Energetics of Magnetic Storms Driven by Corotating Interaction Regions: A Study of Geoeffectiveness

  1. Bruce Tsurutani,
  2. Robert McPherron,
  3. Gang Lu,
  4. José H. A. Sobral and
  5. Natchimuthukonar Gopalswamy
  1. Niescja E. Turner1,
  2. Elizabeth J. Mitchell1,
  3. Delores J. Knipp2 and
  4. Barbara A. Emery3

Published Online: 19 MAR 2013

DOI: 10.1029/167GM11

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Recurrent Magnetic Storms: Corotating Solar Wind Streams

How to Cite

Turner, N. E., Mitchell, E. J., Knipp, D. J. and Emery, B. A. (2006) Energetics of Magnetic Storms Driven by Corotating Interaction Regions: A Study of Geoeffectiveness, 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: 10.1029/167GM11

Author Information

  1. 1

    Florida Institute of Technology, Melbourne, Florida

  2. 2

    United States Air Force Academy, Colorado Springs, Colorado

  3. 3

    High Altitude Observatory, National Center for Atmospheric Research, Boulder, Colorado

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

  • Previous Work

  • Methodology

  • Observations

  • Discussion

  • Conclusions