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  Three-dimensional magnetic field topology in a region of solar coronal heating

Solanki, S. K., Lagg, A., Woch, J., Krupp, N., & Collados, M. (2003). Three-dimensional magnetic field topology in a region of solar coronal heating. Nature, 425, 692-695. doi:10.1038/nature02035.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-EE43-7 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0014-EE44-5
Genre: Journal Article

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 Creators:
Solanki, S. K.1, 2, Author              
Lagg, A.1, 2, Author              
Woch, J.1, Author              
Krupp, N.2, 3, Author              
Collados, M., Author
Affiliations:
1Department Sun and Heliosphere, Max Planck Institute for Solar System Research, Max Planck Society, escidoc:1832289              
2MPI for Aeronomy, Max Planck Institute for Solar System Research, Max Planck Society, escidoc:1832291              
3Department Planets and Comets, Max Planck Institute for Solar System Research, Max Planck Society, escidoc:1832288              

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 MPIS_GROUPS: Sun and Heliosphere
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 Dates: 2003
 Publication Status: Published in print
 Pages: -
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 Rev. Method: Peer
 Identifiers: DOI: 10.1038/nature02035
BibTex Citekey: Solanki:2003-082
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Title: Nature
Source Genre: Journal
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Pages: - Volume / Issue: 425 Sequence Number: - Start / End Page: 692 - 695 Identifier: -