CR, Prague, Czech Republic Kinetic Instabilities, Plasma Turbulence
More informationSPACE WEATHER SUPPORT FOR COMMUNICATIONS. Overview
SPACE WEATHER SUPPORT FOR COMMUNICATIONS Overview Ionospheric variability (space weather) significantly impacts ground and space-based communications. In essence, the electrically charged particles of
More informationA SIMPLIFIED DISCUSSION OF RECONNECTION AND ITS MYTHS By Forrest Mozer
A SIMPLIFIED DISCUSSION OF RECONNECTION AND ITS MYTHS By Forrest Mozer 1 WHY A SIMPLIFIED DISCUSSION OF RECONNECTION? For many people, magnetic field reconnection is too complicated to understand in the
More informationThe microstate of the solar wind
The microstate of the solar wind Radial gradients of kinetic temperatures Velocity distribution functions Ion composition and suprathermal electrons Coulomb collisions in the solar wind Waves and plasma
More informationSolar Wind Control of Density and Temperature in the Near-Earth Plasma Sheet: WIND-GEOTAIL Collaboration. Abstract
1 Geophys. Res. Letters, 24, 935-938, 1997. Solar Wind Control of Density and Temperature in the Near-Earth Plasma Sheet: WIND-GEOTAIL Collaboration T. Terasawa 1, M. Fujimoto 2, T. Mukai 3, I. Shinohara
More informationKeywords: Geomagnetic storms Dst index Space Weather Recovery phase.
MAGNETOSPHERE BEHAVIOUR DURING THE RECOVERY PHASE OF GEOMAGNETIC STORMS JESÚS AGUADO, CONSUELO CID, YOLANDA CERRATO, ELENA SAIZ Departamento de Física. Universidad de Alcalá, E-28871 Alcalá de Henares,
More informationThe solar wind (in 90 minutes) Mathew Owens
The solar wind (in 90 minutes) Mathew Owens 5 th Sept 2013 STFC Advanced Summer School m.j.owens@reading.ac.uk Overview There s simply too much to cover in 90 minutes Hope to touch on: Formation of the
More informationGEOPHYSICS AND GEOCHEMISTRY - Vol.III - Solar Wind And Interplanetary Magnetic Field - Schwenn R. SOLAR WIND AND INTERPLANETARY MAGNETIC FIELD
SOLAR WIND AND INTERPLANETARY MAGNETIC FIELD Schwenn R. Max-Planck-Institut für Aeronomie, Katlenburg-Lindau, Germany Keywords: Sun, corona, solar wind, plasma, magnetic field, reconnection, coronal mass
More informationSpace Weather: An Introduction C. L. Waters. Centre for Space Physics University of Newcastle, Australia
Space Weather: An Introduction C. L. Waters Centre for Space Physics University of Newcastle, Australia 1 Outline Space weather: Conditions on the Sun and in the solar wind, magnetosphere, ionosphere and
More informationAuroral Arc Electrodynamics with FAST Satellite and Optical Data
Auroral Arc Electrodynamics with FAST Satellite and Optical Data Von der Gemeinsamen Naturwissenschaftlichen Fakultät der Technischen Universität Carolo-Wilhelmina zu Braunschweig zur Erlangung des Grades
More informationSolar Storms and Northern lights - how to predict Space Weather and the Aurora
Solar Storms and Northern lights - how to predict Space Weather and the Aurora Pål Brekke Norwegian Space Centre/UNIS Pål Brekke torsdag 12. mars 15 Fleet of satellites watching the Sun Stereo SDO SOHO
More informationSolar Wind: Theory. Parker s solar wind theory
Solar Wind: Theory The supersonic outflow of electrically charged particles, mainly electrons and protons from the solar CORONA, is called the SOLAR WIND. The solar wind was described theoretically by
More informationCoronal Heating Problem
Mani Chandra Arnab Dhabal Raziman T V PHY690C Course Project Indian Institute of Technology Kanpur Outline 1 2 3 Source of the energy Mechanism of energy dissipation Proposed mechanisms Regions of the
More informationThe Theory of Magnetic Reconnection: Past, Present, and Future
The Theory of Magnetic Reconnection: Past, Present, and Future Paul Cassak University of Delaware & West Virginia University 2008 AGU Joint Assembly May 28, 2008 SOHO (ESA & NASA) Magnetic Reconnection
More informationDEGREE: Bachelor's Degree in Industrial Electronics and Automation COURSE: 1º TERM: 2º WEEKLY PLANNING
SESSION WEEK COURSE: Physics II DEGREE: Bachelor's Degree in Industrial Electronics and Automation COURSE: 1º TERM: 2º WEEKLY PLANNING DESCRIPTION GROUPS (mark ) Indicate YES/NO If the session needs 2
More informationSporadic E A Mystery Solved?
