System identification of geomagnetic disturbances initiated by the solar wind.

Details System identification of geomagnetic disturbances initiated by the solar wind. System identification of geomagnetic disturbances initiated by the solar wind.

May 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991acgsn..34..272z&link_type=abstract

Acta Geophys. Sin., Vol. 34, No. 3, p. 272 - 279

Physics

Geomagnetic Field: Disturbances, Geomagnetic Field: Solar Wind

Scientific paper

On the basis of linear and time-invariant supposition, the geomagnetic disturbances initiated by the solar wind have been studied in terms of least square non-parametric identification method. The macro-external description of the response of the magnetosphere to the solar wind is given by the impulse response function. The predicted geomagnetic disturbances are compared with the observations; they are found to agree quite well.

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