Image Details

Choose export citation format:

The Giant Eruption in Solar Cycle 25 Caused by Collisional Shearing

  • Authors: Tao Ding, Jun Zhang, Yijun Hou

Tao Ding et al 2025 The Astrophysical Journal Letters 985 .

  • Provider: AAS Journals

Caption: Figure 3.

Onset and eruption of the flux ropes. Panels (a1)–(a5): the SDO/AIA EUV data. Panel (a6): a time-distance plot along “S1” in panel (a4) displaying the eruption of FR1 and FR2. The white box in panel (a1) marks a brightening. The cyan dotted lines in panels (a2)–(a5) and the green ones in panels (a2) and (a4)–(a5) denote FR1 and FR2, separately. The red and blue closed curves in panels (a4) and (a5) (denoting the emerging dipole in Figure 2(c1)) are the contours of the SDO/HMI LOS magnetogram (11:34:15 UT) at +150 G and −400 G, respectively. To display the eruption process, an animation of the AIA 131 Å, 304 Å, 211 Å, and 193 Å observations from 2024 October 3 12:05 UT to 12:15 UT is available, with a duration of 5 s.

(An animation of this figure is available in the online article.)

(An animation of this figure is available.)

The video/animation of this figure is available in the online journal.

Other Images in This Article
Copyright and Terms & Conditions

Additional terms of reuse