Sporadic E A Mystery Solved? In Part 1 of this QST exclusive, one of the world s leading ionospheric scientists explains the physics of sporadic E and discusses unresolved problems in understanding its
More informationSolar Forcing of Electron and Ion Auroral Inputs
Solar Forcing of Electron and Ion Auroral Inputs Barbara A. Emery (NCAR), Ian G. Richardson (GSFC), David S. Evans (NOAA), Frederick J. Rich (LL/MIT), Gordon Wilson (AFRL), Sarah Gibson (NCAR), Giuliana
More informationJPL ANOMALY ISSUES. Henry B. Garrett Jet Propulsion Laboratory California Institute of Technology Pasadena, CA, 91109
JPL ANOMALY ISSUES Henry B. Garrett Pasadena, CA, 91109 Space Weather Anomaly Concerns for JPL Robotic Mission AGENDA Overview of Space Weather Anomalies on JPL Missions Space Weather Products used by
More informationHow To Understand Space Weather
GOES Data and Products in the Space Weather Prediction Center and National Geophysical Data Center Mary Shouldis Satellite Data Product Development Team Lead NGDC/University of Colorado/CIRES Putting Science
More informationSolar Ast ro p h y s ics
Peter V. Foukal Solar Ast ro p h y s ics Second, Revised Edition WI LEY- VCH WILEY-VCH Verlag Co. KCaA Contents Preface 1 1.1 1.2 1.3 1.4 1.5 1.6 1.7 1.8 1.9 2 2.1 2.1.1 2.1.2 2.2 2.2.1 2.2.2 2.2.3 2.3
More informationSpace Environment and Satellite Systems: Removing Clutter from Ground-to-Satellite Signals. Sigrid Close
Space Environment and Satellite Systems: Removing Clutter from Ground-to-Satellite Signals Sigrid Close Background Overview RF propagation through ionosphere can be problematic Goals Traditionally too
More informationKinetic effects in the turbulent solar wind: capturing ion physics with a Vlasov code
Kinetic effects in the turbulent solar wind: capturing ion physics with a Vlasov code Francesco Valentini francesco.valentini@fis.unical.it S. Servidio, D. Perrone, O. Pezzi, B. Maruca, F. Califano, W.
More informationDiscuss 7 deficiencies/impediments in our understanding. 1
Do We Really Understand Solar-Wind/Magnetosphere Coupling? Joe Borovsky Space Science Institute --- University of Michigan!We have major unsolved issues about A. what controls dayside reconnection B. the
More informationSpace Weather Research in KASI. Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI)
Space Weather Research in KASI Yeon-Han Kim & KASI people Space Science Division(SSD) Korea Astronomy and Space Science Institute(KASI) I. SSD in KASI Sun-Earth Connection (CME geoeffectiveness) Solar
More informationActivities of the Japanese Space Weather Forecast Center at Communications Research Laboratory
J. RADIAT. RES., 43: SUPPL., S53 S57 (2002) Activities of the Japanese Space Weather Forecast Center at Communications Research Laboratory SHINICHI WATARI 1 * and FUMIHIKO TOMITA 1 Space weather / ISES/SEP
More informationChapter 9 Summary and outlook
Chapter 9 Summary and outlook This thesis aimed to address two problems of plasma astrophysics: how are cosmic plasmas isotropized (A 1), and why does the equipartition of the magnetic field energy density
More informationR. Singh B. Veenadhari S. Alex Indian Institute of Geomagnetism, Navi Mumbai - 410218
Very Low Frequency (VLF) studies of ionospheric-magnetospheric electromagnetic phenomena in Indian low latitude region using AWESOME receivers R. Singh B. Veenadhari S. Alex Indian Institute of Geomagnetism,
More informationDiagnostics. Electric probes. Instituto de Plasmas e Fusão Nuclear Instituto Superior Técnico Lisbon, Portugal http://www.ipfn.ist.utl.
