Near-Earth stream decoherence revisited: the limits of orbital similarity

Open Access

Fig. 17

Decoherence lifetime as a function of the semi-major axis and eccentricity with an inclination of 20° using D_{S H} (a), D′ (b), or D_H (c) values in conjunction with a DBSCAN algorithm to determine clustering. Decoherence time was defined as when a fictitious meteoroid stream lost 95% or more of the original stream.

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