Color-inverted and cropped observations of emission from the 30.4 nm (He II) bandpass of SDO/AIA and STEREO-A/SECCHI. STEREO-A was 57° behind the Earth view on the day of the eclipse. The data are flattened to enhance the faint emission in the corona relative to the bright emission in the chromosphere. An animation of the the AIA 30.4 nm data from 0:00 to 19:30 UT on the day of the eclipse is available. The realtime duration of the video is 19 s. Arrows point to specific structures discussed in Section 3.2.

(An animation of this figure is available.)

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