Physics
Scientific paper
Jan 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011jgra..11601204n&link_type=abstract
Journal of Geophysical Research, Volume 116, Issue A1, CiteID A01204
Physics
2
Ionosphere: Wave Propagation (0689, 3285, 4275, 4455, 6934), Magnetospheric Physics: Mhd Waves And Instabilities (2149, 6050, 7836), Magnetospheric Physics: Magnetosphere: Inner, Magnetospheric Physics: Magnetosphere/Ionosphere Interactions (2431), Ionosphere: Plasma Waves And Instabilities (2772)
Scientific paper
We have investigated Pc1 geomagnetic pulsations observed by induction magnetometers at three low-latitude stations (Paratunka (PTK), Moshiri (MSR), and Sata (STA), L=1.2-2.1). A detailed polarization analysis shows that polarization parameters (angle of polarization ellipse orientation, Ψ, and polarization sense, $\varepsilon$) of individual Pc1 bands depend on frequency at all three stations. The dependence of Ψ on frequency was seen in ˜70% of the 93 Pc1 events observed at MSR (L=1.5) from 14 July 2007 to 13 July 2009. The maxima of seasonal and diurnal variations of the occurrence rate were in winter and during the nighttime, as reported previously, indicating that the transmission of observed Pc1 pulsations to lower latitudes is controlled by the density of the F layer plasma. These facts suggest that spatially distributed Pc1 waves with varying frequencies depending on longitude or latitude at high latitudes propagated in the ionospheric duct to cause the frequency dependence of polarization parameters at low latitudes. We also suggest that the Pc1 pearl structure with a repetition period of ˜5-30 s observed at low latitudes is a beat of high-latitude waves with slightly different frequencies.
Nomura Ryo
Pilipenko Viacheslav
Shevtsov B.
Shiokawa Kazuhiko
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