| NN | date | SW geoeffective structure | in short | RH/LH | MC type | CME | EIT signature | EIT time, location | comment | |
| 1 | 1996 10 23 | |||||||||
| 2 | 1997 4 22 | ICME, no shock, MC | ICME | RH | SWN | 16/04 07:35PH | D, W? | 14:36 S18E08 | source questionable. One has a choice between a PH with no EIT signatures (seems to be possible as the CME is very slow) and a good EIT dimming not associated with any detected CME. EIT data gap afterwards, so dimming is seen only in one frame | |
| 3 | 1997 5 15 | close to HCS ahead of MC 2nd ICME? intern+ extern | ICME | LH | SEN | 12/05 06:30H | D, W, A | 04:50 N21W08 | ||
| 4 | 1997 10 11 | intern to mixed | ICME | RH | ESW | 06/10 15:28PH | F, D, A, L | 12:13 S52E16 | ||
| 5 | 1997 11 7 | ICME extern+ intern | ICME | RH | SWN | 11/04 06:10H | D, W, A | 05:57 S17W33 | ||
| 6 | 1997 11 23 | ICME intern+ extern | ICME | RH | ESW | 17/11 08:27H | D, W? | 03:51 N35E50 | source questionable as this CME should probably have arrived earlier. Halo 19.11 probably backsided | |
| 7 | 1998 2 18 | ICME intern | ICME | RH | ESW | 14/02 06:55PH | D | 09:51 S40E20 | source questionable. One has a choice between a PH with VERY weak EIT signatures (seems to be possible as the CME is very slow) and a good EIT dimming not associated with any detected CME | |
| 8 | 1998 3 10 | CH S; short BDE interval though | CIR/CH | CH | 07/03 S30E04 | southern polar CH with its low-latitude extensions | ||||
| 9 | 1998 5 2 | [shock, ICME, MC; internal] | ICME | RH | ESW | 29/04 16:58H | D, W, A | 16:18 S16E21 | compound with the next CME | |
| 1998 5 3 | ICME internal, tail of the previous ICME + probably external of another ICME after the shock | ICME | 01/05 23:40H | D, W, A | 22:39 S19W04 | compound with the previous and the next CMEs | ||||
| 1998 5 4 | no MC extern [not a shock, but a large forward-travelling wave?] | MICME | 02/05 05:31H | D, W, A | 04:53 S20W08 | compound with the previous and the next CMEs. MAY 2-5 IS A COMPOUND EVENT; IT IS NOT EASY TO SEPARATE THE CONTRIBUTIONS OF SEVERAL HALO CMES | ||||
| 1998 5 5 | the same MICME as previous, MC 5/05 | MICME | RH | SWN | 02/05 14:06H | D, W, A, F? | 13:40 S15W16 | compound with the previous CME | ||
| 10 | 1998 6 26 | MICME 2 MC internal | MICME | LH both | SEN, WSE | EIT bakeout | ||||
| 11 | 1998 8 6 | probably no cloud extern intern ICME/CIR see next day | ICME/CIR | SOHO loss | ||||||
| 12 | 1998 8 7 | see previous, CH S | CIR/CH | SOHO loss | ||||||
| 13 | 1998 8 27 | shock ICME CIR - pushed; probably no MC; ICME extern + intern; CH N | ICME/CIR | SOHO loss | ||||||
| 14 | 1998 9 25 | shock, ICME external | ICME | LH | ENW | SOHO loss | ||||
| 15 | 1998 10 19 | ICME exetrnal + internal | ICME | LH | WSE | 15/10 10:04H | F, A, D? | 02:11 N12E10 | extended source | |
| 16 | 1998 11 7 | ICME external sheath internal | ICME | LH | SEN | 04/11 04:18H | D, W?, A | 03:22 N10E03 | compound with the next CME | |
