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- W1986104848 abstract "A new experimental method is suggested to recognize a type of the incident magnetospheric wave following by the time and frequency dependency of the azimuth angle of geomagnetic pulsations close to the terminator. The main idea is based on the fundamental differences between the ionospheric transformation of the Alfvén and magnetosonic waves. The Alfvén waves are associated with some kind of field aligned currents which cannot penetrate into the atmosphere and spread over the high conductive ionosphere. Magnetic effect on the ground is defined mainly by the ionospheric currents caused by the Alfvén wave. In contrast, in the case of magnetosonic wave, the ground current system provides the main contribution to the total current and going from the daylight ionosphere to the night one does not markedly affects on the total current. Equatorial observations revealed the horizontal orientation angle in different frequency ranges. This is inclined to think that in the cases have been under the consideration the oscillations within the range 50∼500 s are generated by the Alfvén waves." @default.
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- W1986104848 date "1996-01-01" @default.
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- W1986104848 title "Determination of Magnetospheric Wave Polarization Using Ground Based Sun-Rise Geomagnetic Observations." @default.
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- W1986104848 doi "https://doi.org/10.5636/jgg.48.79" @default.
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