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Аннотация:The star LS I +61 deg 303 as radio source with unsual properties is considered. We propose a model of an Induced Pulsator for radio outbursts in LS I +61 deg 303. In our model, the relativistic electrons injected by the radiopulsar are captured by the magnetosphere of the Be-star when the pulsar passed near periastron. Then the captured electrons are cooled slowly due to synchrotron losses. The model was applied to data obtained by Gregory & Taylor in August 1977, August-September 1978 and August-September 1981. These data allow to the determination of parameters of the source LS I +61 deg 303.