Daytime quasiperiodic geomagnetic pulsations during the recovery phase of the strong magnetic storm of May 15, 2005

Details Daytime quasiperiodic geomagnetic pulsations during the recovery phase of the strong magnetic storm of May 15, 2005 Daytime quasiperiodic geomagnetic pulsations during the recovery phase of the strong magnetic storm of May 15, 2005

Oct 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ge%26ae..47..580k&link_type=abstract

Geomagnetism and Aeronomy, Volume 47, Issue 5, pp.580-587

Computer Science

3

94.30.Ms, 94.30.Lr, Magnetic Pulsations, Magnetic Storms, Substorms

Scientific paper

Intense quasimonchromatic geomagnetic pulsations with a period of ˜15 min, observed on the Earth’s surface in the near-noon sector at the beginning of the recovery phase of a very strong ( Dst min = -260 nT) magnetic storm of May 15, 2005, are analyzed. The variations were registered at auroral latitudes only in the X field component, and wave activity shifted into the postnoon sector of the polar cap an hour later; in this case pulsations were observed in the X and Y field components. Within the magnetosphere the source of magnetic pulsations could be the surface waves on the magnetopause caused by the pulse of the solar wind magnetic pressure. Geomagnetic pulsations in the polar cap, observed in phase at different latitudes, could apparently reflect quasiperiodic variations in the NBZ system of field-aligned currents. Such variations can originate due to the series of pulsed reconnections in the postnoon outer cusp at large (˜20 nT) positive B z values and large (about -40 nT) negative values of IMF B x .

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