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WIND

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Wind ICME Catalogue

2003

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 2003 026  01/26 21:43  -- 027 01/27 01:40 F 027 16:04 027 01/27 16:04 10.40 520 46 P - H0
2 2003 032  02/01 13:06  -- 033 02/02 19:11 F 034 09:35 034 02/03 09:35 10.17 482 0 P - H0
3 2003 079  03/20 04:30  -- 079 03/20 11:54 F 079 22:23 079 03/20 22:23 11.14 670 17 P - H0
4 2003 167  06/16 22:33  -- 168 06/17 17:48 F 169 08:18 169 06/18 8:18 12.46 480 -18 P - H0
5 2003 216  08/04 20:23  -- 217 08/05 01:10 F 218 02:23 218 08/06 02:23 9.57 442 16 P - H0
6 2003 324  11/20 08:35  Y 324 11/20 11:31 F 325 01:40 325 11/21 01:40 33.20 593 103 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.
Jian, L., Russell, C.T., Luhmann, J.G., Skoug, R.M.: 2006, Solar Phys. 239, 393.
Lepping, R.P., Berdichevsky, D.B., Wu, C.-C., Szabo, A., Narock, T., Mariani, F., Lazarus, A.J., Quivers,A.J.: 2006, Ann. Geophys. 24, 215.
Lepping, R.P., Wu, C.-C., Berdichevsky, D.B., Szabo, A.: 2011, Solar Phys. 274, 345.
Nieves-Chinchilla, T., Hidalgo, M.A., Sequeiros, J.: 2005, Solar Phys. 232, 105.
Richardson, I.G., Cane, H.V.: 2010, Solar Phys. 264, 189.

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