Figure 3 from Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling

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Quasi-periodic Counter-propagating Fast Magnetosonic Wave Trains from Neighboring Flares: SDO/AIA Observations and 3D MHD Modeling

Authors: Leon Ofman and Wei Liu

2018 The Astrophysical Journal 860 54.

Provider: AAS Journals

Caption: Figure 3.

Online animated figure of SDO/AIA 171 Å images (rotated with the solar west up) showing transverse oscillations of trans-equatorial coronal loops associated with the eruptions and QFP wave trains. The most evident oscillating loop is marked with an arrow. The animation runs from 13:30 to 14:20 UT on 2013 May 22.

(An animation of this figure is available.)

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

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