  Application of the theoretical results of the author are presented for the
case of meteor streams of comet Encke. Theoretical determination of meteor
orbit for comet Encke, as a parent body, is presented. Four significant
theoretical meteor streams, corresponding to Tauds N, Tauds S, $\beta$ Tauds
and $\xi$ Perds are found. The meteor stream membership criterion is applied to
the photographic orbits of The IAU Meteor Data Center in Lund: Taurid meteor
stream is found for several possible areas in phase-space of orbital elements.
