  We have measured the radiant of the Leonids meteor storm in November 2001 by
using new observational and analysis techniques. The radiant was measured as
the intersections of lines which were detected and extrapolated from images
obtained at a single observing site (Akeno Observatory, Japan). The images were
obtained by two sets of telephoto lenses equipped with cooled CCD cameras. The
measured radiant, (R.A., Dec.)=(154$^\circ$.35, 21$^\circ$.55) (J2000), is
found to be in reasonable agreement with the theoretical prediction by McNaught
and Asher (2001), which verifies their dust trail theory.
