or
[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 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 from iNTEGRATED SPACE WEATHER ANALYSIS SYSTEM (iSWA) |
REFERENCES | |
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 |