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WIND

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Wind ICME Catalogue

2005

ICME[1] start time (Shock) MO[2] start/end time FR/E[3] MO start/end time ICME end time B[4] Vsw[5] Vexp[6] H0[7]
1 2005 007  01/07 08:44  -- 007 01/07 14:23 F 008 07:12 008 01/08 07:12 17.35 535 -2 P - H0
2 2005 008  01/08 15:12  -- 008 01/08 20:51 F 009 17:45 009 01/09 17:45 8.65 461 13 P - H0
3 2005 016  01/16 09:27  Y 016 01/16 15:35 F 017 07:01 017 01/17 07:01 8.25 530 32 P - H0
4 2005 018  01/18 21:35  -- 019 01/19 00:28 F 020 02:24 020 01/20 02:24 11.82 818 158 P - H0
5 2005 021  01/21 16:58  Y 021 01/21 23:45 E 022 19:12 022 01/22 19:12 14.58 727 - P - H0
6 2005 047  02/16 10:33  -- 047 02/16 12:14 F 047 23:31 047 02/16 23:31 12.40 390 19 P - H0
7 2005 048  02/17 21:35  -- 049 02/18 14:52 E 050 08:23 050 02/19 08:23 5.94 538 - P - H0
8 2005 051  02/20 15:32  Y 051 02/20 20:23 F 053 07:11 053 02/22 07:11 5.40 409 40 P - H0
9 2005 135  05/15 02:10  Y 135 05/15 05:31 F 136 22:47 136 05/16 22:47 23.37 745 257 P - H0
10 2005 140  05/20 04:47  -- 140 05/20 09:35 F 142 02:23 142 05/22 02:23 8.93 427 52 P - H0
11 2005 163  06/12 06:57  Y 163 06/12 15:07 F 164 18:00 164 06/13 18:00 12.37 480 20 P - H0
12 2005 165  06/14 17:55  Y 166 06/15 05:08 F 167 08:23 167 06/16 08:23 9.06 484 32 P - H0
13 2005 191  07/10 02:42  Y 191 07/10 10:47 F 193 14:23 193 07/12 14:23 11.94 438 -8 P - H0
14 2005 198  07/17 14:52  -- 198 07/17 14:52 F 199 06:00 199 07/18 06:00 11.16 426 23 P - H0
15 2005 222  08/10 04:47  -- 222 08/10 06:14 F 222 13:26 222 08/10 13:26 8.12 447 26 P - H0
16 2005 304  10/31 02:23  -- 304 10/31 02:23 F 304 18:43 304 10/31 18:43 10.72 374 19 P - H0
[1] ICME = Interplanetary Coronal Mass Ejection
[2] MO = Magnetic Obstacle
[3] FR/E = Flux-Rope,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.
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. (accepted).
Citation for modeling. Nieves-Chinchilla, T., M. G. Linton, M. A. Hidalgo, A. Vourlidas, N. P. Savani, A. Szabo, C. Farrugia, W. Yu. Circular-cylindrical Flux-rope Analytical Model for Magnetic Clouds. The Astrophysical Journal, 823:27 (13pp), 2016 May 20. doi:10.3847/0004-637X/823/1/27., 1372.
OTHER REFERENCES
Hidalgo, M. A., J. J. Blanco, F. J. Alvarez, and T. Nieves-Chinchilla. 2011, J. Atmos. Sol. Terr. Phys.,73, 1372.
Lepping, R.P., Wu, C.-C., Berdichevsky, D.B., Szabo, A.: 2011, Solar Phys. 274, 345.
Richardson, I.G., Cane, H.V.: 2010, Solar Phys. 264, 189.

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