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| Paper: |
Understanding the Differences in Three Consecutive Large Flares |
| Volume: |
456, The Fifth Hinode Science Meeting |
| Page: |
61 |
| Authors: |
Tarr, L.; Longcope, D. |
| Abstract: |
The active region NOAA 11158 produced three large flares over a 31 hour interval centered on 14 Feb. 2011. The flare ribbons observed in 1600Å AIA images reveal very different characters between the three. We use a model of the coronal magnetic field topology and its evolution to explain the differences in structures and energies of these three flares. |
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