C. Silva Lisboa, Jan. 2014 IST Diagnostics Electric probes Instituto de Plasmas e Fusão Nuclear Instituto Superior Técnico Lisbon, Portugal http://www.ipfn.ist.utl.pt Langmuir probes Simplest diagnostic
More informationProton and He 2+ Temperature Anisotropies in the Solar Wind Driven by Ion Cyclotron Waves
Chin. J. Astron. Astrophys. Vol. 5 (2005), No. 2, 184 192 (http:/www.chjaa.org) Chinese Journal of Astronomy and Astrophysics Proton and He 2+ Temperature Anisotropies in the Solar Wind Driven by Ion Cyclotron
More informationPhysics Aspects of the Dynamic Ergodic Divertor (DED)
Physics Aspects of the Dynamic Ergodic Divertor (DED) FINKEN K. Heinz 1, KOBAYASHI Masahiro 1,2, ABDULLAEV S. Sadrilla 1, JAKUBOWSKI Marcin 1,3 1, Forschungszentrum Jülich GmbH, EURATOM Association, D-52425
More informationAnalysis and Visualization Progress report for 2001
Physics in Space B page 1 Enclosure 3 Uppsala Analysis and Visualization Progress report for 2001 1. Overview of the results During the fiscal year 2001 we have continued our highly successful analysis
More informationCSSAR Space Science Cooperation
CSSAR Space Science Cooperation WANG Shuzhi Center for Space Science and Applied Research Chinese Academy of Science(CSSAR) Table of Contents Brief History of CSSAR International Cooperation CAS Strategic
More informationPlanetary Sciences Ph.D. Track Proposal
Planetary Sciences Ph.D. Track Proposal The purpose of the Planetary Sciences track: Our nation s goals in space exploration require the support of highly trained scientific community. Florida s goals
More informationUnusual declining phase of solar cycle 23: Weak semi-annual variations of auroral hemispheric power and geomagnetic activity
Click Here for Full Article GEOPHYSICAL RESEARCH LETTERS, VOL. 36, L22102, doi:10.1029/2009gl040825, 2009 Unusual declining phase of solar cycle 23: Weak semi-annual variations of auroral hemispheric power
More informationMagnetic Field and Magnetic Forces
Chapter 27 Magnetic Field and Magnetic Forces PowerPoint Lectures for University Physics, Thirteenth Edition Hugh D. Young and Roger A. Freedman Lectures by Wayne Anderson Goals for Chapter 27 Magnets
More informationEASA Safety Information Bulletin
EASA Safety Information Bulletin SIB No.: 2012-09 Issued: 23 May 2012 Subject: Effects of Space Weather on Aviation Ref. Publication: 1. EU OPS 1.390 Cosmic Radiation; 2. SIB 2012-10 Single Event Effects
More informationEMİNE CEREN KALAFATOĞLU EYİGÜLER
EMİNE CEREN KALAFATOĞLU EYİGÜLER SPACE ENVIRONMENT UZB411E 2015-2016 FALL ROOM: 322 / THIRD FLOOR UPPER ATMOSPHERE AND SPACE WEATHER LAB OFFICE HOURS: EVERY TUESDAY AND WEDNESDAY BETWEEN 15-17 FOR OTHER
More informationSolar Wind Heating by MHD Turbulence
Solar Wind Heating by MHD Turbulence C. S. Ng, A. Bhattacharjee, and D. Munsi Space Science Center University of New Hampshire Acknowledgment: P. A. Isenberg Work partially supported by NSF, NASA CMSO
More informationElectron density estimations derived from spacecraft potential measurements on Cluster in tenuous plasma regions
Click Here for Full Article JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 113,, doi:10.1029/2007ja012636, 2008 Electron density estimations derived from spacecraft potential measurements on Cluster in tenuous
More informationHybrid simulation of ion cyclotron resonance in the solar wind: Evolution of velocity distribution functions
