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WIND

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Wind ICME Catalogue

2004

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 2004 094  04/03 09:55  Y 095 04/04 01:11 F 096 19:11 096 04/05 19:11 15.86 431 64 P F H0
2 2004 204  07/22 09:45  Y 204 07/22 13:26 C 206 05:45 206 07/24 05:45 11.51 559 64 P - H0
3 2004 206  07/24 05:32  Y 206 07/24 07:12 F 207 14:38 207 07/25 17:45 20.44 564 32 P F H0
4 2004 207  07/25 17:45  -- 207 07/25 17:45 F 208 03:35 208 07/26 03:35 9.31 678 21 P F H0
5 2004 208  07/26 22:25  Y 209 07/27 01:12 C 209 23:59 209 07/27 23:59 16.97 962 270 P - H0
6 2004 242  08/29 09:09  Y 242 08/29 19:26 F 243 21:21 243 08/30 21:21 12.16 393 8 P F H0
7 2004 257  09/13 19:42  Y 258 09/14 17:59 E 259 14:23 259 09/15 14:23 6.35 557 28 P - H0
8 2004 261  09/17 20:52  -- 262 09/18 12:28 F 263 16:58 263 09/19 16:58 6.03 402 32 P F H0
9 2004 312  11/07 17:58  Y 312 11/07 22:46 F 314 09:21 314 11/09 09:21 16.23 640 60 P F H0
10 2004 314  11/09 18:25  Y 314 11/09 20:38 F 315 16:47 315 11/10 16:47 25.00 731 113 P F H0
11 2004 316  11/11 16:47  Y 317 11/12 08:35 F 318 09:35 318 11/13 09:35 6.95 552 65 P F H0
12 2004 345  12/10 04:47  -- 345 12/10 04:47 F 345 21:35 345 12/10 21:35 8.33 416 12 P F 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. UUnderstanding the Internal Magnetic field configuration of ICMEs using more than 20 years of Wind observations. Solar Physics. DOI: 10.1007/s11207-018-1247-z.
Citation for the fits. Nieves-Chinchilla, T., et al. Reconstruction of the near-Earth interplanetary coronal mass ejections during 1995-2015: Catalog of geometrical and physical properties. (to be submitted).
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.

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