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WIND

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Wind ICME Catalogue

2015

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 2015 007  01/07 05:38  Y 007 01/07 06:28 F 007 21:07 007 01/07 21:07 17.58 450 18 P F H0
2 2015 087  03/28 03:36  -- 087 03/28 11:45 F 088 14:24 088 03/29 14:24 12.03 392 41 P F H0
3 2015 090  03/31 07:32  Y 090 03/31 17:57 F 091 09:50 091 04/01 09:50 12.35 406 1 P F H0
4 2015 099  04/09 09:09  Y 099 04/09 23:02 C 101 09:36 101 04/11 09:36 15.24 391 39 P - H0
5 2015 126  05/06 00:56  Y 126 05/06 16:48 F 127 14:23 127 05/07 14:23 12.89 422 18 P F H0
6 2015 128  05/08 02:52  -- 128 05/08 07:11 F 129 10:34 129 05/09 10:34 6.52 382 -9 P F H0
7 2015 130  05/10 08:23  -- 130 05/10 11:59 F 131 04:47 131 05/11 04:47 11.03 358 19 P F H0
8 2015 173  06/22 18:07  Y 174 06/23 02:23 C 175 13:03 175 06/24 13:03 10.67 598 - P - H0
9 2015 250  09/07 13:05  Y 250 09/07 23:31 F 252 14:52 252 09/09 14:52 14.73 468 83 P F H0
10 2015 279  10/06 21:35  -- 279 10/06 21:35 F 280 10:04 280 10/07 10:04 14.52 424 -40 P F H0
11 2015 297  10/24 17:59  Y 298 10/25 13:11 F 301 13:11 301 10/28 13:28 5.61 391 83 P F H0
12 2015 310  11/06 17:46  Y 311 11/07 07:11 F 312 16:47 312 11/08 16:47 15.68 530 65 P F H0
13 2015 353  12/19 15:35  Y 354 12/20 13:40 F 355 23:02 355 12/21 23:02 15.68 397 15 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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