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 110,, doi:10.1029/2005ja011030, 2005 Hybrid simulation of ion cyclotron resonance in the solar wind: Evolution of velocity distribution functions Xing Li Institute
More informationThe Next Generation European Incoherent Scatter Radar System: EISCAT 3D and related facilities
The Next Generation European Incoherent Scatter Radar System: EISCAT 3D and related facilities Michael Rietveld EISCAT Scientific Association Tromsø Antenna 1 Control Norway Transmitter Antenna 2 Antenna
More informationElectromagnetism and Circular Motion in a Cyclotron
Electromagnetism and Circular Motion in a Cyclotron Contents p. 3 About Physics in Action Funding Availability Videos in the Physics in Action Series p. 5 Physics in Action: Electromagnetism and Circular
More informationSINP SPACE MONITORING DATA CENTER PORTAL
SINP SPACE MONITORING DATA CENTER PORTAL Parunakian D.A. 1, Kalegaev V.V. 2, Bobrovnikov S.Yu. 2, Barinova W.O. 2 1 Moscow State University Skobeltsyn Institute of Nuclear Physics 119991, Russia, e-mail:
More informationSolar Wind: Global Properties
Solar Wind: Global Properties The most fundamental problem in solar system research is still unsolved: how can the Sun with a surface temperature of only 5800 K heat up its atmosphere to more than a million
More informationRadiative effects of clouds, ice sheet and sea ice in the Antarctic
Snow and fee Covers: Interactions with the Atmosphere and Ecosystems (Proceedings of Yokohama Symposia J2 and J5, July 1993). IAHS Publ. no. 223, 1994. 29 Radiative effects of clouds, ice sheet and sea
More informationOn the properties of O + and O 2 + ions in a hybrid model and in Mars Express IMA/ASPERA-3 data: A case study
Planetary and Space Science 56 (2008) 1204 1213 www.elsevier.com/locate/pss On the properties of O and O 2 ions in a hybrid model and in Mars Express IMA/ASPERA-3 data: A case study E. Kallio a,, A. Fedorov
More informationSpace Weather Prediction Research and Services for China Manned Space Mission
Space Weather Prediction Research and Services for China Manned Space Mission Siqing Liu National Space Science Center, CAS Center for Space Science and Applied Research, CAS Outline I. General information
More informationIndiana Content Standards for Educators
Indiana Content for Educators SCIENCE PHYSICAL SCIENCE teachers are expected to have a broad understanding of the knowledge and skills needed for this educator license, and to use that knowledge to help
More informationKolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in
Kolmogorov versus Iroshnikov-Kraichnan spectra: Consequences for ion heating in the solar wind C. S. Ng 1, A. Bhattacharjee 2, D. Munsi 2, P. A. Isenberg 2, and C. W. Smith 2 1 Geophysical Institute, University
More informationCOURSE: PHYSICS DEGREE: COMPUTER ENGINEERING year: 1st SEMESTER: 1st
COURSE: PHYSICS DEGREE: COMPUTER ENGINEERING year: 1st SEMESTER: 1st WEEKLY PROGRAMMING WEE K SESSI ON DESCRIPTION GROUPS GROUPS Special room for LECTU PRAC session RES TICAL (computer classroom, audiovisual
More informationMet Office Space Weather Operations and R&D
Met Office Space Weather Operations and R&D David Jackson Mark Gibbs, Suzy Bingham, Francois Bocquet, Edmund Henley, Sophie Murray WMO / ISES Meeting, August 9-10 2014, Moscow, Russia Met Office Motivation?
