Some general aspects of the Perseid meteoroid stream structure are discussed. A reanalysis of the 1988 and 1989 data clarified the existence of 'new peak' for the entire period under study. The activity peak recurred again in 1995 at the same position (solar longitude 159.6 deg (J2000.0)) as in 1994. Probably the peak ZHR was of the order of 150-200. It is reasonable to expect another return of the peak in 1996.
Proceedings of the International Meteor Conference, 14th IMC, Brandenburg, Germany, 1995
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