The Solar Wind and Geomagnetic Activity as a Function of Time Relative to Corotating Interaction Regions

  1. Bruce Tsurutani,
  2. Robert McPherron,
  3. Gang Lu,
  4. José H. A. Sobral and
  5. Natchimuthukonar Gopalswamy
  1. Robert L. McPherron1 and
  2. James Weygand2

Published Online: 19 MAR 2013

DOI: 10.1029/167GM12

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Recurrent Magnetic Storms: Corotating Solar Wind Streams

How to Cite

McPherron, R. L. and Weygand, J. (2006) The Solar Wind and Geomagnetic Activity as a Function of Time Relative to Corotating Interaction Regions, in Recurrent Magnetic Storms: Corotating Solar Wind Streams (eds B. Tsurutani, R. McPherron, G. Lu, J. H. A. Sobral and N. Gopalswamy), American Geophysical Union, Washington, D. C.. doi: 10.1029/167GM12

Author Information

  1. 1

    Institute of Geophysics and Planetary Physics and Department of Earth and Space Science University of California, Los Angeles, California, USA

  2. 2

    Institute of Geophysics and Planetary Physics at University of California, Los Angeles, California, USA

Publication History

  1. Published Online: 19 MAR 2013
  2. Published Print: 1 JAN 2006

ISBN Information

Print ISBN: 9780875904320

Online ISBN: 9781118666456

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Keywords:

  • Magnetic storms;
  • Corotating interaction regions;
  • Magnetosphere;
  • Atmosphere, Upper

Summary

This chapter contains sections titled:

  • Introduction

  • Data Base and Analysis Method

  • Results of Analysis

  • Discussion