Fig. 4
Distributions of elements of modeled particle orbits approaching the Earth’s orbit at a distance shorter than 0.05 AU at present. Specifically, the relative distributions, in arbitrary units, of perihelion distance a), semi-major axis b), eccentricity c), argument of perihelion d), longitude of ascending node e), and inclination to the ecliptic f) are shown for 8 streams modeled 8 times before the present. The times are indicated in the left or right top corner of each plot. For better transparency, the distribution for each successive time is shifted up relatively to the distribution for the preceding time.
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