Latitudinal variation of Pc3-Pc5 geomagnetic pulsation amplitude across the dip equator in central South America
| Autor: | Graziela Belmira Dias da Silva, Antonio L. Padilha, Lívia Ribeiro Alves |
|---|---|
| Rok vydání: | 2019 |
| Předmět: |
Atmospheric Science
Daytime 010504 meteorology & atmospheric sciences Equator Magnetic dip Magnetosphere Noon 01 natural sciences Latitude Physics::Geophysics 0103 physical sciences Earth and Planetary Sciences (miscellaneous) Astrophysics::Solar and Stellar Astrophysics lcsh:Science 010303 astronomy & astrophysics Physics::Atmospheric and Oceanic Physics 0105 earth and related environmental sciences lcsh:QC801-809 Geology Astronomy and Astrophysics Equatorial electrojet Geophysics lcsh:QC1-999 lcsh:Geophysics. Cosmic physics Earth's magnetic field Space and Planetary Science Physics::Space Physics lcsh:Q lcsh:Physics |
| Zdroj: | Annales Geophysicae, Vol 38, Pp 35-49 (2020) |
| ISSN: | 1432-0576 |
| DOI: | 10.5194/angeo-2019-73 |
| Popis: | In order to clarify the equatorial electrojet effects on ground magnetic pulsations in central South America, we statistically analyzed the amplitude structure of Pc3 and Pc5 pulsations recorded during days considered quiet to moderately disturbed at multiple equatorial stations nearly aligned along the 10∘ magnetic meridian. It was observed that Pc3 amplitudes are attenuated around noon at the dip equator for periods shorter than ∼35 s. It is proposed that daytime Pc3s are related to MHD (magnetohydrodynamic) compressional wave vertically incident on the ionosphere, with the screening effect induced by enhanced conductivity in the dip equator causing wave attenuation. Daytime Pc5s showed amplitude enhancement at all equatorial stations, which can be explained by the model of waves excited at higher latitudes and propagating equatorward in an Earth–ionosphere waveguide. However, a slight depression in Pc5 amplitude compared to neighboring equatorial stations and a phase lag in relation to an off-equatorial station were detected at the dip equator. This wave amplitude depression in the Pc5 frequency band cannot be explained by the ionospheric waveguide model alone, and we propose that an alternative propagation model that allows ULF (ultra-low-frequency) waves to penetrate directly from the magnetosphere to low latitudes could be operating simultaneously to produce these features at the dip equator. Significant effects of the sunrise terminator on Pc3 pulsations were also observed at the stations closest to the dip equator. Contrary to what is reported at other longitudes, in central South America the sunrise effect decreases the D∕H amplitude ratio. We suggest that these differences may arise from the unique characteristics of this sector, with a strong longitudinal variation in the magnetic declination and precipitation of energetic particles due to the presence of the South Atlantic Magnetic Anomaly (SAMA). The H-component amplification can be explained by enhancements of the zonal electric field near the magnetic equator driven by F-region neutral winds and waves in the fast-mode of propagation during sunrise. |
| Databáze: | OpenAIRE |
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