IMF By and the Spatio-Temporal Structure of the Dayside Aurora

  1. Bruce Tsurutani,
  2. Robert McPherron,
  3. Gang Lu,
  4. José H. A. Sobral and
  5. Natchimuthukonar Gopalswamy
  1. P. E. Sandholt1,
  2. C. J. Farrugia2,
  3. E. J. Lund2 and
  4. W. F. Denig3

Published Online: 19 MAR 2013

DOI: 10.1029/167GM18

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Recurrent Magnetic Storms: Corotating Solar Wind Streams

How to Cite

Sandholt, P. E., Farrugia, C. J., Lund, E. J. and Denig, W. F. (2013) IMF By and the Spatio-Temporal Structure of the Dayside Aurora, 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: 10.1029/167GM18

Author Information

  1. 1

    Department of Physics, University of Oslo, Oslo, Norway

  2. 2

    Space Science Center, University of New Hampshire, Durham

  3. 3

    Air Force Research Laboratory, Hanscom AFB

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

  • General Remarks on Dayside Auroral Activity

  • Data Description

  • Discussion

  • Summary