Modeling the Behavior of Corotating Interaction Region Driven Storms in Comparison with Coronal Mass Ejection Driven Storms

  1. Bruce Tsurutani,
  2. Robert McPherron,
  3. Gang Lu,
  4. José H. A. Sobral and
  5. Natchimuthukonar Gopalswamy
  1. Vania K. Jordanova

Published Online: 19 MAR 2013

DOI: 10.1029/167GM08

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Recurrent Magnetic Storms: Corotating Solar Wind Streams

How to Cite

Jordanova, V. K. (2006) Modeling the Behavior of Corotating Interaction Region Driven Storms in Comparison with Coronal Mass Ejection Driven Storms, 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: 10.1029/167GM08

Author Information

  1. Space Science Center, University of New Hampshire, Durham, New Hampshire, 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

  • Kinetic Ring Current Model

  • Model Results and Discussion

  • Summary and Conclusions