Dynamics of Ions of Ionospheric Origin During Magnetic Storms: Their Acceleration Mechanism and Transport Path to Ring Current

  1. Tuija I. Pulkkinen,
  2. Nikolai A. Tsyganenko and
  3. Reiner H.W. Friedel
  1. M. Nosé1,
  2. K. Takahashi2,
  3. S. Ohtani2,
  4. S.P. Christon3 and
  5. R.W. McEntire2

Published Online: 18 MAR 2013

DOI: 10.1029/155GM08

The Inner Magnetosphere: Physics and Modeling

The Inner Magnetosphere: Physics and Modeling

How to Cite

Nosé, M., Takahashi, K., Ohtani, S., Christon, S.P. and McEntire, R.W. (2005) Dynamics of Ions of Ionospheric Origin During Magnetic Storms: Their Acceleration Mechanism and Transport Path to Ring Current, in The Inner Magnetosphere: Physics and Modeling (eds T. I. Pulkkinen, N. A. Tsyganenko and R. H.W. Friedel), American Geophysical Union, Washington, D. C.. doi: 10.1029/155GM08

Author Information

  1. 1

    Data Analysis Center for Geomagnetism and Space Magnetism, Graduate School of Science, Kyoto University, Kyoto, Japan

  2. 2

    Applied Physics Laboratory, Johns Hopkins University, Laurel, Maryland

  3. 3

    Focused Research and Analysis, Columbia, Maryland

Publication History

  1. Published Online: 18 MAR 2013
  2. Published Print: 1 JAN 2005

ISBN Information

Print ISBN: 9780875904207

Online ISBN: 9781118666098

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Keywords:

  • Magnetospheric physics—Simulation methods

Summary

This chapter contains sections titled:

  • Introduction

  • Data Set

  • Observations

  • Discussion

  • Conclusions