Notes. The location of the eruption on the Sun surface is given in Cols. 5 and 6 in Stonyhurst heliographic coordinates, with the mean latitude ⟨HGLT⟩ and mean longitude ⟨HGLN⟩ in degrees. In this system of coordinates, the zero point is set at the intersection of the Sun’s equator and its central meridian as seen from the Earth, which allows us to have a more accurate idea of the direction of a CME, compared to the direction of the Earth. Thus, we classified CMEs in three categories on Col. 7: on disc, far side, and limb, depending on the longitude of the CME. Between −90 and +90, the eruption occurs on the visible surface of the Sun, and therefore noted on disc. On the opposite side. The class of the associated soft X-ray flare measured by GOES is given for CME events originating on the disc, and the availability of the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI; Lin et al. 2002) data for the hard X-ray flux is listed as ‘complete’, ‘OK’, or ‘incomplete’ depending on the quality of the data. Finally, the number of sunspots on the solar surface the day of the event is given to provide a reference of the solar activity.

^( * )Events which suffer from the lack of 3D tracking during the acceleration phase.