Solar Wind-Magnetosphere Interaction as Simulated by a 3D, Em Particle Code

  1. Maha Ashour-Abdalla,
  2. Tom Chang and
  3. Paul Dusenbery
  1. Oscar Buneman1,
  2. Ken-Ichi Nishikawa2 and
  3. Torsten Neubert3

Published Online: 18 MAR 2013

DOI: 10.1029/GM086p0347

Space Plasmas: Coupling Between Small and Medium Scale Processes

Space Plasmas: Coupling Between Small and Medium Scale Processes

How to Cite

Buneman, O., Nishikawa, K.-I. and Neubert, T. (1995) Solar Wind-Magnetosphere Interaction as Simulated by a 3D, Em Particle Code, in Space Plasmas: Coupling Between Small and Medium Scale Processes (eds M. Ashour-Abdalla, T. Chang and P. Dusenbery), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM086p0347

Author Information

  1. 1

    Star Laboratory, Department of Electrical Engineering, Stanford University, Stanford, California

  2. 2

    Department of Physics and Astronomy, the University of Iowa, Iowa City, Iowa

  3. 3

    Space Physics Research Laboratory, the University of Michigan, Ann Arbor, Michigan

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 1995

ISBN Information

Print ISBN: 9780875900438

Online ISBN: 9781118664056

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Keywords:

  • Space plasmas;
  • Geophysics;
  • Astrophysics

Summary

  • Introduction

  • A New 3D Em Particle Simulation Model

  • Simulation Results

  • Discussion