| 1998 11 8 | MICME (consisting of the previous and next ICMEs), shock of the 2nd CME ploughs into the 1st one! | MICME | This is a compound ICME, and it's not very clear how many ICMEs are interacting. Peak of the storm on 08/11 is produced by the INTERACTION of ICMEs. The situation on the Sun is also complicated. Two CMEs are tentatively identified. | |||||||
| 17 | 1998 11 9 | MC intern ICME | ICME | RH | ESW | 05/11 20:44H | D, A | 20:42 N19W30 | compound with the previous CME | |
| 18 | 1998 11 13 | ICME overexpanding MC! intern extern | ICME | RH | ESW | 09/11 17:54PH | D, F, A, W? | 16:48 N19W05 | ||
| 19 | 1999 1 14 | forward shock; CH N; MC? external + internal? | ICME/CIR | SOHO ''vacations'' | ||||||
| 20 | 1999 2 18 | MC in By; int + ext | ICME | RH | ESW | No SOHO data | ||||
| 21 | 1999 9 23 | 3 shocks? 1st assoc. with sector change - MICME devours CIR. 3 ICMEs? Last - MC; int | MICME | RH | SWN | |||||
| 22 | 1999 10 22 | fast and slow forward shocks; overexpanding ICME ahead of CIR, compr from both sides MC ext; CH N, no sector change | ICME/CIR | LH in Bz | NWS | U17/11 23:50PH . | D, F?, A; D, A?; CH 20/10 | 23:11 S28E11 N05E37 N17E21 | Unreported PH CME with apparently two source regions erupting simultaneously. The CME is interacting with the following fast flow from a CH | |
| 23 | 1999 11 13 | ICME, then shock + ICME; no MC | MICME | |||||||
| 24 | 2000 2 12 | shock, following ICME is scratched; external | ICME | |||||||
| 25 | 2000 4 7 | shock, ICME, no MC? [external] | ICME | |||||||
| 26 | 2000 5 24 | ICME? MC? in By 25/05, intern+extern. Hot and very wide sheath? No shock?! Or MICME? | MICME? | RH | ESW | |||||
| 27 | 2000 7 16 | Bastille day event, shock, ICME, MC, extern + intern | ICME | LH | SEN | |||||
| 28 | 2000 8 11 | shock? wide sheath, ICME, no MC; internal (mostly) + external | ICME | 06/08 18:30PH 23:06PH | F?, D, A? | 05/08 22:23 N33W23 | source questionable. One has a choice between PHs with no EIT signatures (seems to be possible as the first CME is very slow) and a good EIT dimming not associated with any detected CME. | |||
| 29 | 2000 8 12 | shock, ICME, MC, internal. Very good example | ICME | LH | SEN | |||||
| 30 | 2000 9 18 | multiple (?) ICME external, no MC | ICME | |||||||
| 31 | 2000 10 3 | shock 0h 3/10, ICME, extern + intern | ICME | |||||||
| 2000 10 4 | another shock?? (15h 3/10) with another ICME, compound with previous and mostly NEXT, internal, MC | MICME | RH in By, Bz | NES | ||||||
| 2000 10 5 | shock, ICME is scratched, mostly external | ICME | ||||||||
| 32 | 2000 10 13 | shock, ICME, external, MC internal | ICME | RH in Bz | NES | |||||
| 33 | 2000 10 29 | ICME, corresponding shock - 18h 28/10; no MC? internal | ICME | LH?? | SEN?? | |||||
| 34 | 2000 11 6 | shock, ICME, extern + intern, MC | ICME | LH | SEN | |||||
| 35 | 2000 11 29 | shocks (beg. 28/11, two more beg. 29/11) - multiple ICME?, extended sheath, no MC, mostly external, then internal | MICME | |||||||
