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High CNO abundance tailward flow, associated with a flux rope in the distant magnetotail: GEOTAIL observations

MPS-Authors
http://pubman.mpdl.mpg.de/cone/persons/resource/persons104294

Wilken,  B.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104317

Zong,  Q.-G.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons103876

Daglis,  I. A.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

http://pubman.mpdl.mpg.de/cone/persons/resource/persons104054

Livi,  S.
MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society;

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Citation

Wilken, B., Zong, Q.-G., Daglis, I. A., Pu, Z. Y., Livi, S., Yamamoto, T., et al. (1995). High CNO abundance tailward flow, associated with a flux rope in the distant magnetotail: GEOTAIL observations. Geophysical Research Letters, 22, 3267-3270.


Cite as: http://hdl.handle.net/11858/00-001M-0000-0014-D4E3-4
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