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Book Categories |
Preface | ||
Solar Wind | ||
Wind Observations of Suprathermal Particles in the Solar Wind | 1 | |
Dayside Magnetosphere | ||
Dayside Electrodynamics Observed by POLAR with Northward IMF | 13 | |
Interball Tail Probe Measurements in Outer Cusp and Boundary Layers | 25 | |
Convection of Plasmaspheric Plasma into the Outer Magnetosphere and Boundary Layer Region: Initial Results | 45 | |
AMPTE-IRM Observations of Particles and Fields at the Dayside Low-Latitude Magnetopause | 51 | |
The Effect of the Interplanetary Magnetic Field on the Dayside Magnetosphere | 67 | |
Entry of Solar Wind Plasma into the Magnetosphere: Observations Encounter Simulation | 73 | |
High-Latitude Ionosphere | ||
Under What Conditions Will Ionospheric Molecular Ion Outflow Occur? | 85 | |
Day-Night Asymmetry Of Polar Outflow Due to the Kinetic Effects of Anisotropic Photoelectrons | 97 | |
POLAR Observations of Properties of H[superscript +] and O[superscript +] Conics in the Cusp Near รค5300 km Attitude | 107 | |
Recent Developments in Ion Acceleration in the Auroral Zone | 115 | |
Aurora | ||
High-Latitude Auroral Boundaries Compared With GEOTAIL Measurements During Two Substorms | 129 | |
Energy Characterization of a Dynamic Auroral Event Using GGS UVI Images | 143 | |
Auroral Observations from the POLAR Ultraviolet Imager (UVI) | 149 | |
Field Line Resonances, Auroral Arcs, and Substorm Intensifications | 161 | |
Magnetotail/Plasma Sheet/Substorms | ||
A New Approach to the Future of Space Physics | 169 | |
Reconnections at Near-Earth Magnetotail and Substorms Studied by a 3-D EM Particle Code | 175 | |
Magnetospheric-Ionospheric Activity During an Isolated Substorm: A Comparison Between WIND/Geotail/IMP 8/CANOPUS Observations and Modeling | 181 | |
Sporadic Localized Reconnections and Multiscale Intermittent Turbulence in the Magnetotail | 193 | |
Geotail Observations of Current Systems in the Plasma Sheet | 201 | |
Near-Earth Plasma Sheet Behavior During Substorms | 213 | |
Separation of Directly-Driven and Unloading Components in the Ionospheric Equivalent Currents During Substorms by the Method of Natural Orthogonal Components | 227 | |
Simulation of the March 9, 1995 Substorm and Initial Comparison to Data | 237 | |
Large-Scale Dynamics of the Magnetospheric Boundary: Comparisons Between Global MHD Simulation Results and ISTP Observations | 247 | |
Study of an Isolated Substorm with ISTP Data | 261 | |
Structure of the Magnetotail Reconnection Layer in 2-D Ideal MHD Model | 275 | |
Particle Acceleration Due to Magnetic Field Reconnection in a Model Current Sheet | 287 | |
Modeling Magnetotail Ion Distributions with Global Magnetohydrodynamic and Ion Trajectory Calculations | 291 | |
Determination of Particle Sources for a Geotail Distribution Function Observed on May 23, 1995 | 297 | |
Three-Dimensional Reconnection in the Earth's Magnetotail: Simulations and Observations | 313 | |
Inner Magnetosphere | ||
Drift-Shell Splitting in an Asymmetric Magnetic Field | 327 | |
Comparison of Photoelectron Theory Against Observations | 333 | |
Determining the Significance of Electrodynamic Coupling Between Superthermal Electrons and Thermal Plasma | 343 | |
A New Magnetic Storm Model | 349 | |
The Magnetospheric Trough | 355 | |
Magnetic Field Models | ||
Data-Based Models of the Global Geospace Magnetic Field: Challenges and Prospects of the ISTP Era | 371 | |
Improvements to the Source Surface Model of the Magnetosphere | 383 |
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Add Geospace mass and energy flow, The International Solar?]Terrestrial Program (ISTP) was conceived by the space agencies of numerous countries as a coordinated effort to determine the global flow of mass, energy and momentum through the solar?]terrestrial system. The physical region of i, Geospace mass and energy flow to the inventory that you are selling on WonderClubX
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Add Geospace mass and energy flow, The International Solar?]Terrestrial Program (ISTP) was conceived by the space agencies of numerous countries as a coordinated effort to determine the global flow of mass, energy and momentum through the solar?]terrestrial system. The physical region of i, Geospace mass and energy flow to your collection on WonderClub |