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Fig. 3

image

Positions of geocentric radiants of theoretical particles (black dots) in the predicted filament F3 and corresponding real-shower meteors of the July ξ-Arietids, shower 533, separated from the CAMS-video (green triangles) and SonotaCo-video (red full squares) databases. The positions are shown in the models for the P–R effect parameter β = 0.00001 and a series of evolutionary times tev = 5 (panel a), 10 (panel b), 20 (panel c), 40 (panel d), and 80 kyr (panel e). To show the radiants, the Sun-centered ecliptic coordinate frame is used.

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