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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. 13.

The r‐component of the Lorentz force (solid line), pressure force (dotted line), and tension force (dashed line) vs. radial height at a longitude of ﹩\phi =41^{\circ }﹩ at the midpoint of the trailing bipole on day 21. The vertical dash‐dotted lines denote the radial height of the QSL (﹩r=1.09﹩ R) and the axis of the flux rope (﹩r=1.28﹩ R)

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