Cluster Observations Showing the Indication of the Formation of a 
Modified-Two-Stream Instability in the Geomagnetic Tail

Mühlbachler, S.; Langmayr, D.; Lui, A. T. Y.; Erkaev, N. V.; Alexeev, I. V.; Daly, P. W.; Biernat, H. K.

doi:10.1016/j.asr.2009.01.012

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Cluster Observations Showing the Indication of the Formation of a Modified-Two-Stream Instability in the Geomagnetic Tail

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Mühlbachler, S.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;

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Daly, P. W.
Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society;
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Mühlbachler, S., Langmayr, D., Lui, A. T. Y., Erkaev, N. V., Alexeev, I. V., Daly, P. W., et al. (2009). Cluster Observations Showing the Indication of the Formation of a Modified-Two-Stream Instability in the Geomagnetic Tail. Advances in Space Research, 43(10), 1588-1593. doi:10.1016/j.asr.2009.01.012.

Cite as: https://hdl.handle.net/11858/00-001M-0000-0015-0023-0

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