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

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.

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 Creators:
Henke, T., Author
Woch, J.1, Author           
Mall, U.2, 3, Author           
Livi, S.2, Author           
Wilken, B.2, Author           
Schwenn, R.1, 2, Author           
Gloeckler, G., Author
von Steiger, R., Author
Forsyth, R. J., Author
Balogh, A., Author
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
3Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832288              

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Free keywords: -
 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: ULYSSES: SWICS
 MPIS_PROJECTS: SOHO
 Abstract: -

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 Dates: 1998
 Publication Status: Issued
 Pages: -
 Publishing info: -
 Table of Contents: -
 Rev. Type: Peer
 Identifiers: BibTex Citekey: Henke:1998-067
 Degree: -

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Title: Geophysical Research Letters
Source Genre: Journal
 Creator(s):
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Publ. Info: -
Pages: - Volume / Issue: 25 Sequence Number: - Start / End Page: 3465 - 3468 Identifier: -