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  A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum

Ruan, P., Wiegelmann, T., Inhester, B., Neukirch, T., Solanki, S. K., & Feng, L. (2008). A first step in reconstructing the solar corona self-consistently with a magnetohydrostatic model during solar activity minimum. Astronomy and Astrophysics, 481, 827-834. doi:10.1051/0004-6361:20078834.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-FF10-E Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0014-FF11-C
Genre: Journal Article

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 Creators:
Ruan, P.1, Author           
Wiegelmann, T.2, Author           
Inhester, B.2, 3, Author           
Neukirch, T., Author
Solanki, S. K.2, 3, Author           
Feng, L.1, 2, Author           
Affiliations:
1IMPRS on Physical Processes in the Solar System and Beyond, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832290              
2Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832289              
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: 2008
 Publication Status: Issued
 Pages: -
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 Rev. Type: Peer
 Identifiers: DOI: 10.1051/0004-6361:20078834
BibTex Citekey: Ruan:2008-064
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 481 Sequence Number: - Start / End Page: 827 - 834 Identifier: -