A new solar Hα flare patrol system was installed at National
Astronomical Observatory, Mitaka and has been in operation since
September, 1991. The new system consists of a φ 4 cm doublet, an
Hα Lyot filter (pass band =0.5 Å), a 2/3 inch CCD camera,
and a digital image analysis and storage unit. In the new system,
Hα flares can be detected and be analyzed in real time by a
computer. The authors
... [Show full abstract] describe the performance of the system and the
methods of Hα flare detection and analysis.