⑥Summary
○The steer-type algorithm is one of the solution of
the requirements for the initial
restoration procedure in solar observation; “good performance of restoration for
complicated structures, especially for diffuse features”,
“single set of parameters which are independent from solar activities”, and “less computational time”.
○The steer-type algorithm shows the
independency from the array configuration, and
availability for FASR’s image in middle and high frequency range.
○For FASR’s image in low frequency range, the
steer-type algorithm can restore very diffuse features well,
however, further studies about the restoration of such images
are necessary.