Energetic Particles in the Magnetosphere and their Relationship to Solar Wind Drivers

  1. Natchimuthukonar Gopalswamy,
  2. Richard Mewaldt and
  3. Jarmo Torsti
  1. I. Roth1,
  2. M. K. Hudson2,
  3. B. T. Kress2 and
  4. K. L. Perry2

Published Online: 27 MAR 2013

DOI: 10.1029/165GM33

Solar Eruptions and Energetic Particles

Solar Eruptions and Energetic Particles

How to Cite

Roth, I., Hudson, M. K., Kress, B. T. and Perry, K. L. (2006) Energetic Particles in the Magnetosphere and their Relationship to Solar Wind Drivers, in Solar Eruptions and Energetic Particles (eds N. Gopalswamy, R. Mewaldt and J. Torsti), American Geophysical Union, Washington, D. C.. doi: 10.1029/165GM33

Author Information

  1. 1

    Space Sciences Laboratory, University of California Berkeley, California

  2. 2

    Department of Physics and Astronomy, Dartmouth College Hanover, New Hampshire

Publication History

  1. Published Online: 27 MAR 2013
  2. Published Print: 1 JAN 2006

ISBN Information

Print ISBN: 9780875904306

Online ISBN: 9781118666203

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Keywords:

  • Coronal mass ejections;
  • Solar energetic particles;
  • Solar activity

Summary

This chapter contains sections titled:

  • Introduction

  • Energization Mechanisms

  • Phase Space

  • Energy and Pitch Angle Diffusion

  • Additional Loss Processes

  • Shock Induced Acceleration

  • Discussion and Conclusions