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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 2.

Running difference SDO/AIA 171 Å images on 2013 May 22 rotated with the solar west up showing (a) outward-propagating QFPs from the primary flare and (b) counter-propagating QFPs (apparently along trans-equatorial loops) from the primary flare on the left and the secondary flare on the right. (An animation of this figure showing the running difference images from 12:40 to 14:20 UT is available online.)

(An animation of this figure is available.)

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

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