| 36 | 2001 3 20 | shock, ICME, extern + intern, MC | ICME | LH in By | WSE | |||||
| 37 | 2001 3 31 | shock, compound hot ICME, no MC; then another shock (see next) | MICME | |||||||
| 2001 4 1 | ICME after the 2nd shock of the previous day, internal; MC? | ICME | LH? | SEN? | ||||||
| 38 | 2001 4 12 | shock, ICME, external, no MC???!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!?!? | ICME | RH in Bz? | SWN? | |||||
| 39 | 2001 4 18 | shock, ICME, no MC, external | ICME | |||||||
| 40 | 2001 4 22 | shock, ICME, MC, internal | ICME | LH in By | WSE | |||||
| 41 | 2001 8 17 | shock, ICME, scratched MC? | ICME | RH in Bz? | SWN? | |||||
| 42 | 2001 9 26 | shock, ICME external, no ICME body? | ICME | |||||||
| 43 | 2001 9 29 | shock, ICME, MC, external + internal | ICME | LH in By | WSE | |||||
| 2001 10 1 | shock end of 30/09, ICME, MC, internal. Compound with previous? | ICME | RH in By | ESW | ||||||
| 44 | 2001 10 3 | shock end of 01/10, then 2 ICMEs, 2nd - toroidal MC | MICME | LH in Bz | NWS | |||||
| 45 | 2001 10 21 | shock, ICME, MC?, external +internal | ICME | LH in By? | WSE? | |||||
| 46 | 2001 10 28 | shock, long sheath, ICME body 30-31/10, no MC, external | ICME | |||||||
| 47 | 2001 11 5 | discontinuity around noon, ICME compound with next ICME, no MC. Bad data | MICME | |||||||
| 2001 11 6 | another shock? ICME compound with previous ICME, no MC? Bad data | MICME | ||||||||
| 48 | 2001 11 24 | shock, ICME, no MC, external | ICME | |||||||
| 49 | 2002 3 24 | shock (several ones), MICME, one of them - MC? A complicated multiple ICME event (interacting with a fast flow on 26/03). At least two ICMEs. | MICME | RH in Bz? | SWN? | 20/03 17:54H | D, A | 17:24 S22W17 | Interacts with (one of) the following CME(s) | |
| 20/03 23:54PH | L, D, A? | 23:12 S28W57 | Not sure if involved? But could have produced at least a shock | |||||||
| No CME reported | D, F?, A? | 21/03 18:12 S36W02 | Probably not involved? | |||||||
| 22/03 11:06H | L, D, A?, P?, W? | 10:36 S19W90 | The CME is not directed towards the Earth, but its shock could have arrived | |||||||
| 50 | 2002 4 18 | shock, sheath, ICME, MC, external plus internal | ICME | RH in Bz | SWN | 15/04 03:50H | D, A | 03:00 S16W04 | ||
| 51 | 2002 4 20 | shock, sheath, then another shock?, then ICME, MC (20-21/04) or just one ICME with a shock? external + internal | MICME? | LH in Bz? | SEN? | 17/04 08:26H | D, W, A | 07:48 S13W35 | Not clear how many ICMEs. | |
| 52 | 2002 5 11 | |||||||||
| 53 | 2002 5 23 | shock, sheath, ICME? MC? Or external only? Or interacting ICMEs? | ICME | LH in Bz? | SEN? | 21/05 21:50PH | D, W?, A | 21:24 N18E40 | The least probable source? Not sure if involved. | |
| 22/05 00:06PH | D, W, A, L | 21/05 23:36 S21W68 | Not sure if involved? | |||||||
| 22/05 03:50H | F, D, W, A, L | 02:48 S19W62 | The most probable source; dimmings are quite extended. May interact with (one of) the previous CME(s). | |||||||
