The inner magnetosphere : physics and modeling

Author(s)

• Pulkkinen, T. (Tuija)
• T︠S︡yganenko, N. A.
• Friedel, Reiner H. W.
• American Geophysical Union

Bibliographic Information

The inner magnetosphere : physics and modeling

Tuija I. Pulkkinen, Nikolai A. Tsyganenko, Reiner H.W. Friedel, editors

（Geophysical monograph, 155）

American Geophysical Union, c2005

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• The inner magnetosphere : physics and modeling / Tuija I. Pulkkinen, Nikolai A. Tsyganenko, Reiner H.W. Friedel, editors

  2005

  HathiTrust

  

Note

Includes bibliographical references and index

Description and Table of Contents

Description

Published by the American Geophysical Union as part of the Geophysical Monograph Series, Volume 155. As we become a space-faring culture, there is an increasing need for reliable methods to forecast the dynamics of electromagnetic fields, thermal plasma, and energetic particles in the geospace environment, as all these factors affect satellite-borne systems. From the electrodynamics viewpoint, on the other hand, the inner magnetosphere is a key element in the Sun-Earth connection chain of processes. Most notably, it is a region where a significant part of the storm-time energy input from the solar wind is deposited and dissipated. Because the most interesting and crucially important phenomena, as noted, develop relatively close to Earth (in the transition region separating the innermost quasi-dipolar geomagnetic field from the magnetotail), understanding them is a complex task. Moreover, the stronger the disturbance, the deeper its impact penetrates into the inner magneto-sphere. In this region plasma no longer behaves like a fluid, and the motion of energetic charged particles becomes important for the dynamics of the system. This fact leaves "particle simulations" as a primary tool for studying and understanding the dynamics of the inner magnetosphere during storms. An integral element of such simulations is an electromagnetic field model. Recent studies of the inner magnetosphere have substantially improved our understanding of its dynamics while creating new paradigms and reviving old controversies.

