Fig. 5 from Models of the Large‐Scale Corona. I. Formation, Evolution, and Liftoff of Magnetic Flux Ropes

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Models of the Large‐Scale Corona. I. Formation, Evolution, and Liftoff of Magnetic Flux Ropes

Authors: D. H. Mackay and A. A. van Ballegooijen

Mackay & van Ballegooijen 2006 The Astrophysical Journal 641 577.

Provider: AAS Journals

Caption: Fig. 5.

Images of the large‐scale coronal field on (a) day 18 and (b) day 40. Strongly sheared field lines representing the axis of a flux rope can be seen on (a) the internal PIL and (b) the external PIL. Besides the strongly sheared field lines, there are also weakly sheared overlying coronal arcades.

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