[1] ICME = Interplanetary Coronal Mass Ejection |
[2] MO = Magnetic Obstacle |
[3] MO Type = Flux-rope (Fr), Small rotation flux-rope (F-), Large rotation flux-rope (F+), Complex (Cx), or Ejecta(E) |
[4] B = Mean magnetic field magnitude value (nT) in the MO interval. |
[5] Vsw = Mean Solar Wind Bulk velocity (km/s) in the MO interval. |
[6] Vexp = Expansion velocity (km/s) in the MO interval. |
[7] Dst = Disturbance Storm-Time index (nT).
The minimum reported Dst index in the MO interval except as noted.
Data from the World Data Center for Geomagnetism, Kyoto Geomagnetic Equatorial Dst index.
|
[8] HO = Heliopheric Overview from iNTEGRATED SPACE WEATHER ANALYSIS SYSTEM (iSWA) |
REFERENCES | |
Citation for the catalog | Nieves-Chinchilla, T., A. Vourlidas, et al. "Understanding the internal magnetic field configurations of ICMEs using more than 20 years of wind observations." Solar Physics 293.2 (2018): 25. DOI: 10.1007/s11207-018-1247-z. |
Citation for the fits | Nieves-Chinchilla, Teresa, et al. "Unraveling the Internal Magnetic Field Structure of the Earth-directed Interplanetary Coronal Mass Ejections During 1995–2015." Solar Physics 294.7 (2019): 89. DOI: 10.1007/s11207-019-1477-8 |
Citation for the modeling | Nieves-Chinchilla, T., M. G. Linton, M. A. Hidalgo, A. Vourlidas, N. P. Savani, A. Szabo, C. Farrugia, W. Yu. "A circular-cylindrical flux-rope analytical model for magnetic clouds." The Astrophysical Journal 823.1 (2016): 27. DOI: 10.3847/0004-637X/823/1/27 |