Table of Contents

Preface viii A Historical Introduction to the Ring Current David P. Stern 1 I. Sources and Losses of Inner Magnetosphere Particle Population Sources, Transport, and Losses of Energetic Particles During Geomagnetic Storms Vania K. Jordanova 9 Energetic Particle Losses From the Inner Magnetosphere Hannu E. J. Koskinen 23 A Numerical Study on the Resonant Scattering Process of Relativistic Electrons via Whistler-Mode Waves in the Outer Radiation Belt Yuto Katoh, Takayuki Ono, and Masahide lizima 33 Structures of Sub-keV Ions Inside the Ring Current Region M. Yamauchi, R. Lundin, L. Eliasson, D. Winningham, H. Reme, C, Vallat, I. Dandouras, and Cluster-CIS team 41 Quick Response of the Near-Earth Magnetotail to Changes in the Interplanetary Magnetic Field Kumiko K. Hashimoto and Takashi Kikuchi 47 Narrow Plasma Streams as a Candidate to Populate the Inner Magnetosphere V. A. Sergeev, D. A. Yahnin, K. Liou, M. F. Thomsen, and G. D. Reeves 55 Dynamics of Ions of Ionospheric Origin During Magnetic Storms: Their Acceleration Mechanism and Transport Path to Ring Current M. Nose, K. Takahashi, S. Ohtani, S. R Christon, and R. W. McEntire 61 II. Energetic Particle Acceleration Mechanisms Particle Acceleration in the Inner Magnetosphere D. N. Baker, S. R. Elkington, X. Li, and M. J. Wiltberger 73 The Energetic Electron Response to Magnetic Storms: HEO Satellite Observations J. E Fennell, J. B. Blake, R. Friedel, and S. Kanekal 87 Global View of Energetic Particles During a Major Magnetic Storm Timo Asikainen, Kalevi Mursula, Raine Kerttula, Reiner Friedel, Daniel Baker, Finn Soraas, Joseph E Fennell, and J. Bernard Blake 97 Magnetospheric Substorms and the Sources of Inner Magnetosphere Particle Acceleration E. E. Antonova 105 Energization of the Inner Magnetosphere by Solar Wind Pressure Pulses W. William Liu 113 Energetic Trapped Proton and Electron Flux Variations at Low Altitudes Measured Onboard CORONAS-F Satellite During 2001, August-December, Their Connection with the Particle Flux Variations in Geostationary Orbit Sergey N. Kuznetsov and Irina N. Myagkova 121 Dynamics of the Earth's Radiation Belts During the Time Period April 14-24, 2002 - Experimental Data Irina N. Myagkova, Sergey N. Kuznetsov, Boris Yu. Yushkov, Yury I. Denisov, Ekaterina A. Murav'eva, and Joseph Lemaire 127 III. External Driving of the Inner Magnetosphere Drivers of the Inner Magnetosphere Natalia Yu. Ganushkina 135 Injection of Energetic Ions During the 31 March 0630 Substorm Scot R. Elkington, Daniel N. Baker, and Michael Wiltberger 147 Storm-Substorm Coupling During 16 Hours of Dst Steadily at -150 nT T. I. Pulkkinen, N. Yu. Ganushkina, GBP Donovan, X. Li, G. D. Reeves, C. T. Russell, H. J. Singer, and J. A. Slavin 155 On the Relation Between Sub-Auroral Electric Fields, the Ring Current and the Plasmasphere P. C. Brandt, J. Goldstein, P. C. Anderson, B.J. Anderson, R. DeMajistre, E. C. Roelof, and D. G. Mitchell 163 Transmission Line Model for Driving Plasma Convection in the Inner Magnetosphere Takashi Kikuchi 1 73 IV. Observational Specification of the Inner Magnetosphere Advances in Inner Magnetosphere Passive and Active Wave Research James L. Green and Shing F. Fung 181 Probabilistic Forecasting of the Dst Index Robert L. McPherron, George Siscoe, Nancy U. Crooker, and Nick Arge 203 Testing the Hypothesis That Charge Exchange Can Cause a Two-Phase Decay M. W. Liemohn and J. U. Kozyra 211 Substorm Associated Spikes in High Energy Particle Precipitation E. Spanswick, GBP Donovan, W. Liu, D. Wallis, A. Aasnes, T. Hiebert, B. Jackel, M. Henderson, and H. Prey 227 Ring Current Behavior as Revealed by Energetic Proton Precipitation F. Soraas, K. Aarsnes, D. V. Carlsen, K. Oksavik, and D. S. Evans 237 Proton Injections Into the Ring Current Associated With 0Z Variations During HILDCAA Events M. I. Sandanger, F. Soraas, K. Aarsnes, K. Oksavik, D. S. Evans, and M. S. Greer 249 What Defines the Polar Cap and Auroral Oval Diameters? Igor I. Alexeev 257 V. Large-Scale Models of the Inner Magnetosphere Modeling Inner Magnetospheric Electric Fields: Latest Self-Consistent Results Stanislav Sazykin, Robert W. Spiro, Richard A. Wolf, Frank R. Toffoletto, Nikolai Tsyganenko, J. Goldstein, and Marc R. Hairston 263 Comparison of MHD Simulations of Isolated and Storm Time Substorms M. Wiltberger, 5. R. Elkington, T Guild, D. N. Baker, and J. G. Lyon 271 Empirical Model of the Inner Magnetosphere H + Pitch Angle Distributions Jacopo De Benedetti, Anna Milillo, Stefano Orsini Alessandro Mura, Elisabetta DeAngelis, and loannis A. Daglis 283 Global Magnetospheric Dynamics During Magnetic Storms of Different Intensities V. V. Kalegaev and N. Yu. Ganushkina 293 A Back-Tracing Code to Study the Magnetosphere Transmission Function for Primary Cosmic Rays Pavol Bobik, Matteo Boschini, Davide Grandi, Massimo Gervasi, Elisabetta Micelotta, and Pier-Giorgio Rancoita 301 Investigation of 3D Energetic Particle Transport Inside Quiet-Time Magnetosphere Using Particle Tracing in Global MHD Model X. Shao, Shing F. Fung, L. C. Tan, K. Papadopoulos, M. Wiltberger, and M. C. Fok 307

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Details

• NCID: BA74338324
• ISBN:
  • 0875904203
• LCCN: 2005015772
• Country Code: us
• Title Language Code: eng
• Text Language Code: eng
• Place of Publication: Washington, D.C.
• Pages/Volumes: x, 318 p.
• Size: 28 cm
• Classification:
  • LCC : QC809.M35
  • DC22 : 538/.766
• Subject Headings:
  • LCSH : Magnetospheric physics -- Simulation methods
• Parent Bibliography ID:
  • BA00442691