①Introduction (Continued)
Each image can be processed manually
and carefully in similar way to non-solar observation. However,
every image must, first, be processed automatically without any
parameter adjustments in order to determine when and where remarkable
phenomena occurred.
Initial restoration procedure in solar observation, therefore, requires
the ability with;
1. Good
performance of restoration for complicated structures, especially for diffuse features.
2. single set of parameters which are
independent from the solar activities.
3. less
computational time.