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  Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and Its Surroundings

Tadesse, T., Wiegelmann, T., Inhester, B., & Pevtsov, A. (2012). Coronal Magnetic Field Structure and Evolution for Flaring AR 11117 and Its Surroundings. Solar Physics, 281, 53-65. doi:10.1007/s11207-012-9961-4.

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Tadesse, Tilaye1, 2, Author              
Wiegelmann, T.1, Author              
Inhester, B.1, 3, Author              
Pevtsov, A., Author
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
2IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
3MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832291              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2012
 Publication Status: Published in print
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 Rev. Type: Peer
 Identifiers: DOI: 10.1007/s11207-012-9961-4
BibTex Citekey: Tadesse:2012-114
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Title: Solar Physics
Source Genre: Journal
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Pages: - Volume / Issue: 281 Sequence Number: - Start / End Page: 53 - 65 Identifier: -