Dynamic parameters of Pc3 geomagnetic pulsations

Details Dynamic parameters of Pc3 geomagnetic pulsations Dynamic parameters of Pc3 geomagnetic pulsations

Dec 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ge%26ae..29..921p&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 29, Nov.-Dec. 1989, p. 921-925. In Russian.

Computer Science

1

Dynamic Characteristics, Geomagnetic Micropulsations, Magnetohydrodynamic Waves, Magnetospheric Instability, Langevin Formula, Nocturnal Variations, Resonant Frequencies, Statistical Analysis

Scientific paper

The inverse-problem method of the statistical theory of oscillations is used to study Pc3 pulsations. It is confirmed that the H component of the geomagnetic field of the pulsations can be described by a linear-oscillator model with an inducing force under the effect of a Langevin source. It is shown that this model can be used to estimate the natural frequency and Q of the magnetospheric Alfven resonator at a specific magnetic shell.

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