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The Double-bubble Coronal Mass Ejection of the 2020 December 14 Total Solar Eclipse

  • Authors: Benjamin Boe, Bryan Yamashiro, Miloslav Druckmüller, and Shadia Habbal

2021 The Astrophysical Journal Letters 914 L39.

  • Provider: AAS Journals

Caption: Figure 4.

MGN processed images from the 17.1 nm (Fe IX) bandpass of SDO/AIA (see Section 3.2). The field of view is identical to that of Figure 3. The bottom panels show traced magnetic field lines from a PFSS model overlaid on the MGN processed 14:00 UT 17.1 nm AIA image (left) and on the ADAPT synoptic magnetic field map (right). Each individual field line trace has a unique color, which is used in both panels. An associated animation of the the AIA data 17.1 nm from 12:00 UT to 16:58 UT on the day of the eclipse is available. The realtime duration of the video is 15 s.

(An animation of this figure is available.)

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

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