More informationA Plan of Action Under LTSP III
A Plan of Action Under LTSP III William Liu and Robert Rankin Department of Physics, University of Alberta David Boteler Geomagnetic Laboratory, Geological Survey of Canada Submitted to the Canadian Space
More informationDr. Juan Alejandro Valdivia Hepp Profesor Titular Director Departamento de Física Facultad de Ciencias Universidad de Chile
Dr. Juan Alejandro Valdivia Hepp Profesor Titular Director Departamento de Física Facultad de Ciencias Universidad de Chile B.Sc. in Physics, University of Maryland, USA, 1991 B.Sc. in Astronomy, University
More informationA Beginner s Guide to Space Weather and GPS Professor Paul M. Kintner, Jr. with acknowledgements to
A Beginner s Guide to Space Weather and GPS Professor Paul M. Kintner, Jr. with acknowledgements to M. Psiaki, T. Humphreys, A. Cerruti, B. Ledvina, A. Mannucci, and E. R. de Paula I. Introduction This
More informationKinetic Models of Solar Wind Electrons, Protons and Heavy Ions
10 Kinetic Models of Solar Wind Electrons, Protons and Heavy Ions Viviane Pierrard Belgian Institute for Space Aeronomy and Université Catholique de Louvain Belgium 1. Introduction In the present chapter,
More informationThe content is based on the National Science Teachers Association (NSTA) standards and is aligned with state standards.
Literacy Advantage Physical Science Physical Science Literacy Advantage offers a tightly focused curriculum designed to address fundamental concepts such as the nature and structure of matter, the characteristics
More informationA slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study
Ann. Geophysicae 17, 674±681 (1999) Ó EGS ± Springer-Verlag 1999 A slow mode wave as a possible source of Pi 2 and associated particle precipitation: a case study O. Saka 1; 2, O. Watanabe 2, K. Okada
More informationPHYSICS - MASTER. Study plan: Name. Qualification awarded Master of Science in Physics.
Study plan: PHYSICS - MASTER Name Bokmål: Nynorsk: English: Physics - master Physics - master Physics - master Qualification awarded Master of Science in Physics. Workload 120 ECTS credits. With a workload
More informationWELCOME to Aurorae In the Solar System. J.E. Klemaszewski
WELCOME to Aurorae In the Solar System Aurorae in the Solar System Sponsoring Projects Galileo Europa Mission Jupiter System Data Analysis Program ACRIMSAT Supporting Projects Ulysses Project Outer Planets
More information4-1-3 Space Weather Forecast Using Real-time Data
4-1-3 Space Weather Forecast Using Real-time Data In recent years, advances in telecommunications technology have made it possible to collect space-based and ground-based observation data needed for space
More informationATMOSPHERIC SCIENCES (ATS) Program Director: Joseph A. Zehnder Department Office: Hixson-Lied Science Building, Room 504
(ATS) Program Director: Joseph A. Zehnder Department Office: Hixson-Lied Science Building, Room 504 Graduate Study in Atmospheric Sciences Creighton University offers courses and experience leading to
More informationScience Standard Articulated by Grade Level Strand 5: Physical Science
Concept 1: Properties of Objects and Materials Classify objects and materials by their observable properties. Kindergarten Grade 1 Grade 2 Grade 3 Grade 4 PO 1. Identify the following observable properties
More informationDanish Arctic Ionosphere Research
Danish Arctic Ionosphere Research JQRGEN TAAGHOLTI HISTORICAL BACKGROUND The Danish Meteorological Institute celebrated its centennial on 1 April this year and on the same date the Ionosphere Laboratory,
