Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind - Université Toulouse III - Paul Sabatier - Toulouse INP Accéder directement au contenu
Article Dans Une Revue Solar Physics Année : 2012

Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind

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hal-02863282 , version 1 (10-06-2020)

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L. van Driel-Gesztelyi, J. Culhane, D. Baker, P. Démoulin, C. Mandrini, et al.. Magnetic Topology of Active Regions and Coronal Holes: Implications for Coronal Outflows and the Solar Wind. Solar Physics, 2012, 281 (1), pp.237-262. ⟨10.1007/s11207-012-0076-8⟩. ⟨hal-02863282⟩
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