Fig. 1.

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Composite image of the solar corona on August 3, 2012, at 04:17 UT spanning from the solar disk center to the extended corona up to approximately 6 R⊙ (created using JHelioviewer; Müller et al. 2017). The running difference image from the SOHO/LASCO C2 white-light coronagraph shows a narrow CME (green arrow) propagating northeast, accompanied by the boundary of the spheroidal shock wave driven by the CME (red arrows). The inner image captured in the 304 Å passband by the SDO/AIA instrument depicts the earlier evolution of the CME. The blue circle marks the origin of the jetlike eruption on the Sun's surface.
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