More informationInterstellar Cosmic-Ray Spectrum from Gamma Rays and Synchrotron
Interstellar Cosmic-Ray Spectrum from Gamma Rays and Synchrotron Chuck Naval Research Laboratory, Washington, DC charles.dermer@nrl.navy.mil Andy Strong Max-Planck-Institut für extraterrestrische Physik,
More informationELECTRON LOSS AND METEORIC DUST IN THE MESOSPHERE
ELECTRON LOSS AND METEORIC DUST IN THE MESOSPHERE Martin Friedrich (1), Markus Rapp (2), Tom Blix (3), Ulf-Peter Hoppe (4), Klaus Torkar (5) (1) Graz University of Technology, Inffeldgasse 12, A-10 Graz,
More informationAtomic Physics Measurements in Support of X-ray Astronomy
Atomic Physics Measurements in Support of X-ray Astronomy Your LDRD Representative Graphic Here (Fit in this rectangle, no caption) Oct 27, 2010 Gatlinburg P. Beiersdorfer G. Brown LLNL M. Frankel LLNL*
More informationLecture 14. Introduction to the Sun
Lecture 14 Introduction to the Sun ALMA discovers planets forming in a protoplanetary disc. Open Q: what physics do we learn about the Sun? 1. Energy - nuclear energy - magnetic energy 2. Radiation - continuum
More informationSPACE WEATHER INTERPRETING THE WIND. Petra Vanlommel & Luciano Rodriguez
SPACE WEATHER INTERPRETING THE WIND Petra Vanlommel & Luciano Rodriguez THE SUN LOSES ENERGY Radiation Mass Particles THE SUN LOSES ENERGY PHYSICAL REPHRASING Total Solar Irradiance Solar Wind Fast Particles
More informationCoordinate generators
SPENVIS Upgrades Coordinate generators Merge orbit generator and grid generator: Simplification of model implementation Simplification of model presentation and navigation Orbit generator: Add NORAD Two
More informationMeeting the Grand Challenge of Protecting an Astronaut s Health: Electrostatic Active Space Radiation Shielding for Deep Space Missions
Meeting the Grand Challenge of Protecting an Astronaut s Health: Electrostatic Active Space Radiation Shielding for Deep Space Missions Ram Tripathi NASA Langley Research Center NIAC 2012 Spring Symposium,
More informationCOMESEP Project : Space Weather Impact Forecasting
COMESEP Project : Space Weather Impact Forecasting Crosby, N.B. 1, Veronig, A. 2, Robbrecht, E. 3, Vrsnak, B. 4, Vennerstrom, S. 5, Malandraki, O. 6, Dalla, S. 7, Rodriguez, L. 3, Srivastava, N. 8, Hesse,
More informationGraduate Certificate Program in Energy Conversion & Transport Offered by the Department of Mechanical and Aerospace Engineering
Graduate Certificate Program in Energy Conversion & Transport Offered by the Department of Mechanical and Aerospace Engineering Intended Audience: Main Campus Students Distance (online students) Both Purpose:
More informationESA Space Weather Initiatives
ESA Space Weather Initiatives The Multi-functional Nature of the Aerospace Domain: a European Approach 22-24 October 2014 Firenze, Italy Juha-Pekka Luntama Space Weather Manager ESA SSA Programme Office
More informationSIO 229 Gravity and Geomagnetism: Class Description and Goals
SIO 229 Gravity and Geomagnetism: Class Description and Goals This graduate class provides an introduction to gravity and geomagnetism at a level suitable for advanced non-specialists in geophysics. Topics
More informationDTIC N N ELEICTE. S CT 319 00u. S Wright-Patterson AFB OH 45433. 1990 Thesis/Dissertation
1990 Thesis/Dissertation A Case Study of the 19 October 1989 Polar Cap Absorption Event Using the Imaging Riometer for Ionospheric Studies Timothy C. Davis AFIT Student at: University of Maryland AFIT/CI/CIA
More informationCourses that Require this Course as a Prerequisite: None.
