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

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

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002angeo..20.1751s&link_type=abstract

Annales Geophysicae, vol. 20, Issue 11, pp.1751-1761

Physics

5

Scientific paper

We present the results of analysis of the dayside 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 observatory, 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 activity.

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