Bursts of ULF noise excited by sudden changes of solar wind dynamic pressure

Abstract. We present the results of analysis of the day-side magnetic pulsation response to a sudden change in solar wind dynamic pressure. We concentrate on the events when a burst or a series of short-lived bursts in the Pc1 frequency range with the repetition period of 7–15 min were observed on the ground around the local noon. Not every impulse of large amplitude caused this phenomenon. We have found that the ULF bursts were excited when the spectrograms of the DMSP satellites showed a signature of 10–30 keV ions in the vicinity of the magnetic flux tube of the ground observa-tory, that may be related to a geomagnetic storm preceding the event. In light of this finding a possible model of the phenomenon is suggested in which the hot protons influence significantly both the generation and modulation of Pc1 ac-tivity. Key words. Magnetospheric physics (solar wind – magne-tosphere interaction; MHD waves and instabilities; storms and substorms)