Goddard Space Flight Center
Wind_Banner_1.jpg

WIND

Two Columns

Filter table:
None
Shock events only
Flux-rope only
Ejecta only
Text filter:

Wind ICME Catalogue

1999

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 1999 022  01/22 20:21  Y 022 01/22 20:21 E 023 14:59 023 01/23 14:59 16.07 610 - P - H0
2 1999 042  02/11 17:41  -- 042 02/11 17:41 F 043 03:35 043 02/12 03:35 19.18 442 -7 P F H0
3 1999 049  02/18 02:48  Y 049 02/18 09:14 E 050 00:00 050 02/19 00:00 15.23 658 2 P - H0
4 1999 148  05/28 21:50  -- 148 05/28 21:50 C 150 10:47 150 05/30 10:47 6.73 397 15 P - H0
5 1999 183  07/02 00:27  Y 184 07/03 08:09 F 186 13:14 186 07/05 13:14 4.42 457 86 P F H0
6 1999 187  07/06 14:23  Y 187 07/06 19:12 C 188 16:47 188 07/07 16:47 7.20 463 -9 P - H0
7 1999 218  08/06 01:55  -- 218 08/06 14:23 F 219 06:18 219 08/07 06:18 9.58 426 -20 P F H0
8 1999 221  08/09 10:12  -- 221 08/09 10:12 F 222 16:04 222 08/10 16:04 9.90 343 26 P F H0
9 1999 264  09/21 18:57  -- 264 09/21 18:57 F 265 11:31 265 09/22 11:31 11.19 358 1 P F H0
10 1999 265  09/22 12:09  Y 265 09/22 17:59 E 266 09:35 266 09/23 09:35 17.83 560 26 P - H0
11 1999 346  12/12 15:50  Y 346 12/12 17:31 C 347 18:28 347 12/13 18:28 11.76 577 43 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. 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.

Filter table:
None
Shock events only
Flux-rope only
Ejecta only
Text filter:
USA Gov . gov NASA Logo - nasa.gov