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

Tadesse, Tilaye; Wiegelmann, T.; Inhester, B.; Pevtsov, A.

doi:10.1007/s11207-012-9961-4

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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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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-095F-2 Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0015-0960-B

Genre: Journal Article

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Creators:
Tadesse, Tilaye^{1, 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: Date issued: 2012

Publication Status: Issued

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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: -