List of CMEs for WG5 Analysis

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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)}
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