ENGR (ASTR) 4190/6190 Planetary Atmospheres, Dynamics, and Magnetospheres The University of Georgia Fall Semester 2012 Professor: David Emory Stooksbury Office: 603 Driftmier Engineering Center Phone:
More informationHyperbolic decay of the Dst Index during the recovery phase of intense geomagnetic storms
Click Here for Full Article JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115,, doi:10.1029/2009ja014658, 2010 Hyperbolic decay of the Dst Index during the recovery phase of intense geomagnetic storms J. Aguado,
More informationKinetic physics of the solar wind
"What science do we need to do in the next six years to prepare for Solar Orbiter and Solar Probe Plus?" Kinetic physics of the solar wind Eckart Marsch Max-Planck-Institut für Sonnensystemforschung Complementary
More informationMETIS Coronagraph on Solar Orbiter and Solar Probe Synergies. INAF - Osservatorio Astronomico di Torino (Italy) & the METIS Team
METIS Coronagraph on Solar Orbiter and Solar Probe Synergies Silvano Fineschi INAF - Osservatorio Astronomico di Torino (Italy) & the METIS Team 3rd METIS Scientific and Technical Meeting Napoli 17 th
More informationINTRODUCTION TO SOLAR WEATHER & HF PROPAGATION. Lewis Thompson W5IFQ September 27, 2011
INTRODUCTION TO SOLAR WEATHER & HF PROPAGATION Lewis Thompson W5IFQ September 27, 2011 PRESENTATION Ionospheric propagation NVIS Long-Range Frequency Selection (Critical Frequency & MUF) Propagation modeling
More informationUNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics
UNIVERSITY OF SASKATCHEWAN Department of Physics and Engineering Physics Physics 111.6 MIDTERM TEST #4 March 15, 2007 Time: 90 minutes NAME: (Last) Please Print (Given) STUDENT NO.: LECTURE SECTION (please
More informationTheory of Magnetic Reconnection for Solar Applications or Why are we still talking about reconnection after 50 years?!?
Theory of Magnetic Reconnection for Solar Applications or Why are we still talking about reconnection after 50 years?!? Paul Cassak West Virginia University 2009 SHINE Workshop August 6, 2009 Acknowledgments
More informationEnergy Transport. Focus on heat transfer. Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids)
Energy Transport Focus on heat transfer Heat Transfer Mechanisms: Conduction Radiation Convection (mass movement of fluids) Conduction Conduction heat transfer occurs only when there is physical contact
More informationCV, PhD Diploma, Transcript
CV, PhD Diploma, Transcript Mihai-Octavian Dima Address : Str. Mendeleev 7-15, Sc. B, Ap. 34 R-70168, Bucharest - Romania Tel. : +40-724-502-557 (cel.) E-mail : modima@cern.ch Web : http://www.ad-astra.ro/whoswho/view_profile.php?user_id=854&lang=en
More informationSpace Weather: Forecasting & Impacts on Critical Infrastructure
Space Weather: Forecasting & Impacts on Critical Infrastructure Dr. Genene Fisher Senior Advisor for Space Weather National Weather Service AMS Washington Forum 12 April 2012 Outline Solar Activity Update
More informationThe University of the State of New York REGENTS HIGH SCHOOL EXAMINATION PHYSICAL SETTING PHYSICS. Friday, June 20, 2014 1:15 to 4:15 p.m.
P.S./PHYSICS The University of the State of New York REGENTS HIGH SCHOOL EXAMINATION PHYSICAL SETTING PHYSICS Friday, June 20, 2014 1:15 to 4:15 p.m., only The possession or use of any communications device
More informationWeather Radar Basics
Weather Radar Basics RADAR: Radio Detection And Ranging Developed during World War II as a method to detect the presence of ships and aircraft (the military considered weather targets as noise) Since WW
More informationAdvanced Topics in Physics: Special Relativity Course Syllabus
Advanced Topics in Physics: Special Relativity Course Syllabus Day Period What How 1. Introduction 2. Course Information 3. Math Pre-Assessment Day 1. Morning 1. Physics Pre-Assessment 2. Coordinate Systems
More informationIonosphere Properties and Behaviors - Part 2 By Marcel H. De Canck, ON5AU
Ionosphere Properties and Behaviors - Part 2 By Marcel H. De Canck, ON5AU I n the previous issue I explained that gyrofrequency depends on the earth s magnetic field and mentioned that this magnetic field
More informationSolar atmosphere. Solar activity and solar wind. Reading for this week: Chap. 6.2, 6.3, 6.5, 6.7 Homework #2 (posted on website) due Oct.
Solar activity and solar wind Solar atmosphere Reading for this week: Chap. 6.2, 6.3, 6.5, 6.7 Homework #2 (posted on website) due Oct. 17 Photosphere - visible surface of sun. Only ~100 km thick. Features
More information