Dayside Ionospheric (GPS) Response to Corotating Solar Wind Streams

  1. Bruce Tsurutani,
  2. Robert McPherron,
  3. Gang Lu,
  4. José H. A. Sobral and
  5. Natchimuthukonar Gopalswamy
  1. B. T. Tsurutani1,
  2. A. J. Mannucci1,
  3. B. A. Iijima1,
  4. A. Komjathy1,
  5. A. Saito2,
  6. T. Tsuda3,
  7. O. P. Verkhoglyadova4,
  8. W. D. Gonzalez5 and
  9. F. L. Guarnieri5

Published Online: 19 MAR 2013

DOI: 10.1029/167GM20

Recurrent Magnetic Storms: Corotating Solar Wind Streams

Recurrent Magnetic Storms: Corotating Solar Wind Streams

How to Cite

Tsurutani, B. T., Mannucci, A. J., Iijima, B. A., Komjathy, A., Saito, A., Tsuda, T., Verkhoglyadova, O. P., Gonzalez, W. D. and Guarnieri, F. L. (2006) Dayside Ionospheric (GPS) Response to Corotating Solar Wind Streams, 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: 10.1029/167GM20

Author Information

  1. 1

    Jet Propulsion Laboratory, Pasadena, California, USA

  2. 2

    Kyoto University, Kyoto, Japan

  3. 3

    RISH, Kyoto University, Uji, 6110-0011, Japan

  4. 4

    IGPP, University of California, Riverside, California, USA

  5. 5

    Brazil National Space Research Institute (INPE)Sao Jose Dos Campos, SP, Sao Paulo, Brazil

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

  • Background

  • Summary

  • Conclusion and Future Work