WG3: Extreme Events Summary N. Gopalswamy & A. Vourlidas.
Flare footpoints and ribbons: The impulsive phase H.S. Hudson Space Sciences Lab, UC Berkeley.
Forbes CME Hones TPE 5101520 50 100 150 200 250 300 Distance in Rs Acceleration (m/s 2 ) CME Acceleration 50100150200 400 600 800 1000 1200 Solar Wind.
Energy partition during initial stages of the CME
Relationships between flares and CMEs
Transients on the Sun
SMESE: a French/Chinese Solar “SMEX” H.S. Hudson Space Sciences Lab, UC Berkeley.
