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- W2185508737 abstract "Geomagnetic pulsations in the frequency range of 0.5-10 mHz during the strong magnetic storm on July 15, 2000 have been analysed by using 1-min sampled digital geomagnetic measurements on 78 globally distributed INTERMAGNET stations. This storm was caused by an interplanetary magnetic cloud impact. The dynamic spectral and wavelet analysis of ground geomagnetic pulsations and IMF and solar wind data from GEOTAIL spacecraft (X ~20 Re, Y ~ -6 Re, Z ~ 2 Re) has been carried out. The analysis showed that the strong IMF and solar wind density variations were observed in the turbulent region, located before the leading edge of the cloud. The spectral structure of the different IMF components was different. The IMF irregularities triggered the magnetic substorm and Pi3 range geomagnetic pulsations in the polar cap with the strongest amplitudes near the footprint of the border between the close and open field lines. We suppose that the polar Pi3 pulsations could be attributed to the wave generation at ionosphere altitudes by the oscillations of the electron precipitation of field aligned currents. The IMF fluctuations behind the leading edge were very small. After the leading edge of magnetic cloud passage, the Pi3 pulsation activity suddenly shifted into day- and night- time inner magnetosphere. The daytime geomagnetic pulsations were associated with the field line resonance and the nighttime pulsations - with substorm activity." @default.
- W2185508737 created "2016-06-24" @default.
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- W2185508737 date "2003-01-01" @default.
- W2185508737 modified "2023-09-27" @default.
- W2185508737 title "GROUND GEOMAGNETIC Pi3 PULSATIONS DURING THE BASTILLE MAGNETIC STORM (JULY 15, 2000)" @default.
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