Upstream Waves and Field Line Resonances — Pulsation Research at the Nagycenk Observatory During Three Solar Cycles

  1. M. J. Engebretson,
  2. K. Takahashi and
  3. M. Scholer
  1. József Verő and
  2. Bertalan Zieger

Published Online: 3 APR 2013

DOI: 10.1029/GM081p0055

Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves

Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves

How to Cite

Verő, J. and Zieger, B. (1994) Upstream Waves and Field Line Resonances — Pulsation Research at the Nagycenk Observatory During Three Solar Cycles, in Solar Wind Sources of Magnetospheric Ultra-Low-Frequency Waves (eds M. J. Engebretson, K. Takahashi and M. Scholer), American Geophysical Union, Washington, D. C.. doi: 10.1029/GM081p0055

Author Information

  1. Geodetic and Geophysical Research Institute of the Hungarian Academy of Sciences, Sopron, Hungary

Publication History

  1. Published Online: 3 APR 2013
  2. Published Print: 1 JAN 1994

ISBN Information

Print ISBN: 9780875900407

Online ISBN: 9781118663943

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Keywords:

  • Magnetosphere;
  • Radio waves;
  • Solar wind

Summary

This chapter contains sections titled:

  • Historical Review