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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. 9.

Evolution of the quasi separatrix layers and flux ropes through the corona, where their radial height is shown as a function of the day of simulations taken in a cut through the center of the bipoles. The solid lines represent the flux ropes and the dashed lines, the quasi separatrix layers or quasi separators. The labeling is as follows: "T" marks the trailing bipole, "L" marks the lead bipole, "E" marks the external PIL, and "C" marks the initial coronal quasi separator.

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