List of shock-driving ICMEs during the solar cycle 23 (E15° ≤ source longitude ≤ W15°).
Selected from the list in Gopalswamy et al. 2010.

MC = Magnetic cloud;
EJ = Ejecta;
+/- = Fluxrope found/not found (Katsuhide Marubashi, links to plots in the first column)

Direction parameter of CME. Asterisk marks updated value. (Roksoon Kim)

Flare Class: EP = Eruptive prominence; BP = Bright point; DIM = Dimming

0 = No metric emission; 1 = Metric emission

0 = No DH radio emission; 1 = In RAD2 (1-14 MHz); 2 = In RAD1 (30 kHz - 1 MHz); 3 = In RAD1+RAD2

Solid vertical line = shock; Dashed vertical lines = ICME; Horizontal lines = threshold levels of 0.8 (O+7/O+6) and 12 (QFe); 1-hour time resolution. (Alysha Reinard)

Comments: (SS = Solar Source)
1 = Wind/WAVES type II date is one day after the CME date.
2 = Possible radio emission; association with this shock has less confidence.
3 = Wind/WAVES type II date is two days after the CME date.
4 = CME association has less confidence, i.e., other possible candidate CMEs exit.
5 = CME width is uncertain due to the compound CME.
6 = Ejecta identification has less confidence.
7 = Clear radio emission but may not be associated with this shock.
8 = Possible complex event. MC onset after >24 hours from the shock.
9 = Possible short ejecta (1-2 hours) after 24 hours of the shock, which may not be associated with this event.
10 = Shock identification has less confidence.