- the individual animations show the distributions plotted in Figs. 3-12 in the paper (Leto et al., 2008); while the plots in these figures illustrate the state in 2 Gyr (or also for few other times), the animations show their evolution during the entire studied period of 2 Gyr, with the snapshots of every Myr.

- all the animations are provided in "avi" format

• fig03.avi
  • the 2-Gyr evolution of the comet population moved into the inner OC from the Jupiter, Saturn, Uranus, Neptune, and Kuiper-belt regions. The green bars illustrate the numbers of bodies in 0.5-AU-wide intervals of the initial proto-planetary disc, which reside in the inner Oort cloud (OC) at the just shown time. The red bars do so for the bodies occuring in the inner OC, at least for a short period, whenever from the beginning of the simulation to the just shown time.
• fig04.avi
  • the 2-Gyr evolution of the heliocentric distance distribution of the OC comets (crosshatched bars). The same distribution of all comets, still bound to the Sun, is also shown (empty bars). the region of heliocentric distance r < 10,000 AU, the distribution of all comets is outside of the chosen vertical scale because of a better transparency of the OC-comet distribution. If all comets in the given interval are in the OC, the crosshatched bar overlaps the entire empty bar, which is not visible in this interval, then.
• fig05.avi
  • the 2-Gyr evolution of the cumulative distribution of bodies in the region of heliocentric distance from 100 to
    100,000 AU (in the logarithmic scale).
• fig06.avi
  • the 2-Gyr evolution of the orbital semi-major axis distribution of bodies residing in the OC (crosshatched bars). The same distribution of all comets, still bound to the Sun, is also shown (empty bars).
• fig07.avi
  • the 2-Gyr evolution of the orbital eccentricity of bodies residing in the inner OC.
• fig08a.avi
  • the 2-Gyr evolution of the inclination to the Galactic- Equator-plane distribution of bodies residing in the inner OC.
• fig08b.avi
  • the 2-Gyr evolution of the inclination to the Ecliptic distribution of bodies residing in the inner OC.
• fig08c.avi
  • the 2-Gyr evolution of the argument-of-perihelion distribution of bodies residing in the inner OC. The referrence frame is galactical.
• fig08d.avi
  • the 2-Gyr evolution of the argument-of-perihelion distribution of bodies residing in the inner OC. The referrence frame is ecliptical.
• fig08e.avi
  • the 2-Gyr evolution of the longitude-of-ascending-node distribution of bodies residing in the inner OC. The referrence frame is galactical.
• fig08f.avi
  • the 2-Gyr evolution of the longitude-of-ascending-node distribution of bodies residing in the inner OC. The referrence frame is ecliptical.
• fig09a.avi
  • the 2-Gyr evolution of the aphelion-point directional distribution of the bodies residing in the inner OC. The referrence frame is galactical. The green curve shows the position of the Ecliptic.
• fig09b.avi
  • the 2-Gyr evolution of the aphelion-point directional distribution of the bodies residing in the inner OC. The referrence frame is ecliptical. The green curve shows the position of the Galactic Equator.
• fig10a.avi
  • the 2-Gyr evolution of the inclination to the Ecliptic vs. semi-major axis of bodies on the orbits with semi-major axis in the interval 50 < a < 22,000 AU. The bodies residing in a given time in the inner OC are shown with red-green asterisks, the other bodies with red crosses.
• fig10b.avi
  • the 2-Gyr evolution of the inclination to the Ecliptic vs. semi-major axis of bodies on the orbits with semi-major axis in the interval 50 < a < 500 AU..
• fig11a.avi
  • the 2-Gyr evolution of the ecliptical rectangular z-component vs. heliocentric distance, "r", of bodies being in the interval 50 < r < 25,000 AU. The bodies residing in a given time in the inner OC are shown with red-green asterisks, the other bodies with red crosses. Because of the obvious fact that "z" cannot be larger than "r", no point can occur above the green line.
• fig11b.avi
  • the 2-Gyr evolution of the ecliptical rectangular z-component vs. heliocentric distance, "r", of the bodies being in the interval 50 < r < 5,000 AU. The bodies residing in a given time in the inner OC are shown with red-green asterisks, the other bodies with red crosses. No TP can occur above the green line.