Fig. 3.
Panels a–c: graduated cylindrical shell (GCS) reconstruction of the CME body. Coronagraph images from: (a) STEREO B/COR 2, (b) SOHO/LASCO C3, and (c) STEREO A/COR 2 at roughly the same time (September 28, 2012 at 01:24 UT). Panels d and e: CME modelled by EUHFORIA. (d) Propagation of the modelled cone CME in the ecliptic and meridional perspectives. (e) CME speeds at the cone surface as seen from Earth. The grey sphere shows the solar wind radial velocity at the inner boundary of EUHFORIA (0.1 AU).
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