Fig. 1a-f. The distributions of orbital elements of the modelled meteor stream associated with comet 14P/Wolf. The theoretical stream is modelled considering . The evolution of orbital elements of the stream is analysed during the period from May 3.56978, 1905 to June 28.70888, 1987, which covers 10 orbital periods of the parent comet. In each plot, the distributions at the beginning of evolution as well as at the end of each period are given. Perihelion distance is given in AU, angular elements in degrees.