Ng. Kleimenova et al., Long-period (1-6 mHz) geomagnetic pulsations during the initial phase of the big magnetic storm of February 21, 1994, GEOMAG AERO, 40(4), 2000, pp. 420-429
The features of the long-period geomagnetic pulsations recorded during the
initial phase (09:00-12:00 UT) of the big magnetic storm of February 21, 19
94, are studied using ground-based observations at the worldwide network of
stations. It has been shown that the initial phase of this magnetic storm
was characterized by the excitation of intense irregular geomagnetic pulsat
ions of the ipcl type in the frequency band 1-6 mHz at the latitudes of the
dayside polar cusp and polar cap. Their amplitude was at a maximum at freq
uencies below 2 mHz. It has been established that the dynamic spectra of th
e pulsations detected in the IMF and solar wind and on the Earth's surface
are similar. The most distinct similarity between the oscillation spectra o
f the geomagnetic pulsations in the polar-cap region and those of the IMF B
-x-component was observed at the sudden commencement (SC). This result allo
ws us to suggest that the polar geomagnetic pulsations were caused by the p
enetration of waves from the interplanetary medium. According to the GEOTAI
L satellite data, the oscillations of the magnetic field and the variations
in the solar-wind density were in antiphase, which can be an indication th
at the compressional wave approached the Earth. In the inner magnetosphere,
low-frequency geomagnetic pulsations apparently result from the generation
of a global cavity mode due to the possible penetration of hydromagnetic w
aves of corresponding periods from the solar wind.