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Observational Evidence of Torus Instability as Trigger Mechanism for Coronal Mass Ejections: The 2011 August 4 Filament Eruption

  • Authors: F. P. Zuccarello, D. B. Seaton, M. Mierla, S. Poedts, L. A. Rachmeler, P. Romano, and F. Zuccarello

Zuccarello et al. 2014 The Astrophysical Journal 785 88.

  • Provider: AAS Journals

Caption: Figure 3.

HMI magnetogram of the active region obtained on 2011 August 3 at 00:00 UT. The three squares indicate the three different regions discussed in the text. Region C is the region that includes the complete sunspot group. Region A is a zoom into the northern sunspot, while Region A2 is a zoom into the locations where the footpoints of the two filaments cross each other. The x and y scales are in image pixels. North is at the top and west to the right.

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