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This study presents observations from various sources including GOES, Hinode, LASCO, ACE, MDI, SOLIS, and SSW to analyze the events that occurred in December 2006 on the Sun, focusing on the magnetic field distribution and its evolution.
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Observations of December 2006 events Yang Liu – Stanford University yliu@solar.stanford.edu
Soft-X ray observation from Hinode (movies from Su et al. 2007)
CMEs and Dst (from Gopalswamy’s group) v(halo)=1774 km/s v(halo)=1042 km/s
Magnetic field on the Sun AR10930
Magnetic distribution over the Sun’s surface MDI AR10930 SOLIS
Vector field on Dec 12 (20:30UT) (from Hinode) Observation Potential Field highly sheared along the neutral line.
Vector field on Dec 13 (04:30UT) (from Hinode) Observation Potential Field
NLFFF (only closed field lines plotted) (from McTiernan’s code available in SSW) Dec 12 20:30 UT Dec 13 04:30 UT
Energy of AR10930 main spot fast-spin spot Vertical electric current Magneticfield Poynting from emerging flux Poynting from surface flow