Image Details

Choose export citation format:

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. 8.

Skew angle of the field vs. normalized distance along the PIL for the trailing bipole. The skew angle is calculated on day 3 (dotted line), day 10 (dashed line), day 15 (solid line), and day 25 (dash‐dotted line). In each case the skew is calculated from the southernmost point of the bipole to the northernmost point, where the normalized distance along the PIL is used, as on each day the length of the PIL changes.

Other Images in This Article

Show More

Copyright and Terms & Conditions