| 54 | 2002 8 1 | 2 shocks, 2 ICMEs, 2 interacting MCs, 2nd ICME may be longer, in both cases external + internal | MICME | RH in Bz | SWN | U29/07 03:30 | D | 02:59 S19W19 | Compound with the next CME | |
| 2002 8 2 | LH in Bz | NWS | 29/07 12:07PH | D . F?, D | 12:00 S02W09 12:00 N35W33 | Compound with the previous CME. Source region is not clear because of LASCO and EIT data gap of 1 hour. | ||||
| 55 | 2002 8 18 | |||||||||
| 2002 8 19 | ||||||||||
| 2002 8 20 | ||||||||||
| 2002 8 21 | ||||||||||
| 56 | 2002 9 4 | ICME (MC?), no shock, then faster wind that pushes the ICME; sector change. External. CH N | ICME/CIR | LH in By? | ENW? | U29/08 15:06PH? . | D CH 31/08 | 13:47 S04W24 S15W05 | Source questionable. No clear halo CME is associated with this eruption, although a lot of continuous inhomogeneous outflow in a large range of PA is present. | |
| 57 | 2002 9 8 | shock, sheath, ICME, no MC, external | ICME | 05/09 16:54H | D, F, W, A | 16:23 N12E28 | ||||
| 58 | 2002 10 1 | shock, ICME, MC, external + internal | ICME | RH in Bz | NES | 26/09 01:31PH | D | 25/09 23:59 N23W34 | A somewhat questionable source as there are several similar eruptions in the same AR. Maybe this corresponds to somewhat turbulent morphology of the ICME. | |
| 59 | 2002 10 4 | shock, ICME, MC, internal | ICME | RH in By | ESW | U29/09 23:54PH | F, D, A | 23:11 S18W11 | A non-local eruption probably leading to an unreported PH. | |
| 60 | 2002 10 7 | CH N polarity | CIR/CH | |||||||
| 61 | 2002 10 14 | |||||||||
| 62 | 2002 11 20 | CIR/CH | ||||||||
| 2002 11 21 | ||||||||||
| 2002 11 22 | ||||||||||
| 63 | 2003 5 30 | |||||||||
| 64 | 2003 6 18 | |||||||||
| 65 | 2003 7 12 | |||||||||
| 66 | 2003 7 16 | |||||||||
| 67 | 2003 8 18 | |||||||||
| 68 | 2003 10 29 | shock, sheath, ICME, MC | ICME | LH | WSE | 28/10 10:54H | D, W, F, A, L | 11:11 S17E08 | Compound with the next event? | |
| 69 | 2003 10 30 | shock, sheath, ICME, MC? | ICME | LH? | NWS? | 29/10 20:54H | D, W, A, L | 20:48 S19W05 | Compound with the previous event? | |
| 70 | 2003 11 20 | shock, ICME, MC | ICME | RH | ESW | 18:11 08:50H | D, W, A, F? | 07:35 S02E17 | ||
| 71 | 2004 1 22 | |||||||||
| 72 | 2004 2 11 | |||||||||
| 73 | 2004 4 4 | |||||||||
| 74 | 2004 7 23 | |||||||||
| 75 | 2004 7 25 | |||||||||
| 76 | 2004 7 27 | |||||||||
| 77 | 2004 8 30 | |||||||||
| 78 | 2004 11 08 | Three shocks 07/11, MICME, MC | MICME | LH | SEN | 03/11 16:06H | D, W, A, L | 15:46 N08E39 | Compound ICMEs. Three shocks correspond to three halo CMEs? The third halo CME is compound: it is produced by two eruptions. | |
| 04/11 09:54PH | D, W, A | 08:46 N09E29 | ||||||||
| 04/11 23:30PH | D, W, A . D, W, A | 21:57 N09E22 23:09 N08E18 | ||||||||
| 79 | 2004 11 10 | Two shocks 09/11, MICME, MC | MICME | LH? | NWS? | 06/11 01:31PH | D, W, A | 00:23 N10E05 | Compound ICMEs. Two shocks correspond to two halo CMEs? The first halo may be compound as well. | |
| 07/11 17:06H | D, W, A, F, L | 15:58 N09W16 | ||||||||