Table 1: Photospheric, chromospheric and coronal observations of AR 8210 on May 1, 1998. $\Delta x$ is the pixel size, $\Delta t$ is the time between two consecutive observations.
Instrument Wavelength Obs. time $\Delta x$ $\Delta t$
SOHO/MDI Ni I at 676.8 nm 17:00-23:00 1 $.\!\!^{\prime\prime}$98 1 min
MSO/IVM FeI at 630.25 nm 17:07-21:40 1 $.\!\!^{\prime\prime}$1 3 min
NSO/BBSO H$\alpha $ at 656.3 nm 17:00-21:08 1 $^{\prime\prime}$ 1 min
MSO/MCCD '' 17:00-22:00 2 $.\!\!^{\prime\prime}$4 15 s
SOHO/EIT Fe XII at 19.5 nm 17:00-23:00 2 $.\!\!^{\prime\prime}$46 15 min
Yohkoh/SXT Soft X-rays 17:16-22:16 4 $.\!\!^{\prime\prime}$9 and 9 $.\!\!^{\prime\prime}$8 $\sim$8 min


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