Modeling the generation of Pc1 geomagnetic pulsations in the magnetosphere. II

Details Modeling the generation of Pc1 geomagnetic pulsations in the magnetosphere. II Modeling the generation of Pc1 geomagnetic pulsations in the magnetosphere. II

Apr 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ge%26ae..27..279a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 27, Mar.-Apr. 1987, p. 279-286. In Russian.

Physics

Geomagnetic Pulsations, Magnetohydrodynamic Waves, Magnetospheric Instability, Wave Packets, Atmospheric Models, Differential Equations, Oscillations

Scientific paper

It is demonstrated that the generation of Fs(t) oscillation packets of Pc1 pulsations of different form can be adequately modeled by the solution of a coupled system of two oscillatory ordinary differential equations. The excitation of these pulsations is connected with the cyclotron instability of the magnetoplasma. One of the equations, describing Y(t) oscillations, is of linear parametric type. An important result is that 'fast' Y(t) oscillations (Alfven waves in this case) are modulated by slower Z(t) oscillations.

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