We hope to observe active regions not far from the disk center, since we apply coordinated observations of Hinode and BBSO/NST; the latter require sunspots to make the adaptive optics (AO) system work. According to the width of the filament, the EIS No. OF POINTING POSITION can be changed.
Highest priority: to observe newly formed or well-developed active regions.
Second priority: to observe decaying active regions.
Lowest priority: to observe the quiet regions or off-limb regions when active regions are absent.
List of past HOPs in which the present proposer was the PI
HOP0124 (Time-varying Doppler velocity diagnosis of X-ray Bright Points)
Publications out of those HOPs Zhang, Ping; Fang, Cheng; Zhang, QingMin, gH counterparts of X-ray bright points in the solar atmosphereh, 2012, Science China, Physics (G), Mechanics, & Astronomy, 55, 907
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