The Effect of the Differential Rotation of Photospheric Magnetic Features on the Synoptic Frame of the Photospheric Magnetic Field
نویسندگان
چکیده
The effect of the advection of magnetic features on synoptic frames has been estimated and it shows that for the time interval ranging from 4 to 14 days the differential rotation of magnetic features accounts for most of the surface transport of photospheric magnetic fields. It is shown that both the 1996.08.27 19:12:30 synoptic frame with the effect of differential rotation included and the footpoint area and the neutral line calculated on the basis of the new synoptic frame differe slightly from that without differential rotation. To determine the improvement made by including the effect of magnetic features’ differential rotation, more samples are needed to compare with observed coronal structures. The 2004 AGU Fall Meeting, December 12 – (14) – 18, 2004, San Francisco
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