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Comparison between the ionospheric plasma drift and the motion of artificially induced irregularities as observed by HF backscatter radars

MPS-Authors
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Oksman,  J.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Nielsen,  E.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Stubbe,  P.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Kopka,  H.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Hanuise, C., Hedberg, A., Oksman, J., Nielsen, E., Stubbe, P., & Kopka, H. (1986). Comparison between the ionospheric plasma drift and the motion of artificially induced irregularities as observed by HF backscatter radars. Annales Geophysicae, 4, 49.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-DDD6-D
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