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- W2064694358 abstract "The new criterion DNfor meteoroid stream identification, based on variables directly linked to observations, is applied to a set of 865 photographic meteor orbits and the results are compared with those obtained using the well-known and widely used DScriterion of Southworth & Hawkins, using thresholds for meteor association computed according to Jopek & Froeschlé. For 15 streams, including the Lyrids, the α Capricornids, the Perseids, the Taurids, the Quadrantids, the Geminids, the Leonids, the Orionids and the southern δ Aquarids, the two searches are in very good agreement, with DNoften adding a few more members to some streams, at the same level of statistical significance as used for DSH. The Andromedids and the σ Leonids, identified as populous streams using DSH, are not recognized using DN; on the other hand, using DNfive additional streams are identified, namely the ɛ Geminids, the Monocerotids, the northern δ Aquarids and the rather populous α Virginids and ɛ Piscids. In general, DNgives results essentially equivalent to those obtained with DSHin many circumstances, the most notable exception being for near-ecliptical streams, where the results differ markedly. We show also that the reduced distance function DRcan be successfully applied to search for meteor showers resulting from the same meteoroid stream; in our study the Quadrantids and the southern and northern δ Aquarid showers have been identified as possibly being originated by a single meteoroid stream." @default.
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- W2064694358 date "1999-04-16" @default.
- W2064694358 modified "2023-09-30" @default.
- W2064694358 title "Meteoroid stream identification: a new approach -- II. Application to 865 photographic meteor orbits" @default.
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- W2064694358 doi "https://doi.org/10.1046/j.1365-8711.1999.02265.x" @default.
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