Goddard Space Flight Center
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WIND

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Wind ICME Catalogue

2008

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 2008 144  05/23 01:12  -- 144 05/23 01:12 F 144 10:47 144 05/23 10:47 5.15 499 21 P F H0
2 2008 247  09/03 16:33  -- 247 09/03 16:33 F 248 03:50 248 09/04 03:50 11.46 466 -21 P F H0
3 2008 261  09/17 00:43  -- 261 09/17 03:57 F 262 08:09 262 09/18 08:09 5.67 407 44 P F H0
4 2008 339  12/04 11:59  -- 339 12/04 16:47 F 340 10:47 340 12/05 10:47 7.04 390 6 P F H0
5 2008 352  12/17 03:35  -- 352 12/17 03:35 F 352 15:35 352 12/17 15:35 7.98 338 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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