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Differences in the O7+ /O6+ ratio of magnetic cloud and non-cloud coronal mass ejections

MPS-Authors
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Woch,  J.
Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society;

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

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

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Schwenn,  R.
Department Sun and Heliosphere, 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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Citation

Henke, T., Woch, J., Mall, U., Livi, S., Wilken, B., Schwenn, R., et al. (1998). Differences in the O7+ /O6+ ratio of magnetic cloud and non-cloud coronal mass ejections. Geophysical Research Letters, 25, 3465-3468.


Cite as: https://hdl.handle.net/11858/00-001M-0000-0014-D9AC-F
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