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Bursts of high energy EAS intensity (the series of EAS), following each otherin short intervals of time were observed by means of Tien-Shan high mountaininstallation. For the lower boundary of EAS, uniting in one series, the sizeNe= 10**6 (primary energies of the order of 4x10**15 eV) was taken. Thecondition of amalgamation into one series was the presence of at least two EASof Ne >10**7. The number of EAS in a series is from 4 to 9 events, with themean time interval between them 1-5 minutes. Five such series were found in thematerial treated (approximately 250 days of pure time of the installation run).For each EAS of each series, all the basic parameters are given: observationdate and time, age parameter S, galactic coordinates, coordinates of EAS axesrelative to the installation center, energy release in the calorimeter and itsdistance from EAS axes, fitting the Nishimura- Kamata- Greisen (NKG) function.It is essential, that the frequency of the appearing of such series is muchhigher, than the probability of the occasional fluctuations in the successionof independent EAS. This probably is in favor of the commonality of theirorigin.

The Eas Bursts - High Energy Extensive Air Showers Correlated in Time