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  Identification of prominence ejecta by the proton distribution function and magnetic fine structure in interplanetary coronal mass ejections in the inner heliosphere

Yao, S., Marsch, E., Tu, C., & Schwenn, R. (2010). Identification of prominence ejecta by the proton distribution function and magnetic fine structure in interplanetary coronal mass ejections in the inner heliosphere. Journal Geophysical Research, 115: A05103. doi:10.1029/2009JA014914.

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 Creators:
Yao, Shuo, Author
Marsch, Eckart1, 2, Author           
Tu, Chuanyi, Author
Schwenn, Rainer1, 2, Author           
Affiliations:
1MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              

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 MPIS_GROUPS: Sun and Heliosphere
 MPIS_PROJECTS: Helios
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 Dates: 2010
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: Peer
 Identifiers: DOI: 10.1029/2009JA014914
BibTex Citekey: Yao:2010-074
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Title: Journal Geophysical Research
Source Genre: Journal
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Pages: - Volume / Issue: 115 Sequence Number: A05103 Start / End Page: - Identifier: -