List of CMEs for WG5 Analysis

List of near-Sun Observations/Determinations of CME Magnetic Fields for WG5

Date and Time	Solar Source (AR # or location)	Method of Magnetic Field Determination	Publication	Miscellaneous	Submitter contact
2011/06/07 06:47 UT	AR NOAA 11226 (CME propagating on the west limb)	The magnetic field in the corona is determined by applying the Rankine-Hugoniot equations to LASCO C2 and C3 white-light images of the CME-driven shock in order to derive a map of the shock Alfvenic Mach number	Bemporad, A. & Mancuso, S. 2010, ApJ 720, 130 (also Bemporad, A., Susino, R., & Mancso, S. ApJ, in preparation)		R. Susino (susino@oato.inaf.it) and A. Bemporad (bemporad@oato.inaf.it)}
2012/03/07 01:14 UT	AR NOAA 11429	The coronal CME magnetic field is estimated by combination of magnetic helicity calculations of the CME source region and forward modeling of the CME along with application of the helicity conservation principle in flux-rope CMEs	Patsourakos, S., Georgoulis, M. K., Vourlidas, A. et al., 2016, ApJ, 817, 14		S. Patsourakos (spatsour@cc.uoi.gr)}
2010-04-03T09:54 UT	AR NOAA 11059	Bz prediction and Kp prediction was using the Bz4Cast model. It is also in the IMF Bz team core event list for MHD modelers. [1]CCMC donki details	Savani, N. P., Vourlidas, A. et al., 2015, Space Weather, 13: 374 [2]10.1002/2015SW001171		N. Savani (neel.savani@nasa.gov)}