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  Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region

Bourdin, P.-A., Bingert, S., & Peter, H. (2013). Observationally driven 3D magnetohydrodynamics model of the solar corona above an active region. Astronomy and Astrophysics, 555: A123. doi:10.1051/0004-6361/201321185.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-0B69-9 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0015-0B6A-7
Genre: Journal Article

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 Creators:
Bourdin, Philippe-A.1, 2, Author              
Bingert, Sven1, Author              
Peter, Hardi1, 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              

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 MPIS_GROUPS: Sun and Heliosphere
 Abstract: -

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 Dates: 2013
 Publication Status: Published in print
 Pages: -
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201321185
BibTex Citekey: Bourdin:2013-073
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 555 Sequence Number: A123 Start / End Page: - Identifier: -