In 2006, a first automatic meteor shower search has been carried out, based on 188,068 single station meteors of the IMO Video Meteor Database. Details were presented at the IMC 2006 and can be found in the corresponding presentation and paper.
Beware that improved analysis results were presented in 2008 and 2009!
In principle, the search consists of two stages.
At the IMC, only the list of meteor showers was presented as the final result. However, there are further showers in the data not found during the first search (e.g. because they were of too short duration). For this reason, here the preliminary results of the first stage are given as well.
The following table contains a link for each solar longitude. Each file contains the number of meteors that were available in the given solar longitude interval, as well as the position (right ascension, declination), velocity, relative strength (i.e. accumulated probability mass) and meteor number. If the radiant resembles a shower from the (old) IMO Working List, it is given as reference.
Beware that only the strongest radiants on top of the list will be real, whereas all weaker ones are only by chance alignments of meteors.