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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 8.

(a) HMI magnetogram of the active region taken on 2011 August 4 at 03:36 UT. The two lines indicate the projections on the magnetogram of the two planes used to display the decay index. The white cubes indicate the reconstructed position of the filament on August 3 at 08:35 UT, while the black cubes highlight the reconstructed position of the filament on August 4 at 03:36 UT. (b) Plot of the decay index for the potential field extrapolation relative to the HMI magnetogram taken on August 3 at 06:00 UT. The decay index is plotted along the plane passing through line II of Figure (a), that is, along part of the axis of the reconstructed filament (white cubes). (c)–(d) Plot of the decay index for the potential field extrapolation relative to the HMI magnetogram from August 4 at 03:36 UT and along the planes passing through lines I and II of Figure (a). The white and black cubes highlight the three-dimensional position of the filament on August 3 at 21:36 UT and on August 4 at 03:36 UT, respectively.

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