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WIND

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Wind ICME Catalogue

Solar Cycle 22

ICME[1] start time (Shock) MO[2] start time FR/E[3] MO end time ICME end time B[4] Vsw[5] Vexp[6] HO
0 1995 038  02/07 19:11  -- 039 02/08 03:21 (FR) 041 21:36 041 02/10 21:36 8.32 377 52 P
1 1995 063  03/04 00:36  Y 063 03/04 11:23 (FR) 064 03:07 064 03/05 03:07 10.86 443 10 P
2 1995 065  03/06 02:11  -- 065 03/06 07:11 (E) 066 02:23 066 03/07 02:23 15.68 529 65 P
3 1995 093  04/03 06:43  -- 093 04/03 06:43 (FR) 094 13:26 094 04/04 13:26 8.83 301 39 P
4 1995 095  04/05 07:11  -- 095 04/05 17:59 (FR) 096 17:16 096 04/06 17:16 7.29 332 -1 P
5 1995 133  05/13 10:19  -- 133 05/13 10:19 (E) 133 16:00 133 05/13 16:00 15.68 529 65 P
6 1995 181  06/30 09:21  -- 181 06/30 14:23 (FR) 183 16:47 183 07/02 16:47 8.58 397 82 P
7 1995 234  08/22 12:56  Y 234 08/22 22:19 (FR) 235 18:43 235 08/23 18:43 9.71 359 16 P
8 1995 269  09/26 15:57  -- 270 09/27 04:33 (FR) 270 21:21 270 09/27 21:21 9.97 376 -34 P
9 1995 291  10/18 10:40  Y 291 10/18 19:11 (FR) 293 02:23 293 10/20 02:23 21.15 407 4 P
10 1995 349  12/15 14:52  -- 350 12/16 07:11 (FR) 350 19:11 350 12/16 19:11 11.03 396 4 P
11 1996 046  02/15 15:07  -- 046 02/15 15:07 (FR) 047 08:59 047 02/16 08:59 6.87 386 23 P
12 1996 095  04/04 11:59  -- 095 04/04 11:59 (FR) 095 21:36 095 04/04 21:36 7.34 388 6 P
13 1996 137  05/16 22:47  -- 138 05/17 01:36 (FR) 138 11:59 138 05/17 11:59 7.08 419 8 P
14 1996 148  05/27 14:45  -- 148 05/27 14:45 (FR) 150 02:23 150 05/29 02:23 9.73 368 28 P
[1] ICME = Interplanetary Coronal Mass Ejection
[2] MO = Magnetic Obstacle
[3] FR = Flux-Rope; E = Ejecta
[4] B = Mean magnetic field magnitude value in the MO interval.
[5] Vsw = Mean Solar Wind Bulk velocity in the MO interval.
[6] Vexp = Expansion velocity in the MO interval.
[7] HO = Heliopheric Overview (NOTE: CME start time is estimated based on the in-situ average solar wind speed. Cygnets will probably differ by days from the actual CME start time. Users will need to adjust the start time manually.).
REFERENCES
Citation for the catalogue. Nieves-Chinchilla, T., A. Vourlidas, et al. Understanding the Internal Magnetic Field Configurations of ICMEs using 20+ years of Wind Observations. (To be submited).

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